Sample records for active ice margin

  1. Correlation studies of passive and active microwave data in the marginal ice zone

    NASA Technical Reports Server (NTRS)

    Comiso, J. C.

    1991-01-01

    The microwave radiative and backscatter characteristics of sea ice in an Arctic marginal ice zone have been studied using near-simultaneous passive and active synthetic aperture radar microwave data. Intermediate-resolution multichannel passive microwave data were registered and analyzed. Passive and active microwave data generally complement each other as the two sensors are especially sensitive to different physical properties of the sea ice. In the inner pack, undeformed first-year ice is observed to have low backscatter values but high brightness temperatures while multiyear ice has generally high backscatter values and low brightness temperatures. However, in the marginal ice zone, the signature and backscatter for multiyear ice are considerably different and closer to those of first-year ice. Some floes identified by photography as snow-covered thick ice have backscatter similar to that of new ice or open water while brash ice has backscatter similar to or higher than that of ridged ice.

  2. Active/passive microwave sensor comparison of MIZ-ice concentration estimates. [Marginal Ice Zone (MIZ)

    NASA Technical Reports Server (NTRS)

    Burns, B. A.; Cavalieri, D. J.; Keller, M. R.

    1986-01-01

    Active and passive microwave data collected during the 1984 summer Marginal Ice Zone Experiment in the Fram Strait (MIZEX 84) are used to compare ice concentration estimates derived from synthetic aperture radar (SAR) data to those obtained from passive microwave imagery at several frequencies. The comparison is carried out to evaluate SAR performance against the more established passive microwave technique, and to investigate discrepancies in terms of how ice surface conditions, imaging geometry, and choice of algorithm parameters affect each sensor. Active and passive estimates of ice concentration agree on average to within 12%. Estimates from the multichannel passive microwave data show best agreement with the SAR estimates because the multichannel algorithm effectively accounts for the range in ice floe brightness temperatures observed in the MIZ.

  3. Changes in ice-margin processes and sediment routing during ice-sheet advance across a marginal moraine

    USGS Publications Warehouse

    Knight, P.G.; Jennings, C.E.; Waller, R.I.; Robinson, Z.P.

    2007-01-01

    Advance of part of the margin of the Greenland ice sheet across a proglacial moraine ridge between 1968 and 2002 caused progressive changes in moraine morphology, basal ice formation, debris release, ice-marginal sediment storage, and sediment transfer to the distal proglacial zone. When the ice margin is behind the moraine, most of the sediment released from the glacier is stored close to the ice margin. As the margin advances across the moraine the potential for ice-proximal sediment storage decreases and distal sediment flux is augmented by reactivation of moraine sediment. For six stages of advance associated with distinctive glacial and sedimentary processes we describe the ice margin, the debris-rich basal ice, debris release from the glacier, sediment routing into the proglacial zone, and geomorphic processes on the moraine. The overtopping of a moraine ridge is a significant glaciological, geomorphological and sedimentological threshold in glacier advance, likely to cause a distinctive pulse in distal sediment accumulation rates that should be taken into account when glacial sediments are interpreted to reconstruct glacier fluctuations. ?? 2007 Swedish Society for Anthropology and Geography.

  4. Remote sensing of the marginal ice zone during Marginal Ice Zone Experiment (MIZEX) 83

    NASA Technical Reports Server (NTRS)

    Shuchman, R. A.; Campbell, W. J.; Burns, B. A.; Ellingsen, E.; Farrelly, B. A.; Gloersen, P.; Grenfell, T. C.; Hollinger, J.; Horn, D.; Johannessen, J. A.

    1984-01-01

    The remote sensing techniques utilized in the Marginal Ice Zone Experiment (MIZEX) to study the physical characteristics and geophysical processes of the Fram Strait Region of the Greenland Sea are described. The studies, which utilized satellites, aircraft, helicopters, and ship and ground-based remote sensors, focused on the use of microwave remote sensors. Results indicate that remote sensors can provide marginal ice zone characteristics which include ice edge and ice boundary locations, ice types and concentration, ice deformation, ice kinematics, gravity waves and swell (in the water and the ice), location of internal wave fields, location of eddies and current boundaries, surface currents and sea surface winds.

  5. Microwave and physical properties of sea ice in the winter marginal ice zone

    NASA Technical Reports Server (NTRS)

    Tucker, W. B., III; Perovich, D. K.; Gow, A. J.; Grenfell, T. C.; Onstott, R. G.

    1991-01-01

    Surface-based active and passive microwave measurements were made in conjunction with ice property measurements for several distinct ice types in the Fram Strait during March and April 1987. Synthesis aperture radar imagery downlinked from an aircraft was used to select study sites. The surface-based radar scattering cross section and emissivity spectra generally support previously inferred qualitative relationships between ice types, exhibiting expected separation between young, first-year and multiyear ice. Gradient ratios, calculated for both active and passive data, appear to allow clear separation of ice types when used jointly. Surface flooding of multiyear floes, resulting from excessive loading and perhaps wave action, causes both active and passive signatures to resemble those of first-year ice. This effect could possibly cause estimates of ice type percentages in the marginal ice zone to be in error when derived from aircraft- or satellite-born sensors.

  6. Ice sheet margins and ice shelves

    NASA Technical Reports Server (NTRS)

    Thomas, R. H.

    1984-01-01

    The effect of climate warming on the size of ice sheet margins in polar regions is considered. Particular attention is given to the possibility of a rapid response to warming on the order of tens to hundreds of years. It is found that the early response of the polar regions to climate warming would be an increase in the area of summer melt on the ice sheets and ice shelves. For sufficiently large warming (5-10C) the delayed effects would include the breakup of the ice shelves by an increase in ice drainage rates, particularly from the ice sheets. On the basis of published data for periodic changes in the thickness and melting rates of the marine ice sheets and fjord glaciers in Greenland and Antarctica, it is shown that the rate of retreat (or advance) of an ice sheet is primarily determined by: bedrock topography; the basal conditions of the grounded ice sheet; and the ice shelf condition downstream of the grounding line. A program of satellite and ground measurements to monitor the state of ice sheet equilibrium is recommended.

  7. Ocean-ice interaction in the marginal ice zone

    NASA Technical Reports Server (NTRS)

    Liu, Antony K.; Peng, Chich Y.

    1994-01-01

    Ocean ice interaction processes in the Marginal Ice Zone (MIZ) by wind, waves, and mesoscale features, such as upwelling and eddies, are studied using ERS-1 Synthetic Aperture Radar (SAR) images and ocean ice interaction model. A sequence of SAR images of the Chukchi Sea MIZ with three days interval are studied for ice edge advance/retreat. Simultaneous current measurements from the northeast Chukchi Sea as well as the Barrow wind record are used to interpret the MIZ dynamics.

  8. Ku band airborne radar altimeter observations of marginal sea ice during the 1984 Marginal Ice Zone Experiment

    NASA Technical Reports Server (NTRS)

    Drinkwater, Mark R.

    1991-01-01

    Pulse-limited, airborne radar data taken in June and July 1984 with a 13.8-GHz altimeter over the Fram Strait marginal ice zone are analyzed with the aid of large-format aerial photography, airborne synthetic aperture radar data, and surface observations. Variations in the radar return pulse waveforms are quantified and correlated with ice properties recorded during the Marginal Ice Zone Experiment. Results indicate that the wide-beam altimeter is a flexible instrument, capable of identifying the ice edge with a high degree of accuracy, calculating the ice concentration, and discriminating a number of different ice classes. This suggests that microwave radar altimeters have a sensitivity to sea ice which has not yet been fully exploited. When fused with SSM/I, AVHRR and ERS-1 synthetic aperture radar imagery, future ERS-1 altimeter data are expected to provide some missing pieces to the sea ice geophysics puzzle.

  9. The role of the margins in ice stream dynamics

    NASA Technical Reports Server (NTRS)

    Echelmeyer, Keith; Harrison, William

    1993-01-01

    At first glance, it would appear that the bed of the active ice stream plays a much more important role in the overall force balance than do the margins, especially because the ratio of the half-width to depth for a typical ice stream is large (15:1 to 50:1). On the other hand, recent observations indicate that at least part of the ice stream is underlain by a layer of very weak till (shear strength about 2 kPa), and this weak basal layer would then imply that some or all of the resistive drag is transferred to the margins. In order to address this question, a detailed velocity profile near Upstream B Camp, which extends from the center of the ice stream, across the chaotic shear margin, and onto the Unicorn, which is part of the slow-moving ice sheet was measured. Comparison of this observed velocity profile with finite-element models of flow shows several interesting features. First, the shear stress at the margin is on the order of 130 kPa, while the mean value along the bed is about 15 kPa. Integration of these stresses along the boundaries indicates that the margins provide 40 to 50 percent, and the bed, 60 to 40 percent of the total resistive drag needed to balance the gravitational driving stress in this region. (The range of values represents calculations for different values of surface slope.) Second, the mean basal stress predicted by the models shows that the entire bed cannot be blanketed by the weak till observed beneath upstream B - instead there must be a distribution of weak till and 'sticky spots' (e.g., 85 percent till and 15 percent sticky spots of resistive stress equal to 100 kPa). If more of the bed were composed of weak till, then the modeled velocity would not match that observed. Third, the ice must exhibit an increasing enhancement factor as the margins are approached (E equals 10 in the chaotic zone), in keeping with laboratory measurements on ice under prolonged shear strain. Also, there is either a narrow zone of somewhat stiffer ice (E

  10. The role of the margins in ice stream dynamics

    NASA Astrophysics Data System (ADS)

    Echelmeyer, Keith; Harrison, William

    1993-07-01

    At first glance, it would appear that the bed of the active ice stream plays a much more important role in the overall force balance than do the margins, especially because the ratio of the half-width to depth for a typical ice stream is large (15:1 to 50:1). On the other hand, recent observations indicate that at least part of the ice stream is underlain by a layer of very weak till (shear strength about 2 kPa), and this weak basal layer would then imply that some or all of the resistive drag is transferred to the margins. In order to address this question, a detailed velocity profile near Upstream B Camp, which extends from the center of the ice stream, across the chaotic shear margin, and onto the Unicorn, which is part of the slow-moving ice sheet was measured. Comparison of this observed velocity profile with finite-element models of flow shows several interesting features. First, the shear stress at the margin is on the order of 130 kPa, while the mean value along the bed is about 15 kPa. Integration of these stresses along the boundaries indicates that the margins provide 40 to 50 percent, and the bed, 60 to 40 percent of the total resistive drag needed to balance the gravitational driving stress in this region. (The range of values represents calculations for different values of surface slope.) Second, the mean basal stress predicted by the models shows that the entire bed cannot be blanketed by the weak till observed beneath upstream B - instead there must be a distribution of weak till and 'sticky spots' (e.g., 85 percent till and 15 percent sticky spots of resistive stress equal to 100 kPa). If more of the bed were composed of weak till, then the modeled velocity would not match that observed. Third, the ice must exhibit an increasing enhancement factor as the margins are approached (E equals 10 in the chaotic zone), in keeping with laboratory measurements on ice under prolonged shear strain. Also, there is either a narrow zone of somewhat stiffer ice (E

  11. Norwegian remote sensing experiment in a marginal ice zone

    USGS Publications Warehouse

    Farrelly, B.; Johannessen, J.A.; Svendsen, E.; Kloster, K.; Horjen, I.; Matzler, C.; Crawford, J.; Harrington, R.; Jones, L.; Swift, C.; Delnore, V.E.; Cavalieri, D.; Gloersen, P.; Hsiao, S.V.; Shemdin, O.H.; Thompson, T.W.; Ramseier, R.O.; Johannessen, O.M.; Campbell, W.J.

    1983-01-01

    The Norwegian Remote Sensing Experiment in the marginal ice zone north of Svalbard took place in fall 1979. Coordinated passive and active microwave measurements were obtained from shipborne, airborne, and satellite instruments together with in situ observations. The obtained spectra of emissivity (frequency range, 5 to 100 gigahertz) should improve identification of ice types and estimates of ice concentration. Mesoscale features along the ice edge were revealed by a 1.215-gigahertz synthetic aperture radar. Ice edge location by the Nimbus 7 scanning multichannel microwave radiometer was shown to be accurate to within 10 kilometers.

  12. Discharge of debris from ice at the margin of the Greenland ice sheet

    USGS Publications Warehouse

    Knight, P.G.; Waller, R.I.; Patterson, C.J.; Jones, A.P.; Robinson, Z.P.

    2002-01-01

    Sediment production at a terrestrial section of the ice-sheet margin in West Greenland is dominated by debris released through the basal ice layer. The debris flux through the basal ice at the margin is estimated to be 12-45 m3 m-1 a-1. This is three orders of magnitude higher than that previously reported for East Antarctica, an order of magnitude higher than sites reported from in Norway, Iceland and Switzerland, but an order of magnitude lower than values previously reported from tidewater glaciers in Alaska and other high-rate environments such as surging glaciers. At our site, only negligible amounts of debris are released through englacial, supraglacial or subglacial sediment transfer. Glacio-fluvial sediment production is highly localized, and long sections of the ice-sheet margin receive no sediment from glaciofluvial sources. These findings differ from those of studies at more temperate glacial settings where glaciofluvial routes are dominant and basal ice contributes only a minor percentage of the debris released at the margin. These data on debris flux through the terrestrial margin of an outlet glacier contribute to our limited knowledge of debris production from the Greenland ice sheet.

  13. Multisensor comparison of ice concentration estimates in the marginal ice zone

    NASA Technical Reports Server (NTRS)

    Burns, B. A.; Cavalieri, D. J.; Gloersen, P.; Keller, M. R.; Campbell, W. J.

    1987-01-01

    Aircraft remote sensing data collected during the 1984 summer Marginal Ice Zone Experiment in the Fram Strait are used to compare ice concentration estimates derived from synthetic aperture radar (SAR) imagery, passive microwave imagery at several frequencies, aerial photography, and spectral photometer data. The comparison is carried out not only to evaluate SAR performance against more established techniques but also to investigate how ice surface conditions, imaging geometry, and choice of algorithm parameters affect estimates made by each sensor.Active and passive microwave sensor estimates of ice concentration derived using similar algorithms show an rms difference of 13 percent. Agreement between each microwave sensor and near-simultaneous aerial photography is approximately the same (14 percent). The availability of high-resolution microwave imagery makes it possible to ascribe the discrepancies in the concentration estimates to variations in ice surface signatures in the scene.

  14. Wave effects on ocean-ice interaction in the marginal ice zone

    NASA Technical Reports Server (NTRS)

    Liu, Antony K.; Hakkinen, Sirpa; Peng, Chih Y.

    1993-01-01

    The effects of wave train on ice-ocean interaction in the marginal ice zone are studied through numerical modeling. A coupled two-dimensional ice-ocean model has been developed to include wave effects and wind stress for the predictions of ice edge dynamics. The sea ice model is coupled to the reduced-gravity ocean model through interfacial stresses. The main dynamic balance in the ice momentum is between water-ice stress, wind stress, and wave radiation stresses. By considering the exchange of momentum between waves and ice pack through radiation stress for decaying waves, a parametric study of the effects of wave stress and wind stress on ice edge dynamics has been performed. The numerical results show significant effects from wave action. The ice edge is sharper, and ice edge meanders form in the marginal ice zone owing to forcing by wave action and refraction of swell system after a couple of days. Upwelling at the ice edge and eddy formation can be enhanced by the nonlinear effects of wave action; wave action sharpens the ice edge and can produce ice meandering, which enhances local Ekman pumping and pycnocline anomalies. The resulting ice concentration, pycnocline changes, and flow velocity field are shown to be consistent with previous observations.

  15. Remote sensing of the Fram Strait marginal ice zone

    USGS Publications Warehouse

    Shuchman, R.A.; Burns, B.A.; Johannessen, O.M.; Josberger, E.G.; Campbell, W.J.; Manley, T.O.; Lannelongue, N.

    1987-01-01

    Sequential remote sensing images of the Fram Strait marginal ice zone played a key role in elucidating the complex interactions of the atmosphere, ocean, and sea ice. Analysis of a subset of these images covering a 1-week period provided quantitative data on the mesoscale ice morphology, including ice edge positions, ice concentrations, floe size distribution, and ice kinematics. The analysis showed that, under light to moderate wind conditions, the morphology of the marginal ice zone reflects the underlying ocean circulation. High-resolution radar observations showed the location and size of ocean eddies near the ice edge. Ice kinematics from sequential radar images revealed an ocean eddy beneath the interior pack ice that was verified by in situ oceanographic measurements.

  16. Evolution of microwave sea ice signatures during early summer and midsummer in the marginal ice zone

    NASA Technical Reports Server (NTRS)

    Onstott, R. G.; Grenfell, T. C.; Matzler, C.; Luther, C. A.; Svendsen, E. A.

    1987-01-01

    Emissivities at frequencies from 5 to 94 GHz and backscatter at frequencies from 1 to 17 GHz were measured from sea ice in Fram Strait during the marginal Ice Zone Experiment in June and July of 1983 and 1984. The ice observed was primarily multiyear; the remainder, first-year ice, was often deformed. Results from this active and passive microwave study include the description of the evolution of the sea ice during early summer and midsummer; the absorption properties of summer snow; the interrelationship between ice thickness and the state and thickness of snow; and the modulation of the microwave signature, especially at the highest frequencies, by the freezing of the upper few centimeters of the ice.

  17. Variations of mesoscale and large-scale sea ice morphology in the 1984 Marginal Ice Zone Experiment as observed by microwave remote sensing

    NASA Technical Reports Server (NTRS)

    Campbell, W. J.; Josberger, E. G.; Gloersen, P.; Johannessen, O. M.; Guest, P. S.

    1987-01-01

    The data acquired during the summer 1984 Marginal Ice Zone Experiment in the Fram Strait-Greenland Sea marginal ice zone, using airborne active and passive microwave sensors and the Nimbus 7 SMMR, were analyzed to compile a sequential description of the mesoscale and large-scale ice morphology variations during the period of June 6 - July 16, 1984. Throughout the experiment, the long ice edge between northwest Svalbard and central Greenland meandered; eddies were repeatedly formed, moved, and disappeared but the ice edge remained within a 100-km-wide zone. The ice pack behind this alternately diffuse and compact edge underwent rapid and pronounced variations in ice concentration over a 200-km-wide zone. The high-resolution ice concentration distributions obtained in the aircraft images agree well with the low-resolution distributions of SMMR images.

  18. Wave-Ice interaction in the Marginal Ice Zone: Toward a Wave-Ocean-Ice Coupled Modeling System

    DTIC Science & Technology

    2015-09-30

    MIZ using WW3 (3 frequency bins, ice retreat in August and ice advance in October); Blue (solid): Based on observations near Antarctica by Meylan...1 DISTRIBUTION STATEMENT A. Approved for public release; distribution is unlimited. Wave- Ice interaction in the Marginal Ice Zone: Toward a...Wave-Ocean- Ice Coupled Modeling System W. E. Rogers Naval Research Laboratory, Code 7322 Stennis Space Center, MS 39529 phone: (228) 688-4727

  19. Wave attenuation in the marginal ice zone during LIMEX

    NASA Technical Reports Server (NTRS)

    Liu, Antony K.; Peng, Chih Y.; Vachon, Paris W.

    1991-01-01

    During LIMEX'87 and '89, the CCRS CV-580 aircraft collected SAR (synthetic aperture radar) data over the marginal ice zone off the coast of Newfoundland. Based upon the wavenumber spectra from SAR data, the wave attenuation rate is estimated and compared with a model. The model-data comparisons are reasonably good for the ice conditions during LIMEX (Labrador Ice Margin Experiment). Both model and SAR-derived wave attenuation rates show a roll-over at high wavenumbers.

  20. Glacitectonic deformation around the retreating margin of the last Irish ice sheet

    NASA Astrophysics Data System (ADS)

    Knight, J.

    2008-12-01

    Evidence for ice-marginal glacitectonic shunting and deformation of bedrock slabs is described from three sites around the west coast of Ireland. These sites (Brandon Bay, County Kerry; Pigeon Point, County Mayo; Inishcrone, County Sligo) are all locations where the late Devensian ice margin retreated on land and was confined to within limestone bedrock embayments. At these sites, flat-lying bedrock slabs (< 8 m long) have been dissociated from rockhead and moved seaward (in the direction of ice flow) by glacitectonic shunting. At all of the sites, bedrock slabs have been variously stacked, rotated, deformed into open folds, and brecciated. Separating the bedrock slabs is either a thin layer (< 20 cm) of brecciated and mylonitised cemented bedrock that shows internal folding; or a thicker (< 50 cm) normally-graded diamicton with a fine matrix. Together, the presence of these features suggests oscillation of a polythermal and clean basal ice margin that was strongly associated with basal freeze-on and the presence of proglacial permafrost. Subglacial sediment-laden meltwater was focused from behind the ice margin and through permafrost taliks. It is suggested that hydrofracturing under high hydraulic pressure, and through a frozen-bed ice margin, forced sediment injection into bedrock fractures and bedding planes and away from the ice margin, and that bedrock slabs were moved in part by hydraulic lift as well as thrust-style ice-marginal tectonics. The presence of a mosaic of warm and frozen ice-bed patches, in combination with strong geologic control and meltwater generation from behind the ice margin, can help explain formation of these unusual bedrock slab features.

  1. Glaciological reconstruction of Holocene ice margins in northwestern Greenland

    NASA Astrophysics Data System (ADS)

    Birkel, S. D.; Osterberg, E. C.; Kelly, M. A.; Axford, Y.

    2014-12-01

    The past few decades of climate warming have brought overall margin retreat to the Greenland Ice Sheet. In order to place recent and projected changes in context, we are undertaking a collaborative field-modeling study that aims to reconstruct the Holocene history of ice-margin fluctuation near Thule (~76.5°N, 68.7°W), and also along the North Ice Cap (NIC) in the Nunatarssuaq region (~76.7°N, 67.4°W). Fieldwork reported by Kelly et al. (2013) reveals that ice in the study areas was less extensive than at present ca. 4700 (GIS) and ca. 880 (NIC) cal. years BP, presumably in response to a warmer climate. We are now exploring Holocene ice-climate coupling using the University of Maine Ice Sheet Model (UMISM). Our approach is to first test what imposed climate anomalies can afford steady state ice margins in accord with field data. A second test encompasses transient simulation of the Holocene, with climate boundary conditions supplied by existing paleo runs of the Community Climate System Model version 4 (CCSM4), and a climate forcing signal derived from Greenland ice cores. In both cases, the full ice sheet is simulated at 10 km resolution with nested domains at 0.5 km for the study areas. UMISM experiments are underway, and results will be reported at the meeting.

  2. Holocene ice marginal fluctuations of the Qassimiut lobe in South Greenland

    PubMed Central

    Larsen, Nicolaj K.; Find, Jesper; Kristensen, Anders; Bjørk, Anders A.; Kjeldsen, Kristian K.; Odgaard, Bent V.; Olsen, Jesper; Kjær, Kurt H.

    2016-01-01

    Knowledge about the Holocene evolution of the Greenland ice sheet (GrIS) is important to put the recent observations of ice loss into a longer-term perspective. In this study, we use six new threshold lake records supplemented with two existing lake records to reconstruct the Holocene ice marginal fluctuations of the Qassimiut lobe (QL) – one of the most dynamic parts of the GrIS in South Greenland. Times when the ice margin was close to present extent are characterized by clastic input from the glacier meltwater, whereas periods when the ice margin was behind its present day extent comprise organic-rich sediments. We find that the overall pattern suggests that the central part of the ice lobe in low-lying areas experienced the most prolonged ice retreat from ~9–0.4 cal. ka BP, whereas the more distal parts of the ice lobe at higher elevation re-advanced and remained close to the present extent during the Neoglacial between ~4.4 and 1.8 cal. ka BP. These results demonstrate that the QL was primarily driven by Holocene climate changes, but also emphasises the role of local topography on the ice marginal fluctuations. PMID:26940998

  3. Satellite microwave and in situ observations of the Weddell Sea ice cover and its marginal ice zone

    NASA Technical Reports Server (NTRS)

    Comiso, J. C.; Sullivan, C. W.

    1986-01-01

    The radiative and physical characteristics of the Weddell Sea ice cover and its marginal ice zone are analyzed using multichannel satellite passive microwave data and ship and helicopter observations obtained during the 1983 Antarctic Marine Ecosystem Research. Winter and spring brightness temperatures are examined; spatial variability in the brightness temperatures of consolidated ice in winter and spring cyclic increases and decrease in brightness temperatures of consolidated ice 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. Ice concentrations are derived using the frequency and polarization techniques, and the data are compared with the helicopter and ship observations. Temporal changes in the ice margin structure and the mass balance of fresh water and of biological features of the marginal ice zone are studied.

  4. Waves and mesoscale features in the marginal ice zone

    NASA Technical Reports Server (NTRS)

    Liu, Antony K.; Peng, Chih Y.

    1993-01-01

    Ocean-ice interaction processes in the Marginal Ice Zone (MIZ) by waves and mesoscale features, such as upwelling and eddies, are studied using ERS-1 Synthetic Aperture Radar (SAR) imagery and wave-ice interaction models. Satellite observations of mesoscale features can play a crucial role in ocean-ice interaction study.

  5. Modeling Wave-Ice Interactions in the Marginal Ice Zone

    NASA Astrophysics Data System (ADS)

    Orzech, Mark; Shi, Fengyan; Bateman, Sam; Veeramony, Jay; Calantoni, Joe

    2015-04-01

    The small-scale (O(m)) interactions between waves and ice floes in the marginal ice zone (MIZ) are investigated with a coupled model system. Waves are simulated with the non-hydrostatic finite-volume model NHWAVE (Ma et al., 2012) and ice floes are represented as bonded collections of smaller particles with the discrete element system LIGGGHTS (Kloss et al., 2012). The physics of fluid and ice are recreated as authentically as possible, to allow the coupled system to supplement and/or substitute for more costly and demanding field experiments. The presentation will first describe the development and validation of the coupled system, then discuss the results of a series of virtual experiments in which ice floe and wave characteristics are varied to examine their effects on energy dissipation, MIZ floe size distribution, and ice pack retreat rates. Although Wadhams et al. (1986) suggest that only a small portion (roughly 10%) of wave energy entering the MIZ is reflected, dissipation mechanisms for the remaining energy have yet to be delineated or measured. The virtual experiments are designed to focus on specific properties and processes - such as floe size and shape, collision and fracturing events, and variations in wave climate - and measure their relative roles the transfer of energy and momentum from waves to ice. Questions to be examined include: How is energy dissipated by ice floe collisions, fracturing, and drag, and how significant is the wave attenuation associated with each process? Do specific wave/floe length scale ratios cause greater wave attenuation? How does ice material strength affect the rate of wave energy loss? The coupled system will ultimately be used to test and improve upon wave-ice parameterizations for large-scale climate models. References: >Kloss, C., C. Goniva, A. Hager, S. Amberger, and S. Pirker (2012). Models, algorithms and validation for opensource DEM and CFD-DEM. Progress in Computational Fluid Dynamics 12(2/3), 140-152. >Ma, G

  6. A coupled ice-ocean model of ice breakup and banding in the marginal ice zone

    NASA Technical Reports Server (NTRS)

    Smedstad, O. M.; Roed, L. P.

    1985-01-01

    A coupled ice-ocean numerical model for the marginal ice zone is considered. The model consists of a nonlinear sea ice model and a two-layer (reduced gravity) ocean model. The dependence of the upwelling response on wind stress direction is discussed. The results confirm earlier analytical work. It is shown that there exist directions for which there is no upwelling, while other directions give maximum upwelling in terms of the volume of uplifted water. The ice and ocean is coupled directly through the stress at the ice-ocean interface. An interesting consequence of the coupling is found in cases when the ice edge is almost stationary. In these cases the ice tends to break up a few tenths of kilometers inside of the ice edge.

  7. Submesoscale Sea Ice-Ocean Interactions in Marginal Ice Zones

    NASA Astrophysics Data System (ADS)

    Manucharyan, Georgy E.; Thompson, Andrew F.

    2017-12-01

    Signatures of ocean eddies, fronts, and filaments are commonly observed within marginal ice zones (MIZs) from satellite images of sea ice concentration, and in situ observations via ice-tethered profilers or underice gliders. However, localized and intermittent sea ice heating and advection by ocean eddies are currently not accounted for in climate models and may contribute to their biases and errors in sea ice forecasts. Here, we explore mechanical sea ice interactions with underlying submesoscale ocean turbulence. We demonstrate that the release of potential energy stored in meltwater fronts can lead to energetic submesoscale motions along MIZs with spatial scales O(10 km) and Rossby numbers O(1). In low-wind conditions, cyclonic eddies and filaments efficiently trap the sea ice and advect it over warmer surface ocean waters where it can effectively melt. The horizontal eddy diffusivity of sea ice mass and heat across the MIZ can reach O(200 m2 s-1). Submesoscale ocean variability also induces large vertical velocities (order 10 m d-1) that can bring relatively warm subsurface waters into the mixed layer. The ocean-sea ice heat fluxes are localized over cyclonic eddies and filaments reaching about 100 W m-2. We speculate that these submesoscale-driven intermittent fluxes of heat and sea ice can contribute to the seasonal evolution of MIZs. With the continuing global warming and sea ice thickness reduction in the Arctic Ocean, submesoscale sea ice-ocean processes are expected to become increasingly prominent.

  8. Percutaneous Renal Cryoablation: Short-Axis Ice-Ball Margin as a Predictor of Outcome.

    PubMed

    Ge, Benjamin H; Guzzo, Thomas J; Nadolski, Gregory J; Soulen, Michael C; Clark, Timothy W I; Malkowicz, Stanley B; Wein, Alan J; Hunt, Stephen J; Stavropoulos, S William

    2016-03-01

    To determine if CT characteristics of intraprocedural ice balls correlate with outcomes after cryoablation. A retrospective review was performed on 63 consecutive patients treated with renal cryoablation. Preprocedural and intraprocedural images were used to identify the size and location of renal tumors and ice balls as well as the tumor coverage and ice-ball margins. Review of follow-up imaging (1 mo and then 3-6-mo intervals) distinguished successful ablations from cases of residual tumor. Patients who underwent successful ablation (n = 50; 79%) had a mean tumor diameter of 2.5 cm (range, 0.9-4.3 cm) and mean ice-ball margin of 0.4 cm (range, 0.2-1.2 cm). Patients with residual tumor (n = 13; 21%) had a mean tumor diameter of 3.8 cm (range, 1.8-4.5 cm) and mean ice-ball margin of -0.4 cm (range, -0.9 to 0.4 cm). Residual and undertreated tumors were larger and had smaller ice-ball margins than successfully treated tumors (P < .01). Ice-ball diameters were significantly smaller after image reformatting (P < .01). Ice-ball margins of 0.15 cm had 90% sensitivity, 92% specificity, and 98% positive predictive value for successful ablation. Success was independent of tumor location or number of cryoprobes. Ice-ball margin and real-time intraprocedural reformatting could be helpful in predicting renal cryoablation outcomes. Although a 0.5-cm margin is preferred, a well-centered ice ball with a short-axis margin greater than 0.15 cm strongly correlated with successful ablation. Copyright © 2016 SIR. Published by Elsevier Inc. All rights reserved.

  9. Holocene Fluctuations of North Ice Cap, a Proxy for Climate Conditions along the Northwestern Margin of the Greenland Ice Sheet

    NASA Astrophysics Data System (ADS)

    Kelly, M. A.; Osterberg, E. C.; Lasher, G. E.; Farnsworth, L. B.; Howley, J. A.; Axford, Y.; Zimmerman, S. R. H.

    2015-12-01

    North Ice Cap (~76.9°N, 68°W, summit elevation 1322 m asl), a small, independent ice cap in northwestern Greenland, is located within ~25 km of the Greenland Ice Sheet margin and Harald Molkte Bræ outlet glacier. We present geochronological, geomorphic and sedimentological data constraining the Holocene extents of North Ice Cap and suggest that its past fluctuations can be used as a proxy for climate conditions along the northwestern margin of the Greenland Ice Sheet. Prior work by Goldthwait (1960) used glacial geomorphology and radiocarbon ages of subfossil plants emerging along shear planes in the ice cap margin to suggest that that North Ice Cap was not present during the early Holocene and nucleated in the middle to late Holocene time, with the onset of colder conditions. Subfossil plants emerging at shear planes in the North Ice Cap margin yield radiocarbon ages of ~4.8-5.9 cal kyr BP (Goldthwait, 1960) and ~AD 1000-1350 (950-600 cal yr BP), indicating times when the ice cap was smaller than at present. In situ subfossil plants exposed by recent ice cap retreat date to ~AD 1500-1840 (450-110 cal yr BP) and indicate small fluctuations of the ice cap margin. 10Be ages of an unweathered, lichen-free drift <100 m from the present North Ice Cap margin range from ~500 to 8000 yrs ago. We suggest that the drift was deposited during the last ~500 yrs and that the older 10Be ages are influenced by 10Be inherited from a prior period of exposure. We also infer ice cap fluctuations using geochemical data from a Holocene-long sediment core from Deltasø, a downstream lake that currently receives meltwater from North Ice Cap. The recent recession of the North Ice Cap margin influenced a catastrophic drainage of a large proglacial lake, Søndre Snesø, that our field team documented in August 2012. To our knowledge, this is the first significant lowering of Søndre Snesø in historical time.

  10. Basal Freeze-on: An Active Component of Hydrology from the Ice Divide to the Margin

    NASA Astrophysics Data System (ADS)

    Bell, R. E.; Tinto, K. J.; Abdi, A.; Creyts, T. T.; Wolovick, M.; Das, I.; Ferraccioli, F.; Csatho, B. M.

    2012-12-01

    Greenland, we have identified 14 distinct basal ice packages over a wide region. The accumulation rate (~17 cm/yr) and ice velocity (~5-200m/yr) are higher than East Antarctica. These accretion bodies are 10-50 km wide, up to 940m thick and can be traced up to 140 km. The volume of the ice enclosed by the accretion ice reflector units is ~70-300 km3. We estimate that the freeze-on process in Petermann has been active for at least 6,000yr. Water has been mapped beneath much of the Greenland ice sheet and adjacent to the inland freeze-on site flat bright reflectors are interpreted as basal water. The onset of fast flow in Petermann Glacier is associated with the development of the thickest unit of freeze-on ice. Other areas of Greenland also have basal freeze-on ice. North of Jakobshavn Isbrae where the ice sheet is ~1000 m thick, evidence exists for a nearly 10 km wide, 200 m thick unit of basal ice in airborne radar. Located close to the site where basal freeze-on outcrops at the ice sheet margin at Pakitsoq, this unit may be the result of freeze-on of water draining from a supraglacial lake. Basal freeze-on is a critical component of subglacial hydrology. The evidence for large scale freeze-on East Antarctica and many areas of Greenland indicates widespread modification of the base of the ice sheet by basal hydrology.

  11. Reconciling records of ice streaming and ice margin retreat to produce a palaeogeographic reconstruction of the deglaciation of the Laurentide Ice Sheet

    NASA Astrophysics Data System (ADS)

    Margold, Martin; Stokes, Chris R.; Clark, Chris D.

    2018-06-01

    This paper reconstructs the deglaciation of the Laurentide Ice Sheet (LIS; including the Innuitian Ice Sheet) from the Last Glacial Maximum (LGM), with a particular focus on the spatial and temporal variations in ice streaming and the associated changes in flow patterns and ice divides. We build on a recent inventory of Laurentide ice streams and use an existing ice margin chronology to produce the first detailed transient reconstruction of the ice stream drainage network in the LIS, which we depict in a series of palaeogeographic maps. Results show that the drainage network at the LGM was similar to modern-day Antarctica. The majority of the ice streams were marine terminating and topographically-controlled and many of these continued to function late into the deglaciation, until the ice sheet lost its marine margin. Ice streams with a terrestrial ice margin in the west and south were more transient and ice flow directions changed with the build-up, peak-phase and collapse of the Cordilleran-Laurentide ice saddle. The south-eastern marine margin in Atlantic Canada started to retreat relatively early and some of the ice streams in this region switched off at or shortly after the LGM. In contrast, the ice streams draining towards the north-western and north-eastern marine margins in the Beaufort Sea and in Baffin Bay appear to have remained stable throughout most of the Late Glacial, and some of them continued to function until after the Younger Dryas (YD). The YD influenced the dynamics of the deglaciation, but there remains uncertainty about the response of the ice sheet in several sectors. We tentatively ascribe the switching-on of some major ice streams during this period (e.g. M'Clintock Channel Ice Stream at the north-west margin), but for other large ice streams whose timing partially overlaps with the YD, the drivers are less clear and ice-dynamical processes, rather than effects of climate and surface mass balance are viewed as more likely drivers. Retreat

  12. Submesoscale sea ice-ocean interactions in marginal ice zones

    NASA Astrophysics Data System (ADS)

    Thompson, A. F.; Manucharyan, G.

    2017-12-01

    Signatures of ocean eddies, fronts and filaments are commonly observed within the marginal ice zones (MIZ) from satellite images of sea ice concentration, in situ observations via ice-tethered profilers or under-ice gliders. Localized and intermittent sea ice heating and advection by ocean eddies are currently not accounted for in climate models and may contribute to their biases and errors in sea ice forecasts. Here, we explore mechanical sea ice interactions with underlying submesoscale ocean turbulence via a suite of numerical simulations. We demonstrate that the release of potential energy stored in meltwater fronts can lead to energetic submesoscale motions along MIZs with sizes O(10 km) and Rossby numbers O(1). In low-wind conditions, cyclonic eddies and filaments efficiently trap the sea ice and advect it over warmer surface ocean waters where it can effectively melt. The horizontal eddy diffusivity of sea ice mass and heat across the MIZ can reach O(200 m2 s-1). Submesoscale ocean variability also induces large vertical velocities (order of 10 m day-1) that can bring relatively warm subsurface waters into the mixed layer. The ocean-sea ice heat fluxes are localized over cyclonic eddies and filaments reaching about 100 W m-2. We speculate that these submesoscale-driven intermittent fluxes of heat and sea ice can potentially contribute to the seasonal evolution of MIZs. With continuing global warming and sea ice thickness reduction in the Arctic Ocean, as well as the large expanse of thin sea ice in the Southern Ocean, submesoscale sea ice-ocean processes are expected to play a significant role in the climate system.

  13. Marginal Ice Zone Processes Observed from Unmanned Aerial Systems

    NASA Astrophysics Data System (ADS)

    Zappa, C. J.

    2015-12-01

    Recent years have seen extreme changes in the Arctic. Marginal ice zones (MIZ), or areas where the "ice-albedo feedback" driven by solar warming is highest and ice melt is extensive, may provide insights into the extent of these changes. Furthermore, MIZ play a central role in setting the air-sea CO2 balance making them a critical component of the global carbon cycle. Incomplete understanding of how the sea-ice modulates gas fluxes renders it difficult to estimate the carbon budget in MIZ. Here, we investigate the turbulent mechanisms driving mixing and gas exchange in leads, polynyas and in the presence of ice floes using both field and laboratory measurements. Measurements from unmanned aerial systems (UAS) in the marginal ice zone were made during 2 experiments: 1) North of Oliktok Point AK in the Beaufort Sea were made during the Marginal Ice Zone Ocean and Ice Observations and Processes EXperiment (MIZOPEX) in July-August 2013 and 2) Fram Strait and Greenland Sea northwest of Ny-Ålesund, Svalbard, Norway during the Air-Sea-Ice Physics and Biogeochemistry Experiment (ASIPBEX) April - May 2015. We developed a number of new payloads that include: i) hyperspectral imaging spectrometers to measure VNIR (400-1000 nm) and NIR (900-1700 nm) spectral radiance; ii) net longwave and net shortwave radiation for ice-ocean albedo studies; iii) air-sea-ice turbulent fluxes as well as wave height, ice freeboard, and surface roughness with a LIDAR; and iv) drone-deployed micro-drifters (DDµD) deployed from the UAS that telemeter temperature, pressure, and RH as it descends through the atmosphere and temperature and salinity of the upper meter of the ocean once it lands on the ocean's surface. Visible and IR imagery of melting ice floes clearly defines the scale of the ice floes. The IR imagery show distinct cooling of the skin sea surface temperature (SST) as well as an intricate circulation and mixing pattern that depends on the surface current, wind speed, and near

  14. A coupled ice-ocean model of upwelling in the marginal ice zone

    NASA Technical Reports Server (NTRS)

    Roed, L. P.; Obrien, J. J.

    1983-01-01

    A dynamical coupled ice-ocean numerical model for the marginal ice zone (MIZ) is suggested and used to study upwelling dynamics in the MIZ. The nonlinear sea ice model has a variable ice concentration and includes internal ice stress. The model is forced by stresses on the air/ocean and air/ice surfaces. The main coupling between the ice and the ocean is in the form of an interfacial stress on the ice/ocean interface. The ocean model is a linear reduced gravity model. The wind stress exerted by the atmosphere on the ocean is proportional to the fraction of open water, while the interfacial stress ice/ocean is proportional to the concentration of ice. A new mechanism for ice edge upwelling is suggested based on a geostrophic equilibrium solution for the sea ice medium. The upwelling reported in previous models invoking a stationary ice cover is shown to be replaced by a weak downwelling due to the ice motion. Most of the upwelling dynamics can be understood by analysis of the divergence of the across ice edge upper ocean transport. On the basis of numerical model, an analytical model is suggested that reproduces most of the upwelling dynamics of the more complex numerical model.

  15. A comparison of radiation budgets in the Fram Strait marginal ice zone

    NASA Technical Reports Server (NTRS)

    Francis, Jennifer A.; Katsaros, Kristina B.; Ackerman, Thomas P.; Lind, Richard J.; Davidson, Kenneth L.

    1991-01-01

    Results are presented from calculations of radiation budgets for the sea-ice and the open-water regimes in the marginal ice zone (MIZ) of the Fram Strait, from measurements of surface irradiances and meteorological conditions made during the 1984 Marginal Ice Zone Experiment. Simultaneous measurements on either side of the ice edge allowed a comparison of the open-water and the sea-ice environments. The results show significant differences between the radiation budgets of the two regimes in the MIZ. The open water absorbed twice as much radiation as did the ice, and the mean cooling rate of the atmosphere over water was approximately 15 percent larger than that over ice. Calculated fluxes and atmospheric cooling rates were found to compare well with available literature data.

  16. Deglaciation-induced uplift of the Petermann glacier ice margin observed with InSAR

    NASA Astrophysics Data System (ADS)

    Lu, Q.; Amelung, F.; Wdowinski, S.

    2016-12-01

    The Greenland ice sheet is rapidly shrinking with the fastest retreat and thinning occurring at the ice sheet margin and near the outlet glaciers. The changes of the ice mass cause an elastic response of the bedrock. Ice mass loss during the summer months is associated with uplift, whereas ice mass increase during the winter months is associated with subsidence.The German TerraSAR-X and TanDEM-X satellites have systematically observed selected sites along the Greenland Petermann ice sheet margin since summer 2012. Here we present ground deformation observations obtained using an InSAR time-series approach based on small baseline interferograms. We observed rapid deglaciation-induced uplift on naked bedrock near the Petermann glacier ice margin Deformation observed by InSAR is consistent with GPS vertical observations. The time series displacement data reveal not only net uplift but also the seasonal variations. There is no strong relative between displacement changes and SMB ice mass change. The seasonal variations in local area may caused by both nearby SMB changes and ice dynamic changes.

  17. Retreat of northern margins of George VI and Wilkins Ice Shelves, Antarctic Peninsula

    USGS Publications Warehouse

    Lucchitta, B.K.; Rosanova, C.E.

    1998-01-01

    The George VI and Wilkins Ice Shelves are considered at risk of disintegration due to a regional atmospheric warming trend on the Antarctic Peninsula. Retreat of the northern margin of the George VI Ice Shelf has been observed previously, but the Wilkins Ice Shelf was thought to be stable. We investigated the positions of the northern fronts of these shelves from the literature and looked for changes on 1974 Landsat and 1992 and 1995 European remote-sensing satellite (ERS) synthetic aperture radar images. Our investigation shows that the northern George VI Ice Shelf lost a total of 906 km2 between 1974 and 1992, and an additional 87 km2 by 1995. The northern margin of the Wilkins Ice Shelf lost 796 km2 between 1990 and 1992, and another 564 km2 between 1992 and 1995. Armadas of tabular icebergs were visible in front of this shelf in the ERS images. These two ice shelves mark the southernmost documented conspicuous retreat of ice-shelf margins.

  18. Investigations of Spatial and Temporal Variability of Ocean and Ice Conditions in and Near the Marginal Ice Zone. The “Marginal Ice Zone Observations and Processes Experiment” (MIZOPEX) Final Campaign Summary

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

    DeMott, P. J.; Hill, T. C.J.

    Despite the significance of the marginal ice zones of the Arctic Ocean, basic parameters such as sea surface temperature (SST) and a range of sea-ice characteristics are still insufficiently understood in these areas, and especially so during the summer melt period. The field campaigns summarized here, identified collectively as the “Marginal Ice Zone Ocean and Ice Observations and Processes Experiment” (MIZOPEX), were funded by U.S. National Aeronautic and Space Administration (NASA) with the intent of helping to address these information gaps through a targeted, intensive observation field campaign that tested and exploited unique capabilities of multiple classes of unmanned aerialmore » systems (UASs). MIZOPEX was conceived and carried out in response to NASA’s request for research efforts that would address a key area of science while also helping to advance the application of UASs in a manner useful to NASA for assessing the relative merits of different UASs. To further exercise the potential of unmanned systems and to expand the science value of the effort, the field campaign added further challenges such as air deployment of miniaturized buoys and coordinating missions involving multiple aircraft. Specific research areas that MIZOPEX data were designed to address include relationships between ocean skin temperatures and subsurface temperatures and how these evolve over time in an Arctic environment during summer; variability in sea-ice conditions such as thickness, age, and albedo within the marginal ice zone (MIZ); interactions of SST, salinity, and ice conditions during the melt cycle; and validation of satellite-derived SST and ice concentration fields provided by satellite imagery and models.« less

  19. Cenozoic ice sheet history from East Antarctic Wilkes Land continental margin sediments

    USGS Publications Warehouse

    Escutia, C.; De Santis, L.; Donda, F.; Dunbar, R.B.; Cooper, A. K.; Brancolini, Giuliano; Eittreim, S.L.

    2005-01-01

    The long-term history of glaciation along the East Antarctic Wilkes Land margin, from the time of the first arrival of the ice sheet to the margin, through the significant periods of Cenozoic climate change is inferred using an integrated geophysical and geological approach. We postulate that the first arrival of the ice sheet to the Wilkes Land margin resulted in the development of a large unconformity (WL-U3) between 33.42 and 30 Ma during the early Oligocene cooling climate trend. Above WL-U3, substantial margin progradation takes place with early glacial strata (e.g., outwash deposits) deposited as low-angle prograding foresets by temperate glaciers. The change in geometry of the prograding wedge across unconformity WL-U8 is interpreted to represent the transition, at the end of the middle Miocene "climatic optimum" (14-10 Ma), from a subpolar regime with dynamic ice sheets (i.e., ice sheets come and go) to a regime with persistent but oscillatory ice sheets. The steep foresets above WL-U8 likely consist of ice proximal sediments (i.e., water-lain till and debris flows) deposited when grounded ice-sheets extended into the shelf. On the continental rise, shelf progradation above WL-U3 results in an up-section increase in the energy of the depositional environment (i.e., seismic facies indicative of more proximal turbidite and of bottom contour current deposition from the deposition of the lower WL-S5 sequence to WL-S7). Maximum rates of sediment delivery to the rise occur during the development of sequences WL-S6 and WL-S7, which we infer to be of middle Miocene age. During deposition of the two uppermost sequences, WL-S8 and WL-S9, there is a marked decrease in the sediment supply to the lower continental rise and a shift in the depocenters to more proximal areas of the margin. We believe WL-S8 records sedimentation during the final transition from a dynamic to a persistent but oscillatory ice sheet in this margin (14-10 Ma). Sequence WL-S9 forms under a polar

  20. 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.

  1. Coupling of Waves, Turbulence and Thermodynamics Across the Marginal Ice Zone

    DTIC Science & Technology

    2013-09-30

    under-predict the observed trend of declining sea ice area over the last decade. A potential explanation for this under-prediction is that models...are missing important feedbacks within the ocean- ice system. Results from the proposed research will contribute to improving the upper ocean and sea ...and solar-radiation-driven thermodynamic forcing in the marginal ice zone. Within the MIZ, the ocean- ice - albedo feedback mechanism is coupled to ice

  2. Sensitivity studies with a coupled ice-ocean model of the marginal ice zone

    NASA Technical Reports Server (NTRS)

    Roed, L. P.

    1983-01-01

    An analytical coupled ice-ocean model is considered which is forced by a specified wind stress acting on the open ocean as well as the ice. The analysis supports the conjecture that the upwelling dynamics at ice edges can be understood by means of a simple analytical model. In similarity with coastal problems it is shown that the ice edge upwelling is determined by the net mass flux at the boundaries of the considered region. The model is used to study the sensitivity of the upwelling dynamics in the marginal ice zone to variation in the controlling parameters. These parameters consist of combinations of the drag coefficients used in the parameterization of the stresses on the three interfaces atmosphere-ice, atmosphere-ocean, and ice-ocean. The response is shown to be sensitive to variations in these parameters in that one set of parameters may give upwelling while a slightly different set of parameters may give downwelling.

  3. Proglacial deltaic landforms and stratigraphic architecture as a proxy for reconstructing past ice-sheet margin positions

    NASA Astrophysics Data System (ADS)

    Dietrich, Pierre; Ghienne, Jean-François; Normandeau, Alexandre; Lajeunesse, Patrick

    2016-04-01

    Deltaic landforms and related stratigraphic architectures are frequently used as proxy for reconstruction of past continental or marine environmental evolutions. Indeed, in addition to autocyclic processes, emplacement of deltaic systems is primarily controlled by changes in sediment supply and relative sea-level (RSL). In our study, we investigated several proglacial deltaic complexes emplaced since the last deglaciation over more than 700 km along the St. Lawrence North Shore (Québec, Canada). Their geomorphic and stratigraphic records allowed us to infer the retreat pattern of the Laurentide Ice Sheet fronts. Field investigation of representative deltaic complexes revealed an archetypal morphostratigraphic evolution forced by the retreat of the ice margin in a context of falling RSL (glacio-isostatic rebound). The base of the stratigraphic successions consists of outwash fan deposits emplaced in the early deglaciation when ice margin stillstanded immediately beyond the depositional area. The middle part of the succession consists of proglacial delta deposits corresponding to the retreat of the ice margin in the hinterland. At that time, glaciogenic supplies allowed an active progradation preventing fluvial entrenchment in spite of the forced regressive context. The upper part of the succession consists of staged shoreline deposits reworking the rim of the proglacial deltas. These deposits mark the retreat of the ice margin from the drainage basin and the subsequent drop in glaciogenics. Important fluvial entrenchment occurred in the same time, though rates of RSL fall were reduced. We generalize this stratigraphic framework by using solely the landforms (from DEM, aerial photographs or satellite images) tied to deltaic complex developments along the St. Lawrence North Shore. This approach permits an integrated study at the scale of the whole basin even where no field data is available. Recognizing the three steps evidenced from the stratigraphic record ads

  4. Ocean-ice interaction in the marginal ice zone using synthetic aperture radar imagery

    NASA Technical Reports Server (NTRS)

    Liu, Antony K.; Peng, Chich Y.; Weingartner, Thomas J.

    1994-01-01

    Ocean-ice interaction processes in the marginal ice zone (MIZ) by wind, waves, and mesoscale features, such as up/downwelling and eddies are studied using Earth Remote-Sensing Satellite (ERS) 1 synthetic aperture radar (SAR) images and an ocean-ice interaction model. A sequence of seven SAR images of the MIZ in the Chukchi Sea with 3 or 6 days interval are investigated for ice edge advance/retreat. Simultaneous current measurements from the northeast Chukchi Sea, as well as the Barrow wind record, are used to interpret the MIZ dynamics. SAR spectra of waves in ice and ocean waves in the Bering and Chukchi Sea are compared for the study of wave propagation and dominant SAR imaging mechanism. By using the SAR-observed ice edge configuration and wind and wave field in the Chukchi Sea as inputs, a numerical simulation has been performed with the ocean-ice interaction model. After 3 days of wind and wave forcing the resulting ice edge configuration, eddy formation, and flow velocity field are shown to be consistent with SAR observations.

  5. Dynamic Inland Propagation of Thinning Due to Ice Loss at the Margins of the Greenland Ice Sheet

    NASA Technical Reports Server (NTRS)

    Wang, Wei Li; Li, Jun J.; Zwally, H. Jay

    2012-01-01

    Mass-balance analysis of the Greenland ice sheet based on surface elevation changes observed by the European Remote-sensing Satellite (ERS) (1992-2002) and Ice, Cloud and land Elevation Satellite (ICESat) (2003-07) indicates that the strongly increased mass loss at lower elevations (<2000 m) of the ice sheet, as observed during 2003-07, appears to induce interior ice thinning at higher elevations. In this paper, we perform a perturbation experiment with a three-dimensional anisotropic ice-flow model (AIF model) to investigate this upstream propagation. Observed thinning rates in the regions below 2000m elevation are used as perturbation inputs. The model runs with perturbation for 10 years show that the extensive mass loss at the ice-sheet margins does in fact cause interior thinning on short timescales (i.e. decadal). The modeled pattern of thinning over the ice sheet agrees with the observations, which implies that the strong mass loss since the early 2000s at low elevations has had a dynamic impact on the entire ice sheet. The modeling results also suggest that even if the large mass loss at the margins stopped, the interior ice sheet would continue thinning for 300 years and would take thousands of years for full dynamic recovery.

  6. Ice Sheet History from Antarctic Continental Margin Sediments: The ANTOSTRAT Approach

    USGS Publications Warehouse

    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.

    1998-01-01

    The Antarctic Ice Sheet is today an important part of the global climate engine, and probably has been so for most of its long existence. However, the details of its history are poorly known, despite the measurement and use, over two decades, of low-latitude proxies of ice sheet volume. An additional way of determining ice sheet history is now available, based on understanding terrigenous sediment transport and deposition under a glacial regime. It requires direct sampling of the prograded wedge of glacial sediments deposited at the Antarctic continental margin (and of derived sediments on the continental rise) at a small number of key sites, and combines the resulting data using numerical models of ice sheet development. The new phase of sampling is embodied mainly in a suite of proposals to the Ocean Drilling Program, generated by separate regional proponent groups co-ordinated through ANTOSTRAT (the Antarctic Offshore Acoustic Stratigraphy initiative). The first set of margin sites has now been drilled as ODP Leg 178 to the Antarctic 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 Antarctic 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 Antarctic Peninsula. These and similar sites from around the Antarctic margin are a valuable resource when linked with ice cores and equivalent sections at lower latitude sites for studies of decadal and millenial-scale climate variation.

  7. Advancing land-terminating ice margin in North Greenland - characteristics, evolution, and first field measurements

    NASA Astrophysics Data System (ADS)

    Steiner, J. F.; Prinz, R.; Abermann, J.

    2017-12-01

    More than 40% of the ice sheet in North Greenland terminate on land, however the characteristics of this ice margin and response to a changing climate have so far received little attention. While land-terminating ice cliffs are a feature commonly found and studied in other regions, detailed investigations in Greenland were only carried out more than six decades ago in the Thule area (Red Rock, Northwest Greenland). These studies showed a continuous advance at one location over multiple years, while the local mass balance was reported negative. The purpose of our study is to revisit the location previously studied and extend the analysis to the complete Northern ice margin employing newly available high-resolution digital terrain models (Arctic DEM). First results show that the advance at Red Rock is indeed long-term, continuing unabated today at rates of up to several meter per year. Similar magnitudes were found for large other stretches along the ice margin. With our study we aim to show (a) the main characteristics of the land-terminating ice margin in Northern Greenland, namely its slope and aspect distribution and comparison to spatial datasets of flow velocity and mass balance and (b) to provide further explanations of physical processes driving the advance. We have therefore mapped the complete ice margin and present the first results of this analysis. First field work provides new data on energy fluxes and ice temperatures at the Red Rock site as well as high resolution DEMs obtained with the use of UAVs.

  8. Firn thickness variations across the Northeast Greenland Ice Stream margins indicating nonlinear densification rates

    NASA Astrophysics Data System (ADS)

    Riverman, K. L.; Anandakrishnan, S.; Alley, R. B.; Peters, L. E.; Christianson, K. A.; Muto, A.

    2013-12-01

    Northeast Greenland Ice Stream (NEGIS) is the largest ice stream in Greenland, draining approximately 8.4% of the ice sheet's area. The flow pattern and stability mechanism of this ice stream are unique to others in Greenland and Antarctica, and merit further study to ascertain the sensitivity of this ice stream to future climate change. Geophysical methods are valuable tools for this application, but their results are sensitive to the structure of the firn and any spatial variations in firn properties across a given study region. Here we present firn data from a 40-km-long seismic profile across the upper reaches of NEGIS, collected in the summer of 2012 as part of an integrated ground-based geophysical survey. We find considerable variations in firn thickness that are coincident with the ice stream shear margins, where a thinner firn layer is present within the margins, and a thicker, more uniform firn layer is present elsewhere in our study region. Higher accumulation rates in the marginal surface troughs due to drift-snow trapping can account for some of this increased densification; however, our seismic results also highlight enhanced anisotropy within the firn and upper ice column that is confined to narrow bands within the shear margins. We thus interpret these large firn thickness variations and abrupt changes in anisotropy as indicators of firn densification dependent on the effective stress state as well as the overburden pressure, suggesting that the strain rate increases nonlinearly with stress across the shear margins. A GPS strain grid maintained for three weeks across both margins observed strong side shearing, with rapid stretching and then compression along particle paths, indicating large deviatoric stresses in the margins. This work demonstrates the importance of developing a high-resolution firn densification model when conducting geophysical field work in regions possessing a complex ice flow history; it also motivates the need for a more

  9. A comparison of Holocene fluctuations of the eastern and western margins of the Greenland Ice Sheet

    NASA Astrophysics Data System (ADS)

    Levy, L.; Kelly, M. A.; Lowell, T. V.; Hall, B. L.; Applegate, P. J.; Howley, J.; Axford, Y.

    2013-12-01

    Determining how the Greenland Ice Sheet (GrIS) responded to past temperature fluctuations is important for assessing its future stability in a changing climate. We present a record of the Holocene extents of the western GrIS margin near Kangerlussuaq (67.0°N, 50.7°W) and compare this with the past fluctuations of Bregne ice cap (71°N, 25.6° W), a small ice cap in the Scoresby Sund region 90 km from the eastern GrIS margin, to examine the mechanisms that influenced past ice margin fluctuations. The past extents of the Bregne ice cap are a proxy for the climatic conditions that influenced the nearby GrIS margin. We used glacial geomorphic mapping, 10Be dating of boulders and bedrock, and sediment cores from proglacial and non-glacial lakes. In western Greenland, 10Be ages on the Keglen moraines, 13 km west of the current GrIS margin and the Ørkendalen moraines, ≤2 km west of the current ice margin date to 7.3 × 0.1 ka (n=6) and 6.8 × 0.3 ka (n=9), respectively. Fresh moraines, ≤50 m from the current ice margin date to AD 1830-1950 and are likely associated with advances during the Little Ice Age (LIA). In some areas, the LIA moraines lie stratigraphically above the Ørkendalen moraines, indicating the GrIS was inboard of the Ørkendalen limit from 6.8 ka to the 20th century. In eastern Greenland, 10Be ages show that Bregne ice cap retreated within its late Holocene limit by 10.7 ka. A lack of clastic sediment in a proglacial lake suggests the ice cap was smaller or completely absent from ~10-2.6 ka. A snowline analysis indicates that temperatures ~0.5°C warmer than present would render the entire ice cap into an ablation zone. Glacial silts in the proglacial lake at ~2.6 and ~1.9 cal kyr BP to present indicate advances of Bregne ice cap. Fresh moraines ≤200 m of Bregne ice cap were deposited ≤2.6 cal kyr BP and mark the largest advance of the Holocene. Both the western GrIS margin and Bregne ice cap were influenced by Northern Hemisphere summer

  10. Local Effects of Ice Floes on Skin Sea Surface Temperature in the Marginal Ice Zone from UAVs

    NASA Astrophysics Data System (ADS)

    Zappa, C. J.; Brown, S.; Emery, W. J.; Adler, J.; Wick, G. A.; Steele, M.; Palo, S. E.; Walker, G.; Maslanik, J. A.

    2013-12-01

    Recent years have seen extreme changes in the Arctic. Particularly striking are changes within the Pacific sector of the Arctic Ocean, and especially in the seas north of the Alaskan coast. These areas have experienced record warming, reduced sea ice extent, and loss of ice in areas that had been ice-covered throughout human memory. Even the oldest and thickest ice types have failed to survive through the summer melt period in areas such as the Beaufort Sea and Canada Basin, and fundamental changes in ocean conditions such as earlier phytoplankton blooms may be underway. Marginal ice zones (MIZ), or areas where the "ice-albedo feedback" driven by solar warming is highest and ice melt is extensive, may provide insights into the extent of these changes. Airborne remote sensing, in particular InfraRed (IR), offers a unique opportunity to observe physical processes at sea-ice margins. It permits monitoring the ice extent and coverage, as well as the ice and ocean temperature variability. It can also be used for derivation of surface flow field allowing investigation of turbulence and mixing at the ice-ocean interface. Here, we present measurements of visible and IR imagery of melting ice floes in the marginal ice zone north of Oliktok Point AK in the Beaufort Sea made during the Marginal Ice Zone Ocean and Ice Observations and Processes EXperiment (MIZOPEX) in July-August 2013. The visible and IR imagery were taken from the unmanned airborne vehicle (UAV) ScanEagle. The visible imagery clearly defines the scale of the ice floes. The IR imagery show distinct cooling of the skin sea surface temperature (SST) as well as a intricate circulation and mixing pattern that depends on the surface current, wind speed, and near-surface vertical temperature/salinity structure. Individual ice floes develop turbulent wakes as they drift and cause transient mixing of an influx of colder surface (fresh) melt water. The upstream side of the ice floe shows the coldest skin SST, and

  11. Passive microwave characteristics of the Bering Sea ice cover during Marginal Ice Zone Experiment (MIZEX) West

    NASA Technical Reports Server (NTRS)

    Cavalieri, D. J.; Gloersen, P.; Wilheit, T. T.; Calhoon, C.

    1984-01-01

    Passive microwave measurements of the Bering Sea were made with the NASA CV-990 airborne laboratory during February. Microwave data were obtained with imaging and dual-polarized, fixed-beam radiometers in a range of frequencies from 10 to 183 GHz. The high resolution imagery at 92 GHz provides a particularly good description of the marginal ice zone delineating regions of open water, ice compactness, and ice-edge structure. Analysis of the fixed-beam data shows that spectral differences increase with a decrease in ice thickness. Polarization at 18 and 37 GHz distinguishes among new, young, and first-year sea ice types.

  12. Extensive dynamic thinning on the margins of the Greenland and Antarctic ice sheets.

    PubMed

    Pritchard, Hamish D; Arthern, Robert J; Vaughan, David G; Edwards, Laura A

    2009-10-15

    Many glaciers along the margins of the Greenland and Antarctic ice sheets are accelerating and, for this reason, contribute increasingly to global sea-level rise. Globally, ice losses contribute approximately 1.8 mm yr(-1) (ref. 8), but this could increase if the retreat of ice shelves and tidewater glaciers further enhances the loss of grounded ice or initiates the large-scale collapse of vulnerable parts of the ice sheets. Ice 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 ice-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 (Ice, Cloud and land Elevation Satellite) laser altimetry to map change along the entire grounded margins of the Greenland and Antarctic ice sheets. To isolate the dynamic signal, we compare rates of elevation change from both fast-flowing and slow-flowing ice 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 Antarctic grounding lines, has endured for decades after ice-shelf collapse, penetrates far into the interior of each ice sheet and is spreading as ice 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 ice sheets currently result from glacier dynamics at ocean margins.

  13. Timing and east-west correlation of south Swedish ice marginal lines during the Late Weichselian

    NASA Astrophysics Data System (ADS)

    Lundqvist, Jan; Wohlfarth, Barbara

    2000-01-01

    The retreat of the Late Weichselian ice sheet over the southern part of Sweden is marked along the southwest coast by distinct marginal moraine ridges. Their timing can directly and indirectly be assessed based on a number of radiocarbon dates and pollen stratigraphic investigations on lake sediment sequences adjacent to the ice marginal lines. Along the southeastern side of the peninsula, the ice recession has been reconstructed based on a combination of clay-varve chronology, pollen and radiocarbon stratigraphy. A morphological correlation of ice marginal lines between the west and east coast is problematic since the distinct west-coast moraines cannot be followed through the central part of the peninsula towards the east coast. This paper is an attempt to reconstruct an age-equivalent west-east extension of the ice-recession lines on the basis of existing data sets. For our correlation we use calibrated radiocarbon ages for ice marginal deposits on the west coast and compare these with a partly radiocarbon-dated clay-varve chronology on the east coast. We conclude that the two oldest moraines on the west coast formed at ˜18,000-16,000 and ˜15,400-14,500 cal yr BP, respectively. During the following rapid deglaciation, which may have coincided with the beginning of the Bølling pollen zone, large parts of southernmost Sweden became ice free, except for higher elevated areas, where stagnant ice remained for another 400-500 yr. A best guess is that the formation of the next younger ice marginal lines may have occurred at ˜14,400-14,200, ˜14,200 and ˜13,400 cal yr BP and during the Younger Dryas cold event.

  14. A coupled dynamic-thermodynamic model of an ice-ocean system in the marginal ice zone

    NASA Technical Reports Server (NTRS)

    Hakkinen, Sirpa

    1987-01-01

    Thermodynamics are incorporated into a coupled ice-ocean model in order to investigate wind-driven ice-ocean processes in the marginal zone. Upswelling at the ice edge which is generated by the difference in the ice-air and air-water surface stresses is found to give rise to a strong entrainment by drawing the pycnocline closer to the surface. Entrainment is shown to be negligible outside the areas affected by the ice edge upswelling. If cooling at the top is included in the model, the heat and salt exchanges are further enhanced in the upswelling areas. It is noted that new ice formation occurs in the region not affected by ice edge upswelling, and it is suggested that the high-salinity mixed layer regions (with a scale of a few Rossby radii of deformation) will overturn due to cooling, possibly contributing to the formation of deep water.

  15. Radar Remote Sensing of Ice and Sea State and Air-Sea Interaction in the Marginal Ice Zone

    DTIC Science & Technology

    2014-09-30

    1 DISTRIBUTION STATEMENT A. Approved for public release; distribution is unlimited. Radar Remote Sensing of Ice and Sea State and Air-Sea...Interaction in the Marginal Ice Zone Hans C. Graber RSMAS – Department of Ocean Sciences Center for Southeastern Tropical Advanced Remote Sensing...scattering and attenuation process of ocean waves interacting with ice . A nautical X-band radar on a vessel dedicated to science would be used to follow the

  16. Holocene temperature history at the west Greenland Ice Sheet margin reconstructed from lake sediments

    NASA Astrophysics Data System (ADS)

    Axford, Y.; Losee, S.; Briner, J. P.; Francis, D.; Langdon, P. G.; Walker, I.

    2011-12-01

    Paleoclimate proxy data can help reduce uncertainties regarding how the Greenland Ice Sheet, and thus global sea level, will respond to future climate change. Studies of terrestrial deposits along Greenland's margins offer opportunities to reconstruct both past temperature changes and the associated changes in Greenland Ice Sheet extent, thus empirically characterizing the ice sheet's response to temperature change. Here we present Holocene paleoclimate reconstructions developed from sediment records of five lakes along the western ice sheet margin, near Jakobshavn Isbræ and Disko Bugt. Insect (Chironomidae, or non-biting midge) remains from North Lake provide quantitative estimates of summer temperatures over the past ca. 7500 years at multi-centennial resolution, and changes in sediment composition at all five lakes offer evidence for glacier fluctuations, changes in lake productivity, and other environmental changes throughout the Holocene. Aims of this study include quantification of warmth in the early to mid Holocene, when summer solar insolation forcing exceeded present-day values at northern latitudes and the local Greenland Ice Sheet margin receded inboard of its present position, and the magnitude of subsequent Neoglacial and Little Ice Age cooling that drove ice sheet expansion. We find that the Jakobshavn Isbrae region experienced the warmest temperatures of the Holocene (with summers 2 to 3.5 degrees C warmer than present) between ~6000 and 4000 years ago. Neoglacial cooling began rather abruptly ~4000 years ago and intensified 3000 years ago. Our proxy data suggest that the coldest summers of the Holocene occurred during the 18th and 19th centuries in the Jakobshavn region. These results agree well with previous glacial geologic studies reconstructing local ice margin positions through the Holocene. Such reconstructions of paleoclimate and past ice sheet extent provide targets for testing and improving ice sheet models.

  17. Upper Ocean Evolution Across the Beaufort Sea Marginal Ice Zone

    NASA Astrophysics Data System (ADS)

    Lee, C.; Rainville, L.; Gobat, J. I.; Perry, M. J.; Freitag, L. E.; Webster, S.

    2016-12-01

    The observed reduction of Arctic summertime sea ice extent and expansion of the marginal ice zone (MIZ) have profound impacts on the balance of processes controlling sea ice evolution, including the introduction of several positive feedback mechanisms that may act to accelerate melting. Examples of such feedbacks include increased upper ocean warming though absorption of solar radiation, elevated internal wave energy and mixing that may entrain heat stored in subsurface watermasses (e.g., the relatively warm Pacific Summer and Atlantic waters), and elevated surface wave energy that acts to deform and fracture sea ice. Spatial and temporal variability in ice properties and open water fraction impact these processes. To investigate how upper ocean structure varies with changing ice cover, how the balance of processes shift as a function of ice fraction and distance from open water, and how these processes impact sea ice evolution, a network of autonomous platforms sampled the atmosphere-ice-ocean system in the Beaufort, beginning in spring, well before the start of melt, and ending with the autumn freeze-up. Four long-endurance autonomous Seagliders occupied sections that extended from open water, through the marginal ice zone, deep into the pack during summer 2014 in the Beaufort Sea. Gliders penetrated up to 200 km into the ice pack, under complete ice cover for up to 10 consecutive days. Sections reveal strong fronts where cold, ice-covered waters meet waters that have been exposed to solar warming, and O(10 km) scale eddies near the ice edge. In the pack, Pacific Summer Water and a deep chlorophyll maximum form distinct layers at roughly 60 m and 80 m, respectively, which become increasingly diffuse late in the season as they progress through the MIZ and into open water. Stratification just above the Pacific Summer Water rapidly weakens near the ice edge and temperature variance increases, likely due to mixing or energetic vertical exchange associated with strong

  18. Modelling wave-induced sea ice break-up in the marginal ice zone

    NASA Astrophysics Data System (ADS)

    Montiel, F.; Squire, V. A.

    2017-10-01

    A model of ice floe break-up under ocean wave forcing in the marginal ice zone (MIZ) is proposed to investigate how floe size distribution (FSD) evolves under repeated wave break-up events. A three-dimensional linear model of ocean wave scattering by a finite array of compliant circular ice floes is coupled to a flexural failure model, which breaks a floe into two floes provided the two-dimensional stress field satisfies a break-up criterion. A closed-feedback loop algorithm is devised, which (i) solves the wave-scattering problem for a given FSD under time-harmonic plane wave forcing, (ii) computes the stress field in all the floes, (iii) fractures the floes satisfying the break-up criterion, and (iv) generates an updated FSD, initializing the geometry for the next iteration of the loop. The FSD after 50 break-up events is unimodal and near normal, or bimodal, suggesting waves alone do not govern the power law observed in some field studies. Multiple scattering is found to enhance break-up for long waves and thin ice, but to reduce break-up for short waves and thick ice. A break-up front marches forward in the latter regime, as wave-induced fracture weakens the ice cover, allowing waves to travel deeper into the MIZ.

  19. Geochronological (OSL) and geomorphological investigations at the presumed Frankfurt ice marginal position in northeast Germany

    NASA Astrophysics Data System (ADS)

    Hardt, Jacob; Lüthgens, Christopher; Hebenstreit, Robert; Böse, Margot

    2016-12-01

    The Weichselian Frankfurt ice marginal position in northeast Germany has been critically discussed in the past owing to weak morphological evidence and a lack of clear sedimentological records. This study aims to contribute to this discussion with new geochronological and geomorphological results. Apart from very few cosmogenic exposure ages, the time frame is to date still based on long distance correlation with radiocarbon chronologies. We selected a study site in a key position regarding the classic location of the Frankfurt ice marginal position and the recently described arcuate ridge structures on the Barnim plateau. For the first time we present Optically Stimulated Luminescence (OSL) ages of quartz from glaciofluvial deposits for this Weichselian phase. Our results indicate an advance of the Scandinavian Ice Sheet (SIS) at around 34.1 ± 4.6 ka. This is in agreement with OSL ages from sandur deposits at the Brandenburg ice marginal position located farther south and could also be correlated with the Klintholm advance in Denmark. The subsequent meltdown phase lasted until around 26.3 ± 3.7 ka. During the meltdown phase a minor oscillation of the SIS caused the formation of the recently described arcuate ridges on the Barnim till plain. Recalculated surface exposure ages of glacigenic boulders with an updated global production rate indicate a landscape stabilization phase at around 22.7 ± 1.6 ka, which is in agreement with our ages. A phase of strong aeolian activity has been dated with OSL to 1 ± 0.1 ka; this may have been triggered by human activities that are documented in this region for the medieval period.

  20. Satellite and aircraft passive microwave observations during the Marginal Ice Zone Experiment in 1984

    NASA Technical Reports Server (NTRS)

    Gloersen, Per; Campbell, William J.

    1988-01-01

    This paper compares satellite data on the marginal ice zone obtained during the Marginal Ice Zone Experiment in 1984 by Nimbus 7 with simultaneous mesoscale aircraft (in particular, the NASA CV-990 airborne laboratory) and surface observations. Total and multiyear sea ice concentrations calculated from the airborne multichannel microwave radiometer were found to agree well with similar calculations using the Nimbus SMMR data. The temperature dependence of the determination of multiyear sea-ice concentration near the melting point was found to be the same for both airborne and satellite data. It was found that low total ice concentrations and open-water storm effects near the ice edge could be reliably distinguished by means of spectral gradient ratio, using data from the 0.33-cm and the 1.55-cm radiometers.

  1. Coupled ice-ocean dynamics in the marginal ice zones Upwelling/downwelling and eddy generation

    NASA Technical Reports Server (NTRS)

    Hakkinen, S.

    1986-01-01

    This study is aimed at modeling mesoscale processes such as upwelling/downwelling and ice edge eddies in the marginal ice zones. A two-dimensional coupled ice-ocean model is used for the study. The ice model is coupled to the reduced gravity ocean model through interfacial stresses. The parameters of the ocean model were chosen so that the dynamics would be nonlinear. The model was tested by studying the dynamics of upwelling. Wings parallel to the ice edge with the ice on the right produce upwelling because the air-ice momentum flux is much greater than air-ocean momentum flux; thus the Ekman transport is greater than the ice than in the open water. The stability of the upwelling and downwelling jets is discussed. The downwelling jet is found to be far more unstable than the upwelling jet because the upwelling jet is stabilized by the divergence. The constant wind field exerted on a varying ice cover will generate vorticity leading to enhanced upwelling/downwelling regions, i.e., wind-forced vortices. Steepening and strengthening of vortices are provided by the nonlinear terms. When forcing is time-varying, the advection terms will also redistribute the vorticity. The wind reversals will separate the vortices from the ice edge, so that the upwelling enhancements are pushed to the open ocean and the downwelling enhancements are pushed underneath the ice.

  2. Modelling wave-induced sea ice break-up in the marginal ice zone

    PubMed Central

    Squire, V. A.

    2017-01-01

    A model of ice floe break-up under ocean wave forcing in the marginal ice zone (MIZ) is proposed to investigate how floe size distribution (FSD) evolves under repeated wave break-up events. A three-dimensional linear model of ocean wave scattering by a finite array of compliant circular ice floes is coupled to a flexural failure model, which breaks a floe into two floes provided the two-dimensional stress field satisfies a break-up criterion. A closed-feedback loop algorithm is devised, which (i) solves the wave-scattering problem for a given FSD under time-harmonic plane wave forcing, (ii) computes the stress field in all the floes, (iii) fractures the floes satisfying the break-up criterion, and (iv) generates an updated FSD, initializing the geometry for the next iteration of the loop. The FSD after 50 break-up events is unimodal and near normal, or bimodal, suggesting waves alone do not govern the power law observed in some field studies. Multiple scattering is found to enhance break-up for long waves and thin ice, but to reduce break-up for short waves and thick ice. A break-up front marches forward in the latter regime, as wave-induced fracture weakens the ice cover, allowing waves to travel deeper into the MIZ. PMID:29118659

  3. Modelling wave-induced sea ice break-up in the marginal ice zone.

    PubMed

    Montiel, F; Squire, V A

    2017-10-01

    A model of ice floe break-up under ocean wave forcing in the marginal ice zone (MIZ) is proposed to investigate how floe size distribution (FSD) evolves under repeated wave break-up events. A three-dimensional linear model of ocean wave scattering by a finite array of compliant circular ice floes is coupled to a flexural failure model, which breaks a floe into two floes provided the two-dimensional stress field satisfies a break-up criterion. A closed-feedback loop algorithm is devised, which (i) solves the wave-scattering problem for a given FSD under time-harmonic plane wave forcing, (ii) computes the stress field in all the floes, (iii) fractures the floes satisfying the break-up criterion, and (iv) generates an updated FSD, initializing the geometry for the next iteration of the loop. The FSD after 50 break-up events is unimodal and near normal, or bimodal, suggesting waves alone do not govern the power law observed in some field studies. Multiple scattering is found to enhance break-up for long waves and thin ice, but to reduce break-up for short waves and thick ice. A break-up front marches forward in the latter regime, as wave-induced fracture weakens the ice cover, allowing waves to travel deeper into the MIZ.

  4. Wave attenuation in the marginal ice zone during LIMEX

    NASA Technical Reports Server (NTRS)

    Liu, Antony K.; Vachon, Paris W.; Peng, Chih Y.; Bhogal, A. S.

    1992-01-01

    The effect of ice cover on ocean-wave attenuation is investigated for waves under flexure in the marginal ice zone (MIZ) with SAR image spectra and the results of models. Directional wavenumber spectra are taken from the SAR image data, and the wave-attenuation rate is evaluated with SAR image spectra and by means of the model by Liu and Mollo-Christensen (1988). Eddy viscosity is described by means of dimensional analysis as a function of ice roughness and wave-induced velocity, and comparisons are made with the remotely sensed data. The model corrects the open-water model by introducing the effects of a continuous ice sheet, and turbulent eddy viscosity is shown to depend on ice thickness, floe sizes, significant wave height, and wave period. SAR and wave-buoy data support the trends described in the model results, and a characteristic rollover is noted in the model and experimental wave-attenuation rates at high wavenumbers.

  5. Weddell-Scotia sea marginal ice zone observations from space, October 1984

    NASA Technical Reports Server (NTRS)

    Carsey, F. D.; Holt, B.; Martin, S.; Rothrock, D. A.; Mcnutt, L.

    1986-01-01

    Imagery from the Shuttle imaging radar-B experiment as well as other satellite and meteorological data are examined to learn more about the open sea ice margin of the Weddell-Scotia Seas region. At the ice edge, the ice forms into bandlike aggregates of small ice floes similar to those observed in the Bering Sea. The radar backscatter characteristics of these bands suggest that their upper surface is wet. Further into the pack, the radar imagery shows a transition to large floes. In the open sea, large icebergs and long surface gravity waves are discernable in the radar images.

  6. Various remote sensing approaches to understanding roughness in the marginal ice zone

    NASA Astrophysics Data System (ADS)

    Gupta, Mukesh

    Multi-platform based measurement approaches to understanding complex marginal ice zone (MIZ) are suggested in this paper. Physical roughness measurements using ship- and helicopter-based laser systems combined with ship-based active microwave backscattering (C-band polarimetric coherences) and dual-polarized passive microwave emission (polarization ratio, PR and spectral gradient ratios, GR at 37 and 89 GHz) are presented to study diverse sea ice types found in the MIZ. Autocorrelation functions are investigated for different sea ice roughness types. Small-scale roughness classes were discriminated using data from a ship-based laser profiler. The polarimetric coherence parameter ρHHVH , is not found to exhibit any observable sensitivity to the surface roughness for all incidence angles. Rubble-ridges, pancake ice, snow-covered frost flowers, and dense frost flowers exhibit separable signatures using GR-H and GR-V at >70° incidence angles. This paper diagnosed changes in sea ice roughness on a spatial scale of ∼0.1-4000 m and on a temporal scale of ∼1-240 days (ice freeze-up to summer melt). The coupling of MIZ wave roughness and aerodynamic roughness in conjunction with microwave emission and backscattering are future avenues of research. Additionally, the integration of various datasets into thermodynamic evolution model of sea ice will open pathways to successful development of inversion models of MIZ behavior.

  7. Diatoms as Proxies for a Fluctuating Ice Cap Margin, Hvitarvatn, Iceland

    NASA Astrophysics Data System (ADS)

    Black, J. L.; Miller, G. H.; Geirsdottir, A.

    2005-12-01

    There are no complete records of terrestrial environmental change for the Holocene (11,000yrs) in Iceland and the status of Icelandic glaciers in the early Holocene remains unclear. It is not even known whether Iceland's large ice caps disappeared in the early Holocene, and if they did, when they re-grew. Icelandic lakes are particularly well suited to address these uncertainties as: 1) Glacial erosion and soft bedrock result in high lacustrine sedimentation rates, 2) Diagnostic tephras aid the geochronology, 3) Iceland's sensitivity to changes in North Atlantic circulation should produce clear signals in key environmental proxies (diatoms) preserved in lacustrine sequences, and 4) Ice-cap profiles are relatively flat so small changes in the equilibrium line altitude result in large changes in accumulation area. Hence, large changes in ice-sheet margins during the Holocene will impact sedimentation in glacier-dominated lakes and the diatom assemblages at those times. Hvitarvatn is a glacier dominated lake located on the eastern margin of Langjokull Ice Cap in central-western Iceland. The uppermost Hvitarvatn sediments reflect a glacially dominated system with planktonic, silica-demanding diatom taxa that suggest a high dissolved silica and turbid water environment consistent with high fluxes of glacial flour. Below this are Neoglacial sediments deposited when Langjokull was active, but outlet glaciers were not in contact with Hvitarvatn. The diatom assemblage here shows a small increase in abundance, but is still dominated by planktic, silica-demanding taxa. A distinct shift in lake conditions is reflected in the lowermost sediments, composed of predominantly benthic diatoms and deposited in clear water conditions with long growing seasons likely found in an environment with warmer summers than present and with no glacial erosion. Langjokull must have disappeared in the early Holocene for such a diverse, benthic dominated diatom assemblage to flourish.

  8. Automatic detection of Floating Ice at Antarctic Continental Margin from Remotely Sensed Image with Object-oriented Matching

    NASA Astrophysics Data System (ADS)

    Zhao, Z.

    2011-12-01

    Changes in ice sheet and floating ices around that have great significance for global change research. In the context of global warming, rapidly changing of Antarctic continental margin, caving of ice 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 ice sheet and the location of ice 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 ice and Ice displacement. This paper proposed an automatic change detection method using object-based segmentation technology. The process includes three parts: ice extraction using image segmentation, object-baed ice 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 ice-object. Different time of LANDSAT ETM+ data, Chinese environment disaster satellite HJ1B date, MODIS 1B date are used to detect changes of Floating ice at Antarctic continental margin respectively. We select different time of ETM+ data(January 7, 2003 and January 16, 2003) with the area around Antarctic 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 Antarctic continental margin area, as a sample. Then we can obtain the area of floating ices reduced 371km2, and the number of them reduced 402 during the time. In addition, the changes of all the floating ices around the margin region of Antarctic within 1200 km are detected using MODIS 1B data. During the time from January 1, 2008 to January 7, 2008, the floating ice area decreased by 21644732 km2, and the number of them reduced by 83080

  9. Wave propagation in the marginal ice zone - Model predictions and comparisons with buoy and synthetic aperture radar data

    NASA Technical Reports Server (NTRS)

    Liu, Antony K.; Holt, Benjamin; Vachon, Paris W.

    1991-01-01

    Ocean wave dispersion relation and viscous attenuation by a sea ice cover are studied for waves propagating into the marginal ice zone (MIZ). The Labrador ice margin experiment (LIMEX), conducted on the MIZ off the east coast of Newfoundland, Canada in March 1987, provided aircraft SAR imagery, ice property and wave buoy data. Wave energy attenuation rates are estimated from SAR data and the ice motion package data that were deployed at the ice edge and into the ice pack, and compared with a model. It is shown that the model data comparisons are quite good for the ice conditions observed during LIMEX 1987.

  10. Wave evolution in the marginal ice zone - Model predictions and comparisons with on-site and remote data

    NASA Technical Reports Server (NTRS)

    Liu, A. K.; Holt, B.; Vachon, P. W.

    1989-01-01

    The ocean-wave dispersion relation and viscous attenuation by a sea ice cover were studied for waves in the marginal ice zone (MIZ). The Labrador ice margin experiment (Limex), conducted off the east coast of Newfoundland, Canada in March 1987, provided aircraft SAR, wave buoy, and ice property data. Based on the wave number spectrum from SAR data, the concurrent wave frequency spectrum from ocean buoy data, and accelerometer data on the ice during Limex '87, the dispersion relation has been derived and compared with the model. Accelerometers were deployed at the ice edge and into the ice pack. Data from the accelerometers were used to estimate wave energy attenuation rates and compared with the model. The model-data comparisons are reasonably good for the ice conditions observed during Limex' 87.

  11. Late Weichselian ice-sheet dynamics and deglaciation history of the northern Svalbard margin

    NASA Astrophysics Data System (ADS)

    Fransner, O.; Noormets, R. R. N. N.; Flink, A.; Hogan, K.; Dowdeswell, J. A.; O'Regan, M.; Jakobsson, M.

    2016-12-01

    The glacial evolution of the northern Svalbard margin is poorly known compared with the western margin. Gravity cores, swath bathymetric, sub-bottom acoustic and 2D airgun data are used to investigate the Late Weichselian Svalbard-Barents Ice Sheet history on the northern Svalbard margin. Prograding sequences in Kvitøya and Albertini trough mouths (TMs) indicate ice streaming to the shelf edge multiple times during the Quaternary. While Kvitøya Trough has an associated trough-mouth fan (TMF), Albertini TM is cut back into the shelf edge. Down-faulted bedrock below Albertini TM suggests larger sediment accommodation space there, explaining the absence of a TMF. The bathymetry indicates that ice flow in Albertini Trough was sourced from Duvefjorden and Albertinibukta. Exposed crystalline bedrock likely kept the two ice flows separated before merging north of Karl XII-Øya. Subglacial landforms in Rijpfjorden and Duvefjorden indicate that both fjords accommodated northward-flowing ice streams during the LGM. The deeper fjord basin and higher elongation ratios of landforms in Duvefjorden suggest a more focused and/or larger ice flow there. Easily erodible sedimentary rocks are common in Duvefjorden, which may explain different ice flow dynamics in these fjords. Kvitøya TMF is flanked by gullies, probably formed through erosive downslope gravity flows triggered by sediment-laden meltwater during early deglaciation. Glacial landforms in Albertini Trough comprise retreat-related landforms indicating slow deglaciation. Iceberg scours in Albertini Trough suggest the importance of calving for mass-loss. Sets of De Geer moraines in Rijpfjorden imply that slow, grounded retreat continued in <210 m water depth. Lack of retreat-related landforms in deeper areas of Rijpfjorden and in Duvefjorden indicates floating glacier fronts influenced by calving. 14C ages suggest that deglaciation of inner Rijpfjorden and central Duvefjorden were complete before 10,434 cal a BP and 10

  12. Performance of an airborne imaging 92/183 GHz radiometer during the Bering Sea Marginal Ice Zone Experiment (MIZEX-WEST)

    NASA Technical Reports Server (NTRS)

    Gagliano, J. A.; Mcsheehy, J. J.; Cavalieri, D. J.

    1983-01-01

    An airborne imaging 92/183 GHz radiometer was recently flown onboard NASA's Convair 990 research aircraft during the February 1983 Bering Sea Marginal Ice Zone Experiment (MIZEX-WEST). The 92 GHz portion of the radiometer was used to gather ice signature data and to generate real-time millimeter wave images of the marginal ice zone. Dry atmospheric conditions in the Arctic resulted in good surface ice signature data for the 183 GHz double sideband (DSB) channel situated + or - 8.75 GHz away from the water vapor absorption line. The radiometer's beam scanner imaged the marginal ice zone over a + or - 45 degrees swath angle about the aircraft nadir position. The aircraft altitude was 30,000 feet (9.20 km) maximum and 3,000 feet (0.92 km) minimum during the various data runs. Calculations of the minimum detectable target (ice) size for the radiometer as a function of aircraft altitude were performed. In addition, the change in the atmospheric attenuation at 92 GHz under varying weather conditions was incorporated into the target size calculations. A radiometric image of surface ice at 92 GHz in the marginal ice zone is included.

  13. Dynamics of coupled ice-ocean system in the marginal ice zone: Study of the mesoscale processes and of constitutive equations for sea ice

    NASA Technical Reports Server (NTRS)

    Hakkinen, S.

    1984-01-01

    This study is aimed at the modelling of mesoscale processed such as up/downwelling and ice edge eddies in the marginal ice zones. A 2-dimensional coupled ice-ocean model is used for the study. The ice model is coupled to the reduced gravity ocean model (f-plane) through interfacial stresses. The constitutive equations of the sea ice are formulated on the basis of the Reiner-Rivlin theory. The internal ice stresses are important only at high ice concentrations (90-100%), otherwise the ice motion is essentially free drift, where the air-ice stress is balanced by the ice-water stress. The model was tested by studying the upwelling dynamics. Winds parallel to the ice edge with the ice on the right produce upwilling because the air-ice momentum flux is much greater that air-ocean momentum flux, and thus the Ekman transport is bigger under the ice than in the open water. The upwelling simulation was extended to include temporally varying forcing, which was chosen to vary sinusoidally with a 4 day period. This forcing resembles successive cyclone passings. In the model with a thin oceanic upper layer, ice bands were formed.

  14. Early and abrupt retreat of the Laurentide Ice Sheet margin from the Mackenzie River valley, southern Northwest Territories

    NASA Astrophysics Data System (ADS)

    Margold, Martin; Froese, Duane G.; Gosse, John C.; Yang, Guang; McKenna, Jillian; Hidy, Alan J.

    2017-04-01

    The detachment of the Laurentide Ice Sheet margin from the Canadian Cordillera opened the present-day drainage route of the Mackenzie River to the Arctic Ocean and an ice-free corridor that allowed for migration of species between Beringia and the mid-latitudes of North America. The existing ice-margin chronology depicts the southern reach of the Mackenzie River between 61 and 63° N as glaciated until about 13 ka, representing the last portion of the Laurentide Ice Sheet margin abutting the eastern foot of the Cordillera. A substantial retreat of the ice sheet margin in this region has been suggested to have occurred during the subsequent Younger Dryas cold period, despite the fact that in many other regions ice masses stabilised or even re-grew at this time. However, until now, deglacial chronometry for this region and the western LIS margin is sparse and consists mostly of minimum-limiting macrofossil and bulk C-14 ages from organics materials overlying glacial sediment. With the aim to bring new data on the deglaciation history of the Mackenzie River valley, we collected samples for Be-10 exposure dating from glacial erratic boulders in the southern Franklin Mountains that bound the Mackenzie River valley from the east. The sampling elevations ranged between 1480 and 800 m a.s.l., however, the measured ages show only a weak correlation with elevation. Instead, 10 out of 12 measured samples cluster tightly around 15 ka, with the remaining two samples likely containing Be-10 inherited from previous periods of exposure. Our results thus indicate a pre-Younger Dryas rapid down-wasting of the ice sheet surface, which we infer was accompanied by an ice margin retreat to the southeast. The southern reach of the Mackenzie River valley at the eastern foot of the Cordillera was, according to our results, ice free shortly after 15 ka, with the prospect that the ice-free corridor might have opened significantly earlier than hitherto anticipated. Further research is

  15. Microwave properties of sea ice in the marginal ice zone

    NASA Technical Reports Server (NTRS)

    Onstott, R. G.; Larson, R. W.

    1986-01-01

    Active microwave properties of summer sea ice were measured. Backscatter data were acquired at frequencies from 1 to 17 GHz, at angles from 0 to 70 deg from vertical, and with like and cross antenna polarizations. Results show that melt-water, snow thickness, snowpack morphology, snow surface roughness, ice surface roughness, and deformation characteristics are the fundamental scene parameters which govern the summer sea ice backscatter response. A thick, wet snow cover dominates the backscatter response and masks any ice sheet features below. However, snow and melt-water are not distributed uniformly and the stage of melt may also be quite variable. These nonuniformities related to ice type are not necessarily well understood and produce unique microwave signature characteristics.

  16. Short-term sea ice forecasts with the RASM-ESRL coupled model: A testbed for improving simulations of ocean-ice-atmosphere interactions in the marginal ice zone

    NASA Astrophysics Data System (ADS)

    Solomon, A.; Cox, C. J.; Hughes, M.; Intrieri, J. M.; Persson, O. P. G.

    2015-12-01

    The dramatic decrease of Arctic sea-ice has led to a new Arctic sea-ice paradigm and to increased commercial activity in the Arctic Ocean. NOAA's mission to provide accurate and timely sea-ice forecasts, as explicitly outlined in the National Ocean Policy and the U.S. National Strategy for the Arctic Region, needs significant improvement across a range of time scales to improve safety for human activity. Unfortunately, the sea-ice evolution in the new Arctic involves the interaction of numerous physical processes in the atmosphere, ice, and ocean, some of which are not yet understood. These include atmospheric forcing of sea-ice movement through stress and stress deformation; atmospheric forcing of sea-ice melt and formation through energy fluxes; and ocean forcing of the atmosphere through new regions of seasonal heat release. Many of these interactions involve emerging complex processes that first need to be understood and then incorporated into forecast models in order to realize the goal of useful sea-ice forecasting. The underlying hypothesis for this study is that errors in simulations of "fast" atmospheric processes significantly impact the forecast of seasonal sea-ice retreat in summer and its advance in autumn in the marginal ice zone (MIZ). We therefore focus on short-term (0-20 day) ice-floe movement, the freeze-up and melt-back processes in the MIZ, and the role of storms in modulating stress and heat fluxes. This study uses a coupled ocean-atmosphere-seaice forecast model as a testbed to investigate; whether ocean-sea ice-atmosphere coupling improves forecasts on subseasonal time scales, where systematic biases develop due to inadequate parameterizations (focusing on mixed-phase clouds and surface fluxes), how increased atmospheric resolution of synoptic features improves the forecasts, and how initialization of sea ice area and thickness and snow depth impacts the skill of the forecasts. Simulations are validated with measurements at pan-Arctic land

  17. Atmospheric boundary layer modification in the marginal ice zone

    NASA Technical Reports Server (NTRS)

    Bennett, Theodore J., Jr.; Hunkins, Kenneth

    1986-01-01

    A case study of the Andreas et al. (1984) data on atmospheric boundary layer modification in the marginal ice zone is made. The model is a two-dimensional, multilevel, linear model with turbulence, lateral and vertical advection, and radiation. Good agreement between observed and modeled temperature cross sections is obtained. In contrast to the hypothesis of Andreas et al., the air flow is found to be stable to secondary circulations. Adiabatic lifting and, at long fetches, cloud top longwave cooling, not an air-to-surface heat flux, dominate the cooling of the boundary layer. The accumulation with fetch over the ice of changes in the surface wind field is shown to have a large effect on estimates of the surface wind stress. It is speculated that the Andreas et al. estimates of the drag coefficient over the compact sea ice are too high.

  18. Sedimentary record of a fluctuating ice margin from the Pennsylvanian of western Gondwana: Paraná Basin, southern Brazil

    NASA Astrophysics Data System (ADS)

    Vesely, Fernando F.; Trzaskos, Barbara; Kipper, Felipe; Assine, Mario Luis; Souza, Paulo A.

    2015-08-01

    The Paraná Basin is a key locality in the context of the Late Paleozoic Ice Age (LPIA) because of its location east of the Andean proto-margin of Gondwana and west of contiguous interior basins today found in western Africa. In this paper we document the sedimentary record associated with an ice margin that reached the eastern border of the Paraná Basin during the Pennsylvanian, with the aim of interpreting the depositional environments and discussing paleogeographic implications. The examined stratigraphic succession is divided in four stacked facies associations that record an upward transition from subglacial to glaciomarine environments. Deposition took place during deglaciation but was punctuated by minor readvances of the ice margin that deformed the sediment pile. Tillites, well-preserved landforms of subglacial erosion and glaciotectonic deformational structures indicate that the ice flowed to the north and northwest and that the ice margin did not advance far throughout the basin during the glacial maximum. Consequently, time-equivalent glacial deposits that crop out in other localities of eastern Paraná Basin are better explained by assuming multiple smaller ice lobes instead of one single large glacier. These ice lobes flowed from an ice cap covering uplifted lands now located in western Namibia, where glacial deposits are younger and occur confined within paleovalleys cut onto the Precambrian basement. This conclusion corroborates the idea of a topographically-controlled ice-spreading center in southwestern Africa and does not support the view of a large polar ice sheet controlling deposition in the Paraná Basin during the LPIA.

  19. Upper Ocean Evolution Across the Beaufort Sea Marginal Ice Zone from Autonomous Gliders

    NASA Astrophysics Data System (ADS)

    Lee, Craig; Rainville, Luc; Perry, Mary Jane

    2016-04-01

    The observed reduction of Arctic summertime sea ice extent and expansion of the marginal ice zone (MIZ) have profound impacts on the balance of processes controlling sea ice evolution, including the introduction of several positive feedback mechanisms that may act to accelerate melting. Examples of such feedbacks include increased upper ocean warming though absorption of solar radiation, elevated internal wave energy and mixing that may entrain heat stored in subsurface watermasses (e.g., the relatively warm Pacific Summer (PSW) and Atlantic (AW) waters), and elevated surface wave energy that acts to deform and fracture sea ice. Spatial and temporal variability in ice properties and open water fraction impact these processes. To investigate how upper ocean structure varies with changing ice cover, and how the balance of processes shift as a function of ice fraction and distance from open water, four long-endurance autonomous Seagliders occupied sections that extended from open water, through the marginal ice zone, deep into the pack during summer 2014 in the Beaufort Sea. Sections reveal strong fronts where cold, ice-covered waters meet waters that have been exposed to solar warming, and O(10 km) scale eddies near the ice edge. In the pack, Pacific Summer Water and a deep chlorophyll maximum form distinct layers at roughly 60 m and 80 m, respectively, which become increasingly diffuse as they progress through the MIZ and into open water. The isopynal layer between 1023 and 1024 kgm-3, just above the PSW, consistently thickens near the ice edge, likely due to mixing or energetic vertical exchange associated with strong lateral gradients in this region. This presentation will discuss the upper ocean variability, its relationship to sea ice extent, and evolution over the summer to the start of freeze up.

  20. Upper Ocean Evolution Across the Beaufort Sea Marginal Ice Zone from Autonomous Gliders

    NASA Astrophysics Data System (ADS)

    Lee, C.; Rainville, L.; Perry, M. J.

    2016-02-01

    The observed reduction of Arctic summertime sea ice extent and expansion of the marginal ice zone (MIZ) have profound impacts on the balance of processes controlling sea ice evolution, including the introduction of several positive feedback mechanisms that may act to accelerate melting. Examples of such feedbacks include increased upper ocean warming though absorption of solar radiation, elevated internal wave energy and mixing that may entrain heat stored in subsurface watermasses (e.g., the relatively warm Pacific Summer (PSW) and Atlantic (AW) waters), and elevated surface wave energy that acts to deform and fracture sea ice. Spatial and temporal variability in ice properties and open water fraction impact these processes. To investigate how upper ocean structure varies with changing ice cover, and how the balance of processes shift as a function of ice fraction and distance from open water, four long-endurance autonomous Seagliders occupied sections that extended from open water, through the marginal ice zone, deep into the pack during summer 2014 in the Beaufort Sea. Sections reveal strong fronts where cold, ice-covered waters meet waters that have been exposed to solar warming, and O(10 km) scale eddies near the ice edge. In the pack, Pacific Summer Water and a deep chlorophyll maximum form distinct layers at roughly 60 m and 80 m, respectively, which become increasingly diffuse as they progress through the MIZ and into open water. The isopynal layer between 1023 and 1024 kg m-3, just above the PSW, consistently thickens near the ice edge, likely due to mixing or energetic vertical exchange associated with strong lateral gradients in this region. This presentation will discuss the upper ocean variability, its relationship to sea ice extent, and evolution over the summer to the start of freeze up.

  1. Seasonal Variability in Regional Ice Flow Due to Meltwater Injection Into the Shear Margins of Jakobshavn Isbræ

    NASA Astrophysics Data System (ADS)

    Cavanagh, J. P.; Lampkin, D. J.; Moon, T.

    2017-12-01

    The impact of meltwater injection into the shear margins of Jakobshavn Isbræ via drainage from water-filled crevasses on ice flow is examined. We use Landsat-8 Operational Land Imager panchromatic, high-resolution imagery to monitor the spatiotemporal variability of seven water-filled crevasse ponds during the summers of 2013 to 2015. The timing of drainage from water-filled crevasses coincides with an increase of 2 to 20% in measured ice velocity beyond Jakobshavn Isbræ shear margins, which we define as extramarginal ice velocity. Some water-filled crevasse groups demonstrate multiple drainage events within a single melt season. Numerical simulations show that hydrologic shear weakening due to water-filled crevasse drainage can accelerate extramarginal flow by as much as 35% within 10 km of the margins and enhance mass flux through the shear margins by 12%. This work demonstrates a novel mechanism through which surface melt can influence regional ice flow.

  2. Sea ice floe size distribution in the marginal ice zone: Theory and numerical experiments

    NASA Astrophysics Data System (ADS)

    Zhang, Jinlun; Schweiger, Axel; Steele, Michael; Stern, Harry

    2015-05-01

    To better describe the state of sea ice in the marginal ice zone (MIZ) with floes of varying thicknesses and sizes, both an ice thickness distribution (ITD) and a floe size distribution (FSD) are needed. In this work, we have developed a FSD theory that is coupled to the ITD theory of Thorndike et al. (1975) in order to explicitly simulate the evolution of FSD and ITD jointly. The FSD theory includes a FSD function and a FSD conservation equation in parallel with the ITD equation. The FSD equation takes into account changes in FSD due to ice advection, thermodynamic growth, and lateral melting. It also includes changes in FSD because of mechanical redistribution of floe size due to ice ridging and, particularly, ice fragmentation induced by stochastic ocean surface waves. The floe size redistribution due to ice fragmentation is based on the assumption that wave-induced breakup is a random process such that when an ice floe is broken, floes of any smaller sizes have an equal opportunity to form, without being either favored or excluded. To focus only on the properties of mechanical floe size redistribution, the FSD theory is implemented in a simplified ITD and FSD sea ice model for idealized numerical experiments. Model results show that the simulated cumulative floe number distribution (CFND) follows a power law as observed by satellites and airborne surveys. The simulated values of the exponent of the power law, with varying levels of ice breakups, are also in the range of the observations. It is found that floe size redistribution and the resulting FSD and mean floe size do not depend on how floe size categories are partitioned over a given floe size range. The ability to explicitly simulate multicategory FSD and ITD together may help to incorporate additional model physics, such as FSD-dependent ice mechanics, surface exchange of heat, mass, and momentum, and wave-ice interactions.

  3. Modelling seasonal meltwater forcing of the velocity of land-terminating margins of the Greenland Ice Sheet

    NASA Astrophysics Data System (ADS)

    Koziol, Conrad P.; Arnold, Neil

    2018-03-01

    Surface runoff at the margin of the Greenland Ice Sheet (GrIS) drains to the ice-sheet bed, leading to enhanced summer ice flow. Ice velocities show a pattern of early summer acceleration followed by mid-summer deceleration due to evolution of the subglacial hydrology system in response to meltwater forcing. Modelling the integrated hydrological-ice dynamics system to reproduce measured velocities at the ice margin remains a key challenge for validating the present understanding of the system and constraining the impact of increasing surface runoff rates on dynamic ice mass loss from the GrIS. Here we show that a multi-component model incorporating supraglacial, subglacial, and ice dynamic components applied to a land-terminating catchment in western Greenland produces modelled velocities which are in reasonable agreement with those observed in GPS records for three melt seasons of varying melt intensities. This provides numerical support for the hypothesis that the subglacial system develops analogously to alpine glaciers and supports recent model formulations capturing the transition between distributed and channelized states. The model shows the growth of efficient conduit-based drainage up-glacier from the ice sheet margin, which develops more extensively, and further inland, as melt intensity increases. This suggests current trends of decadal-timescale slowdown of ice velocities in the ablation zone may continue in the near future. The model results also show a strong scaling between average summer velocities and melt season intensity, particularly in the upper ablation area. Assuming winter velocities are not impacted by channelization, our model suggests an upper bound of a 25 % increase in annual surface velocities as surface melt increases to 4 × present levels.

  4. Coupling of Waves, Turbulence and Thermodynamics Across the Marginal Ice Zone

    DTIC Science & Technology

    2015-09-30

    1 DISTRIBUTION STATEMENT A. Approved for public release; distribution is unlimited. Coupling of Waves, Turbulence and Thermodynamics across...developing Thermodynamically Forced Marginal Ice Zone. Submitted to JGR. Heiles,A. S., NPS thesis, Sep. 2014 Schmidt, B. K., NPS thesis March 2012 Shaw

  5. Vertical motions of passive margins of Greenland: influence of ice sheet, glacial erosion, and sediment transport

    NASA Astrophysics Data System (ADS)

    Souche, A.; Medvedev, S.; Hartz, E. H.

    2009-04-01

    The sub-ice topography of Greenland is characterized by a central depression below the sea level and by elevated (in some places significantly) margins. Whereas the central depression may be explained by significant load of the Greenland ice sheet, the origin of the peripheral relief remains unclear. We analyze the influence of formation of the ice sheet and carving by glacial erosion on the evolution of topography along the margins of Greenland. Our analysis shows that: (1) The heavy ice loading in the central part of Greenland and consecutive peripheral bulging has a negligible effect on amplitude of the uplifted Greenland margins. (2) First order estimates of uplift due to isostatic readjustment caused by glacial erosion and unloading in the fjord systems is up to 1.1 km. (3) The increase of accuracy of topographic data (comparing several data sets of resolution with grid size from 5 km to 50 m) results in increase of the isostatic response in the model. (4) The analysis of mass redistribution during erosion-sedimentation process and data on age of offshore sediments allows us to estimate the timing of erosion along the margins of Greenland. This ongoing analysis, however, requires careful account for the link between sources (localized glacial erosion) and sinks (offshore sedimentary basins around Greenland).

  6. Late glacial and Holocene history of the Greenland Ice Sheet margin, Nunatarssuaq, Northwestern Greenland

    NASA Astrophysics Data System (ADS)

    Farnsworth, L. B.; Kelly, M. A.; Axford, Y.; Bromley, G. R.; Osterberg, E. C.; Howley, J. A.; Zimmerman, S. R. H.; Jackson, M. S.; Lasher, G. E.; McFarlin, J. M.

    2015-12-01

    Defining the late glacial and Holocene fluctuations of the Greenland Ice Sheet (GrIS) margin, particularly during periods that were as warm or warmer than present, provides a longer-term perspective on present ice margin fluctuations and informs how the GrIS may respond to future climate conditions. We focus on mapping and dating past GrIS extents in the Nunatarssuaq region of northwestern Greenland. During the summer of 2014, we conducted geomorphic mapping and collected rock samples for 10Be surface exposure dating as well as subfossil plant samples for 14C dating. We also obtained sediment cores from an ice-proximal lake. Preliminary 10Be ages of boulders deposited during deglaciation of the GrIS subsequent to the Last Glacial Maximum range from ~30-15 ka. The apparently older ages of some samples indicate the presence of 10Be inherited from prior periods of exposure. These ages suggest deglaciation occurred by ~15 ka however further data are needed to test this hypothesis. Subfossil plants exposed at the GrIS margin on shear planes date to ~ 4.6-4.8 cal. ka BP and indicate less extensive ice during middle Holocene time. Additional radiocarbon ages from in situ subfossil plants on a nunatak date to ~3.1 cal. ka BP. Geomorphic mapping of glacial landforms near Nordsø, a large proglacial lake, including grounding lines, moraines, paleo-shorelines, and deltas, indicate the existence of a higher lake level that resulted from a more extensive GrIS margin likely during Holocene time. A fresh drift limit, characterized by unweathered, lichen-free clasts approximately 30-50 m distal to the modern GrIS margin, is estimated to be late Holocene in age. 10Be dating of samples from these geomorphic features is in progress. Radiocarbon ages of subfossil plants exposed by recent retreat of the GrIS margin suggest that the GrIS was at or behind its present location at AD ~1650-1800 and ~1816-1889. Results thus far indicate that the GrIS margin in northwestern Greenland

  7. Sea-ice dynamics strongly promote Snowball Earth initiation and destabilize tropical sea-ice margins

    NASA Astrophysics Data System (ADS)

    Voigt, A.; Abbot, D. S.

    2012-12-01

    The Snowball Earth bifurcation, or runaway ice-albedo feedback, is defined for particular boundary conditions by a critical CO2 and a critical sea-ice cover (SI), both of which are essential for evaluating hypotheses related to Neoproterozoic glaciations. Previous work has shown that the Snowball Earth bifurcation, denoted as (CO2, SI)*, differs greatly among climate models. Here, we study the effect of bare sea-ice albedo, sea-ice dynamics and ocean heat transport on (CO2, SI)* in the atmosphere-ocean general circulation model ECHAM5/MPI-OM with Marinoan (~ 635 Ma) continents and solar insolation (94% of modern). In its standard setup, ECHAM5/MPI-OM initiates a~Snowball Earth much more easily than other climate models at (CO2, SI)* ≈ (500 ppm, 55%). Replacing the model's standard bare sea-ice albedo of 0.75 by a much lower value of 0.45, we find (CO2, SI)* ≈ (204 ppm, 70%). This is consistent with previous work and results from net evaporation and local melting near the sea-ice margin. When we additionally disable sea-ice dynamics, we find that the Snowball Earth bifurcation can be pushed even closer to the equator and occurs at a hundred times lower CO2: (CO2, SI)* ≈ (2 ppm, 85%). Therefore, the simulation of sea-ice dynamics in ECHAM5/MPI-OM is a dominant determinant of its high critical CO2 for Snowball initiation relative to other models. Ocean heat transport has no effect on the critical sea-ice cover and only slightly decreases the critical CO2. For disabled sea-ice dynamics, the state with 85% sea-ice cover is stabilized by the Jormungand mechanism and shares characteristics with the Jormungand climate states. However, there is no indication of the Jormungand bifurcation and hysteresis in ECHAM5/MPI-OM. The state with 85% sea-ice cover therefore is a soft Snowball state rather than a true Jormungand state. Overall, our results demonstrate that differences in sea-ice dynamics schemes can be at least as important as differences in sea-ice albedo for

  8. Local response of a glacier to annual filling and drainage of an ice-marginal lake

    USGS Publications Warehouse

    Walder, J.S.; Trabant, D.C.; Cunico, M.; Fountain, A.G.; Anderson, S.P.; Anderson, R. Scott; Malm, A.

    2006-01-01

    Ice-marginal Hidden Creek Lake, Alaska, USA, outbursts annually over the course of 2-3 days. As the lake fills, survey targets on the surface of the 'ice dam' (the glacier adjacent to the lake) move obliquely to the ice margin and rise substantially. As the lake drains, ice motion speeds up, becomes nearly perpendicular to the face of the ice dam, and the ice surface drops. Vertical movement of the ice dam probably reflects growth and decay of a wedge of water beneath the ice dam, in line with established ideas about jo??kulhlaup mechanics. However, the distribution of vertical ice movement, with a narrow (50-100 m wide) zone where the uplift rate decreases by 90%, cannot be explained by invoking flexure of the ice dam in a fashion analogous to tidal flexure of a floating glacier tongue or ice shelf. Rather, the zone of large uplift-rate gradient is a fault zone: ice-dam deformation is dominated by movement along high-angle faults that cut the ice dam through its entire thickness, with the sense of fault slip reversing as the lake drains. Survey targets spanning the zone of steep uplift gradient move relative to one another in a nearly reversible fashion as the lake fills and drains. The horizontal strain rate also undergoes a reversal across this zone, being compressional as the lake fills, but extensional as the lake drains. Frictional resistance to fault-block motion probably accounts for the fact that lake level falls measurably before the onset of accelerated horizontal motion and vertical downdrop. As the overall fault pattern is the same from year to year, even though ice is lost by calving, the faults must be regularly regenerated, probably by linkage of surface and bottom crevasses as ice is advected toward the lake basin.

  9. Mapping and assessing variability in the Antarctic marginal ice zone, pack ice and coastal polynyas in two sea ice algorithms with implications on breeding success of snow petrels

    NASA Astrophysics Data System (ADS)

    Stroeve, Julienne C.; Jenouvrier, Stephanie; Campbell, G. Garrett; Barbraud, Christophe; Delord, Karine

    2016-08-01

    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 as well as seasonal and interannual variability is essential for understanding how current and future changes in these biologically active regions may impact the Antarctic marine ecosystem. Knowledge of the distribution of MIZ, consolidated pack ice and coastal polynyas in 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 record for assessing the proportion of the sea ice cover that is covered by each of these ice categories. However, estimates of the amount of MIZ, consolidated pack ice and polynyas depend strongly on which sea ice algorithm is used. This study uses two popular passive microwave sea ice algorithms, the NASA Team and Bootstrap, and applies the same thresholds to the sea ice concentrations to evaluate the distribution and variability in the MIZ, the consolidated pack ice and coastal polynyas. Results reveal that the seasonal cycle in the MIZ and pack ice is generally similar between both algorithms, yet the NASA Team algorithm has on average twice the MIZ and half the consolidated pack ice area as the Bootstrap algorithm. Trends also differ, with the Bootstrap algorithm suggesting statistically significant trends towards increased pack ice 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 ice within the consolidated ice 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

  10. MIZEX: A Program for Mesoscale Air-Ice-Ocean Interaction Experiments in Arctic Marginal Ice Zones. MIZEX Bulletin VII.

    DTIC Science & Technology

    1986-03-01

    8217 ILI L2.2363 31-25 UICRQCCW p O TEST C4ART’OPSMa, -f AoA IV 4 86 9 ’ 5 MIZEX BULLETIN SERIES: INFORMATION FOR CONTRIBUTORS The main purpose of the...Ice-Ocean Interaction Experiments in Arctic Marginal Ice Zones MIZEX BULLETIN VII LEC T E SEP 2 9 1986 ’Jl P March 1986 J A ’QOzltnal OontsSn$ ooLoP...studies in both the northern and southern hemispheres. W.D. HIBLER Ill March 1986 ii CONTENTS* Page P reface

  11. Fine Ice Sheet margins topography from swath processing of CryoSat SARIn mode data

    NASA Astrophysics Data System (ADS)

    Gourmelen, N.; Escorihuela, M. J.; Shepherd, A.; Foresta, L.; Muir, A.; Briggs, K.; Hogg, A. E.; Roca, M.; Baker, S.; Drinkwater, M. R.

    2014-12-01

    Reference and repeat-observations of Glacier and Ice Sheet Margin (GISM) topography are critical to identify changes in ice thickness, provide estimates of mass gain or loss and thus quantify the contribution of the cryosphere to sea level change. The lack of such sustained observations was identified in the Integrated Global Observing Strategy (IGOS) Cryosphere Theme Report as a major shortcoming. Conventional altimetry measurements over GISMs exist, but coverage has been sparse and characterized by coarse ground resolution. Additionally, and more importantly, they proved ineffective in the presence of steep slopes, a typical feature of GISM areas. Since the majority of Antarctic and Greenland ice sheet mass loss is estimated to lie within 100 km from the coast, but only about 10% is surveyed, there is the need for more robust and dense observations of GISMs, in both time and space. The ESA Altimetry mission CryoSat aims at gaining better insight into the evolution of the Cryosphere. CryoSat's revolutionary design features a Synthetic Interferometric Radar Altimeter (SIRAL), with two antennas for interferometry. The corresponding SAR Interferometer (SARIn) mode of operation increases spatial resolution while resolving the angular origin of off-nadir echoes occurring over sloping terrain. The SARIn mode is activated over GISMs and the elevation for the Point Of Closest Approach (POCA) is a standard product of the CryoSat mission. Here we present an approach for more comprehensively exploiting the SARIn mode of CryoSat and produce an ice elevation product with enhanced spatial resolution compared to standard CryoSat-2 height products. In this so called L2-swath processing approach, the full CryoSat waveform is exploited under specific conditions of signal and surface characteristics. We will present the rationale, validation exercises and preliminary results from the Eurpean Space Agency's STSE CryoTop study over selected test regions of the margins of the Greenland

  12. Wave Attenuation and Gas Exchange Velocity in Marginal Sea Ice Zone

    NASA Astrophysics Data System (ADS)

    Bigdeli, A.; Hara, T.; Loose, B.; Nguyen, A. T.

    2018-03-01

    The gas transfer velocity in marginal sea ice zones exerts a strong control on the input of anthropogenic gases into the ocean interior. In this study, a sea state-dependent gas exchange parametric model is developed based on the turbulent kinetic energy dissipation rate. The model is tuned to match the conventional gas exchange parametrization in fetch-unlimited, fully developed seas. Next, fetch limitation is introduced in the model and results are compared to fetch limited experiments in lakes, showing that the model captures the effects of finite fetch on gas exchange with good fidelity. Having validated the results in fetch limited waters such as lakes, the model is next applied in sea ice zones using an empirical relation between the sea ice cover and the effective fetch, while accounting for the sea ice motion effect that is unique to sea ice zones. The model results compare favorably with the available field measurements. Applying this parametric model to a regional Arctic numerical model, it is shown that, under the present conditions, gas flux into the Arctic Ocean may be overestimated by 10% if a conventional parameterization is used.

  13. Wave Climate and Wave Mixing in the Marginal Ice Zones of Arctic Seas, Observations and Modelling

    DTIC Science & Technology

    2014-09-30

    At the same time, the PIs participate in Australian efforts of developing wave-ocean- ice coupled models for Antarctica . Specific new physics modules...Wave Mixing in the Marginal Ice Zones of Arctic Seas, Observations and Modelling Alexander V. Babanin Swinburne University of Technology, PO Box...operational forecast. Altimeter climatology and the wave models will be used to study the current and future wind/wave and ice trends. APPROACH

  14. Changes in Arctic Sea Ice Floe Size Distribution in the Marginal Ice Zone in a Thickness and Floe Size Distribution Model

    NASA Astrophysics Data System (ADS)

    Zhang, J.; Stern, H. L., III; Hwang, P. B.; Schweiger, A. J. B.; Stark, M.; Steele, M.

    2015-12-01

    To better describe the state of sea ice in the marginal ice zone (MIZ) with floes of varying thicknesses and sizes, both an ice thickness distribution (ITD) and a floe size distribution (FSD) are needed. We have developed a FSD theory [Zhang et al., 2015] that is coupled to the ITD theory of Thorndike et al. [1975] in order to explicitly simulate the evolution of FSD and ITD jointly. The FSD theory includes a FSD function and a FSD conservation equation in parallel with the ITD equation. The FSD equation takes into account changes in FSD due to ice advection, thermodynamic growth, and lateral melting. It also includes changes in FSD because of mechanical redistribution of floe size due to ice opening, ridging and, particularly, ice fragmentation induced by stochastic ocean surface waves. The floe size redistribution due to ice fragmentation is based on the assumption that wave-induced breakup is a random process such that when an ice floe is broken, floes of any smaller sizes have an equal opportunity to form, without being either favored or excluded. It is also based on the assumption that floes of larger sizes are easier to break because they are subject to larger flexure-induced stresses and strains than smaller floes that are easier to ride with waves with little bending; larger floes also have higher areal coverages and therefore higher probabilities to break. These assumptions with corresponding formulations ensure that the simulated FSD follows a power law as observed by satellites and airborne surveys. The FSD theory has been tested in the Pan-arctic Ice/Ocean Modeling and Assimilation System (PIOMAS). The existing PIOMAS has 12 categories each for ice thickness, ice enthalpy, and snow depth. With the implementation of the FSD theory, PIOMAS is able to represent 12 categories of floe sizes ranging from 0.1 m to ~3000 m. It is found that the simulated 12-category FSD agrees reasonably well with FSD derived from SAR and MODIS images. In this study, we will

  15. Acoustic Transients of the Marginal Sea Ice Zone: A Provisional Catalog

    DTIC Science & Technology

    1989-08-01

    Arctic marine mammals is approximately 20 million individuals. Most of these inhabit the marginal sea ice zone (MIZ), but some species, such as ringed ...Food: molluscs, worms, sea urchins, Arctic cod, occasionally other marine mammals, e.g., ringed and bearded seals, narwhals. Dive: to 80 m...called for. TRANSIENT DESCRIPTION Recordings unavailable DATA SOURCE SERIAL _____ 21 SUPPORTING DATA SOURCE IRIS Ringed Seal, Phoca hispida Circumpolar

  16. Greenland ice sheet retreat since the Little Ice Age

    NASA Astrophysics Data System (ADS)

    Beitch, Marci J.

    Late 20th century and 21st century satellite imagery of the perimeter of the Greenland Ice Sheet (GrIS) provide high resolution observations of the ice sheet margins. Examining changes in ice margin positions over time yield measurements of GrIS area change and rates of margin retreat. However, longer records of ice sheet margin change are needed to establish more accurate predictions of the ice sheet's future response to global conditions. In this study, the trimzone, the area of deglaciated terrain along the ice sheet edge that lacks mature vegetation cover, is used as a marker of the maximum extent of the ice from its most recent major advance during the Little Ice Age. We compile recently acquired Landsat ETM+ scenes covering the perimeter of the GrIS on which we map area loss on land-, lake-, and marine-terminating margins. We measure an area loss of 13,327 +/- 830 km2, which corresponds to 0.8% shrinkage of the ice sheet. This equates to an averaged horizontal retreat of 363 +/- 69 m across the entire GrIS margin. Mapping the areas exposed since the Little Ice Age maximum, circa 1900 C.E., yields a century-scale rate of change. On average the ice sheet lost an area of 120 +/- 16 km 2/yr, or retreated at a rate of 3.3 +/- 0.7 m/yr since the LIA maximum.

  17. Determination of the Nonlethal Margin Inside the Visible 'Ice-Ball' During Percutaneous Cryoablation of Renal Tissue

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

    Georgiades, Christos, E-mail: g_christos@hotmail.com; Rodriguez, Ronald, E-mail: rrodrig@jhmi.edu; Azene, Ezana, E-mail: eazene1@jhmi.edu

    2013-06-15

    Objective. The study was designed to determine the distance between the visible 'ice-ball' and the lethal temperature isotherm for normal renal tissue during cryoablation. Methods. The Animal Care Committee approved the study. Nine adult swine were used: three to determine the optimum tissue stain and six to test the hypotheses. They were anesthetized and the left renal artery was catheterized under fluoroscopy. Under MR guidance, the kidney was ablated and (at end of a complete ablation) the nonfrozen renal tissue (surrounding the 'ice-ball') was stained via renal artery catheter. Kidneys were explanted and sent for slide preparation and examination. Frommore » each slide, we measured the maximum, minimum, and an in-between distance from the stained to the lethal tissue boundaries (margin). We examined each slide for evidence of 'heat pump' effect. Results. A total of 126 measurements of the margin (visible 'ice-ball'-lethal margin) were made. These measurements were obtained from 29 slides prepared from the 6 test animals. Mean width was 0.75 {+-} 0.44 mm (maximum 1.15 {+-} 0.51 mm). It was found to increase adjacent to large blood vessels. No 'heat pump' effect was noted within the lethal zone. Data are limited to normal swine renal tissue. Conclusions. Considering the effects of the 'heat pump' phenomenon for normal renal tissue, the margin was measured to be 1.15 {+-} 0.51 mm. To approximate the efficacy of the 'gold standard' (partial nephrectomy, {approx}98 %), a minimum margin of 3 mm is recommended (3 Multiplication-Sign SD). Given these assumptions and extrapolating for renal cancer, which reportedly is more cryoresistant with a lethal temperature of -40 Degree-Sign C, the recommended margin is 6 mm.« less

  18. The Floe Size Distribution in the Marginal Ice Zone of the Beaufort and Chukchi Seas

    NASA Astrophysics Data System (ADS)

    Schweiger, A. J. B.; Stern, H. L., III; Stark, M.; Zhang, J.; Steele, M.; Hwang, P. B.

    2014-12-01

    Several key processes in the Marginal Ice Zone (MIZ) of the Arctic Ocean are related to the size of the ice floes, whose diameters range from meters to tens of kilometers. The floe size distribution (FSD) influences the mechanical properties of the ice cover, air-sea momentum and heat transfer, lateral melting, and light penetration. However, no existing sea-ice/ocean models currently simulate the FSD in the MIZ. Model development depends on observations of the FSD for parameterization, calibration, and validation. To support the development and implementation of the FSD in the Marginal Ice Zone Modeling and Assimilation System (MIZMAS), we have analyzed the FSD in the Beaufort and Chukchi seas using multiple sources of satellite imagery: NASA's Moderate Resolution Imaging Spectroradiometer (MODIS) on the Terra and Aqua satellites (250 m pixel size), the USGS Landsat 8 satellite (80 m pixel size), the Canadian Space Agency's synthetic aperture radar (SAR) on RADARSAT (50 meter pixel size), and declassified National Technical Means imagery from the Global Fiducials Library (GFL) of the USGS (1 m pixel size). The procedure for identifying ice floes in the imagery begins with manually delineating cloud-free regions (if necessary). A threshold is then chosen to separate ice from water. Morphological operations and other semi-automated techniques are used to identify individual floes, whose properties are then easily calculated. We use the mean caliper diameter as the measure of floe size. The FSD is adequately described by a power-law in which the exponent characterizes the relative number of large and small floes. Changes in the exponent over time and space reflect changes in physical processes in the MIZ, such as sea-ice deformation, fracturing, and melting. We report results of FSD analysis for the spring and summer of 2013 and 2014, and show how the FSD will be incorporated into the MIZMAS model.

  19. In situ observations of Arctic cloud properties across the Beaufort Sea marginal ice zone

    NASA Astrophysics Data System (ADS)

    Corr, C.; Moore, R.; Winstead, E.; Thornhill, K. L., II; Crosbie, E.; Ziemba, L. D.; Beyersdorf, A. J.; Chen, G.; Martin, R.; Shook, M.; Corbett, J.; Smith, W. L., Jr.; Anderson, B. E.

    2016-12-01

    Clouds play an important role in Arctic climate. This is particularly true over the Arctic Ocean where feedbacks between clouds and sea-ice impact the surface radiation budget through modifications of sea-ice extent, ice thickness, cloud base height, and cloud cover. This work summarizes measurements of Arctic cloud properties made aboard the NASA C-130 aircraft over the Beaufort Sea during ARISE (Arctic Radiation - IceBridge Sea&Ice Experiment) in September 2014. The influence of surface-type on cloud properties is also investigated. Specifically, liquid water content (LWC), droplet concentrations, and droplet size distributions are compared for clouds sampled over three distinct regimes in the Beaufort Sea: 1) open water, 2) the marginal ice zone, and 3) sea-ice. Regardless of surface type, nearly all clouds intercepted during ARISE were liquid-phase clouds. However, differences in droplet size distributions and concentrations were evident for the surface types; clouds over the MIZ and sea-ice generally had fewer and larger droplets compared to those over open water. The potential implication these results have for understanding cloud-surface albedo climate feedbacks in Arctic are discussed.

  20. Subsea ice-bearing permafrost on the U.S. Beaufort Margin: 2. Borehole constraints

    USGS Publications Warehouse

    Ruppel, Carolyn D.; Herman, Bruce M.; Brothers, Laura L.; Hart, Patrick E.

    2016-01-01

    Borehole logging data from legacy wells directly constrain the contemporary distribution of subsea permafrost in the sedimentary section at discrete locations on the U.S. Beaufort Margin and complement recent regional analyses of exploration seismic data to delineate the permafrost's offshore extent. Most usable borehole data were acquired on a ∼500 km stretch of the margin and within 30 km of the contemporary coastline from north of Lake Teshekpuk to nearly the U.S.-Canada border. Relying primarily on deep resistivity logs that should be largely unaffected by drilling fluids and hole conditions, the analysis reveals the persistence of several hundred vertical meters of ice-bonded permafrost in nearshore wells near Prudhoe Bay and Foggy Island Bay, with less permafrost detected to the east and west. Permafrost is inferred beneath many barrier islands and in some nearshore and lagoonal (back-barrier) wells. The analysis of borehole logs confirms the offshore pattern of ice-bearing subsea permafrost distribution determined based on regional seismic analyses and reveals that ice content generally diminishes with distance from the coastline. Lacking better well distribution, it is not possible to determine the absolute seaward extent of ice-bearing permafrost, nor the distribution of permafrost beneath the present-day continental shelf at the end of the Pleistocene. However, the recovery of gas hydrate from an outer shelf well (Belcher) and previous delineation of a log signature possibly indicating gas hydrate in an inner shelf well (Hammerhead 2) imply that permafrost may once have extended across much of the shelf offshore Camden Bay.

  1. Multi-frequency SAR, SSM/I and AVHRR derived geophysical information of the marginal ice zone

    NASA Technical Reports Server (NTRS)

    Shuchman, R. A.; Onstott, R. G.; Wackerman, C. C.; Russel, C. A.; Sutherland, L. L.; Johannessen, O. M.; Johannessen, J. A.; Sandven, S.; Gloerson, P.

    1991-01-01

    A description is given of the fusion of synthetic aperture radar (SAR), special sensor microwave imager (SSM/I), and NOAA Advanced Very High Resolution Radiometer (AVHRR) data to study arctic processes. These data were collected during the SIZEX/CEAREX experiments that occurred in the Greenland Sea in March of 1989. Detailed comparisons between the SAR, AVHRR, and SSM/I indicated: (1) The ice edge position was in agreement to within 25 km, (2) The SSM/I SAR total ice concentration compared favorably, however, the SSM/I significantly underpredicted the multiyear fraction, (3) Combining high resolution SAR with SSM/I can potentially map open water and new ice features in the marginal ice zone (MIZ) which cannot be mapped by the single sensors, and (4) The combination of all three sensors provides accurate ice information as well as sea surface temperature and wind speeds.

  2. Exploring changes in vertical ice extent along the margin of the East Antarctic Ice Sheet in western Dronning Maud Land - initial results of the MAGIC-DML collaboration

    NASA Astrophysics Data System (ADS)

    Lifton, N. A.; Newall, J. C.; Fredin, O.; Glasser, N. F.; Fabel, D.; Rogozhina, I.; Bernales, J.; Prange, M.; Sams, S.; Eisen, O.; Hättestrand, C.; Harbor, J.; Stroeven, A. P.

    2017-12-01

    Numerical ice sheet models constrained by theory and refined by comparisons with observational data are a central component of work to address the interactions between the cryosphere and changing climate, at a wide range of scales. Such models are tested and refined by comparing model predictions of past ice geometries with field-based reconstructions from geological, geomorphological, and ice core data. However, on the East Antarctic Ice sheet, there are few empirical data with which to reconstruct changes in ice sheet geometry in the Dronning Maud Land (DML) region. In addition, there is poor control on the regional climate history of the ice sheet margin, because ice core locations, where detailed reconstructions of climate history exist, are located on high inland domes. This leaves numerical models of regional glaciation history in this near-coastal area largely unconstrained. MAGIC-DML is an ongoing Swedish-US-Norwegian-German-UK collaboration with a focus on improving ice sheet models by combining advances in numerical modeling with filling critical data gaps that exist in our knowledge of the timing and pattern of ice surface changes on the western Dronning Maud Land margin. A combination of geomorphological mapping using remote sensing data, field investigations, cosmogenic nuclide surface exposure dating, and numerical ice-sheet modeling are being used in an iterative manner to produce a comprehensive reconstruction of the glacial history of western Dronning Maud Land. We will present an overview of the project, as well as field observations and preliminary in situ cosmogenic nuclide measurements from the 2016/17 expedition.

  3. Seasonal evolution of the Arctic marginal ice zone and its power-law obeying floe size distribution

    NASA Astrophysics Data System (ADS)

    Zhang, J.; Stern, H. L., III; Schweiger, A. J. B.; Steele, M.; Hwang, P. B.

    2017-12-01

    A thickness, floe size, and enthalpy distribution (TFED) sea ice model, implemented numerically into the Pan-arctic Ice-Ocean Modeling and Assimilation System (PIOMAS), is used to investigate the seasonal evolution of the Arctic marginal ice zone (MIZ) and its floe size distribution. The TFED sea ice model, by coupling the Zhang et al. [2015] sea ice floe size distribution (FSD) theory with the Thorndike et al. [1975] ice thickness distribution (ITD) theory, simulates 12-category FSD and ITD explicitly and jointly. A range of ice thickness and floe size observations were used for model calibration and validation. The model creates FSDs that generally obey a power law or upper truncated power law, as observed by satellites and aerial surveys. In this study, we will examine the role of ice fragmentation and lateral melting in altering FSDs in the Arctic MIZ. We will also investigate how changes in FSD impact the seasonal evolution of the MIZ by modifying the thermodynamic processes.

  4. Variations in the Sea Ice Edge and the Marginal Ice Zone on Different Spatial Scales as Observed from Different Satellite Sensor

    NASA Technical Reports Server (NTRS)

    Markus, Thorsten; Henrichs, John

    2006-01-01

    The Marginal sea Ice Zone (MIZ) and the sea ice edge are the most dynamic areas of the sea ice cover. Knowledge of the sea ice edge location is vital for routing shipping in the polar regions. The ice edge is the location of recurrent plankton blooms, and is the habitat for a number of animals, including several which are under severe ecological threat. Polar lows are known to preferentially form along the sea ice edge because of induced atmospheric baroclinicity, and the ice edge is also the location of both vertical and horizontal ocean currents driven by thermal and salinity gradients. Finally, sea ice is both a driver and indicator of climate change and monitoring the position of the ice edge accurately over long time periods enables assessment of the impact of global and regional warming near the poles. Several sensors are currently in orbit that can monitor the sea ice edge. These sensors, though, have different spatial resolutions, different limitations, and different repeat frequencies. Satellite passive microwave sensors can monitor the ice edge on a daily or even twice-daily basis, albeit with low spatial resolution - 25 km for the Special Sensor Microwave Imager (SSM/I) or 12.5 km for the Advanced Microwave Scanning Radiometer (AMSR-E). Although special methods exist that allow the detection of the sea ice edge at a quarter of that nominal resolution (PSSM). Visible and infrared data from the Advanced Very High Resolution Radiometer (AVHRR) and from the Moderate Resolution Imaging Spectroradiometer (MODIS) provide daily coverage at 1 km and 250 m, respectively, but the surface observations me limited to cloud-free periods. The Landsat 7 Enhanced Thematic Mapper (ETM+) has a resolution of 15 to 30 m but is limited to cloud-free periods as well, and does not provide daily coverage. Imagery from Synthetic Aperture Radar (SAR) instruments has resolutions of tens of meters to 100 m, and can be used to distinguish open water and sea ice on the basis of surface

  5. Holocene Activity of the Quelccaya Ice Cap: A Working Model

    NASA Astrophysics Data System (ADS)

    Lowell, T. V.; Smith, C. A.; Kelly, M. A.; Stroup, J. S.

    2012-12-01

    The patterns and magnitudes of past climate change in the topics are still under discussion. We contribute here by reporting on patterns of glacier length changes of the largest glacier in the tropics, Quelccaya Ice Cap (~13.9°S, 70.9°W, summit at 5645 m). This ice cap has several local domes that may have different patterns of length changes because of differing elevations of the domes (high to the north, lower to the south). Prior work (Mark et al. 2003, Abbott et al., 2004; Thompson et al., 2005; Buffen, et al., 2009), new radiocarbon ages, and stratigraphic and geomorphic relationships are used to determine the general pattern of length changes for the outlets from this ice cap. We exploit geomorphic relationships and present new radiocarbon ages on interpreted stratigraphic sections to determine the pattern of length changes for this ice cap. Ice retreated during late glacial times (Rodbell and Seltzer, 2000; Kelly et al., in press). By 11,400 yr BP it had reached a position ~1.2 km beyond its present (2000 AD) extent. While length during the early Holocene is problematic, present evidence permits, but does not prove, extents of 0.5 to 1.0 km down-valley from the present margin. Between 6400 and 4400 yr BP the ice cap was smaller than present, but it advanced multiple times during the late Holocene. Lengths of up to 1 km beyond present were achieved at 3400 yr BP and ~500 yr BP. Additionally, the ice advanced to 0.8 km beyond its present margin at 1600 yr BP. Because these glaciers were temperate, we take these lengths to represent primarily changes in temperature. This may suggest that lowering insolation values in the northern hemisphere during the Holocene provide a first order control on tropical temperatures. Alternatively, it may be that major reorganization of the topical circulation belts about 5000 yr BP yields two configurations of the QIC and hence Holocene temperatures - one at the present ice margin and and the second about 1 km beyond the

  6. Transport of contaminants by Arctic sea ice and surface ocean currents

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

    Pfirman, S.

    1995-12-31

    Sea ice and ocean currents transport contaminants in the Arctic from source areas on the shelves, to biologically active regions often more than a thousand kilometers away. Coastal regions along the Siberian margin are polluted by discharges of agricultural, industrial and military wastes in river runoff, from atmospheric deposition and ocean dumping. The Kara Sea is of particular concern because of deliberate dumping of radioactive waste, as well as the large input of polluted river water. Contaminants are incorporated in ice during suspension freezing on the shelves, and by atmospheric deposition during drift. Ice releases its contaminant load through brinemore » drainage, surface runoff of snow and meltwater, and when the floe disintegrates. The marginal ice zone, a region of intense biological activity, may also be the site of major contaminant release. Potentially contaminated ice from the Kara Sea is likely to influence the marginal ice zones of the Barents and Greenland seas. From studies conducted to date it appears that sea ice from the Kara Sea does not typically enter the Beaufort Gyre, and thus is unlikely to affect the northern Canadian and Alaskan margins.« less

  7. Marginal Ice Zone Bibliography.

    DTIC Science & Technology

    1985-06-01

    A Voyage of Discovery. George Deacon 70th An-niversary Volume, (M. Angel, ed.), Pergamon Press, Oxford, p.15-41. Coachman, L.K., C.A. Barnes, 1961...some polar contrasts. In: S "" RUsium on Antarctic Ice and Water Masses, ( George Deacon, ed.), Sci- 72 Lebedev, A.A., 1968: Zone of possible icing of...Atlantic and Western Europe. British Meteorological Office. Geophysical Memoirs, 4(41). Brost , R.A., J.C. Wyngaard, 1978: A model study of the stably

  8. The northern Uummannaq Ice Stream System, West Greenland: ice dynamics and and controls upon deglaciation

    NASA Astrophysics Data System (ADS)

    Lane, Timothy; Roberts, David; Rea, Brice; Cofaigh, Colm Ó.; Vieli, Andreas

    2013-04-01

    At the Last Glacial Maximum (LGM), the Uummannaq Ice Stream System comprised a series coalescent outlet glaciers which extended along the trough to the shelf edge, draining a large proportion of the West Greenland Ice Sheet. Geomorphological mapping, terrestrial cosmogenic nuclide (TCN) exposure dating, and radiocarbon dating constrain warm-based ice stream activity in the north of the system to 1400 m a.s.l. during the LGM. Intervening plateaux areas (~ 2000 m a.s.l.) either remained ice free, or were covered by cold-based icefields, preventing diffluent or confluent flow throughout the inner to outer fjord region. Beyond the fjords, a topographic sill north of Ubekendt Ejland prevented the majority of westward ice flow, forcing it south through Igdlorssuit Sund, and into the Uummannaq Trough. Here it coalesced with ice from the south, forming the trunk zone of the UISS. Deglaciation of the UISS began at 14.9 cal. ka BP, rapidly retreating through the overdeepened Uummannaq Trough. Once beyond Ubekendt Ejland, the northern UISS retreated northwards, separating from the south. Retreat continued, and ice reached the present fjord confines in northern Uummannaq by 11.6 kyr. Both geomorphological (termino-lateral moraines) and geochronological (14C and TCN) data provide evidence for an ice marginal stabilisation at within Karrat-Rink Fjord, at Karrat Island, from 11.6-6.9 kyr. The Karrat moraines appear similar in both fjord position and form to 'Fjord Stade' moraines identified throughout West Greenland. Though chronologies constraining moraine formation are overlapping (Fjord Stade moraines - 9.3-8.2 kyr, Karrat moraines - 11.6-6.9 kyr), these moraines have not been correlated. This ice margin stabilisation was able to persist during the Holocene Thermal Maximum (~7.2 - 5 kyr). It overrode climatic and oceanic forcings, remaining on Karrat Island throughout peaks of air temperature and relative sea-level, and during the influx of the warm West Greenland Current into

  9. Ice stream activity scaled to ice sheet volume during Laurentide Ice Sheet deglaciation.

    PubMed

    Stokes, C R; Margold, M; Clark, C D; Tarasov, L

    2016-02-18

    The contribution of the Greenland and West Antarctic ice sheets to sea level has increased in recent decades, largely owing to the thinning and retreat of outlet glaciers and ice streams. This dynamic loss is a serious concern, with some modelling studies suggesting that the collapse of a major ice sheet could be imminent or potentially underway in West Antarctica, but others predicting a more limited response. A major problem is that observations used to initialize and calibrate models typically span only a few decades, and, at the ice-sheet scale, it is unclear how the entire drainage network of ice streams evolves over longer timescales. This represents one of the largest sources of uncertainty when predicting the contributions of ice sheets to sea-level rise. A key question is whether ice streams might increase and sustain rates of mass loss over centuries or millennia, beyond those expected for a given ocean-climate forcing. Here we reconstruct the activity of 117 ice streams that operated at various times during deglaciation of the Laurentide Ice Sheet (from about 22,000 to 7,000 years ago) and show that as they activated and deactivated in different locations, their overall number decreased, they occupied a progressively smaller percentage of the ice sheet perimeter and their total discharge decreased. The underlying geology and topography clearly influenced ice stream activity, but--at the ice-sheet scale--their drainage network adjusted and was linked to changes in ice sheet volume. It is unclear whether these findings can be directly translated to modern ice sheets. However, contrary to the view that sees ice streams as unstable entities that can accelerate ice-sheet deglaciation, we conclude that ice streams exerted progressively less influence on ice sheet mass balance during the retreat of the Laurentide Ice Sheet.

  10. Soft-sediment deformation structures from an ice-marginal storm-tide interactive system, Permo-Carboniferous Talchir Formation, Talchir Coalbasin, India

    NASA Astrophysics Data System (ADS)

    Bhattacharya, H. N.; Bhattacharya, Biplab

    2010-01-01

    Permo-Carboniferous Talchir Formation, Talchir Coalbasin, India, records sedimentation during a phase of climatic amelioration in an ice-marginal storm-affected shelf. Evidences of subtidal processes are preserved only under thick mud drapes deposited during waning storm phases. Various soft-sediment deformation structures in some sandstone/siltstone-mudstone interbeds, like syn-sedimentary faults, deformed laminations, sand-silt flows, convolute laminations and various flame structures, suggest liquefaction and fluidization of the beds due to passage of syn-depositional seismic shocks. In the Late Paleozoic ice-marginal shelf, such earthquake tremors could be generated by crustal movements in response to glacioisostatic adjustments of the basin floor.

  11. In situ cosmogenic radiocarbon production and 2-D ice flow line modeling for an Antarctic blue ice area

    NASA Astrophysics Data System (ADS)

    Buizert, Christo; Petrenko, Vasilii V.; Kavanaugh, Jeffrey L.; Cuffey, Kurt M.; Lifton, Nathaniel A.; Brook, Edward J.; Severinghaus, Jeffrey P.

    2012-06-01

    Radiocarbon measurements at ice margin sites and blue ice areas can potentially be used for ice dating, ablation rate estimates and paleoclimatic reconstructions. Part of the measured signal comes from in situ cosmogenic 14C production in ice, and this component must be well understood before useful information can be extracted from 14C data. We combine cosmic ray scaling and production estimates with a two-dimensional ice flow line model to study cosmogenic 14C production at Taylor Glacier, Antarctica. We find (1) that 14C production through thermal neutron capture by nitrogen in air bubbles is negligible; (2) that including ice flow patterns caused by basal topography can lead to a surface 14C activity that differs by up to 25% from the activity calculated using an ablation-only approximation, which is used in all prior work; and (3) that at high ablation margin sites, solar modulation of the cosmic ray flux may change the strength of the dominant spallogenic production by up to 10%. As part of this effort we model two-dimensional ice flow along the central flow line of Taylor Glacier. We present two methods for parameterizing vertical strain rates, and assess which method is more reliable for Taylor Glacier. Finally, we present a sensitivity study from which we conclude that uncertainties in published cosmogenic production rates are the largest source of potential error. The results presented here can inform ongoing and future 14C and ice flow studies at ice margin sites, including important paleoclimatic applications such as the reconstruction of paleoatmospheric 14C content of methane.

  12. The Norwegian remote sensing experiment (Norsex) in a marginal ice zone

    NASA Technical Reports Server (NTRS)

    Farrelly, B.; Johannessen, J.; Johannessen, O. M.; Svendson, E.; Kloster, K.; Horjen, I.; Campbell, W. J.; Crawford, J.; Harrington, R.; Jones, L.

    1981-01-01

    Passive and active microwave measurements from surface based, airborne, and satellite instruments were obtained together with surface observations northwest of Svalbard. Emissivities of different ice patches in the ice edge region over the spectral range from 4.9 to 94 GHz are presented. The combination of a 6.6 GHz microwave radiometer with a 14.6 GHz scatterometer demonstrates the usefulness of an active/passive system in ice classification. A variety of mesoscale features under different meteorological conditions is revealed by a 1.36 GHz synthetic aperture radar. Ice edge location by Nimbus 7 scanning multifrequency microwave radiometer is shown accurate to 10 km when the 37 GHz horizontal polarized channel is used.

  13. Insect-Based Holocene (and Last Interglacial?) Paleothermometry from the E and NW Greenland Ice Sheet Margins: A Fly's-Eye View of Warmth on Greenland

    NASA Astrophysics Data System (ADS)

    Axford, Y.; Bigl, M.; Carrio, C.; Corbett, L. B.; Francis, D. R.; Hall, B. L.; Kelly, M. A.; Levy, L.; Lowell, T. V.; Osterberg, E. C.; Richter, N.; Roy, E.; Schellinger, G. C.

    2013-12-01

    Here we present new paleotemperature reconstructions based upon insect (Chironomidae) assemblages and other proxies from lake sediment cores recovered in east Greenland at ~71° N near Scoresby Sund and in northwest Greenland at ~77° N near Thule/Qaanaaq. In east Greenland, Last Chance Lake (informal name) is a small, non-glacial lake situated ~90 km east of the Greenland Ice Sheet margin. The lake preserves a sedimentary record of the entire Holocene (Levy et al. 2013). Chironomids from Last Chance Lake record cold summer temperatures (and establishment of a cold-climate fauna including abundant Oliveridia and Pseudodiamesa) during the late Holocene, preceded by summer temperatures estimated to have been 3 to 6°C warmer during the first half of the Holocene (when summer insolation forcing was greater than today). In northwest Greenland, Delta Sø and Wax Lips Lake (informal name) both preserve Holocene sediments. Here we discuss the late Holocene chironomid record from Delta Sø, whereas from Wax Lips Lake (a small, non-glacial lake situated ~2 km west of the ice sheet margin) we present a longer sedimentary and biostratigraphic record. The deeper portions of cores from Wax Lips Lake yield pre-Holocene and nonfinite radiocarbon ages, suggesting that this lake preserves sediments predating the Last Glacial Maximum. Abundant chironomids in the pre-glacial sediments appear to record interglacial conditions, and we infer that these sediments may date to the Last Interglacial (Eemian). The preservation of in situ Last Interglacial lacustrine sediments so close to the modern ice sheet margin suggests a minimally erosive glacierization style throughout the last glacial period, like that inferred for other Arctic locales such as on Baffin Island (Briner et al. 2007), ~750 km southwest of our study site. Our study sites are situated nearby key ice core sites (including NEEM, Camp Century, Agassiz and Renland) and very close to the ice sheet margin. These chironomid

  14. Insect-Based Holocene (and Last Interglacial?) Paleothermometry from the E and NW Greenland Ice Sheet Margins: A Fly's-Eye View of Warmth on Greenland

    NASA Astrophysics Data System (ADS)

    Axford, Y.; Bigl, M.; Carrio, C.; Corbett, L. B.; Francis, D. R.; Hall, B. L.; Kelly, M. A.; Levy, L.; Lowell, T. V.; Osterberg, E. C.; Richter, N.; Roy, E.; Schellinger, G. C.

    2011-12-01

    Here we present new paleotemperature reconstructions based upon insect (Chironomidae) assemblages and other proxies from lake sediment cores recovered in east Greenland at ~71° N near Scoresby Sund and in northwest Greenland at ~77° N near Thule/Qaanaaq. In east Greenland, Last Chance Lake (informal name) is a small, non-glacial lake situated ~90 km east of the Greenland Ice Sheet margin. The lake preserves a sedimentary record of the entire Holocene (Levy et al. 2013). Chironomids from Last Chance Lake record cold summer temperatures (and establishment of a cold-climate fauna including abundant Oliveridia and Pseudodiamesa) during the late Holocene, preceded by summer temperatures estimated to have been 3 to 6°C warmer during the first half of the Holocene (when summer insolation forcing was greater than today). In northwest Greenland, Delta Sø and Wax Lips Lake (informal name) both preserve Holocene sediments. Here we discuss the late Holocene chironomid record from Delta Sø, whereas from Wax Lips Lake (a small, non-glacial lake situated ~2 km west of the ice sheet margin) we present a longer sedimentary and biostratigraphic record. The deeper portions of cores from Wax Lips Lake yield pre-Holocene and nonfinite radiocarbon ages, suggesting that this lake preserves sediments predating the Last Glacial Maximum. Abundant chironomids in the pre-glacial sediments appear to record interglacial conditions, and we infer that these sediments may date to the Last Interglacial (Eemian). The preservation of in situ Last Interglacial lacustrine sediments so close to the modern ice sheet margin suggests a minimally erosive glacierization style throughout the last glacial period, like that inferred for other Arctic locales such as on Baffin Island (Briner et al. 2007), ~750 km southwest of our study site. Our study sites are situated nearby key ice core sites (including NEEM, Camp Century, Agassiz and Renland) and very close to the ice sheet margin. These chironomid

  15. Formation processes of sea ice floe size distribution in the interior pack and its relationship to the marginal ice zone off East Antarctica

    NASA Astrophysics Data System (ADS)

    Toyota, Takenobu; Kohout, Alison; Fraser, Alexander D.

    2016-09-01

    To understand the behavior of the Seasonal Ice Zone (SIZ), which is composed of sea-ice floes of various sizes, knowledge of the floe size distribution (FSD) is important. In particular, FSD in the Marginal Ice Zone (MIZ), controlled by wave-ice interaction, plays an important role in determining the retreating rates of sea-ice extent on a global scale because the cumulative perimeter of floes enhances melting. To improve the understanding of wave-ice interaction and subsequent effects on FSD in the MIZ, FSD measurements were conducted off East Antarctica during the second Sea Ice Physics and Ecosystems eXperiment (SIPEX-2) in late winter 2012. Since logistical reasons limited helicopter operations to two interior ice regions, FSD in the interior ice region was determined using a combination of heli-photos and MODIS satellite visible images. The possible effect of wave-ice interaction in the MIZ was examined by comparison with past results obtained in the same MIZ, with our analysis showing: (1) FSD in the interior ice region is basically scale invariant for both small- (<100 m) and large- (>1 km) scale regimes; (2) although fractal dimensions are quite different between these two regimes, they are both rather close to that in the MIZ; and (3) for floes <100 m in diameter, a regime shift which appeared at 20-40 m in the MIZ is absent. These results indicate that one role of wave-ice interaction is to modulate the FSD that already exists in the interior ice region, rather than directly determine it. The possibilities of floe-floe collisions and storm-induced lead formation are considered as possible formation processes of FSD in the interior pack.

  16. Selected physical, biological and biogeochemical implications of a rapidly changing Arctic Marginal Ice Zone

    NASA Astrophysics Data System (ADS)

    Barber, David G.; Hop, Haakon; Mundy, Christopher J.; Else, Brent; Dmitrenko, Igor A.; Tremblay, Jean-Eric; Ehn, Jens K.; Assmy, Philipp; Daase, Malin; Candlish, Lauren M.; Rysgaard, Søren

    2015-12-01

    The Marginal Ice Zone (MIZ) of the Arctic Ocean is changing rapidly due to a warming Arctic climate with commensurate reductions in sea ice extent and thickness. This Pan-Arctic review summarizes the main changes in the Arctic ocean-sea ice-atmosphere (OSA) interface, with implications for primary- and secondary producers in the ice and the underlying water column. Changes in the Arctic MIZ were interpreted for the period 1979-2010, based on best-fit regressions for each month. Trends of increasingly open water were statistically significant for each month, with quadratic fit for August-November, illustrating particularly strong seasonal feedbacks in sea-ice formation and decay. Geographic interpretations of physical and biological changes were based on comparison of regions with significant changes in sea ice: (1) The Pacific Sector of the Arctic Ocean including the Canada Basin and the Beaufort, Chukchi and East Siberian seas; (2) The Canadian Arctic Archipelago; (3) Baffin Bay and Hudson Bay; and (4) the Barents and Kara seas. Changes in ice conditions in the Barents sea/Kara sea region appear to be primarily forced by ocean heat fluxes during winter, whereas changes in the other sectors appear to be more summer-autumn related and primarily atmospherically forced. Effects of seasonal and regional changes in OSA-system with regard to increased open water were summarized for photosynthetically available radiation, nutrient delivery to the euphotic zone, primary production of ice algae and phytoplankton, ice-associated fauna and zooplankton, and gas exchange of CO2. Changes in the physical factors varied amongst regions, and showed direct effects on organisms linked to sea ice. Zooplankton species appear to be more flexible and likely able to adapt to variability in the onset of primary production. The major changes identified for the ice-associated ecosystem are with regard to production timing and abundance or biomass of ice flora and fauna, which are related to

  17. Quantifying the Evolution of Melt Ponds in the Marginal Ice Zone Using High Resolution Optical Imagery and Neural Networks

    NASA Astrophysics Data System (ADS)

    Ortiz, M.; Pinales, J. C.; Graber, H. C.; Wilkinson, J.; Lund, B.

    2016-02-01

    Melt ponds on sea ice play a significant and complex role on the thermodynamics in the Marginal Ice Zone (MIZ). Ponding reduces the sea ice's ability to reflect sunlight, and in consequence, exacerbates the albedo positive feedback cycle. In order to understand how melt ponds work and their effect on the heat uptake of sea ice, we must quantify ponds through their seasonal evolution first. A semi-supervised neural network three-class learning scheme using a gradient descent with momentum and adaptive learning rate backpropagation function is applied to classify melt ponds/melt areas in the Beaufort Sea region. The network uses high resolution panchromatic satellite images from the MEDEA program, which are collocated with autonomous platform arrays from the Marginal Ice Zone Program, including ice mass-balance buoys, arctic weather stations and wave buoys. The goal of the study is to capture the spatial variation of melt onset and freeze-up of the ponds within the MIZ, and gather ponding statistics such as size and concentration. The innovation of this work comes from training the neural network as the melt ponds evolve over time; making the machine learning algorithm time-dependent, which has not been previously done. We will achieve this by analyzing the image histograms through quantification of the minima and maxima intensity changes as well as linking textural variation information of the imagery. We will compare the evolution of the melt ponds against several different array sites on the sea ice to explore if there are spatial differences among the separated platforms in the MIZ.

  18. Ice, Ocean and Atmosphere Interactions in the Arctic Marginal Ice Zone

    DTIC Science & Technology

    2015-09-30

    the northward retreat of the ice edge. Through the long-term measurement of the key oceanic, atmospheric, and sea ice processes that...began to move southward towards the Alaskan coast. In 2104 the anomalous areas of ice retreat were the region north of Alaska...and Siberia. (see figures below). This is not uncommon as these regions have seen the greatest retreat in sea ice. See http://nsidc.org

  19. Pedestal Craters in Utopia Planitia and Malea Planum: Evidence for a Past Ice-Rich Substrate from Marginal Sublimation Pits.

    NASA Astrophysics Data System (ADS)

    Kadish, S. J.; Head, J. W.; Barlow, N. G.; Marchant, D. R.

    2008-09-01

    Introduction: Pedestal craters (Pd) are a subclass of impact craters unique to Mars [1] characterized by a crater perched near the center of a pedestal (mesa or plateau) that is surrounded by a quasi-circular, outward-facing scarp. The marginal scarp is usually several crater diameters from the crater rim (Figs. 2,4,5), and tens to over 100 meters above the surrounding plains (Fig. 2). Pd have been interpreted to form by armoring of the proximal substrate during the impact event. Hypotheses for the armoring mechanism include an ejecta covering [e.g., 3], increased ejecta mobilization caused by volatile substrates [4], distal glassy/melt-rich veneers [5], and/or an atmospheric blast/thermal effect [6]. Subsequently, a marginal scarp forms by preferential erosion of the substrate surrounding the armored region, most commonly thought to involve eolian removal of fine-grained, non-armored material [e.g., 3]. An understanding of the distribution of Pd, which form predominantly poleward of ~40°N and S latitude [7-9] (Fig. 1), and the role of redistribution of ice and dust during periods of climate change [e.g., 10-11], suggests that the substrate might have been volatile-rich [8-9, 12-14]. As such, some researchers [e.g., 8-9] have proposed a model for Pd formation that involves impact during periods of higher obliquity, when mid- to high-latitude substrates were characterized by thick deposits of snow and ice [e.g., 15]. Subsequent sublimation of the volatile units, except below the armored regions, yielded the perched Pd. Thus, this model predicts that thick deposits of snow/ice should underlie Pd. This is in contrast to the eolian model [3], which calls primarily for deflation of sand and dust. Here, we show the results of our study [8,16] that has documented and characterized 2461 Pd on Mars equatorward of ~65° N and S latitude (Fig. 1) in order to test these hypotheses for the origin of pedestal craters. In particular, we report on the detection of 50 Pd in Utopia

  20. Ice-sheet dynamics through the Quaternary on the mid-Norwegian continental margin inferred from 3D seismic data.

    PubMed

    Montelli, A; Dowdeswell, J A; Ottesen, D; Johansen, S E

    2017-02-01

    Reconstructing the evolution of ice sheets is critical to our understanding of the global environmental system, but most detailed palaeo-glaciological reconstructions have hitherto focused on the very recent history of ice sheets. Here, we present a three-dimensional (3D) reconstruction of the changing nature of ice-sheet derived sedimentary architecture through the Quaternary Ice Age of almost 3 Ma. An extensive geophysical record documents a marine-terminating, calving Fennoscandian Ice Sheet (FIS) margin present periodically on the mid-Norwegian shelf since the beginning of the Quaternary. Spatial and temporal variability of the FIS is illustrated by the gradual development of fast-flowing ice streams and associated intensification of focused glacial erosion and sedimentation since that time. Buried subglacial landforms reveal a complex and dynamic ice sheet, with converging palaeo-ice streams and several flow-switching events that may reflect major changes in topography and basal thermal regime. Lack of major subglacial meltwater channels suggests a largely distributed drainage system beneath the marine-terminating part of the FIS. This palaeo-environmental examination of the FIS provides a useful framework for ice-sheet modelling and shows that fragmentary preservation of buried surfaces and variability of ice-sheet dynamics should be taken into account when reconstructing glacial history from spatially limited datasets.

  1. Influence of aeolian activities on the distribution of microbial abundance in glacier ice

    NASA Astrophysics Data System (ADS)

    Chen, Y.; Li, X.-K.; Si, J.; Wu, G.-J.; Tian, L.-D.; Xiang, S.-R.

    2014-10-01

    Microorganisms are continuously blown onto the glacier snow, and thus the glacial depth profiles provide excellent archives of microbial communities and climatic and environmental changes. However, it is uncertain about how aeolian processes that cause climatic changes control the distribution of microorganisms in the glacier ice. In the present study, microbial density, stable isotopic ratios, 18O / 16O in the precipitation, and mineral particle concentrations along the glacial depth profiles were collected from ice cores from the Muztag Ata glacier and the Dunde ice cap. The ice core data showed that microbial abundance was often, but not always associated with high concentrations of particles. Results also revealed clear seasonal patterning with high microbial abundance occurring in both the cooling autumn and warming spring-summer seasons. Microbial comparisons among the neighbouring glaciers display a heterogeneous spatial pattern, with the highest microbial cell density in the glaciers lying adjacent to the central Asian deserts and lowest microbial density in the southwestern margin of the Tibetan Plateau. In conclusion, microbial data of the glaciers indicates the aeolian deposits of microorganisms in the glacier ice and that the spatial patterns of microorgansisms are related to differences in sources of microbial flux and intensity of aeolian activities in the current regions. The results strongly support our hypothesis of aeolian activities being the main agents controlling microbial load in the glacier ice.

  2. Polar Ice Caps: a Canary for the Greenland Ice Sheet

    NASA Astrophysics Data System (ADS)

    Honsaker, W.; Lowell, T. V.; Sagredo, E.; Kelly, M. A.; Hall, B. L.

    2010-12-01

    Ice caps are glacier masses that are highly sensitive to climate change. Because of their hypsometry they can have a binary state. When relatively slight changes in the equilibrium line altitude (ELA) either intersect or rise above the land the ice can become established or disappear. Thus these upland ice masses have a fast response time. Here we consider a way to extract the ELA signal from independent ice caps adjacent to the Greenland Ice Sheet margin. It may be that these ice caps are sensitive trackers of climate change that also impact the ice sheet margin. One example is the Istorvet Ice Cap located in Liverpool Land, East Greenland (70.881°N, 22.156°W). The ice cap topography and the underlying bedrock surface dips to the north, with peak elevation of the current ice ranging in elevation from 1050 to 745 m.a.s.l. On the eastern side of the ice mass the outlet glaciers extending down to sea level. The western margin has several small lobes in topographic depressions, with the margin reaching down to 300 m.a.s.l. Topographic highs separate the ice cap into at least 5 main catchments, each having a pair of outlet lobes toward either side of the ice cap. Because of the regional bedrock slope each catchment has its own elevation range. Therefore, as the ELA changes it is possible for some catchments of the ice cap to experience positive mass balance while others have a negative balance. Based on weather observations we estimate the present day ELA to be ~1000 m.a.s.l, meaning mass balance is negative for the majority of the ice cap. By tracking glacier presence/absence in these different catchments, we can reconstruct small changes in the ELA. Another example is the High Ice Cap (informal name) in Milne Land (70.903°N, 25.626°W, 1080 m), East Greenland. Here at least 4 unconformities in ice layers found near the southern margin of the ice cap record changing intervals of accumulation and ablation. Therefore, this location may also be sensitive to slight

  3. Abbot Ice Shelf, the Amundsen Sea Continental Margin and the Southern Boundary of the Bellingshausen Plate Seaward of West Antarctica

    NASA Astrophysics Data System (ADS)

    Cochran, J. R.; Tinto, K. J.; Bell, R. E.

    2014-12-01

    The Abbot Ice Shelf extends 450 km along the coast of West Antarctica between 103°W and 89°W and straddles the boundary between the Bellingshausen Sea continental margin, which overlies a former subduction zone, and Amundsen Sea rifted continental margin. Inversion of NASA Operation IceBridge airborne gravity data for sub-ice bathymetry shows that the western part of the ice shelf, as well as Cosgrove Ice Shelf to the south, are underlain by a series of east-west trending rift basins. The eastern boundary of the rifted terrain coincides with the eastern boundary of rifting between Antarctica and Zealandia and the rifts formed during the early stages of this rifting. Extension in these rifts is minor as rifting quickly jumped north of Thurston Island. The southern boundary of the Cosgrove Rift is aligned with the southern boundary of a sedimentary basin under the Amundsen Embayment continental shelf to the west, also formed by Antarctica-Zealandia rifting. The shelf basin has an extension factor, β, of 1.5 - 1.7 with 80 -100 km of extension occurring in an area now ~250 km wide. Following this extension early in the rifting process, rifting centered to the north of the present shelf edge and proceeded to continental rupture. Since then, the Amundsen Embayment continental shelf has been tectonically quiescent and has primarily been shaped though subsidence, sedimentation and the passage of the West Antarctic Ice Sheet back and forth across it. The former Bellingshausen Plate was located seaward of the Amundsen Sea margin prior to its incorporation into the Antarctic Plate at ~62 Ma. During the latter part of its existence, Bellingshausen plate motion had a clockwise rotational component relative to Antarctica producing convergence between the Bellingshausen and Antarctic plates east of 102°W. Seismic reflection and gravity data show that this convergence is expressed by an area of intensely deformed sediments beneath the continental slope from 102°W to 95°W and

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

    NASA Astrophysics Data System (ADS)

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

    2017-08-01

    This study analyzed shipboard air-sea measurements acquired by the icebreaker Aurora Australis during its off-winter operation in December 2010 to May 2012. Mean conditions over 7 months (October-April) were compiled from a total of 22 ship tracks. The icebreaker traversed the water between Hobart, Tasmania, and the Antarctic continent, providing valuable in situ insight into two dynamically important, yet poorly sampled, regimes: the sub-Antarctic Southern Ocean and the Antarctic marginal ice zone (MIZ) in the Indian Ocean sector. The transition from the open water to the ice-covered surface creates sharp changes in albedo, surface roughness, and air temperature, leading to consequential effects on air-sea variables and fluxes. Major effort was made to estimate the air-sea fluxes in the MIZ using the bulk flux algorithms that are tuned specifically for the sea-ice effects, while computing the fluxes over the sub-Antarctic section using the COARE3.0 algorithm. The study evidenced strong sea-ice modulations on winds, with the southerly airflow showing deceleration (convergence) in the MIZ and acceleration (divergence) when moving away from the MIZ. Marked seasonal variations in heat exchanges between the atmosphere and the ice margin were noted. The monotonic increase in turbulent latent and sensible heat fluxes after summer turned the MIZ quickly into a heat loss regime, while at the same time the sub-Antarctic surface water continued to receive heat from the atmosphere. The drastic increase in turbulent heat loss in the MIZ contrasted sharply to the nonsignificant and seasonally invariant turbulent heat loss over the sub-Antarctic open water.Plain Language SummaryThe icebreaker Aurora Australis is a research and supply vessel that is regularly chartered by the Australian Antarctic Division during the southern summer to operate in waters between Hobart, Tasmania, and Antarctica. The vessel serves as the main lifeline to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSHE24A1420P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSHE24A1420P"><span>Modeling Primary Productivity in the <span class="hlt">Margin</span> <span class="hlt">Ice</span> Zone from Glider-Based Measurements of Chlorophyll and Light during the 2014 Miz Program</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Perry, M. J.; Lee, C.; Rainville, L.; Cetinic, I.; Yang, E. J.; Kang, S. H.</p> <p>2016-02-01</p> <p>In late summer 2014 during the <span class="hlt">Marginal</span> <span class="hlt">Ice</span> Zone (MIZ) Experiment, an international project sponsored by ONR, four Seagliders transited open water, through the <span class="hlt">marginal</span> <span class="hlt">ice</span> zone, and under <span class="hlt">ice</span>-covered regions in the Beaufort Sea, penetrating as far as 100 km into the <span class="hlt">ice</span> pack. The gliders navigated either by GPS in open water or, when under the <span class="hlt">ice</span>, by acoustics from sound sources embedded in the MIZ autonomous observing array. The glider sensor suite included temperature, temperature microstructure, salinity, oxygen, chlorophyll fluorescence, optical backscatter, and multi-spectral downwelling irradiance. Cruises on the IBRV Araon operating in the open Beaufort Sea and on the R/V Ukpik and Norseman operating in continental shelf waters off Alaska's north slope allowed us to construct proxy libraries for converting chlorophyll fluorescence to chlorophyll concentration and optical backscatter to particulate organic carbon concentration. Water samples were collected for chlorophyll and particulate organic carbon analysis on the cruises and aligned with optical profiles of fluorescence and backscatter using sensors that were factory calibrated at the same time as the glider sensors. Fields of chlorophyll, particulate organic carbon, light, and primary productivity are constructed from the glider data. Productivity is modeled as a function of chlorophyll and light, using photosynthesis-light (PE) models with available PE parameters from Arctic measurements. During August the region under the <span class="hlt">ice</span> was characterized by a deep chlorophyll maximum layer with low rates of production in overlying waters. A phytoplankton bloom developed in open water at the end of September, preceding the rapid reformation of <span class="hlt">ice</span>, despite shorter days and reduce irradiation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.G31A0888L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.G31A0888L"><span>Deglaciation-induced uplift and seasonal variations patterns of bedrock displacement in Greenland <span class="hlt">ice</span> sheet <span class="hlt">margin</span> observed from GPS, GRACE and InSAR</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lu, Q.; Amelung, F.; Wdowinski, S.</p> <p>2017-12-01</p> <p>The Greenland <span class="hlt">ice</span> sheet is rapidly shrinking with the fastest retreat and thinning occurring at the <span class="hlt">ice</span> sheet <span class="hlt">margin</span> and near the outlet glaciers. The changes of the <span class="hlt">ice</span> mass cause an elastic response of the bedrock. Theoretically, <span class="hlt">ice</span> mass loss during the summer melting season is associated with bedrock uplift, whereas increasing <span class="hlt">ice</span> mass during the winter months is associated with bedrock subsidence. Here we examine the annual changes of the vertical displacements measured at 37 GPS stations and compare the results with Greenland drainage basins' gravity from GRACE. We use both Fourier Series (FS) analysis and Cubic Smoothing Spline (CSS) method to estimate the phases and amplitudes of seasonal variations. Both methods show significant differences seasonal behaviors in southern and northern Greenland. The average amplitude of bedrock displacements (3.29±0.02mm) in south Greenland is about 2 times larger than the north (1.65±0.02mm). The phase of bedrock maximum uplift (November) is considerably consistent with the time of minimum <span class="hlt">ice</span> mass load in south Greenland (October). However, the phase of bedrock maximum uplift in north Greenland (February) is 4 months later than the minimum <span class="hlt">ice</span> mass load in north Greenland basins (October). In addition, we present ground deformation near several famous glaciers in Greenland such as Petermann glacier and Jakobshavn glacier. We process InSAR data from TerraSAR-X and Sentinel satellite, based on small baseline interferograms. We observed rapid deglaciation-induced uplift and seasonal variations on naked bedrock near the glacier <span class="hlt">ice</span> <span class="hlt">margin</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.8433B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.8433B"><span>Dynamic behaviour of <span class="hlt">ice</span> streams: the North East Greenland <span class="hlt">Ice</span> Stream</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bons, Paul D.; Jansen, Daniela; Schaufler, Svenja; de Riese, Tamara; Sachau, Till; Weikusat, Ilka</p> <p>2017-04-01</p> <p>The flow of <span class="hlt">ice</span> towards the <span class="hlt">margins</span> of <span class="hlt">ice</span> sheets is far from homogeneous. <span class="hlt">Ice</span> streams show much higher flow velocities than their surroundings and may extend, for example the North East Greenland <span class="hlt">Ice</span> Stream (NEGIS), towards the centre of the sheet. The elevated flow velocity inside an <span class="hlt">ice</span> stream causes <span class="hlt">marginal</span> shearing and convergent flow, which in turn leads to folding of <span class="hlt">ice</span> layers. Such folding was documented in the Petermann Glacier in northern Greenland (Bons et al., 2016). 3-dimensional structural modelling using radargrams shows that folding is more intense adjacent to NEGIS than inside it, despite the strong flow perturbation at NEGIS. Analysis of fold amplitude as a function of stratigraphic level indicates that folding adjacent to NEGIS ceased in the early Holocene, while it is currently <span class="hlt">active</span> inside NEGIS. The presence of folds adjacent of NEGIS, but also at other sites far in the interior of the Greenland <span class="hlt">Ice</span> Sheet with no direct connection to the present-day surface velocity field, indicates that <span class="hlt">ice</span> flow is not only heterogeneous in space (as the present-day flow velocity field shows), but also in time. The observations suggest that <span class="hlt">ice</span> streams are dynamic, ephemeral structures that emerge and die out, and may possibly shift during their existence, but leave traces within the stratigraphic layering of the <span class="hlt">ice</span>. The dynamic nature of <span class="hlt">ice</span> streams such as NEGIS speaks against deterministic models for their accelerated flow rates, such as bedrock topography or thermal perturbations at their base. Instead, we suggest that <span class="hlt">ice</span> streams can also result from strain localisation induced inside the <span class="hlt">ice</span> sheet by the complex coupling of rheology, anisotropy, grain-size changes and possibly shear heating. Bons, P.D., Jansen, D., Mundel, F., Bauer, C.C., Binder, T., Eisen, O., Jessell, M.W., Llorens, M.-G, Steinbach, F., Steinhage, D. & Weikusat, I. 2016. Converging flow and anisotropy cause large-scale folding in Greenland's <span class="hlt">ice</span> sheet. Nature Communications 7</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23197526','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23197526"><span><span class="hlt">Ice</span>-sheet response to oceanic forcing.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Joughin, Ian; Alley, Richard B; Holland, David M</p> <p>2012-11-30</p> <p>The <span class="hlt">ice</span> sheets of Greenland and Antarctica are losing <span class="hlt">ice</span> at accelerating rates, much of which is a response to oceanic forcing, especially of the floating <span class="hlt">ice</span> shelves. Recent observations establish a clear correspondence between the increased delivery of oceanic heat to the <span class="hlt">ice</span>-sheet <span class="hlt">margin</span> and increased <span class="hlt">ice</span> loss. In Antarctica, most of these processes are reasonably well understood but have not been rigorously quantified. In Greenland, an understanding of the processes by which warmer ocean temperatures drive the observed retreat remains elusive. Experiments designed to identify the relevant processes are confounded by the logistical difficulties of instrumenting <span class="hlt">ice</span>-choked fjords with <span class="hlt">actively</span> calving glaciers. For both <span class="hlt">ice</span> sheets, multiple challenges remain before the fully coupled <span class="hlt">ice</span>-ocean-atmosphere models needed for rigorous sea-level projection are available.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUFM.V12B..01G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUFM.V12B..01G"><span><span class="hlt">Ice</span> Thickness, Melting Rates and Styles of <span class="hlt">Activity</span> in <span class="hlt">Ice</span>-Volcano Interaction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gudmundsson, M. T.</p> <p>2005-12-01</p> <p>In most cases when eruptions occur within glaciers they lead to rapid <span class="hlt">ice</span> melting, jokulhlaups and/or lahars. Many parameters influence the style of <span class="hlt">activity</span> and its impact on the environment. These include <span class="hlt">ice</span> thickness (size of glacier), bedrock geometry, magma flow rate and magma composition. The eruptions that have been observed can roughly be divided into: (1) eruptions under several hundred meters thick <span class="hlt">ice</span> on a relatively flat bedrock, (2) eruptions on flat or sloping bed through relatively thin <span class="hlt">ice</span>, and (3) volcanism where effects are limitied to confinement of lava flows or melting of <span class="hlt">ice</span> by pyroclastic flows or surges. This last category (<span class="hlt">ice</span>-contact volcanism) need not cause much <span class="hlt">ice</span> melting. Many of the deposits formed by Pleistocene volcanism in Iceland, British Columbia and Antarctica belong to the first category. An important difference between this type of <span class="hlt">activity</span> and submarine <span class="hlt">activity</span> (where pressure is hydrostatic) is that pressure at vents may in many cases be much lower than glaciostatic due to partial support of <span class="hlt">ice</span> cover over vents by the surrounding glacier. Reduced pressure favours explosive <span class="hlt">activity</span>. Thus the effusive/explosive transition may occur several hundred metres underneath the <span class="hlt">ice</span> surface. Explosive fragmentation of magma leads to much higher rates of heat transfer than does effusive eruption of pillow lavas, and hence much higher melting rates. This effect of reduced pressure at vents will be less pronounced in a large <span class="hlt">ice</span> sheet than in a smaller glacier or <span class="hlt">ice</span> cap, since the hydraulic gradient that drives water away from an eruption site will be lower in the large glacier. This may have implications for form and type of eruption deposits and their relationship with <span class="hlt">ice</span> thickness and glacier size.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19840008344&hterms=sea+world&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dsea%2Bworld','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19840008344&hterms=sea+world&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dsea%2Bworld"><span>Spaceborne SAR and 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>Weeks, W. F.</p> <p>1983-01-01</p> <p>A number of remote sensing systems deployed in satellites to view the Earth which are successful in gathering data on the behavior of the world's snow and <span class="hlt">ice</span> covers are described. Considering sea <span class="hlt">ice</span> which covers over 10% of the world ocean, systems that have proven capable to collect useful data include those operating in the visible, near-infrared, infrared, and microwave frequency ranges. The microwave systems have the essential advantage in observing the <span class="hlt">ice</span> under all weather and lighting conditions. Without this capability data are lost during the long polar night and during times of storm passage, periods when <span class="hlt">ice</span> <span class="hlt">activity</span> can be intense. The <span class="hlt">margins</span> of the <span class="hlt">ice</span> pack, a region of particular interest, is shrouded in cloud between 80 and 90% of the time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C51E..07C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C51E..07C"><span>Investigation of Controls on <span class="hlt">Ice</span> Dynamics in Northeast Greenland from <span class="hlt">Ice</span>-Thickness Change Record Using <span class="hlt">Ice</span> Sheet System Model (ISSM)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Csatho, B. M.; Larour, E. Y.; Schenk, A. F.; Schlegel, N.; Duncan, K.</p> <p>2015-12-01</p> <p>We present a new, complete <span class="hlt">ice</span> thickness change reconstruction of the NE sector of the Greenland <span class="hlt">Ice</span> Sheet for 1978-2014, partitioned into changes due to surface processes and <span class="hlt">ice</span> dynamics. Elevation changes are computed from all available stereoscopic DEMs, and laser altimetry data (ICESat, ATM, LVIS). Surface Mass Balance and firn-compaction estimates are from RACMO2.3. Originating nearly at the divide of the Greenland <span class="hlt">Ice</span> Sheet (GrIS), the dynamically <span class="hlt">active</span> North East <span class="hlt">Ice</span> Stream (NEGIS) is capable of rapidly transmitting <span class="hlt">ice-marginal</span> forcing far inland. Thus, NEGIS provides a possible mechanism for a rapid drawdown of <span class="hlt">ice</span> from the <span class="hlt">ice</span> sheet interior as <span class="hlt">marginal</span> warming, thinning and retreat continues. Our altimetry record shows accelerating dynamic thinning of Zachariæ Isstrom, initially limited to the deepest part of the fjord near the calving front (1978-2000) and then extending at least 75 km inland. At the same time, changes over the Nioghalvfjerdsfjorden (N79) Glacier are negligible. We also detect localized large dynamic changes at higher elevations on the <span class="hlt">ice</span> sheet. These thickness changes, often occurring at the onset of fast flow, could indicate rapid variations of basal lubrication due to rerouting of subglacial drainage. We investigate the possible causes of the observed spatiotemporal pattern of <span class="hlt">ice</span> sheet elevation changes using the <span class="hlt">Ice</span> Sheet System Model (ISSM). This work build on our previous studies examining the sensitivity of <span class="hlt">ice</span> flow within the Northeast Greenland <span class="hlt">Ice</span> Stream (NEGIS) to key fields, including <span class="hlt">ice</span> viscosity, basal drag. We assimilate the new altimetry record into ISSM to improve the reconstruction of basal friction and <span class="hlt">ice</span> viscosity. Finally, airborne geophysical (gravity, magnetic) and <span class="hlt">ice</span>-penetrating radar data is examined to identify the potential geologic controls on the <span class="hlt">ice</span> thickness change pattern. Our study provides the first comprehensive reconstruction of <span class="hlt">ice</span> thickness changes for the entire NEGIS drainage basin during</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMOS11B1649M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMOS11B1649M"><span>Evolution of a Directional Wave Spectrum in a 3D <span class="hlt">Marginal</span> <span class="hlt">Ice</span> Zone with Random 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>Montiel, F.; Squire, V. A.</p> <p>2013-12-01</p> <p>A new ocean wave/sea-<span class="hlt">ice</span> interaction model is proposed that simulates how a directional wave spectrum evolves as it travels through a realistic <span class="hlt">marginal</span> <span class="hlt">ice</span> zone (MIZ), where wave/<span class="hlt">ice</span> dynamics are entirely governed by coherent conservative wave scattering effects. Field experiments conducted by Wadhams et al. (1986) in the Greenland Sea generated important data on wave attenuation in the MIZ and, particularly, on whether the wave spectrum spreads directionally or collimates with distance from the <span class="hlt">ice</span> edge. The data suggest that angular isotropy, arising from multiple scattering by <span class="hlt">ice</span> floes, occurs close to the edge and thenceforth dominates wave propagation throughout the MIZ. Although several attempts have been made to replicate this finding theoretically, including by the use of numerical models, none have confronted this problem in a 3D MIZ with fully randomised floe distribution properties. We construct such a model by subdividing the discontinuous <span class="hlt">ice</span> cover into adjacent infinite slabs of finite width parallel to the <span class="hlt">ice</span> edge. Each slab contains an arbitrary (but finite) number of circular <span class="hlt">ice</span> floes with randomly distributed properties. <span class="hlt">Ice</span> floes are modeled as thin elastic plates with uniform thickness and finite draught. We consider a directional wave spectrum with harmonic time dependence incident on the MIZ from the open ocean, defined as a continuous superposition of plane waves traveling at different angles. The scattering problem within each slab is then solved using Graf's interaction theory for an arbitrary incident directional plane wave spectrum. Using an appropriate integral representation of the Hankel function of the first kind (see Cincotti et al., 1993), we map the outgoing circular wave field from each floe on the slab boundaries into a directional spectrum of plane waves, which characterizes the slab reflected and transmitted fields. Discretizing the angular spectrum, we can obtain a scattering matrix for each slab. Standard recursive</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19870007751&hterms=helicopter+sea&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dhelicopter%2Bsea','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19870007751&hterms=helicopter+sea&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dhelicopter%2Bsea"><span>An inter-sensor comparison of the microwave signatures of Arctic 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>Onstott, R. G.</p> <p>1986-01-01</p> <p><span class="hlt">Active</span> and passive microwave and physical properties of Arctic sea <span class="hlt">ice</span> in the <span class="hlt">marginal</span> <span class="hlt">ice</span> zone were measured during the summer. Results of an intercomparison of data acquired by an aircraft synthetic aperture radar, a passive microwave imager and a helicopter-mounted scatterometer indicate that early-to-mid summer sea <span class="hlt">ice</span> microwave signatures are dominated by snowpack characteristics. Measurements show that the greatest contrast between thin first-year and multiyear sea <span class="hlt">ice</span> occurs when operating <span class="hlt">actively</span> between 5 and 10 GHz. Significant information about the state of melt of snow and <span class="hlt">ice</span> is contained in the <span class="hlt">active</span> and passive microwave signatures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.7868H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.7868H"><span><span class="hlt">Activity</span> of different proteinaceous <span class="hlt">ice</span> nucleating particles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hartmann, Susann; Augustin-Bauditz, Stefanie; Grawe, Sarah; Ling, Meilee; Hellner, Lisa; Zapf, Jean-Michel; Šantl-Temkiv, Tina; Pummer, Bernhard; Boesen, Thomas; Wex, Heike; Finster, Kai; Stratmann, Frank</p> <p>2017-04-01</p> <p>A variety of microorganisms (bacteria, fungi, lichen) from land produce protein structures, which act as a template for <span class="hlt">ice</span> nucleation [1]. Also marine sources of <span class="hlt">ice</span> nucleating particles (INPs) came in focus in the recent years. The atmospheric spatio-temporal distribution of INPs from microorganisms is still not well known. However, it is often assumed that the observed onset of atmospheric <span class="hlt">ice</span> nucleation (T>-20°C) is due to the existence of <span class="hlt">ice</span>-nucleation <span class="hlt">active</span> biological particles. In this study we compare the <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> of different proteinaceous particles produced by bacteria and fungi. For bacteria we investigate (i) cells and fragments of Pseudomonas syringae from commercially available SnomaxTM and (ii) the Pseudomonas syringae INA protein expressed in living Escherichia coli bacteria. We also analyzed freeze-dried leaves [2] where we assume that proteinaceous particles are responsible for the <span class="hlt">ice</span> nucleation <span class="hlt">activity</span>. For fungi the widespread soil fungus Mortierella alpina was investigated which had been extracted from natural soil [3]. Immersion freezing experiments are performed at the cold stage LINA (Leipzig <span class="hlt">Ice</span> Nucleation Array). We attempt to describe the <span class="hlt">activity</span> of a single proteinaceous <span class="hlt">ice</span> nucleating particle [4] in order to achieve direct comparability. Further, the results are compared with complex natural systems e.g. soil dust. The objectives of this study are to clarify potential differences in the <span class="hlt">ice</span> nucleation potential of proteinaceous particles and to draw conclusions concerning the need to differentiate them for modelling purposes. 1. Szyrmer, W. and I. Zawadzki, Biogenic and anthropogenic sources of <span class="hlt">ice</span>-forming nuclei: A review, Bull. Amer. Meteorol. Soc., 1997. 2. Schnell, R.C. and G. Vali, Biogenic <span class="hlt">ice</span> nucleai .1: Terrestrial and marine sources, doi: 10.1175/1520-0469(1976)033<1554:binpit>2.0.co;2, 1976. 3. Froehlich-Nowoisky, J. et al., <span class="hlt">Ice</span> nucleation <span class="hlt">activity</span> in the widespread soil fungus Mortierella alpina, doi: 10</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19840008345&hterms=feeling&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dfeeling','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19840008345&hterms=feeling&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dfeeling"><span>Radar image interpretation techniques applied to sea <span class="hlt">ice</span> geophysical problems</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Carsey, F. D.</p> <p>1983-01-01</p> <p>The geophysical science problems in the sea <span class="hlt">ice</span> area which at present concern understanding the <span class="hlt">ice</span> budget, where <span class="hlt">ice</span> is formed, how thick it grows and where it melts, and the processes which control the interaction of air-sea and <span class="hlt">ice</span> at the <span class="hlt">ice</span> <span class="hlt">margins</span> is discussed. The science problems relate to basic questions of sea <span class="hlt">ice</span>: how much is there, thickness, drift rate, production rate, determination of the morphology of the <span class="hlt">ice</span> <span class="hlt">margin</span>, storms feeling for the <span class="hlt">ice</span>, storms and influence at the <span class="hlt">margin</span> to alter the pack, and ocean response to a storm at the <span class="hlt">margin</span>. Some of these questions are descriptive and some require complex modeling of interactions between the <span class="hlt">ice</span>, the ocean, the atmosphere and the radiation fields. All involve measurements of the character of the <span class="hlt">ice</span> pack, and SAR plays a significant role in the measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900047002&hterms=water&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DTitle%26N%3D0%26No%3D80%26Ntt%3Dwater','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900047002&hterms=water&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DTitle%26N%3D0%26No%3D80%26Ntt%3Dwater"><span>Airborne discrimination between <span class="hlt">ice</span> and water - Application to the laser measurement of chlorophyll-in-water in a <span class="hlt">marginal</span> <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>Hoge, Frank E.; Wright, C. Wayne; Swift, Robert N.; Yungel, James K.</p> <p>1989-01-01</p> <p>The concurrent <span class="hlt">active</span>-passive measurement capabilities of the NASA Airborne Oceanographic Lidar have been used to (1) discriminate between <span class="hlt">ice</span> and water in a large <span class="hlt">ice</span> field within the Greenland Sea and (2) achieve the detection and measurement of chlorophyll-in-water by laser-induced and water-Raman-normalized pigment fluorescence. Passive upwelled radiances from sea <span class="hlt">ice</span> are significantly stronger than those from the neighboring water, even when the optical receiver field-of-view is only partially filled with <span class="hlt">ice</span>. Thus, weaker passive upwelled radiances, together with concurrently acquired laser-induced spectra, can rather confidently be assigned to the intervening water column. The laser-induced spectrum can then be processed using previously established methods to measure the chlorophyll-in-water concentration. Significant phytoplankton patchiness and elevated chlorophyll concentrations were found within the waters of the melting <span class="hlt">ice</span> compared to <span class="hlt">ice</span>-free regions just outside the <span class="hlt">ice</span> field.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70012038','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70012038"><span>Sea <span class="hlt">ice</span> melting in the <span class="hlt">marginal</span> <span class="hlt">ice</span> zone.</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Josberger, E.G.</p> <p>1983-01-01</p> <p>The heat and salt flux boundary conditions together with the freezing curve relationship are a necessary component of any <span class="hlt">ice</span>- sea water thermodynamic model. A neutral two-layer oceanic planetary boundary layer model that incorporates these boundary conditions is used. The results are discussed. -from Author</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1035130','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1035130"><span>Air-Sea Interactions in the <span class="hlt">Marginal</span> <span class="hlt">Ice</span> Zone</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2016-03-31</p> <p>Arctic Ocean has increased with the significant retreat of the seasonal sea-<span class="hlt">ice</span> extent. Here, we use wind, wave, turbulence, and <span class="hlt">ice</span> measurements to...which has experienced a significant retreat of the seasonal <span class="hlt">ice</span> extent (Comiso and Nishio, 2008; Comiso et al., 2008). Thomson and Rogers (2014) showed</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018QSRv..179...24P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018QSRv..179...24P"><span>Large-scale glacitectonic deformation in response to <span class="hlt">active</span> <span class="hlt">ice</span> sheet retreat across Dogger Bank (southern central North Sea) during the Last Glacial Maximum</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Phillips, Emrys; Cotterill, Carol; Johnson, Kirstin; Crombie, Kirstin; James, Leo; Carr, Simon; Ruiter, Astrid</p> <p>2018-01-01</p> <p>High resolution seismic data from the Dogger Bank in the central southern North Sea has revealed that the Dogger Bank Formation records a complex history of sedimentation and penecontemporaneous, large-scale, <span class="hlt">ice-marginal</span> to proglacial glacitectonic deformation. These processes led to the development of a large thrust-block moraine complex which is buried beneath a thin sequence of Holocene sediments. This buried glacitectonic landsystem comprises a series of elongate, arcuate moraine ridges (200 m up to > 15 km across; over 40-50 km long) separated by low-lying <span class="hlt">ice</span> <span class="hlt">marginal</span> to proglacial sedimentary basins and/or meltwater channels, preserving the shape of the <span class="hlt">margin</span> of this former <span class="hlt">ice</span> sheet. The moraines are composed of highly deformed (folded and thrust) Dogger Bank Formation with the lower boundary of the deformed sequence (up to 40-50 m thick) being marked by a laterally extensive décollement. The <span class="hlt">ice</span>-distal parts of the thrust moraine complex are interpreted as a "forward" propagating imbricate thrust stack developed in response to S/SE-directed <span class="hlt">ice</span>-push. The more complex folding and thrusting within the more <span class="hlt">ice</span>-proximal parts of the thrust-block moraines record the accretion of thrust slices of highly deformed sediment as the <span class="hlt">ice</span> repeatedly reoccupied this <span class="hlt">ice</span> <span class="hlt">marginal</span> position. Consequently, the internal structure of the Dogger Bank thrust-moraine complexes can be directly related to <span class="hlt">ice</span> sheet dynamics, recording the former positions of a highly dynamic, oscillating Weichselian <span class="hlt">ice</span> sheet <span class="hlt">margin</span> as it retreated northwards at the end of the Last Glacial Maximum.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C53C0741N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C53C0741N"><span>The Acoustic Signature of Glaciated <span class="hlt">Margins</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Newton, A. M. W.; Huuse, M.</p> <p>2016-12-01</p> <p>As climate warms it has become increasingly clear that, in order to fully understand how it might evolve in the future, we need to look for examples of how climate has changed in the past. The Late Cenozoic history of the Arctic Ocean and its surrounding seas has been dominated by glacial-interglacials cycles. This has resulted in major environmental changes in relative sea levels, <span class="hlt">ice</span> volumes, sea <span class="hlt">ice</span> conditions, and ocean circulation as marine and terrestrially-based <span class="hlt">ice</span> sheets waxed and waned. In this work, the acoustic signatures of several glaciated <span class="hlt">margins</span> in the Northern Hemisphere are investigated and compared. This includes: NW Greenland, West Greenland, East Greenland, mid-Norway, Northern Norway, and the North Sea. These shelf successions preserve a geomorphological record of multiple glaciations and are imaged using seismic reflection data. To date, the majority of work in these areas has tended to focus on the most recent glaciations, which are well known. Here, the focus of the work is to look at the overall stratigraphic setting and how it influences (and is influenced by) the evolution of <span class="hlt">ice</span> sheets throughout the glacial succession. Landform records are imaged using seismic data to provide a long-term insight into the styles of glaciation on each <span class="hlt">margin</span> and what relation this may have had on climate, whilst the stratigraphic architectures across each site demonstrate how the inherited geology and tectonic setting can provide a fundamental control on the <span class="hlt">ice</span> sheet and depositional styles. For example, Scoresby Sund is characterised by significant aggradation that is likely related to subsidence induced by lithospheric cooling rather than rapid glacial deposition, whilst the subsidence of the mid-Norwegian <span class="hlt">margin</span> can be related to rapid glacial deposition and trapping of sediments behind inversion structures such as the Helland-Hansen Arch. The insights from this multi-<span class="hlt">margin</span> study allow for regional, basin-wide, glaciological records to be developed</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/2014AGUFM.C53A0283P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.C53A0283P"><span>Emergent Dead Vegetation and Paired Cosmogenic Isotope Constraints on <span class="hlt">Ice</span> Cap <span class="hlt">Activity</span>, Baffin Island, Arctic Canada</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pendleton, S.; Miller, G. H.</p> <p>2014-12-01</p> <p>Recent summer warming has now raised the equilibrium line above almost all <span class="hlt">ice</span> caps on Baffin Island, resulting in surface lowering and <span class="hlt">marginal</span> recession everywhere. As cold-based <span class="hlt">ice</span> recedes it frequently exposes in situ tundra plants that were living at the time <span class="hlt">ice</span> expanded across the site. Radiocarbon dates for each plant records when cold summers dropped regional snowline below the site, killing the plants, and snowline remained below the site until the collection date. The kill dates also represent the last time that the climate was warm enough to expose the sampling location. Seventy-six vegetation samples collected in 2013 from the Penny <span class="hlt">Ice</span> Cap region have been dated, with significant age populations at ~0.5, 1.8, 2.3, and 3.6 ka. The absence of ages around ~1, 2, 3, 4.5, and 5.5 ka suggest periods of either no snowline depression or stability. Sixteen vegetation samples returned ages of >45 ka (2 revisited sites from 2010, 14 new). It is postulated that these radiocarbon dead samples were last exposed during the last interglaciation (~120 ka), the last time climate was as warm as present. In addition to plant collections, bedrock exposures at the <span class="hlt">ice</span> <span class="hlt">margins</span> were sampled for 26Al/10Be cosmogenic nuclide dating. Seven samples from and around the Penny <span class="hlt">Ice</span> cap have returned maximum exposure ages from ~ 0.6-0.9 ma and total histories of ~0.6-1.5 ma. In general, samples from the larger Penny <span class="hlt">Ice</span> Cap exhibited lower amounts of exposure (~20% of total history) than those samples from smaller, localized <span class="hlt">ice</span> caps (~55%). Radiocarbon dead sites north of the Penny <span class="hlt">Ice</span> cap experienced significantly more exposure over their lifetimes than their counterparts east of the Penny <span class="hlt">Ice</span> cap, suggesting significant differences in local and regional land <span class="hlt">ice</span> fluctuations over the last 2 million years. Utilizing both the method of in situ moss and 26Al/10Be dating provides new insight into both the recent <span class="hlt">activity</span> and long-term evolution of <span class="hlt">ice</span> on Baffin Island. In particular</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1013719','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1013719"><span><span class="hlt">Marginal</span> <span class="hlt">Ice</span> Zone: Biogeochemical Sampling with Gliders</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2015-09-30</p> <p>chlorophyll primary productivity model to estimate and compare phytoplankton productivity under full <span class="hlt">ice</span> cover, in the MIZ, and in open <span class="hlt">ice</span>-free water...observing array (Fig. 1). The glider sensor suite included temperature, temperature microstructure, salinity, oxygen, chlorophyll fluorescence, optical...operating in continental shelf waters off Alaska’s north slope allowed us to construct proxy libraries for converting chlorophyll fluorescence to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA145351','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA145351"><span>MIZEX. A Program for Mesoscale Air-<span class="hlt">Ice</span>-Ocean Interaction Experiments in Arctic <span class="hlt">Marginal</span> <span class="hlt">Ice</span> Zones. III. Modeling the <span class="hlt">Marginal</span> <span class="hlt">Ice</span> Zone,</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1984-04-01</p> <p>Ii TS C]r.I2 TAB 0] Unzanro’ unoed 0 justi fica ~r: 0 April 1984 vs - ASValabilitY Codes lvyall and/or U.S. Army Cold Regions Research and Engineering...coupled model. Fig. 1. Annual average simulated velocity fields. 3 192 Aloka 190 / 902 190+ WOO S’,. o <span class="hlt">Ice</span> OnlY Mod" D"’, 55*w F~tth Yea’ <span class="hlt">Ice</span> Ocean Model...A more precise delinga- inflow boundary conditions. 12 4- a. [ o ll ii traspert 00 0 0- 0e a I " i i , - - I I 1161 63 15 67 69 Ti 73 75 77 1980 *= 4h</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4438723','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4438723"><span>Shallow methylmercury production in the <span class="hlt">marginal</span> sea <span class="hlt">ice</span> zone of the central Arctic Ocean</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Heimbürger, Lars-Eric; Sonke, Jeroen E.; Cossa, Daniel; Point, David; Lagane, Christelle; Laffont, Laure; Galfond, Benjamin T.; Nicolaus, Marcel; Rabe, Benjamin; van der Loeff, Michiel Rutgers</p> <p>2015-01-01</p> <p>Methylmercury (MeHg) is a neurotoxic compound that threatens wildlife and human health across the Arctic region. Though much is known about the source and dynamics of its inorganic mercury (Hg) precursor, the exact origin of the high MeHg concentrations in Arctic biota remains uncertain. Arctic coastal sediments, coastal marine waters and surface snow are known sites for MeHg production. Observations on marine Hg dynamics, however, have been restricted to the Canadian Archipelago and the Beaufort Sea (<79°N). Here we present the first central Arctic Ocean (79–90°N) profiles for total mercury (tHg) and MeHg. We find elevated tHg and MeHg concentrations in the <span class="hlt">marginal</span> sea <span class="hlt">ice</span> zone (81–85°N). Similar to other open ocean basins, Arctic MeHg concentration maxima also occur in the pycnocline waters, but at much shallower depths (150–200 m). The shallow MeHg maxima just below the productive surface layer possibly result in enhanced biological uptake at the base of the Arctic marine food web and may explain the elevated MeHg concentrations in Arctic biota. We suggest that Arctic warming, through thinning sea <span class="hlt">ice</span>, extension of the seasonal sea <span class="hlt">ice</span> zone, intensified surface ocean stratification and shifts in plankton ecodynamics, will likely lead to higher marine MeHg production. PMID:25993348</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25993348','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25993348"><span>Shallow methylmercury production in the <span class="hlt">marginal</span> sea <span class="hlt">ice</span> zone of the central Arctic Ocean.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Heimbürger, Lars-Eric; Sonke, Jeroen E; Cossa, Daniel; Point, David; Lagane, Christelle; Laffont, Laure; Galfond, Benjamin T; Nicolaus, Marcel; Rabe, Benjamin; van der Loeff, Michiel Rutgers</p> <p>2015-05-20</p> <p>Methylmercury (MeHg) is a neurotoxic compound that threatens wildlife and human health across the Arctic region. Though much is known about the source and dynamics of its inorganic mercury (Hg) precursor, the exact origin of the high MeHg concentrations in Arctic biota remains uncertain. Arctic coastal sediments, coastal marine waters and surface snow are known sites for MeHg production. Observations on marine Hg dynamics, however, have been restricted to the Canadian Archipelago and the Beaufort Sea (<79 °N). Here we present the first central Arctic Ocean (79-90 °N) profiles for total mercury (tHg) and MeHg. We find elevated tHg and MeHg concentrations in the <span class="hlt">marginal</span> sea <span class="hlt">ice</span> zone (81-85 °N). Similar to other open ocean basins, Arctic MeHg concentration maxima also occur in the pycnocline waters, but at much shallower depths (150-200 m). The shallow MeHg maxima just below the productive surface layer possibly result in enhanced biological uptake at the base of the Arctic marine food web and may explain the elevated MeHg concentrations in Arctic biota. We suggest that Arctic warming, through thinning sea <span class="hlt">ice</span>, extension of the seasonal sea <span class="hlt">ice</span> zone, intensified surface ocean stratification and shifts in plankton ecodynamics, will likely lead to higher marine MeHg production.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013ACP....13.4223M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013ACP....13.4223M"><span>Urediospores of rust fungi are <span class="hlt">ice</span> nucleation <span class="hlt">active</span> at > -10 °C and harbor <span class="hlt">ice</span> nucleation <span class="hlt">active</span> bacteria</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Morris, C. E.; Sands, D. C.; Glaux, C.; Samsatly, J.; Asaad, S.; Moukahel, A. R.; Gonçalves, F. L. T.; Bigg, E. K.</p> <p>2013-04-01</p> <p>Various features of the biology of the rust fungi and of the epidemiology of the plant diseases they cause illustrate the important role of rainfall in their life history. Based on this insight we have characterized the <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> (INA) of the aerially disseminated spores (urediospores) of this group of fungi. Urediospores of this obligate plant parasite were collected from natural infections of 7 species of weeds in France, from coffee in Brazil and from field and greenhouse-grown wheat in France, the USA, Turkey and Syria. Immersion freezing was used to determine freezing onset temperatures and the abundance of <span class="hlt">ice</span> nuclei in suspensions of washed spores. Microbiological analyses of spores from France, the USA and Brazil, and subsequent tests of the <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> of the bacteria associated with spores were deployed to quantify the contribution of bacteria to the <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> of the spores. All samples of spores were <span class="hlt">ice</span> nucleation <span class="hlt">active</span>, having freezing onset temperatures as high as -4 °C. Spores in most of the samples carried cells of <span class="hlt">ice</span> nucleation-<span class="hlt">active</span> strains of the bacterium Pseudomonas syringae (at rates of less than 1 bacterial cell per 100 urediospores), but bacterial INA accounted for only a small fraction of the INA observed in spore suspensions. Changes in the INA of spore suspensions after treatment with lysozyme suggest that the INA of urediospores involves a polysaccharide. Based on data from the literature, we have estimated the concentrations of urediospores in air at cloud height and in rainfall. These quantities are very similar to those reported for other biological <span class="hlt">ice</span> nucleators in these same substrates. However, at cloud level convective <span class="hlt">activity</span> leads to widely varying concentrations of particles of surface origin, so that mean concentrations can underestimate their possible effects on clouds. We propose that spatial and temporal concentrations of biological <span class="hlt">ice</span> nucleators <span class="hlt">active</span> at temperatures > -10 </p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70018690','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70018690"><span>Satellite imagery of the onset of streaming flow of <span class="hlt">ice</span> streams C and D, West 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>Hodge, S.M.; Doppelhammer, S.K.</p> <p>1996-01-01</p> <p>Five overlapping Landsat multispectral scanner satellite images of the interior of the West Antarctic <span class="hlt">ice</span> sheet were enhanced with principal component analysis, high-pass filtering, and linear contrast stretching and merged into a mosaic by aligning surface features in the overlap areas. The mosaic was registered to geodetic coordinates, to an accuracy of about 1 km, using the five scene centers as control points. The onset of streaming flow of two tributaries of <span class="hlt">ice</span> stream C and one tributary of <span class="hlt">ice</span> stream D is visible in the mosaic. The onset appears to occur within a relatively short distance, less than the width of the <span class="hlt">ice</span> stream, typically at a subglacial topographic feature such as a step or ridge. The <span class="hlt">ice</span> streams extend farther up into the interior than previously mapped. <span class="hlt">Ice</span> stream D starts about 150 km from the <span class="hlt">ice</span> divide, at an altitude of about 1500 m, approximately halfway up the convex-upward dome shape of the interior <span class="hlt">ice</span> sheet. <span class="hlt">Ice</span> stream D is relatively much longer than <span class="hlt">ice</span> stream C, possibly because <span class="hlt">ice</span> stream D is currently <span class="hlt">active</span> whereas <span class="hlt">ice</span> stream C is currently inactive. The grounded portion of the West Antarctic <span class="hlt">ice</span> sheet is perhaps best conceptualized as an <span class="hlt">ice</span> sheet in which <span class="hlt">ice</span> streams are embedded over most of its area, with slow moving <span class="hlt">ice</span> converging into fast moving <span class="hlt">ice</span> streams in a widely distributed pattern, much like that of streams and rivers in a hydrologic basin. A relic <span class="hlt">margin</span> appears to parallel most of the south <span class="hlt">margin</span> of the tributary of <span class="hlt">ice</span> stream D, separated from the <span class="hlt">active</span> shear <span class="hlt">margin</span> by about 10 km or less for a distance of over 200 km. This means there is now evidence for recent changes having occurred in three of the five major <span class="hlt">ice</span> streams which drain most of West Antarctica (B, C, and D), two of which (B and D) are currently <span class="hlt">active</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA617625','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA617625"><span><span class="hlt">Marginal</span> <span class="hlt">Ice</span> Zone: Biogeochemical Sampling with Gliders</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2014-09-30</p> <p>chlorophyll primary productivity model to estimate and compare phytoplankton productivity under full <span class="hlt">ice</span> cover, in the MIZ, and in open <span class="hlt">ice</span>-free water...September, the gliders and still operating but will be retrieved in early October from the R/V Norseman. All gliders carried sensors for chlorophyll ...program, with modification for local conditions. The specific protocols for each sensor – backscatter and chlorophyll fluorescence – are described in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ACP....17.1595M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ACP....17.1595M"><span>Pre-<span class="hlt">activation</span> of aerosol particles by <span class="hlt">ice</span> preserved in pores</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marcolli, Claudia</p> <p>2017-02-01</p> <p>Pre-<span class="hlt">activation</span> denotes the capability of particles or materials to nucleate <span class="hlt">ice</span> at lower relative humidities or higher temperatures compared to their intrinsic <span class="hlt">ice</span> nucleation efficiency after having experienced an <span class="hlt">ice</span> nucleation event or low temperature before. This review presumes that <span class="hlt">ice</span> preserved in pores is responsible for pre-<span class="hlt">activation</span> and analyses pre-<span class="hlt">activation</span> under this presumption. Idealized trajectories of air parcels are used to discuss the pore characteristics needed for <span class="hlt">ice</span> to persist in pores and to induce macroscopic <span class="hlt">ice</span> growth out of the pores. The pore width needed to keep pores filled with water decreases with decreasing relative humidity as described by the inverse Kelvin equation. Thus, narrow pores remain filled with <span class="hlt">ice</span> well below <span class="hlt">ice</span> saturation. However, the smaller the pore width, the larger the melting and freezing point depressions within the pores. Therefore, pre-<span class="hlt">activation</span> due to pore <span class="hlt">ice</span> is constrained by the melting of <span class="hlt">ice</span> in narrow pores and the sublimation of <span class="hlt">ice</span> from wide pores imposing restrictions on the temperature and relative humidity range of pre-<span class="hlt">activation</span> for cylindrical pores. <span class="hlt">Ice</span> is better protected in ink-bottle-shaped pores with a narrow opening leading to a large cavity. However, whether pre-<span class="hlt">activation</span> is efficient also depends on the capability of <span class="hlt">ice</span> to grow macroscopically, i.e. out of the pore. A strong effect of pre-<span class="hlt">activation</span> is expected for swelling pores, because at low relative humidity (RH) their openings narrow and protect the <span class="hlt">ice</span> within them against sublimation. At high relative humidities, they open up and the <span class="hlt">ice</span> can grow to macroscopic size and form an <span class="hlt">ice</span> crystal. Similarly, <span class="hlt">ice</span> protected in pockets is perfectly sheltered against sublimation but needs the dissolution of the surrounding matrix to be effective. Pores partially filled with condensable material may also show pre-<span class="hlt">activation</span>. In this case, complete filling occurs at lower RH than for empty pores and freezing shifts to lower temperatures.Pre-<span class="hlt">activation</span></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><span class="hlt">Active</span> volcanism beneath the West Antarctic <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 Antarctic <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 <span class="hlt">active</span> 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 <span class="hlt">active</span> portion of the West Antarctic 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('https://pubs.er.usgs.gov/publication/70030660','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70030660"><span>Glacial Lake Musselshell: Late Wisconsin slackwater on the Laurentide <span class="hlt">ice</span> <span class="hlt">margin</span> in central Montana, USA</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Davis, N.K.; Locke, W. W.; Pierce, K.L.; Finkel, R.C.</p> <p>2006-01-01</p> <p>Cosmogenic surface exposure ages of glacial boulders deposited in <span class="hlt">ice-marginal</span> Lake Musselshell suggest that the lake existed between 20 and 11.5 ka during the Late Wisconsin glacial stage (MIS 2), rather than during the Late Illinoian stage (MIS 6) as traditionally thought. The altitude of the highest <span class="hlt">ice</span>-rafted boulders and the lowest passes on the modern divide indicate that glacial lake water in the Musselshell River basin reached at least 920-930 m above sea level and generally remained below 940 m. Exposures of rhythmically bedded silt and fine sand indicate that Lake Musselshell is best described as a slackwater system, in which the <span class="hlt">ice</span>-dammed Missouri and Musselshell Rivers rose and fell progressively throughout the existence of the lake rather than establishing a lake surface with a stable elevation. The absence of varves, deltas and shorelines also implies an unstable lake. The changing volume of the lake implies that the Laurentide <span class="hlt">ice</span> sheet was not stable at its southernmost position in central Montana. A continuous sequence of alternating slackwater lake sediment and lacustrine sheetflood deposits indicates that at least three advances of the Laurentide <span class="hlt">ice</span> sheet occurred in central Montana between 20 and 11.5 ka. Between each advance, it appears that Lake Musselshell drained to the north and formed two outlet channels that are now occupied by extremely underfit streams. A third outlet formed when the water in Lake Musselshell fully breached the Larb Hills, resulting in the final drainage of the lake. The channel through the Larb Hills is now occupied by the Missouri River, implying that the present Missouri River channel east of the Musselshell River confluence was not created until the Late Wisconsin, possibly as late as 11.5 ka. ?? 2005 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRD..122.4924W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRD..122.4924W"><span>Heterogeneous <span class="hlt">ice</span> nucleation of α-pinene SOA particles before and after <span class="hlt">ice</span> cloud processing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wagner, Robert; Höhler, Kristina; Huang, Wei; Kiselev, Alexei; Möhler, Ottmar; Mohr, Claudia; Pajunoja, Aki; Saathoff, Harald; Schiebel, Thea; Shen, Xiaoli; Virtanen, Annele</p> <p>2017-05-01</p> <p>The <span class="hlt">ice</span> nucleation ability of α-pinene secondary organic aerosol (SOA) particles was investigated at temperatures between 253 and 205 K in the Aerosol Interaction and Dynamics in the Atmosphere cloud simulation chamber. Pristine SOA particles were nucleated and grown from pure gas precursors and then subjected to repeated expansion cooling cycles to compare their intrinsic <span class="hlt">ice</span> nucleation ability during the first nucleation event with that observed after <span class="hlt">ice</span> cloud processing. The unprocessed α-pinene SOA particles were found to be inefficient <span class="hlt">ice</span>-nucleating particles at cirrus temperatures, with nucleation onsets (for an <span class="hlt">activated</span> fraction of 0.1%) as high as for the homogeneous freezing of aqueous solution droplets. <span class="hlt">Ice</span> cloud processing at temperatures below 235 K only <span class="hlt">marginally</span> improved the particles' <span class="hlt">ice</span> nucleation ability and did not significantly alter their morphology. In contrast, the particles' morphology and <span class="hlt">ice</span> nucleation ability was substantially modified upon <span class="hlt">ice</span> cloud processing in a simulated convective cloud system, where the α-pinene SOA particles were first <span class="hlt">activated</span> to supercooled cloud droplets and then froze homogeneously at about 235 K. As evidenced by electron microscopy, the α-pinene SOA particles adopted a highly porous morphology during such a freeze-drying cycle. When probing the freeze-dried particles in succeeding expansion cooling runs in the mixed-phase cloud regime up to 253 K, the increase in relative humidity led to a collapse of the porous structure. Heterogeneous <span class="hlt">ice</span> formation was observed after the droplet <span class="hlt">activation</span> of the collapsed, freeze-dried SOA particles, presumably caused by <span class="hlt">ice</span> remnants in the highly viscous material or the larger surface area of the particles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C11E..01W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C11E..01W"><span>Rapid Collapse of the Vavilov <span class="hlt">Ice</span> Cap, Russian High Arctic.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Willis, M. J.; Zheng, W.; Durkin, W. J., IV; Pritchard, M. E.; Ramage, J. M.; Dowdeswell, J. A.; Benham, T. J.; Glazovsky, A.; Macheret, Y.; Porter, C. C.</p> <p>2016-12-01</p> <p>Cold based <span class="hlt">ice</span> caps and glaciers are thought to respond slowly to environmental changes. As sea <span class="hlt">ice</span> cover evolves in the Arctic, a feedback process alters air-temperatures and precipitation patterns across the region. During the last decades of the 20th century the land-terminating western <span class="hlt">margin</span> of the Vavilov <span class="hlt">Ice</span> Cap, on October Revolution Island of the Severnaya Zemlya Archipelago, advanced slowly westwards. The advance was driven by precipitation changes that occurred about half a millennia ago. InSAR shows that in 1996 the <span class="hlt">margin</span> sustained <span class="hlt">ice</span> speeds of around 20 m/yr. By 2000 the <span class="hlt">ice</span> front had moved a short distance into the Kara Sea and had transitioned to a marine-terminating front, although an <span class="hlt">ice</span> apron around the <span class="hlt">ice</span> <span class="hlt">margin</span> indicates the <span class="hlt">ice</span> there was still frozen to the bed and there is no evidence of calving in satellite imagery. In 2013 <span class="hlt">ice</span> motions near the terminus had accelerated to around 1 m/day. By late 2015 the main trunk of the newly <span class="hlt">activated</span> outlet glacier attained speeds of 25 m/day and the inland portion of the <span class="hlt">ice</span> cap thinned at rates of more than 0.3 m/day. The acceleration of the outlet glacier occurred due to its advance over weak, water-saturated marine sediments that provide little resistance to <span class="hlt">ice</span> flow, and to the removal of lateral resistive stresses as the glacier advanced out into an open embayment. Longitudinal stretching at the front forces an increase in the surface slope upstream. Rapid rates of motion inland generate frictional melt at the bed, possibly aided by cryohydrological warming. Large areas of the interior of the Vavilov <span class="hlt">ice</span> cap are now below the equilibrium line and the grounded portion of the <span class="hlt">ice</span> cap is losing mass at a rate of 4.5 km3 w.e./year. The changes at the Vavilov are likely irrecoverable in a warming climate due to a reduction in the accumulation area of the <span class="hlt">ice</span> cap. Increased precipitation drove the advance, which accelerated due to the presence of soft sediments. The acceleration lowered the elevation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004GPC....42..279S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004GPC....42..279S"><span>Glacier <span class="hlt">ice</span> mass fluctuations and fault instability in tectonically <span class="hlt">active</span> Southern Alaska</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sauber, Jeanne M.; Molnia, Bruce F.</p> <p>2004-07-01</p> <p> change during the 1899-1979 time period to calculate the change in the fault stability <span class="hlt">margin</span> (FSM) prior to the 1979 St. Elias earthquake. Our results suggest that a cumulative decrease in the fault stability <span class="hlt">margin</span> at seismogenic depths, due to <span class="hlt">ice</span> wastage over 80 years, was large, up to ˜2 MPa. <span class="hlt">Ice</span> wastage would promote thrust faulting in events such as the 1979 earthquake and subsequent aftershocks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70026696','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70026696"><span>Glacier <span class="hlt">ice</span> mass fluctuations and fault instability in tectonically <span class="hlt">active</span> Southern 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>Sauber, J.M.; Molnia, B.F.</p> <p>2004-01-01</p> <p> change during the 1899-1979 time period to calculate the change in the fault stability <span class="hlt">margin</span> (FSM) prior to the 1979 St. Elias earthquake. Our results suggest that a cumulative decrease in the fault stability <span class="hlt">margin</span> at seismogenic depths, due to <span class="hlt">ice</span> wastage over 80 years, was large, up to ???2 MPa. <span class="hlt">Ice</span> wastage would promote thrust faulting in events such as the 1979 earthquake and subsequent aftershocks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70020753','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70020753"><span>Laurentide glacial landscapes: the role of <span class="hlt">ice</span> streams</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Patterson, C.J.</p> <p>1998-01-01</p> <p>Glacial landforms of the North American prairie can be divided into two suites that result from different styles of <span class="hlt">ice</span> flow: 1) a lowland suite of level-to-streamlined till consistent with formation beneath <span class="hlt">ice</span> streams, and 2) an upland and lobe-<span class="hlt">margin</span> suite of thick, hummocky till and glacial thrust blocks consistent with formation at <span class="hlt">ice</span>-stream and <span class="hlt">ice</span>-lobe <span class="hlt">margins</span>. Southern Laurentide <span class="hlt">ice</span> lobes hypothetically functioned as outlets of <span class="hlt">ice</span> streams. Broad branching lowlands bounded by escarpments mark the stable positions of the <span class="hlt">ice</span> streams that fed the lobes. If the lobes and <span class="hlt">ice</span> streams were similar to modern <span class="hlt">ice</span> streams, their fast flow was facilitated by high subglacial water pressure. Favorable geology and topography in the midcontinent encouraged nonuniform <span class="hlt">ice</span> flow and controlled the location of <span class="hlt">ice</span> streams and outlet lobes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.C43C0565R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.C43C0565R"><span>Deglaciation of the Western <span class="hlt">Margin</span> of the Barents Sea <span class="hlt">Ice</span> Sheet - a Swath Bathymetric and Sub-Bottom Seismic Study from Eglacom Nice-Streams Data in the Kveithola Trough</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rebesco, M.; Liu, Y.; Camerlenghi, A.; Winsborrow, M. C.; Laberg, J.; Caburlotto, A.; Diviacco, P.; Accettella, D.; Sauli, C.; Wardell, N.</p> <p>2010-12-01</p> <p>IPY <span class="hlt">Activity</span> N. 367 focusing on Neogene <span class="hlt">ice</span> streams and sedimentary processes on high- latitude continental <span class="hlt">margins</span> (NICE-STREAMS) resulted in two coordinated cruises on the adjacent Storfjorden and Kveithola trough-mouth fans in the NW Barents Sea: SVAIS Cruise of BIO Hespérides, summer 2007, and EGLACOM Cruise of Cruise R/V OGS-Explora, summer 2008. The objectives were to acquire a high-resolution set of bathymetric, seismic and sediment core data in order to decipher the Neogene architectural development of the glacially-dominated NW Barents Sea continental <span class="hlt">margin</span> in response to natural climate change. The paleo-<span class="hlt">ice</span> streams drained <span class="hlt">ice</span> from southern Spitsbergen, Spitsbergen Bank, and Bear Island. The short distance from the <span class="hlt">ice</span> source to the calving front produced a short residence time of <span class="hlt">ice</span>, and therefore a rapid response to climatic changes. We describe here the EGLACOM data collected within the Kveithola Trough, an E-W trending glacial trough in the NW Barents Sea, NW of the Bear Island. Swath bathymetry shows that the seafloor is characterised by E-W trending mega-scale glacial lineations (MSGL) that record a fast flowing <span class="hlt">ice</span> stream draining the Svalbard/Barents Sea <span class="hlt">Ice</span> Sheet (SBIS) during the Last Glacial Maximum (LGM). MSGL are overprinted by transverse sediment ridges about 15 km apart which give rise to a staircase axial profile of the trough. Such transverse ridges are interpreted as grounding-zone wedges (GZW) formed by deposition of unconsolidated, saturated subglacial till during episodic <span class="hlt">ice</span> stream retreat. Sub-bottom (CHIRP) and multi-channel reflection seismic data show that present-day morphology is largely inherited from the palaeo-seafloor topography at the time of deposition of the transverse ridges, overlain by a draping glaciomarine unit up to over 15 m thick. Our data allow the reconstruction of depositional processes that accompanied the deglaciation of the Spitsbergen Bank area. The sedimentary drape deposited on top of the GZWs which</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1984LPSC...14..409L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1984LPSC...14..409L"><span><span class="hlt">Ice</span> and debris in the fretted terrain, Mars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lucchitta, B. K.</p> <p>1984-02-01</p> <p>Viking moderate and high resolution images along the northern highland <span class="hlt">margin</span> have been monoscopically and stereoscopically examined in order to study the development of fretted terrain. Young debris aprons around mesas and debris in tributary channels create typical fretted morphologies identical to ancient fretted morphologies. This suggests that the debris-apron process operating relatively recently also shaped the fretted terrain of the past. The debris aprons were lubricated by interstitial <span class="hlt">ice</span> derived from ground <span class="hlt">ice</span>. Abundant collapse features suggest that ground <span class="hlt">ice</span> existed and may have flowed in places. The fretting process has been <span class="hlt">active</span> for a long period and may be <span class="hlt">active</span> today. The location of debris aprons in two latitudinal belts may be controlled by atmospheric conditions that permit <span class="hlt">ice</span> in the region to remain in the ground below depths of about one meter and temperatures warm enough for <span class="hlt">ice</span> to flow.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA601293','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA601293"><span>Coupling of Waves, Turbulence and Thermodynamics Across the <span class="hlt">Marginal</span> <span class="hlt">Ice</span> Zone</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><span class="hlt">ice</span> . The albedo of sea <span class="hlt">ice</span> is large compared to open water, and most of the incoming solar radiation...ocean and the <span class="hlt">ice</span> pack where the seasonal retreat of the main <span class="hlt">ice</span> pack takes place. It is a highly variable sea <span class="hlt">ice</span> environment, usually comprised of...many individual floes of variable shape and size and made of mixed <span class="hlt">ice</span> types, from young forming <span class="hlt">ice</span> to fragmented multiyear <span class="hlt">ice</span> . The presence of sea</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA259765','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA259765"><span><span class="hlt">Active</span> and Passive Remote Sensing of <span class="hlt">Ice</span></span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1993-01-26</p> <p>92 4. TITLE AND SUBTITLE S. FUNDING NUMBERS <span class="hlt">Active</span> and Passive Remote Sensing of <span class="hlt">Ice</span> NO0014-89-J-l 107 6. AUTHOR(S) 425f023-08 Prof. J.A. Kong 7... REMOTE SENSING OF <span class="hlt">ICE</span> Sponsored by: Department of the Navy Office of Naval Research Contract number: N00014-89-J-1107 Research Organization: Center for...J. A. Kong Period covered: October 1, 1988 - November 30, 1992 St <span class="hlt">ACTIVE</span> AND PASSIVE REMOTE SENSING OF <span class="hlt">ICE</span> FINAL REPORT This annual report covers</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.B33A2075C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.B33A2075C"><span>Multi-proxy Organic Geochemical Reconstruction of Holocene Hydroclimate Near the Western Greenland <span class="hlt">Ice</span> Sheet <span class="hlt">Margin</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cluett, A.; Thomas, E. K.</p> <p>2017-12-01</p> <p>Anthropogenic warming is projected to drive profound change to the Arctic hydrological cycle within the century, most notably in the intensification of rainfall, with potential feedbacks to the climate system and cryosphere. However, the relationship between hydroclimate and cryosphere variability is poorly constrained in the long-term due to a scarcity of high-resolution hydroclimate records from the Arctic. We analyze the stable hydrogen isotopes (dD) of leaf wax biomarkers from lacustrine sediments spanning the Holocene to 9000 cal. year B.P. from Lake Gus (67.032ºN, 52.427ºW, 300 m a.s.l.; informal name), a small lake approximately 90 km from the modern western <span class="hlt">margin</span> of the Greenland <span class="hlt">Ice</span> Sheet. We interpret the signal of aquatic leaf wax isotopes in the context of a survey of 100 modern lake water samples from western Greenland across an aridity gradient to better understand the combined climatological and hydrological controls on lake water dD in the study area. We compare variability of aquatic and terrestrial leaf wax isotopes to infer changes in relative moisture throughout the Holocene, and complement our leaf wax record with analysis of glycerol dialkyl glycerol tetraethers (GDGTs) and alkenones, to produce records of summer temperature. Pairing temperature and leaf wax isotope records provides a means to constrain the changing dD-temperature relationship throughout the Holocene and infer moisture source variability. In combination, these proxies produce a comprehensive hydroclimate record at approximately centennial scale to evaluate shifts in relative moisture, temperature, and moisture source, and to investigate the interaction between hydroclimate and Greenland <span class="hlt">Ice</span> Sheet <span class="hlt">margin</span> fluctuations through the Holocene.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21898102','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21898102"><span>Environmental controls on microbial abundance and <span class="hlt">activity</span> on the greenland <span class="hlt">ice</span> sheet: a multivariate analysis approach.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Stibal, Marek; Telling, Jon; Cook, Joe; Mak, Ka Man; Hodson, Andy; Anesio, Alexandre M</p> <p>2012-01-01</p> <p>Microbes in supraglacial ecosystems have been proposed to be significant contributors to regional and possibly global carbon cycling, and quantifying the biogeochemical cycling of carbon in glacial ecosystems is of great significance for global carbon flow estimations. Here we present data on microbial abundance and productivity, collected along a transect across the ablation zone of the Greenland <span class="hlt">ice</span> sheet (GrIS) in summer 2010. We analyse the relationships between the physical, chemical and biological variables using multivariate statistical analysis. Concentrations of debris-bound nutrients increased with distance from the <span class="hlt">ice</span> sheet <span class="hlt">margin</span>, as did both cell numbers and <span class="hlt">activity</span> rates before reaching a peak (photosynthesis) or a plateau (respiration, abundance) between 10 and 20 km from the <span class="hlt">margin</span>. The results of productivity measurements suggest an overall net autotrophy on the GrIS and support the proposed role of <span class="hlt">ice</span> sheet ecosystems in carbon cycling as regional sinks of CO(2) and places of production of organic matter that can be a potential source of nutrients for downstream ecosystems. Principal component analysis based on chemical and biological data revealed three clusters of sites, corresponding to three 'glacier ecological zones', confirmed by a redundancy analysis (RDA) using physical data as predictors. RDA using data from the largest 'bare <span class="hlt">ice</span> zone' showed that glacier surface slope, a proxy for melt water flow, accounted for most of the variation in the data. Variation in the chemical data was fully explainable by the determined physical variables. Abundance of phototrophic microbes and their proportion in the community were identified as significant controls of the carbon cycling-related microbial processes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=physical+AND+activity+AND+importance&pg=2&id=EJ914304','ERIC'); return false;" href="https://eric.ed.gov/?q=physical+AND+activity+AND+importance&pg=2&id=EJ914304"><span>Got <span class="hlt">Ice</span>? Teaching <span class="hlt">Ice</span>-Skating as a Lifelong <span class="hlt">Activity</span></span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Tarkinton, Brenda C.; Karp, Grace Goc</p> <p>2010-01-01</p> <p>With today's focus on the importance of lifelong physical <span class="hlt">activity</span>, educators are increasingly offering a variety of such <span class="hlt">activities</span> in their classes, as well as in before- and after-school programs. This article describes the benefits of offering <span class="hlt">ice</span> skating as a challenging and rewarding lifetime <span class="hlt">activity</span>, either before or after school or in…</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> cover 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> cover 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> cover inferred from the winter data is approximately 25 to 40% less than the summer <span class="hlt">ice</span> cover 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> cover. 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 Antarctic, some multiyear <span class="hlt">ice</span> floes in the Arctic, especially those near the summer <span class="hlt">marginal</span> <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 <span class="hlt">marginal</span> <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> cover. 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> cover.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010cosp...38.1763V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010cosp...38.1763V"><span>The Little <span class="hlt">Ice</span> Age and Solar <span class="hlt">Activity</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Velasco Herrera, Victor Manuel; Leal Silva, C. M. Carmen; Velasco Herrera, Graciela</p> <p></p> <p>We analyze the <span class="hlt">ice</span> winter severity index on the Baltic region since 1501-1995. We found that the variability of this index is modulated among other factors by the secular solar <span class="hlt">activity</span>. The little <span class="hlt">ice</span> ages that have appeared in the North Hemisphere occurred during periods of low solar <span class="hlt">activity</span>. Seemingly our star is experiencing a new quiet stage compared with Maunder or Dalton minimum, this is important because it is estimated that even small changes in weather can represent a great impact in <span class="hlt">ice</span> index. These results are relevant since <span class="hlt">ice</span> is a very important element in the climate system of the Baltic region and it can affect directly or indirectly many of the oceanographic, climatic, eco-logical, economical and cultural patterns.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.C33A0662C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.C33A0662C"><span>Holocene history of North <span class="hlt">Ice</span> Cap, northwestern Greenland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Corbett, L. B.; Kelly, M. A.; Osterberg, E. C.; Axford, Y.; Bigl, M.; Roy, E. P.; Thompson, J. T.</p> <p>2013-12-01</p> <p>Although much research has focused on the past extents of the Greenland <span class="hlt">Ice</span> Sheet, less is known about the smaller <span class="hlt">ice</span> caps on Greenland and how they have evolved over time. These small <span class="hlt">ice</span> caps respond sensitively to summer temperatures and, to a lesser extent, winter precipitation, and provide valuable information about climatic conditions along the Greenland <span class="hlt">Ice</span> Sheet <span class="hlt">margins</span>. Here, we investigate the Holocene history of North <span class="hlt">Ice</span> Cap (76°55'N 68°00'W), located in the Nunatarssuaq region near Thule, northwest Greenland. Our results are based on glacial geomorphic mapping, 10Be dating, and analyses of sediment cores from a glacially fed lake. Fresh, unweathered and unvegetated boulders comprise moraines and drift that mark an extent of North <span class="hlt">Ice</span> Cap ~25 m outboard of the present <span class="hlt">ice</span> <span class="hlt">margin</span>. It is likely that these deposits were formed during late Holocene time and we are currently employing 10Be surface exposure dating to examine this hypothesis. Just outboard of the fresh moraines and drift, boulders and bedrock show significant weathering and are covered with lichen. Based on glacial geomorphic mapping and detailed site investigations, including stone counts, we suggest that the weathered boulders and bedrock were once covered by erosive Greenland <span class="hlt">Ice</span> Sheet flow from southeast to northwest over the Nunatarssuaq region. Five 10Be ages from the more weathered landscape only 100-200 m outboard of the modern North <span class="hlt">Ice</span> Cap <span class="hlt">margin</span> are 52 and 53 ka (bedrock) and 16, 23, and 31 ka (boulders). These ages indicate that recent <span class="hlt">ice</span> cover has likely been cold-based and non-erosive, failing to remove inherited cosmogenic nuclides from previous periods of exposure, although the youngest boulder may provide a maximum limiting deglaciation age. Sediment cores collected from Delta Sø, a glacially-fed lake ~1.5 km outside of the modern North <span class="hlt">Ice</span> Cap <span class="hlt">margin</span>, contain 130 cm of finely laminated sediments overlying coarse sands and glacial till. Radiocarbon ages from just above</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMOS11B1656S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMOS11B1656S"><span>Quantifying the Floe Size Distribution in the <span class="hlt">Marginal</span> <span class="hlt">Ice</span> Zone from Satellite Imagery for use in Model Development and Validation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schweiger, A. J.; Stern, H. L.; Stark, M.; Zhang, J.; Hwang, P.; Steele, M.</p> <p>2013-12-01</p> <p>Several key processes in the <span class="hlt">Marginal</span> <span class="hlt">Ice</span> Zone (MIZ) of the Arctic Ocean are related to the size of the <span class="hlt">ice</span> floes, whose diameters range from meters to tens of kilometers. The floe size distribution (FSD) influences mechanical properties of the <span class="hlt">ice</span> and thus its response to winds, currents, and waves, which is likely to modify the air-sea momentum transfer. The FSD also influences the air-sea heat transfer and the response of the MIZ <span class="hlt">ice</span> cover to the thermal forcing. The FSD also has a significant role in lateral melting. No existing sea-<span class="hlt">ice</span>/ocean models currently simulate the FSD in the MIZ. Significant uncertainties in FSD-related processes hinder model incorporation of the FSD, and model development must heavily depend on observations of the FSD for parameterization, calibration, and validation. To support the development and implementation of the FSD in the <span class="hlt">Marginal</span> <span class="hlt">Ice</span> Zone Modeling and Assimilation System (MIZMAS), we have conducted an analysis of the FSD in the Beaufort and Chukchi seas using three sources of satellite imagery: NASA's Moderate Resolution Imaging Spectroradiometer (MODIS) on the Terra and Aqua satellites, the Canadian Space Agency's synthetic aperture radar (SAR) on RADARSAT, and declassified National Technical Means imagery from the Global Fiducials Library (GFL) of the U.S. Geological Survey. The MODIS visible and short-wave infrared bands have a pixel size of 250 meters, and are only useful in cloud-free regions. The SAR imagery is unaffected by clouds and darkness, and has a pixel size of 50 meters. The GFL visible imagery, with a pixel size of 1 meter, is only useful in cloud-free regions. The resolution and spatial extent of the various image products allows us to identify <span class="hlt">ice</span> floes of all sizes from 10 meters to 100 kilometers. The general procedure for identifying <span class="hlt">ice</span> floes in the imagery is as follows: delineate cloud-free regions (if necessary); choose a threshold to separate <span class="hlt">ice</span> from water, and create a binary image; apply the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018QSRv..186..186N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018QSRv..186..186N"><span>Geomorphology and till architecture of terrestrial palaeo-<span class="hlt">ice</span> streams of the southwest Laurentide <span class="hlt">Ice</span> Sheet: A borehole stratigraphic approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Norris, Sophie L.; Evans, David J. A.; Cofaigh, Colm Ó.</p> <p>2018-04-01</p> <p>A multidimensional study, utilising geomorphological mapping and the analysis of regional borehole stratigraphy, is employed to elucidate the regional till architecture of terrestrial palaeo-<span class="hlt">ice</span> streams relating to the Late Wisconsinan southwest Laurentide <span class="hlt">Ice</span> Sheet. Detailed mapping over a 57,400 km2 area of southwestern Saskatchewan confirms previous reconstructions of a former southerly flowing <span class="hlt">ice</span> stream, demarcated by a 800 km long corridor of megaflutes and mega-scale glacial lineations (<span class="hlt">Ice</span> Stream 1) and cross cut by three, formerly southeast flowing <span class="hlt">ice</span> streams (<span class="hlt">Ice</span> Streams 2A, B and C). Analysis of the lithologic and geophysical characteristics of 197 borehole samples within these corridors reveals 17 stratigraphic units comprising multiple tills and associated stratified sediments overlying preglacial deposits, the till thicknesses varying with both topography and distance down corridor. Reconciling this regional till architecture with the surficial geomorphology reveals that surficial units are spatially consistent with a dynamic switch in flow direction, recorded by the cross cutting corridors of <span class="hlt">Ice</span> Streams 1, 2A, B and C. The general thickening of tills towards lobate <span class="hlt">ice</span> stream <span class="hlt">margins</span> is consistent with subglacial deformation theory and variations in this pattern on a more localised scale are attributed to influences of subglacial topography including thickening at buried valley <span class="hlt">margins</span>, thinning over uplands and thickening in overridden <span class="hlt">ice-marginal</span> landforms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.H23E1429C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.H23E1429C"><span>Continuous monitoring of deep groundwater at the <span class="hlt">ice</span> <span class="hlt">margin</span>, Kangerlussuaq, 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>Claesson Liljedahl, L.; Lehtinen, A. M.; Ruskeeniemi, T.; Engström, J.; Hansson, K.; Sundberg, J.; Henkemans, E.; Frape, S.; Johansson, S.; Acuna, J.</p> <p>2012-12-01</p> <p>The deep geologic repository (DGR) concept for the long-term management of used nuclear fuel involves the containment and isolation of used nuclear fuel at depths of approximately 500-1000 m below ground surface within a suitable geological formation for hundreds of thousands of years. A key objective of the used fuel DGR research programs of the Swedish, Finnish and Canadian nuclear waste management organizations (SKB, POSIVA and NWMO, respectively) is to further understanding of geosphere stability and long-term evolution. Future glaciation represents an intense external perturbation of a DGR situated in northern latitudes. To advance the understanding of processes associated with glaciation and their impact on the long-term performance of a DGR, the Greenland Analogue Project (GAP) was initiated by SKB, POSIVA and NWMO. The GAP was initiated in 2008 as a four-year field and modelling study utilizing the Greenland <span class="hlt">ice</span> sheet and sub-surface conditions in West Greenland as an analogue for the conditions expected to prevail in Fennoscandia and Canada during future glacial cycles. One of the main aims of the GAP is to improve the understanding of how groundwater flow and water chemistry is influenced by an existing <span class="hlt">ice</span> sheet and continuous permafrost. One way to study this is by monitoring deep drillholes. A 645 m deep drillhole (DH-GAP04) was drilled and instrumented in July 2011 at the <span class="hlt">ice</span>-sheet <span class="hlt">margin</span> in Kangerlussuaq, West Greenland to investigate the hydrogeochemical and hydrogeological conditions of a subglacial environment. Of particular interest is the recharge of glacial meltwater, and understanding to what depth it intrudes into the bedrock and whether it affects the chemistry and physico-chemical properties of the deep groundwater. DH-GAP04 is instrumented with a two-packer multi-sensor system, installed at a depth of 560 m, dividing the hole into three sections. The upper section extends from the base of permafrost (about 350 m) down to the upper packer</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFMPP31A1300S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFMPP31A1300S"><span>Little <span class="hlt">Ice</span> Age Fluctuations of Quelccaya <span class="hlt">Ice</span> Cap, Peru</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stroup, J. S.; Kelly, M. A.; Lowell, T.</p> <p>2009-12-01</p> <p>A record of the past extents of Quelccaya <span class="hlt">Ice</span> Cap (QIC) provides valuable information about tropical climate change from late glacial to recent time. Here, we examine the timing and regional significance of fluctuations of QIC during the Little <span class="hlt">Ice</span> Age (LIA; ~1300-1850 AD). One prominent set of moraines, known as the Huancane I moraines, is located ~1 km from the present-day western <span class="hlt">ice</span> cap <span class="hlt">margin</span> and provides a near-continuous outline of the most recent advance of QIC. This moraine set was radiocarbon dated (~298 ± 134 and 831 ± 87 yr BP) by Mercer and Palacios (1977) and presented as some of the first evidence for cooling in the tropics during the Little <span class="hlt">Ice</span> Age. Recent field investigations in the QIC region focused on refining the chronology of the Huancane I moraines. In 2008, new stratigraphic sections exposed by local lake-flooding events revealed multiple layers of peat within the Huancane I moraines. In both 2008 and 2009, samples were obtained for 10Be dating of boulders on Huancane I moraines. A combination of radiocarbon and 10Be ages indicate that the Huancane I moraines were deposited by <span class="hlt">ice</span> cap expansion after ~3800 yr BP and likely by multiple advances at approximately 1000, 600, 400, and 200 yr BP. Radiocarbon and 10Be chronologies of the Huancane I moraines are compared with the Quelccaya <span class="hlt">ice</span> core records (Thompson et al., 1985; 1986; 2006). Accumulation data from the <span class="hlt">ice</span> core records are interpreted to indicate a significant wet period at ~1500-1700 AD followed by a significant drought at ~1720-1860 AD. We examine <span class="hlt">ice</span> <span class="hlt">marginal</span> fluctuations during these times to determine influence of such events on the <span class="hlt">ice</span> cap extent.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010JGRB..115.1102D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010JGRB..115.1102D"><span>Tectonomagmatic <span class="hlt">activity</span> and <span class="hlt">ice</span> dynamics in the Bransfield Strait back-arc basin, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dziak, Robert P.; Park, Minkyu; Lee, Won Sang; Matsumoto, Haru; Bohnenstiehl, Delwayne R.; Haxel, Joseph H.</p> <p>2010-01-01</p> <p>An array of moored hydrophones was used to monitor the spatiotemporal distribution of small- to moderate-sized earthquakes and <span class="hlt">ice</span>-generated sounds within the Bransfield Strait, Antarctica. During a 2 year period, a total of 3900 earthquakes, 5925 icequakes and numerous <span class="hlt">ice</span> tremor events were located throughout the region. The seismic <span class="hlt">activity</span> included eight space-time earthquake clusters, positioned along the central neovolcanic rift zone of the young Bransfield back-arc basin. These sequences of small magnitude earthquakes, or swarms, suggest ongoing magmatic <span class="hlt">activity</span> that becomes localized along isolated volcanic features and fissure-like ridges in the southwest portion of the basin. A total of 122 earthquakes were located along the South Shetland trench, indicating continued deformation and possibly ongoing subduction along this <span class="hlt">margin</span>. The large number of icequakes observed show a temporal pattern related to seasonal freeze-thaw cycles and a spatial distribution consistent with channeling of sea <span class="hlt">ice</span> along submarine canyons from glacier fronts. Several harmonic tremor episodes were sourced from a large (˜30 km2) iceberg that entered northeast portion of the basin. The spectral character of these signals suggests they were produced by either resonance of a small chamber of fluid within the iceberg, or more likely, due to periodicity of discrete stick-slip events caused by contact of the moving iceberg with the seafloor. These pressure waves appear to have been excited by abrasion of the iceberg along the seafloor as it passed Clarence and Elephant Islands.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28035668','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28035668"><span><span class="hlt">Ice</span> and anti-nucleating <span class="hlt">activities</span> of an <span class="hlt">ice</span>-binding protein from the annual grass, Brachypodium distachyon.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bredow, Melissa; Tomalty, Heather E; Smith, Lindsay; Walker, Virginia K</p> <p>2018-05-01</p> <p>Plants exposed to sub-zero temperatures face unique challenges that threaten their survival. The growth of <span class="hlt">ice</span> crystals in the extracellular space can cause cellular dehydration, plasma membrane rupture and eventual cell death. Additionally, some pathogenic bacteria cause tissue damage by initiating <span class="hlt">ice</span> crystal growth at high sub-zero temperatures through the use of <span class="hlt">ice</span>-nucleating proteins (INPs), presumably to access nutrients from lysed cells. An annual species of brome grass, Brachypodium distachyon (Bd), produces an <span class="hlt">ice</span>-binding protein (IBP) that shapes <span class="hlt">ice</span> with a modest depression of the freezing point (~0.1 °C at 1 mg/mL), but high <span class="hlt">ice</span>-recrystallization inhibition (IRI) <span class="hlt">activity</span>, allowing <span class="hlt">ice</span> crystals to remain small at near melting temperatures. This IBP, known as BdIRI, is unlike other characterized IBPs with a single <span class="hlt">ice</span>-binding face, as mutational analysis indicates that BdIRI adsorbs to <span class="hlt">ice</span> on two faces. BdIRI also dramatically attenuates the nucleation of <span class="hlt">ice</span> by bacterial INPs (up to -2.26 °C). This 'anti-nucleating' <span class="hlt">activity</span> is significantly higher than previously documented for any IBP. © 2016 John Wiley & Sons Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1816263P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1816263P"><span>Soot Aerosol Particles as Cloud Condensation Nuclei: from <span class="hlt">Ice</span> Nucleation <span class="hlt">Activity</span> to <span class="hlt">Ice</span> Crystal Morphology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pirim, Claire; Ikhenazene, Raouf; Ortega, Isamel Kenneth; Carpentier, Yvain; Focsa, Cristian; Chazallon, Bertrand; Ouf, François-Xavier</p> <p>2016-04-01</p> <p>Emissions of solid-state particles (soot) from engine exhausts due to incomplete fuel combustion is considered to influence <span class="hlt">ice</span> and liquid water cloud droplet <span class="hlt">activation</span> [1]. The <span class="hlt">activity</span> of these aerosols would originate from their ability to be important centers of <span class="hlt">ice</span>-particle nucleation, as they would promote <span class="hlt">ice</span> formation above water homogeneous freezing point. Soot particles are reported to be generally worse <span class="hlt">ice</span> nuclei than mineral dust because they <span class="hlt">activate</span> nucleation at higher <span class="hlt">ice</span>-supersaturations for deposition nucleation and at lower temperatures for immersion freezing than ratios usually expected for homogeneous nucleation [2]. In fact, there are still numerous opened questions as to whether and how soot's physico-chemical properties (structure, morphology and chemical composition) can influence their nucleation ability. Therefore, systematic investigations of soot aerosol nucleation <span class="hlt">activity</span> via one specific nucleation mode, here deposition nucleation, combined with thorough structural and compositional analyzes are needed in order to establish any association between the particles' <span class="hlt">activity</span> and their physico-chemical properties. In addition, since the morphology of the <span class="hlt">ice</span> crystals can influence their radiative properties [3], we investigated their morphology as they grow over both soot and pristine substrates at different temperatures and humidity ratios. In the present work, Combustion Aerosol STandart soot samples were produced from propane using various experimental conditions. Their nucleation <span class="hlt">activity</span> was studied in deposition mode (from water vapor), and monitored using a temperature-controlled reactor in which the sample's relative humidity is precisely measured with a cryo-hygrometer. Formation of water/<span class="hlt">ice</span> onto the particles is followed both optically and spectroscopically, using a microscope coupled to a Raman spectrometer. Vibrational signatures of hydroxyls (O-H) emerge when the particle becomes hydrated and are used to characterize <span class="hlt">ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GML....36...81C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GML....36...81C"><span>Glaciomarine sedimentation and bottom current <span class="hlt">activity</span> on the north-western and northern continental <span class="hlt">margins</span> of Svalbard during the late Quaternary</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chauhan, Teena; Noormets, Riko; Rasmussen, Tine L.</p> <p>2016-04-01</p> <p>Palaeo-bottom current strength of the West Spitsbergen Current (WSC) and the influence of the Svalbard-Barents Sea <span class="hlt">Ice</span> Sheet (SBIS) on the depositional environment along the northern Svalbard <span class="hlt">margins</span> are poorly known. Two gravity cores from the southern Yermak Plateau and the upper slope north of Nordaustlandet, covering marine isotope stage (MIS) 1 to MIS 5, are investigated. Five lithofacies, based on grain size distribution, silt/clay ratio, content and mean of sortable silt (SS), are distinguished to characterise the contourite-dominated sedimentary environments. In addition, depositional environments are described using total organic carbon (TOC), total sulphur (TS) and calcium carbonate (CaCO3) contents of sediments. Facies A, containing coarse SS, suggests strong bottom current <span class="hlt">activity</span> and good bottom water ventilation conditions as inferred from low TOC content. This facies was deposited during the glacial periods MIS 4, MIS 2 and during the late Holocene. Facies B is dominated by fine SS indicating weak bottom current and poor ventilation (cf. high TOC content of 1.2-1.6%), and correlates with the MIS 4/3 and MIS 2/1 transition periods. With an equal amount of clay and sand, fine SS and high content of TOC, facies C indicates reduced bottom current strength for intervals with sediment supply from proximal sources such as icebergs, sea <span class="hlt">ice</span> or meltwater discharge. This facies was deposited during the last glacial maximum. Facies D represents mass-flow deposits on the northern Svalbard <span class="hlt">margin</span> attributed to the SBIS advance at or near the shelf edge. Facies E sediments indicating moderate bottom current strength were deposited during MIS 5 and MIS 3, and during parts of MIS 2. This first late Quaternary proxy record of the WSC flow and sedimentation history from the northern Svalbard <span class="hlt">margin</span> suggests that the oceanographic conditions and <span class="hlt">ice</span> sheet processes have exerted first-order control on sediment properties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA138558','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA138558"><span>Investigation of <span class="hlt">Ice</span> Dynamics in the <span class="hlt">Marginal</span> Zone.</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1983-12-01</p> <p>Unclassified SECURITV CLASSIFICATIGON OF THIS PAGE (111mon Dole Rntormi) Unclassified MTY CLASMSFICATION OF THIS PA6SS16M POW & 6m " trength rather...modeling work, two points are recognized to need a deep consideration: transient cases and stochastic modeling. It is not certain how the velocity...if the thickness effect is indeed significant. The nature of the <span class="hlt">ice</span> edge jet should be shown: is it transient or steady, forced or caused by <span class="hlt">ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70028746','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70028746"><span>Hydrography and circulation of <span class="hlt">ice-marginal</span> lakes at Bering Glacier, 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>Josberger, E.G.; Shuchman, R.A.; Meadows, G.A.; Savage, S.; Payne, J.</p> <p>2006-01-01</p> <p>An extensive suite of physical oceanographic, remotely sensed, and water quality measurements, collected from 2001 through 2004 in two <span class="hlt">ice-marginal</span> lakes at Bering Glacier, Alaska-Berg Lake and Vitus Lake-show that each has a unique circulation controlled by their specific physical forcing within the glacial system. Conductivity profiles from Berg Lake, perched 135 m a.s.l., show no salt in the lake, but the temperature profiles indicate an apparently unstable situation, the 4??C density maximum is located at 10 m depth, not at the bottom of the lake (90 m depth). Subglacial discharge from the Steller Glacier into the bottom of the lake must inject a suspended sediment load sufficient to <span class="hlt">marginally</span> stabilize the water column throughout the lake. In Vitus Lake, terminus positions derived from satellite imagery show that the glacier terminus rapidly retreated from 1995 to the present resulting in a substantial expansion of the volume of Vitus Lake. Conductivity and temperature profiles from the tidally influenced Vitus Lake show a complex four-layer system with diluted (???50%) seawater in the bottom of the lake. This lake has a complex vertical structure that is the result of convection generated by <span class="hlt">ice</span> melting in salt water, stratification within the lake, and freshwater entering the lake from beneath the glacier and surface runoff. Four consecutive years, from 2001 to 2004, of these observations in Vitus Lake show little change in the deep temperature and salinity conditions, indicating limited deep water renewal. The combination of the lake level measurements with discharge measurements, through a tidal cycle, by an acoustic Doppler Current Profiler (ADCP) deployed in the Seal River, which drains the entire Bering system, showed a strong tidal influence but no seawater entry into Vitus Lake. The ADCP measurements combined with lake level measurements established a relationship between lake level and discharge, which when integrated over a tidal cycle, gives a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28626650','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28626650"><span>Recrystallization inhibition in <span class="hlt">ice</span> due to <span class="hlt">ice</span> binding protein <span class="hlt">activity</span> detected by nuclear magnetic resonance.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Brown, Jennifer R; Seymour, Joseph D; Brox, Timothy I; Skidmore, Mark L; Wang, Chen; Christner, Brent C; Luo, Bing-Hao; Codd, Sarah L</p> <p>2014-09-01</p> <p>Liquid water present in polycrystalline <span class="hlt">ice</span> at the interstices between <span class="hlt">ice</span> crystals results in a network of liquid-filled veins and nodes within a solid <span class="hlt">ice</span> matrix, making <span class="hlt">ice</span> a low porosity porous media. Here we used nuclear magnetic resonance (NMR) relaxation and time dependent self-diffusion measurements developed for porous media applications to monitor three dimensional changes to the vein network in <span class="hlt">ices</span> with and without a bacterial <span class="hlt">ice</span> binding protein (IBP). Shorter effective diffusion distances were detected as a function of increased irreversible <span class="hlt">ice</span> binding <span class="hlt">activity</span>, indicating inhibition of <span class="hlt">ice</span> recrystallization and persistent small crystal structure. The modification of <span class="hlt">ice</span> structure by the IBP demonstrates a potential mechanism for the microorganism to enhance survivability in <span class="hlt">ice</span>. These results highlight the potential of NMR techniques in evaluation of the impact of IBPs on vein network structure and recrystallization processes; information useful for continued development of <span class="hlt">ice</span>-interacting proteins for biotechnology applications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998QSRv...17..243D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998QSRv...17..243D"><span>Glacimarine Sedimentary Processes and Facies on the Polar North Atlantic <span class="hlt">Margins</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dowdeswell, J. A.; Elverhfi, A.; Spielhagen, R.</p> <p></p> <p>Major contrasts in the glaciological, oceanic and atmospheric parameters affecting the Polar North Atlantic, both over space between its eastern and western <span class="hlt">margins</span>, and through time from full glacial to interglacial conditions, have lead to the deposition of a wide variety of sedimentary facies in these <span class="hlt">ice</span>-influenced seas. The dynamics of the glaciers and <span class="hlt">ice</span> sheets on the hinterlands surrounding the Polar North Atlantic have exterted a major influence on the processes, rates and patterns of sedimentation on the continental <span class="hlt">margins</span> of the Norwegian and Greenland seas over the Late Cenozoic. The western <span class="hlt">margin</span> is influenced by the cold East Greenland Current and the Svalbard <span class="hlt">margin</span> by the northernmost extent of the warm North Atlantic Drift and the passage of relatively warm cyclonic air masses. In the fjords of Spitsbergen and the northwestern Barents Sea, glacial meltwater is dominant in delivering sediments. In the fjords of East Greenland the large numbers of icebergs produced from fast-flowing outlets of the Greenland <span class="hlt">Ice</span> Sheet play a more significant role in sedimentation. During full glacials, sediments are delivered to the shelf break from fast-flowing <span class="hlt">ice</span> streams, which drain huge basins within the parent <span class="hlt">ice</span> sheet. Large prograding fans located on the continental slope offshore of these <span class="hlt">ice</span> streams are made up of stacked debris flows. Large-scale mass failures, turbidity currents, and gas-escape structures also rework debris in continental slope and shelf settings. Even during interglacials, both the <span class="hlt">margins</span> and the deep ocean basins beyond them retain a glacimarine overprint derived from debris in far-travelled icebergs and sea <span class="hlt">ice</span>. Under full glacial conditions, the glacier influence is correspondingly stronger, and this is reflected in the glacial and glacimarine facies deposited at these times.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.C33A0663K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.C33A0663K"><span>Evidence for smaller extents of the northwestern Greenland <span class="hlt">Ice</span> Sheet and North <span class="hlt">Ice</span> Cap 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>Kelly, M. A.; Osterberg, E. C.; Axford, Y.; Bigl, M.; Birkel, S. D.; Corbett, L. B.; Roy, E. P.; Thompson, J. T.; Whitecloud, S.</p> <p>2013-12-01</p> <p>The Greenland <span class="hlt">Ice</span> Sheet (GrIS) and local glaciers on Greenland are responding dynamically to warming temperatures with widespread retreat. GRACE satellite data (e.g., Kahn et al., 2010) and the Petermann Glacier calving events document the recent expansion of <span class="hlt">ice</span> loss into northwestern Greenland. To improve the ability to estimate future <span class="hlt">ice</span> loss in a warming climate, we are developing records of the response of the northwestern Greenlandic cryosphere to Holocene climatic conditions, with a focus on past warm periods. Our ongoing research includes analyses of glacial geology, sub-fossil vegetation, lake sediment cores, chironomid assemblages and <span class="hlt">ice</span> cores combined with glaciological modeling. To constrain past <span class="hlt">ice</span> extents that were as small as, or smaller than, at present, we recovered sub-fossil vegetation exposed at the receding <span class="hlt">margins</span> of the GrIS and North <span class="hlt">Ice</span> Cap (NIC) in the Nunatarssuaq region (~76.7°N, 67.4°W) and of the GrIS near Thule (~76.5°N, 68.7°W). We present vegetation types and radiocarbon ages of 30 plant samples collected in August 2012. In the Nunatarssuaq region, five ages of in situ (rooted) vegetation including Polytrichum moss, Saxifraga nathorstii and grasses located <5 m outboard of the GrIS <span class="hlt">margin</span> are ~120-200 cal yr BP (range of medians of the 2-sigma calibrated age ranges). Nine ages of in situ Polytrichum, Saxifraga oppositafolia and grasses from ~1-5 m inboard of the NIC <span class="hlt">margin</span> (excavated from beneath <span class="hlt">ice</span>) range from ~50 to 310 cal yr BP. The growth of these plants occurred when the GrIS and NIC were at least as small as at present and their ages suggest that <span class="hlt">ice</span> advances occurred in the last 50-120 yrs. In addition to the in situ samples, we collected plants from well-preserved ground material exposed along shear planes in the GrIS <span class="hlt">margins</span>. In Nunatarssuaq, two Polytrichum mosses rooted in ground material and exposed along a shear plane in the GrIS <span class="hlt">margin</span> date to 4680 and 4730 cal yr BP. Near Thule, three ages of Salix arctica</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013ACP....13.5751H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013ACP....13.5751H"><span>Immersion freezing of <span class="hlt">ice</span> nucleation <span class="hlt">active</span> protein complexes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hartmann, S.; Augustin, S.; Clauss, T.; Wex, H.; Šantl-Temkiv, T.; Voigtländer, J.; Niedermeier, D.; Stratmann, F.</p> <p>2013-06-01</p> <p>Utilising the Leipzig Aerosol Cloud Interaction Simulator (LACIS), the immersion freezing behaviour of droplet ensembles containing monodisperse particles, generated from a Snomax™ solution/suspension, was investigated. Thereto <span class="hlt">ice</span> fractions were measured in the temperature range between -5 °C to -38 °C. Snomax™ is an industrial product applied for artificial snow production and contains Pseudomonas syringae} bacteria which have long been used as model organism for atmospheric relevant <span class="hlt">ice</span> nucleation <span class="hlt">active</span> (INA) bacteria. The <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> of such bacteria is controlled by INA protein complexes in their outer membrane. In our experiments, <span class="hlt">ice</span> fractions increased steeply in the temperature range from about -6 °C to about -10 °C and then levelled off at <span class="hlt">ice</span> fractions smaller than one. The plateau implies that not all examined droplets contained an INA protein complex. Assuming the INA protein complexes to be Poisson distributed over the investigated droplet populations, we developed the CHESS model (stoCHastic modEl of similar and poiSSon distributed <span class="hlt">ice</span> nuclei) which allows for the calculation of <span class="hlt">ice</span> fractions as function of temperature and time for a given nucleation rate. Matching calculated and measured <span class="hlt">ice</span> fractions, we determined and parameterised the nucleation rate of INA protein complexes exhibiting class III <span class="hlt">ice</span> nucleation behaviour. Utilising the CHESS model, together with the determined nucleation rate, we compared predictions from the model to experimental data from the literature and found good agreement. We found that (a) the heterogeneous <span class="hlt">ice</span> nucleation rate expression quantifying the <span class="hlt">ice</span> nucleation behaviour of the INA protein complex is capable of describing the <span class="hlt">ice</span> nucleation behaviour observed in various experiments for both, Snomax™ and P. syringae bacteria, (b) the <span class="hlt">ice</span> nucleation rate, and its temperature dependence, seem to be very similar regardless of whether the INA protein complexes inducing <span class="hlt">ice</span> nucleation are attached</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/29921005','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29921005"><span>Microbial life under <span class="hlt">ice</span>: Metagenome diversity and in situ <span class="hlt">activity</span> of Verrucomicrobia in seasonally <span class="hlt">ice</span>-covered lakes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tran, Patricia; Ramachandran, Arthi; Khawasek, Ola; Beisner, Beatrix E; Rautio, Milla; Huot, Yannick; Walsh, David A</p> <p>2018-06-19</p> <p>Northern lakes are <span class="hlt">ice</span>-covered for a large part of the year, yet our understanding of microbial diversity and <span class="hlt">activity</span> during winter lags behind that of the <span class="hlt">ice</span>-free period. In this study, we investigated under-<span class="hlt">ice</span> diversity and metabolism of Verrucomicrobia in seasonally <span class="hlt">ice</span>-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 <span class="hlt">ice</span>-covered periods. A diversity of Verrucomicrobia genomes were reconstructed from Quebec lake metagenomes. Several genomes were associated with the <span class="hlt">ice</span>-covered period and were represented in winter metatranscriptomes, supporting the notion that Verrucomicrobia are metabolically <span class="hlt">active</span> under <span class="hlt">ice</span>. Verrucomicrobia transcriptome analysis revealed a range of metabolisms potentially occurring under <span class="hlt">ice</span>, 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 <span class="hlt">actively</span> sensing and responding to winter nutrient pulses, such as phytoplankton blooms. These results increase our understanding on the diversity and metabolic processes occurring under <span class="hlt">ice</span> in northern lakes ecosystems. This article is protected by copyright. All rights reserved. © 2018 Society for Applied Microbiology and John Wiley & Sons Ltd.</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 Antarctic <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 Antarctic <span class="hlt">ice</span> sheet, but <span class="hlt">ice</span>-proximal evidence from the Antarctic <span class="hlt">margin</span> 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 Antarctic <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-Antarctic temperatures. The geochemical provenance of detrital material deposited during these warm intervals suggests <span class="hlt">active</span> erosion of continental bedrock from within the Wilkes Subglacial Basin, an area today buried beneath the East Antarctic <span class="hlt">ice</span> sheet. We interpret this erosion to be associated with retreat of the <span class="hlt">ice</span> sheet <span class="hlt">margin</span> several hundreds of kilometres inland and conclude that the East Antarctic <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/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> covers</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</span>-covered 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 <span class="hlt">marginal</span> <span class="hlt">ice</span> zone. All <span class="hlt">ice</span> covers attenuate wave energy. Only long swells can penetrate deep into an <span class="hlt">ice</span> cover. Being closest to open water, wave propagation in the <span class="hlt">marginal</span> <span class="hlt">ice</span> zone is the most complex to model. The physical appearance of sea <span class="hlt">ice</span> in the <span class="hlt">marginal</span> <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> cover: 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> covers 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> covers, 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('http://adsabs.harvard.edu/abs/2016GeoRL..4311720J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GeoRL..4311720J"><span>Accelerated <span class="hlt">ice</span> shelf rifting and retreat at Pine Island Glacier, West Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jeong, Seongsu; Howat, Ian M.; Bassis, Jeremy N.</p> <p>2016-11-01</p> <p>Pine Island Glacier has undergone several major iceberg calving events over the past decades. These typically occurred when a rift at the heavily fractured shear <span class="hlt">margin</span> propagated across the width of the <span class="hlt">ice</span> shelf. This type of calving is common on polar <span class="hlt">ice</span> shelves, with no clear connection to ocean-<span class="hlt">ice</span> dynamic forcing. In contrast, we report on the recent development of multiple rifts initiating from basal crevasses in the center of the <span class="hlt">ice</span> shelf, resulted in calving further upglacier than previously observed. Coincident with rift formation was the sudden disintegration of the <span class="hlt">ice</span> mélange that filled the northern shear <span class="hlt">margin</span>, resulting in <span class="hlt">ice</span> sheet detachment from this <span class="hlt">margin</span>. Examination of <span class="hlt">ice</span> velocity suggests that this internal rifting resulted from the combination of a change in <span class="hlt">ice</span> shelf stress regime caused by disintegration of the mélange and intensified melting within basal crevasses, both of which may be linked to ocean forcing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28753208','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28753208"><span><span class="hlt">Ice</span> nucleation <span class="hlt">active</span> bacteria in precipitation are genetically diverse and nucleate <span class="hlt">ice</span> by employing different mechanisms.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Failor, K C; Schmale, D G; Vinatzer, B A; Monteil, C L</p> <p>2017-12-01</p> <p>A growing body of circumstantial evidence suggests that <span class="hlt">ice</span> nucleation <span class="hlt">active</span> (<span class="hlt">Ice</span> + ) bacteria contribute to the initiation of precipitation by heterologous freezing of super-cooled water in clouds. However, little is known about the concentration of <span class="hlt">Ice</span> + bacteria in precipitation, their genetic and phenotypic diversity, and their relationship to air mass trajectories and precipitation chemistry. In this study, 23 precipitation events were collected over 15 months in Virginia, USA. Air mass trajectories and water chemistry were determined and 33 134 isolates were screened for <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> (INA) at -8 °C. Of 1144 isolates that tested positive during initial screening, 593 had confirmed INA at -8 °C in repeated tests. Concentrations of <span class="hlt">Ice</span> + strains in precipitation were found to range from 0 to 13 219 colony forming units per liter, with a mean of 384±147. Most <span class="hlt">Ice</span> + bacteria were identified as members of known and unknown <span class="hlt">Ice</span> + species in the Pseudomonadaceae, Enterobacteriaceae and Xanthomonadaceae families, which nucleate <span class="hlt">ice</span> employing the well-characterized membrane-bound INA protein. Two <span class="hlt">Ice</span> + strains, however, were identified as Lysinibacillus, a Gram-positive genus not previously known to include <span class="hlt">Ice</span> + bacteria. INA of the Lysinibacillus strains is due to a nanometer-sized molecule that is heat resistant, lysozyme and proteinase resistant, and secreted. <span class="hlt">Ice</span> + bacteria and the INA mechanisms they employ are thus more diverse than expected. We discuss to what extent the concentration of culturable <span class="hlt">Ice</span> + bacteria in precipitation and the identification of a new heat-resistant biological INA mechanism support a role for <span class="hlt">Ice</span> + bacteria in the initiation of precipitation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999SedG..123..163E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999SedG..123..163E"><span>Hummocky moraine: sedimentary record of stagnant Laurentide <span class="hlt">Ice</span> Sheet lobes resting on soft beds</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Eyles, N.; Boyce, J. I.; Barendregt, R. W.</p> <p>1999-02-01</p> <p>Over large areas of the western interior plains of North America, hummocky moraine (HM) formed at the <span class="hlt">margins</span> of Laurentide <span class="hlt">Ice</span> Sheet (LIS) lobes that flowed upslope against topographic highs. Current depositional models argue that HM was deposited supraglacially from stagnant debris-rich <span class="hlt">ice</span> (`disintegration moraine'). Across southern Alberta, Canada, map and outcrop data show that HM is composed of fine-grained till as much as 25 m thick containing rafts of soft, glaciotectonized bedrock and sediment. Chaotic, non-oriented HM commonly passes downslope into weakly-oriented hummocks (`washboard moraine') that are transitional to drumlins in topographic lows; the same subsurface stratigraphy and till facies is present throughout. These landforms, and others such as doughnut-like `rim ridges', flat-topped `moraine plateaux' and linear disintegration ridges, are identified as belonging to subglacially-deposited soft-bed terrain. This terrain is the record of <span class="hlt">ice</span> lobes moving over deformation till derived from weakly-lithified, bentonite-rich shale. Drumlins record continued <span class="hlt">active</span> <span class="hlt">ice</span> flow in topographic lows during deglaciation whereas HM was produced below the outer stagnant <span class="hlt">margins</span> of <span class="hlt">ice</span> lobes by gravitational loading (`pressing') of remnant dead <span class="hlt">ice</span> blocks into wet, plastic till. Intervening zones of washboard moraine mark the former boundary of <span class="hlt">active</span> and stagnant <span class="hlt">ice</span> and show `hybrid' drumlins whose streamlined form has been altered by subglacial pressing (` humdrums') below dead <span class="hlt">ice</span>. The presence of hummocky moraine over a very large area of interior North America provides additional support for glaciological models of a soft-bedded Laurentide <span class="hlt">Ice</span> Sheet.</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 Antarctic <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 Antarctic <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> <span class="hlt">margin</span> during warm intervals of the Oligocene-Miocene. Flat-lying bedrock plateaus are indicative of an <span class="hlt">ice</span> sheet <span class="hlt">margin</span> 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> <span class="hlt">margin</span> retreat of the scale seen during the early EAIS.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.1805B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.1805B"><span><span class="hlt">Ice</span> nucleation <span class="hlt">activity</span> of polysaccharides</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bichler, Magdalena; Felgitsch, Laura; Haeusler, Thomas; Seidl-Seiboth, Verena; Grothe, Hinrich</p> <p>2015-04-01</p> <p>Heterogeneous <span class="hlt">ice</span> nucleation is an important process in the atmosphere. It shows direct impact on our climate by triggering <span class="hlt">ice</span> cloud formation and therefore it has much influence on the radiation balance of our planet (Lohmann et al. 2002; Mishchenko et al. 1996). The process itself is not completely understood so far and many questions remain open. Different substances have been found to exhibit <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> (INA). Due to their vast differences in chemistry and morphology it is difficult to predict what substance will make good <span class="hlt">ice</span> nuclei and which will not. Hence simple model substances must be found and be tested regarding INA. Our work aims at gaining to a deeper understanding of heterogeneous <span class="hlt">ice</span> nucleation. We intend to find some reference standards with defined chemistry, which may explain the mechanisms of heterogeneous <span class="hlt">ice</span> nucleation. A particular focus lies on biological carbohydrates in regards to their INA. Biological carbohydrates are widely distributed in all kingdoms of life. Mostly they are specific for certain organisms and have well defined purposes, e.g. structural polysaccharides like chitin (in fungi and insects) and pectin (in plants), which has also water-binding properties. Since they are widely distributed throughout our biosphere and mostly safe to use for nutrition purposes, they are well studied and easily accessible, rendering them ideal candidates as proxies. In our experiments we examined various carbohydrates, like the already mentioned chitin and pectin, as well as their chemical modifications. Lohmann U.; A Glaciation Indirect Aerosol Effect Caused by Soot Aerosols; J. Geoph. Res.; Vol. 24 No.4; pp 11-1 - 11-4; 2002 Mishchenko M.I., Rossow W.B., Macke A., Lacis A. A.; Sensitivity of Cirrus Cloud Albedo, Bidirectional Reflectance and Optical Thickness Retrieval Accuracy to <span class="hlt">Ice</span> Particle Shape, J. Geoph. Res.; Vol. 101, No D12; pp. 16,973 - 16,985; 1996</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017QSRv..163..114D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017QSRv..163..114D"><span>Phased occupation and retreat of the last British-Irish <span class="hlt">Ice</span> Sheet in the southern North Sea; geomorphic and seismostratigraphic evidence of a dynamic <span class="hlt">ice</span> lobe</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dove, Dayton; Evans, David J. A.; Lee, Jonathan R.; Roberts, David H.; Tappin, David R.; Mellett, Claire L.; Long, David; Callard, S. Louise</p> <p>2017-05-01</p> <p>Along the terrestrial <span class="hlt">margin</span> of the southern North Sea, previous studies of the MIS 2 glaciation impacting eastern Britain have played a significant role in the development of principles relating to <span class="hlt">ice</span> sheet dynamics (e.g. deformable beds), and the practice of reconstructing the style, timing, and spatial configuration of palaeo-<span class="hlt">ice</span> sheets. These detailed terrestrially-based findings have however relied on observations made from only the outer edges of the former <span class="hlt">ice</span> mass, as the North Sea Lobe (NSL) of the British-Irish <span class="hlt">Ice</span> Sheet (BIIS) occupied an area that is now almost entirely submarine (c.21-15 ka). Compounded by the fact that marine-acquired data have been primarily of insufficient quality and density, the configuration and behaviour of the last BIIS in the southern North Sea remains surprisingly poorly constrained. This paper presents analysis of a new, integrated set of extensive seabed geomorphological and seismo-stratigraphic observations that both advances the principles developed previously onshore (e.g. multiple advance and retreat cycles), and provides a more detailed and accurate reconstruction of the BIIS at its southern-most extent in the North Sea. A new bathymetry compilation of the region reveals a series of broad sedimentary wedges and associated moraines that represent several terminal positions of the NSL. These former still-stand <span class="hlt">ice</span> <span class="hlt">margins</span> (1-4) are also found to relate to newly-identified architectural patterns (shallow stacked sedimentary wedges) in the region's seismic stratigraphy (previously mapped singularly as the Bolders Bank Formation). With ground-truthing constraint provided by sediment cores, these wedges are interpreted as sub-<span class="hlt">marginal</span> till wedges, formed by complex subglacial accretionary processes that resulted in till thickening towards the former <span class="hlt">ice</span>-sheet <span class="hlt">margins</span>. The newly sub-divided shallow seismic stratigraphy (at least five units) also provides an indication of the relative event chronology of the NSL. While there</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2012-12-27/pdf/2012-31125.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2012-12-27/pdf/2012-31125.pdf"><span>77 FR 76316 - Self-Regulatory Organizations; <span class="hlt">ICE</span> Clear Europe Limited; Notice of Filing and Immediate...</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2012-12-27</p> <p>... enhancement to the SPAN for the <span class="hlt">ICE</span> <span class="hlt">Margining</span> algorithm employed to calculate Original <span class="hlt">Margin</span>. All capitalized... Allocation Methodology is an enhancement to the SPAN[supreg] \\6\\ for the <span class="hlt">ICE</span> <span class="hlt">Margining</span> algorithm employed to... the SPAN <span class="hlt">margin</span> calculation algorithm itself has not been changed. As of August 30, 2011, Position...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA566290','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA566290"><span><span class="hlt">Marginal</span> <span class="hlt">Ice</span> Zone (MIZ) Program: Science and Experiment Plan</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2012-10-01</p> <p>decline and greatest loss in arctic summer <span class="hlt">ice</span> (Shimada et al ., 2006 ). The Beaufort Sea lends its name to the Beaufort Gyre, the anti-cyclonic...which in turn influences regional atmospheric circulation patterns and temperature profiles, especially along the seasonal MIZ (Rinke et al ., 2006 ...coupling (Krinner et al ., 2010; Gerdes, 2006 ). Both for scientific and practical reasons, prediction of sea <span class="hlt">ice</span> cover is particularly important as it</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20160006706&hterms=energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Denergy','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20160006706&hterms=energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Denergy"><span>Thermodynamic Derivation of the <span class="hlt">Activation</span> Energy for <span class="hlt">Ice</span> Nucleation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Barahona, D.</p> <p>2015-01-01</p> <p>Cirrus clouds play a key role in the radiative and hydrological balance of the upper troposphere. Their correct representation in atmospheric models requires an understanding of the microscopic processes leading to <span class="hlt">ice</span> nucleation. A key parameter in the theoretical description of <span class="hlt">ice</span> nucleation is the <span class="hlt">activation</span> energy, which controls the flux of water molecules from the bulk of the liquid to the solid during the early stages of <span class="hlt">ice</span> formation. In most studies it is estimated by direct association with the bulk properties of water, typically viscosity and self-diffusivity. As the environment in the <span class="hlt">ice</span>-liquid interface may differ from that of the bulk, this approach may introduce bias in calculated nucleation rates. In this work a theoretical model is proposed to describe the transfer of water molecules across the <span class="hlt">ice</span>-liquid interface. Within this framework the <span class="hlt">activation</span> energy naturally emerges from the combination of the energy required to break hydrogen bonds in the liquid, i.e., the bulk diffusion process, and the work dissipated from the molecular rearrangement of water molecules within the <span class="hlt">ice</span>-liquid interface. The new expression is introduced into a generalized form of classical nucleation theory. Even though no nucleation rate measurements are used to fit any of the parameters of the theory the predicted nucleation rate is in good agreement with experimental results, even at temperature as low as 190 K, where it tends to be underestimated by most models. It is shown that the <span class="hlt">activation</span> energy has a strong dependency on temperature and a weak dependency on water <span class="hlt">activity</span>. Such dependencies are masked by thermodynamic effects at temperatures typical of homogeneous freezing of cloud droplets; however, they may affect the formation of <span class="hlt">ice</span> in haze aerosol particles. The new model provides an independent estimation of the <span class="hlt">activation</span> energy and the homogeneous <span class="hlt">ice</span> nucleation rate, and it may help to improve the interpretation of experimental results and the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19759618','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19759618"><span>Holocene thinning of the Greenland <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>Vinther, B M; Buchardt, S L; Clausen, H B; Dahl-Jensen, D; Johnsen, S J; Fisher, D A; Koerner, R M; Raynaud, D; Lipenkov, V; Andersen, K K; Blunier, T; Rasmussen, S O; Steffensen, J P; Svensson, A M</p> <p>2009-09-17</p> <p>On entering an era of global warming, the stability of the Greenland <span class="hlt">ice</span> sheet (GIS) is an important concern, especially in the light of new evidence of rapidly changing flow and melt conditions at the GIS <span class="hlt">margins</span>. Studying the response of the GIS to past climatic change may help to advance our understanding of GIS dynamics. The previous interpretation of evidence from stable isotopes (delta(18)O) in water from GIS <span class="hlt">ice</span> cores was that Holocene climate variability on the GIS differed spatially and that a consistent Holocene climate optimum-the unusually warm period from about 9,000 to 6,000 years ago found in many northern-latitude palaeoclimate records-did not exist. Here we extract both the Greenland Holocene temperature history and the evolution of GIS surface elevation at four GIS locations. We achieve this by comparing delta(18)O from GIS <span class="hlt">ice</span> cores with delta(18)O from <span class="hlt">ice</span> cores from small <span class="hlt">marginal</span> icecaps. Contrary to the earlier interpretation of delta(18)O evidence from <span class="hlt">ice</span> cores, our new temperature history reveals a pronounced Holocene climatic optimum in Greenland coinciding with maximum thinning near the GIS <span class="hlt">margins</span>. Our delta(18)O-based results are corroborated by the air content of <span class="hlt">ice</span> cores, a proxy for surface elevation. State-of-the-art <span class="hlt">ice</span> sheet models are generally found to be underestimating the extent and changes in GIS elevation and area; our findings may help to improve the ability of models to reproduce the GIS response to Holocene climate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C41B0661K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C41B0661K"><span>The development of blue <span class="hlt">ice</span> moraines from englacial debris bands as detected by GPR, Mt Achernar, central Transantarctic Mountains, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kassab, C.; Lindback, K.; Pettersson, R.; Licht, K.; Graly, J. A.; Kaplan, M. R.</p> <p>2016-12-01</p> <p>Blue <span class="hlt">ice</span> moraines cover a small percentage of Antarctica, but can contain a significant record of <span class="hlt">ice</span> sheet dynamics and climate over multiple glacial cycles. Previous work has focused on the temporal and provenance record contained within these moraines and less on mechanisms by which such deposits form and their temporal evolution. In order to create a conceptual model of their formation, >25 km of ground penetrating radar transects at 25 and 100 MHz frequencies were collected at the Mt Achernar moraine adjacent to Law Glacier. Here, <span class="hlt">ice</span> ablation causes debris bands to emerge and deliver sediment to the surface. Most transects were collected perpendicular to the <span class="hlt">ice</span>-moraine <span class="hlt">margin</span>, and extend from the <span class="hlt">actively</span> flowing Law Glacier <span class="hlt">ice</span> to a distance of 2 km into the moraine. The 25 and 100 MHz transects penetrate to a depth of 200 m and 60 m respectively and reveal a relatively complex internal stratigraphy. Closest to the <span class="hlt">ice</span>-moraine <span class="hlt">margin</span>, stratigraphy is not well resolved due to a high amount of clutter. Steeply dipping parallel reflections first emerge 400m away from the <span class="hlt">ice</span> <span class="hlt">margin</span> and dip toward Law Glacier. These reflections continue inwards to 1450m, where the reflections become more closely spaced. Hummocky topography and parallel ridge/trough topography dominate the geomorphic expression. The hummocky topography corresponds to the region where reflections are not well resolved. The ridges are interpreted to be debris bands that are emerging at the surface, similar to those along the <span class="hlt">margin</span> of the Law Glacier where debris is newly emerging. The reflections in the GPR transects indicate that debris is transported from depth to the surface of the <span class="hlt">ice</span> where it accumulates forming the Mt Achernar moraine. It appears that the various reflection patterns correspond to unique surface geomorphic expressions. The reflections also indicate that at least the first 2 km of debris rich buried <span class="hlt">ice</span> in the moraine can be linked to the <span class="hlt">actively</span> flowing Law Glacier</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C51B0690L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C51B0690L"><span>New constraints on the deglaciation chronology of the southeastern <span class="hlt">margin</span> of the Greenland <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>Levy, L.; Larsen, N. K.; Kjaer, K. H.; Bjork, A. A.; Kjeldsen, K. K.; Funder, S.; Kelly, M. A.; Howley, J. A.; Zimmerman, S. R. H.</p> <p>2015-12-01</p> <p>The Greenland <span class="hlt">Ice</span> Sheet (GrIS) is responding rapidly to climate change. Marine terminating outlet glaciers that drain the GrIS have responded especially sensitively to present-day climate change by accelerating, thinning and retreating. In southeastern Greenland several outlet glaciers are undergoing rapid changes in mass balance and <span class="hlt">ice</span> dynamics. To improve our understanding of the future, long-term response of these marine-terminating outlet glaciers to climate change, we focus on the response of three outlet glaciers to climate change since the Last Glacial Maximum. The timing and rates of late-glacial and early Holocene deglaciation of the southeastern sector of the GrIS are relatively unconstrained due to the inaccessibility of the region. Using a helicopter and a sailboat, we collected samples for 10Be surface exposure dating from three fjords in southeastern Greenland: Skjoldungen (63.4N), Uvtorsiutit (62.7N), and Lindenow (60.6N). These fjords drain marine terminating glaciers of the GrIS. Here we present 18 new 10Be ages from ~50 km long transects along these fjords that mark the timing of deglaciation from the outer coast inland to the present-day GrIS <span class="hlt">margin</span>. Together with previously constrained deglaciation chronologies from Bernstorffs, Sermilik, and Kangerdlussuaq fjords in southeastern Greenland, these new chronologies offer insight into the late-glacial and early Holocene dynamics of the southeastern GrIS outlet glaciers. We compare the timing and rate of deglaciation in southeastern Greenland to climate records from the region to examine the mechanisms that drove deglaciation during late-glacial and early Holocene time. These new 10Be ages provide a longer-term perspective of marine terminating outlet glacier fluctuations in southeastern Greenland and can be used to model the <span class="hlt">ice</span> sheet's response to late-glacial and early Holocene climate changes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70032866','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70032866"><span>Sediment geochemical records of productivity and oxygen depletion along the <span class="hlt">margin</span> of western North America during the past 60,000 years: teleconnections with Greenland <span class="hlt">Ice</span> and the Cariaco Basin</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Dean, W.E.</p> <p>2007-01-01</p> <p>Many sediment records from the <span class="hlt">margins</span> of the Californias (Alta and Baja) collected in water depths between 60 and 1200 m contain anoxic intervals (laminated sediments) that can be correlated with interstadial intervals as defined by the oxygen-isotope composition of Greenland <span class="hlt">ice</span> (Dansgaard-Oeschger, D-O, cycles). These intervals include all or parts of Oxygen Isotope Stage 3 (OIS3; 60-24 cal ka), the Bo??lling/Allero??d warm interval (B/A; 15-13 cal ka), and the Holocene. This study uses organic carbon (Corg) and trace-element proxies for anoxia and productivity, namely elevated concentrations and accumulation rates of molybdenum and cadmium, in these laminated sediments to suggest that productivity may be more important than ventilation in producing changes in bottom-water oxygen (BWO) conditions on open, highly productive continental <span class="hlt">margins</span>. The main conclusion from these proxies is that during the last glacial interval (LGI; 24-15 cal ka) and the Younger Dryas cold interval (YD; 13-11.6 cal ka) productivity was lower and BWO levels were higher than during OIS3, the B/A, and the Holocene on all <span class="hlt">margins</span> of the Californias. The Corg and trace-element profiles in the LGI-B/A-Holocene transition in the Cariaco Basin on the <span class="hlt">margin</span> of northern Venezuela are remarkably similar to those in the transition on the northern California <span class="hlt">margin</span>. Correlation between D-O cycles in Greenland <span class="hlt">ice</span> with gray-scale measurements in varved sediments in the Cariaco Basin also is well established. Synchronous climate-driven changes as recorded in the sediments on the <span class="hlt">margins</span> of the Californias, sediments from the Cariaco Basin, and in the GISP-2 Greenland <span class="hlt">ice</span> core support the hypothesis that changes in atmospheric dynamics played a major role in abrupt climate change during the last 60 ka. Millennial-scale cycles in productivity and oxygen depletion on the <span class="hlt">margins</span> of the Californias demonstrate that the California Current System was poised at a threshold whereby perturbations of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFMED33A0619H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFMED33A0619H"><span><span class="hlt">Ice</span>, <span class="hlt">Ice</span>, Baby!</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hamilton, C.</p> <p>2008-12-01</p> <p>The Center for Remote Sensing of <span class="hlt">Ice</span> Sheets (CReSIS) has developed an outreach program based on hands-on <span class="hlt">activities</span> called "<span class="hlt">Ice</span>, <span class="hlt">Ice</span>, Baby". These lessons are designed to teach the science principles of displacement, forces of motion, density, and states of matter. These properties are easily taught through the interesting topics of glaciers, icebergs, and sea level rise in K-8 classrooms. The <span class="hlt">activities</span> are fun, engaging, and simple enough to be used at science fairs and family science nights. Students who have participated in "<span class="hlt">Ice</span>, <span class="hlt">Ice</span>, Baby" have successfully taught these to adults and students at informal events. The lessons are based on education standards which are available on our website www.cresis.ku.edu. This presentation will provide information on the <span class="hlt">activities</span>, survey results from teachers who have used the material, and other suggested material that can be used before and after the <span class="hlt">activities</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMEP11A..03R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMEP11A..03R"><span>Sediment movement and dispersal patterns on the Grand Banks continental shelf and slope were tied to the dynamics of the Laurentide <span class="hlt">ice</span>-sheet <span class="hlt">margin</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rashid, H.; MacKillop, K.; Piper, D.; Vermooten, M.; Higgins, J.; Marche, B.; Langer, K.; Brockway, B.; Spicer, H. E.; Webb, M. D.; Fournier, E.</p> <p>2015-12-01</p> <p>The expansion and contraction of the late Pleistocene Laurentide <span class="hlt">ice</span>-sheet (LIS) was the crucial determining factor for the geomorphic features and shelf and slope sediment mobility on the eastern Canadian continental <span class="hlt">margin</span>, with abundant mass-transport deposits (MTDs) seaward of <span class="hlt">ice</span> <span class="hlt">margins</span> on the upper slope. Here, we report for the first time sediment failure and mass-transport deposits from the central Grand Banks slope in the Salar and Carson petroleum basins. High-resolution seismic profiles and multibeam bathymetry show numerous sediment failure scarps in 500-1600 m water depth. There is no evidence for an <span class="hlt">ice</span> <span class="hlt">margin</span> on the upper slope younger than MIS 6. Centimeter-scale X-ray fluorescence analysis (XRF), grain size, and oxygen isotope data from piston cores constrain sediment processes over the past 46 ka. Geotechnical measurements including Atterberg limit tests, vane shear measurements and triaxial and multi-stage isotropic consolidation tests allowed us to assess the instability on the continental <span class="hlt">margin</span>. Cores with continuous undisturbed stratigraphy in contourite silty muds show normal downcore increase in bulk density and undrained peak shear strength. Heinrich (H) layers are identifiable by a marked increase in the bulk density, high Ca (ppm), increase in iceberg-rafted debris and lighter δ18O in the polar planktonic foram Neogloboquadrina pachyderma (sinistral): with a few C-14 dates they provide a robust chronology. There is no evidence for significant supply of sediment from the Grand Banks at the last-glacial maximum. Mass-transport deposits (MTD) are marked by variability in the bulk density, undrained shear strength and little variation in bulk density or Ca (ppm) values. The MTD are older than 46 ka on the central Grand Banks slope, whereas younger MTDs are present in southern Flemish Pass. Factor of safety calculations suggest the slope is statically stable up to gradients of 10°, but more intervals of silty mud may fail during earthquake</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMOS11B1654B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMOS11B1654B"><span>Skin Temperature Processes in the Presence of 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>Brumer, S. E.; Zappa, C. J.; Brown, S.; McGillis, W. R.; Loose, B.</p> <p>2013-12-01</p> <p>Monitoring the sea-<span class="hlt">ice</span> <span class="hlt">margins</span> of polar oceans and understanding the physical processes at play at the <span class="hlt">ice</span>-ocean-air interface is essential in the perspective of a changing climate in which we face an accelerated decline of <span class="hlt">ice</span> caps and sea <span class="hlt">ice</span>. Remote sensing and in particular InfraRed (IR) imaging offer a unique opportunity not only to observe physical processes at sea-<span class="hlt">ice</span> <span class="hlt">margins</span>, but also to measure air-sea exchanges near <span class="hlt">ice</span>. It permits monitoring <span class="hlt">ice</span> and ocean temperature variability, and can be used for derivation of surface flow field allowing investigating turbulence and shearing at the <span class="hlt">ice</span>-ocean interface as well as ocean-atmosphere gas transfer. Here we present experiments conducted with the aim of gaining an insight on how the presence of sea <span class="hlt">ice</span> affects the momentum exchange between the atmosphere and ocean and investigate turbulence production in the interplay of <span class="hlt">ice</span>-water shear, convection, waves and wind. A set of over 200 high resolution IR imagery records was taken at the US Army Cold Regions Research and Engineering Laboratory (CRREL, Hanover NH) under varying <span class="hlt">ice</span> coverage, fan and pump settings. In situ instruments provided air and water temperature, salinity, subsurface currents and wave height. Air side profiling provided environmental parameters such as wind speed, humidity and heat fluxes. The study aims to investigate what can be gained from small-scale high-resolution IR imaging of the <span class="hlt">ice</span>-ocean-air interface; in particular how sea <span class="hlt">ice</span> modulates local physics and gas transfer. The relationship between water and <span class="hlt">ice</span> temperatures with current and wind will be addressed looking at the ocean and <span class="hlt">ice</span> temperature variance. Various skin temperature and gas transfer parameterizations will be evaluated at <span class="hlt">ice</span> <span class="hlt">margins</span> under varying environmental conditions. Furthermore the accuracy of various techniques used to determine surface flow will be assessed from which turbulence statistics will be determined. This will give an insight on how <span class="hlt">ice</span> presence</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..1513402T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..1513402T"><span>Export of <span class="hlt">Ice</span>-Cavity Water from Pine Island <span class="hlt">Ice</span> Shelf, West Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thurnherr, Andreas; Jacobs, Stanley; Dutrieux, Pierre</p> <p>2013-04-01</p> <p> significant mean upward motion within the cove strongly suggests that the upwelling takes place within the highly fractured <span class="hlt">ice</span> along the southern shear <span class="hlt">margin</span> of the <span class="hlt">ice</span> shelf. If so, the upwelling water is likely to contribute to both the volume of apparent "basal" melting and to the weakness of that shear <span class="hlt">margin</span>.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_10 --> <div id="page_11" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="201"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70030522','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70030522"><span>Terrestrial <span class="hlt">ice</span> streams-a view from the lobe</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Jennings, C.E.</p> <p>2006-01-01</p> <p>The glacial landforms of Minnesota are interpreted as the products of the lobate extensions of <span class="hlt">ice</span> streams that issued from various <span class="hlt">ice</span> sheds within the Laurentide <span class="hlt">Ice</span> Sheet. Low-relief till plains, trough-shaped lowlands, boulder pavements, and streamlined forms make up the subglacial landsystem in Minnesota that is interpreted as having been formed by streaming <span class="hlt">ice</span>. Extremely uniform tills are created subglacially in a way that remains somewhat mysterious. At the <span class="hlt">ice</span> <span class="hlt">margins</span>, thrust moraines and hummocky stagnation topography are more common than single-crested, simple moraines if the <span class="hlt">ice</span> lobes had repeated advances. Subglacial drainage features are obscure up-<span class="hlt">ice</span> but are present down-<span class="hlt">ice</span> in the form of tunnel valleys, eskers, Spooner hills, and associated <span class="hlt">ice-marginal</span> fans. <span class="hlt">Ice</span> streaming may occur when basal shear stress is lowered as a result of high subglacial water pressure. Subglacial conditions that allow the retention of water will allow an <span class="hlt">ice</span> lobe to extend far beyond the <span class="hlt">ice</span> sheet as long as the <span class="hlt">ice</span> shed also supports the advance by supplying adequate <span class="hlt">ice</span>. Even with adequate <span class="hlt">ice</span> flux, however, the advance of an <span class="hlt">ice</span> lobe may be terminated, at least temporarily, if the subglacial water is drained, through tunnel valleys or perhaps a permeable substrate. Thrust moraines, and <span class="hlt">ice</span> stagnation topography will result from sudden drainage. Although climate change is ultimately responsible for the accumulation of <span class="hlt">ice</span> in the Laurentide <span class="hlt">Ice</span> Sheet, the asynchronous advances and retreats of the <span class="hlt">ice</span> lobes in the mid-continent are strongly overprinted by the internal dynamics of individual <span class="hlt">ice</span> streams as well as the interaction of <span class="hlt">ice</span> sheds, which obscure the climate signal. ?? 2005 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20030110723&hterms=BELT+CONVEYOR&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DBELT%2BCONVEYOR','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20030110723&hterms=BELT+CONVEYOR&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DBELT%2BCONVEYOR"><span>The Broken Belt: Meteorite Concentrations on Stranded <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>Harvey, R. P.</p> <p>2003-01-01</p> <p>Since the first Antarctic meteorite concentrations were discovered more than 25 years ago, many theories regarding the role of iceflow in the production of meteorite concentrations have been put forward, and most agree on the basic principles. These models suggest that as the East Antarctic icesheet flows toward the <span class="hlt">margins</span> of the continent, meteorites randomly located within the volume of <span class="hlt">ice</span> are transported toward the icesheet <span class="hlt">margin</span>. Where mountains or subsurface obstructions block glacial flow, diversion of <span class="hlt">ice</span> around or over an obstruction reduces horizontal <span class="hlt">ice</span> movement rates adjacent to the barriers and creates a vertical (upward) component of movement. If local mechanisms for <span class="hlt">ice</span> loss (ablation) exist at such sites, an equilibrium surface will develop according to the balance between <span class="hlt">ice</span> supply and loss, and the cargo of meteorites is exhumed on a blue <span class="hlt">ice</span> surface. The result is a conceptual conveyor belt bringing meteorite-bearing volumes of <span class="hlt">ice</span> from the interior of the continent to stagnant or slowmoving surfaces where <span class="hlt">ice</span> is then lost and a precious cargo is left as a lag deposit. Cassidy et al. provides an excellent overview of how this model has been adapted to several Antarctic stranding surfaces.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4368087','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4368087"><span>Identification of <span class="hlt">Ice</span> Nucleation <span class="hlt">Active</span> Sites on Feldspar Dust Particles</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p></p> <p>2015-01-01</p> <p>Mineral dusts originating from Earth’s crust are known to be important atmospheric <span class="hlt">ice</span> nuclei. In agreement with earlier studies, feldspar was found as the most <span class="hlt">active</span> of the tested natural mineral dusts. Here we investigated in closer detail the reasons for its <span class="hlt">activity</span> and the difference in the <span class="hlt">activity</span> of the different feldspars. Conclusions are drawn from scanning electron microscopy, X-ray powder diffraction, infrared spectroscopy, and oil-immersion freezing experiments. K-feldspar showed by far the highest <span class="hlt">ice</span> nucleation <span class="hlt">activity</span>. Finally, we give a potential explanation of this effect, finding alkali-metal ions having different hydration shells and thus an influence on the <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> of feldspar surfaces. PMID:25584435</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2013-01-03/pdf/2012-31568.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2013-01-03/pdf/2012-31568.pdf"><span>78 FR 330 - Self-Regulatory Organizations; <span class="hlt">ICE</span> Clear Europe Limited; Notice of Filing and Immediate...</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2013-01-03</p> <p>... Rule Change To Amend SPAN <span class="hlt">Margin</span> Parameters for <span class="hlt">ICE</span> OTC Natural Gas Liquids Contracts December 27, 2012... Rule Change The purpose of the change is to amend SPAN <span class="hlt">Margin</span> Parameters for <span class="hlt">ICE</span> OTC Natural Gas Liquids (NGL) Contracts. All capitalized terms not defined herein are defined in the <span class="hlt">ICE</span> Clear Europe...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14.5202G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.5202G"><span>The <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> of biological aerosols</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Grothe, H.; Pummer, B.; Bauer, H.; Bernardi, J.</p> <p>2012-04-01</p> <p>Primary Biological Aerosol Particles (PBAPs), including bacteria, spores and pollen may be important for several atmospheric processes. Particularly, the <span class="hlt">ice</span> nucleation caused by PBAPs is a topic of growing interest, since their impact on <span class="hlt">ice</span> cloud formation and thus on radiative forcing, an important parameter in global climate is not yet fully understood. In laboratory model studies we investigated the <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> of selected PBAPs. We studied the immersion mode freezing using water-oil emulsion, which we observed by optical microscopy. We particularly focused on pollen. We show that pollen of different species strongly differ in their <span class="hlt">ice</span> nucleation behavior. The average freezing temperatures in laboratory experiments range from 240 K to 255 K. As the most efficient nuclei (silver birch, Scots pine and common juniper pollen) have a distribution area up to the Northern timberline, their <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> might be a cryoprotective mechanism. For comparison the <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> of Snomax, fungal spores, and mushrooms will be discussed as well. In the past, pollen have been rejected as important atmospheric IN, as they are not as abundant in the atmosphere as bacteria or mineral dust and are too heavy to reach higher altitudes. However, in our experiments (Pummer et al. 2011) it turned out that water, which had been in contact with pollen and then been separated from the bodies, nucleates as good as the pollen grains themselves. So the <span class="hlt">ice</span> nuclei have to be easily-suspendable macromolecules (100-300 kDa) located on the pollen. Once extracted, they can be distributed further through the atmosphere than the heavy pollen grains and so augment the impact of pollen on <span class="hlt">ice</span> cloud formation even in the upper troposphere. It is widely known, that material from the pollen, like allergens and sugars, can indeed leave the pollen body and be distributed independently. The most probable mechanism is the pollen grain bursting by rain, which releases</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.C41E0469B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.C41E0469B"><span><span class="hlt">Ice</span>Bridge Provides Novel Evidence for Thick Units of Basal Freeze-on <span class="hlt">Ice</span> Along Petermann Glacier, Greenland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bell, R. E.; Tinto, K. J.; Wolovick, M.; Block, A. E.; Frearson, N.; Das, I.; Abdi, A.; Creyts, T. T.; Cochran, J. R.; Csatho, B. M.; Babonis, G. S.</p> <p>2011-12-01</p> <p>The Petermann Glacier, one of the major outlet glaciers in Greenland, drains six percent of the Greenland <span class="hlt">ice</span> from a basin largely below sea level. Petermann Glacier and its large <span class="hlt">ice</span> shelf may be susceptible to increased change as the waters along the Greenland <span class="hlt">margin</span> warm. The 2010 and 2011 Operation <span class="hlt">Ice</span>Bridge mission, acquired a comprehensive aerogeophysical data set over the Petermann Glacier that provides insights into the <span class="hlt">ice</span> sheet structure. This analysis employs most of the data streams acquired by the Icebridge platform including <span class="hlt">ice</span>-penetrating radar, laser altimetry, gravity and magnetics. An orthogonal 10 km grid extends from 60 km upstream of the grounding line to 240 km inland. The <span class="hlt">ice</span> velocities in the region range from <50m/yr to >200m/yr. On the interior lines the internal layers are pulled down over 2-3 km wide regions. Up to 400m of <span class="hlt">ice</span> from the base of the <span class="hlt">ice</span> sheet appears to be absent in these regions. We interpret these pulled down regions as basal melt. These melt regions are mainly located along the upstream side of a 80 km wide east-west trending topographic ridge that separates the interior <span class="hlt">ice</span> from the Petermann Fjord. The <span class="hlt">Ice</span>Bridge magnetic data indicates that this broad flat ridge is the boundary between the Franklinian Basins and the Ellsmerian Foldbelt to the north. Downstream of these pull-down layers we have identified 4 distinct packages of <span class="hlt">ice</span> that thicken downstream and are characterized by a strong upper reflector. These packages develop at the base of the <span class="hlt">ice</span> sheet and reach thicknesses of 500-700m over distances of 10-20 km. These basal packages can be traced for 30-100 km following the direction of flow, and may be present close to the grounding line. These basal reflectors deflect the overlying internal layers upward indicating the addition of <span class="hlt">ice</span> to the base of the <span class="hlt">ice</span> sheet. The <span class="hlt">Ice</span>Bridge gravity data indicates that these features are probably not off-nadir topography since these would show up as around 30mGal anomalies</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19890009373&hterms=sutherland&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dsutherland','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19890009373&hterms=sutherland&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dsutherland"><span>Intercomparison of synthetic- and real-aperture radar observations of Arctic sea <span class="hlt">ice</span> during winter MIZEX '87</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Schuchmann, R. A.; Onstott, R. G.; Sutherland, L. L.; Wackerman, C. C.</p> <p>1988-01-01</p> <p><span class="hlt">Active</span> microwave measurements were made of various sea <span class="hlt">ice</span> forms in March and April 1987 during the <span class="hlt">Marginal</span> <span class="hlt">Ice</span> Zone Experiment, at 1, 5, 10, 18, and 35 GHz using a synthetic aperture radar (SAR) and helicopter and ship-based scatterometers. The X-band (9.8 GHz) SAR data were compared to the scatterometer data and it was determined that for 5 GHz and higher frequencies both the SAR and scatterometers can differentiate open water, new <span class="hlt">ice</span> (5 to 30 cm), first-year <span class="hlt">ice</span> with rubble (0.60 -1.5 m), and multiyear <span class="hlt">ice</span>. The analysis further confirmed that the C-band (5 GHz) SAR's flying on ESA ERS-1 and Radarsat will differentiate the mentioned <span class="hlt">ice</span> types.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910044122&hterms=refraction&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Drefraction','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910044122&hterms=refraction&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Drefraction"><span>Observation of wave refraction at an <span class="hlt">ice</span> edge by synthetic aperture radar</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Liu, Antony K.; Vachon, Paris W.; Peng, Chih Y.</p> <p>1991-01-01</p> <p>In this note the refraction of waves at the <span class="hlt">ice</span> edge is studied by using aircraft synthesis aperture radar (SAR). Penetration of a dominant swell from open ocean into the <span class="hlt">ice</span> cover was observed by SAR during the Labrador <span class="hlt">Ice</span> <span class="hlt">Margin</span> Experiment (LIMEX), conducted on the <span class="hlt">marginal</span> <span class="hlt">ice</span> zone (MIZ) off the east coast of Newfoundland, Canada, in March 1987. At an <span class="hlt">ice</span> edge with a large curvature, the dominant swell component disappeared locally in the SAR imagery. Six subscenes of waves in the MIZ from the SAR image have been processed, revealing total reflection, refraction, and energy reduction of the ocean waves by the <span class="hlt">ice</span> cover. The observed variations of wave spectra from SAR near the <span class="hlt">ice</span> edge are consistent with the model prediction of wave refraction at the <span class="hlt">ice</span> edge due to the change of wave dispersion relation in <span class="hlt">ice</span> developed by Liu and Mollo-Christensen (1988).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012ACPD...1226143M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012ACPD...1226143M"><span>Urediospores of Puccinia spp. and other rusts are warm-temperature <span class="hlt">ice</span> nucleators and harbor <span class="hlt">ice</span> nucleation <span class="hlt">active</span> bacteria</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Morris, C. E.; Sands, D. C.; Glaux, C.; Samsatly, J.; Asaad, S.; Moukahel, A. R.; Gonçalves, F. L. T.; Bigg, E. K.</p> <p>2012-10-01</p> <p>In light of various features of the biology of the rust fungi and of the epidemiology of the plant diseases they cause that illustrate the important role of rainfall in their life history, we have characterized the <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> (INA) of the aerially disseminated spores (urediospores) of this group of fungi. Urediospores of this obligate plant parasite were collected from natural infections from 7 species of weeds in France, from coffee in Brazil and from field and greenhouse-grown wheat in France, the USA, Turkey and Syria. Immersion freezing was used to determine freezing onset temperatures and the abundance of <span class="hlt">ice</span> nuclei in suspensions of washed spores. Microbiological analyses of spores and subsequent tests of the <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> of the bacteria associated with spores were deployed to quantify the contribution of bacteria to the <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> of the spores. All samples of spores were <span class="hlt">ice</span> nucleation <span class="hlt">active</span> having freezing onset temperatures as warm as -4 °C. Spores in most of the samples carried cells of <span class="hlt">ice</span> nucleation-<span class="hlt">active</span> strains of the bacterium Pseudomonas syringae (at rates of less than 1 bacterial cell per 100 urediospores), but bacterial INA accounted for only a small fraction of the INA observed in spore suspensions. Changes in the INA of spore suspensions after treatment with lysozyme suggest that the INA of urediospores involves a polysaccharide. Based on data from the literature, we have estimated the concentrations of urediospores in air at cloud height and in rainfall. These quantities are very similar to those reported for other biological <span class="hlt">ice</span> nucleators in these same substrates. We suggest that air sampling techniques have ignored the spatial and temporal variability of atmospheric concentrations that occur under conditions propitious for precipitation that could increase their local abundance intermittently. Nevertheless, we propose that the relative low abundance of warm-temperature biological <span class="hlt">ice</span> nucleators in the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA602481','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA602481"><span><span class="hlt">Marginal</span> <span class="hlt">Ice</span> Zone: Biogeochemical Sampling with Gliders</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>melt and phytoplankton optical properties under Arctic <span class="hlt">ice</span>. The project specific goals are to build collaboration with Arctic biogeochemists at...the ship to the larger spatial scales sampled by the gliders, and to estimate the contribution of phytoplankton to heating in the water column...Seagliders with from shipboard measurements taken on the R/V Araon and develop optical proxies for phytoplankton concentration, pigment spectral absorption</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA258067','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA258067"><span>Sediment Flux, East Greenland <span class="hlt">Margin</span></span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1991-09-17</p> <p>D.. T 0ATE [3. AEORT TYPE AND ý -2-’S .’:2,E.i 09/17/91 Final Oct. . 1988 - Seot.l. 1991 4. TITLE AND SU.3TITLE S. F*.i1CjG . AU • 12..5 Sediment Flux...and s le ,; its ditribution is unlimited. 13. ABSTRACT (Maximum 2CO words) We investigated sediment flux across an <span class="hlt">ice</span>-dominated, high latitude...investigated an area off the East Greenland <span class="hlt">margin</span> where the world’s second largest <span class="hlt">ice</span> sheet still exists and where information on the extent of glaciation on</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1715613W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1715613W"><span>The impacts of intense moisture transport on the deep and <span class="hlt">marginal</span> sea-<span class="hlt">ice</span> zones of the Arctic during winter</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Woods, Cian; Caballero, Rodrigo</p> <p>2015-04-01</p> <p> warming at the surface. There are an average of 14 such events that enter the polar cap each winter, driving about 50% of the seasonal variation in surface temperature over the deep Arctic. We show that, over the last 30 years, the <span class="hlt">marginal</span> <span class="hlt">ice</span>-zones in the Barents, Labrador and Chukchi Seas have experienced roughly a doubling in the frequency of these intense moisture intrusion events during winter. Interestingly, these are the regions that have experienced the most rapid wintertime <span class="hlt">ice</span> loss in the Arctic, raising the question: to what extent has the recent Arctic warming been driven by local vs. interannual/remote processes?</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008DSRII..55.2330T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008DSRII..55.2330T"><span>Pelagic and sympagic contribution of organic matter to zooplankton and vertical export in the Barents Sea <span class="hlt">marginal</span> <span class="hlt">ice</span> zone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tamelander, Tobias; Reigstad, Marit; Hop, Haakon; Carroll, Michael L.; Wassmann, Paul</p> <p>2008-10-01</p> <p> exported from the euphotic zone was derived from pelagic primary production, but at 3 of 11 stations within the <span class="hlt">marginal</span> <span class="hlt">ice</span> zone (MIZ), the <span class="hlt">ice</span> algal signal dominated the isotope composition of sinking material. The δ 13C of settling organic matter was positively related to the vertical flux of particulate organic carbon, with maximum values around -21‰ during the peak bloom phase. Sedimentation of isotopically light copepod faecal pellets (mean δ 13C -25.4‰) was reflected in a depletion of 13C in the sinking material. The results illustrate tight pelagic-benthic coupling in the Barents Sea MIZ through vertical export of fresh phytodetritus during phytoplankton blooms and episodic export of <span class="hlt">ice</span> algae.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6395368-natural-constraints-exploring-antarctica-continental-margin-existing-geophysical-geological-data-basis-proposed-drilling-program','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6395368-natural-constraints-exploring-antarctica-continental-margin-existing-geophysical-geological-data-basis-proposed-drilling-program"><span>Natural constraints on exploring Antarctica's continental <span class="hlt">margin</span>, existing geophysical and geological data basis, and proposed drilling program</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Anderson, J.B.</p> <p>1987-05-01</p> <p>There have been a number of multichannel seismic reflection and seismic refraction surveys of the Antarctic continental shelf. While glacial erosion has left acoustic basement exposed on portions of the inner shelf, thick sedimentary sequences occur on the passive <span class="hlt">margin</span> of east Antarctica. The thickness and age of these strata vary due to different breakup histories of the <span class="hlt">margin</span>. Several sedimentary basins have been identified. Most are rift basins formed during the early stages of Antarctica's separation from other Gondwana continents and plateaus. The west Antarctic continental shelf is extensive, being approximately twice the size of the Gulf of Mexicomore » shelf. It has been poorly surveyed to date, owing mainly to its perennial sea <span class="hlt">ice</span> cover. Gradual subduction of the spreading center from south to north along the <span class="hlt">margin</span> resulted in old <span class="hlt">active</span> <span class="hlt">margin</span> sequences being buried beneath passive <span class="hlt">margin</span> sequences. The latter should increase in thickness from north to south along the <span class="hlt">margin</span> although no data bear this out. Hydrocarbon potential on the northern portion of the west Antarctic <span class="hlt">margin</span> is considered low due to a probable lack of reservoir rocks. Establishment of <span class="hlt">ice</span> sheets on Antarctica caused destruction of land vegetation and greatly restricted siliciclastic sand-producing environments. So only sedimentary basins which contain pre-early Miocene deposits have good hydrocarbon prospectivity. The Antarctic continental shelf is the deepest in the world, averaging 500 m and in places being more than a kilometer deep. The shelf has been left rugged by glacial erosion and is therefore prone to sediment mass movement. Widespread sediment gravity flow deposits attest to this. The shelf is covered with sea <span class="hlt">ice</span> most of the year and in a few areas throughout the year. Icebergs, drift freely in the deep waters of the shelf; drift speeds of 1 to 2.5 km/year are not uncommon.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA637421','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA637421"><span>On Wave-<span class="hlt">Ice</span> Interaction in the Arctic <span class="hlt">Marginal</span> <span class="hlt">Ice</span> Zone: Dispersion, Attenuation, and <span class="hlt">Ice</span> Response</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2016-06-01</p> <p>PROJECT NUMBER 5e. TASK NUMBER 5f. WORK UNIT NUMBER 2. REPORT TYPE1. REPORT DATE (DD-MM-YYYY) 4. TITLE AND SUBTITLE 6. AUTHOR(S) 8. PERFORMING...schemes and contributes to a change of wave height (and direction) analogous to shoaling and refraction. A method for jointly measuring dispersion and...46 APPENDEX B: WAVE HEIGHTS MEASURED IN ARTIC <span class="hlt">ICE</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20977900','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20977900"><span><span class="hlt">Ice</span> restructuring inhibition <span class="hlt">activities</span> in antifreeze proteins with distinct differences in thermal hysteresis.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yu, Sally O; Brown, Alan; Middleton, Adam J; Tomczak, Melanie M; Walker, Virginia K; Davies, Peter L</p> <p>2010-12-01</p> <p>Antifreeze proteins (AFPs) share two related properties: the ability to depress the freezing temperature below the melting point of <span class="hlt">ice</span> (thermal hysteresis; TH); and the ability to inhibit the restructuring of <span class="hlt">ice</span> into larger crystals. Since the 'hyperactive' AFPs, which have been more recently discovered, show an order of magnitude more TH than previously characterized AFPs, we have now determined their <span class="hlt">activities</span> in <span class="hlt">ice</span> restructuring inhibition (IrI) assays. IrI <span class="hlt">activities</span> of three TH-hyperactive AFPs and three less TH-<span class="hlt">active</span> AFPs varied over an 8-fold range. There was no obvious correlation between high TH <span class="hlt">activity</span> and high IrI <span class="hlt">activity</span>. However, the use of mutant AFPs demonstrated that severe disruption of <span class="hlt">ice</span>-binding residues diminished both TH and IrI similarly, revealing that that the same <span class="hlt">ice</span>-binding residues are crucial for both <span class="hlt">activities</span>. In addition, bicarbonate ions, which are known to enhance the TH <span class="hlt">activity</span> of AFPs, also enhanced their IrI <span class="hlt">activity</span>. We suggest that these seemingly contradictory observations can be partially explained by differences in the coverage of <span class="hlt">ice</span> by TH-hyperactive and non-hyperactive AFPs, and by differences in the stability of AFP-bound <span class="hlt">ice</span> under supercooled and recrystallization conditions. Copyright © 2010 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018QSRv..182...93K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018QSRv..182...93K"><span>Changes in sea <span class="hlt">ice</span> cover and <span class="hlt">ice</span> sheet extent at the Yermak Plateau during the last 160 ka - Reconstructions from biomarker records</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kremer, A.; Stein, R.; Fahl, K.; Ji, Z.; Yang, Z.; Wiers, S.; Matthiessen, J.; Forwick, M.; Löwemark, L.; O'Regan, M.; Chen, J.; Snowball, I.</p> <p>2018-02-01</p> <p>The Yermak Plateau is located north of Svalbard at the entrance to the Arctic Ocean, i.e. in an area highly sensitive to climate change. A multi proxy approach was carried out on Core PS92/039-2 to study glacial-interglacial environmental changes at the northern Barents Sea <span class="hlt">margin</span> during the last 160 ka. The main emphasis was on the reconstruction of sea <span class="hlt">ice</span> cover, based on the sea <span class="hlt">ice</span> proxy IP25 and the related phytoplankton - sea <span class="hlt">ice</span> index PIP25. Sea <span class="hlt">ice</span> was present most of the time but showed significant temporal variability decisively affected by movements of the Svalbard Barents Sea <span class="hlt">Ice</span> Sheet. For the first time, we prove the occurrence of seasonal sea <span class="hlt">ice</span> at the eastern Yermak Plateau during glacial intervals, probably steered by a major northward advance of the <span class="hlt">ice</span> sheet and the formation of a coastal polynya in front of it. Maximum accumulation of terrigenous organic carbon, IP25 and the phytoplankton biomarkers (brassicasterol, dinosterol, HBI III) can be correlated to distinct deglaciation events. More severe, but variable sea <span class="hlt">ice</span> cover prevailed at the Yermak Plateau during interglacials. The general proximity to the sea <span class="hlt">ice</span> <span class="hlt">margin</span> is further indicated by biomarker (GDGT) - based sea surface temperatures below 2.5 °C.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19850017731&hterms=climate+exchange&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dclimate%2Bexchange','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19850017731&hterms=climate+exchange&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dclimate%2Bexchange"><span>Sea <span class="hlt">Ice</span>, Climate and Fram Strait</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hunkins, K.</p> <p>1984-01-01</p> <p>When sea <span class="hlt">ice</span> is formed the albedo of the ocean surface increases from its open water value of about 0.1 to a value as high as 0.8. This albedo change effects the radiation balance and thus has the potential to alter climate. Sea <span class="hlt">ice</span> also partially seals off the ocean from the atmosphere, reducing the exchange of gases such as carbon dioxide. This is another possible mechanism by which climate might be affected. The <span class="hlt">Marginal</span> <span class="hlt">Ice</span> Zone Experiment (MIZEX 83 to 84) is an international, multidisciplinary study of processes controlling the edge of the <span class="hlt">ice</span> pack in that area including the interactions between sea, air and <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930022706&hterms=climate+change+evidence&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dclimate%2Bchange%2Bevidence','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930022706&hterms=climate+change+evidence&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dclimate%2Bchange%2Bevidence"><span>Aerogeophysical evidence for <span class="hlt">active</span> volcanism beneath the West Antarctic <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>Blankenship, Donald D.; Bell, Robin E.; Hodge, Steven M.; Brozena, John M.; Behrendt, John C.</p> <p>1993-01-01</p> <p>Although it is widely understood that the collapse of the West Antarctic <span class="hlt">Ice</span> Sheet (WAIS) would cause a global sea-level rise of 6 m, there continues to be considerable debate about the response of this <span class="hlt">ice</span> sheet to climate change. The stability of the WAIS, which is characterized by a bed grounded well below sea level, may depend on geologically controlled conditions at the base, which are independent of climate. <span class="hlt">Ice</span> streams moving up to 750 m/yr disperse material from the interior through to the oceans. As these <span class="hlt">ice</span> streams tend to buffer the reservoir of slow-moving inland <span class="hlt">ice</span> from exposure to oceanic degradation, understanding the <span class="hlt">ice</span>-streaming process is important for evaluating WAIS stability. There is strong evidence that <span class="hlt">ice</span> streams slide on a lubricating layer of water-saturated till. Development of this basal layer requires both water and easily eroded sediments. <span class="hlt">Active</span> lithospheric extension may elevate regional heat flux, increase basal melting, and trigger <span class="hlt">ice</span> streaming. If a geologically defined boundary with a sharp contrast in geothermal flux exists beneath the WAIS, <span class="hlt">ice</span> streams may only be capable of operating as a buffer over a restricted region. Should ocean waters penetrate beyond this boundary, the <span class="hlt">ice</span>-stream buffer would disappear, possibly triggering a collapse of the inland <span class="hlt">ice</span> reservoir. Aerogeophysical evidence for <span class="hlt">active</span> volcanism and elevated heat flux beneath the WAIS near the critical region where <span class="hlt">ice</span> streaming begins is presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19790001950','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19790001950"><span>Rocket effluent: Its <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> and related properties</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parungo, F. P.; Allee, P. A.</p> <p>1978-01-01</p> <p>To investigate the possibility of inadvertent weather modification from rocket effluent, aerosol samples were collected from an instrumented aircraft subsequent to the Voyager 1 and 2 launches. The aerosol's morphology, concentration, and size distribution were examined with an electron microscope. The elemental compositions of individual particles were analyzed with an X-ray energy spectrometer. <span class="hlt">Ice</span> nucleus concentration was measured with a thermal diffusion chamber. The particles' physical and chemical properties were related to their <span class="hlt">ice</span> nucleation <span class="hlt">activity</span>. A laboratory experiment on rocket propellant exhaust was conducted under controlled conditions. Both laboratory and field experimental results indicated that rocket propellant exhaust can produce <span class="hlt">active</span> <span class="hlt">ice</span> nuclei and modify local weather in suitable meteorological conditions.</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/2015EGUGA..17.5282N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.5282N"><span>Can we define an asymptotic value for the <span class="hlt">ice</span> <span class="hlt">active</span> surface site density for heterogeneous <span class="hlt">ice</span> nucleation?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Niedermeier, Dennis; Augustin-Bauditz, Stefanie; Hartmann, Susan; Wex, Heike; Ignatius, Karoliina; Stratmann, Frank</p> <p>2015-04-01</p> <p>The formation of <span class="hlt">ice</span> in atmospheric clouds has a substantial influence on the radiative properties of clouds as well as on the formation of precipitation. Therefore much effort has been made to understand and quantify the major <span class="hlt">ice</span> formation processes in clouds. Immersion freezing has been suggested to be a dominant primary <span class="hlt">ice</span> formation process in low and mid-level clouds (mixed-phase cloud conditions). It also has been shown that mineral dust particles are the most abundant <span class="hlt">ice</span> nucleating particles in the atmosphere and thus may play an important role for atmospheric <span class="hlt">ice</span> nucleation (Murray et al., 2012). Additionally, biological particles like bacteria and pollen are suggested to be potentially involved in atmospheric <span class="hlt">ice</span> formation, at least on a regional scale (Murray et al., 2012). In recent studies for biological particles (SNOMAX and birch pollen), it has been demonstrated that freezing is induced by <span class="hlt">ice</span> nucleating macromolecules and that an asymptotic value for the mass density of these <span class="hlt">ice</span> nucleating macromolecules can be determined (Hartmann et al., 2013; Augustin et al., 2013, Wex et al., 2014). The question arises whether such an asymptotic value can also be determined for the <span class="hlt">ice</span> <span class="hlt">active</span> surface site density ns, a parameter which is commonly used to describe the <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> of e.g., mineral dust. Such an asymptotic value for ns could be an important input parameter for atmospheric modeling applications. In the presented study, we therefore investigated the immersion freezing behavior of droplets containing size-segregated, monodisperse feldspar particles utilizing the Leipzig Aerosol Cloud Interaction Simulator (LACIS). For all particle sizes considered in the experiments, we observed a leveling off of the frozen droplet fraction reaching a plateau within the heterogeneous freezing temperature regime (T > -38°C) which was proportional to the particle surface area. Based on these findings, we could determine an asymptotic value for the <span class="hlt">ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19840019243','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19840019243"><span>Observations of sea <span class="hlt">ice</span> and icebergs from satellite radar altimeters</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rapley, C. G.</p> <p>1984-01-01</p> <p>Satellite radar altimeters can make useful contributions to the study of sea <span class="hlt">ice</span> both by enhancing observations from other instruments and by providing a unique probe of ocean-<span class="hlt">ice</span> interaction in the <span class="hlt">Marginal</span> <span class="hlt">Ice</span> Zone (MIZ). The problems, results and future potential of such observations are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22164468','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22164468"><span>[The economic <span class="hlt">margins</span> of <span class="hlt">activities</span> of a bovine practitioner on dairy farms].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>van Genugten, A J M; van Haaften, J A; Hogeveen, H</p> <p>2011-11-01</p> <p>Because of lower <span class="hlt">margins</span> and market liberalisation veterinarians and farmers are increasingly negotiating rates. Therefore, the <span class="hlt">margins</span> of veterinarians are under pressure. In addition, the sales if drugs, performance of operations or giving of advice are more and more separated. These developments give veterinarians uncertainty about the profitability of their <span class="hlt">activities</span> for dairy farmers. Not much is known about <span class="hlt">margins</span> on veterinary <span class="hlt">activities</span> on dairy farms. Moreover, it is interesting to see how much <span class="hlt">margins</span> of the bovine practitioner differ between veterinary practises and dairy farms. In this study, invoices for bovine <span class="hlt">activities</span> of 14 veterinary practises were combined with milk production registration data of the dairy farms of these practices. This way, the gross <span class="hlt">margin</span> per bovine practitioner could be studied for the different veterinary practise. Moreover the relation between gross <span class="hlt">margin</span> and specification of the veterinary practise could be studied. Finally, the gross <span class="hlt">margin</span> per dairy farm and the factors that influenced this gross <span class="hlt">margin</span> were studied. The most important result was the observation that the gross <span class="hlt">margin</span> per bovine practitioner was dependent on the number of dairy farms per practitioner, the <span class="hlt">margin</span> on drugs and the region of the veterinary practise. The size of the veterinary practise, the share of the dairy farming within the practise and the source of the gross <span class="hlt">margin</span> (drugs, time or operations) did not influence the gross <span class="hlt">margin</span>. Variables that explained the gross <span class="hlt">margin</span> per dairy farm were, amongst others, the number of dairy cows, the milk production level of the farms and participation in PIR-DAP (a system to support the veterinarians herd health and management program). There is no relation of gross <span class="hlt">margin</span> per dairy farm and the veterinary practise or region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21637255','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21637255"><span>A dynamic early East Antarctic <span class="hlt">Ice</span> Sheet suggested by <span class="hlt">ice</span>-covered fjord landscapes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>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</p> <p>2011-06-02</p> <p>The first Cenozoic <span class="hlt">ice</span> 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 <span class="hlt">ice</span>-sheet expansion to the continental <span class="hlt">margin</span>, 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. <span class="hlt">Ice</span>-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 <span class="hlt">ice</span>, 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 <span class="hlt">ice</span>-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 <span class="hlt">ice</span>-sheet configurations substantially different from today's. At different stages during its fluctuations, the edge of the East Antarctic <span class="hlt">Ice</span> Sheet lay pinned along the <span class="hlt">margins</span> 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.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930022698&hterms=HRV&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DHRV','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930022698&hterms=HRV&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DHRV"><span>SPOT satellite mapping of <span class="hlt">Ice</span> Stream B</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Merry, Carolyn J.</p> <p>1993-01-01</p> <p>Numerous features of glaciological significance appear on two adjoining SPOT High Resolution Visible (HRV) images that cover the onset region of <span class="hlt">ice</span> stream B. Many small-scale features, such as crevasses and drift plumes, have been previously observed in aerial photography. Subtle features, such as long flow traces that have not been mapped previously, are also clear in the satellite imagery. Newly discovered features include ladder-like runners and rungs within certain shear <span class="hlt">margins</span>, flow traces that are parallel to <span class="hlt">ice</span> flow, unusual crevasse patterns, and flow traces originating within shear <span class="hlt">margins</span>. An objective of our work is to contribute to an understanding of the genesis of the features observed in satellite imagery. The genetic possibilities for flow traces, other lineations, bands of transverse crevasses, shear <span class="hlt">margins</span>, mottles, and lumps and warps are described.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.C13B0432L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.C13B0432L"><span>Middle to late Holocene fluctuations of the Vindue glacier, an outlet glacier of the Greenland <span class="hlt">Ice</span> Sheet, central East Greenland.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Levy, L.; Hammer, S. K.; Kelly, M. A.; Lowell, T. V.; Hall, B. L.; Howley, J. A.; Wilcox, P.; Medford, A.</p> <p>2014-12-01</p> <p>The <span class="hlt">margins</span> of the Greenland <span class="hlt">Ice</span> Sheet are currently responding to present-day climate changes. Determining how the <span class="hlt">ice</span> sheet <span class="hlt">margins</span> have responded to past climate changes provides a means to understand how they may respond in the future. Here we present a multi-proxy record used to reconstruct the Holocene fluctuations of the Vindue glacier, an <span class="hlt">ice</span> sheet outlet glacier in eastern Greenland. Lake sediment cores from Qiviut lake (informal name), located ~0.75 km from the present-day Vindue glacier <span class="hlt">margin</span> contain a sharp transition from medium sand/coarse silt to laminated gyttja just prior to 6,340±130 cal yr BP. We interpret this transition to indicate a time when the Vindue glacier retreated sufficiently to cease glacial sedimentation into the lake basin. Above this contact the core contains laminated gyttja with prominent, ~0.5 cm thick, silt layers. 10Be ages of boulders on bedrock located between Qiviut lake and the present-day <span class="hlt">ice</span> <span class="hlt">margin</span> date to 6.81 ± 0.67 ka (n = 3), indicating the time of deglaciation. These ages also agree well with the radiocarbon age of the silt-gyttja transition in Qiviut lake cores. 10Be ages on boulders on bedrock located more proximal to the <span class="hlt">ice</span> <span class="hlt">margin</span> (~0.5 km) yield ages of 2.67 ± 0.18 ka (n = 2). These ages indicate either the continued recession of the <span class="hlt">ice</span> <span class="hlt">margin</span> during the late Holocene or an advance at this time. Boulders on the historical moraines show that <span class="hlt">ice</span> retreated from the moraine by AD 1620 ± 20 yrs (n = 2). These results are in contrast with some areas of the western <span class="hlt">margin</span> of the <span class="hlt">ice</span> sheet where 10Be ages indicate that the <span class="hlt">ice</span> sheet was behind its Historical limit from the middle Holocene (~6-7 ka) to Historical time. This may indicate that the eastern <span class="hlt">margin</span> may have responded to late Holocene cooling more sensitively or that the advance associated with the Historical moraines overran any evidence of late Holocene fluctuations along the western <span class="hlt">margin</span> of the <span class="hlt">ice</span> sheet.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70037436','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70037436"><span>Geochronology and paleoclimatic implications of the last deglaciation of the Mauna Kea <span class="hlt">Ice</span> Cap, Hawaii</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Anslow, Faron S.; Clark, P.U.; Kurz, M.D.; Hostetler, S.W.</p> <p>2010-01-01</p> <p>We present new 3He surface exposure ages on moraines and bedrock near the summit of Mauna Kea, Hawaii, which refine the age of the Mauna Kea <span class="hlt">Ice</span> Cap during the Local Last Glacial Maximum (LLGM) and identify a subsequent fluctuation of the <span class="hlt">ice</span> <span class="hlt">margin</span>. The 3He ages, when combined with those reported previously, indicate that the local <span class="hlt">ice</span>-cap <span class="hlt">margin</span> began to retreat from its LLGM extent at 20.5??2.5ka, in agreement with the age of deglaciation determined from LLGM moraines elsewhere in the tropics. The <span class="hlt">ice</span>-cap <span class="hlt">margin</span> receded to a position at least 3km upslope for ~4.5-5.0kyr before readvancing nearly to its LLGM extent. The timing of this readvance at ~15.4ka corresponds to a large reduction of the Atlantic meridional overturning circulation (AMOC) following Heinrich Event 1. Subsequent <span class="hlt">ice-margin</span> retreat began at 14.6??1.9ka, corresponding to a rapid resumption of the AMOC and onset of the B??lling warm interval, with the <span class="hlt">ice</span> cap melting rapidly to complete deglaciation. Additional 3He ages obtained from a flood deposit date the catastrophic outburst of a moraine-dammed lake roughly coeval with the Younger Dryas cold interval, suggesting a more <span class="hlt">active</span> hydrological cycle on Mauna Kea at this time. A coupled mass balance and <span class="hlt">ice</span> dynamics model is used to constrain the climate required to generate <span class="hlt">ice</span> caps of LLGM and readvance sizes. The depression of the LLGM equilibrium line altitude requires atmospheric cooling of 4.5??1??C, whereas the mass balance modeling indicates an accompanying increase in precipitation of as much as three times that of present. We hypothesize (1) that the LLGM temperature depression was associated with global cooling, (2) that the temperature depression that contributed to the readvance occurred in response to an atmospheric teleconnection to the North Atlantic, and (3) that the precipitation enhancement associated with both events occurred in response to a southward shift in the position of the inter-tropical convergence zone (ITCZ). Such a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1993EOSTr..74..225M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1993EOSTr..74..225M"><span>Polar continental <span class="hlt">margins</span>: Studies off East Greenland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mienert, J.; Thiede, J.; Kenyon, N. H.; Hollender, F.-J.</p> <p></p> <p>The passive continental <span class="hlt">margin</span> off east Greenland has been shaped by tectonic and sedimentary processes, and typical physiographic patterns have evolved over the past few million years under the influence of the late Cenozoic Northern Hemisphere glaciations. The Greenland <span class="hlt">ice</span> shield has been particularly affected.GLORIA (Geological Long Range Inclined Asdic), the Institute of Oceanographic Sciences' (IOS) long-range, side-scan sonar, was used on a 1992 RV Livonia cruise to map large-scale changes in sedimentary patterns along the east Greenland continental <span class="hlt">margin</span>. The overall objective of this research program was to determine the variety of large-scale seafloor processes to improve our understanding of the interaction between <span class="hlt">ice</span> sheets, current regimes, and sedimentary processes. In cooperation with IOS and the RV Livonia, a high-quality set of seafloor data has been produced. GLORIA'S first survey of east Greenland's continental <span class="hlt">margin</span> covered several 1000- × 50-km-wide swaths (Figure 1) and yielded an impressive sidescan sonar image of the complete Greenland Basin and <span class="hlt">margin</span> (about 250,000 km2). A mosaic of the data was made at a scale of 1:375,000. The base map was prepared with a polar stereographic projection having a standard parallel of 71°.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1813422S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1813422S"><span><span class="hlt">Ice</span> Nucleation <span class="hlt">Activity</span> of Various Agricultural Soil Dust Aerosol Particles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schiebel, Thea; Höhler, Kristina; Funk, Roger; Hill, Thomas C. J.; Levin, Ezra J. T.; Nadolny, Jens; Steinke, Isabelle; Suski, Kaitlyn J.; Ullrich, Romy; Wagner, Robert; Weber, Ines; DeMott, Paul J.; Möhler, Ottmar</p> <p>2016-04-01</p> <p>Recent investigations at the cloud simulation chamber AIDA (Aerosol Interactions and Dynamics in the Atmosphere) suggest that agricultural soil dust has an <span class="hlt">ice</span> nucleation ability that is enhanced up to a factor of 10 compared to desert dust, especially at temperatures above -26 °C (Steinke et al., in preparation for submission). This enhancement might be caused by the contribution of very <span class="hlt">ice-active</span> biological particles. In addition, soil dust aerosol particles often contain a considerably higher amount of organic matter compared to desert dust particles. To test agricultural soil dust as a source of <span class="hlt">ice</span> nucleating particles, especially for <span class="hlt">ice</span> formation in warm clouds, we conducted a series of laboratory measurements with different soil dust samples to extend the existing AIDA dataset. The AIDA has a volume of 84 m3 and operates under atmospherically relevant conditions over wide ranges of temperature, pressure and humidity. By controlled adiabatic expansions, the ascent of an air parcel in the troposphere can be simulated. As a supplement to the AIDA facility, we use the INKA (<span class="hlt">Ice</span> Nucleation Instrument of the KArlsruhe Institute of Technology) continuous flow diffusion chamber based on the design by Rogers (1988) to expose the sampled aerosol particles to a continuously increasing saturation ratio by keeping the aerosol temperature constant. For our experiments, soil dust was dry dispersed into the AIDA vessel. First, fast saturation ratio scans at different temperatures were performed with INKA, sampling soil dust aerosol particles directly from the AIDA vessel. Then, we conducted the AIDA expansion experiment starting at a preset temperature. The combination of these two different methods provides a robust data set on the temperature-dependent <span class="hlt">ice</span> <span class="hlt">activity</span> of various agriculture soil dust aerosol particles with a special focus on relatively high temperatures. In addition, to extend the data set, we investigated the role of biological and organic matter in more</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DyAtO..79...10S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DyAtO..79...10S"><span>Sensitivity of open-water <span class="hlt">ice</span> growth and <span class="hlt">ice</span> concentration evolution in a coupled atmosphere-ocean-sea <span class="hlt">ice</span> model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shi, Xiaoxu; Lohmann, Gerrit</p> <p>2017-09-01</p> <p>A coupled atmosphere-ocean-sea <span class="hlt">ice</span> model is applied to investigate to what degree the area-thickness distribution of new <span class="hlt">ice</span> formed in open water affects the <span class="hlt">ice</span> and ocean properties. Two sensitivity experiments are performed which modify the horizontal-to-vertical aspect ratio of open-water <span class="hlt">ice</span> growth. The resulting changes in the Arctic sea-<span class="hlt">ice</span> concentration strongly affect the surface albedo, the ocean heat release to the atmosphere, and the sea-<span class="hlt">ice</span> production. The changes are further amplified through a positive feedback mechanism among the Arctic sea <span class="hlt">ice</span>, the Atlantic Meridional Overturning Circulation (AMOC), and the surface air temperature in the Arctic, as the Fram Strait sea <span class="hlt">ice</span> import influences the freshwater budget in the North Atlantic Ocean. Anomalies in sea-<span class="hlt">ice</span> transport lead to changes in sea surface properties of the North Atlantic and the strength of AMOC. For the Southern Ocean, the most pronounced change is a warming along the Antarctic Circumpolar Current (ACC), owing to the interhemispheric bipolar seasaw linked to AMOC weakening. Another insight of this study lies on the improvement of our climate model. The ocean component FESOM is a newly developed ocean-sea <span class="hlt">ice</span> model with an unstructured mesh and multi-resolution. We find that the subpolar sea-<span class="hlt">ice</span> boundary in the Northern Hemisphere can be improved by tuning the process of open-water <span class="hlt">ice</span> growth, which strongly influences the sea <span class="hlt">ice</span> concentration in the <span class="hlt">marginal</span> <span class="hlt">ice</span> zone, the North Atlantic circulation, salinity and Arctic sea <span class="hlt">ice</span> volume. Since the distribution of new <span class="hlt">ice</span> on open water relies on many uncertain parameters and the knowledge of the detailed processes is currently too crude, it is a challenge to implement the processes realistically into models. Based on our sensitivity experiments, we conclude a pronounced uncertainty related to open-water sea <span class="hlt">ice</span> growth which could significantly affect the climate system sensitivity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5688310-asynchronous-ice-lobe-retreat-glacial-lake-bascom-deglaciation-hoosic-vermont-valleys-southwestern-vermont','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5688310-asynchronous-ice-lobe-retreat-glacial-lake-bascom-deglaciation-hoosic-vermont-valleys-southwestern-vermont"><span>Asynchronous <span class="hlt">ice</span> lobe retreat and glacial Lake Bascom: Deglaciation of the Hoosic and Vermont valleys, southwestern Vermont</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>Small, E.; Desimone, D.</p> <p></p> <p>Deglaciation of the Hoosic River drainage basin in southwestern Vermont was more complex than previously described. Detailed surficial mapping, stratigraphic relationships, and terrace levels/delta elevations reveal new details in the chronology of glacial Lake Bascom: (1) a pre-Wisconsinan proglacial lake was present in a similar position to Lake Bascom as <span class="hlt">ice</span> advanced: (2) the northern <span class="hlt">margin</span> of 275m (900 ft) glacial Lake Bascom extended 10 km up the Vermont Valley; (3) the 215m (705 ft) Bascom level was stable and long lived; (4) intermediate water planes existed between 215m and 190m (625 ft) levels; and (5) a separate <span class="hlt">ice</span> tonguemore » existed in Shaftsbury Hollow damming a small glacial lake, here named glacial Lake Emmons. This information is used to correlate <span class="hlt">ice</span> <span class="hlt">margins</span> to different lake levels. Distance of <span class="hlt">ice</span> <span class="hlt">margin</span> retreat during a lake level can be measured. Lake levels are then used as control points on a Lake Bascom relative time line to compare rate of retreat of different <span class="hlt">ice</span> tongues. Correlation of <span class="hlt">ice</span> <span class="hlt">margins</span> to Bascom levels indicates <span class="hlt">ice</span> retreat was asynchronous between nearby tongues in southwestern Vermont. The Vermont Valley <span class="hlt">ice</span> tongue retreated between two and four times faster than the Hoosic Valley tongue during the Bascom 275m level. Rate of retreat of the Vermont Valley tongue slowed to one-half of the Hoosic tongue during the 215m--190m lake levels. Factors responsible for varying rates of retreat are subglacial bedrock gradient, proximity to the Hudson-Champlain lobe, and the presence of absence of a calving <span class="hlt">margins</span>. Asynchronous retreat produced splayed <span class="hlt">ice</span> <span class="hlt">margins</span> in southwestern Vermont. Findings from this study do not support the model of parallel, synchronous retreat proposed by many workers for this region.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4882034','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4882034"><span><span class="hlt">Ice-Active</span> Substances from the Infective Juveniles of the Freeze Tolerant Entomopathogenic Nematode, Steinernema feltiae</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ali, Farman; Wharton, David A.</p> <p>2016-01-01</p> <p>Steinernema feltiae is a moderately freezing tolerant nematode, that can withstand intracellular <span class="hlt">ice</span> formation. We investigated recrystallization inhibition, thermal hysteresis and <span class="hlt">ice</span> nucleation <span class="hlt">activities</span> in the infective juveniles of S. feltiae. Both the splat cooling assay and optical recrystallometry indicate the presence of <span class="hlt">ice</span> <span class="hlt">active</span> substances that inhibit recrystallization in the nematode extract. The substance is relatively heat stable and largely retains the recrystallization inhibition <span class="hlt">activity</span> after heating. No thermal hysteresis <span class="hlt">activity</span> was detected but the extract had a typical hexagonal crystal shape when grown from a single seed crystal and weak <span class="hlt">ice</span> nucleation <span class="hlt">activity</span>. An <span class="hlt">ice</span> <span class="hlt">active</span> substance is present in a low concentration, which may be involved in the freezing survival of this species by inhibiting <span class="hlt">ice</span> recrystallization. PMID:27227961</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27227961','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27227961"><span><span class="hlt">Ice-Active</span> Substances from the Infective Juveniles of the Freeze Tolerant Entomopathogenic Nematode, Steinernema feltiae.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ali, Farman; Wharton, David A</p> <p>2016-01-01</p> <p>Steinernema feltiae is a moderately freezing tolerant nematode, that can withstand intracellular <span class="hlt">ice</span> formation. We investigated recrystallization inhibition, thermal hysteresis and <span class="hlt">ice</span> nucleation <span class="hlt">activities</span> in the infective juveniles of S. feltiae. Both the splat cooling assay and optical recrystallometry indicate the presence of <span class="hlt">ice</span> <span class="hlt">active</span> substances that inhibit recrystallization in the nematode extract. The substance is relatively heat stable and largely retains the recrystallization inhibition <span class="hlt">activity</span> after heating. No thermal hysteresis <span class="hlt">activity</span> was detected but the extract had a typical hexagonal crystal shape when grown from a single seed crystal and weak <span class="hlt">ice</span> nucleation <span class="hlt">activity</span>. An <span class="hlt">ice</span> <span class="hlt">active</span> substance is present in a low concentration, which may be involved in the freezing survival of this species by inhibiting <span class="hlt">ice</span> recrystallization.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28715207','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28715207"><span>Antifreeze Protein Mimetic Metallohelices with Potent <span class="hlt">Ice</span> Recrystallization Inhibition <span class="hlt">Activity</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mitchell, Daniel E; Clarkson, Guy; Fox, David J; Vipond, Rebecca A; Scott, Peter; Gibson, Matthew I</p> <p>2017-07-26</p> <p>Antifreeze proteins are produced by extremophile species to control <span class="hlt">ice</span> formation and growth, and they have potential applications in many fields. There are few examples of synthetic materials which can reproduce their potent <span class="hlt">ice</span> recrystallization inhibition property. We report that self-assembled enantiomerically pure, amphipathic metallohelicies inhibited <span class="hlt">ice</span> growth at just 20 μM. Structure-property relationships and calculations support the hypothesis that amphipathicity is the key motif for <span class="hlt">activity</span>. This opens up a new field of metallo-organic antifreeze protein mimetics and provides insight into the origins of <span class="hlt">ice</span>-growth inhibition.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.C23B0656F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.C23B0656F"><span>An Imaging System capable of monitoring en-glacial and sub-glacial processes of glaciers, streaming <span class="hlt">ice</span> and <span class="hlt">ice</span> <span class="hlt">margins</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Frearson, N.</p> <p>2012-12-01</p> <p>Columbia University in New York is developing a geophysical instrumentation package that is capable of monitoring dynamic en-glacial and sub-glacial processes. The instruments include a Riegl Scanning Laser for precise measurements of the <span class="hlt">ice</span> surface elevation, Stereo photogrammetry from a high sensitivity (~20mK) Infra-Red camera and a high resolution Visible Imaging camera (2456 x 2058 pixels) to document fine scale <span class="hlt">ice</span> temperature changes and surface features, near surface <span class="hlt">ice</span> penetrating radar and an <span class="hlt">ice</span> depth measuring radar that can be used to study interior and basal processes of <span class="hlt">ice</span> shelves, glaciers, <span class="hlt">ice</span> streams and <span class="hlt">ice</span>-sheets. All instrument data sets will be time-tagged and geo-referenced using precision GPS satellite data. Aircraft orientation will be corrected using inertial measurement technology integrated into the pod. This instrumentation will be flown across some of the planets largest outlet glaciers in Antarctica and Greenland. However, a key aspect of the design is that at the conclusion of the program, the Pod, Deployment Arm, Data Acquisition and Power and Environmental Management system will become available for use by the science community at large to install their own instruments onto. It will also be possible to mount the Icepod onto other airframes. The sensor system will become part of a research facility operated for the science community, and data will be maintained at and made available through a Polar Data Center.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19920040056&hterms=data+types&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Ddata%2Btypes','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19920040056&hterms=data+types&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Ddata%2Btypes"><span>Effects of weather on the retrieval of sea <span class="hlt">ice</span> concentration and <span class="hlt">ice</span> type from passive microwave data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Maslanik, J. A.</p> <p>1992-01-01</p> <p>Effects of wind, water vapor, and cloud liquid water on <span class="hlt">ice</span> concentration and <span class="hlt">ice</span> type calculated from passive microwave data are assessed through radiative transfer calculations and observations. These weather effects can cause overestimates in <span class="hlt">ice</span> concentration and more substantial underestimates in multi-year <span class="hlt">ice</span> percentage by decreasing polarization and by decreasing the gradient between frequencies. The effect of surface temperature and air temperature on the magnitudes of weather-related errors is small for <span class="hlt">ice</span> concentration and substantial for multiyear <span class="hlt">ice</span> percentage. The existing weather filter in the NASA Team Algorithm addresses only weather effects over open ocean; the additional use of local open-ocean tie points and an alternative weather correction for the <span class="hlt">marginal</span> <span class="hlt">ice</span> zone can further reduce errors due to weather. <span class="hlt">Ice</span> concentrations calculated using 37 versus 18 GHz data show little difference in total <span class="hlt">ice</span> covered area, but greater differences in intermediate concentration classes. Given the magnitude of weather-related errors in <span class="hlt">ice</span> classification from passive microwave data, corrections for weather effects may be necessary to detect small trends in <span class="hlt">ice</span> covered area and <span class="hlt">ice</span> type for climate studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70019840','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70019840"><span>Southern Laurentide <span class="hlt">ice</span> lobes were created by <span class="hlt">ice</span> streams: Des Moines Lobe in Minnesota, USA</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Patterson, C.J.</p> <p>1997-01-01</p> <p>Regional mapping in southern Minnesota has illuminated a suite of landforms developed by the Des Moines Lobe that delimit the position of the lobe at its maximum and at lesser readvances. The <span class="hlt">ice</span> lobe repeatedly advanced, discharged its subglacial water, and subsequently stagnated. Recent glaciological research on Antarctic <span class="hlt">ice</span> streams has led some glacial geologists to postulate that <span class="hlt">ice</span> streams drained parts of the marine-based areas of the Laurentide <span class="hlt">Ice</span> Sheet. I postulate that such <span class="hlt">ice</span> streams may develop in land-based areas of an <span class="hlt">ice</span> sheet as well, and that the Des Moines Lobe, 200 km wide and 900 km long, was an outlet glacier of an <span class="hlt">ice</span> stream. It appears to have been able to advance beyond the Laurentide <span class="hlt">Ice</span> Sheet as long as adequate water pressure was maintained. However, the outer part of the lobe stagnated because subglacial water that facilitated the flow was able to drain away through tunnel valleys. Stagnation of the lobe is not equivalent to stoppage of the <span class="hlt">ice</span> stream, because <span class="hlt">ice</span> repeatedly advanced into and onto the stagnant <span class="hlt">margins</span>, stacking <span class="hlt">ice</span> and debris. Similar landforms are also seen in other lobes of the upper midwestern United States.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA151741','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA151741"><span><span class="hlt">Active</span> and Passive Remote Sensing of <span class="hlt">Ice</span>.</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1985-01-01</p> <p>This is a report on the progress that has been made in the study of <span class="hlt">active</span> and passive remote sensing of <span class="hlt">ice</span> during the period of August 1, 1984...<span class="hlt">active</span> and passive microwave remote sensing , (2) used the strong fluctuation theory and the fluctuation-dissipation theorem to calculate the brightness</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 lakes.</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 lakes 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 Lake Agassiz. Several large <span class="hlt">ice</span>-dammed lakes, 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 lakes was a significant reduction of <span class="hlt">ice</span> sheet melting at the southern <span class="hlt">margin</span> 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 lake-induced decreases in moisture and hence snowfall, such as has been reported earlier for Lake Agassiz. We conclude that the summer cooling mechanism from proglacial lakes 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('https://www.osti.gov/biblio/7246961-earthquakes-north-atlantic-passive-margins','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/7246961-earthquakes-north-atlantic-passive-margins"><span>Earthquakes at North Atlantic passive <span class="hlt">margins</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>Gregersen, S.; Basham, P.W.</p> <p>1989-01-01</p> <p>The main focus of this volume is the earthquakes that occur at and near the continental <span class="hlt">margins</span> on both sides of the North Atlantic. The book, which contains the proceedings of the NATO workshop on Causes and Effects of Earthquakes at Passive <span class="hlt">Margins</span> and in Areas of Postglacial Rebound on Both Sides of the North Atlantic, draws together the fields of geophysics, geology and geodesy to address the stress and strain in the Earth's crust. The resulting earthquakes produced on ancient geological fault zones and the associated seismic hazards these pose to man are also addressed. Postglacial rebound in Northmore » America and Fennoscandia is a minor source of earthquakes today, during the interglacial period, but evidence is presented to suggest that the <span class="hlt">ice</span> sheets suppressed earthquake strain while they were in place, and released this strain as a pulse of significant earthquakes after the <span class="hlt">ice</span> melted about 9000 years ago.« 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_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_12 --> <div id="page_13" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="241"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170011211','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170011211"><span><span class="hlt">Ice</span> Crystal <span class="hlt">Icing</span> Research at NASA</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Flegel, Ashlie B.</p> <p>2017-01-01</p> <p><span class="hlt">Ice</span> crystals found at high altitude near convective clouds are known to cause jet engine power-loss events. These events occur due to <span class="hlt">ice</span> crystals entering a propulsion system's core flowpath and accreting <span class="hlt">ice</span> resulting in events such as uncommanded loss of thrust (rollback), engine stall, surge, and damage due to <span class="hlt">ice</span> shedding. As part of a community with a growing need to understand the underlying physics of <span class="hlt">ice</span> crystal <span class="hlt">icing</span>, NASA has been performing experimental efforts aimed at providing datasets that can be used to generate models to predict the <span class="hlt">ice</span> accretion inside current and future engine designs. Fundamental <span class="hlt">icing</span> physics studies on particle impacts, accretion on a single airfoil, and <span class="hlt">ice</span> accretions observed during a rollback event inside a full-scale engine in the Propulsion Systems Laboratory are summarized. Low fidelity code development using the results from the engine tests which identify key parameters for <span class="hlt">ice</span> accretion risk and the development of high fidelity codes are described. These <span class="hlt">activities</span> have been conducted internal to NASA and through collaboration efforts with industry, academia, and other government agencies. The details of the research <span class="hlt">activities</span> and progress made to date in addressing <span class="hlt">ice</span> crystal <span class="hlt">icing</span> research challenges are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170006539','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170006539"><span><span class="hlt">Ice</span> Crystal <span class="hlt">Icing</span> Research at NASA</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Flegel, Ashlie B.</p> <p>2017-01-01</p> <p><span class="hlt">Ice</span> crystals found at high altitude near convective clouds are known to cause jet engine power-loss events. These events occur due to <span class="hlt">ice</span> crystals entering a propulsion systems core flowpath and accreting <span class="hlt">ice</span> resulting in events such as uncommanded loss of thrust (rollback), engine stall, surge, and damage due to <span class="hlt">ice</span> shedding. As part of a community with a growing need to understand the underlying physics of <span class="hlt">ice</span> crystal <span class="hlt">icing</span>, NASA has been performing experimental efforts aimed at providing datasets that can be used to generate models to predict the <span class="hlt">ice</span> accretion inside current and future engine designs. Fundamental <span class="hlt">icing</span> physics studies on particle impacts, accretion on a single airfoil, and <span class="hlt">ice</span> accretions observed during a rollback event inside a full-scale engine in the Propulsion Systems Laboratory are summarized. Low fidelity code development using the results from the engine tests which identify key parameters for <span class="hlt">ice</span> accretion risk and the development of high fidelity codes are described. These <span class="hlt">activities</span> have been conducted internal to NASA and through collaboration efforts with industry, academia, and other government agencies. The details of the research <span class="hlt">activities</span> and progress made to date in addressing <span class="hlt">ice</span> crystal <span class="hlt">icing</span> research challenges are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ISPAr42W7.1585Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ISPAr42W7.1585Z"><span><span class="hlt">Ice</span> Water Classification Using Statistical Distribution Based Conditional Random Fields in RADARSAT-2 Dual Polarization Imagery</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Y.; Li, F.; Zhang, S.; Hao, W.; Zhu, T.; Yuan, L.; Xiao, F.</p> <p>2017-09-01</p> <p>In this paper, Statistical Distribution based Conditional Random Fields (STA-CRF) algorithm is exploited for improving <span class="hlt">marginal</span> <span class="hlt">ice</span>-water classification. Pixel level <span class="hlt">ice</span> concentration is presented as the comparison of methods based on CRF. Furthermore, in order to explore the effective statistical distribution model to be integrated into STA-CRF, five statistical distribution models are investigated. The STA-CRF methods are tested on 2 scenes around Prydz Bay and Adélie Depression, where contain a variety of <span class="hlt">ice</span> types during melt season. Experimental results indicate that the proposed method can resolve sea <span class="hlt">ice</span> edge well in <span class="hlt">Marginal</span> <span class="hlt">Ice</span> Zone (MIZ) and show a robust distinction of <span class="hlt">ice</span> and water.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRD..12113559S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRD..12113559S"><span><span class="hlt">Ice</span> nucleation <span class="hlt">activity</span> of agricultural soil dust aerosols from Mongolia, Argentina, and Germany</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Steinke, I.; Funk, R.; Busse, J.; Iturri, A.; Kirchen, S.; Leue, M.; Möhler, O.; Schwartz, T.; Schnaiter, M.; Sierau, B.; Toprak, E.; Ullrich, R.; Ulrich, A.; Hoose, C.; Leisner, T.</p> <p>2016-11-01</p> <p>Soil dust particles emitted from agricultural areas contain considerable mass fractions of organic material. Also, soil dust particles may act as carriers for potentially <span class="hlt">ice-active</span> biological particles. In this work, we present <span class="hlt">ice</span> nucleation experiments conducted in the Aerosol Interaction and Dynamics in the Atmosphere (AIDA) cloud chamber. We investigated the <span class="hlt">ice</span> nucleation efficiency of four types of soil dust from different regions of the world. The results are expressed as <span class="hlt">ice</span> nucleation <span class="hlt">active</span> surface site (INAS) densities and presented for the immersion freezing and the deposition nucleation mode. For immersion freezing occurring at 254 K, samples from Argentina, China, and Germany show <span class="hlt">ice</span> nucleation efficiencies which are by a factor of 10 higher than desert dusts. On average, the difference in <span class="hlt">ice</span> nucleation efficiencies between agricultural and desert dusts becomes significantly smaller at temperatures below 247 K. In the deposition mode the soil dusts showed higher <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> than Arizona Test Dust over a temperature range between 232 and 248 K and humidities RHice up to 125%. INAS densities varied between 109 and 1011 m-2 for these thermodynamic conditions. For one soil dust sample (Argentinian Soil), the effect of treatments with heat was investigated. Heat treatments (383 K) did not affect the <span class="hlt">ice</span> nucleation efficiency observed at 249 K. This finding presumably excludes proteinaceous <span class="hlt">ice</span>-nucleating entities as the only source of the increased <span class="hlt">ice</span> nucleation efficiency.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.C11E0714W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.C11E0714W"><span>The Influence of Subglacial Hydrology on <span class="hlt">Ice</span> Stream Velocity in a Physical Model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wagman, B. M.; Catania, G.; Buttles, J. L.</p> <p>2011-12-01</p> <p>We use a physical model to investigate how changes in subglacial hydrology affect <span class="hlt">ice</span> motion in <span class="hlt">ice</span> streams found in the West Antarctic <span class="hlt">Ice</span> Sheet. <span class="hlt">Ice</span> streams are modeled using silicone polymer placed over a thin water layer to simulate <span class="hlt">ice</span> flow dominated by basal sliding. Dynamic similarity between modeled and natural <span class="hlt">ice</span> streams is achieved through direct comparison of the glacier force balance using the conditions on Whillans <span class="hlt">Ice</span> Stream (WIS) as our goal.This <span class="hlt">ice</span> stream has a force balance that has evolved through time due to increased basal resistance. Currently, between 50-90% of the driving stress is supported by the <span class="hlt">ice</span> stream shear <span class="hlt">margins</span> [Stearns et al., JGlac 2005]. A similar force balance can be achieved in our model with a surface slope of 0.025. We test two hypotheses; 1) the distribution and thickness of the subglacial water layer influences the <span class="hlt">ice</span> flow speed and thus the force balance and can reproduce the observed slowdown of WIS and; 2) shear <span class="hlt">margins</span> are locations where transitions in water layer thickness occur.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.B54B..06M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.B54B..06M"><span>Microbial <span class="hlt">activity</span> in debris-rich basal <span class="hlt">ice</span>; adaption to sub-zero, saline conditions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Montross, S. N.; Skidmore, M. L.; Christner, B. C.; Griggs, R.; Tison, J.; Sowers, T. A.</p> <p>2011-12-01</p> <p>Polycrystalline <span class="hlt">ice</span> in glaciers and <span class="hlt">ice</span> sheets has a high preservation potential for biological material and chemical compounds that can be used to document the presence of <span class="hlt">active</span> microbial metabolism at sub-zero temperatures. The concentration and isotopic composition of gases, in conjunction with other aqueous chemical species in debris-rich basal glacier <span class="hlt">ice</span> from Taylor Glacier, Antarctica were used as direct evidence that cells entrained in the <span class="hlt">ice</span> remain metabolically <span class="hlt">active</span> at temperatures as low as -17°C, likely in thin films of liquid water along <span class="hlt">ice</span> crystal and mineral grain boundaries. δ18O2 and δ13CO2 values measured in the <span class="hlt">ice</span> are consistent with the hypothesis that abrupt changes measured in O2 and CO2 concentrations between debris-rich and debris-poor <span class="hlt">ice</span> are due to in situ microbial mineralization of organic carbon. Low temperature culture-based experiments conducted using organisms isolated from the <span class="hlt">ice</span> indicate the ability to respire organic carbon to CO2 under oxic conditions and under anoxic conditions couple carbon mineralization to dissimilatory iron reduction using Fe3+ as an electron acceptor. Microorganisms that are <span class="hlt">active</span> in the debris-rich basal <span class="hlt">ice</span> layers in terrestrial polar <span class="hlt">ice</span> masses need to be adapted to surviving subzero temperatures and saline conditions on extended timescales. Thus these terrestrial glacial systems and the isotopic and geochemical biomarkers therein provide good analogues for guiding exploration and analysis of debris-rich <span class="hlt">ices</span> in extraterrestrial settings, for example, on Mars.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1991JGR....96.6829M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1991JGR....96.6829M"><span>Unlocking the <span class="hlt">Ice</span> House: Oligocene-Miocene oxygen isotopes, eustasy, and <span class="hlt">margin</span> erosion</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Miller, Kenneth G.; Wright, James D.; Fairbanks, Richard G.</p> <p>1991-04-01</p> <p>Oxygen isotope records and glaciomarine sediments indicate at least an intermittent presence of large continental <span class="hlt">ice</span> sheets on Antarctica since the earliest Oligocene (circa 35 Ma). The growth and decay of <span class="hlt">ice</span> sheets during the Oligocene to modern "<span class="hlt">ice</span> house world" caused glacioeustatic sea level changes. The early Eocene was an <span class="hlt">ice</span>-free "greenhouse world," but it is not clear if <span class="hlt">ice</span> sheets existed during the middle to late Eocene "doubt house world." Benthic foraminiferal δ18O records place limits on the history of glaciation, suggesting the presence of <span class="hlt">ice</span> sheets at least intermittently since the earliest Oligocene. The best indicator of <span class="hlt">ice</span> growth is a coeval increase in global benthic and western equatorial planktonic δ18O records. Although planktonic isotope records from the western equatorial regions are limited, subtropical planktonic foraminifera may also record such <span class="hlt">ice</span> volume changes. It is difficult to apply these established principles to the Cenozoic δ18O record because of the lack of adequate data and problems in stratigraphic correlations that obscure isotope events. We improved Oligocene to Miocene correlations of δ18O records and erected eight oxygen isotope zones (Oi1-Oi2, Mi1-Mi6). Benthic foraminiferal δ18O increases which are associated with the bases of Zones Oil (circa 35.8 Ma), Oi2 (circa 32.5 Ma), and Mil (circa 23.5 Ma) can be linked with δ18O increases in subtropical planktonic foraminifera and with intervals of glacial sedimentation on or near Antarctica. Our new correlations of middle Miocene benthic and western equatorial planktonic δ18O records show remarkable agreement in timing and amplitude. We interpret benthic-planktonic covariance to reflect substantial <span class="hlt">ice</span> volume increases near the bases of Zones Mi2 (circa 16.1 Ma), Mi3 (circa 13.6 Ma), and possibly Mi5 (circa 11.3 Ma). Possible glacioeustatic lowerings are associated with the δ18O increases which culminated with the bases of Zone Mi4 (circa 12.6 Ma) and Mi6 (circa 9</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.C11D0699A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.C11D0699A"><span>Programme for Monitoring of the Greenland <span class="hlt">Ice</span> Sheet - <span class="hlt">Ice</span> Surface Velocities</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Andersen, S. B.; Ahlstrom, A. P.; Boncori, J. M.; Dall, J.</p> <p>2011-12-01</p> <p>In 2007, the Danish Ministry of Climate and Energy launched the Programme for Monitoring of the Greenland <span class="hlt">Ice</span> Sheet (PROMICE) as an ongoing effort to assess changes in the mass budget of the Greenland <span class="hlt">Ice</span> Sheet. Iceberg calving from the outlet glaciers of the Greenland <span class="hlt">Ice</span> Sheet, often termed the <span class="hlt">ice</span>-dynamic mass loss, is responsible for an important part of the mass loss during the last decade. To quantify this part of the mass loss, we combine airborne surveys yielding <span class="hlt">ice</span>-sheet thickness along the entire <span class="hlt">margin</span>, with surface velocities derived from satellite synthetic-aperture radar (SAR). In order to derive <span class="hlt">ice</span> sheet surface velocities from SAR a processing chain has been developed for GEUS by DTU Space based on a commercial software package distributed by GAMMA Remote Sensing. The processor, named SUSIE (Scripts and Utilities for SAR <span class="hlt">Ice</span>-motion Estimation), can use both differential SAR interferometry and offset-tracking techniques to measure the horizontal velocity components, providing also an estimate of the corresponding measurement error. So far surface velocities have been derived for a number of sites including Nioghalvfjerdsfjord Glacier, the Kangerlussuaq region, the Nuuk region, Helheim Glacier and Daugaard-Jensen Glacier using data from ERS-1/ERS-2, ENVISAT ASAR and ALOS Palsar. Here we will present these first results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24190391','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24190391"><span>Bacterial <span class="hlt">activity</span> in sea <span class="hlt">ice</span> and open water of the Weddell Sea, Antarctica: A microautoradiographic study.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Grossmann, S</p> <p>1994-07-01</p> <p>Metabolic <span class="hlt">activity</span> of bacteria was investigated in open water, newly forming sea <span class="hlt">ice</span>, and successive stages of pack <span class="hlt">ice</span> in the Weddell Sea. Microautoradiography, using [(3)H]leucine as substrate, was compared with incorporation rates of [(3)H]leucine into proteins. Relation of [(3)H]leucine incorporation to the biomass of <span class="hlt">active</span> bacteria provides information about changes of specific metabolic <span class="hlt">activity</span> of cells. During a phytoplankton bloom in an <span class="hlt">ice</span>-free, stratified water column, total numbers of bacteria in the euphotic zone averaged 2.3 × 10(5) ml(-1), but only about 13% showed <span class="hlt">activity</span> via leucine uptake. Growth rate of the <span class="hlt">active</span> bacteria was estimated as 0.3-0.4 days(-1). Total cell concentration of bacteria in 400 m depth was 6.6 × 10(4) ml(-1). Nearly 50% of these cells were <span class="hlt">active</span>, although biomass production and specific growth rate were only about one-tenth that of the surface populations. When sea <span class="hlt">ice</span> was forming in high concentrations of phytoplankton, bacterial biomass in the newly formed <span class="hlt">ice</span> was 49.1 ng C ml(-1), exceeding that in open water by about one order of magnitude. Attachment of large bacteria to algal cells seems to cause their enrichment in the new <span class="hlt">ice</span>, since specific bacterial <span class="hlt">activity</span> was reduced during <span class="hlt">ice</span> formation, and enrichment of bacteria was not observed when <span class="hlt">ice</span> formed at low algal concentration. During growth of pack <span class="hlt">ice</span>, biomass of bacteria increased within the brine channel system. Specific <span class="hlt">activity</span> was still reduced at these later stages of <span class="hlt">ice</span> development, and percentages of <span class="hlt">active</span> cells were as low as 3-5%. In old, thick pack <span class="hlt">ice</span>, bacterial <span class="hlt">activity</span> was high and about 30% of cells were <span class="hlt">active</span>. However, biomass-specific <span class="hlt">activity</span> of bacteria remained significantly lower than that in open water. It is concluded that bacterial assemblages different to those of open water developed within the <span class="hlt">ice</span> and were dominated by bacteria with lower average metabolic <span class="hlt">activity</span> than those of <span class="hlt">ice</span>-free water.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22538614','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22538614"><span>Antarctic <span class="hlt">ice</span>-sheet loss driven by basal melting of <span class="hlt">ice</span> shelves.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pritchard, H D; Ligtenberg, S R M; Fricker, H A; Vaughan, D G; van den Broeke, M R; Padman, L</p> <p>2012-04-25</p> <p>Accurate prediction of global sea-level rise requires that we understand the cause of recent, widespread and intensifying glacier acceleration along Antarctic <span class="hlt">ice</span>-sheet coastal <span class="hlt">margins</span>. Atmospheric and oceanic forcing have the potential to reduce the thickness and extent of floating <span class="hlt">ice</span> shelves, potentially limiting their ability to buttress the flow of grounded tributary glaciers. Indeed, recent <span class="hlt">ice</span>-shelf collapse led to retreat and acceleration of several glaciers on the Antarctic Peninsula. But the extent and magnitude of <span class="hlt">ice</span>-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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span>-shelf thinning through increased basal melt. We deduce that this increased melt is the primary control of Antarctic <span class="hlt">ice</span>-sheet loss, through a reduction in buttressing of the adjacent <span class="hlt">ice</span> sheet leading to accelerated glacier flow. The highest thinning rates occur where warm water at depth can access thick <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span>-sheet mass balance, and hence global sea level, on annual to decadal timescales.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1026542','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1026542"><span>Ocean Profile Measurements During the Seasonal <span class="hlt">Ice</span> Zone Reconnaissance Surveys Ocean Profiles</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2017-01-01</p> <p>repeated ocean, <span class="hlt">ice</span>, and atmospheric measurements across the Beaufort-Chukchi sea seasonal sea <span class="hlt">ice</span> zone (SIZ) utilizing US Coast Guard Arctic Domain...contributing to the rapid decline in summer <span class="hlt">ice</span> extent that has occurred in recent years. The SIZ is the region between maximum winter sea <span class="hlt">ice</span> extent and...minimum summer sea <span class="hlt">ice</span> extent. As such, it contains the full range of positions of the <span class="hlt">marginal</span> <span class="hlt">ice</span> zone (MIZ) where sea <span class="hlt">ice</span> interacts with open water</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.B33K0614C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.B33K0614C"><span>Carbon and hydrogen isotopic systematics of dissolved methane in small seasonally <span class="hlt">ice</span>-covered lakes near the <span class="hlt">margin</span> of the Greenland <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>Cadieux, S. B.; White, J. R.; Pratt, L. M.; Peng, Y.; Young, S. A.</p> <p>2013-12-01</p> <p>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 <span class="hlt">ice</span>-free conditions have been conducted in Alaskan, Swedish and Siberian lakes. However, there is little information on CH4 cycling under <span class="hlt">ice</span>-covered conditions, and few stable isotopic measurements, which can help elucidate production and consumption pathways. In order to better understand methane dynamics of <span class="hlt">ice</span>-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 <span class="hlt">ice</span>-cover. Lakes in the study area are <span class="hlt">ice</span>-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 <span class="hlt">ice</span>, 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 <span class="hlt">ice</span> 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 <span class="hlt">activity</span>. 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</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018RvGeo..56..142P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018RvGeo..56..142P"><span>Ocean Tide Influences on the Antarctic and Greenland <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>Padman, Laurie; Siegfried, Matthew R.; Fricker, Helen A.</p> <p>2018-03-01</p> <p>Ocean tides are the main source of high-frequency variability in the vertical and horizontal motion of <span class="hlt">ice</span> sheets near their marine <span class="hlt">margins</span>. Floating <span class="hlt">ice</span> shelves, which occupy about three quarters of the perimeter of Antarctica and the termini of four outlet glaciers in northern Greenland, rise and fall in synchrony with the ocean tide. Lateral motion of floating and grounded portions of <span class="hlt">ice</span> sheets near their marine <span class="hlt">margins</span> can also include a tidal component. These tide-induced signals provide insight into the processes by which the oceans can affect <span class="hlt">ice</span> sheet mass balance and dynamics. In this review, we summarize in situ and satellite-based measurements of the tidal response of <span class="hlt">ice</span> shelves and grounded <span class="hlt">ice</span>, and spatial variability of ocean tide heights and currents around the <span class="hlt">ice</span> sheets. We review sensitivity of tide heights and currents as ocean geometry responds to variations in sea level, <span class="hlt">ice</span> shelf thickness, and <span class="hlt">ice</span> sheet mass and extent. We then describe coupled <span class="hlt">ice</span>-ocean models and analytical glacier models that quantify the effect of ocean tides on lower-frequency <span class="hlt">ice</span> sheet mass loss and motion. We suggest new observations and model developments to improve the representation of tides in coupled models that are used to predict future <span class="hlt">ice</span> sheet mass loss and the associated contribution to sea level change. The most critical need is for new data to improve maps of bathymetry, <span class="hlt">ice</span> shelf draft, spatial variability of the drag coefficient at the <span class="hlt">ice</span>-ocean interface, and higher-resolution models with improved representation of tidal energy sinks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20100028441&hterms=hydrate&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dhydrate','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20100028441&hterms=hydrate&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dhydrate"><span>One-Hundred-km-Scale Basins on Enceladus: Evidence for an <span class="hlt">Active</span> <span class="hlt">Ice</span> Shell</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Schenk, Paul M.; McKinnon, William B.</p> <p>2009-01-01</p> <p>Stereo-derived topographic mapping of 50% of Enceladus reveals at least 6 large-scale, ovoid depressions (basins) 90-175 km across and 800-to-1500 m deep and uncorrelated with geologic boundaries. Their shape and scale are inconsistent with impact, geoid deflection, or with dynamically supported topography. Isostatic thinning of Enceladus <span class="hlt">ice</span> shell associated with upwellings (and tidally-driven <span class="hlt">ice</span> melting) can plausibly account for the basins. Thinning implies upwarping of the base of the shell of 10-20 km beneath the depressions, depending on total shell thickness; loss of near-surface porosity due to enhanced heat flow may also contribute to basin lows. Alternatively, the basins may overly cold, inactive, and hence denser <span class="hlt">ice</span>, but thermal isostasy alone requires thermal expansion more consistent with clathrate hydrate than water <span class="hlt">ice</span>. In contrast to the basins, the south polar depression (SPD) is larger (350 wide) and shallower (0.4-to-0.8 km deep) and correlates with the area of tectonic deformation and <span class="hlt">active</span> resurfacing. The SPD also differs in that the floor is relatively flat (i.e., conforms roughly to the global triaxial shape, or geoid) with broad, gently sloping flanks. The relative flatness across the SPD suggests that it is in or near isostatic equilibrium, and underlain by denser material, supporting the polar sea hypothesis of Collins and Goodman. Near flatness is also predicted by a crustal spreading origin for the "tiger stripes (McKinnon and Barr 2007, Barr 2008); the extraordinary, high CIRS heat flows imply half-spreading rates in excess of 10 cm/yr, a very young surface age (250,000 yr), and a rather thin lithosphere (hence modest thermal topography). Topographic rises in places along the outer <span class="hlt">margin</span> of the SPD correlate with parallel ridges and deformation along the edge of the resurfaced terrain, consistent with a compressional, imbricate thrust origin for these ridges, driven by the spreading.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1710208L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1710208L"><span>Identification and quantification of <span class="hlt">ice</span> nucleation <span class="hlt">active</span> microorganisms by digital droplet PCR (ddPCR)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Linden, Martin; Pöschl, Ulrich; Fröhlich-Nowoisky, Janine</p> <p>2015-04-01</p> <p>Several bioaerosol types, including bacteria, fungi, pollen and lichen, have been identified as sources of biological <span class="hlt">ice</span> nucleators (IN) which induce <span class="hlt">ice</span> formation already at temperatures as high as -10 °C or above. Accordingly, they potentially contribute widely to environmental <span class="hlt">ice</span> nucleation in the atmosphere and are of great interest in the study of natural heterogenous <span class="hlt">ice</span> nucleation processes. <span class="hlt">Ice</span> nucleation <span class="hlt">active</span> microorganisms have been found and studied among bacteria (Proteobacteria) and fungi (phyla Basidiomycota and Ascomycota). The mechanisms enabling the microorganisms to <span class="hlt">ice</span> nucleation are subject to ongoing research. While it has been demonstrated that whole cells can act as <span class="hlt">ice</span> nucleators in the case of bacteria due to the presence of specific membrane proteins, cell-free <span class="hlt">ice</span> nucleation <span class="hlt">active</span> particles seem to be responsible for this phenomenon in fungi and lichen. The identification and quantification of these <span class="hlt">ice</span> nucleation <span class="hlt">active</span> microorganisms and their IN in atmospheric samples is crucial to understand their contribution to the pool of atmospheric IN. This is not a trivial task since the respective microorganisms are often prevalent in lowest concentrations and a variety of states, be it viable cells, spores or cell debris from dead cells. Molecular biology provides tools to identify and quantify <span class="hlt">ice</span> nucleation <span class="hlt">active</span> microorganisms independent of their state by detecting genetic markers specific for the organism of interest. Those methods are not without their drawbacks in terms of sample material concentration required or reliable standardization. Digital Droplet Polymerase Chain Reaction (ddPCR) was chosen for our demands as a more elegant, quick and specific method in the investigation of <span class="hlt">ice</span> nucleation <span class="hlt">active</span> microorganisms in atmospheric samples. The advantages of ddPCR lie in the simultaneous detection and quantification of genetic markers and their original copy numbers in a sample. This is facilitated by the fractionation of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.9500M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.9500M"><span>The effects of sub-<span class="hlt">ice</span>-shelf melting on dense shelf water formation and export in idealized simulations of Antarctic <span class="hlt">margins</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marques, Gustavo; Stern, Alon; Harrison, Matthew; Sergienko, Olga; Hallberg, Robert</p> <p>2017-04-01</p> <p>Dense shelf water (DSW) is formed in coastal polynyas around Antarctica as a result of intense cooling and brine rejection. A fraction of this water reaches <span class="hlt">ice</span> shelves cavities and is modified due to interactions with sub-<span class="hlt">ice</span>-shelf melt water. This modified water mass contributes to the formation of Antarctic Bottom Water, and consequently, influences the large-scale ocean circulation. Here, we investigate the role of sub-<span class="hlt">ice</span>-shelf melting in the formation and export of DSW using idealized simulations with an isopycnal ocean model (MOM6) coupled with a sea <span class="hlt">ice</span> model (SIS2) and a thermodynamic <span class="hlt">active</span> <span class="hlt">ice</span> shelf. A set of experiments is conducted with variable horizontal grid resolutions (0.5, 1.0 and 2.0 km), <span class="hlt">ice</span> shelf geometries and atmospheric forcing. In all simulations DSW is spontaneously formed in coastal polynyas due to the combined effect of the imposed atmospheric forcing and the ocean state. Our results show that sub-<span class="hlt">ice</span>-shelf melting can significantly change the rate of dense shelf water outflows, highlighting the importance of this process to correctly represent bottom water formation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2000QuRes..53..285G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2000QuRes..53..285G"><span>Glacio-isostasy and Glacial <span class="hlt">Ice</span> Load at Law Dome, Wilkes Land, 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>Goodwin, Ian D.; Zweck, Christopher</p> <p>2000-05-01</p> <p>The Holocene sea-level high stand or "marine limit" in Wilkes Land, East Antarctica, reached ˜30 m above present sea level at a few dispersed sites. The most detailed marine limit data have been recorded for the Windmill Islands and Budd Coast at the <span class="hlt">margin</span> of the Law Dome <span class="hlt">ice</span> cap, a dome of the East Antarctic <span class="hlt">Ice</span> Sheet (EAIS). Relative sea-level lowering of 30 m and the associated emergence of the Windmill Islands have occurred since 6900 14C (corr.) yr B.P. Numerical modeling of the Earth's rheology is used to determine the glacio-isostatic component of the observed relative sea-level lowering. Glaciological evidence suggests that most of EAIS thickening occurred around its <span class="hlt">margin</span>, with expansion onto the continental shelf. Consequently, a regional <span class="hlt">ice</span> history for the last glacial maximum (LGM) was applied in the glacio-isostatic modeling to test whether the observed relative sea-level lowering was primarily produced by regional <span class="hlt">ice</span>-sheet changes. The results of the modeling indicate that the postglacial (13,000 to 8000 14C yr B.P) removal of an <span class="hlt">ice</span> load of between 770 and 1000 m from around the <span class="hlt">margin</span> of the Law Dome and adjacent EAIS have produced the observed relative sea-level lowering. Such an additional <span class="hlt">ice</span> load would have been associated with a 40- to 65-km expansion of the Law Dome to near the continental shelf break, together with a few hundred meters of <span class="hlt">ice</span> thickening on the adjoining coastal slope of the EAIS up to 2000 m elevation. Whereas the observed changes in relative sea level are shown to be strongly influenced by regional <span class="hlt">ice</span> sheet changes, the glacio-isostatic response at the Windmill Islands results from a combination of regional and, to a lesser extent, Antarctic-wide effects. The correspondence between the Holocene relative sea-level lowering interpreted at the <span class="hlt">margin</span> of the Law Dome and the lowering interpreted along the remainder of the Wilkes Land and Oates Land coasts (105°-160° E) suggests that a similar <span class="hlt">ice</span> load of up to 1000 m</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.B21F..01H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.B21F..01H"><span>Pedogenesis on <span class="hlt">ice</span> (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hodson, A. J.</p> <p>2010-12-01</p> <p>It is well known from <span class="hlt">ice</span> cores that organic and mineral debris accumulates within glacier <span class="hlt">ice</span> following atmospheric deposition. However, the concentrations of such debris are usually greatest upon the <span class="hlt">ice</span> surface, especially at the <span class="hlt">margins</span> of continental glaciers and <span class="hlt">ice</span> sheets, where it forms mm-scale aggregate particles called “cryoconite”. According to the literature, cryoconite covers about 2 % of the ablation areas of glaciers outside Greenland and Antarctica, equivalent to a mass loading of ca. 25 g/m2. Of the great <span class="hlt">ice</span> sheets not included in this figure, Greenland is the easiest to estimate, and new observations from the NE and SW sectors indicate mass loadings in the range 17 - 440 g/m2. Studies of cryoconite often report the presence of a significant biomass (usually 10^4 - 10^7 cells/g) that is capable of a wide range of biogeochemical functions. The first part of this presentation will therefore explore the contention that the formation of cryoconite represents the first stages of pedogenesis, resulting in the production of soil-type aggregates that inoculate glacial forefields following glacier retreat. Emphasis will be given to the relevant processes that result in aggregate formation, including rapid cell-mineral attachment within melting snowpacks and the slower, biological processes of cementation within thermodynamically stable habitats such as cryoconite holes. The second part of the presentation will use examples from Svalbard, Greenland and Antarctica to consider the carbon balance of the cryoconite during the longest phase of its life cycle: upon the <span class="hlt">ice</span>. It will be demonstrated how the efficacy of photosynthesis is strongly influenced by thermodynamic conditions at or near this surface. Data from the Greenland and Antarctic <span class="hlt">ice</span> sheets will show how thermal equilibration decouples variations in photosynthesis from variations in incident radiation over timescales > 1 d, resulting in an equitable, low-carbon economy for aggregates within</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008JGRF..113.2010F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008JGRF..113.2010F"><span>Mechanisms of basal <span class="hlt">ice</span> formation in polar glaciers: An evaluation of the apron entrainment model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fitzsimons, Sean; Webb, Nicola; Mager, Sarah; MacDonell, Shelley; Lorrain, Regi; Samyn, Denis</p> <p>2008-06-01</p> <p>Previous studies of polar glaciers have argued that basal <span class="hlt">ice</span> can form when these glaciers override and entrain <span class="hlt">ice</span> <span class="hlt">marginal</span> aprons that accumulate adjacent to steep <span class="hlt">ice</span> cliffs. To test this idea, we have studied the morphology, structure, composition, and deformation of the apron and basal <span class="hlt">ice</span> at the terminus of Victoria Upper Glacier in the McMurdo dry valleys, which are located on the western coast of the Ross Sea at 77°S in southern Victoria Land, Antarctica. Our results show that the apron has two structural elements: an inner element that consists of strongly foliated <span class="hlt">ice</span> that has a steep up-glacier dip, and an outer element that lacks a consistent foliation and has a down-glacier, slope-parallel dip. Although strain measurements show that the entire apron is deforming, the inner element is characterized by high strain rates, whereas relatively low rates of strain characterize the outer part of the apron. Co-isotopic analyses of the <span class="hlt">ice</span>, together with analysis of solute chemistry and sedimentary characteristics, show that the apron is compositionally different from the basal <span class="hlt">ice</span>. Our observations show that aprons may become deformed and partially entrained by advancing glaciers. However, such an <span class="hlt">ice</span> <span class="hlt">marginal</span> process does not provide a satisfactory explanation for the origin of basal <span class="hlt">ice</span> observed at the <span class="hlt">ice</span> <span class="hlt">margin</span>. Our interpretation of the origin of basal <span class="hlt">ice</span> is that it is formed by subglacial processes, which are likely to include deformation and entrainment of subglacial permafrost.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26709352','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26709352"><span>Abbot <span class="hlt">Ice</span> Shelf, structure of the Amundsen Sea continental <span class="hlt">margin</span> and the southern boundary of the Bellingshausen Plate seaward of West Antarctica.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cochran, James R; Tinto, Kirsty J; Bell, Robin E</p> <p>2015-05-01</p> <p>Inversion of NASA Operation <span class="hlt">Ice</span>Bridge airborne gravity over the Abbot <span class="hlt">Ice</span> Shelf in West Antarctica for subice bathymetry defines an extensional terrain made up of east-west trending rift basins formed during the early stages of Antarctica/Zealandia rifting. Extension is minor, as rifting jumped north of Thurston Island early in the rifting process. The Amundsen Sea Embayment continental shelf west of the rifted terrain is underlain by a deeper, more extensive sedimentary basin also formed during rifting between Antarctica and Zealandia. A well-defined boundary zone separates the mildly extended Abbot extensional terrain from the deeper Amundsen Embayment shelf basin. The shelf basin has an extension factor, β , of 1.5-1.7 with 80-100 km of extension occurring across an area now 250 km wide. Following this extension, rifting centered north of the present shelf edge and proceeded to continental rupture. Since then, the Amundsen Embayment continental shelf appears to have been tectonically quiescent and shaped by subsidence, sedimentation, and the advance and retreat of the West Antarctic <span class="hlt">Ice</span> Sheet. The Bellingshausen Plate was located seaward of the Amundsen Sea <span class="hlt">margin</span> prior to incorporation into the Antarctic Plate at about 62 Ma. During the latter part of its independent existence, Bellingshausen plate motion had a clockwise rotational component relative to Antarctica producing convergence across the north-south trending Bellingshausen Gravity Anomaly structure at 94°W and compressive deformation on the continental slope between 94°W and 102°W. Farther west, the relative motion was extensional along an east-west trending zone occupied by the Marie Byrd Seamounts. Abbot <span class="hlt">Ice</span> Shelf is underlain by E-W rift basins created at ∼90 Ma Amundsen shelf shaped by subsidence, sedimentation, and passage of the <span class="hlt">ice</span> sheet Bellingshausen plate boundary is located near the base of continental slope and rise.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_13 --> <div id="page_14" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="261"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4681458','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4681458"><span>Abbot <span class="hlt">Ice</span> Shelf, structure of the Amundsen Sea continental <span class="hlt">margin</span> and the southern boundary of the Bellingshausen Plate seaward of West Antarctica</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Cochran, James R; Tinto, Kirsty J; Bell, Robin E</p> <p>2015-01-01</p> <p>Inversion of NASA Operation <span class="hlt">Ice</span>Bridge airborne gravity over the Abbot <span class="hlt">Ice</span> Shelf in West Antarctica for subice bathymetry defines an extensional terrain made up of east-west trending rift basins formed during the early stages of Antarctica/Zealandia rifting. Extension is minor, as rifting jumped north of Thurston Island early in the rifting process. The Amundsen Sea Embayment continental shelf west of the rifted terrain is underlain by a deeper, more extensive sedimentary basin also formed during rifting between Antarctica and Zealandia. A well-defined boundary zone separates the mildly extended Abbot extensional terrain from the deeper Amundsen Embayment shelf basin. The shelf basin has an extension factor, β, of 1.5–1.7 with 80–100 km of extension occurring across an area now 250 km wide. Following this extension, rifting centered north of the present shelf edge and proceeded to continental rupture. Since then, the Amundsen Embayment continental shelf appears to have been tectonically quiescent and shaped by subsidence, sedimentation, and the advance and retreat of the West Antarctic <span class="hlt">Ice</span> Sheet. The Bellingshausen Plate was located seaward of the Amundsen Sea <span class="hlt">margin</span> prior to incorporation into the Antarctic Plate at about 62 Ma. During the latter part of its independent existence, Bellingshausen plate motion had a clockwise rotational component relative to Antarctica producing convergence across the north-south trending Bellingshausen Gravity Anomaly structure at 94°W and compressive deformation on the continental slope between 94°W and 102°W. Farther west, the relative motion was extensional along an east-west trending zone occupied by the Marie Byrd Seamounts. Key Points: Abbot <span class="hlt">Ice</span> Shelf is underlain by E-W rift basins created at ∼90 Ma Amundsen shelf shaped by subsidence, sedimentation, and passage of the <span class="hlt">ice</span> sheet Bellingshausen plate boundary is located near the base of continental slope and rise PMID:26709352</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26896764','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26896764"><span>Intermediate <span class="hlt">activity</span> of midge antifreeze protein is due to a tyrosine-rich <span class="hlt">ice</span>-binding site and atypical <span class="hlt">ice</span> plane affinity.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Basu, Koli; Wasserman, Samantha S; Jeronimo, Paul S; Graham, Laurie A; Davies, Peter L</p> <p>2016-04-01</p> <p>An antifreeze protein (AFP) from a midge (Chironomidae) was recently discovered and modelled as a tightly wound disulfide-braced solenoid with a surface-exposed rank of stacked tyrosines. New isoforms of the midge AFP have been identified from RT-PCR and are fully consistent with the model. Although they differ in the number of 10-residue coils, the row of tyrosines that form the putative <span class="hlt">ice</span>-binding site is conserved. Recombinant midge AFP has been produced, and the properly folded form purified by <span class="hlt">ice</span> affinity. This monomeric AFP has a distinct circular dichroism spectrum, a melting temperature between 35 and 50 °C and is fully renaturable on cooling. Mutagenesis of the middle tyrosine in the rank of seven eliminates antifreeze <span class="hlt">activity</span>, whereas mutation of a tyrosine off this predicted <span class="hlt">ice</span>-binding face had no such effect. This AFP has unusual properties compared to other known AFPs. First, its freezing-point depression <span class="hlt">activity</span> is intermediate between that of the hyperactive and moderately <span class="hlt">active</span> AFPs. As with hyperactive AFPs, when midge AFP-bound <span class="hlt">ice</span> crystals exceed their freezing-point depression, <span class="hlt">ice</span> grows explosively perpendicular to the c-axis. However, midge AFP does not bind to the basal plane of <span class="hlt">ice</span> as do hyperactive AFPs, but rather to a pyramidal plane that is at a shallower angle relative to the basal plane than binding planes of moderate AFPs. These properties distinguish midge AFP from all other <span class="hlt">ice</span>-binding proteins and the intermediate <span class="hlt">activity</span> level fits well to the modest challenge of protecting newly emerged adult insects from late spring frosts. Nucleotide sequences of new midge AFP isoforms are available in the GenBank database under accession numbers KU094814-8. Sequences will be released after publication. © 2016 Federation of European Biochemical Societies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.U53C..03T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.U53C..03T"><span>Whillans <span class="hlt">Ice</span> Stream Subglacial Access Research Drilling (WISSARD): Integrative Study of Marine <span class="hlt">Ice</span> Sheet Stability and Subglacial Life Habitats (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.; Anandakrishnan, S.; Behar, A. E.; Christner, B. C.; Fisher, A. T.; Fricker, H. A.; Holland, D. M.; Jacobel, R. W.; Mikucki, J.; Mitchell, A. C.; Powell, R. D.; Priscu, J. C.; Scherer, R. P.; Severinghaus, J. P.</p> <p>2009-12-01</p> <p>The WISSARD project is a large, NSF-funded, interdisciplinary initiative focused on scientific drilling, exploration, and investigation of Antarctic subglacial aquatic environments. The project consists of three interrelated components: (1) LISSARD - Lake and <span class="hlt">Ice</span> Stream Subglacial Access Research Drilling, (2) RAGES - Robotic Access to Grounding-zones for Exploration and Science, and (3) GBASE - GeomicroBiology of Antarctic Subglacial Environments). A number of previous studies in West Antarctica highlighted the importance of understanding <span class="hlt">ice</span> sheet interactions with water, either at the basal boundary where <span class="hlt">ice</span> streams come in contact with <span class="hlt">active</span> subglacial hydrologic and geological systems or at the marine <span class="hlt">margin</span> where the <span class="hlt">ice</span> sheet is exposed to forcing from the global ocean and sedimentation. Recent biological investigations of Antarctic subglacial environments show that they provide a significant habitat for life and source of bacterial carbon in a setting that was previously thought to be inhospitable. Subglacial microbial ecosystems also enhance biogeochemical weathering, mobilizing elements from long term geological storage. The overarching scientific objective of WISSARD is to examine the subglacial hydrological system of West Antarctica in glaciological, geological, microbiological, geochemical, and oceanographic contexts. Direct sampling will yield seminal information on these systems and test the overarching hypothesis that <span class="hlt">active</span> hydrological systems connect various subglacial environments and exert major control on <span class="hlt">ice</span> sheet dynamics, subglacial sediment transfer, geochemistry, metabolic and phylogenetic diversity, and biogeochemical transformations and geological records of <span class="hlt">ice</span> sheet history. Technological advances during WISSARD will provide the US-science community with a capability to access and study sub-<span class="hlt">ice</span> sheet environments. Developing this technological infrastructure will benefit the broader science community and it will be available for</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JGRC..120.8327H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JGRC..120.8327H"><span>Short-term sea <span class="hlt">ice</span> forecasting: An assessment of <span class="hlt">ice</span> concentration and <span class="hlt">ice</span> drift forecasts using the U.S. Navy's Arctic Cap Nowcast/Forecast System</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hebert, David A.; Allard, Richard A.; Metzger, E. Joseph; Posey, Pamela G.; Preller, Ruth H.; Wallcraft, Alan J.; Phelps, Michael W.; Smedstad, Ole Martin</p> <p>2015-12-01</p> <p>In this study the forecast skill of the U.S. Navy operational Arctic sea <span class="hlt">ice</span> forecast system, the Arctic Cap Nowcast/Forecast System (ACNFS), is presented for the period February 2014 to June 2015. ACNFS is designed to provide short term, 1-7 day forecasts of Arctic sea <span class="hlt">ice</span> and ocean conditions. Many quantities are forecast by ACNFS; the most commonly used include <span class="hlt">ice</span> concentration, <span class="hlt">ice</span> thickness, <span class="hlt">ice</span> velocity, sea surface temperature, sea surface salinity, and sea surface velocities. <span class="hlt">Ice</span> concentration forecast skill is compared to a persistent <span class="hlt">ice</span> state and historical sea <span class="hlt">ice</span> climatology. Skill scores are focused on areas where <span class="hlt">ice</span> concentration changes by ±5% or more, and are therefore limited to primarily the <span class="hlt">marginal</span> <span class="hlt">ice</span> zone. We demonstrate that ACNFS forecasts are skilful compared to assuming a persistent <span class="hlt">ice</span> state, especially beyond 24 h. ACNFS is also shown to be particularly skilful compared to a climatologic state for forecasts up to 102 h. Modeled <span class="hlt">ice</span> drift velocity is compared to observed buoy data from the International Arctic Buoy Programme. A seasonal bias is shown where ACNFS is slower than IABP velocity in the summer months and faster in the winter months. In February 2015, ACNFS began to assimilate a blended <span class="hlt">ice</span> concentration derived from Advanced Microwave Scanning Radiometer 2 (AMSR2) and the Interactive Multisensor Snow and <span class="hlt">Ice</span> Mapping System (IMS). Preliminary results show that assimilating AMSR2 blended with IMS improves the short-term forecast skill and <span class="hlt">ice</span> edge location compared to the independently derived National <span class="hlt">Ice</span> Center <span class="hlt">Ice</span> Edge product.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..44.7826N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..44.7826N"><span><span class="hlt">Ice</span> stream reorganization and glacial retreat on the northwest Greenland shelf</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Newton, A. M. W.; Knutz, P. C.; Huuse, M.; Gannon, P.; Brocklehurst, S. H.; Clausen, O. R.; Gong, Y.</p> <p>2017-08-01</p> <p>Understanding conditions at the grounding-line of marine-based <span class="hlt">ice</span> sheets is essential for understanding <span class="hlt">ice</span> sheet evolution. Offshore northwest Greenland, knowledge of the Last Glacial Maximum (LGM) <span class="hlt">ice</span> sheet extent in Melville Bugt was previously based on sparse geological evidence. This study uses multibeam bathymetry, combined with 2-D and 3-D seismic reflection data, to present a detailed landform record from Melville Bugt. Seabed landforms include mega-scale glacial lineations, grounding-zone wedges, iceberg scours, and a lateral shear <span class="hlt">margin</span> moraine, formed during the last glacial cycle. The geomorphology indicates that the LGM <span class="hlt">ice</span> sheet reached the shelf edge before undergoing flow reorganization. After retreat of 80 km across the outer shelf, the <span class="hlt">margin</span> stabilized in a mid-shelf position, possibly during the Younger Dryas (12.9-11.7 ka). The <span class="hlt">ice</span> sheet then decoupled from the seafloor and retreated to a coast-proximal position. This landform record provides an important constraint on deglaciation history offshore northwest Greenland.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014TCry....8.2409L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014TCry....8.2409L"><span><span class="hlt">Ice</span> and AIS: ship speed data and sea <span class="hlt">ice</span> forecasts in the Baltic Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Löptien, U.; Axell, L.</p> <p>2014-12-01</p> <p>The Baltic Sea is a seasonally <span class="hlt">ice</span>-covered <span class="hlt">marginal</span> sea located in a densely populated area in northern Europe. Severe sea <span class="hlt">ice</span> conditions have the potential to hinder the intense ship traffic considerably. Thus, sea <span class="hlt">ice</span> fore- and nowcasts are regularly provided by the national weather services. Typically, the forecast comprises several <span class="hlt">ice</span> properties that are distributed as prognostic variables, but their actual usefulness is difficult to measure, and the ship captains must determine their relative importance and relevance for optimal ship speed and safety ad hoc. The present study provides a more objective approach by comparing the ship speeds, obtained by the automatic identification system (AIS), with the respective forecasted <span class="hlt">ice</span> conditions. We find that, despite an unavoidable random component, this information is useful to constrain and rate fore- and nowcasts. More precisely, 62-67% of ship speed variations can be explained by the forecasted <span class="hlt">ice</span> properties when fitting a mixed-effect model. This statistical fit is based on a test region in the Bothnian Sea during the severe winter 2011 and employs 15 to 25 min averages of ship speed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014TCD.....8.3811L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014TCD.....8.3811L"><span><span class="hlt">Ice</span> and AIS: ship speed data and sea <span class="hlt">ice</span> forecasts in the Baltic Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Löptien, U.; Axell, L.</p> <p>2014-07-01</p> <p>The Baltic Sea is a seasonally <span class="hlt">ice</span> covered <span class="hlt">marginal</span> sea located in a densely populated area in northern Europe. Severe sea <span class="hlt">ice</span> conditions have the potential to hinder the intense ship traffic considerably. Thus, sea <span class="hlt">ice</span> fore- and nowcasts are regularly provided by the national weather services. Typically, several <span class="hlt">ice</span> properties are allocated, but their actual usefulness is difficult to measure and the ship captains must determine their relative importance and relevance for optimal ship speed and safety ad hoc. The present study provides a more objective approach by comparing the ship speeds, obtained by the Automatic Identification System (AIS), with the respective forecasted <span class="hlt">ice</span> conditions. We find that, despite an unavoidable random component, this information is useful to constrain and rate fore- and nowcasts. More precisely, 62-67% of ship speed variations can be explained by the forecasted <span class="hlt">ice</span> properties when fitting a mixed effect model. This statistical fit is based on a test region in the Bothnian Bay during the severe winter 2011 and employes 15 to 25 min averages of ship speed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.C22B..07G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.C22B..07G"><span>A new, multi-resolution bedrock elevation map of the Greenland <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>Griggs, J. A.; Bamber, J. L.; Grisbed Consortium</p> <p>2010-12-01</p> <p>Gridded bedrock elevation for the Greenland <span class="hlt">ice</span> sheet has previously been constructed with a 5 km posting. The true resolution of the data set was, in places, however, considerably coarser than this due to the across-track spacing of <span class="hlt">ice</span>-penetrating radar transects. Errors were estimated to be on the order of a few percent in the centre of the <span class="hlt">ice</span> sheet, increasing markedly in relative magnitude near the <span class="hlt">margins</span>, where accurate thickness is particularly critical for numerical modelling and other applications. We use new airborne and satellite estimates of <span class="hlt">ice</span> thickness and surface elevation to determine the bed topography for the whole of Greenland. This is a dynamic product, which will be updated frequently as new data, such as that from NASA’s Operation <span class="hlt">Ice</span> Bridge, becomes available. The University of Kansas has in recent years, flown an airborne <span class="hlt">ice</span>-penetrating radar system with close flightline spacing over several key outlet glacier systems. This allows us to produce a multi-resolution bedrock elevation dataset with the high spatial resolution needed for <span class="hlt">ice</span> dynamic modelling over these key outlet glaciers and coarser resolution over the more sparsely sampled interior. Airborne <span class="hlt">ice</span> thickness and elevation from CReSIS obtained between 1993 and 2009 are combined with JPL/UCI/Iowa data collected by the WISE (Warm <span class="hlt">Ice</span> Sounding Experiment) covering the <span class="hlt">marginal</span> areas along the south west coast from 2009. Data collected in the 1970’s by the Technical University of Denmark were also used in interior areas with sparse coverage from other sources. <span class="hlt">Marginal</span> elevation data from the ICESat laser altimeter and the Greenland <span class="hlt">Ice</span> Mapping Program were used to help constrain the <span class="hlt">ice</span> thickness and bed topography close to the <span class="hlt">ice</span> sheet <span class="hlt">margin</span> where, typically, the terrestrial observations have poor sampling between flight tracks. The GRISBed consortium currently consists of: W. Blake, S. Gogineni, A. Hoch, C. M. Laird, C. Leuschen, J. Meisel, J. Paden, J. Plummer, F</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16357267','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16357267"><span><span class="hlt">Ice</span> recrystallization inhibition in <span class="hlt">ice</span> cream as affected by <span class="hlt">ice</span> structuring proteins from winter wheat grass.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Regand, A; Goff, H D</p> <p>2006-01-01</p> <p><span class="hlt">Ice</span> recrystallization in quiescently frozen sucrose solutions that contained some of the ingredients commonly found in <span class="hlt">ice</span> cream and in <span class="hlt">ice</span> cream manufactured under commercial conditions, with or without <span class="hlt">ice</span> structuring proteins (ISP) from cold-acclimated winter wheat grass extract (AWWE), was assessed by bright field microscopy. In sucrose solutions, critical differences in moisture content, viscosity, ionic strength, and other properties derived from the presence of other ingredients (skim milk powder, corn syrup solids, locust bean gum) caused a reduction in <span class="hlt">ice</span> crystal growth. Significant ISP <span class="hlt">activity</span> in retarding <span class="hlt">ice</span> crystal growth was observed in all solutions (44% for the most complex mix) containing 0.13% total protein from AWWE. In heat-shocked <span class="hlt">ice</span> cream, <span class="hlt">ice</span> recrystallization rates were significantly reduced 40 and 46% with the addition of 0.0025 and 0.0037% total protein from AWWE. The ISP <span class="hlt">activity</span> in <span class="hlt">ice</span> cream was not hindered by its inclusion in mix prior to pasteurization. A synergistic effect between ISP and stabilizer was observed, as ISP <span class="hlt">activity</span> was reduced in the absence of stabilizer in <span class="hlt">ice</span> cream formulations. A remarkably smoother texture for <span class="hlt">ice</span> creams containing ISP after heat-shock storage was evident by sensory evaluation. The efficiency of ISP from AWWE in controlling <span class="hlt">ice</span> crystal growth in <span class="hlt">ice</span> cream has been demonstrated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSHE24A1441S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSHE24A1441S"><span><span class="hlt">Ice</span> Floe Breaking in Contemporary Third Generation Operational Wave Models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sévigny, C.; Baudry, J.; Gauthier, J. C.; Dumont, D.</p> <p>2016-02-01</p> <p>The dynamical zone observed at the edge of the consolidated <span class="hlt">ice</span> area where are found the wave-fractured floes (i.e. <span class="hlt">marginal</span> <span class="hlt">ice</span> zone or MIZ) has become an important topic in ocean modeling. As both operational and climate ocean models now seek to reproduce the complex atmosphere-<span class="hlt">ice</span>-ocean system with realistic coupling processes, many theoretical and numerical studies have focused on understanding and modeling this zone. Few attempts have been made to embed wave-<span class="hlt">ice</span> interactions specific to the MIZ within a two-dimensional model, giving the possibility to calculate both the attenuation of surface waves by sea <span class="hlt">ice</span> and the concomitant breaking of the sea <span class="hlt">ice</span>-cover into smaller floes. One of the first challenges consists in improving the parameterization of wave-<span class="hlt">ice</span> dynamics in contemporary third generation operational wave models. A simple waves-in-<span class="hlt">ice</span> model (WIM) similar to the one proposed by Williams et al. (2013a,b) was implemented in WAVEWATCH III. This WIM considers <span class="hlt">ice</span> floes as floating elastic plates and predicts the dimensionless attenuation coefficient by the use of a lookup-table-based, wave scattering scheme. As in Dumont et al. (2011), the different frequencies are treated individually and floe breaking occurs for a particular frequency when the expected wave amplitude exceeds the allowed strain amplitude, which considers <span class="hlt">ice</span> floes properties and wavelength in <span class="hlt">ice</span> field. The model is here further refined and tested in idealized two-dimensional cases, giving preliminary results of the performance and sensitivity of the parameterization to initial wave and <span class="hlt">ice</span> conditions. The effects of the wave-<span class="hlt">ice</span> coupling over the incident wave spectrum are analyzed as well as the resulting floe size distribution. The model gives prognostic values of the lateral extent of the <span class="hlt">marginal</span> <span class="hlt">ice</span> zone with maximum <span class="hlt">ice</span> floe diameter that progressively increases with distance from the <span class="hlt">ice</span> edge.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSHE34A1451P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSHE34A1451P"><span>Effects of an Arctic under-<span class="hlt">ice</span> phytoplankton bloom on bio-optical properties of surface waters during the Norwegian Young Sea <span class="hlt">Ice</span> Cruise (N-<span class="hlt">ICE</span>2015)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pavlov, A. K.; Granskog, M. A.; Hudson, S. R.; Taskjelle, T.; Kauko, H.; Hamre, B.; Assmy, P.; Mundy, C. J.; Nicolaus, M.; Kowalczuk, P.; Stedmon, C. A.; Fernandez Mendez, M.</p> <p>2016-02-01</p> <p>A thinner and younger Arctic sea-<span class="hlt">ice</span> cover has led to an increase in solar light transmission into the surface ocean, especially during late spring and summer. A description of the seasonal evolution of polar surface water optical properties is essential, in order to understand how changes are affecting light availability for photosynthetic organisms and the surface ocean energy budget. The development of the bio-optical properties of Arctic surface waters under predominantly first-year sea <span class="hlt">ice</span> in the southern Nansen Basin were studied from January to June 2015 during the Norwegian Young Sea <span class="hlt">Ice</span> Cruise (N-<span class="hlt">ICE</span>2015). Observations included inherent optical properties, absorption by colored dissolved organic matter and particles, as well as radiometric measurements. We documented a rapid transition from relatively clear and transparent waters in winter to turbid waters in late May and June. This transition was associated with a strong under-<span class="hlt">ice</span> phytoplankton bloom detected first under the compact <span class="hlt">ice</span> pack and then monitored during drift across the <span class="hlt">marginal</span> <span class="hlt">ice</span> zone. We discuss potential implications of underwater light availability for photosynthesis, heat redistribution in the upper ocean layer, and energy budget of the sea-<span class="hlt">ice</span> - ocean system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45.1647G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45.1647G"><span>Oxidative Processing Lowers the <span class="hlt">Ice</span> Nucleation <span class="hlt">Activity</span> of Birch and Alder Pollen</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gute, Ellen; Abbatt, Jonathan P. D.</p> <p>2018-02-01</p> <p>Pollen carry water extractable compounds with <span class="hlt">ice</span> nucleating (IN) <span class="hlt">activity</span>. This study investigates whether the hydroxyl radical, as the major atmospheric oxidant, can affect the IN <span class="hlt">activity</span> of silver birch and grey alder subpollen particles under in-cloud conditions for deposition freezing mode conditions at 234 K. It is found that oxidation increases the supersaturation ratio with respect to <span class="hlt">ice</span> necessary for the onset of <span class="hlt">ice</span> nucleation and decreases the fraction of particles which initiate <span class="hlt">ice</span> nucleation. This reduction of IN <span class="hlt">activity</span> under equivalent oxidation conditions does not occur with a mineral dust sample (Arizona Test Dust). Chemical analysis of fresh and oxidized pollen material indicates a change of molecular structure with a loss of conjugation and an increase in oxidized functional groups, such as carbonyls. This is the first demonstration that in-cloud oxidation may lower the IN abilities of biological particles such as pollen.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28876070','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28876070"><span>Role of Salt, Pressure, and Water <span class="hlt">Activity</span> on Homogeneous <span class="hlt">Ice</span> Nucleation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Espinosa, Jorge R; Soria, Guiomar D; Ramirez, Jorge; Valeriani, Chantal; Vega, Carlos; Sanz, Eduardo</p> <p>2017-09-21</p> <p>Pure water can be substantially supercooled below the melting temperature without transforming into <span class="hlt">ice</span>. The achievable supercooling can be enhanced by adding solutes or by applying hydrostatic pressure. Avoiding <span class="hlt">ice</span> formation is of great importance in the cryopreservation of food or biological samples. In this Letter, we investigate the similarity between the effects of pressure and salt on <span class="hlt">ice</span> formation using a combination of state-of-the-art simulation techniques. We find that both hinder <span class="hlt">ice</span> formation by increasing the energetic cost of creating the <span class="hlt">ice</span>-fluid interface. Moreover, we examine the widely accepted proposal that the <span class="hlt">ice</span> nucleation rate for different pressures and solute concentrations can be mapped through the <span class="hlt">activity</span> of water [ Koop , L. ; Tsias , P. Nature , 2000 , 406 , 611 ]. We show that such a proposal is not consistent with the nucleation rates predicted in our simulations because it does not include all parameters affecting <span class="hlt">ice</span> nucleation. Therefore, even though salt and pressure have a qualitatively similar effect on <span class="hlt">ice</span> formation, they cannot be quantitatively mapped onto one another.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012JGRF..117.2038G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012JGRF..117.2038G"><span>Investigation of land <span class="hlt">ice</span>-ocean interaction with a fully coupled <span class="hlt">ice</span>-ocean model: 2. Sensitivity to external forcings</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goldberg, D. N.; Little, C. M.; Sergienko, O. V.; Gnanadesikan, A.; Hallberg, R.; Oppenheimer, M.</p> <p>2012-06-01</p> <p>A coupled <span class="hlt">ice</span> stream-<span class="hlt">ice</span> shelf-ocean cavity model is used to assess the sensitivity of the coupled system to far-field ocean temperatures, varying from 0.0 to 1.8°C, as well as sensitivity to the parameters controlling grounded <span class="hlt">ice</span> flow. A response to warming is seen in grounding line retreat and grounded <span class="hlt">ice</span> loss that cannot be inferred from the response of integrated melt rates alone. This is due to concentrated thinning at the <span class="hlt">ice</span> shelf lateral <span class="hlt">margin</span>, and to processes that contribute to this thinning. Parameters controlling the flow of grounded <span class="hlt">ice</span> have a strong influence on the response to sub-<span class="hlt">ice</span> shelf melting, but this influence is not seen until several years after an initial perturbation in temperatures. The simulated melt rates are on the order of that observed for Pine Island Glacier in the 1990s. However, retreat rates are much slower, possibly due to unrepresented bedrock features.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016QSRv..146..300W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016QSRv..146..300W"><span>Sedimentary and structural evolution of a Pleistocene small-scale push moraine in eastern Poland: New insight into paleoenvironmental conditions at the <span class="hlt">margin</span> of an advancing <span class="hlt">ice</span> lobe</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Włodarski, Wojciech; Godlewska, Anna</p> <p>2016-08-01</p> <p>Recent studies of push moraines have focused on the interplay between the dynamics of <span class="hlt">ice</span> <span class="hlt">margins</span> and the environmental variables of the foreland into which they advance. These studies showed that the spatial distribution, geometry and style of the glaciotectonic deformation of push moraines are controlled by <span class="hlt">ice</span>-induced stresses, the strain rate, the rheology of the deposits and hydraulic conductivity. In this work, we provide new insight into this interplay at a small spatio-temporal scale, specifically, the ancient glacial system of the Liwiec <span class="hlt">ice</span> lobe within the younger Saalian <span class="hlt">ice</span> sheet in eastern Poland. The paleoenvironmental variables that are analysed here refer to the dynamics of the hydrological processes that affected the patterns and sediment deposition rate on the terminoglacial fan and the resulting mechanical stratigraphy and hydraulic conductivity of the foreland. We document the progradational sequence of the fan deposits that developed as a result of the <span class="hlt">ice</span> lobe thickening and the steepening of its stationary front. The sedimentary features of the fan, the lithology of its basement and the hydraulic conductivity of the foreland strongly influenced the geometry and kinematics of fold growth during the advance of the <span class="hlt">ice</span> lobe. The predominance of flexural slip and the development of fractures, including fold-accommodation faults, were interpreted to be an effect of buckle folding due to horizontal shortening induced by <span class="hlt">ice</span> advance. The partial overriding of the push moraine by the <span class="hlt">ice</span> lobe and, thus, the submarginal conditions for deformation were inferred from the significant hinge migration and internal deformation of the strata under undrained conditions in one of the folds. The synfolding deposition pattern of the fan growth strata allowed us to suggest that the push moraine was probably formed by a sustained advance rather than surge.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP51B1070U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP51B1070U"><span>Geochemical evidences of methane hydrate dissociation in Alaskan Beaufort <span class="hlt">Margin</span> during Holocene</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Uchida, M.; Rella, S.; Kubota, Y.; Kumata, H.; Mantoku, K.; Nishino, S.; Itoh, M.</p> <p>2017-12-01</p> <p>Alaskan Beaufort <span class="hlt">margin</span> bear large abundances of sub-sea and permafrost methane hydrate[Ruppel, 2016]. During the Last Glacial, previous reported direct and indirect evidences accumulated from geochemical data from <span class="hlt">marginal</span> sea sediment suggests that methane episodically released from hydrate trapped in the seafloor sediments[Kennett et al., 2000; Uchida et al., 2006, 2008; Cook et al, 2011]. Here we analyzed stable isotopes of foraminifera and molecular marker derived from the <span class="hlt">activity</span> of methanotrophic bacteria from piston cores collected by the 2010 R/V Mirai cruise in Alaskan Beaufort <span class="hlt">Margin</span>. Our data showed highly depleted 13C compositions of benthic foraminifera, suggesting indirect records of enhanced incorporation of 13C-depleted CO2 formed by methanotrophic process that use 12C-enriched methane as their main source of carbon. This is the first evidence of methane hydrate dissociation in Alaskan <span class="hlt">margin</span>. Here we discussed timing of signals of methane dissociation with variability of sea <span class="hlt">ice</span> and intermediate Atlantic water temperature. The dissociation of methane hydrate in the Alaskan <span class="hlt">Margin</span> may be modulated by Atlantic warm intermediate water warming. Our results suggest that Arctic <span class="hlt">marginal</span> regions bearing large amount methane hydrate may be a profound effect on future warming climate changes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C53C0754M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C53C0754M"><span>Quaternary evolution of the Fennoscandian <span class="hlt">Ice</span> Sheet from 3D seismic data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Montelli, A.; Dowdeswell, J. A.; Ottesen, D.; Johansen, S. E.</p> <p>2016-12-01</p> <p>The Quaternary seismic stratigraphy and architecture of the mid-Norwegian continental shelf and slope are investigated using extensive grids of marine 2D and 3D seismic reflection data that cover more than 100,000 km2 of the continental <span class="hlt">margin</span>. At least 26 distinct regional palaeo-surfaces have been interpreted within the stratigraphy of the Quaternary Naust Formation on the mid-Norwegian <span class="hlt">margin</span>. Multiple assemblages of buried glacigenic landforms are preserved within the Naust Formation across most of the study area, facilitating detailed palaeo-glaciological reconstructions. We document a marine-terminating, calving Fennoscandian <span class="hlt">Ice</span> Sheet (FIS) <span class="hlt">margin</span> present periodically on the Norwegian shelf since at least the beginning of the Quaternary. Elongate, streamlined landforms interpreted as mega-scale glacial lineations (MSGLs) have been found within the upper part of the Naust sequence N ( 1.9-1.6 Ma), sugesting the development of fast-flowing <span class="hlt">ice</span> streams since that time. Shifts in the location of depocentres and direction of features indicative of fast <span class="hlt">ice</span>-flow suggest that several reorganisations in the FIS drainage have occurred since 1.5 Ma. Subglacial landforms reveal a complex and dynamic <span class="hlt">ice</span> sheet, with converging palaeo-<span class="hlt">ice</span> streams and several flow-switching events that may reflect major changes in topography and internal <span class="hlt">ice</span>-sheet structure. Lack of subglacial meltwater channels suggests a largely distributed, low-volume meltwater system that drained the FIS through permeable subglacial till without leaving much erosional evidence. This regional palaeo-environmental examination of the FIS provides a useful framework for <span class="hlt">ice</span>-sheet modelling and shows that fragmentary preservation of buried surfaces and variability of <span class="hlt">ice</span>-sheet dynamics should be taken into account when reconstructing glacial history from spatially limited datasets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.4366H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.4366H"><span>Deciphering the evolution of the last Eurasian <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>Hughes, Anna; Gyllencreutz, Richard; Mangerud, Jan; Svendsen, John Inge</p> <p>2016-04-01</p> <p>Glacial geologists need <span class="hlt">ice</span> sheet-scale chronological reconstructions of former <span class="hlt">ice</span> extent to set individual records in a wider context and compare interpretations of <span class="hlt">ice</span> sheet response to records of past environmental changes. <span class="hlt">Ice</span> sheet modellers require empirical reconstructions on size and volume of past <span class="hlt">ice</span> sheets that are fully documented, specified in time and include uncertainty estimates for model validation or constraints. Motivated by these demands, in 2005 we started a project (Database of the Eurasian Deglaciation, DATED) to compile and archive all published dates relevant to constraining the build-up and retreat of the last Eurasian <span class="hlt">ice</span> sheets, including the British-Irish, Scandinavian and Svalbard-Barents-Kara Seas <span class="hlt">ice</span> sheets (BIIS, SIS and SBKIS respectively). Over 5000 dates were assessed for reliability and used together with published <span class="hlt">ice</span>-sheet <span class="hlt">margin</span> positions to reconstruct time-slice maps of the <span class="hlt">ice</span> sheets' extent, with uncertainty bounds, every 1000 years between 25-10 kyr ago and at four additional periods back to 40 kyr ago. Ten years after the idea for a database was conceived, the first version of results (DATED-1) has now been released (Hughes et al. 2016). We observe that: i) both the BIIS and SBKIS achieve maximum extent, and commence retreat earlier than the larger SIS; ii) the eastern terrestrial <span class="hlt">margin</span> of the SIS reached its maximum extent up to 7000 years later than the westernmost marine <span class="hlt">margin</span>; iii) the combined maximum <span class="hlt">ice</span> volume (~24 m sea-level equivalent) was reached c. 21 ka; iv) large uncertainties exist; predominantly across marine sectors (e.g. the timing of coalescence and separation of the SIS and BKIS) but also in well-studied areas due to conflicting yet equally robust data. In just three years since the DATED-1 census (1 January 2013), the volume of new information (from both dates and mapped glacial geomorphology) has grown significantly (~1000 new dates). Here, we present the DATED-1 results in the context of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19970003047','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19970003047"><span>Multi-Year Elevation Changes Near the West <span class="hlt">Margin</span> of the Greenland <span class="hlt">Ice</span> Sheet from Satellite Radar Altimetry</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lingle, Craig S.; Brenner, Anita C.; Zwally, H. Jay; DiMarzio, John P.</p> <p>1991-01-01</p> <p>Mean changes in the surface elevation near the west <span class="hlt">margin</span> of the Greenland <span class="hlt">ice</span> sheet are measured using Seasat altimetry and altimetry from the Geosat Exact Repeat Mission (ERM). The Seasat data extend from early July through early October 1978. The ERM data extend from winter 1986-87 through fall 1988. Both seasonal and multi-year changes are measured using altimetry referenced to GEM T2 orbits. The possible effects of orbit error are minimized by adjusting the orbits into a common ocean surface. Seasonal mean changes in the surface height are recognizable during the Geosat ERM. The multi-year measurements indicate the surface was lower by 0.4 +/- 0.4 m on average in late summer 1987 than in late summer 1978. The surface was lower by 0.2 +/- 0.5 m on average in late summer 1988 than in late summer 1978. As a control case, the computations art also carried out using altimetry referenced to orbits not adjusted into a common ocean surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12.5274C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12.5274C"><span>Seafloor Morphology And Sediment Discharge Of The Storfjorden And Kveithola Palaeo-<span class="hlt">Ice</span> Streams (NW Barents Sea) During The Last Deglaciation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Camerlenghi, Angelo; Rebesco, Michele; Pedrosa, Mayte; Demol, Ben; Giulia Lucchi, Renata; Urgeles, Roger; Colmenero-Hidalgo, Elena; Andreassen, Karin; Sverre Laberg, Jan; Winsborrow, Monica</p> <p>2010-05-01</p> <p>IPY <span class="hlt">Activity</span> N. 367 focusing on Neogene <span class="hlt">ice</span> streams and sedimentary processes on high- latitude continental <span class="hlt">margins</span> (NICE-STREAMS) resulted in two coordinated cruises on the adjacent Storfjorden and Kveithola trough-mouth fans in the NW Barents Sea: SVAIS Cruise of BIO Hespérides, summer 2007, and EGLACOM Cruise of Cruise R/V OGS-Explora, summer 2008. The objectives were to acquire a high-resolution set of bathymetric, seismic and sediment core data in order to decipher the Neogene architectural development of the glacially-dominated NW Barents Sea continental <span class="hlt">margin</span> in response to natural climate change. The paleo-<span class="hlt">ice</span> streams drained <span class="hlt">ice</span> from southern Spitsbergen, Spitsbergen Bank, and Bear Island. The short distance from the <span class="hlt">ice</span> source to the calving front produced a short residence time of <span class="hlt">ice</span>, and therefore a rapid response to climatic changes. In the outer trough of southern Storfjorden, lobate moraines superimpose and are cut by very large linear features attributed to mega-iceberg scours. In the adjacent Kveithola trough, a fresh morphology includes mega-scale glacial lineations overprinted by transverse grounding-zone wedges, diagnostic of episodic <span class="hlt">ice</span> stream retreat. A 15 m thick glacimarine drape suggests an high post-deglaciation sedimentation rate. Preliminary interpretation suggests that the retreat of the Svalbard/Barents Sea <span class="hlt">Ice</span> Sheet was highly dynamic and that grounded <span class="hlt">ice</span> persisted on Spitsbergen Bank for some thousands years after the main Barents Sea deglaciation.The Storfjorden continental slope is divided into three wide lobes. Opposite the two northernmost lobes the slope is dominated by straight gullies in the upper part, and deposition of debris lobes on the mid and lower parts. In contrast, the southernmost lobe is characterized by widespread occurrence of submarine landslides. Sediment failure has accompanied the evolution of the southern Storfjorden and Kveithola <span class="hlt">margin</span> throughout the Late Neogene, with very large mass transport</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_14 --> <div id="page_15" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="281"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1813675Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1813675Y"><span>Characterization of the <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> of an airborne Penicillium species</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yordanova, Petya; Hill, Thomas C. J.; Pummer, Bernhard G.; Franc, Gary D.; Pöschl, Ulrich; Fröhlich-Nowoisky, Janine</p> <p>2016-04-01</p> <p>Microorganisms are ubiquitous both on and above the Earth. Several bacterial and fungal spe-cies are the focus of atmospheric studies due to their ability to trigger <span class="hlt">ice</span> formation at high subzero temperatures. Thus, they have potential to modify cloud albedo, lifetime and precipita-tion, and ultimately the hydrological cycle. Several fungal strains have already been identified as possessing <span class="hlt">ice</span> nucleation (IN) <span class="hlt">activity</span>, and recent studies have shown that IN <span class="hlt">active</span> fungi are present in the cultivable community of air and soil samples [1, 2]. However, the abundance, diversity, and sources of fungal <span class="hlt">ice</span> nuclei in the atmosphere are still poorly characterized. In this study, fungal colonies obtained from air samples were screened for IN <span class="hlt">activity</span> in the droplet-freezing assay described in Fröhlich-Nowoisky et al., 2015 [2]. Out of 128 tested iso-lates, two were found to catalyze <span class="hlt">ice</span> formation at temperatures up to -4°C. By DNA analysis, both isolates were classified as Penicillium spp. The freezing <span class="hlt">activity</span> of both was further char-acterized after different filtration, heat, and enzymatic treatments in the temperature range from -4°C to -15°C. Preliminary results show that a proteinaceous compound is responsible for the IN <span class="hlt">activity</span>. Furthermore, ongoing experiments indicate that the <span class="hlt">activity</span> is associated only with the hyphae. [1] Huffman, et al. (2013): Atmos. Chem. Phys., 13, 6151-6164. [2] Fröhlich-Nowoisky et al. (2015): Biogeosciences, 12: 1057-1071.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19850017733&hterms=glacier+melt&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dglacier%2Bmelt','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19850017733&hterms=glacier+melt&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dglacier%2Bmelt"><span>Potential Climatic Effects on the Greenland <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. A.</p> <p>1984-01-01</p> <p>The Greenland <span class="hlt">Ice</span> Sheet covers an area of 1,720,000 sq. km and contains approximately 2,600,000 cu km of <span class="hlt">ice</span>. Most of the <span class="hlt">ice</span> sheet receives an excess of snow accumulation over the amount of <span class="hlt">ice</span> lost to wind, meltwater run-off or other ablative processes. The majority of mass loss occurs at the <span class="hlt">margin</span> of the <span class="hlt">ice</span> sheet as either surface melt, which flows into the sea or calving of icebergs from the tongues of outlet glaciers. Many estimates of these processes were published. An average of five published estimates is summarized. If these estimates are correct, then the Greenland <span class="hlt">Ice</span> Sheet is in approximate equilibrium and contributes 490 cu km/a of fresh water to the North Atlantic and Arctic Oceans. Climate effects, <span class="hlt">ice</span> sheet flow, and application of remote sensing to tracking of the <span class="hlt">ice</span> sheet are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1610721F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1610721F"><span>The last forests in Greenland, and the age of the <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>Funder, Svend; Schmidt, Astrid M. Z.; Dahl-Jensen, Dorthe; Steffensen, Jørgen Peder; Willerslev, Eske</p> <p>2014-05-01</p> <p>Recently ancient DNA (aDNA) studies of the basal <span class="hlt">ice</span> in the Camp Century <span class="hlt">ice</span> core, northern Greenland, have shown that mixed coniferous-deciduous forest grew here before the area was invaded and permanently covered by the <span class="hlt">ice</span> sheet. The coring site is situated only 100 km from the present <span class="hlt">ice</span> <span class="hlt">margin</span> and more than 500 km from the <span class="hlt">ice</span> divide, indicating that since this last inception the northern part of the <span class="hlt">ice</span> sheet never receded more than 100 km from its present <span class="hlt">margin</span>. Dating of the basal <span class="hlt">ice</span> and obtaining an age for the forest and for the beginning of the <span class="hlt">ice</span> sheet's permanency has been attempted by analyzing for optically stimulated luminescence (OSL), meteoric 10Be/36Cl cosmogenic nuclides, 234U/238U recoil. These methods all provide only minimum ages and show that the forest at Cap Century is older than 500 ka. Comparison with other Pleistocene "forest sites" in Greenland - the Kap København Formation in northernmost Greenland, the DYE-3 <span class="hlt">ice</span> core in the south, the ODP boring 646 south of Greenland, as well as results from basal <span class="hlt">ice</span> in the GRIP <span class="hlt">ice</span> core - extends the minimum age to c. 1 ma. The maximum age is provided by the Kap København Formation, which must be older - or contemporaneous. The formation has recently been confirmed to date within the interval 2-2.5 ma, with a preferred age of 2.3-2.4 ma. Surprisingly, application of the molecular clock of insect COI sequences on the Camp Century aDNA now seem to push the minimum age just as far back - to 2.4 ma, suggesting that the timberline boreal forest at Kap København is contemporaneous with the mixed forest at Camp Century, 600 km to the south. From this we conclude that the northern <span class="hlt">ice</span> sheet dome, which today contains 85% of the total <span class="hlt">ice</span> sheet volume, has remained within 100 km of its present <span class="hlt">margin</span> for at least 1 ma, and possibly may go back as far as 2.4 ma. The <span class="hlt">ice</span> sheet has therefore survived both interglacials and "super interglacials" that were both warmer and longer than the present. This</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002JGRB..107.2076D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002JGRB..107.2076D"><span>Form and flow of the Academy of Sciences <span class="hlt">Ice</span> Cap, Severnaya Zemlya, Russian High Arctic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dowdeswell, J. A.; Bassford, R. P.; Gorman, M. R.; Williams, M.; Glazovsky, A. F.; Macheret, Y. Y.; Shepherd, A. P.; Vasilenko, Y. V.; Savatyuguin, L. M.; Hubberten, H.-W.; Miller, H.</p> <p>2002-04-01</p> <p>The 5,575-km2 Academy of Sciences <span class="hlt">Ice</span> Cap is the largest in the Russian Arctic. A 100-MHz airborne radar, digital Landsat imagery, and satellite synthetic aperture radar (SAR) interferometry are used to investigate its form and flow, including the proportion of mass lost through iceberg calving. The <span class="hlt">ice</span> cap was covered by a 10-km-spaced grid of radar flight paths, and the central portion was covered by a grid at 5-km intervals: a total of 1,657 km of radar data. Digital elevation models (DEMs) of <span class="hlt">ice</span> surface elevation, <span class="hlt">ice</span> thickness, and bed elevation data sets were produced (cell size 500 m). The DEMs were used in the selection of a deep <span class="hlt">ice</span> core drill site. Total <span class="hlt">ice</span> cap volume is 2,184 km3 (~5.5 mm sea level equivalent). The <span class="hlt">ice</span> cap has a single dome reaching 749 m. Maximum <span class="hlt">ice</span> thickness is 819 m. About 200 km, or 42%, of the <span class="hlt">ice</span> <span class="hlt">margin</span> is marine. About 50% of the <span class="hlt">ice</span> cap bed is below sea level. The central divide of the <span class="hlt">ice</span> cap and several major drainage basins, in the south and east of the <span class="hlt">ice</span> cap and of up to 975 km2, are delimited from satellite imagery. There is no evidence of past surge <span class="hlt">activity</span> on the <span class="hlt">ice</span> cap. SAR interferometric fringes and phase-unwrapped velocities for the whole <span class="hlt">ice</span> cap indicate slow flow in the interior and much of the <span class="hlt">margin</span>, punctuated by four fast flowing features with lateral shear zones and maximum velocity of 140 m yr-1. These <span class="hlt">ice</span> streams extend back into the slower moving <span class="hlt">ice</span> to within 5-10 km of the <span class="hlt">ice</span> cap crest. They have lengths of 17-37 km and widths of 4-8 km. Mass flux from these <span class="hlt">ice</span> streams is ~0.54 km3 yr-1. Tabular icebergs up to ~1.7 km long are produced. Total iceberg flux from the <span class="hlt">ice</span> cap is ~0.65 km3 yr-1 and probably represents ~40% of the overall mass loss, with the remainder coming from surface melting. Driving stresses are generally lowest (<40 kPa) close to the <span class="hlt">ice</span> cap divides and in several of the <span class="hlt">ice</span> streams. <span class="hlt">Ice</span> stream motion is likely to include a significant basal component and may involve deformable</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19810068605','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19810068605"><span>Effects of <span class="hlt">Ice</span> Formations on Airplane Performance in Level Cruising Flight</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Preston, G. Merritt; Blackman, Calvin C.</p> <p>1948-01-01</p> <p>A flight investigation in natural <span class="hlt">icing</span> conditions was conducted by the NACA to determine the effect of <span class="hlt">ice</span> accretion on airplane performance. The maximum loss in propeller efficiency encountered due to <span class="hlt">ice</span> formation on the propeller blades was 19 percent. During 87 percent of the propeller <span class="hlt">icing</span> encounters, losses of 10 percent or less were observed. <span class="hlt">Ice</span> formations on all of the components of the airplane except the propellers during one <span class="hlt">icing</span> encounter resulted in an increase in parasite drag of the airplane of 81 percent. The control response of the airplane in this condition was <span class="hlt">marginal</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C41A0644M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C41A0644M"><span>Modelling of Sea <span class="hlt">Ice</span> Thermodynamics and Biogeochemistry during the N-<span class="hlt">ICE</span>2015 Expedition in the Arctic Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Meyer, A.; Duarte, P.; Mork Olsen, L.; Kauko, H.; Assmy, P.; Rösel, A.; Itkin, P.; Hudson, S. R.; Granskog, M. A.; Gerland, S.; Sundfjord, A.; Steen, H.; Jeffery, N.; Hunke, E. C.; Elliott, S.; Turner, A. K.</p> <p>2016-12-01</p> <p>Changes in the sea <span class="hlt">ice</span> regime of the Arctic Ocean over the last decades from a thick perennial multiyear <span class="hlt">ice</span> to a first year <span class="hlt">ice</span> have been well documented. These changes in the sea <span class="hlt">ice</span> regime will affect feedback mechanisms between the sea <span class="hlt">ice</span>, atmosphere and ocean. Here we evaluate the performance of the Los Alamos Sea <span class="hlt">Ice</span> Model (CICE), a state of the art sea <span class="hlt">ice</span> model, to predict sea <span class="hlt">ice</span> physical and biogeochemical properties at time scales of a few weeks. We also identify the most problematic prognostic variables and what is necessary to improve their forecast. The availability of a complete data set of forcing collected during the Norwegian Young sea <span class="hlt">Ice</span> (N-<span class="hlt">ICE</span>-2015) expedition north of Svalbard opens the possibility to properly test CICE. Oceanographic, atmospheric, sea <span class="hlt">ice</span>, snow, and biological data were collected above, on, and below the <span class="hlt">ice</span> using R/V Lance as the base for the <span class="hlt">ice</span> camps that were drifting south towards the Fram Strait. Over six months, four different drifts took place, from the Nansen Basin, through the <span class="hlt">marginal</span> <span class="hlt">ice</span> zone, to the open ocean. Obtained results from the model show a good performance regarding <span class="hlt">ice</span> thickness, salinity and temperature. Nutrients and sea <span class="hlt">ice</span> algae are however not modelled as accurately. We hypothesize that improvements in biogeochemical modeling may be achieved by complementing brine drainage with a diffusion parameterization and biogeochemical modeling with the introduction of an explicit formulation to forecast chlorophyll and regulate photosynthetic efficiency.</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 lakes 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 lake water moves between lakes and rapidly drains, causing catastrophic floods. The exact mechanisms by which subglacial lakes influence <span class="hlt">ice</span>-sheet dynamics are unknown, however, and large subglacial lakes 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 lakes, similar in total area to Lake 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 lakes 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 <span class="hlt">margins</span> of these four subglacial lakes. We conclude that the subglacial lakes initiate and maintain rapid <span class="hlt">ice</span> flow through either <span class="hlt">active</span> modification of the basal thermal regime of the <span class="hlt">ice</span> sheet by lake accretion or through scouring bedrock channels in periodic drainage events. We suggest that the role of subglacial lakes needs to be considered in <span class="hlt">ice</span>-sheet mass balance assessments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA154406','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA154406"><span><span class="hlt">Active</span> and Passive Remote Sensing of <span class="hlt">Ice</span>.</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1984-09-01</p> <p>This is a report on the progress that has been made in the study of <span class="hlt">active</span> and passive remote sensing of <span class="hlt">ice</span> during the period of February 1, 1984...the emissivities as functions of viewing angles and polarizations. They are used to interpret the passive microwave remote sensing data from</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.4621R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.4621R"><span>State of Arctic Sea <span class="hlt">Ice</span> North of Svalbard during N-<span class="hlt">ICE</span>2015</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rösel, Anja; King, Jennifer; Gerland, Sebastian</p> <p>2016-04-01</p> <p>The N-<span class="hlt">ICE</span>2015 cruise, led by the Norwegian Polar Institute, was a drift experiment with the research vessel R/V Lance from January to June 2015, where the ship started the drift North of Svalbard at 83°14.45' N, 21°31.41' E. The drift was repeated as soon as the vessel drifted free. Altogether, 4 <span class="hlt">ice</span> stations where installed and the complex ocean-sea <span class="hlt">ice</span>-atmosphere system was studied with an interdisciplinary Approach. During the N-<span class="hlt">ICE</span>2015 cruise, extensive <span class="hlt">ice</span> thickness and snow depth measurements were performed during both, winter and summer conditions. Total <span class="hlt">ice</span> and snow thickness was measured with ground-based and airborne electromagnetic instruments; snow depth was measured with a GPS snow depth probe. Additionally, <span class="hlt">ice</span> mass balance and snow buoys were deployed. Snow and <span class="hlt">ice</span> thickness measurements were performed on repeated transects to quantify the <span class="hlt">ice</span> growth or loss as well as the snow accumulation and melt rate. Additionally, we collected independent values on surveys to determine the general <span class="hlt">ice</span> thickness distribution. Average snow depths of 32 cm on first year <span class="hlt">ice</span>, and 52 cm on multi-year <span class="hlt">ice</span> were measured in January, the mean snow depth on all <span class="hlt">ice</span> types even increased until end of March to 49 cm. The average total <span class="hlt">ice</span> and snow thickness in winter conditions was 1.92 m. During winter we found a small growth rate on multi-year <span class="hlt">ice</span> of about 15 cm in 2 months, due to above-average snow depths and some extraordinary storm events that came along with mild temperatures. In contrast thereto, we also were able to study new <span class="hlt">ice</span> formation and thin <span class="hlt">ice</span> on newly formed leads. In summer conditions an enormous melt rate, mainly driven by a warm Atlantic water inflow in the <span class="hlt">marginal</span> <span class="hlt">ice</span> zone, was observed during two <span class="hlt">ice</span> stations with melt rates of up to 20 cm per 24 hours. To reinforce the local measurements around the ship and to confirm their significance on a larger scale, we compare them to airborne thickness measurements and classified SAR-satellite scenes. The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..1212967E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..1212967E"><span>Unveiling climate and <span class="hlt">ice</span>-sheet history from drilling in high-latitude <span class="hlt">margins</span> and future perspectives</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Escutia Dotti, Carlota</p> <p>2010-05-01</p> <p>Polar <span class="hlt">ice</span> is an important component of the climate system, affecting global sea level, ocean circulation and heat transport, marine productivity, and albedo. During the last decades drilling in the Arctic (IODP ACEX and Bering Expeditions) and in Antarctica (ODP Legs 178, 188, IODP Expedition 318 and ANDRILL) has revealed regional information about sea <span class="hlt">ice</span> and <span class="hlt">ice</span> sheets development and evolution. Integration of this data with numerical modeling provide an understanding of the early development of the <span class="hlt">ice</span> sheets and their variability through the Cenozoic. Much of this work points to atmospheric CO2 and other greenhouse gases concentrations as important triggering mechanism driving the onset of glaciation and subsequent <span class="hlt">ice</span> volume variability. With current increasing atmospheric greenhouse gases concentrations resulting in rapidly rising global temperatures, studies of polar climates become increasingly prominent on the research agenda. Despite of the relevance of the high-latitudes in the global climate systems, the short- and long-term history of the <span class="hlt">ice</span> sheets and sea-<span class="hlt">ice</span> and its relationships with paleoclimatic, paleoceanographic, and sea level changes is still poorly understood. A multinational, multiplatform scientific drilling strategy is being developed to recover key physical evidence from selected high-latitude areas. This strategy is aimed at addressing key knowledge gaps about the role of polar <span class="hlt">ice</span> in climate change, targeting questions such as timing of events, rates of change, tipping points, regional variations, and northern vs. southern hemispheres (in phase or out-of-phase) variability. This data is critical to provide constrains to sea-<span class="hlt">ice</span> and <span class="hlt">ice</span> sheet models, which are the basis for forecasting the future of the cryosphere in a warming world.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP13D1110R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP13D1110R"><span>Discharge of water and sediment from <span class="hlt">ice</span>-streams on the southeastern Laurentide <span class="hlt">Ice</span> Sheet during Heinrich events: timing and magnitude</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rashid, H.; Piper, D.</p> <p>2017-12-01</p> <p>Several <span class="hlt">ice</span>-streams on the southeastern sector of the Laurentide <span class="hlt">Ice</span> Sheet discharged icebergs, meltwater, and fine-grained sediments into the North Atlantic during Heinrich (H) events. The principal contribution was through Hudson Strait, which is the only source clearly identified in H <span class="hlt">ice</span>-rafted layers in the central North Atlantic. The role of direct supply of meltwater in modifying the Atlantic meridional circulation generally has been regarded as secondary. The relative chronology of discharge in different <span class="hlt">ice</span>-streams is poorly known. Here, we re-assess these questions using continental <span class="hlt">margin</span> cores constrained by high-resolution seismic profiles and multibeam bathymetry data. Relative importance of <span class="hlt">ice</span> streams likely scales with cross-sectional area of their erosional troughs. On that basis, the Hudson Strait <span class="hlt">ice</span> stream was twice as large as that in the Laurentian Channel and 3-4 times larger than smaller troughs. Several <span class="hlt">ice</span> streams supplied petrographically and geochemically distinct sediment including black shales from Cumberland Sound, limestone and dolomite in particular proportions from Frobisher Bay and Hudson Strait, and red sandstones and shales ± carbonates from NE Newfoundland and Laurentian Channel. In several cases, detrital carbonate H layers derived predominantly from Hudson Strait are preceded by enhanced IRD deposition from smaller <span class="hlt">ice</span> streams, e.g. deposits from Cumberland Sound on the Labrador slope, from NE Newfoundland in Orphan Basin, and from Laurentian Channel on the Nova Scotian <span class="hlt">margin</span>. Gravel petrology indicates that Hudson Strait sources make up >90% of the <span class="hlt">ice</span>-rafted component of distal H layers. H layers proximal to the Hudson Strait <span class="hlt">ice</span>-streams are 4 to 12 meters thick compared to a few centimeters thick seaward of the Trinity Trough and Laurentian <span class="hlt">ice</span>-streams, comparable to the thickness of the North Atlantic. This underscores the great importance of meltwater and suspended sediment close to <span class="hlt">ice</span> stream outlets. Morphological</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFMGC12A..03K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFMGC12A..03K"><span>Late-glacial and Holocene history of changes in Quelccaya <span class="hlt">Ice</span> Cap, Peru</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kelly, M. A.; Lowell, T. V.; Schaefer, J. M.; Finkel, R. C.</p> <p>2008-12-01</p> <p>Quelccaya <span class="hlt">Ice</span> Cap in the southeastern Peruvian Andes (~13-14° S latitude) is an icon for climate change. Its rapidly receding outlet, Qori Kalis Glacier, has been monitored since the 1970's. Cores from Quelccaya <span class="hlt">Ice</span> Cap provide high-resolution information about temperature and precipitation during the past 1,500 years. We extend the understanding of past changes in Quelccaya <span class="hlt">Ice</span> Cap based on mapping and dating of glacial moraines and associated deposits. Our results include fifty 10Be ages of moraines and bedrock as well as twenty-nine 14C ages of organic material associated with moraines. These results form the basis of a chronology of changes in Quelccaya <span class="hlt">Ice</span> Cap from ~16,000 yr BP to late Holocene time. Results from 10Be and 14C dating indicate that Quelccaya <span class="hlt">Ice</span> Cap experienced a significant advance at 12,700-11,400 yr BP. Subsequent to this advance, the <span class="hlt">ice</span> <span class="hlt">margin</span> deposited at least three recessional moraine sets. Quelccaya <span class="hlt">Ice</span> Cap receded to near its present-day <span class="hlt">margin</span> by ~10,000 yr BP. Neoglacial advances began by ~3,000 yr BP and culminated with a maximum advance during the Little <span class="hlt">Ice</span> Age. This chronology fits well with prior work which indicates a restricted Quelccaya <span class="hlt">Ice</span> Cap during middle Holocene time. Moreover, the overlap between moraine and <span class="hlt">ice</span> core data for the last 1,500 years provides a unique opportunity to assess the influences of temperature and precipitation on past <span class="hlt">ice</span> cap extents.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.T41D2966S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.T41D2966S"><span>Core-seismic investigation of Surveyor Channel tributaries: Glacial history of the southern Alaskan <span class="hlt">margin</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Somchat, K.; Reece, R.; Gulick, S. P. S.; Asahi, H.; Mix, A. C.</p> <p>2016-12-01</p> <p>The low angle subduction and collision of the Yakutat microplate with the North America Plate created, and continues to contribute to the uplift of the Chugach-St. Elias Range. This heavily glaciated, high topography proximal to the shoreline creates a unique source-to-sink system in which glacial sediment is transported and preserved offshore in a deep sea fan without much interruption. The product of this sediment is the Surveyor Fan and Channel system. Four tributary channels form the head of the Surveyor Channel complex and merge into the main channel trunk 200 km from the shelf edge. We integrate drill core and seismic reflection data to study the evolution of these tributaries in order to decipher glacial history of the southern Alaskan <span class="hlt">margin</span> since the mid-Pleistocene (1.2 Ma). Updated age models from Integrated Ocean Drilling Program Expedition 341 Sites U1417 and U1418 provide a higher resolution chronology of sediment delivery to the Surveyor Fan than previous studies. We regionally extended the mapping of seismic subunits previously identified by Exp. 341 scientists at sites U1417 and U1418 and analyzed regional patterns of sediment deposition. Two-way travel time (isopach) maps of the three subunits show a trend of sediment depocenter shifting to the east since 1.2 Ma, where the Yakutat and Alsek tributaries have increasing sediment flux through time. Changes in sediment flux in each system represent the changes in locations and amplitudes of glacial <span class="hlt">ice</span> over successive glacial intervals. Additionally, seismic analysis of channel geomorphology shows that each system contains distinct geomorphological evolutions. Since glacial erosion provides the sediment for the fan, the history of glacial <span class="hlt">ice</span> onshore can be inferred from seismic geomorphology, where changes in glacial <span class="hlt">ice</span> affect sediment supply and therefore shifts in depocenters and sedimentation pathways. This study shows an interaction between glacial <span class="hlt">activity</span> onshore and deep sea fan sediment</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018TCry...12.1867S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018TCry...12.1867S"><span>Snow depth on Arctic sea <span class="hlt">ice</span> from historical in situ data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shalina, Elena V.; Sandven, Stein</p> <p>2018-06-01</p> <p>The snow data from the Soviet airborne expeditions Sever in the Arctic collected over several decades in March, April and May have been analyzed in this study. The Sever data included more measurements and covered a much wider area, particularly in the Eurasian <span class="hlt">marginal</span> seas (Kara Sea, Laptev Sea, East Siberian Sea and Chukchi Sea), compared to the Soviet North Pole drifting stations. The latter collected data mainly in the central part of the Arctic Basin. The following snow parameters have been analyzed: average snow depth on the level <span class="hlt">ice</span> (undisturbed snow) height and area of sastrugi, depth of snow dunes attached to <span class="hlt">ice</span> ridges and depth of snow on hummocks. In the 1970s-1980s, in the central Arctic, the average depth of undisturbed snow was 21.2 cm, the depth of sastrugi (that occupied about 30 % of the <span class="hlt">ice</span> surface) was 36.2 cm and the average depth of snow near hummocks and ridges was about 65 cm. For the <span class="hlt">marginal</span> seas, the average depth of undisturbed snow on the level <span class="hlt">ice</span> varied from 9.8 cm in the Laptev Sea to 15.3 cm in the East Siberian Sea, which had a larger fraction of multiyear <span class="hlt">ice</span>. In the <span class="hlt">marginal</span> seas the spatial variability of snow depth was characterized by standard deviation varying between 66 and 100 %. The average height of sastrugi varied from 23 cm to about 32 cm with standard deviation between 50 and 56 %. The average area covered by sastrugi in the <span class="hlt">marginal</span> seas was estimated to be 36.5 % of the total <span class="hlt">ice</span> area where sastrugi were observed. The main result of the study is a new snow depth climatology for the late winter using data from both the Sever expeditions and the North Pole drifting stations. The snow load on the <span class="hlt">ice</span> observed by Sever expeditions has been described as a combination of the depth of undisturbed snow on the level <span class="hlt">ice</span> and snow depth of sastrugi weighted in proportion to the sastrugi area. The height of snow accumulated near the <span class="hlt">ice</span> ridges was not included in the calculations because there are no estimates of the area</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110012877','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110012877"><span>Evaluation of Arctic Sea <span class="hlt">Ice</span> Thickness Simulated by AOMIP Models</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Johnson, Mark; Proshutinsky, Andrey; Aksenov, Yevgeny; Nguyen, An T.; Lindsay, Ron; Haas, Christian; Zhang, Jinlun; Diansky, Nimolay; Kwok, Ron; Maslowski, Wieslaw; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20110012877'); toggleEditAbsImage('author_20110012877_show'); toggleEditAbsImage('author_20110012877_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20110012877_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20110012877_hide"></p> <p>2011-01-01</p> <p>We compare results from six AOMIP model simulations with estimates of sea <span class="hlt">ice</span> thickness obtained from ICESat, moored and submarine-based upward looking sensors, airborne electromagnetic measurements and drill holes. Our goal is to find patterns of model performance to guide model improvement. The satellite data is pan-arctic from 2004-2008, <span class="hlt">ice</span>-draft data is from moored instruments in Fram Strait, the Greenland Sea and the Beaufort Sea from 1992-2008 and from submarines from 1975-2000. The drill hole data are from the Laptev and East Siberian <span class="hlt">marginal</span> seas from 1982-1986 and from coastal stations from 1998-2009. While there are important caveats when comparing modeled results with measurements from different platforms and time periods such as these, the models agree well with moored ULS data. In general, the AOMIP models underestimate the thickness of measured <span class="hlt">ice</span> thicker than about 2 m and overestimate thickness of <span class="hlt">ice</span> thinner than 2 m. The simulated results are poor over the fast <span class="hlt">ice</span> and <span class="hlt">marginal</span> seas of the Siberian shelves. Averaging over all observational data sets, the better correlations and smaller differences from observed thickness are from the ECCO2 and UW models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014QSRv..100...31A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014QSRv..100...31A"><span>Ross Sea paleo-<span class="hlt">ice</span> sheet drainage and deglacial history during and since the LGM</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Anderson, John B.; Conway, Howard; Bart, Philip J.; Witus, Alexandra E.; Greenwood, Sarah L.; McKay, Robert M.; Hall, Brenda L.; Ackert, Robert P.; Licht, Kathy; Jakobsson, Martin; Stone, John O.</p> <p>2014-09-01</p> <p>Onshore and offshore studies show that an expanded, grounded <span class="hlt">ice</span> sheet occupied the Ross Sea Embayment during the Last Glacial Maximum (LGM). Results from studies of till provenance and the orientation of geomorphic features on the continental shelf show that more than half of the grounded <span class="hlt">ice</span> sheet consisted of East Antarctic <span class="hlt">ice</span> flowing through Transantarctic Mountain (TAM) outlet glaciers; the remainder came from West Antarctica. Terrestrial data indicate little or no thickening in the upper catchment regions in both West and East Antarctica during the LGM. In contrast, evidence from the mouths of the southern and central TAM outlet glaciers indicate surface elevations between 1000 m and 1100 m (above present-day sea level). Farther north along the western <span class="hlt">margin</span> of the Ross <span class="hlt">Ice</span> Sheet, surface elevations reached 720 m on Ross Island, and 400 m at Terra Nova Bay. Evidence from Marie Byrd Land at the eastern <span class="hlt">margin</span> of the <span class="hlt">ice</span> sheet indicates that the elevation near the present-day grounding line was more than 800 m asl, while at Siple Dome in the central Ross Embayment, the surface elevation was about 950 m asl. Farther north, evidence that the <span class="hlt">ice</span> sheet was grounded on the middle and the outer continental shelf during the LGM implies that surface elevations had to be at least 100 m above the LGM sea level. The apparent low surface profile and implied low basal shear stress in the central and eastern embayment suggests that although the <span class="hlt">ice</span> streams may have slowed during the LGM, they remained <span class="hlt">active</span>. <span class="hlt">Ice</span>-sheet retreat from the western Ross Embayment during the Holocene is constrained by marine and terrestrial data. Ages from marine sediments suggest that the grounding line had retreated from its LGM outer shelf location only a few tens of kilometer to a location south of Coulman Island by ˜13 ka BP. The <span class="hlt">ice</span> sheet <span class="hlt">margin</span> was located in the vicinity of the Drygalski <span class="hlt">Ice</span> Tongue by ˜11 ka BP, just north of Ross Island by ˜7.8 ka BP, and near Hatherton Glacier by </p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C51F..01D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C51F..01D"><span>The geomorphic signature of past <span class="hlt">ice</span> sheets in the marine record</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dowdeswell, J. A.</p> <p>2016-12-01</p> <p>The deglaciation of high-latitude continental shelves since the Last Glacial Maximum has revealed suites of subglacial and <span class="hlt">ice</span>-contact landforms that have remained well-preserved beneath tens to hundreds of metres of water. Once <span class="hlt">ice</span> has retreated, sedimentation is generally low on polar shelves during interglacials and the submarine landforms have not, therefore, been buried by subsequent sedimentation. By contrast, the beds of modern <span class="hlt">ice</span> sheets are hidden by several thousand metres of <span class="hlt">ice</span>, which is much more difficult than water to penetrate using geophysical methods. These submarine glacial landforms provide insights into past <span class="hlt">ice</span>-sheet form and flow, and information on the processes that have taken place beneath former <span class="hlt">ice</span> sheets. Examples will be shown of streamlined subglacial landforms that indicate the distribution and dimensions of former <span class="hlt">ice</span> streams on high-latitde continental <span class="hlt">margins</span>. Distinctive landform assemblages characterise <span class="hlt">ice</span> stream and inter-<span class="hlt">ice</span> stream areas. Landforms, including subglacially formed channel systems in inner- and mid-shelf areas, and the lack of them on sedimentary outer shelves, allow inferences to be made about subglacial hydrology. The distribution of grounding-zone wedges and other transverse moraine ridges also provides evidence on the nature of <span class="hlt">ice</span>-sheet retreat - whether by rapid collapse, episodic retreat or by the slow retreat of grounded <span class="hlt">ice</span>. Such information can be used to test the predictive capability of <span class="hlt">ice</span>-sheet numerical models. These marine geophysical and geological observations of submarine glacial landforms enhance our understanding of the form and flow of past <span class="hlt">ice</span> masses at scales ranging from <span class="hlt">ice</span> sheets (1000s of km in flow-line and <span class="hlt">margin</span> length), through <span class="hlt">ice</span> streams (100s of km long), to surge-type glaciers (10s of km long).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4729839','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4729839"><span><span class="hlt">Ice</span>-sheet-driven methane storage and release in the 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>Portnov, Alexey; Vadakkepuliyambatta, Sunil; Mienert, Jürgen; Hubbard, Alun</p> <p>2016-01-01</p> <p>It is established that late-twentieth and twenty-first century ocean warming has forced dissociation of gas hydrates with concomitant seabed methane release. However, recent dating of methane expulsion sites suggests that gas release has been ongoing over many millennia. Here we synthesize observations of ∼1,900 fluid escape features—pockmarks and <span class="hlt">active</span> gas flares—across a previously glaciated Arctic <span class="hlt">margin</span> with <span class="hlt">ice</span>-sheet thermomechanical and gas hydrate stability zone modelling. Our results indicate that even under conservative estimates of <span class="hlt">ice</span> thickness with temperate subglacial conditions, a 500-m thick gas hydrate stability zone—which could serve as a methane sink—existed beneath the <span class="hlt">ice</span> sheet. Moreover, we reveal that in water depths 150–520 m methane release also persisted through a 20-km-wide window between the subsea and subglacial gas hydrate stability zone. This window expanded in response to post-glacial climate warming and deglaciation thereby opening the Arctic shelf for methane release. PMID:26739497</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2012-12-27/pdf/2012-31126.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2012-12-27/pdf/2012-31126.pdf"><span>77 FR 76318 - Self-Regulatory Organizations; <span class="hlt">ICE</span> Clear Europe Limited; Notice of Filing and Immediate...</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2012-12-27</p> <p>... Methodology is an enhancement to the SPAN for the <span class="hlt">ICE</span> <span class="hlt">Margining</span> algorithm employed to calculate Original... <span class="hlt">Margining</span> algorithm employed to calculate Original <span class="hlt">Margin</span> and was designed to optimize and improve <span class="hlt">margin</span>... framework algorithm. The enhancement will be additionally applied to: GOA: Gas Oil 1-Month CSO; BRZ: Brent...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GeoRL..43.6775H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GeoRL..43.6775H"><span>Recent tectonic <span class="hlt">activity</span> on Pluto driven by phase changes in the <span class="hlt">ice</span> shell</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hammond, Noah P.; Barr, Amy C.; Parmentier, Edgar M.</p> <p>2016-07-01</p> <p>The New Horizons spacecraft has found evidence for geologic <span class="hlt">activity</span> on the surface of Pluto, including extensional tectonic deformation of its water <span class="hlt">ice</span> bedrock see Moore et al. (2016). One mechanism that could drive extensional tectonic <span class="hlt">activity</span> is global surface expansion due to the partial freezing of an ocean. We use updated physical properties for Pluto and simulate its thermal evolution to understand the survival of a possible subsurface ocean. For thermal conductivities of rock less than 3 W m-1 K-1, an ocean forms and at least partially freezes, leading to recent extensional stresses in the <span class="hlt">ice</span> shell. In scenarios where the ocean freezes and the <span class="hlt">ice</span> shell is thicker than 260 km, <span class="hlt">ice</span> II forms and causes global volume contraction. Since there is no evidence for recent compressional tectonic features, we argue that <span class="hlt">ice</span> II has not formed and that Pluto's ocean has likely survived to present day.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_15 --> <div id="page_16" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="301"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014GeoRL..41.5506D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014GeoRL..41.5506D"><span>Basal terraces on melting <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>Dutrieux, Pierre; Stewart, Craig; Jenkins, Adrian; Nicholls, Keith W.; Corr, Hugh F. J.; Rignot, Eric; Steffen, Konrad</p> <p>2014-08-01</p> <p>Ocean waters melt the <span class="hlt">margins</span> of Antarctic and Greenland glaciers, and individual glaciers' responses and the integrity of their <span class="hlt">ice</span> shelves are expected to depend on the spatial distribution of melt. The bases of the <span class="hlt">ice</span> shelves associated with Pine Island Glacier (West Antarctica) and Petermann Glacier (Greenland) have similar geometries, including kilometer-wide, hundreds-of-meter high channels oriented along and across the direction of <span class="hlt">ice</span> flow. The channels are enhanced by, and constrain, oceanic melt. New meter-scale observations of basal topography reveal peculiar glaciated landscapes. Channel flanks are not smooth, but are instead stepped, with hundreds-of-meters-wide flat terraces separated by 5-50 m high walls. Melting is shown to be modulated by the geometry: constant across each terrace, changing from one terrace to the next, and greatly enhanced on the ~45° inclined walls. Melting is therefore fundamentally heterogeneous and likely associated with stratification in the <span class="hlt">ice</span>-ocean boundary layer, challenging current models of <span class="hlt">ice</span> shelf-ocean interactions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.C32B..06D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.C32B..06D"><span>Basal Terraces on Melting <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>Dutrieux, P.; Stewart, C.; Jenkins, A.; Nicholls, K. W.; Corr, H. F. J.; Rignot, E. J.; Steffen, K.</p> <p>2014-12-01</p> <p>Ocean waters melt the <span class="hlt">margins</span> of Antarctic and Greenland glaciers and individualglaciers' responses and the integrity of their <span class="hlt">ice</span> shelves are expected to depend on thespatial distribution of melt. The bases of the <span class="hlt">ice</span> shelves associated with Pine IslandGlacier (West Antarctica) and Petermann Glacier (Greenland) have similar geometries,including kilometers-wide, hundreds-of-meter-high channels oriented along and acrossthe direction of <span class="hlt">ice</span> flow. The channels are enhanced by, and constrain, oceanic melt.New, meter-scale observations of basal topography reveal peculiar glaciated landscapes.Channel flanks are not smooth, but are instead stepped, with hundreds-of-meters-wideflat terraces separated by 5-50 m-high walls. Melting is shown to be modulated by thegeometry: constant across each terrace, changing from one terrace to the next, and greatlyenhanced on the ~45°-inclined walls. Melting is therefore fundamentally heterogeneousand likely associated with stratification in the <span class="hlt">ice</span>-ocean boundary layer, challengingcurrent models of <span class="hlt">ice</span> shelf-ocean interactions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70014093','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70014093"><span>Glaciotectonic origin of the Massachusetts coastal end moraines and a fluctuating late Wisconsinan <span class="hlt">ice</span> <span class="hlt">margin</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>Oldale, R.N.; O'Hara, C. J.</p> <p>1984-01-01</p> <p>Late Wisconsinan end moraines on Cape Cod and islands south and west of Cape Cod are believed to be glaciotectonic features formed by advancing <span class="hlt">ice</span> fronts. Evidence for major <span class="hlt">ice</span> readvances during general recession includes the moraines themselves, till atop stratified drift, and the numerous basal tills that are inferred to exist beneath Cape Cod Bay. The Thompson Glacier end moraine in the Canadian Arctic Archipelago is considered to be a modern example of how late Wisconsinan end moraines on Cape Cod and the islands were formed. It is overriding its outwash plain, displacing outwash deposits forward and upward beyond the <span class="hlt">ice</span> front. New sheets are added to the base of the moraine as the <span class="hlt">ice</span> overrides it. Retreat of the <span class="hlt">ice</span> from Cape Cod and the islands may have been similar to the retreat of the Lake Michigan lobe, deposits of which contain evidence of at least 12 moraine-building episodes caused by readvancing <span class="hlt">ice</span>.-from Authors</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110015207','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110015207"><span>Regional Changes in the Sea <span class="hlt">Ice</span> Cover and <span class="hlt">Ice</span> Production in the Antarctic</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>2011-01-01</p> <p>Coastal polynyas around the Antarctic continent have been regarded as sea <span class="hlt">ice</span> factories because of high <span class="hlt">ice</span> production rates in these regions. The observation of a positive trend in the extent of Antarctic sea <span class="hlt">ice</span> during the satellite era has been intriguing in light of the observed rapid decline of the <span class="hlt">ice</span> 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 <span class="hlt">marginal</span> <span class="hlt">ice</span> 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 <span class="hlt">ice</span> cover could be caused primarily by enhanced <span class="hlt">ice</span> 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 <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 km2 per year. For a characteristic <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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-<span class="hlt">ice</span> shelf.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28851908','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28851908"><span>Arctic Ocean sea <span class="hlt">ice</span> cover during the penultimate glacial and the last interglacial.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Stein, Ruediger; Fahl, Kirsten; Gierz, Paul; Niessen, Frank; Lohmann, Gerrit</p> <p>2017-08-29</p> <p>Coinciding with global warming, Arctic sea <span class="hlt">ice</span> has rapidly decreased during the last four decades and climate scenarios suggest that sea <span class="hlt">ice</span> may completely disappear during summer within the next about 50-100 years. Here we produce Arctic sea <span class="hlt">ice</span> biomarker proxy records for the penultimate glacial (Marine Isotope Stage 6) and the subsequent last interglacial (Marine Isotope Stage 5e). The latter is a time interval when the high latitudes were significantly warmer than today. We document that even under such warmer climate conditions, sea <span class="hlt">ice</span> existed in the central Arctic Ocean during summer, whereas sea <span class="hlt">ice</span> was significantly reduced along the Barents Sea continental <span class="hlt">margin</span> influenced by Atlantic Water inflow. Our proxy reconstruction of the last interglacial sea <span class="hlt">ice</span> cover is supported by climate simulations, although some proxy data/model inconsistencies still exist. During late Marine Isotope Stage 6, polynya-type conditions occurred off the major <span class="hlt">ice</span> sheets along the northern Barents and East Siberian continental <span class="hlt">margins</span>, contradicting a giant Marine Isotope Stage 6 <span class="hlt">ice</span> shelf that covered the entire Arctic Ocean.Coinciding with global warming, Arctic sea <span class="hlt">ice</span> has rapidly decreased during the last four decades. Here, using biomarker records, the authors show that permanent sea <span class="hlt">ice</span> was still present in the central Arctic Ocean during the last interglacial, when high latitudes were warmer than present.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C21A0658Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C21A0658Z"><span>Changes in Arctic Sea <span class="hlt">Ice</span> Thickness and Floe Size</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, J.; Schweiger, A. J. B.; Stern, H. L., III; Steele, M.</p> <p>2016-12-01</p> <p>A thickness, floe size, and enthalpy distribution sea <span class="hlt">ice</span> model was implemented into the Pan-arctic <span class="hlt">Ice</span>-Ocean Modeling and Assimilation System (PIOMAS) by coupling the Zhang et al. [2015] sea <span class="hlt">ice</span> floe size distribution (FSD) theory with the Thorndike et al. [1975] <span class="hlt">ice</span> thickness distribution (ITD) theory in order to explicitly simulate multicategory FSD and ITD simultaneously. A range of <span class="hlt">ice</span> thickness and floe size observations were used for model calibration and validation. The expanded, validated PIOMAS was used to study sea <span class="hlt">ice</span> response to atmospheric and oceanic changes in the Arctic, focusing on the interannual variability and trends of <span class="hlt">ice</span> thickness and floe size over the period 1979-2015. It is found that over the study period both <span class="hlt">ice</span> thickness and floe size have been decreasing steadily in the Arctic. The simulated <span class="hlt">ice</span> thickness shows considerable spatiotemporal variability in recent years. As the <span class="hlt">ice</span> cover becomes thinner and weaker, the model simulates an increasing number of small floes (at the low end of the FSD), which affects sea <span class="hlt">ice</span> properties, particularly in the <span class="hlt">marginal</span> <span class="hlt">ice</span> zone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26407233','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26407233"><span>Latent <span class="hlt">Ice</span> Recrystallization Inhibition <span class="hlt">Activity</span> in Nonantifreeze Proteins: Ca2+-<span class="hlt">Activated</span> Plant Lectins and Cation-<span class="hlt">Activated</span> Antimicrobial Peptides.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mitchell, Daniel E; Gibson, Matthew I</p> <p>2015-10-12</p> <p>Organisms living in polar regions have evolved a series of antifreeze (glyco) proteins (AFGPs) to enable them to survive by modulating the structure of <span class="hlt">ice</span>. These proteins have huge potential for use in cellular cryopreservation, <span class="hlt">ice</span>-resistant surfaces, frozen food, and cryosurgery, but they are limited by their relatively low availability and questions regarding their mode of action. This has triggered the search for biomimetic materials capable of reproducing this function. The identification of new structures and sequences capable of inhibiting <span class="hlt">ice</span> growth is crucial to aid our understanding of these proteins. Here, we show that plant c-type lectins, which have similar biological function to human c-type lectins (glycan recognition) but no sequence homology to AFPs, display calcium-dependent <span class="hlt">ice</span> recrystallization inhibition (IRI) <span class="hlt">activity</span>. This IRI <span class="hlt">activity</span> can be switched on/off by changing the Ca2+ concentration. To show that more (nonantifreeze) proteins may exist with the potential to display IRI, a second motif was considered, amphipathicity. All known AFPs have defined hydrophobic/hydrophilic domains, rationalizing this choice. The cheap, and widely used, antimicrobial Nisin was found to have cation-dependent IRI <span class="hlt">activity</span>, controlled by either acid or addition of histidine-binding ions such as zinc or nickel, which promote its amphipathic structure. These results demonstrate a new approach in the identification of antifreeze protein mimetic macromolecules and may help in the development of synthetic mimics of AFPs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1912834H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1912834H"><span>The <span class="hlt">Ice</span> Nucleation <span class="hlt">Activity</span> of Surface Modified Soot</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Häusler, Thomas; Witek, Lorenz; Felgitsch, Laura; Hitzenberger, Regina; Grothe, Hinrich</p> <p>2017-04-01</p> <p>The <span class="hlt">ice</span> nucleation efficiency of many important atmospheric particles remains poorly understood. Since soot is ubiquitous in the Earth's troposphere, they might have the potential to significantly impact the Earth's climate (Finlayson-Pitts and Pitts, 2000; Seinfeld and Pandis, 1998). Here we present the <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> (INA) in immersion freezing mode of different types of soot. Therefor a CAST (combustion aerosol standard) generator was used to produce different kinds of soot samples. The CAST generator combusts a propane-air-mixture and deposits thereby produced soot on a polyvinyl fluoride filter. By varying the propane to air ratio, the amount of organic portion of the soot can be varied from black carbon (BC) with no organic content to brown carbon (BrC) with high organic content. To investigate the impact of functional sites of <span class="hlt">ice</span> nuclei (IN), the soot samples were exposed to NO2 gas for a certain amount of time (30 to 360 minutes) to chemically modify the surface. Immersion freezing experiments were carried out in a unique reaction gadget. In this device a water-in-oil suspension (with the soot suspended in the aqueous phase) was cooled till the freezing point and was observed through a microscope (Pummer et al., 2012; Zolles et al., 2015) It was found that neither modified nor unmodified BC shows INA. On the contrary, unmodified BrC shows an INA at -32˚ C, which can be increased up to -20˚ C. The INA of BrC depends on the duration of NO2- exposure. To clarify the characteristics of the surface modifications, surface sensitive analysis like infrared spectroscopy and X-ray photoelectron spectroscopy were carried out. Finlayson-Pitts, B. J. and Pitts, J. N. J.: Chemistry of the Upper and Lower Atmosphere, Elsevier, New York, 2000. Pummer, B. G., Bauer, H., Bernardi, J., Bleicher, S., and Grothe, H.: Suspendable macromolecules are responsible for <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> of birch and conifer pollen, Atmos Chem Phys, 12, 2541-2550, 2012. Seinfeld, J</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T22D..06T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T22D..06T"><span>New Crustal Boundary Revealed Beneath the Ross <span class="hlt">Ice</span> Shelf, Antarctica, through ROSETTA-<span class="hlt">Ice</span> Integrated Aerogeophysics, Geology, and Ocean Research</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tinto, K. J.; Siddoway, C. S.; Bell, R. E.; Lockett, A.; Wilner, J.</p> <p>2017-12-01</p> <p>Now submerged within marine plateaus and rises bordering Antarctica, Australia and Zealandia, the East Gondwana accretionary <span class="hlt">margin</span> was a belt of terranes and stitched by magmatic arcs, later stretched into continental ribbons separated by narrow elongate rifts. This crustal architecture is known from marine geophysical exploration and ocean drilling of the mid-latitude coastal plateaus and rises. A concealed sector of the former East Gondwana <span class="hlt">margin</span> that underlies the Ross <span class="hlt">Ice</span> Shelf (RIS), Antarctica, is the focus of ROSETTA-<span class="hlt">ICE</span>, a new airborne data acquisition campaign that explores the crustal makeup, tectonic boundaries and seafloor bathymetry beneath RIS. Gravimeters and a magnetometer are deployed by LC130 aircraft surveying along E-W lines spaced at 10 km, and N-S tie lines at 55 km, connect 1970s points (RIGGS) for controls on ocean depth and gravity. The ROSETTA-<span class="hlt">ICE</span> survey, 2/3 completed thus far, provides magnetic anomalies, Werner depth-to-basement solutions, a new gravity-based bathymetric model at 20-km resolution, and a new crustal density map tied to the 1970s data. Surprisingly, the data reveal that the major lithospheric boundary separating East and West Antarctica lies 300 km east of the Transantarctic Mountains, beneath the floating RIS. The East and West regions have contrasting geophysical characteristics and bathymetry, with relatively dense lithosphere, low amplitude magnetic anomalies, and deep bathymetry on the East Antarctica side, and high amplitude magnetic anomalies, lower overall density and shallower water depths on the West Antarctic side. The Central High, a basement structure cored at DSDP Site 270 and seismically imaged in the Ross Sea, continues beneath RIS as a faulted but coherent crustal ribbon coincident with the tectonic boundary. The continuity of Gondwana <span class="hlt">margin</span> crustal architecture discovered beneath the West Antarctic <span class="hlt">Ice</span> Sheet requires a revision of the existing tectonic framework. The sub-RIS narrow rift basins and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20000101018&hterms=Antarctic+icebergs&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DAntarctic%2Bicebergs','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20000101018&hterms=Antarctic+icebergs&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DAntarctic%2Bicebergs"><span><span class="hlt">Active</span> Microwave Remote Sensing Observations of Weddell 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>Drinkwater, Mark R.</p> <p>1997-01-01</p> <p>Since July 1991, the European Space Agency's ERS-1 and ERS-2 satellites have acquired radar data of the Weddell Sea, Antarctica. The <span class="hlt">Active</span> Microwave Instrument on board ERS has two modes; SAR and Scatterometer. Two receiving stations enable direct downlink and recording of high bit-rate, high resolution SAR image data of this region. When not in an imaging mode, when direct SAR downlink is not possible, or when a receiving station is inoperable, the latter mode allows normalized radar cross-section data to be acquired. These low bit-rate ERS scatterometer data are tape recorded, downlinked and processed off-line. Recent advances in image generation from Scatterometer backscatter measurements enable complementary medium-scale resolution images to be made during periods when SAR images cannot be acquired. Together, these combined C-band microwave image data have for the first time enabled uninterrupted night and day coverage of the Weddell Sea region at both high (25 m) and medium-scale (-20 km) resolutions. C-band ERS-1 radar data are analyzed in conjunction with field data from two simultaneous field experiments in 1992. Satellite radar signature data are compared with shipborne radar data to extract a regional and seasonal signature database for recognition of <span class="hlt">ice</span> types in the images. Performance of automated sea-<span class="hlt">ice</span> tracking algorithms is tested on Antarctic data to evaluate their success. Examples demonstrate that both winter and summer <span class="hlt">ice</span> can be effectively tracked. The kinematics of the main <span class="hlt">ice</span> zones within the Weddell Sea are illustrated, together with the complementary time-dependencies in their radar signatures. Time-series of satellite images are used to illustrate the development of the Weddell Sea <span class="hlt">ice</span> cover from its austral summer minimum (February) to its winter maximum (September). The combination of time-dependent microwave signatures and <span class="hlt">ice</span> dynamics tracking enable various drift regimes to be defined which relate closely to the circulation of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19880015729','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19880015729"><span>National plans for aircraft <span class="hlt">icing</span> and improved aircraft <span class="hlt">icing</span> forecasts and associated warning services</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Pass, Ralph P.</p> <p>1988-01-01</p> <p>Recently, the United States has increased its <span class="hlt">activities</span> related to aircraft <span class="hlt">icing</span> in numerous fields: <span class="hlt">ice</span> phobics, revised characterization of <span class="hlt">icing</span> conditions, instrument development/evaluation, de-<span class="hlt">ice/anti-ice</span> devices, simulated supercooled clouds, computer simulation and flight tests. The Federal Coordinator for Meteorology is involved in two efforts, one a National Plan on Aircraft <span class="hlt">Icing</span> and the other a plan for Improved Aircraft <span class="hlt">Icing</span> Forecasts and Associated Warning Services. These two plans will provide an approved structure for future U.S. <span class="hlt">activities</span> related to aircraft <span class="hlt">icing</span>. The recommended <span class="hlt">activities</span> will significantly improve the position of government agencies to perform mandated <span class="hlt">activities</span> and to enable U.S. manufacturers to be competitive in the world market.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.P11D..03P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.P11D..03P"><span>Refractory Organic Compounds in Enceladus' <span class="hlt">Ice</span> Grains and Hydrothermal <span class="hlt">Activity</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Postberg, F.; Khawaja, N.; Hsu, H. W.; Sekine, Y.; Shibuya, T.</p> <p>2015-12-01</p> <p>Cassini's Cosmic Dust Analyzer (CDA) generates time-of-flight mass spectra of individual grains impinging on the instruments target-plate. Following the analysis of salt rich <span class="hlt">ice</span> grains emitted by Enceladus that indicated a salt-water ocean in contact with the moon's rocky core [1,2] a recent CDA analysis of nano-phase silica particles pointed at hydrothermal <span class="hlt">activity</span> at the moon's rock/water interface [3]. The results imply temperatures above 80 - 90°C and alkaline pH values around 10 reminiscent of alkaline hydrothermal vents on Earth like the Lost City Hydrothermal Field. In this context the compositional analysis of organic components in CDA mass spectra of the ejected <span class="hlt">ice</span> grains is of particular relevance. A multitude of volatile organic species has already been identified in the gas component of the plume [4]. As expected, we find more complex organic molecules in <span class="hlt">ice</span> grains than in the gas indicating aromatic species, amines, and carbonyl group species. The composition of organic-bearing <span class="hlt">ice</span> grains displays a great diversity indicating a variety of different organic species in varying concentrations. Recent spatially resolved CDA in situ measurements inside Enceladus' plume indicate that these organic compounds are especially frequent in 'young' <span class="hlt">ice</span> grains that have just been ejected by high velocity jets. We investigate the implications of our findings with respect to <span class="hlt">ice</span> grain formation at the water surface and inside the icy vents. We constrain the generation of organic compounds at the rock/water interface in the light of hydrothermal <span class="hlt">activity</span> and the potential for the formation of life precursor molecules in Enceladus' ocean. Ref:[1] Postberg et al., Nature 459, 1098-1101 (2009). [2] Postberg et al., Nature 474, 620-622 (2011). [3]. Hsu, Postberg, Sekine et al., Nature, 519, 207-210 (2015). [4] Waite et al., Nature 460, 487-490 (2009).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.C44A..06B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.C44A..06B"><span>Widespread Refreezing of Both Surface and Basal Melt Water Beneath the Greenland <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>Bell, R. E.; Tinto, K. J.; Das, I.; Wolovick, M.; Chu, W.; Creyts, T. T.; Frearson, N.</p> <p>2013-12-01</p> <p>The isotopically and chemically distinct, bubble-free <span class="hlt">ice</span> observed along the Greenland <span class="hlt">Ice</span> Sheet <span class="hlt">margin</span> both in the Russell Glacier and north of Jacobshavn must have formed when water froze from subglacial networks. Where this refreezing occurs and what impact it has on <span class="hlt">ice</span> sheet processes remain unclear. We use airborne radar data to demonstrate that freeze-on to the <span class="hlt">ice</span> sheet base and associated deformation produce large <span class="hlt">ice</span> units up to 700 m thick throughout northern Greenland. Along the <span class="hlt">ice</span> sheet <span class="hlt">margin</span>, in the ablation zone, surface meltwater, delivered via moulins, refreezes to the <span class="hlt">ice</span> sheet base over rugged topography. In the interior, water melted from the <span class="hlt">ice</span> sheet base is refrozen and surrounded by folded <span class="hlt">ice</span>. A significant fraction of the <span class="hlt">ice</span> sheet is modified by basal freeze-on and associated deformation. For the Eqip and Petermann catchments, representing the <span class="hlt">ice</span> sheet <span class="hlt">margin</span> and interior respectively, extensive airborne radar datasets show that 10%-13% of the base of the <span class="hlt">ice</span> sheet and up to a third of the catchment width is modified by basal freeze-on. The interior units develop over relatively subdued topography with modest water flux from basal melt where conductive cooling likely dominates. Steps in the bed topography associated with subglacial valley networks may foster glaciohydraulic supercooling. The ablation zone units develop where both surface melt and crevassing are widespread and large volumes of surface meltwater will reach the base of the <span class="hlt">ice</span> sheet. The relatively steep topography at the upslope edge of the ablation zone units combined with the larger water flux suggests that supercooling plays a greater role in their formation. The <span class="hlt">ice</span> qualities of the ablation zone units should reflect the relatively fresh surface melt whereas the chemistry of the interior units should reflect solute-rich basal melt. Changes in basal conditions such as the presence of till patches may contribute to the formation of the large basal units near the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMPP54A..05R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMPP54A..05R"><span>The dynamics of climate-induced deglacial <span class="hlt">ice</span> stream acceleration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Robel, A.; Tziperman, E.</p> <p>2015-12-01</p> <p>Geological observations indicate that <span class="hlt">ice</span> streams were a significant contributor to <span class="hlt">ice</span> flow in the Laurentide <span class="hlt">Ice</span> Sheet during the Last Glacial Maximum. Conceptual and simple model studies have also argued that the gradual development of <span class="hlt">ice</span> streams increases the sensitivity of large <span class="hlt">ice</span> sheets to weak climate forcing. In this study, we use an idealized configuration of the Parallel <span class="hlt">Ice</span> Sheet Model to explore the role of <span class="hlt">ice</span> streams in rapid deglaciation. In a growing <span class="hlt">ice</span> sheet, <span class="hlt">ice</span> streams develop gradually as the bed warms and the <span class="hlt">margin</span> expands outward onto the continental shelf. Then, a weak change in equilibrium line altitude commensurate with Milankovitch forcing results in a rapid deglacial response, as <span class="hlt">ice</span> stream acceleration leads to enhanced calving and surface melting at low elevations. We explain the dynamical mechanism that drives this <span class="hlt">ice</span> stream acceleration and its broader applicability as a feedback for enhancing <span class="hlt">ice</span> sheet decay in response to climate forcing. We show how our idealized <span class="hlt">ice</span> sheet simulations match geomorphological observations of deglacial <span class="hlt">ice</span> stream variability and previous model-data analyses. We conclude with observations on the potential for interaction between <span class="hlt">ice</span> streams and other feedback mechanisms within the earth system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=321258','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=321258"><span>Bacterial <span class="hlt">Activity</span> at −2 to −20°C in Arctic Wintertime Sea <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>Junge, Karen; Eicken, Hajo; Deming, Jody W.</p> <p>2004-01-01</p> <p>Arctic wintertime sea-<span class="hlt">ice</span> cores, characterized by a temperature gradient of −2 to −20°C, were investigated to better understand constraints on bacterial abundance, <span class="hlt">activity</span>, and diversity at subzero temperatures. With the fluorescent stains 4′,6′-diamidino-2-phenylindole 2HCl (DAPI) (for DNA) and 5-cyano-2,3-ditoyl tetrazolium chloride (CTC) (for O2-based respiration), the abundances of total, particle-associated (>3-μm), free-living, and <span class="hlt">actively</span> respiring bacteria were determined for <span class="hlt">ice</span>-core samples melted at their in situ temperatures (−2 to −20°C) and at the corresponding salinities of their brine inclusions (38 to 209 ppt). Fluorescence in situ hybridization was applied to determine the proportions of Bacteria, Cytophaga-Flavobacteria-Bacteroides (CFB), and Archaea. Microtome-prepared <span class="hlt">ice</span> sections also were examined microscopically under in situ conditions to evaluate bacterial abundance (by DAPI staining) and particle associations within the brine-inclusion network of the <span class="hlt">ice</span>. For both melted and intact <span class="hlt">ice</span> sections, more than 50% of cells were found to be associated with particles or surfaces (sediment grains, detritus, and <span class="hlt">ice</span>-crystal boundaries). CTC-<span class="hlt">active</span> bacteria (0.5 to 4% of the total) and cells detectable by rRNA probes (18 to 86% of the total) were found in all <span class="hlt">ice</span> samples, including the coldest (−20°C), where virtually all <span class="hlt">active</span> cells were particle associated. The percentage of <span class="hlt">active</span> bacteria associated with particles increased with decreasing temperature, as did the percentages of CFB (16 to 82% of Bacteria) and Archaea (0.0 to 3.4% of total cells). These results, combined with correlation analyses between bacterial variables and measures of particulate matter in the <span class="hlt">ice</span> as well as the increase in CFB at lower temperatures, confirm the importance of particle or surface association to bacterial <span class="hlt">activity</span> at subzero temperatures. Measuring <span class="hlt">activity</span> down to −20°C adds to the concept that liquid inclusions in frozen environments</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 Antarctic <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 Antarctic <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 Antarctic 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 <span class="hlt">active</span> dense water formation along the Antarctic coastal <span class="hlt">margins</span>. The signals at the seafloor extend along the topography, showing a horizontal distribution similar to the observed spreading of Antarctic 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('http://adsabs.harvard.edu/abs/2017AGUFM.C51A0947C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C51A0947C"><span><span class="hlt">Ice</span>-sheet thinning and acceleration at Camp Century, Greenlan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Colgan, W. T.</p> <p>2017-12-01</p> <p>Camp Century, Greenland (77.18 °N, 61.12 °W, 1900 m), is located approximately 150 km inland from the <span class="hlt">ice</span>-sheet <span class="hlt">margin</span> in Northwest Greenland. In-situ and remotely-sensed measurements of <span class="hlt">ice</span>-sheet elevation at Camp Century exhibit a thinning trend between 1964 and the present. A comparison of 1966 and 2017 firn density profiles indicates that a portion of this <span class="hlt">ice</span>-sheet thinning is attributable to increased firn compaction rate. In-situ measurements of increasing <span class="hlt">ice</span> surface velocity over the 1977-2017 period indicate that enhanced horizontal divergence of <span class="hlt">ice</span> flux is also contributing to <span class="hlt">ice</span> dynamic thinning at Camp Century. This apparent <span class="hlt">ice</span> dynamic thinning could potentially result from a migrating local flow divide or decreasing effective <span class="hlt">ice</span> viscosity. In a shorter-term context, observations of decadal-scale <span class="hlt">ice</span>-sheet thinning and acceleration at Camp Century highlights underappreciated transience in inland <span class="hlt">ice</span> form and flow during the satellite era. In a longer-term context, these multi-decadal observations contrast with inferences of millennial-scale <span class="hlt">ice</span>-sheet thickening and deceleration at Camp Century.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1986QuRes..26....3D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1986QuRes..26....3D"><span>Global <span class="hlt">ice</span>-sheet system interlocked by sea level</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Denton, George H.; Hughes, Terence J.; Karlén, Wibjörn</p> <p>1986-07-01</p> <p>Denton and Hughes (1983, Quaternary Research20, 125-144) postulated that sea level linked a global <span class="hlt">ice</span>-sheet system with both terrestrial and grounded marine components during late Quaternary <span class="hlt">ice</span> ages. Summer temperature changes near Northern Hemisphere melting <span class="hlt">margins</span> initiated sea-level fluctuations that controlled marine components in both polar hemispheres. It was further proposed that variations of this <span class="hlt">ice</span>-sheet system amplified and transmitted Milankovitch summer half-year insolation changes between 45 and 75°N into global climatic changes. New tests of this hypothesis implicate sea level as a major control of the areal extent of grounded portions of the Antarctic <span class="hlt">Ice</span> Sheet, thus fitting the concept of a globally interlocked <span class="hlt">ice</span>-sheet system. But recent atmospheric modeling results ( Manabe and Broccoli, 1985, Journal of Geophysical Research90, 2167-2190) suggest that factors other than areal changes of the grounded Antarctic <span class="hlt">Ice</span> Sheet strongly influenced Southern Hemisphere climate and terminated the last <span class="hlt">ice</span> age simultaneously in both polar hemispheres. Atmospheric carbon dioxide linked to high-latitude oceans is the most likely candidate ( Shackleton and Pisias, 1985, Atmospheric carbon dioxide, orbital forcing, and climate. In "The Carbon Cycle and Atmospheric CO 2: Natural Variations Archean to Present" (E. T. Sundquest and W. S. Broecker, Eds.), pp. 303-318. Geophysical Monograph 32, American Geophysical Union, Washington, D.C.), but another potential influence was high-frequency climatic oscillations (2500 yr). It is postulated that variations in atmospheric carbon dioxide acted through an Antarctic <span class="hlt">ice</span> shelf linked to the grounded <span class="hlt">ice</span> sheet to produce and terminate Southern Hemisphere <span class="hlt">ice</span>-age climate. It is further postulated that Milankovitch summer insolation combined with a warm high-frequency oscillation caused marked recession of Northern Hemisphere <span class="hlt">ice</span>-sheet melting <span class="hlt">margins</span> and the North Atlantic polar front about 14,000 14C yr B.P. This</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..1211532P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..1211532P"><span>10Be in <span class="hlt">ice</span> at high resolution: Solar <span class="hlt">activity</span> and climate signals observed and GCM-modeled in Law Dome <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>Pedro, Joel; Heikkilä, Ulla; van Ommen, T. D.; Smith, A. M.</p> <p>2010-05-01</p> <p>Changes in solar <span class="hlt">activity</span> modulate the galactic cosmic ray flux, and in turn, the production rate of 10Be in the earth's atmosphere. The best archives of past changes in 10Be production rate are the polar <span class="hlt">ice</span> cores. Key challenges in interpreting these archives as proxies for past solar <span class="hlt">activity</span> lie in separating the useful solar <span class="hlt">activity</span> (or production) signal from the interfering meteorological (or climate) signal, and furthermore, in determining the atmospheric source regions of 10Be deposited to the <span class="hlt">ice</span> core site. In this study we use a new monthly resolution composite 10Be record, which spans the past decade, and a general circulation model (ECHAM5-HAM), to constrain both the production and climate signals in 10Be concentrations at the Law Dome <span class="hlt">ice</span> core site, East Antarctica. This study differs from most previous work on 10Be in Antarctica due to the very high sample resolution achieved. This high resolution, through a time period where accurate instrumental measurements of solar <span class="hlt">activity</span> and climate are available, allows us to examine the response of 10Be concentrations in <span class="hlt">ice</span> to short-term (monthly to annual) variations in solar <span class="hlt">activity</span>, and to short-term variations in climate, including seasonality. We find a significant correlation (r2 = 0.56, P < 0.005, n = 92) between observed 10Be concentrations and solar <span class="hlt">activity</span> (represented by the neutron counting rate). The most pervasive climate influence is a seasonal cycle, which shows maximum concentrations in mid-to-late-summer and minimum concentrations in winter. Model results show reasonable agreement with observations; both a solar <span class="hlt">activity</span> signal and seasonal cycle in 10Be are captured. However, the modeled snow accumulation rate is too high by approximately 60%. According to the model, the main atmospheric source region of 10Be deposited to Law Dome is the 30-90°S stratosphere (~50%), followed by the 30-90°S troposphere (~30%). An enhancement in the fraction of 10Be arriving to Law Dome from the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1912473S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1912473S"><span>Adjustments of a global Finite-Element Sea <span class="hlt">Ice</span> Ocean Model configuration to improve the general ocean circulation in the North Pacific and its <span class="hlt">marginal</span> seas.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Scholz, Patrick; Lohmann, Gerrit</p> <p>2017-04-01</p> <p>The sub-Arctic oceans like the Sea of Okhotsk, the Bering Sea, the Labrador Sea or the Greenland- Irminger-Norwegian (GIN) Sea react particularly sensitive to global climate changes and have the potential to reversely regulate climate change by CO2 uptake in the other areas of the world. So far, the natural processes in the Arctic and Subarctic system, especially over the Pacific realm, remain poorly understood in terms of numerical modeling. As such, in this study we focus on the North Pacific and its adjacent <span class="hlt">marginal</span> seas (e.g. the Sea of Okhotsk, the Bering Sea and the Sea of Japan), which have nowadays a significant role in the climate system of the Northwest Pacific by influencing the atmospheric and oceanic circulation as well as the hydrology of the Pacific water masses. The Sea of Okhotsk, in particular, is characterized by a highly dynamical sea-<span class="hlt">ice</span> coverage, where, in autumn and winter, due to massive sea <span class="hlt">ice</span> formation and brine rejection, the Sea of Okhotsk Intermediate Water (SOIW) is formed which contributes to the mid-depth (500-1000m) water layer of the North Pacific known as newly formed North Pacific Intermediate Water (NPIW). By employing a Finite-Element Sea-<span class="hlt">Ice</span> Ocean Model (FESOM), in a global configuration, but with high resolution over the <span class="hlt">marginal</span> seas of the Northwest Pacific Ocean ( 7 km), we tested different meshes and forcing improvements to correct the general ocean circulation in the North Pacific realm towards a more realistic pattern. By using different forcing data (e.g. CORE2, ERA-40/interim, CCMP-correction), adapting the mesh resolutions in the tropical and subtropical North Pacific and changing the bathymetry over important inflow straits (e.g. Amukta Passage, Kruzenstern Strait), we show that the better results are obtained (when compared with observational data) via a combination of CCMP corrected COREv2 forcing with increased resolution in the pathway of the Kuroshio Extension Current and Northern Equatorial Current.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_16 --> <div id="page_17" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="321"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25193694','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25193694"><span>Perturbation of bacterial <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> by a grass antifreeze protein.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tomalty, Heather E; Walker, Virginia K</p> <p>2014-09-26</p> <p>Certain plant-associating bacteria produce <span class="hlt">ice</span> nucleation proteins (INPs) which allow the crystallization of water at high subzero temperatures. Many of these microbes are considered plant pathogens since the formed <span class="hlt">ice</span> can damage tissues, allowing access to nutrients. Intriguingly, certain plants that host these bacteria synthesize antifreeze proteins (AFPs). Once freezing has occurred, plant AFPs likely function to inhibit the growth of large damaging <span class="hlt">ice</span> crystals. However, we postulated that such AFPs might also serve as defensive mechanisms against bacterial-mediated <span class="hlt">ice</span> nucleation. Recombinant AFP derived from the perennial ryegrass Lolium perenne (LpAFP) was combined with INP preparations originating from the grass epiphyte, Pseudomonas syringae. The presence of INPs had no effect on AFP <span class="hlt">activity</span>, including thermal hysteresis and <span class="hlt">ice</span> recrystallization inhibition. Strikingly, the <span class="hlt">ice</span> nucleation point of the INP was depressed up to 1.9°C in the presence of LpAFP, but a recombinant fish AFP did not lower the INP-imposed freezing point. Assays with mutant LpAFPs and the visualization of bacterially-displayed fluorescent plant AFP suggest that INP and LpAFP can interact. Thus, we postulate that in addition to controlling <span class="hlt">ice</span> growth, plant AFPs may also function as a defensive strategy against the damaging effects of <span class="hlt">ice</span>-nucleating bacteria. Crown Copyright © 2014. Published by Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C21E1167C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C21E1167C"><span>Integrating terrestrial and marine records of the LGM in McMurdo Sound, Antarctica: implications for grounded <span class="hlt">ice</span> expansion, <span class="hlt">ice</span> flow, and deglaciation of the Ross Sea Embayment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Christ, A. J.; Marchant, D. R.</p> <p>2017-12-01</p> <p>During the LGM, grounded glacier <span class="hlt">ice</span> filled the Ross Embayment and deposited glacial drift on volcanic islands and peninsulas in McMurdo Sound, as well as along coastal regions of the Transantarctic Mountains (TAM), including the McMurdo Dry Valleys and Royal Society Range. The flow geometry and retreat history of this <span class="hlt">ice</span> remains debated, with contrasting views yielding divergent implications for both the fundamental cause of Antarctic <span class="hlt">ice</span> expansion as well as the interaction and behavior of <span class="hlt">ice</span> derived from East and West Antarctica during late Quaternary time. We present terrestrial geomorphologic evidence that enables the reconstruction of former <span class="hlt">ice</span> elevations, <span class="hlt">ice</span>-flow paths, and <span class="hlt">ice-marginal</span> environments in McMurdo Sound. Radiocarbon dates of fossil algae interbedded with <span class="hlt">ice-marginal</span> sediments provide a coherent timeline for local <span class="hlt">ice</span> retreat. These data are integrated with marine-sediment records and multi-beam data to reconstruct late glacial dynamics of grounded <span class="hlt">ice</span> in McMurdo Sound and the western Ross Sea. The combined dataset suggest a dominance of <span class="hlt">ice</span> flow toward the TAM in McMurdo Sound during all phases of glaciation, with thick, grounded <span class="hlt">ice</span> at or near its maximum extent between 19.6 and 12.3 calibrated thousands of years before present (cal. ka). Our data show no significant advance of locally derived <span class="hlt">ice</span> from the TAM into McMurdo Sound, consistent with the assertion that Late Pleistocene expansion of grounded <span class="hlt">ice</span> in McMurdo Sound, and throughout the wider Ross Embayment, occurs in response to lower eustatic sea level and the resulting advance of marine-based outlet glaciers and <span class="hlt">ice</span> streams (and perhaps also reduced oceanic heat flux), rather than local increases in precipitation and <span class="hlt">ice</span> accumulation. Finally, when combined with allied data across the wider Ross Embayment, which show that widespread deglaciation outside McMurdo Sound did not commence until 13.1 ka, the implication is that retreat of grounded glacier <span class="hlt">ice</span> in the Ross Embayment did</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.8068J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.8068J"><span>Sea-<span class="hlt">ice</span> cover in the Nordic Seas and the sensitivity to Atlantic water temperatures</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jensen, Mari F.; Nisancioglu, Kerim H.; Spall, Michael A.</p> <p>2017-04-01</p> <p>Changes in the sea-<span class="hlt">ice</span> cover of the Nordic Seas have been proposed to play a key role for the dramatic temperature excursions associated with the Dansgaard-Oeschger events during the last glacial. However, with its proximity to the warm Atlantic water, how a sea-<span class="hlt">ice</span> cover can persist in the Nordic Seas is not well understood. In this study, we apply an eddy-resolving configuration of the Massachusetts Institute of Technology general circulation model with an idealized topography to study the presence of sea <span class="hlt">ice</span> in a Nordic Seas-like domain. We assume an infinite amount of warm Atlantic water present in the south by restoring the southern area to constant temperatures. The sea-surface temperatures are restored toward cold, atmospheric temperatures, and as a result, sea <span class="hlt">ice</span> is present in the interior of the domain. However, the sea-<span class="hlt">ice</span> cover in the <span class="hlt">margins</span> of the Nordic Seas, an area with a warm, cyclonic boundary current, is sensitive to the amount of heat entering the domain, i.e., the restoring temperature in the south. When the temperature of the warm, cyclonic boundary current is high, the <span class="hlt">margins</span> are free of sea <span class="hlt">ice</span> and heat is released to the atmosphere. We show that with a small reduction in the temperature of the incoming Atlantic water, the Nordic Seas-like domain is fully covered in sea <span class="hlt">ice</span>. Warm water is still entering the Nordic Seas, however, this happens at depths below a cold, fresh surface layer produced by melted sea <span class="hlt">ice</span>. Consequently, the heat release to the atmosphere is reduced along with the eddy heat fluxes. Results suggest a threshold value in the amount of heat entering the Nordic Seas before the sea-<span class="hlt">ice</span> cover disappears in the <span class="hlt">margins</span>. We study the sensitivity of this threshold to changes in atmospheric temperatures and vertical diffusivity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70012219','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70012219"><span><span class="hlt">Ice</span>-Sheet Glaciation of the Puget lowland, Washington, during the Vashon Stade (late pleistocene)</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Thorson, R.M.</p> <p>1980-01-01</p> <p>During the Vashon Stade of the Fraser Glaciation, about 15,000-13,000 yr B.P., a lobe of the Cordilleran <span class="hlt">Ice</span> Sheet occupied the Puget lowland of western Washington. At its maximum extent about 14,000 yr ago, the <span class="hlt">ice</span> sheet extended across the Puget lowland between the Cascade Range and Olympic Mountains and terminated about 80 km south of Seattle. Meltwater streams drained southwest to the Pacific Ocean and built broad outwash trains south of the <span class="hlt">ice</span> <span class="hlt">margin</span>. Reconstructed longitudinal profiles for the Puget lobe at its maximum extent are similar to the modern profile of Malaspina Glacier, Alaska, suggesting that the <span class="hlt">ice</span> sheet may have been in a near-equilibrium state at the glacial maximum. Progressive northward retreat from the terminal zone was accompanied by the development of <span class="hlt">ice-marginal</span> streams and proglacial lakes that drained southward during initial retreat, but northward during late Vashon time. Relatively rapid retreat of the Juan de Fuca lobe may have contributed to partial stagnation of the northwestern part of the Puget lobe. Final destruction of the Puget lobe occurred when the <span class="hlt">ice</span> retreated north of Admiralty Inlet. The sea entered the Puget lowland at this time, allowing the deposition of glacial-marine sediments which now occur as high as 50 m altitude. These deposits, together with <span class="hlt">ice-marginal</span> meltwater channels presumed to have formed above sea level during deglaciation, suggest that a significant amount of postglacial isostatic and(or) tectonic deformation has occurred in the Puget lowland since deglaciation. ?? 1980.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030020763','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030020763"><span>Understanding Recent Mass Balance Changes of the Greenland <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>vanderVeen, Cornelius</p> <p>2003-01-01</p> <p>The ultimate goal of this project is to better understand the current transfer of mass between the Greenland <span class="hlt">Ice</span> Sheet, the world's oceans and the atmosphere, and to identify processes controlling the rate of this transfer, to be able to predict with greater confidence future contributions to global sea level rise. During the first year of this project, we focused on establishing longer-term records of change of selected outlet glaciers, reevaluation of mass input to the <span class="hlt">ice</span> sheet and analysis of climate records derived from <span class="hlt">ice</span> cores, and modeling meltwater production and runoff from the <span class="hlt">margins</span> of the <span class="hlt">ice</span> sheet.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910030932&hterms=sutherland&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dsutherland','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910030932&hterms=sutherland&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dsutherland"><span>The discrimination of sea <span class="hlt">ice</span> types using SAR backscatter statistics</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Shuchman, Robert A.; Wackerman, Christopher C.; Maffett, Andrew L.; Onstott, Robert G.; Sutherland, Laura L.</p> <p>1989-01-01</p> <p>X-band (HH) synthetic aperture radar (SAR) data of sea <span class="hlt">ice</span> collected during the <span class="hlt">Marginal</span> <span class="hlt">Ice</span> Zone Experiment in March and April of 1987 was statistically analyzed with respect to discriminating open water, first-year <span class="hlt">ice</span>, multiyear <span class="hlt">ice</span>, and Odden. Odden are large expanses of nilas <span class="hlt">ice</span> that rapidly form in the Greenland Sea and transform into pancake <span class="hlt">ice</span>. A first-order statistical analysis indicated that mean versus variance can segment out open water and first-year <span class="hlt">ice</span>, and skewness versus modified skewness can segment the Odden and multilayer categories. In additions to first-order statistics, a model has been generated for the distribution function of the SAR <span class="hlt">ice</span> data. Segmentation of <span class="hlt">ice</span> types was also attempted using textural measurements. In this case, the general co-occurency matrix was evaluated. The textural method did not generate better results than the first-order statistical approach.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.A11B0031H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.A11B0031H"><span>Direct Quantification of <span class="hlt">Ice</span> Nucleation <span class="hlt">Active</span> Bacteria in Aerosols and Precipitation: Their Potential Contribution as <span class="hlt">Ice</span> Nuclei</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hill, T. C.; DeMott, P. J.; Garcia, E.; Moffett, B. F.; Prenni, A. J.; Kreidenweis, S. M.; Franc, G. D.</p> <p>2013-12-01</p> <p><span class="hlt">Ice</span> nucleation <span class="hlt">active</span> (INA) bacteria are a potentially prodigious source of highly <span class="hlt">active</span> (≥-12°C) atmospheric <span class="hlt">ice</span> nuclei, especially from agricultural land. However, we know little about the conditions that promote their release (eg, daily or seasonal cycles, precipitation, harvesting or post-harvest decay of litter) or their typical contribution to the pool of boundary layer <span class="hlt">ice</span> nucleating particles (INP). To initiate these investigations we developed a quantitative Polymerase Chain Reaction (qPCR) test of the ina gene, the gene that codes for the <span class="hlt">ice</span> nucleating protein, to directly count INA bacteria in environmental samples. The qPCR test amplifies most forms of the gene and is highly sensitive, able to detect perhaps a single gene copy (ie, a single bacterium) in DNA extracted from precipitation. Direct measurement of the INA bacteria is essential because environmental populations will be a mixture of living, viable-but-not culturable, moribund and dead cells, all of which may retain <span class="hlt">ice</span> nucleating proteins. Using the qPCR test on leaf washings of plants from three farms in Wyoming, Colorado and Nebraska we found INA bacteria to be abundant on crops, especially on cereals. Mid-summer populations on wheat and barley were ~108/g fresh weigh of foliage. Broadleaf crops, such as corn, alfalfa, sugar beet and potato supported 105-107/g. Unexpectedly, however, in the absence of a significant physical disturbance, such as harvesting, we were unable to detect the ina gene in aerosols sampled above the crops. Likewise, in fresh snow samples taken over two winters, ina genes from a range of INA bacteria were detected in about half the samples but at abundances that equated to INA bacterial numbers that accounted for only a minor proportion of INP <span class="hlt">active</span> at -10°C. By contrast, in a hail sample from a summer thunderstorm we found 0.3 INA bacteria per INP at -10°C and ~0.5 per hail stone. Although the role of the INA bacteria as warm-temperature INP in these samples</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28518108','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28518108"><span>Identification of Plant <span class="hlt">Ice</span>-binding Proteins Through Assessment of <span class="hlt">Ice</span>-recrystallization Inhibition and Isolation Using <span class="hlt">Ice</span>-affinity Purification.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bredow, Melissa; Tomalty, Heather E; Walker, Virginia K</p> <p>2017-05-05</p> <p><span class="hlt">Ice</span>-binding proteins (IBPs) belong to a family of stress-induced proteins that are synthesized by certain organisms exposed to subzero temperatures. In plants, freeze damage occurs when extracellular <span class="hlt">ice</span> crystals grow, resulting in the rupture of plasma membranes and possible cell death. Adsorption of IBPs to <span class="hlt">ice</span> crystals restricts further growth by a process known as <span class="hlt">ice</span>-recrystallization inhibition (IRI), thereby reducing cellular damage. IBPs also demonstrate the ability to depress the freezing point of a solution below the equilibrium melting point, a property known as thermal hysteresis (TH) <span class="hlt">activity</span>. These protective properties have raised interest in the identification of novel IBPs due to their potential use in industrial, medical and agricultural applications. This paper describes the identification of plant IBPs through 1) the induction and extraction of IBPs in plant tissue, 2) the screening of extracts for IRI <span class="hlt">activity</span>, and 3) the isolation and purification of IBPs. Following the induction of IBPs by low temperature exposure, extracts are tested for IRI <span class="hlt">activity</span> using a 'splat assay', which allows the observation of <span class="hlt">ice</span> crystal growth using a standard light microscope. This assay requires a low protein concentration and generates results that are quickly obtained and easily interpreted, providing an initial screen for <span class="hlt">ice</span> binding <span class="hlt">activity</span>. IBPs can then be isolated from contaminating proteins by utilizing the property of IBPs to adsorb to <span class="hlt">ice</span>, through a technique called '<span class="hlt">ice</span>-affinity purification'. Using cell lysates collected from plant extracts, an <span class="hlt">ice</span> hemisphere can be slowly grown on a brass probe. This incorporates IBPs into the crystalline structure of the polycrystalline <span class="hlt">ice</span>. Requiring no a priori biochemical or structural knowledge of the IBP, this method allows for recovery of <span class="hlt">active</span> protein. <span class="hlt">Ice</span>-purified protein fractions can be used for downstream applications including the identification of peptide sequences by mass spectrometry and the</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 Antarctic <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 <span class="hlt">active</span> microbial ecosystems capable of cycling important greenhouse gases, such as methane (CH4). A large methane reservoir is thought to exist beneath the West Antarctic <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 Lake 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 <span class="hlt">margins</span> and during periods of deglaciation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFMGC43E1005H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFMGC43E1005H"><span>Glacial-marine sediments record <span class="hlt">ice</span>-shelf retreat during the late Holocene in Beascochea Bay on the western <span class="hlt">margin</span> of the Antarctic Peninsula</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hardin, L. A.; Wellner, J. S.</p> <p>2010-12-01</p> <p>Beascochea Bay has an overall rapid rate of sedimentation due to retreating fast-flowing <span class="hlt">ice</span>, and thus contains high-resolution records of Antarctica’s glacial and climate history. Beascochea Bay is a 16 km long by 8 km wide bay located on the western <span class="hlt">margin</span> of the Antarctica Peninsula, centered between Anvers Island and Renaud Island, but open to the Bellingshausen Sea. Currently, three tidewater glaciers draining the Bruce Plateau of Graham Land enter into the fjords of Beascochea Bay, releasing terrigenous sediments which have left a record of the fluctuations of the Antarctic Peninsula <span class="hlt">Ice</span> Cap since the grounded <span class="hlt">ice</span> decoupled from the seafloor after the last glacial maximum. These three glaciers have played a significant role in providing sediment to the main basin, allowing a detailed sediment facies analysis to be conducted from eight sediment cores which were collected during the austral summer of 2007. Pebbly silty clay sediment cores, along with 3.5 kHz seismic data and multibeam swath bathymetry data, are integrated to reconstruct a glacial retreat timeline for the middle to late Holocene, which can be compared to the recent retreat rates over the last century. Paleoenvironment of deposition is determined by mapping lateral facies changes from the side fjords (proximal) to the outer basin (distal), as each region records the transition from glacial-marine sediments to open-marine sediments. As the <span class="hlt">ice</span> retreated from the outer basin to the inner basin, and most recently leaving the side fjords, each facies deposited can be age-constrained by radiocarbon, 210Pb, and 137Cs dating methods. A distinct 137Cs signal is readily seen in two kasten cores from a side fjord and the inner basin of Beascochea Bay. This dating method revealed an average sedimentation rate of 2.7 mm per year for approximately the last century, which is comparable to 210Pb rates obtained in other studies. Lithology variations in each sediment core record indications of <span class="hlt">ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017BVol...79...89M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017BVol...79...89M"><span>Remote sensing evidence of lava-ground <span class="hlt">ice</span> interactions associated with the Lost Jim Lava Flow, Seward Peninsula, Alaska</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marcucci, Emma C.; Hamilton, Christopher W.; Herrick, Robert R.</p> <p>2017-12-01</p> <p>Thermokarst terrains develop when <span class="hlt">ice</span>-bearing permafrost melts and causes the overlying surface to subside or collapse. This process occurs widely throughout Arctic regions due to environmental and climatological factors, but can also be induced by localized melting of ground <span class="hlt">ice</span> by <span class="hlt">active</span> lava flows. The Lost Jim Lava Flow (LJLF) on the Seward Peninsula of Alaska provides evidence of former lava-ground <span class="hlt">ice</span> interactions. Associated geomorphic features, on the scale of meters to tens of meters, were identified using satellite orthoimages and stereo-derived digital terrain models. The flow exhibits positive- and mixed-relief features, including tumuli ( N = 26) and shatter rings ( N = 4), as well as negative-relief features, such as lava tube skylights ( N = 100) and irregularly shaped topographic depressions ( N = 1188) that are interpreted to include lava-rise pits and lava-induced thermokarst terrain. Along the <span class="hlt">margins</span> of the flow, there are also clusters of small peripheral pits that may be the products of meltwater or steam escape. On Mars, we observed morphologically similar pits near lava flow <span class="hlt">margins</span> in northeastern Elysium Planitia, which suggests a common formation mechanism. Investigating the LJLF may therefore help to elucidate processes of lava-ground <span class="hlt">ice</span> interaction on both Earth and Mars.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFMGC23H..08S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFMGC23H..08S"><span>Correlating <span class="hlt">Ice</span> Cores from Quelccaya <span class="hlt">Ice</span> Cap with Chronology from Little <span class="hlt">Ice</span> Age Glacial Extents</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stroup, J. S.; Kelly, M. A.; Lowell, T. V.</p> <p>2010-12-01</p> <p>Proxy records indicate Southern Hemisphere climatic changes during the Little <span class="hlt">Ice</span> Age (LIA; ~1300-1850 AD). In particular, records of change in and around the tropical latitudes require attention because these areas are sensitive to climatic change and record the dynamic interplay between hemispheres (Oerlemans, 2005). Despite this significance, relatively few records exist for the southern tropics. Here we present a reconstruction of glacial fluctuations of Quelccaya <span class="hlt">Ice</span> Cap (QIC), Peruvian Andes, from pre-LIA up to the present day. In the Qori Kalis valley, extensive sets of moraines exist beginning with the 1963 AD <span class="hlt">ice</span> <span class="hlt">margin</span> (Thompson et al., 2006) and getting progressively older down valley. Several of these older moraines can be traced and are continuous with moraines in the Challpa Cocha valley. These moraines have been dated at <1050-1350-AD (Mercer and Palacios, 1977) and interpreted to have been deposited during the Little <span class="hlt">Ice</span> Age. We present a new suite of surface exposure and radiocarbon dates collected in 2008 and 2009 that constrain the ages of these moraines. Preliminary 10Be ages of boulder surfaces atop the moraines range from ~350-1370 AD. Maximum and minimum-limiting radiocarbon ages bracketing the moraines are ~0-1800 AD. The chronology of past <span class="hlt">ice</span> cap extents are correlated with <span class="hlt">ice</span> core records from QIC which show an accumulation increase during ~1500-1700 AD and an accumulation decrease during ~1720-1860 AD (Thompson et al., 1985; 1986; 2006). In addition, other proxy records from Peru and the tropics are correlated with the records at QIC as a means to understand climate conditions during the LIA. This work forms the basis for future modeling of the glacial system during the LIA at QIC and for modeling of past temperature and precipitation regimes at high altitude in the tropics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12154613','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12154613"><span>Ecology of southern ocean pack <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>Brierley, Andrew S; Thomas, David N</p> <p>2002-01-01</p> <p>Around Antarctica the annual five-fold growth and decay of sea <span class="hlt">ice</span> is the most prominent physical process and has a profound impact on marine life there. In winter the pack <span class="hlt">ice</span> canopy extends to cover almost 20 million square kilometres--some 8% of the southern hemisphere and an area larger than the Antarctic continent itself (13.2 million square kilometres)--and is one of the largest, most dynamic ecosystems on earth. Biological <span class="hlt">activity</span> is associated with all physical components of the sea-<span class="hlt">ice</span> system: the sea-<span class="hlt">ice</span> surface; the internal sea-<span class="hlt">ice</span> matrix and brine channel system; the underside of sea <span class="hlt">ice</span> and the waters in the vicinity of sea <span class="hlt">ice</span> that are modified by the presence of sea <span class="hlt">ice</span>. Microbial and microalgal communities proliferate on and within sea <span class="hlt">ice</span> and are grazed by a wide range of proto- and macrozooplankton that inhabit the sea <span class="hlt">ice</span> in large concentrations. Grazing organisms also exploit biogenic material released from the sea <span class="hlt">ice</span> at <span class="hlt">ice</span> break-up or melt. Although rates of primary production in the underlying water column are often low because of shading by sea-<span class="hlt">ice</span> cover, sea <span class="hlt">ice</span> itself forms a substratum that provides standing stocks of bacteria, algae and grazers significantly higher than those in <span class="hlt">ice</span>-free areas. Decay of sea <span class="hlt">ice</span> in summer releases particulate and dissolved organic matter to the water column, playing a major role in biogeochemical cycling as well as seeding water column phytoplankton blooms. Numerous zooplankton species graze sea-<span class="hlt">ice</span> algae, benefiting additionally because the overlying sea-<span class="hlt">ice</span> ceiling provides a refuge from surface predators. Sea <span class="hlt">ice</span> is an important nursery habitat for Antarctic krill, the pivotal species in the Southern Ocean marine ecosystem. Some deep-water fish migrate to shallow depths beneath sea <span class="hlt">ice</span> to exploit the elevated concentrations of some zooplankton there. The increased secondary production associated with pack <span class="hlt">ice</span> and the sea-<span class="hlt">ice</span> edge is exploited by many higher predators, with seals, seabirds and whales</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4646349','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4646349"><span>Latent <span class="hlt">Ice</span> Recrystallization Inhibition <span class="hlt">Activity</span> in Nonantifreeze Proteins: Ca2+-<span class="hlt">Activated</span> Plant Lectins and Cation-<span class="hlt">Activated</span> Antimicrobial Peptides</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p></p> <p>2015-01-01</p> <p>Organisms living in polar regions have evolved a series of antifreeze (glyco) proteins (AFGPs) to enable them to survive by modulating the structure of <span class="hlt">ice</span>. These proteins have huge potential for use in cellular cryopreservation, <span class="hlt">ice</span>-resistant surfaces, frozen food, and cryosurgery, but they are limited by their relatively low availability and questions regarding their mode of action. This has triggered the search for biomimetic materials capable of reproducing this function. The identification of new structures and sequences capable of inhibiting <span class="hlt">ice</span> growth is crucial to aid our understanding of these proteins. Here, we show that plant c-type lectins, which have similar biological function to human c-type lectins (glycan recognition) but no sequence homology to AFPs, display calcium-dependent <span class="hlt">ice</span> recrystallization inhibition (IRI) <span class="hlt">activity</span>. This IRI <span class="hlt">activity</span> can be switched on/off by changing the Ca2+ concentration. To show that more (nonantifreeze) proteins may exist with the potential to display IRI, a second motif was considered, amphipathicity. All known AFPs have defined hydrophobic/hydrophilic domains, rationalizing this choice. The cheap, and widely used, antimicrobial Nisin was found to have cation-dependent IRI <span class="hlt">activity</span>, controlled by either acid or addition of histidine-binding ions such as zinc or nickel, which promote its amphipathic structure. These results demonstrate a new approach in the identification of antifreeze protein mimetic macromolecules and may help in the development of synthetic mimics of AFPs. PMID:26407233</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015ACPD...1531665L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015ACPD...1531665L"><span>Investigation of <span class="hlt">ice</span> particle habits to be used for <span class="hlt">ice</span> cloud remote sensing for the GCOM-C satellite mission</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Letu, H.; Ishimoto, H.; Riedi, J.; Nakajima, T. Y.; -Labonnote, L. C.; Baran, A. J.; Nagao, T. M.; Skiguchi, M.</p> <p>2015-11-01</p> <p> found that the SAD, for bullet-rosette particle, with radii of equivalent volume spheres (r<span style="position: relative; top: -.5em; left: -.65em;">~<i style=" <span class="hlt">margin</span>-left:-.7em">) ranging between 6 to 10 μm, and the Voronoi particle, with r<span style="position: relative; top: -.5em; left: -.65em;">~<i style=" <span class="hlt">margin</span>-left:-.7em"> ranging between 28 to 38 μm, and 70 to 100 μm, is distributed stably as the scattering angle increases. It is confirmed that the SAD of small bullet rosette and all sizes of voronoi particles has a low angular dependence, indicating that the combination of the bullet-rosette and Voronoi models are sufficient for retrieval of the <span class="hlt">ice</span> cloud spherical albedo and optical thickness as an effective habit models of the SGLI sensor. Finally, SAD analysis based on the Voronoi habit model with moderate particles (r<span style="position: relative; top: -.5em; left: -.65em;">~<i style=" <span class="hlt">margin</span>-left:-.7em"> = 30 μm) is compared to the conventional General Habit Mixture (GHM), Inhomogeneous Hexagonal Monocrystal (IHM), 5-plate aggregate and ensemble <span class="hlt">ice</span> particle model. It is confirmed that the Voronoi habit model has an effect similar to the counterparts of some conventional models on the retrieval of <span class="hlt">ice</span> cloud properties from space-borne radiometric observations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C31A..01G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C31A..01G"><span>Seasonal Changes of Arctic Sea <span class="hlt">Ice</span> Physical Properties Observed During N-<span class="hlt">ICE</span>2015: An Overview</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gerland, S.; Spreen, G.; Granskog, M. A.; Divine, D.; Ehn, J. K.; Eltoft, T.; Gallet, J. C.; Haapala, J. J.; Hudson, S. R.; Hughes, N. E.; Itkin, P.; King, J.; Krumpen, T.; Kustov, V. Y.; Liston, G. E.; Mundy, C. J.; Nicolaus, M.; Pavlov, A.; Polashenski, C.; Provost, C.; Richter-Menge, J.; Rösel, A.; Sennechael, N.; Shestov, A.; Taskjelle, T.; Wilkinson, J.; Steen, H.</p> <p>2015-12-01</p> <p>Arctic sea <span class="hlt">ice</span> is changing, and for improving the understanding of the cryosphere, data is needed to describe the status and processes controlling current seasonal sea <span class="hlt">ice</span> growth, change and decay. We present preliminary results from in-situ observations on sea <span class="hlt">ice</span> in the Arctic Basin north of Svalbard from January to June 2015. Over that time, the Norwegian research vessel «Lance» was moored to in total four <span class="hlt">ice</span> floes, drifting with the sea <span class="hlt">ice</span> and allowing an international group of scientists to conduct detailed research. Each drift lasted until the ship reached the <span class="hlt">marginal</span> <span class="hlt">ice</span> zone and <span class="hlt">ice</span> started to break up, before moving further north and starting the next drift. The ship stayed within the area approximately 80°-83° N and 5°-25° E. While the expedition covered measurements in the atmosphere, the snow and sea <span class="hlt">ice</span> system, and in the ocean, as well as biological studies, in this presentation we focus on physics of snow and sea <span class="hlt">ice</span>. Different <span class="hlt">ice</span> types could be investigated: young <span class="hlt">ice</span> in refrozen leads, first year <span class="hlt">ice</span>, and old <span class="hlt">ice</span>. Snow surveys included regular snow pits with standardized measurements of physical properties and sampling. Snow and <span class="hlt">ice</span> thickness were measured at stake fields, along transects with electromagnetics, and in drillholes. For quantifying <span class="hlt">ice</span> physical properties and texture, <span class="hlt">ice</span> cores were obtained regularly and analyzed. Optical properties of snow and <span class="hlt">ice</span> were measured both with fixed installed radiometers, and from mobile systems, a sledge and an ROV. For six weeks, the surface topography was scanned with a ground LIDAR system. Spatial scales of surveys ranged from spot measurements to regional surveys from helicopter (<span class="hlt">ice</span> thickness, photography) during two months of the expedition, and by means of an array of autonomous buoys in the region. Other regional information was obtained from SAR satellite imagery and from satellite based radar altimetry. The analysis of the data collected has started, and first results will be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1616930P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1616930P"><span>The extent and timing of the last British-Irish <span class="hlt">Ice</span> Sheet offshore of west Ireland-preliminary findings</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Peters, Jared; Benetti, Sara; Dunlop, Paul; Cofaigh, Colm Ó.</p> <p>2014-05-01</p> <p>Recently interpreted marine geophysical data from the western Irish shelf has provided the first direct evidence that the last British-Irish <span class="hlt">Ice</span> Sheet (BIIS) extended westwards onto the Irish continental shelf as a grounded <span class="hlt">ice</span> mass composed of several lobes with marine-terminating <span class="hlt">margins</span>. Marine terminating <span class="hlt">ice</span> <span class="hlt">margins</span> are known to be sensitive to external forcing mechanisms and currently there is concern regarding the future stability of marine based <span class="hlt">ice</span> sheets, such as the West Antarctic <span class="hlt">Ice</span> Sheet, in a warming world. Given its position, the glaciated western Irish continental shelf is a prime location to investigate the processes of how marine-based <span class="hlt">ice</span> sheets responded to past climatic and oceanic events, which may in turn help us better predict the future trajectory of the marine sectors of modern <span class="hlt">Ice</span> Sheets. However, despite the potential importance of the former Irish <span class="hlt">ice</span> <span class="hlt">margin</span> to our understanding of <span class="hlt">ice</span> sheet behaviour, the timing and nature of its advance and retreat is currently poorly understood. This study aims to describe the depositional history of the last BIIS on the continental shelf west of Ireland and age-constrain the rate of retreat of two <span class="hlt">ice</span> lobes that extended from Galway Bay and Clew Bay. This is being accomplished through a multifaceted analysis of at least 29 sediment cores gathered across the continental shelf offshore of counties Galway and Mayo, Ireland. This poster shows results from initial sedimentological descriptions of cores from the mid to outer shelf, which support previous geomorphic interpretations of BIIS history. Preliminary palaeoenvironmental results from ongoing micropaleontological analyses are also discussed and provide new data that verifies sedimentary interpretations on <span class="hlt">ice</span> proximity. Finally, results from several radiocarbon dates are discussed, which limit these deposits to the last glacial maximum and constrain the timings of <span class="hlt">ice</span> advance and retreat on the continental shelf west of Ireland.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25345526','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25345526"><span>Immersion freezing of supermicron mineral dust particles: freezing results, testing different schemes for describing <span class="hlt">ice</span> nucleation, and <span class="hlt">ice</span> nucleation <span class="hlt">active</span> site densities.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wheeler, M J; Mason, R H; Steunenberg, K; Wagstaff, M; Chou, C; Bertram, A K</p> <p>2015-05-14</p> <p><span class="hlt">Ice</span> nucleation on mineral dust particles is known to be an important process in the atmosphere. To accurately implement <span class="hlt">ice</span> nucleation on mineral dust particles in atmospheric simulations, a suitable theory or scheme is desirable to describe laboratory freezing data in atmospheric models. In the following, we investigated <span class="hlt">ice</span> nucleation by supermicron mineral dust particles [kaolinite and Arizona Test Dust (ATD)] in the immersion mode. The median freezing temperature for ATD was measured to be approximately -30 °C compared with approximately -36 °C for kaolinite. The freezing results were then used to test four different schemes previously used to describe <span class="hlt">ice</span> nucleation in atmospheric models. In terms of ability to fit the data (quantified by calculating the reduced chi-squared values), the following order was found for ATD (from best to worst): <span class="hlt">active</span> site, pdf-α, deterministic, single-α. For kaolinite, the following order was found (from best to worst): <span class="hlt">active</span> site, deterministic, pdf-α, single-α. The variation in the predicted median freezing temperature per decade change in the cooling rate for each of the schemes was also compared with experimental results from other studies. The deterministic model predicts the median freezing temperature to be independent of cooling rate, while experimental results show a weak dependence on cooling rate. The single-α, pdf-α, and <span class="hlt">active</span> site schemes all agree with the experimental results within roughly a factor of 2. On the basis of our results and previous results where different schemes were tested, the <span class="hlt">active</span> site scheme is recommended for describing the freezing of ATD and kaolinite particles. We also used our <span class="hlt">ice</span> nucleation results to determine the <span class="hlt">ice</span> nucleation <span class="hlt">active</span> site (INAS) density for the supermicron dust particles tested. Using the data, we show that the INAS densities of supermicron kaolinite and ATD particles studied here are smaller than the INAS densities of submicron kaolinite and ATD particles</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17..992F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17..992F"><span><span class="hlt">Ice</span> elevation change from Swath Processing of CryoSat SARIn Mode Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Foresta, Luca; Gourmelen, Noel; Shepherd, Andrew; Muir, Alan; Nienow, Pete</p> <p>2015-04-01</p> <p>Reference and repeat-observations of Glacier and <span class="hlt">Ice</span> Sheet <span class="hlt">Margin</span> (GISM) topography are critical to identify changes in <span class="hlt">ice</span> elevation, provide estimates of mass gain or loss and thus quantify the contribution of the cryosphere to sea level rise (e.g. McMillan et al., 2014). The Synthetic Interferometric Radar Altimeter (SIRAL) onboard the ESA radar altimetry CryoSat (CS) mission has collected <span class="hlt">ice</span> elevation measurements since 2010. The corresponding SARIn mode of operation, <span class="hlt">activated</span> over GISM areas, provides high spatial resolution in the along-track direction while resolving the angular origin of echoes (i.e. across-track). The current ESA SARIn processor calculates the elevation of the Point Of Closest Approach (POCA) within each waveform and maps of elevation change in Antarctica and Greenland have been produced using the regular CS height product (McMillan et al., 2014; Helm et al., 2014). Data from the CS-SARIn mode has also been used to produce measurements of <span class="hlt">ice</span> elevation beyond the POCA, also known as swath elevation (Hawley et al. 2009; Gray et al., 2013; ESA-STSE CryoTop project). Here we use the swath processing approach to generate maps of <span class="hlt">ice</span> elevation change from selected regions around the <span class="hlt">margins</span> of the Greenland and Antarctic <span class="hlt">Ice</span> Sheets. We discuss the impact of the swath processing on the spatial resolution and precision of the resulting <span class="hlt">ice</span> elevation field and compare our results to current dh/dt estimates. References: ESA STSE CryoTop project - http://www.stse-cryotop.org/ Gray L., Burgess D., Copland L., Cullen R., Galin N., Hawley R. and Helm V. Interferometric swath processing of Cryosat data for glacial <span class="hlt">ice</span> topography. The Cryosphere, 7(6):1857-1867, December 2013. Hawley R.L., Shepherd A., Cullen R., Helm V. and WIngham D.J. <span class="hlt">Ice</span>-sheet elevations from across-track processing of airborne interferometric radar altimetry. Geophysical Research Letters, 36(22):L22501, November 2009. Helm V., Humbert A. and Miller H. Elevation and elevation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C23D..04M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C23D..04M"><span>Role of <span class="hlt">ice</span> sheet dynamics in the collapse of the early-Holocene Laurentide <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>Matero, I. S. O.; Gregoire, L. J.; Cornford, S. L.; Ivanovic, R. F.</p> <p>2017-12-01</p> <p>The last stage of the deglaciation of the Laurentide <span class="hlt">Ice</span> Sheet (LIS) during the early Holocene Thermal Maximum ( 9000 to 7000 years ago) provides an analogy and insight to the possible responses of contemporary <span class="hlt">ice</span> sheets in a warming climate. What makes LIS particularly interesting is that meltwater from the collapse of an <span class="hlt">ice</span> saddle over Hudson Bay was recently shown to be the primary forcing for the period of abrupt northern hemisphere cooling known as the 8.2 ka event. The evolution of the LIS during this period was likely influenced by its interaction with <span class="hlt">marginal</span> lakes and the ocean, and its major <span class="hlt">ice</span> stream, which exported <span class="hlt">ice</span> towards Hudson Strait. Accurately simulating the early Holocene LIS evolution thus requires a model such as BISICLES, capable of accurately and efficiently resolving <span class="hlt">ice</span> stream dynamics and grounding line migration thanks to the combined use of higher order physics and adaptive mesh refinement. We drive the BISICLES model using a positive degree day mass balance scheme with monthly precipitation and temperature from the HadCM3 climate model under climatic conditions from 10,000 to 8,000 years ago. We test the effect of varying the initial topographies and <span class="hlt">ice</span> thicknesses from different timeslices in the <span class="hlt">ICE</span>-6Gc reconstruction. We also test different parameterisations for the basal friction based on the thicknesses of the underlying sediments. These simulations evaluate the role of the Hudson Strait <span class="hlt">ice</span> stream, <span class="hlt">ice</span> sheet dynamics and interactions with the adjacent proglacial Lake Agassiz and North Atlantic Ocean in the collapse of the LIS. Our results highlight that the choice of parameterisation for basal friction has major effects on <span class="hlt">ice</span> sheet dynamics and evolution.</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://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 Lake Michigan lobe of the Laurentide <span class="hlt">ice</span> sheet from <span class="hlt">ice</span>-walled lake 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 Lake 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 lakes. We analyze the precision and accuracy of 15 AMS 14C ages of plant macrofossils obtained from a single <span class="hlt">ice</span>-walled lake 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 <span class="hlt">active</span> <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 lake 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 <span class="hlt">margin</span> of the Lake Michigan lobe have been assessed using this method. There is no overlap of time intervals documenting when <span class="hlt">ice</span>-walled lakes 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 lake 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=5468641','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5468641"><span>High Arctic Holocene temperature record from the Agassiz <span class="hlt">ice</span> cap and Greenland <span class="hlt">ice</span> sheet evolution</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Lecavalier, Benoit S.; Fisher, David A.; Milne, Glenn A.; Vinther, Bo M.; Tarasov, Lev; Lacelle, Denis; Main, Brittany; Zheng, James; Bourgeois, Jocelyne; Dyke, Arthur S.</p> <p>2017-01-01</p> <p>We present a revised and extended high Arctic air temperature reconstruction from a single proxy that spans the past ∼12,000 y (up to 2009 CE). Our reconstruction from the Agassiz <span class="hlt">ice</span> cap (Ellesmere Island, Canada) indicates an earlier and warmer Holocene thermal maximum with early Holocene temperatures that are 4–5 °C warmer compared with a previous reconstruction, and regularly exceed contemporary values for a period of ∼3,000 y. Our results show that air temperatures in this region are now at their warmest in the past 6,800–7,800 y, and that the recent rate of temperature change is unprecedented over the entire Holocene. The warmer early Holocene inferred from the Agassiz <span class="hlt">ice</span> core leads to an estimated ∼1 km of <span class="hlt">ice</span> thinning in northwest Greenland during the early Holocene using the Camp Century <span class="hlt">ice</span> core. <span class="hlt">Ice</span> modeling results show that this large thinning is consistent with our air temperature reconstruction. The modeling results also demonstrate the broader significance of the enhanced warming, with a retreat of the northern <span class="hlt">ice</span> <span class="hlt">margin</span> behind its present position in the mid Holocene and a ∼25% increase in total Greenland <span class="hlt">ice</span> sheet mass loss (∼1.4 m sea-level equivalent) during the last deglaciation, both of which have implications for interpreting geodetic measurements of land uplift and gravity changes in northern Greenland. PMID:28512225</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3753075','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3753075"><span>Provider’s Perspectives on the Impact of Immigration and Customs Enforcement (<span class="hlt">ICE</span>) <span class="hlt">Activity</span> on Immigrant Health</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Hacker, Karen; Chu, Jocelyn; Arsenault, Lisa; Marlin, Robert P.</p> <p>2013-01-01</p> <p>Introduction Increasing Immigration and Customs Enforcement (<span class="hlt">ICE</span>) <span class="hlt">activities</span> such as raids, detention and deportation may be affecting the health and well-being of immigrants. This study sought to understand the impact of <span class="hlt">ICE</span> <span class="hlt">activities</span> on immigrant health from the perspective of health care providers. Methods An online survey of primary care and emergency medicine providers was conducted to determine whether <span class="hlt">ICE</span> <span class="hlt">activity</span> was negatively affecting immigrant patients. Results Of 327 providers surveyed, 163 responded (50%) and 156 (48%) met criteria for inclusion. Seventy-five (48%) of them observed negative effects of <span class="hlt">ICE</span> enforcement on the health or health access of immigrant patients. Forty-three providers gave examples of the impact on emotional health, ability to comply with health care recommendations and access. Conclusions Health care providers are witnessing the negative effects of <span class="hlt">ICE</span> <span class="hlt">activities</span> on their immigrant patients’ psychological and physical health. This should be considered an important determinant of immigrant health. PMID:22643614</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19727498','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19727498"><span>Cloud condensation nuclei and <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> of hydrophobic and hydrophilic soot particles.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Koehler, Kirsten A; DeMott, Paul J; Kreidenweis, Sonia M; Popovicheva, Olga B; Petters, Markus D; Carrico, Christian M; Kireeva, Elena D; Khokhlova, Tatiana D; Shonija, Natalia K</p> <p>2009-09-28</p> <p>Cloud condensation nuclei (CCN) <span class="hlt">activity</span> and <span class="hlt">ice</span> nucleation behavior (for temperatures<or=-40 degrees C) of soot aerosols relevant for atmospheric studies were investigated. Soots were chosen to represent a range of physico-chemical properties, from hydrophobic through a range of hydrophilicity, to hygroscopic. These characteristics were achieved through generation by three different combustion sources; three soots from natural gas pyrolysis (original: TS; graphitized: GTS; and oxidized: TOS), soot from a diffusion flame in an oil lamp burning aviation kerosene (TC1), and soot from a turbulent diffusion flame in an aircraft engine combustor (AEC). All of the samples exhibited some heterogeneity in our experiments, which showed evidence of two or more particle sub-types even within a narrow size cut. The heterogeneity could have resulted from both chemical and sizing differences, the latter attributable in part to particle non-sphericity. Neither GTS nor TS, hydrophobic particles distinguished only by the lower porosity and polarity of the GTS surface, showed CCN <span class="hlt">activity</span> at or below water supersaturations required for wettable, insoluble particles (the Kelvin limit). TC1 soot particles, despite classification as hydrophilic, did not show CCN <span class="hlt">activity</span> at or below the Kelvin limit. We attribute this result to the microporosity of this soot. In contrast, oxidized, non-porous, and hydrophilic TOS particles exhibited CCN <span class="hlt">activation</span> at very near the Kelvin limit, with a small percentage of these particles CCN-<span class="hlt">active</span> even at lower supersaturations. Due to containing a range of surface coverage of organic and inorganic hydrophilic and hygroscopic compounds, up to approximately 35% of hygroscopic AEC particles were <span class="hlt">active</span> as CCN, with a small percentage of these particles CCN-<span class="hlt">active</span> at lower supersaturations. In <span class="hlt">ice</span> nucleation experiments below -40 degrees C, AEC particles nucleated <span class="hlt">ice</span> near the expected condition for homogeneous freezing of water from aqueous solutions. In</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.4260C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.4260C"><span>Landforms, sediments and dates to constrain rates and style of marine-influenced <span class="hlt">ice</span> sheet decay; the BRITICE-CHRONO project.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clark, Chris</p> <p>2014-05-01</p> <p>Uncertainty exists regarding the future mass of the Antarctic and Greenland <span class="hlt">ice</span> sheets and how they will respond to forcings from sea level, and atmospheric and ocean temperatures. If we want to know more about the mechanisms and rate of change of shrinking <span class="hlt">ice</span> sheets, then why not examine an <span class="hlt">ice</span> sheet that has fully disappeared and track its retreat through time? If achieved in enough detail such information on <span class="hlt">ice</span> retreat could be a data-rich playground for improving the next breed of numerical <span class="hlt">ice</span> sheet models to be used in <span class="hlt">ice</span> and sea level forecasting. We regard that the last British-Irish <span class="hlt">Ice</span> Sheet is a good target for this work, on account of its small size, density of information and with its numerous researchers already investigating it. Geomorphological mapping across the British Isles and the surrounding continental shelf has revealed the nature and distribution of glacial landforms. Here we demonstrate how such data have been used to build a pattern of <span class="hlt">ice</span> <span class="hlt">margin</span> retreat. The BRITICE-CHRONO consortium of Quaternary scientists and glaciologists, are now working on a project running from 2012 - 2017 to produce an <span class="hlt">ice</span> sheet wide database of geochronometric dates to constrain and then understand <span class="hlt">ice</span> <span class="hlt">margin</span> retreat. This is being achieved by focusing on 8 transects running from the continental shelf edge to a short distance (10s km) onshore and acquiring marine and terrestrial samples for geochronometric dating. The project includes funding for 587 radiocarbon, 140 OSL and 158 TCN samples for surface exposure dating; with sampling accomplished by two research cruises and 16 fieldwork campaigns. Results will reveal the timing and rate of change of <span class="hlt">ice</span> <span class="hlt">margin</span> recession for each transect, and combined with existing landform and dating databases, will be used to build an <span class="hlt">ice</span> sheet-wide empirical reconstruction of retreat. Simulations using two numerical <span class="hlt">ice</span> sheet models, fitted against the <span class="hlt">margin</span> data, will help us understand the nature and significance of sea</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930026876&hterms=ice+mechanics&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dice%2Bmechanics','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930026876&hterms=ice+mechanics&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dice%2Bmechanics"><span><span class="hlt">Ice</span> tracking techniques, implementation, performance, and applications</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rothrock, D. A.; Carsey, F. D.; Curlander, J. C.; Holt, B.; Kwok, R.; Weeks, W. F.</p> <p>1992-01-01</p> <p>Present techniques of <span class="hlt">ice</span> tracking make use both of cross-correlation and of edge tracking, the former being more successful in heavy pack <span class="hlt">ice</span>, the latter being critical for the broken <span class="hlt">ice</span> of the pack <span class="hlt">margins</span>. Algorithms must assume some constraints on the spatial variations of displacements to eliminate fliers, but must avoid introducing any errors into the spatial statistics of the measured displacement field. We draw our illustrations from the implementation of an automated tracking system for kinematic analyses of ERS-1 and JERS-1 SAR imagery at the University of Alaska - the Alaska SAR Facility's Geophysical Processor System. Analyses of the <span class="hlt">ice</span> kinematic data that might have some general interest to analysts of cloud-derived wind fields are the spatial structure of the fields, and the evaluation and variability of average deformation and its invariants: divergence, vorticity and shear. Many problems in sea <span class="hlt">ice</span> dynamics and mechanics can be addressed with the kinematic data from SAR.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.pet.hw.ac.uk/icgh7/programme.html','USGSPUBS'); return false;" href="http://www.pet.hw.ac.uk/icgh7/programme.html"><span>Evidence and biogeochemical implications for glacially-derived sediments in an <span class="hlt">active</span> <span class="hlt">margin</span> cold seep</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Pohlman, John W.; Riedel, Michael; Novosel, Ivana; Bauer, James E.; Canuel, Elizabeth A.; Paull, Charles K.; Coffin, Richard B.; Grabowski, Kenneth S.; Knies, David L.; Hyndman, Roy D.; Spence, George D.</p> <p>2011-01-01</p> <p>Delineating sediment organic matter origins and sediment accumulation rates at gas hydratebearing and hydrocarbon seeps is complicated by the microbial transfer of 13C-depleted and 14Cdepleted methane carbon into sedimentary pools. Sediment 13C and 14C measurements from four cores recovered at Bullseye vent on the northern Cascadia <span class="hlt">margin</span> are used to identify methane carbon assimilation into different carbon pools. While the total organic carbon (TOC) is mostly unaltered and primarily terrigenous in origin, planktonic foraminifera and the bulk carbonate display evidence of methane overprinting. Mass balance models are applied to determine the extent to which methane overprinting increased the radiocarbon ages of the biogenic foraminifera. The corrected and calibrated foraminifera ages between sediment depths of 70 and 573 cm are from 14.9 to 15.9 ka BP, which coincides with the retreat of the late Quaternary Cordilleran <span class="hlt">Ice</span> Sheet from Vancouver Island. Uniform TOC _13C values of -24.5 ± 0.5‰ from the upper 8 meters of sediment at Bullseye vent suggest all cored material is Pleistocene-derived glacimarine material deposited as the <span class="hlt">ice</span> edge retreated landward. Bullseye vent is located within an uplifted sediment block isolated from turbidite deposition and has been a site of non-deposition since the <span class="hlt">ice</span> sheet retreated from the shelf. Biogeochemical implications of seep sediments being dominated by aged, organic-poor (<0.4 wt% TOC) material are that methane is the primary energy source, and microbes directly and indirectly associated with the anaerobic oxidation of methane (AOM) will dominate the seep microbial community.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C53C0724S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C53C0724S"><span>Ross <span class="hlt">Ice</span> Shelf, Antarctica: Bathymetry, Structural Geology and Ocean Circulation from New <span class="hlt">Ice</span>Pod Airborne Geophysical Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Siddoway, C. S.; Tinto, K. J.; Bell, R. E.; Padman, L.; Fricker, H. A.; Springer, S. R.</p> <p>2016-12-01</p> <p>Rock exposures in the Ford Ranges, Marie Byrd Land (MBL), on the eastern <span class="hlt">margin</span> of the Ross Embayment, contain direct evidence of the geological processes that led to formation of West Antarctica's continental lithosphere. Processes include wide regional extension, volcanism, and thermal reequilibration, with creation of crustal structures that are prone to reactivation today. Marie Byrd Land is tectonically <span class="hlt">active</span>, as is evident from Late Pleistocene to Holocene eruptive centers, englacial volcanic tephra as young as 2200 years, a site of magma propagation inferred from POLEnet seismic records, and the occurrence of a 2012 earthquake cluster of magnitude M4.4 to M5.5 north of Edward VII Peninsula. However, the lithosphere underlying the Ross <span class="hlt">Ice</span> Shelf (RIS) is poorly known due to the thick cover of shelf <span class="hlt">ice</span> floating on the ocean, difficult to penetrate by satellite remote sensing or other methods. Airborne geophysical data for the Ford Ranges and the Ross <span class="hlt">Ice</span> Shelf (RIS) suggest that the rock formations and structures that underlie MBL continue beneath the RIS. Notable features known in outcrop and detected/inferred from potential fields data are Pleistocene or younger mafic volcanic centers and Cretaceous core complexes, both likely associated with wrench faults. The Ford Ranges legacy dataset that now provides a fundamental basis for sub-RIS geological interpretation is a product of research in coastal MBL led by B.P. Luyendyk from 1989 - 2006. To improve our knowledge of lithospheric evolution, identify <span class="hlt">active</span> faults and prospective zones of volcanism/heat flow, and to determine the sub-RIS bathymetry, the RIS sector is being explored via new Icepod aerogeophysics acquisition during the ROSETTA-<span class="hlt">Ice</span> project (Ross Ocean and <span class="hlt">ice</span> Shelf Environment, and Tectonic setting Through Aerogeophysical surveys and modeling), now underway over this vast under-explored sector of the Ross Embayment. ROSETTA-<span class="hlt">Ice</span> collects and employs new gravity data with magnetics to delineate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910031085&hterms=marginal&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dmarginal','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910031085&hterms=marginal&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dmarginal"><span>Preliminary observations of Labrador Sea <span class="hlt">marginal</span> <span class="hlt">ice</span> zone rheology using C-band SAR</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Drinkwater, Mark R.; Squire, Vernon A.</p> <p>1989-01-01</p> <p>SAR imagery collected in the Labrador Sea during Limex '87 are used to interpret modes of sea-<span class="hlt">ice</span> deformation. The <span class="hlt">ice</span> canopy exhibited two distinct rheologies separated by a clear line of shear; a quasi-brittle inner regime and a nonlinear viscous outer regime. A single constitutive relation capable of modeling both is unlikely within a plastic rate-independent formulation. Rate dependent effects are discussed as an explanation for brittle fracture in ductile materials.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018CliPa..14..619B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018CliPa..14..619B"><span>Simulation of the Greenland <span class="hlt">Ice</span> Sheet over two glacial-interglacial cycles: investigating a sub-<span class="hlt">ice</span>-shelf melt parameterization and relative sea level forcing in an <span class="hlt">ice-sheet-ice</span>-shelf model</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 L.; Reerink, Thomas J.; van de Wal, Roderik S. W.; Helsen, Michiel M.</p> <p>2018-05-01</p> <p>Observational evidence, including offshore moraines and sediment cores, confirm that at the Last Glacial Maximum (LGM) the Greenland <span class="hlt">ice</span> sheet (GrIS) expanded to a significantly larger spatial extent than seen at present, grounding into Baffin Bay and out onto the continental shelf break. Given this larger spatial extent and its close proximity to the neighbouring Laurentide <span class="hlt">Ice</span> Sheet (LIS) and Innuitian <span class="hlt">Ice</span> Sheet (IIS), it is likely these <span class="hlt">ice</span> sheets will have had a strong non-local influence on the spatial and temporal behaviour of the GrIS. Most previous paleo <span class="hlt">ice</span>-sheet modelling simulations recreated an <span class="hlt">ice</span> sheet that either did not extend out onto the continental shelf or utilized a simplified marine <span class="hlt">ice</span> parameterization which did not fully include the effect of <span class="hlt">ice</span> shelves or neglected the sensitivity of the GrIS to this non-local bedrock signal from the surrounding <span class="hlt">ice</span> sheets. In this paper, we investigated the evolution of the GrIS over the two most recent glacial-interglacial cycles (240 ka BP to the present day) using the <span class="hlt">ice-sheet-ice</span>-shelf model IMAU-<span class="hlt">ICE</span>. We investigated the solid earth influence of the LIS and IIS via an offline relative sea level (RSL) forcing generated by a glacial isostatic adjustment (GIA) model. The RSL forcing governed the spatial and temporal pattern of sub-<span class="hlt">ice</span>-shelf melting via changes in the water depth below the <span class="hlt">ice</span> shelves. In the ensemble of simulations, at the glacial maximums, the GrIS coalesced with the IIS to the north and expanded to the continental shelf break to the southwest but remained too restricted to the northeast. In terms of the global mean sea level contribution, at the Last Interglacial (LIG) and LGM the <span class="hlt">ice</span> sheet added 1.46 and -2.59 m, respectively. This LGM contribution by the GrIS is considerably higher (˜ 1.26 m) than most previous studies whereas the contribution to the LIG highstand is lower (˜ 0.7 m). The spatial and temporal behaviour of the northern <span class="hlt">margin</span> was highly variable in all simulations</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140009622','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140009622"><span>Insights into Spatial Sensitivities of <span class="hlt">Ice</span> Mass Response to Environmental Change from the SeaRISE <span class="hlt">Ice</span> Sheet Modeling Project I: Antarctica</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nowicki, Sophie; Bindschadler, Robert A.; Abe-Ouchi, Ayako; Aschwanden, Andy; Bueler, Ed; Choi, Hyengu; Fastook, Jim; Granzow, Glen; Greve, Ralf; Gutowski, Gail; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20140009622'); toggleEditAbsImage('author_20140009622_show'); toggleEditAbsImage('author_20140009622_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20140009622_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20140009622_hide"></p> <p>2013-01-01</p> <p>Atmospheric, oceanic, and subglacial forcing scenarios from the Sea-level Response to <span class="hlt">Ice</span> Sheet Evolution (SeaRISE) project are applied to six three-dimensional thermomechanical <span class="hlt">ice</span>-sheet models to assess Antarctic <span class="hlt">ice</span> sheet sensitivity over a 500 year timescale and to inform future modeling and field studies. Results indicate (i) growth with warming, except within low-latitude basins (where inland thickening is outpaced by <span class="hlt">marginal</span> thinning); (ii) mass loss with enhanced sliding (with basins dominated by high driving stresses affected more than basins with low-surface-slope streaming <span class="hlt">ice</span>); and (iii) mass loss with enhanced <span class="hlt">ice</span> shelf melting (with changes in West Antarctica dominating the signal due to its marine setting and extensive <span class="hlt">ice</span> shelves; cf. minimal impact in the Terre Adelie, George V, Oates, and Victoria Land region of East Antarctica). <span class="hlt">Ice</span> loss due to dynamic changes associated with enhanced sliding and/or sub-shelf melting exceeds the gain due to increased precipitation. Furthermore, differences in results between and within basins as well as the controlling impact of sub-shelf melting on <span class="hlt">ice</span> dynamics highlight the need for improved understanding of basal conditions, grounding-zone processes, ocean-<span class="hlt">ice</span> interactions, and the numerical representation of all three.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70021530','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70021530"><span>Antarctic glacial history from numerical models and continental <span class="hlt">margin</span> sediments</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.; Cooper, A. K.; Huybrechts, P.</p> <p>1999-01-01</p> <p>The climate record of glacially transported sediments in prograded wedges around the Antarctic outer continental shelf, and their derivatives in continental rise drifts, may be combined to produce an Antarctic <span class="hlt">ice</span> sheet history, using numerical models of <span class="hlt">ice</span> sheet response to temperature and sea-level change. Examination of published models suggests several preliminary conclusions about <span class="hlt">ice</span> sheet history. The <span class="hlt">ice</span> sheet's present high sensitivity to sea-level change at short (orbital) periods was developed gradually as its size increased, replacing a declining sensitivity to temperature. Models suggest that the <span class="hlt">ice</span> sheet grew abruptly to 40% (or possibly more) of its present size at the Eocene-Oligocene boundary, mainly as a result of its own temperature sensitivity. A large but more gradual middle Miocene change was externally driven, probably by development of the Antarctic Circumpolar Current (ACC) and Polar Front, provided that a few million years' delay can be explained. The Oligocene <span class="hlt">ice</span> sheet varied considerably in size and areal extent, but the late Miocene <span class="hlt">ice</span> sheet was more stable, though significantly warmer than today's. This difference probably relates to the confining effect of the Antarctic continental <span class="hlt">margin</span>. Present-day numerical models of <span class="hlt">ice</span> sheet development are sufficient to guide current sampling plans, but sea-<span class="hlt">ice</span> formation, polar wander, basal topography and <span class="hlt">ice</span> streaming can be identified as factors meriting additional modelling effort in the future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002JMS....38...77H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002JMS....38...77H"><span>Distribution of bacterial biomass and <span class="hlt">activity</span> in the <span class="hlt">marginal</span> <span class="hlt">ice</span> zone of the central Barents Sea during summer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Howard-Jones, M. H.; Ballard, V. D.; Allen, A. E.; Frischer, M. E.; Verity, P. G.</p> <p>2002-12-01</p> <p>The purpose of this study was to determine bacterioplankton abundance and <span class="hlt">activity</span> in the Barents Sea using the novel modified vital stain and probe (mVSP) method. The mVSP is a protocol that combines DAPI and propidium iodide staining with 16S rRNA eubacterial-specific oligonucleotide probes to determine the physiological status of individual microbial cells. Bacterial abundance and metabolic <span class="hlt">activity</span> were measured in near-surface waters and with depth at stations in the central Barents Sea during a cruise in June/July 1999. Viral abundance was also determined for 19 transect stations and at depth (2-200 m) for five intensive 24-h stations. In general, bacterial and viral abundances varied across the transect, but showed peaks of abundance (6×10 9 cells l -1, 9×10 9 viruses l -1) in Polar Front water masses. Viruses were abundant in seawater and exceeded bacterial abundance. Metabolic <span class="hlt">activity</span> was determined for individual cells using 16S rRNA eubacterial-specific oligonucleotide probes, and for the total community with 3H-leucine incorporation. <span class="hlt">Activity</span> measured by oligonucleotide probes increased from south to north. The fraction of cells that were <span class="hlt">active</span> was lowest in the southern Barents Sea (20%) and highest in the Polar Front (53%). The proportion of cells at the 24-h stations that were determined to be <span class="hlt">active</span> decreased with depth, but not with distance from <span class="hlt">ice</span> cover. Leucine incorporation rates varied significantly and did not always correlate with probe measurements. The proportion of total cells that had compromised membranes and were therefore considered dead remained relatively constant (<10%) across the transect. The percent of dead cells in the near surface waters and at depth were statistically similar. The percent dead cells made up only a small fraction of the total population at the 24-h stations. The largest and most variable fraction of cells were those classified as low <span class="hlt">activity</span> (25-80%), which supports the hypothesis that a significant</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 Antarctic <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 Antarctic <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> <span class="hlt">margin</span> 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> <span class="hlt">margin</span> 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/2016QSRv..153...97P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016QSRv..153...97P"><span>The build-up, configuration, and dynamical sensitivity of the Eurasian <span class="hlt">ice</span>-sheet complex to Late Weichselian climatic and oceanic forcing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Patton, Henry; Hubbard, Alun; Andreassen, Karin; Winsborrow, Monica; Stroeven, Arjen P.</p> <p>2016-12-01</p> <p>The Eurasian <span class="hlt">ice</span>-sheet complex (EISC) was the third largest <span class="hlt">ice</span> mass during the Last Glacial Maximum (LGM), after the Antarctic and North American <span class="hlt">ice</span> sheets. Despite its global significance, a comprehensive account of its evolution from independent nucleation centres to its maximum extent is conspicuously lacking. Here, a first-order, thermomechanical model, robustly constrained by empirical evidence, is used to investigate the dynamics of the EISC throughout its build-up to its maximum configuration. The <span class="hlt">ice</span> flow model is coupled to a reference climate and applied at 10 km spatial resolution across a domain that includes the three main spreading centres of the Celtic, Fennoscandian and Barents Sea <span class="hlt">ice</span> sheets. The model is forced with the NGRIP palaeo-isotope curve from 37 ka BP onwards and model skill is assessed against collated flowsets, <span class="hlt">marginal</span> moraines, exposure ages and relative sea-level history. The evolution of the EISC to its LGM configuration was complex and asynchronous; the western, maritime <span class="hlt">margins</span> of the Fennoscandian and Celtic <span class="hlt">ice</span> sheets responded rapidly and advanced across their continental shelves by 29 ka BP, yet the maximum aerial extent (5.48 × 106 km2) and volume (7.18 × 106 km3) of the <span class="hlt">ice</span> complex was attained some 6 ka later at c. 22.7 ka BP. This maximum stand was short-lived as the North Sea and Atlantic <span class="hlt">margins</span> were already in retreat whilst eastern <span class="hlt">margins</span> were still advancing up until c. 20 ka BP. High rates of basal erosion are modelled beneath <span class="hlt">ice</span> streams and outlet glaciers draining the Celtic and Fennoscandian <span class="hlt">ice</span> sheets with extensive preservation elsewhere due to frozen subglacial conditions, including much of the Barents and Kara seas. Here, and elsewhere across the Norwegian shelf and North Sea, high pressure subglacial conditions would have promoted localised gas hydrate formation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018BGeo...15..529C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018BGeo...15..529C"><span>Spatial variations in snowpack chemistry, isotopic composition of NO3- and nitrogen deposition from the <span class="hlt">ice</span> sheet <span class="hlt">margin</span> to the coast of western Greenland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Curtis, Chris J.; Kaiser, Jan; Marca, Alina; Anderson, N. John; Simpson, Gavin; Jones, Vivienne; Whiteford, Erika</p> <p>2018-01-01</p> <p>The relative roles of anthropogenic nitrogen (N) deposition and climate change in causing ecological change in remote Arctic ecosystems, especially lakes, have been the subject of debate over the last decade. Some palaeoecological studies have cited isotopic signals (δ(15N)) preserved in lake sediments as evidence linking N deposition with ecological change, but a key limitation has been the lack of co-located data on both deposition input fluxes and isotopic composition of deposited nitrate (NO3-). In Arctic lakes, including those in western Greenland, previous palaeolimnological studies have indicated a spatial variation in δ(15N) trends in lake sediments but data are lacking for deposition chemistry, input fluxes and stable isotope composition of NO3-. In the present study, snowpack chemistry, NO3- stable isotopes and net deposition fluxes for the largest <span class="hlt">ice</span>-free region in Greenland were investigated to determine whether there are spatial gradients from the <span class="hlt">ice</span> sheet <span class="hlt">margin</span> to the coast linked to a gradient in precipitation. Late-season snowpack was sampled in March 2011 at eight locations within three lake catchments in each of three regions (<span class="hlt">ice</span> sheet <span class="hlt">margin</span> in the east, the central area near Kelly Ville and the coastal zone to the west). At the coast, snowpack accumulation averaged 181 mm snow water equivalent (SWE) compared with 36 mm SWE by the <span class="hlt">ice</span> sheet. Coastal snowpack showed significantly greater concentrations of marine salts (Na+, Cl-, other major cations), ammonium (NH4+; regional means 1.4-2.7 µmol L-1), total and non-sea-salt sulfate (SO42-; total 1.8-7.7, non-sea-salt 1.0-1.8 µmol L-1) than the two inland regions. Nitrate (1.5-2.4 µmol L-1) showed significantly lower concentrations at the coast. Despite lower concentrations, higher precipitation at the coast results in greater net deposition for NO3- as well as NH4+ and non-sea-salt sulfate (nss-SO42-) relative to the inland regions (lowest at Kelly Ville 6, 4 and 3; highest at coast 9, 17</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EPSC....9..636S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EPSC....9..636S"><span>The impact of radiatively <span class="hlt">active</span> water-<span class="hlt">ice</span> clouds on Martian mesoscale atmospheric circulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Spiga, A.; Madeleine, J.-B.; Hinson, D.; Navarro, T.; Forget, F.</p> <p>2014-04-01</p> <p>Background and Goals Water <span class="hlt">ice</span> clouds are a key component of the Martian climate [1]. Understanding the properties of the Martian water <span class="hlt">ice</span> clouds is crucial to constrain the Red Planet's climate and hydrological cycle both in the present and in the past [2]. In recent years, this statement have become all the more true as it was shown that the radiative effects of water <span class="hlt">ice</span> clouds is far from being as negligible as hitherto believed; water <span class="hlt">ice</span> clouds plays instead a key role in the large-scale thermal structure and dynamics of the Martian atmosphere [3, 4, 5]. Nevertheless, the radiative effect of water <span class="hlt">ice</span> clouds at lower scales than the large synoptic scale (the so-called meso-scales) is still left to be explored. Here we use for the first time mesoscale modeling with radiatively <span class="hlt">active</span> water <span class="hlt">ice</span> clouds to address this open question.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70027352','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70027352"><span>Fault-dominated deformation in an <span class="hlt">ice</span> dam during annual filling and drainage of a <span class="hlt">marginal</span> lake</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Walder, J.S.; Trabant, D.C.; Cunico, M.; Anderson, S.P.; Anderson, R. Scott; Fountain, A.G.; Malm, A.</p> <p>2005-01-01</p> <p><span class="hlt">Ice</span>-dammed Hidden Creek Lake, Alaska, USA, outbursts annually in about 2-3 days. As the lake fills, a wedge of water penetrates beneath the glacier, and the surface of this '<span class="hlt">ice</span> dam' rises; the surface then falls as the lake drains. Detailed optical surveying of the glacier near the lake allows characterization of <span class="hlt">ice</span>-dam deformation. Surface uplift rate is close to the rate of lake-level rise within about 400 m of the lake, then decreases by 90% over about 100 m. Such a steep gradient in uplift rate cannot be explained in terms of <span class="hlt">ice</span>-dam flexure. Moreover, survey targets spanning the zone of steep uplift gradient move relative to one another in a nearly reversible fashion as the lake fills and drains. Evidently, the zone of steep uplift gradient is a fault zone, with the faults penetrating the entire thickness of the <span class="hlt">ice</span> dam. Fault motion is in a reverse sense as the lake fills, but in a normal sense as the lake drains. As the overall fault pattern is the same from year to year, even though <span class="hlt">ice</span> is lost by calving, the faults must be regularly regenerated, probably by linkage of surface and bottom crevasses as <span class="hlt">ice</span> is advected toward the lake basin.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70013260','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70013260"><span><span class="hlt">ICE</span> AND DEBRIS IN THE FRETTED TERRAIN, 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>Lucchitta, Baerbel K.</p> <p>1984-01-01</p> <p>Viking moderate- and high-resolution images along the northern highland <span class="hlt">margin</span> were studied monoscopically and stereoscopically to contribute to an understanding of the development of fretted terrain. Results support the hypothesis that the fretting process involved flow facilitated by interstitial <span class="hlt">ice</span>. The process apparently continued for a long period of time, and debris-apron formation shaped the fretted terrain in the past as well as the present. Interstitial <span class="hlt">ice</span> in debris aprons is most likely derived from ground <span class="hlt">ice</span> obtained by sapping or scarp collapse. Debris aprons could have been removed by sublimation if they consisted mostly of <span class="hlt">ice</span>, or by deflation if they consisted mostly of debris. To remove the debris, wind erosion was either very intense early in martian history, or was intermittent, perhaps owing to climatic cycles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014APS..MARG40002H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014APS..MARG40002H"><span><span class="hlt">Ice</span> sheet-ocean interactions and sea level change</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Heimbach, Patrick</p> <p>2014-03-01</p> <p>Mass loss from the Greenland and Antarctic <span class="hlt">ice</span> sheets has increased rapidly since the mid-1990s. Their combined loss now accounts for about one-third of global sea level rise. In Greenland, a growing body of evidence points to the marine <span class="hlt">margins</span> of these glaciers as the region from which this dynamic response originated. Similarly, <span class="hlt">ice</span> streams in West Antarctica that feed vast floating <span class="hlt">ice</span> shelves have exhibited large decadal changes. We review observational evidence and present physical mechanisms that might explain the observed changes, in particular in the context of <span class="hlt">ice</span> sheet-ocean interactions. Processes involve cover 7 orders of magnitudes of scales, ranging from mm boundary-layer processes to basin-scale coupled atmosphere-ocean variability. We discuss observational needs to fill the gap in our mechanistic understanding.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_18 --> <div id="page_19" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="361"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA134872','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA134872"><span>MIZEX. A Program for Mesoscale Air-<span class="hlt">Ice</span>-Ocean Interaction Experiments in Arctic <span class="hlt">Marginal</span> <span class="hlt">Ice</span> Zones. II. A Science Plan for a Summer <span class="hlt">Marginal</span> <span class="hlt">Ice</span> Zone Experiment in the Fram Strait/Greenland Sea: 1984.</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1983-05-01</p> <p>size and thickness characteris- tics. N’ore complete analysis will require combin- ing <span class="hlt">ice</span> data with data obtained by the oceano - graphic... sol concentration and microwave brightness tem- perature. A long-range aircraft and a light aircraft Hying from Spitzbergen will study mesoscale</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 lake 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 lake outburst floods (GLOFs) remain poorly understood. This study used measurements of lake level at fifteen minute intervals and known lake bathymetry to calculate lake outflow during two GLOF events from the northern <span class="hlt">margin</span> 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. Lake 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-marginal</span> lakes. As <span class="hlt">ice</span> overburden pressure relative to lake 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 lake level, drainage timing, lake water temperature and consequently rising stage lake outflow and flood evolution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28942726','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28942726"><span>Screening of plant resources with anti-<span class="hlt">ice</span> nucleation <span class="hlt">activity</span> for frost damage prevention.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Suzuki, Shingo; Fukuda, Satoshi; Fukushi, Yukiharu; Arakawa, Keita</p> <p>2017-11-01</p> <p>Previous studies have shown that some polyphenols have anti-<span class="hlt">ice</span> nucleation <span class="hlt">activity</span> (anti-INA) against <span class="hlt">ice</span>-nucleating bacteria that contribute to frost damage. In the present study, leaf disk freezing assay, a test of in vitro application to plant leaves, was performed for the screening of anti-INA, which inhibits the <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> of an <span class="hlt">ice</span>-nucleating bacterium Erwinia ananas in water droplets on the leaf surfaces. The application of polyphenols with anti-INA, kaempferol 7-O-β-glucoside and (-)-epigallocatechin gallate, to the leaf disk freezing assay by cooling at -4--6 °C for 3 h, revealed that both the compounds showed anti-INAs against E. ananas in water droplets on the leaf surfaces. Further, this assay also revealed that the extracts of five plant leaves showed high anti-INA against E. ananas in water droplets on leaf surfaces, indicating that they are the candidate resources to protect crops from frost damage.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.1926B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.1926B"><span>BRITICE-CHRONO and GLANAM: new exciting developments in the study of circum-North Atlantic <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>Benetti, Sara; Clark, Chris D.; Petter Serjup, Hans</p> <p>2013-04-01</p> <p>This talk will present two newly funded projects on the reconstruction of former marine-based <span class="hlt">ice</span> sheets bordering the North Atlantic Ocean and their effects on the surrounding continental <span class="hlt">margins</span>. The NERC-funded BRITICE-CHRONO started in October 2012 and its consortium involves scientists from all over the UK with partners in Ireland, Canada and Norway. It aims to carry out a systematic campaign to collect and date material to constrain the timing and rates of change of the collapse of the former British-Irish <span class="hlt">Ice</span> Sheet. This will be achieved by focussing on eight transects running from the shelf edge to a short distance onshore and acquiring marine and terrestrial samples for geochronometric dating. The sampling will be accomplished by two research cruises and eight fieldwork campaigns around UK and Ireland. The project will result in the world's best empirical reconstruction of a shrinking <span class="hlt">ice</span> sheet, for use in improving <span class="hlt">ice</span> sheet models, and to provide the long term context against which contemporary observations can be assessed. The FP7-funded Marie Curie Initial Training Networks GLANAM (Glaciated North Atlantic <span class="hlt">Margins</span>) will start in April 2013 and aims at improving the career prospects and development of young researchers in both the public and private sector within the field of earth science, focusing specifically on North Atlantic glaciated <span class="hlt">margins</span>. The training network comprises ten partner institutions, both academic and industrial, from Norway, UK and Denmark and will train eleven PhD and four postdoctoral researchers. The young scientists will perform multi-disciplinary research and receive training through three interconnected workpackages that collectively address knowledge gaps related to the glacial sedimentary depocentres on the North Atlantic <span class="hlt">margins</span>. Filling these gaps will not only result in major new insights regarding glacial processes on continental <span class="hlt">margins</span> in general, but critically will have particular impact on the exploitation of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27951652','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27951652"><span>Multivalent Display of Antifreeze Proteins by Fusion to Self-Assembling Protein Cages Enhances <span class="hlt">Ice</span>-Binding <span class="hlt">Activities</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Phippen, Sean W; Stevens, Corey A; Vance, Tyler D R; King, Neil P; Baker, David; Davies, Peter L</p> <p>2016-12-13</p> <p>Antifreeze proteins (AFPs) are small monomeric proteins that adsorb to the surface of <span class="hlt">ice</span> to inhibit <span class="hlt">ice</span> crystal growth and impart freeze resistance to the organisms producing them. Previously, monomeric AFPs have been conjugated to the termini of branched polymers to increase their <span class="hlt">activity</span> through the simultaneous binding of more than one AFP to <span class="hlt">ice</span>. Here, we describe a superior approach to increasing AFP <span class="hlt">activity</span> through oligomerization that eliminates the need for conjugation reactions with varying levels of efficiency. A moderately <span class="hlt">active</span> AFP from a fish and a hyperactive AFP from an Antarctic bacterium were genetically fused to the C-termini of one component of the 24-subunit protein cage T33-21, resulting in protein nanoparticles that multivalently display exactly 12 AFPs. The resulting nanoparticles exhibited freezing point depression >50-fold greater than that seen with the same concentration of monomeric AFP and a similar increase in the level of <span class="hlt">ice</span>-recrystallization inhibition. These results support the anchored clathrate mechanism of binding of AFP to <span class="hlt">ice</span>. The enhanced freezing point depression could be due to the difficulty of overgrowing a larger AFP on the <span class="hlt">ice</span> surface and the improved <span class="hlt">ice</span>-recrystallization inhibition to the ability of the nanoparticle to simultaneously bind multiple <span class="hlt">ice</span> grains. Oligomerization of these proteins using self-assembling protein cages will be useful in a variety of biotechnology and cryobiology applications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.A11Q..02M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.A11Q..02M"><span>The Fifth International <span class="hlt">Ice</span> Nucleation Workshop <span class="hlt">Activities</span> FIN-1 and FIN-2: Overview and Selected Results</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moehler, O.; Cziczo, D. J.; DeMott, P. J.; Hiranuma, N.; Petters, M. D.</p> <p>2015-12-01</p> <p>The role of aerosol particles for <span class="hlt">ice</span> formation in clouds is one of the largest uncertainties in understanding the Earth's weather and climate systems, which is related to the poor knowledge of <span class="hlt">ice</span> nucleation microphysics or of the nature and atmospheric abundance of <span class="hlt">ice</span> nucleating particles (INPs). During the recent years, new mobile instruments were developed for measuring the concentration, size and chemical composition of INPs, which were tested during the three-part Fifth International <span class="hlt">Ice</span> Nucleation (FIN) workshop. The FIN <span class="hlt">activities</span> addressed not only instrument issues, but also important science topics like the nature of atmospheric INP and cloud <span class="hlt">ice</span> residuals, the <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> of relevant atmospheric aerosols, or the parameterization of <span class="hlt">ice</span> formation in atmospheric weather and climate models. The first <span class="hlt">activity</span> FIN-1 was conducted during November 2014 at the AIDA cloud chamber. It involved co-locating nine single particle mass spectrometers to evaluate how well they resolve the INP and <span class="hlt">ice</span> residual composition and how spectra from different instruments compare for relevant atmospheric aerosols. We conducted about 90 experiments with mineral, carbonaceous and biological aerosol types, some also coated with organic and inorganic compounds. The second <span class="hlt">activity</span> FIN-2 was conducted during March 2015 at the AIDA facility. A total of nine mobile INP instruments directly sampled from the AIDA aerosol chambers. Wet suspension and filter samples were also taken for offline INP processing. A refereed blind intercomparison was conducted during two days of the FIN-2 <span class="hlt">activity</span>. The third <span class="hlt">activity</span> FIN-3 will take place at the Desert Research Institute's Storm Peak Laboratory (SPL) in order to test the instruments' performance in the field. This contribution will introduce the FIN <span class="hlt">activities</span>, summarize first results from the formal part of FIN-2, and discuss selected results, mainly from FIN-1 for the effect of coating on the <span class="hlt">ice</span> nucleation (IN) by mineral</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2013-03-13/pdf/2013-05791.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2013-03-13/pdf/2013-05791.pdf"><span>78 FR 15876 - <span class="hlt">Activation</span> of <span class="hlt">Ice</span> Protection</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2013-03-13</p> <p>... procedures in the Airplane Flight Manual for operating in <span class="hlt">icing</span> conditions must be initiated. (2) Visual cues... procedures in the Airplane Flight Manual for operating in <span class="hlt">icing</span> conditions must be initiated. (3) If the... operating rules for flight in <span class="hlt">icing</span> conditions. This document corrects an error in the amendatory language...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C41B0701R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C41B0701R"><span>The Relationship Between Arctic Sea <span class="hlt">Ice</span> Albedo and the Geophysical Parameters of the <span class="hlt">Ice</span> Cover</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Riihelä, A.</p> <p>2015-12-01</p> <p>The Arctic sea <span class="hlt">ice</span> cover is thinning and retreating. Remote sensing observations have also shown that the mean albedo of the remaining <span class="hlt">ice</span> cover is decreasing on decadal time scales, albeit with significant annual variability (Riihelä et al., 2013, Pistone et al., 2014). Attribution of the albedo decrease between its different drivers, such as decreasing <span class="hlt">ice</span> concentration and enhanced surface melt of the <span class="hlt">ice</span>, remains an important research question for the forecasting of future conditions of the <span class="hlt">ice</span> cover. A necessary step towards this goal is understanding the relationships between Arctic sea <span class="hlt">ice</span> albedo and the geophysical parameters of the <span class="hlt">ice</span> cover. Particularly the question of the relationship between sea <span class="hlt">ice</span> albedo and <span class="hlt">ice</span> age is both interesting and not widely studied. The recent changes in the Arctic sea <span class="hlt">ice</span> zone have led to a substantial decrease of its multi-year sea <span class="hlt">ice</span>, as old <span class="hlt">ice</span> melts and is replaced by first-year <span class="hlt">ice</span> during the next freezing season. It is generally known that younger sea <span class="hlt">ice</span> tends to have a lower albedo than older <span class="hlt">ice</span> because of several reasons, such as wetter snow cover and enhanced melt ponding. However, the quantitative correlation between sea <span class="hlt">ice</span> age and sea <span class="hlt">ice</span> albedo has not been extensively studied to date, excepting in-situ measurement based studies which are, by necessity, focused on a limited area of the Arctic Ocean (Perovich and Polashenski, 2012).In this study, I analyze the dependencies of Arctic sea <span class="hlt">ice</span> albedo relative to the geophysical parameters of the <span class="hlt">ice</span> field. I use remote sensing datasets such as the CM SAF CLARA-A1 (Karlsson et al., 2013) and the NASA MeaSUREs (Anderson et al., 2014) as data sources for the analysis. The studied period is 1982-2009. The datasets are spatiotemporally collocated and analysed. The changes in sea <span class="hlt">ice</span> albedo as a function of sea <span class="hlt">ice</span> age are presented for the whole Arctic Ocean and for potentially interesting <span class="hlt">marginal</span> sea cases. This allows us to see if the the albedo of the older sea</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFMED13B0590H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFMED13B0590H"><span><span class="hlt">Ice</span>, <span class="hlt">Ice</span>, Baby: A Program for Sustained, Classroom-Based K-8 Teacher Professional Development</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hamilton, C.</p> <p>2009-12-01</p> <p><span class="hlt">Ice</span>, <span class="hlt">Ice</span>, Baby is a K-8 science program created by the education team at the Center for the Remote Sensing of <span class="hlt">Ice</span> Sheets (CReSIS), an NSF-funded science and technology center headquartered at the University of Kansas. The twenty-four hands-on <span class="hlt">activities</span>, which constitute the <span class="hlt">Ice</span>, <span class="hlt">Ice</span>, Baby curriculum, were developed to help students understand the role of polar <span class="hlt">ice</span> sheets in sea level rise. These <span class="hlt">activities</span>, presented in classrooms by CReSIS' Educational Outreach Coordinator, demonstrate many of the scientific properties of <span class="hlt">ice</span>, including displacement and density. Student journals are utilized with each lesson as a strategy for improving students' science process skills. Journals also help the instructor identify misconceptions, assess comprehension, and provide students with a year-long science reference log. Pre- and post- assessments are given to both teachers and students before and after the program, providing data for evaluation and improvement of the <span class="hlt">Ice</span>, <span class="hlt">Ice</span>, Baby program. While students are <span class="hlt">actively</span> engaged in hands-on learning about the unusual topics of <span class="hlt">ice</span> sheets, glaciers, icebergs and sea <span class="hlt">ice</span>, the CReSIS' Educational Coordinator is able to model best practices in science education, such as questioning and inquiry-based methods of instruction. In this way, the <span class="hlt">Ice</span>, <span class="hlt">Ice</span>, Baby program also serves as ongoing, in-class, professional development for teachers. Teachers are also provided supplemental <span class="hlt">activities</span> to do with their classes between CReSIS' visits to encourage additional science lessons, reinforce concepts taught in the <span class="hlt">Ice</span>, <span class="hlt">Ice</span>, Baby program, and to foster teachers' progression toward more reform-based science instruction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5446900-unlocking-ice-house-oligocene-miocene-oxygen-isotopes-eustasy-margin-erosion','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5446900-unlocking-ice-house-oligocene-miocene-oxygen-isotopes-eustasy-margin-erosion"><span>Unlocking the <span class="hlt">ice</span> house: Oligocene-Miocene oxygen isotopes, eustasy, and <span class="hlt">margin</span> erosion</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>Miller, K.G.; Wright, J.D.; Fairbanks, R.G.</p> <p>1991-04-10</p> <p>Benthic foraminiferal {delta}{sup 18}O records place limits on the history of glaciation, suggesting the presence of <span class="hlt">ice</span> sheets at least intermittently since the earliest Oligocene. The best indicator of <span class="hlt">ice</span> growth is a coeval increase in global benthic and western equatorial planktonic {delta}{sup 18}O records. Although planktonic isotope records from the western equatorial regions are limited, subtropical planktonic foraminifera may also record such <span class="hlt">ice</span> volume changes. It is difficult to apply these established principles to the Cenozoic {delta}{sup 18}O record because of the lack of adequate data and problems in stratigraphic correlations that obscure isotope events. The authors improved Oligocenemore » to Miocene correlations of {delta}{sup 18}O records and erected eight oxygen isotope zones (Oi1-Oi2, Mi1-Mi6). Benthic foraminiferal {delta}{sup 18}O increases which can be linked with {delta}{sup 18}O increases in subtropical planktonic foraminifera and with intervals of glacial sedimentation on or near Antarctica. These new correlations of middle Miocene benthic and western equatorial planktonic {delta}{sup 18}O records show remarkable agreement in timing and amplitude. They interpret benthic-planktonic covariance to reflect substantial <span class="hlt">ice</span> volume increases near the bases of Zones Mi2 (circa 16.1 Ma), Mi3 (circa 13.6 Ma), and possibly Mi5 (circa 11.3 Ma). Possible glacioeustatic lowerings are associated with the {delta}{sup 18}O increases which culminated with the bases of Zone Mi4 (circa 12.6 Ma) and Mi6 (circa 9.6 Ma), although low-latitude planktonic {delta}{sup 18}O records are required to test this. These inferred glacioeustatic lowerings can be linked to seismic and rock disconformities.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930063900&hterms=reciprocity&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dreciprocity','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930063900&hterms=reciprocity&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dreciprocity"><span>Application of theoretical models to <span class="hlt">active</span> and passive remote sensing of saline <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>Han, H. C.; Kong, J. A.; Shin, R. T.; Nghiem, S. V.; Kwok, R.</p> <p>1992-01-01</p> <p>The random medium model is used to interpret the polarimetric <span class="hlt">active</span> and passive measurements of saline <span class="hlt">ice</span>. The <span class="hlt">ice</span> layer is described as a host <span class="hlt">ice</span> medium embedded with randomly distributed inhomogeneities, and the underlying sea water is considered as a homogeneous half-space. The scatterers in the <span class="hlt">ice</span> layer are modeled with an ellipsoidal correlation function. The orientation of the scatterers is vertically aligned and azimuthally random. The strong permittivity fluctuation theory is used to calculate the effective permittivity and the distorted Born approximation is used to obtain the polarimetric scattering coefficients. Thermal emissions based on the reciprocity and energy conservation principles are calculated. The effects of the random roughness at the air-<span class="hlt">ice</span>, and <span class="hlt">ice</span>-water interfaces are explained by adding the surface scattering to the volume scattering return incoherently. The theoretical model, which has been successfully applied to analyze the radar backscatter data of first-year sea <span class="hlt">ice</span>, is used to interpret the measurements performed in the Cold Regions Research and Engineering Laboratory's CRRELEX program.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19930003898','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930003898"><span>Application of theoretical models to <span class="hlt">active</span> and passive remote sensing of saline <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>Han, H. C.; Kong, Jin AU; Shin, Robert T.; Nghiem, Son V.; Kwok, R.</p> <p>1992-01-01</p> <p>The random medium model is used to interpret the polarimetric <span class="hlt">active</span> and passive measurements of saline <span class="hlt">ice</span>. The <span class="hlt">ice</span> layer is described as a host <span class="hlt">ice</span> medium embedded with randomly distributed inhomogeneities, and the underlying sea water is considered as a homogeneous half-space. The scatterers in the <span class="hlt">ice</span> layer are modeled with an ellipsoidal correlation function. The orientation of the scatterers is vertically aligned and azimuthally random. The strong permittivity fluctuation theory is employed to calculate the effective permittivity and the distorted Born approximation is used to obtain the polarimetric scattering coefficients. We also calculate the thermal emissions based on the reciprocity and energy conservation principles. The effects of the random roughness at the air-<span class="hlt">ice</span>, and <span class="hlt">ice</span>-water interfaces are accounted for by adding the surface scattering to the volume scattering return incoherently. The above theoretical model, which has been successfully applied to analyze the radar backscatter data of the first-year sea <span class="hlt">ice</span> near Point Barrow, AK, is used to interpret the measurements performed in the CRRELEX program.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C11E..08R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C11E..08R"><span>Chronicling <span class="hlt">ice</span> shelf history in the sediments left behind</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rosenheim, B. E.; Subt, C.; Shevenell, A.; Guitard, M.; Vadman, K. J.; DeCesare, M.; Wellner, J. S.; Bart, P. J.; Lee, J. I.; Domack, E. W.; Yoo, K. C.; Hayes, J. M.</p> <p>2017-12-01</p> <p>Collapsing and retreating <span class="hlt">ice</span> shelves leave unmistakable sediment sequences on the Antarctic <span class="hlt">margin</span>. These sequences tell unequivocal stories of collapse or retreat through a typical progression of sub-<span class="hlt">ice</span> shelf diamicton (marking the past positions of grounding lines), sequentially overlain by a granulated facies from beneath the <span class="hlt">ice</span> shelf, <span class="hlt">ice</span> rafted debris from the calving line, and finally open marine sediment. The timelines to these stories, however, are troublesome. Difficulties in chronicling these stories recorded in sediment have betrayed their importance to our understanding of a warming world in many cases. The difficulties involve the concerted lack of preservation/production of calcium carbonate tests from the water column above and admixture of relict organic material from older sources of carbon. Here, we summarize our advances in the last decade of overcoming difficulties associated with the paucity of carbonate and creating chronologies of <span class="hlt">ice</span> shelf retreat into the deglacial history of Antarctica by exploiting the range of thermochemical stability in organic matter (Ramped PyrOx) from these sediment sequences. We describe our success in comparing Ramped PyrOx 14C dates with foraminiferal dates, the relationship between sediment facies and radiocarbon age spectrum, and our ability to push limits of dating sediments deposited underneath <span class="hlt">ice</span> shelves. With attention to the caveats of recent dating developments, we summarize expectations that geologist should have when coring the Antarctic <span class="hlt">margins</span> to discern deglacial history. Perhaps most important among these expectations is the ability to design coring expeditions without regard to our ability to date calcium carbonate microfossils within the cores, in essence removing suspense of knowing whether cores taken from crucial paleo <span class="hlt">ice</span> channels and other bathymetric features will ultimately yield a robust chronology for its sedimentary sequence.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26258729','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26258729"><span>Probing the Biomimetic <span class="hlt">Ice</span> Nucleation Inhibition <span class="hlt">Activity</span> of Poly(vinyl alcohol) and Comparison to Synthetic and Biological Polymers.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Congdon, Thomas; Dean, Bethany T; Kasperczak-Wright, James; Biggs, Caroline I; Notman, Rebecca; Gibson, Matthew I</p> <p>2015-09-14</p> <p>Nature has evolved many elegant solutions to enable life to flourish at low temperatures by either allowing (tolerance) or preventing (avoidance) <span class="hlt">ice</span> formation. These processes are typically controlled by <span class="hlt">ice</span> nucleating proteins or antifreeze proteins, which act to either promote nucleation, prevent nucleation or inhibit <span class="hlt">ice</span> growth depending on the specific need, respectively. These proteins can be expensive and their mechanisms of action are not understood, limiting their translation, especially into biomedical cryopreservation applications. Here well-defined poly(vinyl alcohol), synthesized by RAFT/MADIX polymerization, is investigated for its <span class="hlt">ice</span> nucleation inhibition (INI) <span class="hlt">activity</span>, in contrast to its established <span class="hlt">ice</span> growth inhibitory properties and compared to other synthetic polymers. It is shown that <span class="hlt">ice</span> nucleation inhibition <span class="hlt">activity</span> of PVA has a strong molecular weight dependence; polymers with a degree of polymerization below 200 being an effective inhibitor at just 1 mg.mL(-1). Other synthetic and natural polymers, both with and without hydroxyl-functional side chains, showed negligible <span class="hlt">activity</span>, highlighting the unique <span class="hlt">ice</span>/water interacting properties of PVA. These findings both aid our understanding of <span class="hlt">ice</span> nucleation but demonstrate the potential of engineering synthetic polymers as new biomimetics to control <span class="hlt">ice</span> formation/growth processes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4577968','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4577968"><span>Probing the Biomimetic <span class="hlt">Ice</span> Nucleation Inhibition <span class="hlt">Activity</span> of Poly(vinyl alcohol) and Comparison to Synthetic and Biological Polymers</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p></p> <p>2015-01-01</p> <p>Nature has evolved many elegant solutions to enable life to flourish at low temperatures by either allowing (tolerance) or preventing (avoidance) <span class="hlt">ice</span> formation. These processes are typically controlled by <span class="hlt">ice</span> nucleating proteins or antifreeze proteins, which act to either promote nucleation, prevent nucleation or inhibit <span class="hlt">ice</span> growth depending on the specific need, respectively. These proteins can be expensive and their mechanisms of action are not understood, limiting their translation, especially into biomedical cryopreservation applications. Here well-defined poly(vinyl alcohol), synthesized by RAFT/MADIX polymerization, is investigated for its <span class="hlt">ice</span> nucleation inhibition (INI) <span class="hlt">activity</span>, in contrast to its established <span class="hlt">ice</span> growth inhibitory properties and compared to other synthetic polymers. It is shown that <span class="hlt">ice</span> nucleation inhibition <span class="hlt">activity</span> of PVA has a strong molecular weight dependence; polymers with a degree of polymerization below 200 being an effective inhibitor at just 1 mg.mL–1. Other synthetic and natural polymers, both with and without hydroxyl-functional side chains, showed negligible <span class="hlt">activity</span>, highlighting the unique <span class="hlt">ice</span>/water interacting properties of PVA. These findings both aid our understanding of <span class="hlt">ice</span> nucleation but demonstrate the potential of engineering synthetic polymers as new biomimetics to control <span class="hlt">ice</span> formation/growth processes PMID:26258729</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16349347','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16349347"><span>Bacterial Standing Stock, <span class="hlt">Activity</span>, and Carbon Production during Formation and Growth of Sea <span class="hlt">Ice</span> in the Weddell Sea, Antarctica.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Grossmann, S; Dieckmann, G S</p> <p>1994-08-01</p> <p>Bacterial response to formation and growth of sea <span class="hlt">ice</span> was investigated during autumn in the northeastern Weddell Sea. Changes in standing stock, <span class="hlt">activity</span>, and carbon production of bacteria were determined in successive stages of <span class="hlt">ice</span> development. During initial <span class="hlt">ice</span> formation, concentrations of bacterial cells, in the order of 1 x 10 to 3 x 10 liter, were not enhanced within the <span class="hlt">ice</span> matrix. This suggests that physical enrichment of bacteria by <span class="hlt">ice</span> crystals is not effective. Due to low concentrations of phytoplankton in the water column during freezing, incorporation of bacteria into newly formed <span class="hlt">ice</span> via attachment to algal cells or aggregates was not recorded in this study. As soon as the <span class="hlt">ice</span> had formed, the general metabolic <span class="hlt">activity</span> of bacterial populations was strongly suppressed. Furthermore, the ratio of [H]leucine incorporation into proteins to [H]thymidine incorporation into DNA changed during <span class="hlt">ice</span> growth. In thick pack <span class="hlt">ice</span>, bacterial <span class="hlt">activity</span> recovered and growth rates up to 0.6 day indicated <span class="hlt">actively</span> dividing populations. However, biomass-specific utilization of organic compounds remained lower than in open water. Bacterial concentrations of up to 2.8 x 10 cells liter along with considerably enlarged cell volumes accumulated within thick pack <span class="hlt">ice</span>, suggesting reduced mortality rates of bacteria within the small brine pores. In the course of <span class="hlt">ice</span> development, bacterial carbon production increased from about 0.01 to 0.4 mug of C liter h. In thick <span class="hlt">ice</span>, bacterial secondary production exceeded primary production of microalgae.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1997PhDT........88C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1997PhDT........88C"><span>Neoglacial fluctuations of terrestrial, tidewater, and calving lacustrine glaciers, Blackstone-Spencer <span class="hlt">Ice</span> Complex, Kenai Mountains, Alaska</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Crossen, Kristine June</p> <p>1997-12-01</p> <p>The glaciers surrounding the Blackstone-Spencer <span class="hlt">Ice</span> Complex display a variety of termini types: Tebenkov, Spencer, Bartlett, Skookum, Trail, Burns, Shakespeare, Marquette, Lawrence, and Ripon glaciers end in terrestrial <span class="hlt">margins</span>; Blackstone and Beloit glaciers have tidewater termini; and Portage Glacier has a calving lacustrine <span class="hlt">margin</span>. In addition, steep temperature and precipitation gradients exist across the <span class="hlt">ice</span> complex from the maritime environment of Prince William Sound to the colder, drier interior. The Neoglacial history of Tebenkov Glacier, as based on overrun trees near the terminus, shows advances ca. 250- 430 AD (calibrated date), ca. 1215-1275 AD (calibrated date), and ca. 1320-1430 AD (tree ring evidence), all intervals of glacier advance around the Gulf of Alaska. However, two tidewater glaciers in Blackstone Bay retreated from their outermost moraines by 1350 AD, apparently asynchronously with respect to the regional climate signal. The most extensive Kenai Mountain glacier expansions during Neoglaciation occurred in the late Little <span class="hlt">Ice</span> Age. The outermost moraines are adjacent to mature forest stands and bog peats that yield dates as old as 5,600 BP. Prince William Sound glaciers advanced during two Little <span class="hlt">Ice</span> Age cold periods, 1380-1680 and 1830-1900 AD. The terrestrial glaciers around the Blackstone-Spencer <span class="hlt">Ice</span> Complex all built moraines during the 19th century and began retreating between 1875 and 1900 AD. Portage and Burns glaciers began retreating between 1790 and 1810 AD, but their <span class="hlt">margins</span> remained close to the outermost moraines during the 19th century. Regional glacier fluctuations are broadly synchronous in the Gulf of Alaska region. With the exception of the two tidewater glaciers in Blackstone Bay, all glaciers in the Kenai Mountains, no matter their sizes, altitudes, orientations, or types of <span class="hlt">margins</span>, retreated at the end of the Little <span class="hlt">Ice</span> Age. The climate signal, especially temperature, appears to be the strongest control on glacier</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27192099','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27192099"><span>Passive Anti-<span class="hlt">Icing</span> and <span class="hlt">Active</span> Deicing Films.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Tuo; Zheng, Yonghao; Raji, Abdul-Rahman O; Li, Yilun; Sikkema, William K A; Tour, James M</p> <p>2016-06-08</p> <p>Anti-<span class="hlt">icing</span> and deicing are the two major pathways for suppressing adhesion of <span class="hlt">ice</span> on surfaces, yet materials with dual capabilities are rare. In this work, we have designed a perfluorododecylated graphene nanoribbon (FDO-GNR) film that takes advantage of both the low polarizability of perfluorinated carbons and the intrinsic conductive nature of graphene nanoribbons. The FDO-GNR films are superhydrophobic with a sheet resistance below 8 kΩ·sq(-1) and then exhibit an anti-<span class="hlt">icing</span> property that prevents freezing of incoming <span class="hlt">ice</span>-cold water down to -14 °C. After that point, voltage can be applied to the films to resistively heat and deice the surface. Further a lubricating liquid can be employed to create a slippery surface to improve the film's deicing performance. The FDO-GNR films can be easily switched between the superhydrophobic anti-<span class="hlt">icing</span> mode and the slippery deicing mode by applying the lubricant. A spray-coating method makes it suitable for large-scale applications. The anti-<span class="hlt">icing</span> and deicing properties render the FDO-GNR films with promise for use in extreme environments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19850003124','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19850003124"><span><span class="hlt">Active</span> microwave measurements of sea <span class="hlt">ice</span> under fall conditions: The RADARSAT/FIREX fall experiment. [in the Canadian Arctic</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Onstott, R. G.; Kim, Y. S.; Moore, R. K.</p> <p>1984-01-01</p> <p>A series of measurements of the <span class="hlt">active</span> microwave properties of sea <span class="hlt">ice</span> under fall growing conditions was conducted. <span class="hlt">Ice</span> in the inland waters of Mould Bay, Crozier Channel, and intrepid inlet and <span class="hlt">ice</span> in the Arctic Ocean near Hardinge Bay was investigated. <span class="hlt">Active</span> microwave data were acquired using a helicopter borne scatterometer. Results show that multiyear <span class="hlt">ice</span> frozen in grey or first year <span class="hlt">ice</span> is easily detected under cold fall conditions. Multiyear <span class="hlt">ice</span> returns were dynamic due to response to two of its scene constituents. Floe boundaries between thick and thin <span class="hlt">ice</span> are well defined. Multiyear pressure ridge returns are similar in level to background <span class="hlt">ice</span> returns. Backscatter from homogeneous first year <span class="hlt">ice</span> is seen to be primarily due to surface scattering. Operation at 9.6 GHz is more sensitive to the detailed changes in scene roughness, while operation at 5.6 GHz seems to track roughness changes less ably.</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 Antarctic <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 Antarctic 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 Antarctic 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 Antarctic basins are an order of magnitude larger (100's km compared to 10's km), with presumably much less influence of confining <span class="hlt">margins</span>.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 Antarctic retreat in warm-Pliocene and future warming scenarios.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_19 --> <div id="page_20" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="381"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C51B0727H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C51B0727H"><span>Albedo and its relationship with seasonal surface roughness using repeat UAV survey across the Kangerlussuaq sector of the Greenland <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>Hubbard, A., II; Ryan, J.; Box, J. E.; Snooke, N.</p> <p>2015-12-01</p> <p>Surface albedo is a primary control on absorbed radiation and hence <span class="hlt">ice</span> surface darkening is a powerful amplifier of melt across the <span class="hlt">margin</span> of the Greenland <span class="hlt">ice</span> sheet. To investigate the relationship between <span class="hlt">ice</span> surface roughness and variations in albedo in space and time at ~dm resolution, a suite of Unmanned Aerial Vehicles (UAVs) were deployed from the <span class="hlt">margin</span> of Russell Glacier between June and August, 2014. The UAVs were equipped with digital and multispectral cameras, GoPros, fast response broadband pyranometers and temperature and humidity sensors. The primary mission was regular repeat longitudinal transects attaining data from the <span class="hlt">margin</span> to the equilibrium line 80 km into the <span class="hlt">ice</span> sheet interior and which were complimented by selected watershed and catchment surveys. The pyranometers reliably measure bare <span class="hlt">ice</span> surface albedo between 0.34 and 0.58 that correlate well against concurrent MODIS data (where available). Repeat digital photogrammetric analysis enables investigation of relationship between changing meso- and micro-scale albedo and melt processes modulated by <span class="hlt">ice</span> surface roughness that, in turn, are related to the seasonally evolving surface energy balance recorded at three AWS on the flight path.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1612477L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1612477L"><span>Ship speeds and sea <span class="hlt">ice</span> forecasts - how are they related?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Loeptien, Ulrike; Axell, Lars</p> <p>2014-05-01</p> <p>The Baltic Sea is a shallow <span class="hlt">marginal</span> sea, located in northern Europe. A seasonally occurring sea <span class="hlt">ice</span> cover has the potential to hinder the intense ship traffic substantially. There are thus considerable efforts to fore- and nowcast <span class="hlt">ice</span> conditions. Here we take a somewhat opposite approach and relate ship speeds, as observed via the Automatic Identification System (AIS) network, back to the prevailing sea <span class="hlt">ice</span> conditions. We show that these information are useful to constrain fore- and nowcasts. More specifically we find, by fitting a statistical model (mixed effect model) for a test region in the Bothnian Bay, that the forecasted <span class="hlt">ice</span> properties can explain 60-65% of the ship speed variations (based on 25 minute averages).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1990JGR....9522229N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1990JGR....9522229N"><span>Physical and biological oceanographic interaction in the spring bloom at the Bering Sea <span class="hlt">marginal</span> <span class="hlt">ice</span> edge zone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Niebauer, H. J.; Alexander, Vera; Henrichs, Susan</p> <p>1990-12-01</p> <p>At the edge of the melting sea <span class="hlt">ice</span> pack in the Bering Sea in spring, physical, biological, and chemical oceanographic processes combine to generate a short-lived, intense phytoplankton bloom that is associated with the retreating <span class="hlt">ice</span> edge. The bloom begins a week or so before the first of May triggered by insolation and by the low-salinity meltwater stratification in the presence of high nitrate concentrations (˜ > 25 μM). Meltwater (salinity) stratification delineates <span class="hlt">ice</span> edge blooms from open water blooms where temperature gradients generate the stratification. Five cross-<span class="hlt">ice</span> sections of temperature, salinity, σt, chlorophyll, and nitrate are presented as a time series from April 27 to May 5 illustrating the bloom. Evidence of two separate but concurrent blooms in the <span class="hlt">ice</span> edge zone are presented. In addition, meteorological and oceanographic conditions were observed that should have been conducive to <span class="hlt">ice</span> edge up welling. While significant <span class="hlt">ice</span> and water movement occurred, upwelling was not observed. Finally, the Bering Sea <span class="hlt">ice</span> edge spring bloom is compared with other <span class="hlt">ice</span> edge systems in both hemispheres, showing that initial Bering Sea nitrate concentrations are among the highest observed but quickly become limiting owing to the rapid build up of phytoplankton populations. This primary production is not coupled to the pelagic Zooplankton because Zooplankton are largely absent on account of the cold temperatures. Observed maximum chlorophyll concentrations in the bloom are several times greater than those observed in other systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19840066094&hterms=growth+pole&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dgrowth%2Bpole','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19840066094&hterms=growth+pole&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dgrowth%2Bpole"><span>Concentration gradients and growth/decay characteristics of the seasonal sea <span class="hlt">ice</span> cover</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.; Zwally, H. J.</p> <p>1984-01-01</p> <p>The characteristics of sea <span class="hlt">ice</span> cover in both hemispheres are analyzed and compared. The areal sea <span class="hlt">ice</span> cover in the entire polar regions and in various geographical sectors is quantified for various concentration intervals and is analyzed in a consistent manner. Radial profiles of brightness temperatures from the poles across the <span class="hlt">marginal</span> zone are also evaluated at different transects along regular longitudinal intervals during different times of the year. These radial profiles provide statistical information about the <span class="hlt">ice</span> concentration gradients and the rates at which the <span class="hlt">ice</span> edge advances or retreats during a complete annual cycle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSCT24A0145K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSCT24A0145K"><span>210Po/210Pb <span class="hlt">Activity</span> Ratios as a Possible `Dating Tool' of <span class="hlt">Ice</span> Cores and <span class="hlt">Ice</span>-rafted Sediments from the Western Arctic Ocean - Preliminary Results</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Krupp, K.; Baskaran, M. M.</p> <p>2016-02-01</p> <p>We have collected and analyzed a suite of surface snow samples, <span class="hlt">ice</span> cores, <span class="hlt">ice</span>-rafted sediments (IRS) and aerosol samples from the Western Arctic for Po-210 and Pb-210 to examine the extent of disequilibrium between this pair to possibly use 210Po/210Pb <span class="hlt">activity</span> ratio to date different layers of <span class="hlt">ice</span> cores and time of incorporation of <span class="hlt">ice</span>-rafted sediments into the sea <span class="hlt">ice</span>. We have earlier reported that the <span class="hlt">activity</span> concentrations of 210Pb in IRS vary over an order of magnitude and it is 1-2 orders of magnitude higher than that of the benthic sediments (1-2 dpm/g in benthic sediments compared to 25 to 300 dpm/g in IRS). In this study, we have measured 210Po/210Pb <span class="hlt">activity</span> ratios in aerosols from the Arctic Ocean to constrain the initial 210Po/210Pb ratio at the time of deposition during precipitation. The 210Po <span class="hlt">activity</span> concentration in recent snow is compared to surface <span class="hlt">ice</span> samples. The `age' of IRS incorporation can be calculated as follows: [210Po]measured = [210Po]initial + [210Pb] (1 - exp(-λt)) (1) where λ is the decay constant of 210Po, 138.4 days, and `t' is the in-growth time period. From this equation, `t' can be calculated as follows: t = (-1/λ) [ln (1- ((210Po/210Pb)measured - (210Po/210Pb)initial)] (2) The assumption involved in this approach are: i) there is no preferential uptake of 210Po (highly biogenic - S group); and iii) both 210Po and 210Pb remain as closed system. The calculated age using equation (2) will be discussed and presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C23A1195A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C23A1195A"><span>Contribution of the Greenland <span class="hlt">Ice</span> Sheet to Sea-Level over the Next Millennium</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aschwanden, A.; Fahnestock, M. A.; Truffer, M.</p> <p>2017-12-01</p> <p>The contribution of Greenland's outlet glaciers to sea-level remains a wild card in global sea level predictions but progress in mapping <span class="hlt">ice</span> thickness combined with high-resolution flow modeling now allow to revisit questions about the long-term stability of the <span class="hlt">ice</span> sheet. Here we present the first outlet glacier resolving assessment of Greenland's contribution to sea-level over the next millennium. We find that increased <span class="hlt">ice</span> discharge resulting from acceleration of outlet glaciers due to <span class="hlt">ice</span> melt at tidewater glacier <span class="hlt">margins</span> dominates mass loss during the 21st century. However, as the <span class="hlt">ice</span> sheet surfaces lowers, surface melt increases and over the course of the millennium, the relative contribution of <span class="hlt">ice</span> discharge to total mass loss decreases. By the end of the 22nd century, most outlet glaciers in the north-west will have retreated out of tide-water, while in south-east enhanced precipitation partially offsets high <span class="hlt">ice</span> discharge. The outlet glaciers of the central west coast, most notably Jakobshavn Isbrae, play a key role in dynamic mass loss due to their submarine connection to the interior reservoir. We find that coast-ward advection of cold <span class="hlt">ice</span> from the interior counteracts outlet glacier acceleration by increasing <span class="hlt">ice</span> viscosity and thereby reducing vertical shearing. Under the RCP 8.5 scenario, the <span class="hlt">ice</span> <span class="hlt">margin</span> in north and north-east Greenland retreats far enough to reach the vast interior where the subglacial topography is below sea level. This leads to a dramatic retreat in the second part of the millenium, and Greenland could shrink to 10% of its current volume by the end of the millennium.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70010688','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70010688"><span>Age of <span class="hlt">marginal</span> Wisconsin drift at corry, northwestern Pennsylvania</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Droste, J.B.; Rubin, M.; White, G.W.</p> <p>1959-01-01</p> <p>Marl began to accumulate about 14,000 years ago, as determined by radiocarbon dating, in a pond in a kettle hole in Kent drift at Corry, Pa., 9 miles inside the Wisconsin drift <span class="hlt">margin</span>. This radiocarbon age represents the minimum time since the disappearance of the <span class="hlt">ice</span> from Corry and confirms an assignment of Cary age to the drift.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..1511590V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..1511590V"><span>Translating hydrologically-relevant variables from the <span class="hlt">ice</span> sheet model SICOPOLIS to the Greenland Analog Project hydrologic modeling domain</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vallot, Dorothée; Applegate, Patrick; Pettersson, Rickard</p> <p>2013-04-01</p> <p>Projecting future climate and <span class="hlt">ice</span> sheet development requires sophisticated models and extensive field observations. Given the present state of our knowledge, it is very difficult to say what will happen with certainty. Despite the ongoing increase in atmospheric greenhouse gas concentrations, the possibility that a new <span class="hlt">ice</span> sheet might form over Scandinavia in the far distant future cannot be excluded. The growth of a new Scandinavian <span class="hlt">Ice</span> Sheet would have important consequences for buried nuclear waste repositories. The Greenland Analogue Project, initiated by the Swedish Nuclear Fuel and Waste Management Company (SKB), is working to assess the effects of a possible future <span class="hlt">ice</span> sheet on groundwater flow by studying a constrained domain in Western Greenland by field measurements (including deep bedrock drilling in front of the <span class="hlt">ice</span> sheet) combined with numerical modeling. To address the needs of the GAP project, we interpolated results from an ensemble of <span class="hlt">ice</span> sheet model runs to the smaller and more finely resolved modeling domain used in the GAP project's hydrologic modeling. Three runs have been chosen with three fairly different positive degree-day factors among those that reproduced the modern <span class="hlt">ice</span> <span class="hlt">margin</span> at the borehole position. The interpolated results describe changes in hydrologically-relevant variables over two time periods, 115 ka to 80 ka, and 20 ka to 1 ka. In the first of these time periods, the <span class="hlt">ice</span> <span class="hlt">margin</span> advances over the model domain; in the second time period, the <span class="hlt">ice</span> <span class="hlt">margin</span> retreats over the model domain. The spatially-and temporally dependent variables that we treated include the <span class="hlt">ice</span> thickness, basal melting rate, surface mass balance, basal temperature, basal thermal regime (frozen or thawed), surface temperature, and basal water pressure. The melt flux is also calculated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150004436','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150004436"><span>Sea-<span class="hlt">Ice</span> Freeboard Retrieval Using Digital Photon-Counting Laser Altimetry</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Farrell, Sinead L.; Brunt, Kelly M.; Ruth, Julia M.; Kuhn, John M.; Connor, Laurence N.; Walsh, Kaitlin M.</p> <p>2015-01-01</p> <p>Airborne and spaceborne altimeters provide measurements of sea-<span class="hlt">ice</span> elevation, from which sea-<span class="hlt">ice</span> freeboard and thickness may be derived. Observations of the Arctic <span class="hlt">ice</span> pack by satellite altimeters indicate a significant decline in <span class="hlt">ice</span> thickness, and volume, over the last decade. NASA's <span class="hlt">Ice</span>, Cloud and land Elevation Satellite-2 (ICESat-2) is a next-generation laser altimeter designed to continue key sea-<span class="hlt">ice</span> observations through the end of this decade. An airborne simulator for ICESat-2, the Multiple Altimeter Beam Experimental Lidar (MABEL), has been deployed to gather pre-launch data for mission development. We present an analysis of MABEL data gathered over sea <span class="hlt">ice</span> in the Greenland Sea and assess the capabilities of photon-counting techniques for sea-<span class="hlt">ice</span> freeboard retrieval. We compare freeboard estimates in the <span class="hlt">marginal</span> <span class="hlt">ice</span> zone derived from MABEL photon-counting data with coincident data collected by a conventional airborne laser altimeter. We find that freeboard estimates agree to within 0.03m in the areas where sea-<span class="hlt">ice</span> floes were interspersed with wide leads, and to within 0.07m elsewhere. MABEL data may also be used to infer sea-<span class="hlt">ice</span> thickness, and when compared with coincident but independent <span class="hlt">ice</span> thickness estimates, MABEL <span class="hlt">ice</span> thicknesses agreed to within 0.65m or better.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5911803','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5911803"><span><span class="hlt">Ice</span> Nucleation <span class="hlt">Activity</span> of Graphene and Graphene Oxides</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p></p> <p>2018-01-01</p> <p>Aerosols can act as cloud condensation nuclei and/or <span class="hlt">ice</span>-nucleating particles (INPs), influencing cloud properties. In particular, INPs show a variety of different and complex mechanisms when interacting with water during the freezing process. To gain a fundamental understanding of the heterogeneous freezing mechanisms, studies with proxies for atmospheric INPs must be performed. Graphene and its derivatives offer suitable model systems for soot particles, which are ubiquitous aerosols in the atmosphere. In this work, we present an investigation of the <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> (INA) of different types of graphene and graphene oxides. Immersion droplet freezing experiments as well as additional analytical analyses, such as X-ray photoelectron spectroscopy, Raman spectroscopy, and transmission electron microscopy, were performed. We show within a group of samples that a highly ordered graphene lattice (Raman G band intensity >50%) can support <span class="hlt">ice</span> nucleation more effectively than a lowly ordered graphene lattice (Raman G band intensity <20%). Ammonia-functionalized graphene revealed the highest INA of all samples. Atmospheric ammonia is known to play a primary role in the formation of secondary particulate matter, forming ammonium-containing aerosols. The influence of functionalization on interactions between the particle interface and water molecules, as well as on hydrophobicity and agglomeration processes, is discussed. PMID:29707097</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70121037','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70121037"><span>Glacial landforms on German Bank, Scotian Shelf: evidence for Late Wisconsinan <span class="hlt">ice</span>-sheet dynamics and implications for the formation of De Geer moraines</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Todd, Brian J.; Valentine, Page C.; Longva, Oddvar; Shaw, John</p> <p>2007-01-01</p> <p>The extent and behaviour of the southeast <span class="hlt">margin</span> of the Laurentide <span class="hlt">Ice</span> Sheet in Atlantic Canada is of significance in the study of Late Wisconsinan <span class="hlt">ice</span> sheet-ocean interactions. Multibeam sonar imagery of subglacial, <span class="hlt">ice-marginal</span> and glaciomarine landforms on German Bank, Scotian Shelf, provides evidence of the pattern of glacial-dynamic events in the eastern Gulf of Maine. Northwest-southeast trending drumlins and megaflutes dominate northern German Bank. On southern German Bank, megaflutes of thin glacial deposits create a distinct northwest-southeast grain. Lobate regional moraines (>10km long) are concave to the northwest, up-<span class="hlt">ice</span> direction and strike southwest-northeast, normal to the direction of <span class="hlt">ice</span> flow. Ubiquitous, overlying De Geer moraines (</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA602483','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA602483"><span>An Integrative Wave Model for the <span class="hlt">Marginal</span> <span class="hlt">Ice</span> Zone based on a Rheological Parameterization</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>climate in the present and future Arctic seas. OBJECTIVES 1. To build a comprehensive wave-<span class="hlt">ice</span> interaction mathematical framework for a wide...group (e.g. Fox and Squire, 1994, Meylan and Squire, 1996, Bennetts and Squire, 2009) is also applicable to the case of <span class="hlt">ice</span> floes imbedded in a frazil...environmental protection purposes: such as navigation route planning, offshore structure design in the Arctic , and coastal erosion prevention. They</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4233703','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4233703"><span><span class="hlt">Ice</span>-binding proteins that accumulate on different <span class="hlt">ice</span> crystal planes produce distinct thermal hysteresis dynamics</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Drori, Ran; Celik, Yeliz; Davies, Peter L.; Braslavsky, Ido</p> <p>2014-01-01</p> <p><span class="hlt">Ice</span>-binding proteins that aid the survival of freeze-avoiding, cold-adapted organisms by inhibiting the growth of endogenous <span class="hlt">ice</span> crystals are called antifreeze proteins (AFPs). The binding of AFPs to <span class="hlt">ice</span> causes a separation between the melting point and the freezing point of the <span class="hlt">ice</span> crystal (thermal hysteresis, TH). TH produced by hyperactive AFPs is an order of magnitude higher than that produced by a typical fish AFP. The basis for this difference in <span class="hlt">activity</span> remains unclear. Here, we have compared the time dependence of TH <span class="hlt">activity</span> for both hyperactive and moderately <span class="hlt">active</span> AFPs using a custom-made nanolitre osmometer and a novel microfluidics system. We found that the TH <span class="hlt">activities</span> of hyperactive AFPs were time-dependent, and that the TH <span class="hlt">activity</span> of a moderate AFP was almost insensitive to time. Fluorescence microscopy measurement revealed that despite their higher TH <span class="hlt">activity</span>, hyperactive AFPs from two insects (moth and beetle) took far longer to accumulate on the <span class="hlt">ice</span> surface than did a moderately <span class="hlt">active</span> fish AFP. An <span class="hlt">ice</span>-binding protein from a bacterium that functions as an <span class="hlt">ice</span> adhesin rather than as an antifreeze had intermediate TH properties. Nevertheless, the accumulation of this <span class="hlt">ice</span> adhesion protein and the two hyperactive AFPs on the basal plane of <span class="hlt">ice</span> is distinct and extensive, but not detectable for moderately <span class="hlt">active</span> AFPs. Basal <span class="hlt">ice</span> plane binding is the distinguishing feature of antifreeze hyperactivity, which is not strictly needed in fish that require only approximately 1°C of TH. Here, we found a correlation between the accumulation kinetics of the hyperactive AFP at the basal plane and the time sensitivity of the measured TH. PMID:25008081</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21235213','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21235213"><span>Homogeneous <span class="hlt">ice</span> nucleation from aqueous inorganic/organic particles representative of biomass burning: water <span class="hlt">activity</span>, freezing temperatures, nucleation rates.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Knopf, Daniel A; Rigg, Yannick J</p> <p>2011-02-10</p> <p>Homogeneous <span class="hlt">ice</span> nucleation plays an important role in the formation of cirrus clouds with subsequent effects on the global radiative budget. Here we report on homogeneous <span class="hlt">ice</span> nucleation temperatures and corresponding nucleation rate coefficients of aqueous droplets serving as surrogates of biomass burning aerosol. Micrometer-sized (NH(4))(2)SO(4)/levoglucosan droplets with mass ratios of 10:1, 1:1, 1:5, and 1:10 and aqueous multicomponent organic droplets with and without (NH(4))(2)SO(4) under typical tropospheric temperatures and relative humidities are investigated experimentally using a droplet conditioning and <span class="hlt">ice</span> nucleation apparatus coupled to an optical microscope with image analysis. Homogeneous freezing was determined as a function of temperature and water <span class="hlt">activity</span>, a(w), which was set at droplet preparation conditions. The <span class="hlt">ice</span> nucleation data indicate that minor addition of (NH(4))(2)SO(4) to the aqueous organic droplets renders the temperature dependency of water <span class="hlt">activity</span> negligible in contrast to the case of aqueous organic solution droplets. The mean homogeneous <span class="hlt">ice</span> nucleation rate coefficient derived from 8 different aqueous droplet compositions with average diameters of ∼60 μm for temperatures as low as 195 K and a(w) of 0.82-1 is 2.18 × 10(6) cm(-3) s(-1). The experimentally derived freezing temperatures and homogeneous <span class="hlt">ice</span> nucleation rate coefficients are in agreement with predictions of the water <span class="hlt">activity</span>-based homogeneous <span class="hlt">ice</span> nucleation theory when taking predictive uncertainties into account. However, the presented <span class="hlt">ice</span> nucleation data indicate that the water <span class="hlt">activity</span>-based homogeneous <span class="hlt">ice</span> nucleation theory overpredicts the freezing temperatures by up to 3 K and corresponding <span class="hlt">ice</span> nucleation rate coefficients by up to ∼2 orders of magnitude. A shift of 0.01 in a(w), which is well within the uncertainty of typical field and laboratory relative humidity measurements, brings experimental and predicted freezing temperatures and homogeneous <span class="hlt">ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Geomo.306..235D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Geomo.306..235D"><span>Irish <span class="hlt">Ice</span> Sheet dynamics during deglaciation of the central Irish Midlands: Evidence of <span class="hlt">ice</span> streaming and surging from airborne LiDAR</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Delaney, Catherine A.; McCarron, Stephen; Davis, Stephen</p> <p>2018-04-01</p> <p>High resolution digital terrain models (DTMs) generated from airborne LiDAR data and supplemented by field evidence are used to map glacial landform assemblages dating from the last glaciation (Midlandian glaciation; OI stages 2-3) in the central Irish Midlands. The DTMs reveal previously unrecognised low-amplitude landforms, including crevasse-squeeze ridges and mega-scale glacial lineations overprinted by conduit fills leading to <span class="hlt">ice-marginal</span> subaqueous deposits. We interpret this landform assemblage as evidence for surging behaviour during <span class="hlt">ice</span> recession. The data indicate that two separate phases of accelerated <span class="hlt">ice</span> flow were followed by <span class="hlt">ice</span> sheet stagnation during overall deglaciation. The second surge event was followed by a subglacial outburst flood, forming an intricate esker and crevasse-fill network. The data provide the first clear evidence that <span class="hlt">ice</span> flow direction was eastward along the eastern watershed of the Shannon River basin, at odds with previous models, and raise the possibility that an <span class="hlt">ice</span> stream existed in this area. Our work demonstrates the potential for airborne LiDAR surveys to produce detailed paleoglaciological reconstructions and to enhance our understanding of complex palaeo-<span class="hlt">ice</span> sheet dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140013018','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140013018"><span>Analysis of the Effect of Water <span class="hlt">Activity</span> on <span class="hlt">Ice</span> Formation Using a New Theory of Nucleation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Barahona, Donifan</p> <p>2013-01-01</p> <p>In this work a new theory of nucleation is developed and used to investigate the effect of water <span class="hlt">activity</span> on the formation of <span class="hlt">ice</span> within super-cooled droplets. The new theory is based on a novel concept where the interface is assumed to be made of liquid molecules trapped by the solid matrix. Using this concept new expressions are developed for the critical <span class="hlt">ice</span> germ size and the nucleation work, with explicit dependencies on temperature and water <span class="hlt">activity</span>. However unlike previous approaches, the new theory does not depend on the interfacial tension between liquid and <span class="hlt">ice</span>. Comparison against experimental results shows that the new theory is able to reproduce the observed effect of water <span class="hlt">activity</span> on nucleation rate and freezing temperature. It allows for the first time a theoretical derivation of the constant shift in water <span class="hlt">activity</span> between melting and nucleation. The new theory offers a consistent thermodynamic view of <span class="hlt">ice</span> nucleation, simple enough to be applied in atmospheric models of cloud formation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19492339','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19492339"><span><span class="hlt">Ice</span> nucleation temperature influences recovery of <span class="hlt">activity</span> of a model protein after freeze drying.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cochran, Teresa; Nail, Steven L</p> <p>2009-09-01</p> <p>The objective of this study was to determine whether a relationship exists between <span class="hlt">ice</span> nucleation temperature and recovery of <span class="hlt">activity</span> of a model protein, lactate dehydrogenase, after freeze drying. Aqueous buffer systems containing 50 microg/mL of protein were frozen in vials with externally mounted thermocouples on the shelf of a freeze dryer, then freeze dried. Various methods were used to establish a wide range of <span class="hlt">ice</span> nucleation temperatures. An inverse relationship was found between the extent of supercooling during freezing and recovery of <span class="hlt">activity</span> in the reconstituted solution. The data are consistent with a mechanism of inactivation resulting from adsorption of protein at the <span class="hlt">ice</span>/freeze-concentrate interface during the freezing process.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMIN31D..08C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMIN31D..08C"><span>Operational Use of Near Real Time Remote sensing Data at the U.S. National <span class="hlt">Ice</span> Center (NIC)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clemente-Colon, P.</p> <p>2012-12-01</p> <p>The National <span class="hlt">Ice</span> Center (NIC) is a U.S. Government agency that brings together the Department of Defense - Navy, Department of Commerce - National Oceanic and Atmospheric Administration (NOAA), and the Department of Homeland Security - U.S. Coast Guard (USCG) to support coastal and marine sea <span class="hlt">ice</span> operations and research in the Polar Regions. The NIC provides specialized strategic and tactical <span class="hlt">ice</span> analyses to meet the operational needs of the U.S. government and is the only operational <span class="hlt">ice</span> service in the world that monitors sea <span class="hlt">ice</span> in both the Arctic, Antarctic regions as well as in other <span class="hlt">ice</span> infested waters. NIC utilizes multiple sources of near real time satellite and in-situ observations as well as NWP and ocean-sea <span class="hlt">ice</span> model output to produce sea <span class="hlt">ice</span> analyses. Key users of NIC products in the Arctic include the Navy submarine force, National Weather Service, USCG and Canadian Coast Guard icebreakers, Military Sealift Command on re-supply missions to Antarctica and Greenland, and NOAA research vessels operating near sea <span class="hlt">ice</span> cover in both hemispheres as well. Time series of NIC weekly or bi-weekly <span class="hlt">ice</span> analysis charts, daily <span class="hlt">marginal</span> <span class="hlt">ice</span> zone and <span class="hlt">ice</span> edge routine products, as well as tactical support annotated imagery are generated by expert analysts with wide access to near real time satellite imagery from VIS/IR to passive and <span class="hlt">active</span> microwave sensors. The status of these satellite data streams and the expected availability of new capabilities in the near future will be discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015GGG....16.1421C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015GGG....16.1421C"><span>Abbot <span class="hlt">Ice</span> Shelf, structure of the Amundsen Sea continental <span class="hlt">margin</span> and the southern boundary of the Bellingshausen Plate seaward of West Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cochran, James R.; Tinto, Kirsty J.; Bell, Robin E.</p> <p>2015-05-01</p> <p>Inversion of NASA Operation <span class="hlt">Ice</span>Bridge airborne gravity over the Abbot <span class="hlt">Ice</span> Shelf in West Antarctica for subice bathymetry defines an extensional terrain made up of east-west trending rift basins formed during the early stages of Antarctica/Zealandia rifting. Extension is minor, as rifting jumped north of Thurston Island early in the rifting process. The Amundsen Sea Embayment continental shelf west of the rifted terrain is underlain by a deeper, more extensive sedimentary basin also formed during rifting between Antarctica and Zealandia. A well-defined boundary zone separates the mildly extended Abbot extensional terrain from the deeper Amundsen Embayment shelf basin. The shelf basin has an extension factor, β, of 1.5-1.7 with 80-100 km of extension occurring across an area now 250 km wide. Following this extension, rifting centered north of the present shelf edge and proceeded to continental rupture. Since then, the Amundsen Embayment continental shelf appears to have been tectonically quiescent and shaped by subsidence, sedimentation, and the advance and retreat of the West Antarctic <span class="hlt">Ice</span> Sheet. The Bellingshausen Plate was located seaward of the Amundsen Sea <span class="hlt">margin</span> prior to incorporation into the Antarctic Plate at about 62 Ma. During the latter part of its independent existence, Bellingshausen plate motion had a clockwise rotational component relative to Antarctica producing convergence across the north-south trending Bellingshausen Gravity Anomaly structure at 94°W and compressive deformation on the continental slope between 94°W and 102°W. Farther west, the relative motion was extensional along an east-west trending zone occupied by the Marie Byrd Seamounts. The copyright line for this article was changed on 5 JUN 2015 after original online publication.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70022547','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70022547"><span>Classification methods for monitoring Arctic sea <span class="hlt">ice</span> using OKEAN passive/<span class="hlt">active</span> two-channel microwave data</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Belchansky, Gennady I.; Douglas, David C.</p> <p>2000-01-01</p> <p>This paper presents methods for classifying Arctic sea <span class="hlt">ice</span> using both passive and <span class="hlt">active</span> (2-channel) microwave imagery acquired by the Russian OKEAN 01 polar-orbiting satellite series. Methods and results are compared to sea <span class="hlt">ice</span> classifications derived from nearly coincident Special Sensor Microwave Imager (SSM/I) and Advanced Very High Resolution Radiometer (AVHRR) image data of the Barents, Kara, and Laptev Seas. The Russian OKEAN 01 satellite data were collected over weekly intervals during October 1995 through December 1997. Methods are presented for calibrating, georeferencing and classifying the raw <span class="hlt">active</span> radar and passive microwave OKEAN 01 data, and for correcting the OKEAN 01 microwave radiometer calibration wedge based on concurrent 37 GHz horizontal polarization SSM/I brightness temperature data. Sea <span class="hlt">ice</span> type and <span class="hlt">ice</span> concentration algorithms utilized OKEAN's two-channel radar and passive microwave data in a linear mixture model based on the measured values of brightness temperature and radar backscatter, together with a priori knowledge about the scattering parameters and natural emissivities of basic sea <span class="hlt">ice</span> types. OKEAN 01 data and algorithms tended to classify lower concentrations of young or first-year sea <span class="hlt">ice</span> when concentrations were less than 60%, and to produce higher concentrations of multi-year sea <span class="hlt">ice</span> when concentrations were greater than 40%, when compared to estimates produced from SSM/I data. Overall, total sea <span class="hlt">ice</span> concentration maps derived independently from OKEAN 01, SSM/I, and AVHRR satellite imagery were all highly correlated, with uniform biases, and mean differences in total <span class="hlt">ice</span> concentration of less than four percent (sd<15%).</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_20 --> <div id="page_21" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="401"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2013-01-03/pdf/2012-31570.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2013-01-03/pdf/2012-31570.pdf"><span>78 FR 332 - Self-Regulatory Organizations; <span class="hlt">ICE</span> Clear Europe Limited; Notice of Filing and Immediate...</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2013-01-03</p> <p>..., the SPAN Arrays published by <span class="hlt">ICE</span> Clear Europe include the Volatility Risk Credit Rate (the Offset Rate... Rule Change Related to SPAN <span class="hlt">Margin</span> Methodology Enhancements to Inter-Contract Credits and Average..., the Proposed Rule Change In addition to providing clearing services for credit default swaps, <span class="hlt">ICE</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70034535','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70034535"><span>Provenance of Des Moines lobe till records <span class="hlt">ice</span>-stream catchment evolution during Laurentide deglaciation</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Lusardi, B.A.; Jennings, C.E.; Harris, K.L.</p> <p>2011-01-01</p> <p>Mapping and analysis of deposits of the Des Moines lobe of the Laurentide <span class="hlt">Ice</span> Sheet, <span class="hlt">active</span> after the Last Glacial Maximum (LGM), reveal several texturally and lithologically distinct tills within what had been considered to be a homogeneous deposit. Although the differences between tills are subtle, minor distinctions are predictable and mappable, and till sheets within the area covered by the lobe can be correlated for hundreds of kilometres parallel to <span class="hlt">ice</span> flow. Lateral till-sheet contacts are abrupt or overlap in a narrow zone, coincident with a geomorphic discontinuity interpreted to be a shear <span class="hlt">margin</span>. Till sheets 10 to 20m thick show mixing in their lower 2 to 3m. We suggest that: (i) lithologically distinct till sheets correspond to unique <span class="hlt">ice</span>-stream source areas; (ii) the sequence of tills deposited by the Des Moines lobe was the result of the evolution and varying dominance of nearby and competing <span class="hlt">ice</span> streams and their tributaries; and (iii) in at least one instance, more than one <span class="hlt">ice</span> stream simultaneously contributed to the lobe. Therefore the complex sequence of tills of subtly different provenances, and the unconformities between them record the evolution of an <span class="hlt">ice</span>-catchment area during Laurentide <span class="hlt">Ice</span> Sheet drawdown. Till provenance data suggest that, after till is created in the <span class="hlt">ice</span>-stream source area, the subglacial conditions required for transporting till decline and incorporation of new material is limited. ?? 2011 The Authors. Boreas ?? 2011 The Boreas Collegium.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008APS..MARH25003B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008APS..MARH25003B"><span>Why are hyperactive <span class="hlt">ice</span>-binding-proteins so <span class="hlt">active</span>?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Braslavsky, Ido; Celik, Yeliz; Pertaya, Natalya; Eun Choi, Young; Bar, Maya; Davies, Peter L.</p> <p>2008-03-01</p> <p><span class="hlt">Ice</span> binding proteins (IBPs), also called `antifreeze proteins' or `<span class="hlt">ice</span> structuring proteins', are a class of proteins that protect organisms from freezing injury. These proteins have many applications in medicine and agriculture, and as a platform for future biotechnology applications. One of the interesting questions in this field focuses on the hyperactivity of some IBPs. <span class="hlt">Ice</span> binding proteins can be classified in two groups: moderate ones that can depress the freezing point up to ˜1.0 ^oC and hyperactive ones that can depress the freezing point several-fold further even at lower concentrations. It has been suggested that the hyperactivity of IBPs stem from the fact that they block growth out of specific <span class="hlt">ice</span> surfaces, more specifically the basal planes of <span class="hlt">ice</span>. Here we show experimental results based on fluorescence microscopy, highlighting the differences between moderate IBPs and hyperactive IBPs. These include direct evidence for basal plane affinity of hyperactive IBPs, the effects of IBPs on growth-melt behavior of <span class="hlt">ice</span> and the dynamics of their interaction with <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C23A1194T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C23A1194T"><span>The Sensitivity of the Greenland <span class="hlt">Ice</span> Sheet to Glacial-Interglacial Oceanic Forcing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tabone, I.; Blasco Navarro, J.; Robinson, A.; Alvarez-Solas, J.; Montoya, M.</p> <p>2017-12-01</p> <p>Up to now, the scientific community has mainly focused on the sensitivity of the Greenland <span class="hlt">Ice</span> Sheet (GrIS) to atmospheric variations. However, several studies suggest that the enhanced <span class="hlt">ice</span> mass loss experienced by the GrIS in the past decades is directly connected to the increasing North Atlantic temperatures. Melting of GrIS outlet glaciers triggers grounding-line retreat increasing <span class="hlt">ice</span> discharge into the ocean. This new evidence leads to consider the ocean as a relevant driver to be taken into account when modeling the evolution of the GrIS. The <span class="hlt">ice</span>-ocean interaction is a primary factor controling not only the likely future retreat of GrIS outlet glaciers, or the huge <span class="hlt">ice</span> loss in past warming climates, but also, and more strongly, the past GrIS glacial expansion. The latter assumption is supported by reconstructions which propose the GrIS to be fully marine-based during glacials, and thus more exposed to the influence of the ocean. Here, for the first time, we investigate the response of the GrIS to past oceanic changes using a three-dimensional hybrid <span class="hlt">ice-sheet/ice</span>-shelf model, which combines the Shallow <span class="hlt">Ice</span> Approximation (SIA) for slow grounded <span class="hlt">ice</span> sheets and the Shallow Shelf Approximation (SSA) in <span class="hlt">ice</span> shelves and <span class="hlt">ice</span> streams. The model accounts for a time-dependent parametrisation of the marine basal melting rate, which is used to reproduce past oceanic variations. In this work simulations of the last two glacial cycles are performed. Our results show that the GrIS is very sensitive to the ocean-triggered submarine melting (freezing). Mild oceanic temperature variations lead to a rapid retreat (expansion) of the GrIS <span class="hlt">margins</span>, which, inducing a dynamic adjustment of the grounded <span class="hlt">ice</span> sheet, drive the evolution of the whole <span class="hlt">ice</span> sheet. Our results strongly suggest the need to consider the ocean as an <span class="hlt">active</span> forcing in paleo <span class="hlt">ice</span> sheet models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2007/1047/srp/srp106/of2007-1047srp106.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2007/1047/srp/srp106/of2007-1047srp106.pdf"><span>Records of past <span class="hlt">ice</span> sheet fluctuations in interior East 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>Liu, Xiaohan; Huang, Feixin; Kong, Ping; Fang, Aimin; Li, Xiaoli</p> <p>2007-01-01</p> <p>The results of a land-based multi-disciplinary study of the past <span class="hlt">ice</span> surface elevation in the Grove Mountains of interior East Antarctica support a dynamic evolution of the East Antarctic <span class="hlt">Ice</span> Sheet (EAIS). Moraine boulders of sedimentary rocks and spore pollen assemblage imply a significant shrinkage of the EAIS, with its <span class="hlt">margin</span> retreating south of the Grove Mountains (~450 km south of recent coast line) before the middle Pliocene. The exposure ages indicate that the <span class="hlt">ice</span> sheet subsequently re-advanced, with the <span class="hlt">ice</span> surface rising locally at least 450 m higher than today. It then went back down constantly from before 2.3 Ma to 1.6 Ma. The glacial topography and existence of soil show that the <span class="hlt">ice</span> surface fluctuation continued since the early Quaternary, but with highest levels never exceeding ~100 m higher than today.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C21B0673W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C21B0673W"><span>Damage Mechanics in the Community <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>Whitcomb, R.; Cathles, L. M. M., IV; Bassis, J. N.; Lipscomb, W. H.; Price, S. F.</p> <p>2016-12-01</p> <p>Half of the mass that floating <span class="hlt">ice</span> shelves lose to the ocean comes from iceberg calving, which is a difficult process to simulate accurately. This is especially true in the large-scale <span class="hlt">ice</span> dynamics models that couple changes in the cryosphere to climate projections. Damage mechanics provide a powerful technique with the potential to overcome this obstacle by describing how fractures in <span class="hlt">ice</span> evolve over time. Here, we demonstrate the application of a damage model to <span class="hlt">ice</span> shelves that predicts realistic geometries. We incorporated this solver into the Community <span class="hlt">Ice</span> Sheet Model, a three dimensional <span class="hlt">ice</span> sheet model developed at Los Alamos National Laboratory. The damage mechanics formulation that we use comes from a first principles-based evolution law for the depth of basal and surface crevasses and depends on the large scale strain rate, stress state, and basal melt. We show that under idealized conditions it produces <span class="hlt">ice</span> tongue lengths that match well with observations for a selection of natural <span class="hlt">ice</span> tongues, including Erebus, Drygalski, and Pine Island in Antarctica, as well as Petermann in Greenland. We also apply the model to more generalized ideal <span class="hlt">ice</span> shelf geometries and show that it produces realistic calving front positions. Although our results are preliminary, the damage mechanics model that we developed provides a promising first principles method for predicting <span class="hlt">ice</span> shelf extent and how the calving <span class="hlt">margins</span> of <span class="hlt">ice</span> shelves respond to climate change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19890024803&hterms=Phytoplankton&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3DPhytoplankton','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19890024803&hterms=Phytoplankton&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3DPhytoplankton"><span>Phytoplankton standing crops within an Antarctic <span class="hlt">ice</span> edge assessed by satellite remote sensing</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sullivan, C. W.; Mcclain, C. R.; Comiso, J. C.; Smith, W. O., Jr.</p> <p>1988-01-01</p> <p>The dynamic interactions between the pack-<span class="hlt">ice</span> recession and the occurrence of <span class="hlt">ice</span> blooms of phytoplankton in waters of the <span class="hlt">marginal</span> <span class="hlt">ice</span> zone within an Antarctic <span class="hlt">ice</span> edge were investigated using CZCS and SMMR imageries from the Nimbus 7 satellite (September 16-December 17, 1983), together with in situ measurements of pigments and sea <span class="hlt">ice</span> concentration carried out from November 7 to December 2. A substantial amount of spatial variability in pigment concentration was observed to occur along the <span class="hlt">ice</span> edge in the Weddell Sea. The relationships among light, <span class="hlt">ice</span> distribution, and vertical stability and their effects on observed spatial variations in phytoplankton biomass are discussed. The results of this investigation suggest that the retreat of <span class="hlt">ice</span> provides an input of significant volumes of meltwater which creates vertical stability for a period necessary to permit growth and accumulation of phytoplankton.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5293020','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5293020"><span>Observing the formation of <span class="hlt">ice</span> and organic crystals in <span class="hlt">active</span> sites</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Campbell, James M.; Meldrum, Fiona C.; Christenson, Hugo K.</p> <p>2017-01-01</p> <p>Heterogeneous nucleation is vital to a wide range of areas as diverse as <span class="hlt">ice</span> nucleation on atmospheric aerosols and the fabrication of high-performance thin films. There is excellent evidence that surface topography is a key factor in directing crystallization in real systems; however, the mechanisms by which nanoscale pits and pores promote nucleation remain unclear. Here, we use natural cleavage defects on Muscovite mica to investigate the <span class="hlt">activity</span> of topographical features in the nucleation from vapor of <span class="hlt">ice</span> and various organic crystals. Direct observation of crystallization within surface pockets using optical microscopy and also interferometry demonstrates that these sharply acute features provide extremely effective nucleation sites and allows us to determine the mechanism by which this occurs. A confined phase is first seen to form along the apex of the wedge and then grows out of the pocket opening to generate a bulk crystal after a threshold saturation has been achieved. <span class="hlt">Ice</span> nucleation proceeds in a comparable manner, although our resolution is insufficient to directly observe a condensate before the growth of a bulk crystal. These results provide insight into the mechanism of crystal deposition from vapor on real surfaces, where this will ultimately enable us to use topography to control crystal deposition on surfaces. They are also particularly relevant to our understanding of processes such as cirrus cloud formation, where such topographical features are likely candidates for the “<span class="hlt">active</span> sites” that make clay particles effective nucleants for <span class="hlt">ice</span> in the atmosphere. PMID:27994140</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004AGUSM.C42A..02D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUSM.C42A..02D"><span>Operationally Monitoring Sea <span class="hlt">Ice</span> at the Canadian <span class="hlt">Ice</span> Service</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>de Abreu, R.; Flett, D.; Carrieres, T.; Falkingham, J.</p> <p>2004-05-01</p> <p>The Canadian <span class="hlt">Ice</span> Service (CIS) of the Meteorological Service of Canada promotes safe and efficient maritime operations and protects Canada's environment by providing reliable and timely information about <span class="hlt">ice</span> and iceberg conditions in Canadian waters. Daily and seasonal charts describing the extent, type and concentration of sea <span class="hlt">ice</span> and icebergs are provided to support navigation and other <span class="hlt">activities</span> (e.g. oil and gas) in coastal waters. The CIS relies on a suite of spaceborne visible, infrared and microwave sensors to operationally monitor <span class="hlt">ice</span> conditions in Canadian coastal and inland waterways. These efforts are complemented by operational sea <span class="hlt">ice</span> models that are customized and run at the CIS. The archive of these data represent a 35 year archive of <span class="hlt">ice</span> conditions and have proven to be a valuable dataset for historical sea <span class="hlt">ice</span> analysis. This presentation will describe the daily integration of remote sensing observations and modelled <span class="hlt">ice</span> conditions used to produce <span class="hlt">ice</span> and iceberg products. A review of the decadal evolution of this process will be presented, as well as a glimpse into the future of <span class="hlt">ice</span> and iceberg monitoring. Examples of the utility of the CIS digital sea <span class="hlt">ice</span> archive for climate studies will also be presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18044830','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18044830"><span>Inhibition of <span class="hlt">ice</span> crystal growth in <span class="hlt">ice</span> cream mix by gelatin hydrolysate.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Damodaran, Srinivasan</p> <p>2007-12-26</p> <p>The inhibition of <span class="hlt">ice</span> crystal growth in <span class="hlt">ice</span> cream mix by gelatin hydrolysate produced by papain action was studied. The <span class="hlt">ice</span> crystal growth was monitored by thermal cycling between -14 and -12 degrees C at a rate of one cycle per 3 min. It is shown that the hydrolysate fraction containing peptides in the molecular weight range of about 2000-5000 Da exhibited the highest inhibitory <span class="hlt">activity</span> on <span class="hlt">ice</span> crystal growth in <span class="hlt">ice</span> cream mix, whereas fractions containing peptides greater than 7000 Da did not inhibit <span class="hlt">ice</span> crystal growth. The size distribution of gelatin peptides formed in the hydrolysate was influenced by the pH of hydrolysis. The optimum hydrolysis conditions for producing peptides with maximum <span class="hlt">ice</span> crystal growth inhibitory <span class="hlt">activity</span> was pH 7 at 37 degrees C for 10 min at a papain to gelatin ratio of 1:100. However, this may depend on the type and source of gelatin. The possible mechanism of <span class="hlt">ice</span> crystal growth inhibition by peptides from gelatin is discussed. Molecular modeling of model gelatin peptides revealed that they form an oxygen triad plane at the C-terminus with oxygen-oxygen distances similar to those found in <span class="hlt">ice</span> nuclei. Binding of this oxygen triad plane to the prism face of <span class="hlt">ice</span> nuclei via hydrogen bonding appears to be the mechanism by which gelatin hydrolysate might be inhibiting <span class="hlt">ice</span> crystal growth in <span class="hlt">ice</span> cream mix.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP31C1292S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP31C1292S"><span>Late Holocene spatio-temporal variability of the south Greenland <span class="hlt">Ice</span> Sheet and adjacent mountain glaciers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sinclair, G.; Carlson, A. E.; Rood, D. H.; Axford, Y.</p> <p>2017-12-01</p> <p>The late Holocene, with its spatially complex pattern of centennial-scale climate variation, is an ideal time period to test the response of the cryosphere to atmospheric and oceanic temperature changes. The south Greenland <span class="hlt">Ice</span> Sheet (sGrIS), with its proximity to areas of North Atlantic Deep Water formation and a large spectrum of glaciological regimes over a relatively small area, provides an excellent location to examine the spatial heterogeneity of <span class="hlt">ice</span>-sheet and glacier responses to climate change. Here, we will present 50 Be-10 surface exposure ages from eight moraines in six locations around the <span class="hlt">margin</span> of the sGrIS. These moraines are located just outboard of historical moraines, and will therefore allow us to constrain the timing of the most extensive prehistoric late-Holocene advance and retreat of <span class="hlt">ice</span> <span class="hlt">margins</span> draining the sGrIS and independent valley glaciers. The dataset includes both marine- and land-terminating glaciers draining the sGrIS, the low-altitude Qassimiut lobe, the high-altitude alpine Julianhåb <span class="hlt">ice</span> cap and isolated valley glaciers. This diverse dataset will allow us to determine to what extent late-Holocene centennial-scale behavior of the <span class="hlt">ice</span>-sheet and glacier <span class="hlt">margins</span> were synchronous, perhaps in response to an external climate forcing, or more stochastic, governed instead by local factors such as basal thermal regime, bedrock topography, or microclimates. This has implications for understanding the forcings and responses of cryospheric changes at timescales relevant to human society. In addition to providing context for paleoclimatic and glacial geologic investigations, this work will inform future sea-level projections by providing targets for validating high-resolution <span class="hlt">ice</span>-sheet and glacier models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27348980','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27348980"><span>Microbial Contamination of <span class="hlt">Ice</span> Machines Is Mediated by <span class="hlt">Activated</span> Charcoal Filtration Systems in a City Hospital.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yorioka, Katsuhiro; Oie, Shigeharu; Hayashi, Koji; Kimoto, Hiroo; Furukawa, Hiroyuki</p> <p>2016-06-01</p> <p>Although microbial contamination of <span class="hlt">ice</span> machines has been reported, no previous study has addressed microbial contamination of <span class="hlt">ice</span> produced by machines equipped with <span class="hlt">activated</span> charcoal (AC) filters in hospitals. The aim of this study was to provide clinical data for evaluating AC filters to prevent microbial contamination of <span class="hlt">ice</span>. We compared microbial contamination in <span class="hlt">ice</span> samples produced by machines with (n = 20) and without an AC filter (n = 40) in Shunan City Shinnanyo Municipal Hospital. All samples from the <span class="hlt">ice</span> machine equipped with an AC filter contained 10-116 CFUs/g of glucose nonfermenting gram-negative bacteria such as Pseudomonas aeruginosa and Chryseobacterium meningosepticum. No microorganisms were detected in samples from <span class="hlt">ice</span> machines without AC filters. After the AC filter was removed from the <span class="hlt">ice</span> machine that tested positive for Gram-negative bacteria, the <span class="hlt">ice</span> was resampled (n = 20). Analysis found no contaminants. <span class="hlt">Ice</span> machines equipped with AC filters pose a serious risk factor for <span class="hlt">ice</span> contamination. New filter-use guidelines and regulations on bacterial detection limits to prevent contamination of <span class="hlt">ice</span> in healthcare facilities are necessary.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19860050945&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=19860050945&hterms=microwaves+water+structure&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dmicrowaves%2Bwater%2Bstructure"><span>Aircraft and satellite passive microwave observations of the Bering Sea <span class="hlt">ice</span> cover during MIZEX West</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.; Gloersen, P.; Wilheit, T. T., Jr.</p> <p>1986-01-01</p> <p>Passive microwave measurements of the Bering Sea were made with the NASA CV-990 airborne laboratory during February. Microwave data were obtained with imaging and dual-polarized, fixed-beam radiometers in a range of frequencies from 10 to 183 GHz. The high resolution imagery at 92 GHz provides a particularly good description of the <span class="hlt">marginal</span> <span class="hlt">ice</span> zone delineating regions of open water, <span class="hlt">ice</span> compactness, and <span class="hlt">ice</span>-edge structure. Analysis of the fixed-beam data shows that spectral differences increase with a decrease in <span class="hlt">ice</span> thickness. Polarization at 18 and 37 GHz distinguishes among new, young, and first-year <span class="hlt">ice</span> types.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GMD....10.3105P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GMD....10.3105P"><span>Sea-<span class="hlt">ice</span> evaluation of NEMO-Nordic 1.0: a NEMO-LIM3.6-based ocean-sea-<span class="hlt">ice</span> model setup for the North Sea and Baltic Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pemberton, Per; Löptien, Ulrike; Hordoir, Robinson; Höglund, Anders; Schimanke, Semjon; Axell, Lars; Haapala, Jari</p> <p>2017-08-01</p> <p>The Baltic Sea is a seasonally <span class="hlt">ice</span>-covered <span class="hlt">marginal</span> sea in northern Europe with intense wintertime ship traffic and a sensitive ecosystem. Understanding and modeling the evolution of the sea-<span class="hlt">ice</span> pack is important for climate effect studies and forecasting purposes. Here we present and evaluate the sea-<span class="hlt">ice</span> component of a new NEMO-LIM3.6-based ocean-sea-<span class="hlt">ice</span> setup for the North Sea and Baltic Sea region (NEMO-Nordic). The setup includes a new depth-based fast-<span class="hlt">ice</span> parametrization for the Baltic Sea. The evaluation focuses on long-term statistics, from a 45-year long hindcast, although short-term daily performance is also briefly evaluated. We show that NEMO-Nordic is well suited for simulating the mean sea-<span class="hlt">ice</span> extent, concentration, and thickness as compared to the best available observational data set. The variability of the annual maximum Baltic Sea <span class="hlt">ice</span> extent is well in line with the observations, but the 1961-2006 trend is underestimated. Capturing the correct <span class="hlt">ice</span> thickness distribution is more challenging. Based on the simulated <span class="hlt">ice</span> thickness distribution we estimate the undeformed and deformed <span class="hlt">ice</span> thickness and concentration in the Baltic Sea, which compares reasonably well with observations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014ESSD....6..367L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014ESSD....6..367L"><span>Sea <span class="hlt">ice</span> in the Baltic Sea - revisiting BASIS <span class="hlt">ice</span>, a historical data set covering the period 1960/1961-1978/1979</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Löptien, U.; Dietze, H.</p> <p>2014-12-01</p> <p>The Baltic Sea is a seasonally <span class="hlt">ice</span>-covered, <span class="hlt">marginal</span> sea in central northern Europe. It is an essential waterway connecting highly industrialised countries. Because ship traffic is intermittently hindered by sea <span class="hlt">ice</span>, the local weather services have been monitoring sea <span class="hlt">ice</span> conditions for decades. In the present study we revisit a historical monitoring data set, covering the winters 1960/1961 to 1978/1979. This data set, dubbed Data Bank for Baltic Sea <span class="hlt">Ice</span> and Sea Surface Temperatures (BASIS) <span class="hlt">ice</span>, is based on hand-drawn maps that were collected and then digitised in 1981 in a joint project of the Finnish Institute of Marine Research (today the Finnish Meteorological Institute (FMI)) and the Swedish Meteorological and Hydrological Institute (SMHI). BASIS <span class="hlt">ice</span> was designed for storage on punch cards and all <span class="hlt">ice</span> information is encoded by five digits. This makes the data hard to access. Here we present a post-processed product based on the original five-digit code. Specifically, we convert to standard <span class="hlt">ice</span> quantities (including information on <span class="hlt">ice</span> types), which we distribute in the current and free Network Common Data Format (NetCDF). Our post-processed data set will help to assess numerical <span class="hlt">ice</span> models and provide easy-to-access unique historical reference material for sea <span class="hlt">ice</span> in the Baltic Sea. In addition we provide statistics showcasing the data quality. The website http://www.baltic-ocean.org hosts the post-processed data and the conversion code. The data are also archived at the Data Publisher for Earth & Environmental Science, PANGAEA (doi:10.1594/PANGAEA.832353).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014NatGe...7..497B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014NatGe...7..497B"><span>Deformation, warming and softening of Greenland’s <span class="hlt">ice</span> by refreezing meltwater</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bell, Robin E.; Tinto, Kirsteen; Das, Indrani; Wolovick, Michael; Chu, Winnie; Creyts, Timothy T.; Frearson, Nicholas; Abdi, Abdulhakim; Paden, John D.</p> <p>2014-07-01</p> <p>Meltwater beneath the large <span class="hlt">ice</span> sheets can influence <span class="hlt">ice</span> flow by lubrication at the base or by softening when meltwater refreezes to form relatively warm <span class="hlt">ice</span>. Refreezing has produced large basal <span class="hlt">ice</span> units in East Antarctica. Bubble-free basal <span class="hlt">ice</span> units also outcrop at the edge of the Greenland <span class="hlt">ice</span> sheet, but the extent of refreezing and its influence on Greenland’s <span class="hlt">ice</span> flow dynamics are unknown. Here we demonstrate that refreezing of meltwater produces distinct basal <span class="hlt">ice</span> units throughout northern Greenland with thicknesses of up to 1,100 m. We compare airborne gravity data with modelled gravity anomalies to show that these basal units are <span class="hlt">ice</span>. Using radar data we determine the extent of the units, which significantly disrupt the overlying <span class="hlt">ice</span> sheet stratigraphy. The units consist of refrozen basal water commonly surrounded by heavily deformed meteoric <span class="hlt">ice</span> derived from snowfall. We map these units along the <span class="hlt">ice</span> sheet <span class="hlt">margins</span> where surface melt is the largest source of water, as well as in the interior where basal melting is the only source of water. Beneath Petermann Glacier, basal units coincide with the onset of fast flow and channels in the floating <span class="hlt">ice</span> tongue. We suggest that refreezing of meltwater and the resulting deformation of the surrounding basal <span class="hlt">ice</span> warms the Greenland <span class="hlt">ice</span> sheet, modifying the temperature structure of the <span class="hlt">ice</span> column and influencing <span class="hlt">ice</span> flow and grounding line melting.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.7150N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.7150N"><span>Vertical distribution of tropospheric BrO in the <span class="hlt">marginal</span> sea <span class="hlt">ice</span> zone of the Northern Weddell Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nasse, Jan-Marcus; Zielcke, Johannes; Lampel, Johannes; Buxmann, Joelle; Frieß, Udo; Platt, Ulrich</p> <p>2015-04-01</p> <p>The free radical bromine monoxide (BrO) strongly influences the chemistry of the troposphere in Polar regions. During springtime with the return of sunlight after Polar night BrO is released in an autocatalytic reaction mechanism from saline surfaces (bromine explosion). Then BrO affects the oxidative properties of the lower atmosphere and can induce complete depletion of ozone within a matter of days or even hours. In addition, elemental mercury can be oxidized by BrO which makes this toxic compound soluble leading to a deposition into the biosphere. Despite numerous observations of elevated BrO levels in the Polar troposphere, bromine radical sources, as well as the details of the mechanisms leading to bromine explosions and the interactions between atmospheric dynamics and chemistry are not yet completely understood. To improve the understanding of these processes, an accurate determination of the spatio-temporal distribution of BrO is crucial. Here we present measurements of BrO performed during two cruises of the German research <span class="hlt">ice</span> breaker Polarstern in the <span class="hlt">marginal</span> sea <span class="hlt">ice</span> zone of the Antarctic Weddell Sea between June and October 2013 when four major periods with elevated BrO concentrations and simultaneous ozone depletion occurred. The events were observed by (1) a ship-based Multi AXis Differential Absorption Spectroscopy (MAX-DOAS) instrument on Polarstern and (2) a compact MAX-DOAS instrument operated on a helicopter. Several flights were performed in the boundary layer as well as in the free troposphere up to altitudes of 2300 m on days with elevated BrO levels. Vertical profiles of aerosol extinction and BrO concentrations were retrieved for both instruments using our HEIPRO (HEIdelberg Profile) retrieval algorithm based on optimal estimation. Elevated BrO levels in the time series from ship-borne measurements show a strong correlation to southerly wind directions indicating transport from sea <span class="hlt">ice</span> areas. Maximum retrieved BrO mixing ratios at ground</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.8973H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.8973H"><span>Capturing total chronological and spatial uncertainties in palaeo-<span class="hlt">ice</span> sheet reconstructions: the DATED example</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hughes, Anna; Gyllencreutz, Richard; Mangerud, Jan; Svendsen, John Inge</p> <p>2017-04-01</p> <p>Glacial geologists generate empirical reconstructions of former <span class="hlt">ice</span>-sheet dynamics by combining evidence from the preserved record of glacial landforms (e.g. end moraines, lineations) and sediments with chronological evidence (mainly numerical dates derived predominantly from radiocarbon, exposure and luminescence techniques). However the geomorphological and sedimentological footprints and chronological data are both incomplete records in both space and time, and all have multiple types of uncertainty associated with them. To understand <span class="hlt">ice</span> sheets' response to climate we need numerical models of <span class="hlt">ice</span>-sheet dynamics based on physical principles. To test and/or constrain such models, empirical reconstructions of past <span class="hlt">ice</span> sheets that capture and acknowledge all uncertainties are required. In 2005 we started a project (Database of the Eurasian Deglaciation, DATED) to produce an empirical reconstruction of the evolution of the last Eurasian <span class="hlt">ice</span> sheets, (including the British-Irish, Scandinavian and Svalbard-Barents-Kara Seas <span class="hlt">ice</span> sheets) that is fully documented, specified in time, and includes uncertainty estimates. Over 5000 dates relevant to constraining <span class="hlt">ice</span> build-up and retreat were assessed for reliability and used together with published <span class="hlt">ice</span>-sheet <span class="hlt">margin</span> positions based on glacial geomorphology to reconstruct time-slice maps of the <span class="hlt">ice</span> sheets' extent. The DATED maps show synchronous <span class="hlt">ice</span> <span class="hlt">margins</span> with maximum-minimum uncertainty bounds for every 1000 years between 25-10 kyr ago. In the first version of results (DATED-1; Hughes et al. 2016) all uncertainties (both quantitative and qualitative, e.g. precision and accuracy of numerical dates, correlation of moraines, stratigraphic interpretations) were combined based on our best glaciological-geological assessment and expressed in terms of distance as a 'fuzzy' <span class="hlt">margin</span>. Large uncertainties (>100 km) exist; predominantly across marine sectors and other locations where there are spatial gaps in the dating record (e.g. the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C31D..01S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C31D..01S"><span>The Sea-<span class="hlt">Ice</span> 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>Stern, H. L., III; Schweiger, A. J. B.; Zhang, J.; Steele, M.</p> <p>2017-12-01</p> <p>The size distribution of <span class="hlt">ice</span> floes in the polar seas affects the dynamics and thermodynamics of the <span class="hlt">ice</span> cover and its interaction with the ocean and atmosphere. <span class="hlt">Ice</span>-ocean models are now beginning to include the floe size distribution (FSD) in their simulations. In order to characterize seasonal changes of the FSD and provide validation data for our <span class="hlt">ice</span>-ocean model, we calculated the FSD in the Beaufort and Chukchi seas over two spring-summer-fall seasons (2013 and 2014) using more than 250 cloud-free visible-band scenes from the MODIS sensors on NASA's Terra and Aqua satellites, identifying nearly 250,000 <span class="hlt">ice</span> floes between 2 and 30 km in diameter. We found that the FSD follows a power-law distribution at all locations, with a seasonally varying exponent that reflects floe break-up in spring, loss of smaller floes in summer, and the return of larger floes after fall freeze-up. We extended the results to floe sizes from 10 m to 2 km at selected time/space locations using more than 50 high-resolution radar and visible-band satellite images. Our analysis used more data and applied greater statistical rigor than any previous study of the FSD. The incorporation of the FSD into our <span class="hlt">ice</span>-ocean model resulted in reduced sea-<span class="hlt">ice</span> thickness, mainly in the <span class="hlt">marginal</span> <span class="hlt">ice</span> zone, which improved the simulation of sea-<span class="hlt">ice</span> extent and yielded an earlier <span class="hlt">ice</span> retreat. We also examined results from 17 previous studies of the FSD, most of which report power-law FSDs but with widely varying exponents. It is difficult to reconcile the range of results due to different study areas, seasons, and methods of analysis. We review the power-law representation of the FSD in these studies and discuss some mathematical details that are important to consider in any future analysis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMPP53B2008W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMPP53B2008W"><span>Greenhouse to Icehouse Antarctic Paleoclimate and <span class="hlt">Ice</span> History from George V Land and Adélie Land Shelf Sediments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Williams, T.; Escutia, C.; De Santis, L.; O'Brien, P.; Pekar, S. F.; Brinkhuis, H.; Domack, E. W.</p> <p>2013-12-01</p> <p>Along the George V and Adélie Land continental shelf of East Antarctica, shallowly-buried strata contain a record of Antarctica's climate and <span class="hlt">ice</span> history from the lush forests of the Eocene greenhouse to the dynamic <span class="hlt">ice</span> sheet <span class="hlt">margins</span> of the Neogene. Short piston cores and dredges have recovered Early Cretaceous and Eocene organic-rich sediment at the seabed, and in 2010, IODP Expedition 318 recovered earliest Oligocene and early Pliocene subglacial and proglacial diamictites. However, challenging <span class="hlt">ice</span> and drilling conditions from the JOIDES Resolution on the shelf resulted in poor core recovery and sites had to be abandoned before the stratigraphic targets could be reached. Therefore, in a new IODP drilling proposal submitted earlier this year, we propose to use the MeBo sea bed drill for improved core recovery and easier access to the shelf, and drill a stratigraphic transect of shallow (~80m) holes. To investigate the evolution of the Antarctic <span class="hlt">ice</span> sheet in this sector, we target strata above and below regional erosional and downlap surfaces to date and characterize major episodes of <span class="hlt">ice</span> sheet advance and retreat. These direct records of <span class="hlt">ice</span> extent on the shelf can be set in the context of Southern Ocean records of temperature, <span class="hlt">ice</span>-rafted debris (IRD) and latitudinal fluctuations of the opal belt, and hence we can relate <span class="hlt">ice</span> sheet evolution to paleoclimate conditions. Targets include possible late Eocene precursor glaciations, the Eocene/Oligocene boundary erosion surface, Oligocene and Miocene <span class="hlt">ice</span> extents, and <span class="hlt">ice</span> <span class="hlt">margin</span> fluctuations in the Pliocene. At the Cretaceous and Eocene proposed sites, marine and terrestrial temperature proxies and palynological records will provide information on high-latitude paleoenvironments and pole-equator temperature gradients. Here we present existing data from the area and the proposed new drill sites. The <span class="hlt">ice</span> and climate history of the George V and Adélie Land <span class="hlt">margin</span> can provide warm-world scenarios to help understand <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_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/16782607','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16782607"><span><span class="hlt">Ice</span>-sheet contributions to future sea-level change.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gregory, J M; Huybrechts, P</p> <p>2006-07-15</p> <p>Accurate simulation of <span class="hlt">ice</span>-sheet surface mass balance requires higher spatial resolution than is afforded by typical atmosphere-ocean general circulation models (AOGCMs), owing, in particular, to the need to resolve the narrow and steep <span class="hlt">margins</span> where the majority of precipitation and ablation occurs. We have developed a method for calculating mass-balance changes by combining <span class="hlt">ice</span>-sheet average time-series from AOGCM projections for future centuries, both with information from high-resolution climate models run for short periods and with a 20km <span class="hlt">ice</span>-sheet mass-balance model. Antarctica contributes negatively to sea level on account of increased accumulation, while Greenland contributes positively because ablation increases more rapidly. The uncertainty in the results is about 20% for Antarctica and 35% for Greenland. Changes in <span class="hlt">ice</span>-sheet topography and dynamics are not included, but we discuss their possible effects. For an annual- and area-average warming exceeding 4.5+/-0.9K in Greenland and 3.1+/-0.8K in the global average, the net surface mass balance of the Greenland <span class="hlt">ice</span> sheet becomes negative, in which case it is likely that the <span class="hlt">ice</span> sheet would eventually be eliminated, raising global-average sea level by 7m.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016DPS....4822022H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016DPS....4822022H"><span>Synoptic Traveling Weather Systems on Mars: Effects of Radiatively-<span class="hlt">Active</span> Water <span class="hlt">Ice</span> Clouds</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hollingsworth, Jeffery L.; Kahre, Melinda A.; Haberle, Robert; Atsuki Urata, Richard</p> <p>2016-10-01</p> <p>Atmospheric aerosols on Mars are critical in determining the nature of its thermal structure, its large-scale circulation, and hence the overall climate of the planet. We conduct multi-annual simulations with the latest version of the NASA Ames Mars global climate model (GCM), gcm2.3+, that includes a modernized radiative-transfer package and complex water-<span class="hlt">ice</span> cloud microphysics package which permit radiative effects and interactions of suspended atmospheric aerosols (e.g., water <span class="hlt">ice</span> clouds, water vapor, dust, and mutual interactions) to influence the net diabatic heating. Results indicate that radiatively <span class="hlt">active</span> water <span class="hlt">ice</span> clouds profoundly affect the seasonal and annual mean climate. The mean thermal structure and balanced circulation patterns are strongly modified near the surface and aloft. Warming of the subtropical atmosphere at altitude and cooling of the high latitude atmosphere at low levels takes place, which increases the mean pole-to-equator temperature contrast (i.e., "baroclinicity"). With radiatively <span class="hlt">active</span> water <span class="hlt">ice</span> clouds (RAC) compared to radiatively inert water <span class="hlt">ice</span> clouds (nonRAC), significant changes in the intensity of the mean state and forced stationary Rossby modes occur, both of which affect the vigor and intensity of traveling, synoptic period weather systems. Such weather systems not only act as key agents in the transport of heat and momentum beyond the extent of the Hadley circulation, but also the transport of trace species such as water vapor, water <span class="hlt">ice</span>-clouds, dust and others. The northern hemisphere (NH) forced Rossby waves and resultant wave train are augmented in the RAC case: the modes are more intense and the wave train is shifted equatorward. Significant changes also occur within the subtropics and tropics. The Rossby wave train sets up, combined with the traveling synoptic-period weather systems (i.e., cyclones and anticyclones), the geographic extent of storm zones (or storm tracks) within the NH. A variety of circulation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170002698','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170002698"><span>Synoptic Traveling Weather Systems on Mars: Effects of Radiatively-<span class="hlt">Active</span> Water <span class="hlt">Ice</span> Clouds</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hollingsworth, Jeffery; Kahre, Melinda; Haberle, Robert; Urata, Richard</p> <p>2017-01-01</p> <p>Atmospheric aerosols on Mars are critical in determining the nature of its thermal structure, its large-scale circulation, and hence the overall climate of the planet. We conduct multi-annual simulations with the latest version of the NASA Ames Mars global climate model (GCM), gcm2.3+, that includes a modernized radiative-transfer package and complex water-<span class="hlt">ice</span> cloud microphysics package which permit radiative effects and interactions of suspended atmospheric aerosols (e.g., water <span class="hlt">ice</span> clouds, water vapor, dust, and mutual interactions) to influence the net diabatic heating. Results indicate that radiatively <span class="hlt">active</span> water <span class="hlt">ice</span> clouds profoundly affect the seasonal and annual mean climate. The mean thermal structure and balanced circulation patterns are strongly modified near the surface and aloft. Warming of the subtropical atmosphere at altitude and cooling of the high latitude atmosphere at low levels takes place, which increases the mean pole-to-equator temperature contrast (i.e., "baroclinicity"). With radiatively <span class="hlt">active</span> water <span class="hlt">ice</span> clouds (RAC) compared to radiatively inert water <span class="hlt">ice</span> clouds (nonRAC), significant changes in the intensity of the mean state and forced stationary Rossby modes occur, both of which affect the vigor and intensity of traveling, synoptic period weather systems. Such weather systems not only act as key agents in the transport of heat and momentum beyond the extent of the Hadley circulation, but also the transport of trace species such as water vapor, water <span class="hlt">ice</span>-clouds, dust and others. The northern hemisphere (NH) forced Rossby waves and resultant wave train are augmented in the RAC case: the modes are more intense and the wave train is shifted equatorward. Significant changes also occur within the subtropics and tropics. The Rossby wave train sets up, combined with the traveling synoptic period weather systems (i.e., cyclones and anticyclones), the geographic extent of storm zones (or storm tracks) within the NH. A variety of circulation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170006193','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170006193"><span>Synoptic Traveling Weather Systems on Mars: Effects of Radiatively-<span class="hlt">Active</span> Water <span class="hlt">Ice</span> Clouds</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hollingsworth, Jeffery; Kahre, Melinda; Haberle, Robert; Urata, Richard</p> <p>2017-01-01</p> <p>Atmospheric aerosols on Mars are critical in determining the nature of its thermal structure, its large-scale circulation, and hence the overall climate of the planet. We conduct multi-annual simulations with the latest version of the NASA Ames Mars global climate model (GCM), gcm2.3+, that includes a modernized radiative-transfer package and complex water-<span class="hlt">ice</span> cloud microphysics package which permit radiative effects and interactions of suspended atmospheric aerosols (e.g., water <span class="hlt">ice</span> clouds, water vapor, dust, and mutual interactions) to influence the net diabatic heating. Results indicate that radiatively <span class="hlt">active</span> water <span class="hlt">ice</span> clouds profoundly affect the seasonal and annual mean climate. The mean thermal structure and balanced circulation patterns are strongly modified near the surface and aloft. Warming of the subtropical atmosphere at altitude and cooling of the high latitude atmosphere at low levels takes place, which increases the mean pole-to-equator temperature contrast (i.e., "baroclinicity"). With radiatively <span class="hlt">active</span> water <span class="hlt">ice</span> clouds (RAC) compared to radiatively inert water <span class="hlt">ice</span> clouds (nonRAC), significant changes in the intensity of the mean state and forced stationary Rossby modes occur, both of which affect the vigor and intensity of traveling, synoptic period weather systems.Such weather systems not only act as key agents in the transport of heat and momentum beyond the extent of the Hadley circulation, but also the transport of trace species such as water vapor, water <span class="hlt">ice</span>-clouds, dust and others. The northern hemisphere (NH) forced Rossby waves and resultant wave train are augmented in the RAC case: the modes are more intense and the wave train is shifted equatorward. Significant changes also occur within the subtropics and tropics. The Rossby wave train sets up, combined with the traveling synoptic period weather systems (i.e., cyclones and anticyclones), the geographic extent of storm zones (or storm tracks) within the NH. A variety of circulation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1813508S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1813508S"><span>The Impact of Geothermal Heat on the Scandinavian <span class="hlt">Ice</span> Sheet's LGM Extent</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Szuman, Izabela; Ewertowski, Marek W.; Kalita, Jakub Z.</p> <p>2016-04-01</p> <p>The last Scandinavian <span class="hlt">ice</span> sheet attained its most southern extent over Poland and Germany, protruding c. 200 km south of the main <span class="hlt">ice</span> sheet mass. There are number of factors that may control <span class="hlt">ice</span> sheet dynamics and extent. One of the less recognised is geothermal heat, which is heat that is supplied to the base of the <span class="hlt">ice</span> sheet. A heat at the <span class="hlt">ice</span>/bed interface plays a crucial role in controlling <span class="hlt">ice</span> sheet stability, as well as impacting basal temperatures, melting, and <span class="hlt">ice</span> flow velocities. However, the influence of geothermal heat is still virtually neglected in reconstructions and modelling of paleo-<span class="hlt">ice</span> sheets behaviour. Only in a few papers is geothermal heat recalled though often in the context of past climatic conditions. Thus, the major question is if and how spatial differences in geothermal heat had influenced paleo-<span class="hlt">ice</span> sheet dynamics and in consequence their extent. Here, we assumed that the configuration of the <span class="hlt">ice</span> sheet along its southern <span class="hlt">margin</span> was moderately to strongly correlated with geothermal heat for Poland and non or negatively correlated for Germany.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-GSFC_20171208_Archive_e002002.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-GSFC_20171208_Archive_e002002.html"><span><span class="hlt">Ice</span> Island Calves off Petermann Glacier</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>NASA image acquired August 11, 2010. After breaking off the Petermann Glacier on August 5, 2010, a massive <span class="hlt">ice</span> island floated slowly down the fjord toward the Nares Strait. The Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) on NASA’s Terra satellite captured this false-color image of the <span class="hlt">ice</span> island on August 11, 2010. In this image, <span class="hlt">ice</span> is light blue, water is nearly black, and clouds are nearly white. Although a bank of thin clouds hovers over the fjord, the southernmost <span class="hlt">margin</span> of the <span class="hlt">ice</span> island is still visible. Toward the north, the leading edge of the <span class="hlt">ice</span> island retains the same shape it had days earlier, at the time of the initial calving. NASA Earth Observatory image created by Jesse Allen, using data provided courtesy of NASA/GSFC/METI/ERSDAC/JAROS, and U.S./Japan ASTER Science Team. Caption by Michon Scott. Instrument: Terra - ASTER To see more images from of the glacier go to: earthobservatory.nasa.gov/NaturalHazards/event.php?id=45116 NASA Goddard Space Flight Center is home to the nation's largest organization of combined scientists, engineers and technologists that build spacecraft, instruments and new technology to study the Earth, the sun, our solar system, and the universe. Follow us on Twitter Join us on Facebook</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ATel10801....1L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ATel10801....1L"><span>AGILE confirmation of gamma-ray <span class="hlt">activity</span> from the <span class="hlt">Ice</span>Cube-170922A error region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lucarelli, F.; Piano, G.; Pittori, C.; Verrecchia, F.; Tavani, M.; Bulgarelli, A.; Munar-Adrover, P.; Minervini, G.; Ursi, A.; Vercellone, S.; Donnarumma, I.; Fioretti, V.; Zoli, A.; Striani, E.; Cardillo, M.; Gianotti, F.; Trifoglio, M.; Giuliani, A.; Mereghetti, S.; Caraveo, P.; Perotti, F.; Chen, A.; Argan, A.; Costa, E.; Del Monte, E.; Evangelista, Y.; Feroci, M.; Lazzarotto, F.; Lapshov, I.; Pacciani, L.; Soffitta, P.; Sabatini, S.; Vittorini, V.; Pucella, G.; Rapisarda, M.; Di Cocco, G.; Fuschino, F.; Galli, M.; Labanti, C.; Marisaldi, M.; Pellizzoni, A.; Pilia, M.; Trois, A.; Barbiellini, G.; Vallazza, E.; Longo, F.; Morselli, A.; Picozza, P.; Prest, M.; Lipari, P.; Zanello, D.; Cattaneo, P. W.; Rappoldi, A.; Colafrancesco, S.; Parmiggiani, N.; Ferrari, A.; Paoletti, F.; Antonelli, A.; Giommi, P.; Salotti, L.; Valentini, G.; D'Amico, F.</p> <p>2017-09-01</p> <p>Following the <span class="hlt">Ice</span>Cube observation of a high-energy neutrino candidate event, <span class="hlt">Ice</span>Cube-170922A, at T0 = 17/09/22 20:54:30.43 UT (https://gcn.gsfc.nasa.gov/gcn3/21916.gcn3), and the detection of increased gamma-ray <span class="hlt">activity</span> from a previously known Fermi-LAT gamma-ray source (3FGL J0509.4+0541) in the <span class="hlt">Ice</span>Cube-170922A error region (ATel #10791), we have analysed the AGILE-GRID data acquired in the days before and after the neutrino event T0, searching for significant gamma-ray excess above 100 MeV from a position compatible with the <span class="hlt">Ice</span>Cube and Fermi-LAT error regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C41A1187C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C41A1187C"><span>Formation and interpretation of eskers beneath retreating <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>Creyts, T. T.; Hewitt, I.</p> <p>2017-12-01</p> <p>The retreat of the <span class="hlt">ice</span> sheets during the Pleistocene left large and spectacular subglacial features exposed. Understanding these features gives us insight into how the <span class="hlt">ice</span> sheets retreated, how meltwater influenced retreat, and can help inform our understanding of potential future rates of <span class="hlt">ice</span> sheet retreat. Among these features, eskers, long sinuous ridges primarily composed of clastic sediments, lack a detailed explanation of how surface melt rates and <span class="hlt">ice</span> sheet retreat rates influence their growth and spatial distribution. Here, we develop a theory for esker formation based on the initial work of Rothlisberger modified for sediment transport and inclusion of surface meltwater forcing. The primary subglacial ingredients include water flow through subglacial tunnels with the addition of mass balances for sediment transport. We show how eskers when water flow slows below a critical stress for sediment motion. This implies that eskers are deposited in a localized region near the snout of the <span class="hlt">ice</span> sheet. Our findings suggest that very long eskers form sequentially as the <span class="hlt">ice</span> front retreats. The position of the esker follows the path of the channel mouth through time, which does not necessarily coincide with the instantaneous route of the feeding channel. However, in most cases, we expect those locations to be similar. The role of surface meltwater and the climatology associated with the forcing is crucial to the lateral spacing of the eskers. We predict that high surface melt rates lead to narrower catchments but that the greater extent of the ablation area means that channels are likely larger. At the same time, for a given channel size (and hence sediment flux), the size of a deposited esker depends on a <span class="hlt">margin</span> retreat rate. Hence, the size of the eskers is related delicately to the balance between surface melt rates and <span class="hlt">margin</span> retreat rates. We discuss how our theory can be combined with observed esker distributions to infer the relationship between these two rates</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.6195B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.6195B"><span>The glacial geomorphology of the Lago Buenos Aires and Lago Puerreydón <span class="hlt">ice</span> lobes, Central Patagonia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bendle, Jacob; Thorndycraft, Varyl; Palmer, Adrian</p> <p>2016-04-01</p> <p>Patagonia is ideally located for reconstructions of late Quaternary <span class="hlt">ice</span>-climate interaction(s) in the Southern Hemisphere mid-latitudes, yet many questions remain concerning post-LGM <span class="hlt">ice</span> sheet retreat dynamics across the region. While modern-day glaciation is restricted to three small icefields (the North and South Patagonian and Cordillera Darwin icefields), during the Quaternary, and at the LGM, episodes of significant <span class="hlt">ice</span> advance culminated in an expansive Patagonian <span class="hlt">ice</span> sheet (PIS) centered over the southern Andes, for which a long and well-preserved landform record exists. Previous mapping in the region has either aimed to achieve regional coverage, necessarily omitting more subtle/complex features suggestive of certain <span class="hlt">ice-marginal</span> processes, or has focused on the identification of palaeo-<span class="hlt">ice</span> limits (e.g. moraine ridges) for geochronological applications, with little attention given to other (e.g. glaciofluvial, glaciolacustrine) features that are significant for understanding post-LGM <span class="hlt">ice</span> sheet retreat dynamics. This poster presents a comprehensive and highly detailed (<30m spatial resolution) map of the glacial geomorphology of the Lago Buenos Aires (46.4°S) and Lago Puerreydón (47.2°S) <span class="hlt">ice</span> lobes, major outlet glaciers of the central sector of the former PIS. The map allows refined reconstructions of glacial and, in particular, deglacial <span class="hlt">ice-marginal</span> processes, and will underpin further analysis on the retreat history of the palaeo-<span class="hlt">ice</span> lobes using high-resolution lithostratigraphic (varve) analyses.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ACP....1613359B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ACP....1613359B"><span>Effect of particle surface area on <span class="hlt">ice</span> <span class="hlt">active</span> site densities retrieved from droplet freezing spectra</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Beydoun, Hassan; Polen, Michael; Sullivan, Ryan C.</p> <p>2016-10-01</p> <p>Heterogeneous <span class="hlt">ice</span> nucleation remains one of the outstanding problems in cloud physics and atmospheric science. Experimental challenges in properly simulating particle-induced freezing processes under atmospherically relevant conditions have largely contributed to the absence of a well-established parameterization of immersion freezing properties. Here, we formulate an <span class="hlt">ice</span> <span class="hlt">active</span>, surface-site-based stochastic model of heterogeneous freezing with the unique feature of invoking a continuum assumption on the <span class="hlt">ice</span> nucleating <span class="hlt">activity</span> (contact angle) of an aerosol particle's surface that requires no assumptions about the size or number of <span class="hlt">active</span> sites. The result is a particle-specific property g that defines a distribution of local <span class="hlt">ice</span> nucleation rates. Upon integration, this yields a full freezing probability function for an <span class="hlt">ice</span> nucleating particle. Current cold plate droplet freezing measurements provide a valuable and inexpensive resource for studying the freezing properties of many atmospheric aerosol systems. We apply our g framework to explain the observed dependence of the freezing temperature of droplets in a cold plate on the concentration of the particle species investigated. Normalizing to the total particle mass or surface area present to derive the commonly used <span class="hlt">ice</span> nuclei <span class="hlt">active</span> surface (INAS) density (ns) often cannot account for the effects of particle concentration, yet concentration is typically varied to span a wider measurable freezing temperature range. A method based on determining what is denoted an <span class="hlt">ice</span> nucleating species' specific critical surface area is presented and explains the concentration dependence as a result of increasing the variability in <span class="hlt">ice</span> nucleating <span class="hlt">active</span> sites between droplets. By applying this method to experimental droplet freezing data from four different systems, we demonstrate its ability to interpret immersion freezing temperature spectra of droplets containing variable particle concentrations. It is shown that general</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUSM.C23A..04S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUSM.C23A..04S"><span>Effects of Atmospheric Water and Surface Wind on Passive Microwave Retrievals of Sea <span class="hlt">Ice</span> Concentration: a Simulation Study</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shin, D.; Chiu, L. S.; Clemente-Colon, P.</p> <p>2006-05-01</p> <p>The atmospheric effects on the retrieval of sea <span class="hlt">ice</span> concentration from passive microwave sensors are examined using simulated data typical for the Arctic summer. The simulation includes atmospheric contributions of cloud liquid water, water vapor and surface wind on the microwave signatures. A plane parallel radiative transfer model is used to compute brightness temperatures at SSM/I frequencies over surfaces that contain open water, first-year (FY) <span class="hlt">ice</span> and multi-year (MY) <span class="hlt">ice</span> and their combinations. Synthetic retrievals in this study use the NASA Team (NT) algorithm for the estimation of sea <span class="hlt">ice</span> concentrations. This study shows that if the satellite sensor's field of view is filled with only FY <span class="hlt">ice</span> the retrieval is not much affected by the atmospheric conditions due to the high contrast between emission signals from FY <span class="hlt">ice</span> surface and the signals from the atmosphere. Pure MY <span class="hlt">ice</span> concentration is generally underestimated due to the low MY <span class="hlt">ice</span> surface emissivity that results in the enhancement of emission signals from the atmospheric parameters. Simulation results in <span class="hlt">marginal</span> <span class="hlt">ice</span> areas also show that the atmospheric effects from cloud liquid water, water vapor and surface wind tend to degrade the accuracy at low sea <span class="hlt">ice</span> concentration. FY <span class="hlt">ice</span> concentration is overestimated and MY <span class="hlt">ice</span> concentration is underestimated in the presence of atmospheric water and surface wind at low <span class="hlt">ice</span> concentration. This compensating effect reduces the retrieval uncertainties of total (FY and MY) <span class="hlt">ice</span> concentration. Over <span class="hlt">marginal</span> <span class="hlt">ice</span> zones, our results suggest that strong surface wind is more important than atmospheric water in contributing to the retrieval errors of total <span class="hlt">ice</span> concentrations in the normal ranges of these variables.</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 <span class="hlt">active</span> bacterial community linked to high chl-a concentrations in Antarctic 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>Antarctic 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 cover 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 Antarctic 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 Antarctic sea <span class="hlt">ice</span> can stay <span class="hlt">active</span> 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 Antarctic sea-<span class="hlt">ice</span> zone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009QSRv...28.3101G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009QSRv...28.3101G"><span>Reconstructing the last Irish <span class="hlt">Ice</span> Sheet 2: a geomorphologically-driven model of <span class="hlt">ice</span> sheet growth, retreat and dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Greenwood, Sarah L.; Clark, Chris D.</p> <p>2009-12-01</p> <p>The <span class="hlt">ice</span> sheet that once covered Ireland has a long history of investigation. Much prior work focussed on localised evidence-based reconstructions and <span class="hlt">ice-marginal</span> dynamics and chronologies, with less attention paid to an <span class="hlt">ice</span> sheet wide view of the first order properties of the <span class="hlt">ice</span> sheet: centres of mass, <span class="hlt">ice</span> divide structure, <span class="hlt">ice</span> flow geometry and behaviour and changes thereof. In this paper we focus on the latter aspect and use our new, countrywide glacial geomorphological mapping of the Irish landscape (>39 000 landforms), and our analysis of the palaeo-glaciological significance of observed landform assemblages (article Part 1), to build an <span class="hlt">ice</span> sheet reconstruction yielding these fundamental <span class="hlt">ice</span> sheet properties. We present a seven stage model of <span class="hlt">ice</span> sheet evolution, from initiation to demise, in the form of palaeo-geographic maps. An early incursion of <span class="hlt">ice</span> from Scotland likely coalesced with local <span class="hlt">ice</span> caps and spread in a south-westerly direction 200 km across Ireland. A semi-independent Irish <span class="hlt">Ice</span> Sheet was then established during <span class="hlt">ice</span> sheet growth, with a branching <span class="hlt">ice</span> divide structure whose main axis migrated up to 140 km from the west coast towards the east. <span class="hlt">Ice</span> stream systems converging on Donegal Bay in the west and funnelling through the North Channel and Irish Sea Basin in the east emerge as major flow components of the maximum stages of glaciation. <span class="hlt">Ice</span> cover is reconstructed as extending to the continental shelf break. The Irish <span class="hlt">Ice</span> Sheet became autonomous (i.e. separate from the British <span class="hlt">Ice</span> Sheet) during deglaciation and fragmented into multiple <span class="hlt">ice</span> masses, each decaying towards the west. Final sites of demise were likely over the mountains of Donegal, Leitrim and Connemara. Patterns of growth and decay of the <span class="hlt">ice</span> sheet are shown to be radically different: asynchronous and asymmetric in both spatial and temporal domains. We implicate collapse of the <span class="hlt">ice</span> stream system in the North Channel - Irish Sea Basin in driving such asymmetry, since rapid</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMPP21B1327O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMPP21B1327O"><span><span class="hlt">Ice</span> Core Records of Recent Northwest Greenland Climate</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Osterberg, E. C.; Wong, G. J.; Ferris, D.; Lutz, E.; Howley, J. A.; Kelly, M. A.; Axford, Y.; Hawley, R. L.</p> <p>2014-12-01</p> <p>Meteorological station data from NW Greenland indicate a 3oC temperature rise since 1990, with most of the warming occurring in fall and winter. According to remote sensing data, the NW Greenland <span class="hlt">ice</span> sheet (GIS) and coastal <span class="hlt">ice</span> caps are responding with <span class="hlt">ice</span> mass loss and <span class="hlt">margin</span> retreat, but the cryosphere's response to previous climate variability is poorly constrained in this region. We are developing multi-proxy records (lake sediment cores, <span class="hlt">ice</span> cores, glacial geologic data, glaciological models) of Holocene climate change and cryospheric response in NW Greenland to improve projections of future <span class="hlt">ice</span> loss and sea level rise in a warming climate. As part of our efforts to develop a millennial-length <span class="hlt">ice</span> core paleoclimate record from the Thule region, we collected and analyzed snow pit samples and short firn cores (up to 21 m) from the coastal region of the GIS (2Barrel site; 76.9317o N, 63.1467o W, 1685 m el.) and the summit of North <span class="hlt">Ice</span> Cap (76.938o N, 67.671o W, 1273 m el.) in 2011, 2012 and 2014. The 2Barrel <span class="hlt">ice</span> core record has statistically significant relationships with regional spring and fall Baffin Bay sea <span class="hlt">ice</span> extent, summertime temperature, and annual precipitation. Here we evaluate relationships between the 2014 North <span class="hlt">Ice</span> Cap firn core glaciochemical record and climate variability from regional instrumental stations and reanalysis datasets. We compare the coastal North <span class="hlt">Ice</span> Cap record to more inland records from 2Barrel, Camp Century and NEEM to evaluate spatial and elevational gradients in recent NW Greenland climate change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030054467','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030054467"><span><span class="hlt">Iced</span> Aircraft Flight Data for Flight Simulator Validation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ratvasky, Thomas P.; Blankenship, Kurt; Rieke, William; Brinker, David J.</p> <p>2003-01-01</p> <p>NASA is developing and validating technology to incorporate aircraft <span class="hlt">icing</span> effects into a flight training device concept demonstrator. Flight simulation models of a DHC-6 Twin Otter were developed from wind tunnel data using a subscale, complete aircraft model with and without simulated <span class="hlt">ice</span>, and from previously acquired flight data. The validation of the simulation models required additional aircraft response time histories of the airplane configured with simulated <span class="hlt">ice</span> similar to the subscale model testing. Therefore, a flight test was conducted using the NASA Twin Otter <span class="hlt">Icing</span> Research Aircraft. Over 500 maneuvers of various types were conducted in this flight test. The validation data consisted of aircraft state parameters, pilot inputs, propulsion, weight, center of gravity, and moments of inertia with the airplane configured with different amounts of simulated <span class="hlt">ice</span>. Emphasis was made to acquire data at wing stall and tailplane stall since these events are of primary interest to model accurately in the flight training device. Analyses of several datasets are described regarding wing and tailplane stall. Key findings from these analyses are that the simulated wing <span class="hlt">ice</span> shapes significantly reduced the C , max, while the simulated tail <span class="hlt">ice</span> caused elevator control force anomalies and tailplane stall when flaps were deflected 30 deg or greater. This effectively reduced the safe operating <span class="hlt">margins</span> between <span class="hlt">iced</span> wing and <span class="hlt">iced</span> tail stall as flap deflection and thrust were increased. This flight test demonstrated that the critical aspects to be modeled in the <span class="hlt">icing</span> effects flight training device include: <span class="hlt">iced</span> wing and tail stall speeds, flap and thrust effects, control forces, and control effectiveness.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70038745','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70038745"><span>History of the Greenland <span class="hlt">Ice</span> Sheet: paleoclimatic insights</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Alley, Richard B.; Andrews, John T.; Brigham-Grette, J.; Clarke, G.K.C.; Cuffey, Kurt M.; Fitzpatrick, J.J.; Funder, S.; Marshall, S.J.; Miller, G.H.; Mitrovica, J.X.; Muhs, D.R.; Otto-Bliesner, B. L.; Polyak, L.; White, J.W.C.</p> <p>2010-01-01</p> <p>Paleoclimatic records show that the Greenland<span class="hlt">Ice</span> Sheet consistently has lost mass in response to warming, and grown in response to cooling. Such changes have occurred even at times of slow or zero sea-level change, so changing sea level cannot have been the cause of at least some of the <span class="hlt">ice</span>-sheet changes. In contrast, there are no documented major <span class="hlt">ice</span>-sheet changes that occurred independent of temperature changes. Moreover, snowfall has increased when the climate warmed, but the <span class="hlt">ice</span> sheet lost mass nonetheless; increased accumulation in the <span class="hlt">ice</span> sheet's center has not been sufficient to counteract increased melting and flow near the edges. Most documented forcings and <span class="hlt">ice</span>-sheet responses spanned periods of several thousand years, but limited data also show rapid response to rapid forcings. In particular, regions near the <span class="hlt">ice</span> <span class="hlt">margin</span> have responded within decades. However, major changes of central regions of the <span class="hlt">ice</span> sheet are thought to require centuries to millennia. The paleoclimatic record does not yet strongly constrain how rapidly a major shrinkage or nearly complete loss of the <span class="hlt">ice</span> sheet could occur. The evidence suggests nearly total <span class="hlt">ice</span>-sheet loss may result from warming of more than a few degrees above mean 20th century values, but this threshold is poorly defined (perhaps as little as 2 °C or more than 7 °C). Paleoclimatic records are sufficiently sketchy that the <span class="hlt">ice</span> sheet may have grown temporarily in response to warming, or changes may have been induced by factors other than temperature, without having been recorded.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19890018779','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19890018779"><span><span class="hlt">Ice</span> sheet radar altimetry</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zwally, J.</p> <p>1988-01-01</p> <p>The surface topography of the Greenland and Antarctic <span class="hlt">ice</span> sheets between 72 degrees north and south was mapped using radar altimetry data from the U.S. Navy GEOSAT. The glaciological objectives of this <span class="hlt">activity</span> were to study the dynamics of the <span class="hlt">ice</span> flow, changes in the position of floating <span class="hlt">ice</span>-shelf fronts, and ultimately to measure temporal changes in <span class="hlt">ice</span> surface elevation indicative of <span class="hlt">ice</span> sheet mass balance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19870065965&hterms=sars&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dsars','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19870065965&hterms=sars&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dsars"><span>Observing rotation and deformation of sea <span class="hlt">ice</span> with synthetic aperture radar</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Vesecky, J. F.; Samadani, R.; Daida, J. M.; Smith, M. P.; Bracewell, R. N.</p> <p>1987-01-01</p> <p>The ESA's ERS-1 satellite will carry SARs over the polar regions; an important component in the use of these data is an automated scheme for the extraction of sea <span class="hlt">ice</span> velocity fields from a sequence of SAR images of the same geographical region. The image pyramid area-correlation hierarchical method is noted to be vulnerable to uncertainties for sea <span class="hlt">ice</span> rotations greater than 10-15 deg between SAR observations. Rotation-invariant methods can successfully track isolated floes in the <span class="hlt">marginal</span> <span class="hlt">ice</span> zone. Hu's (1962) invariant moments are also worth considering as a possible basis for rotation-invariant tracking methods. Feature tracking is inherently robust for tracking rotating sea <span class="hlt">ice</span>, but is limited when features are floe-lead boundaries. A variety of techniques appears neccessary.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1013707','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1013707"><span>Evolution of the <span class="hlt">Marginal</span> <span class="hlt">Ice</span> Zone: Adaptive Sampling with Autonomous Gliders</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2015-09-30</p> <p>kinetic energy (ε). Gliders also sampled dissolved oxygen, optical backscatter ( chlorophyll and CDOM fluorescence) and multi-spectral downwelling...Fig. 2). In the pack, Pacific Summer Water and a deep chlorophyll maximum form distinct layers at roughly 60 m and 80 m, respectively, which become...Sections across the <span class="hlt">ice</span> edge just prior to recovery, during freeze-up, reveal elevated chlorophyll fluorescence throughout the mixed layer (Fig. 4</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018BGeo...15.1987S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018BGeo...15.1987S"><span>Do pelagic grazers benefit from sea <span class="hlt">ice</span>? Insights from the Antarctic sea <span class="hlt">ice</span> proxy IPSO25</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schmidt, Katrin; Brown, Thomas A.; Belt, Simon T.; Ireland, Louise C.; Taylor, Kyle W. R.; Thorpe, Sally E.; Ward, Peter; Atkinson, Angus</p> <p>2018-04-01</p> <p>Sea <span class="hlt">ice</span> affects primary production in polar regions in multiple ways. It can dampen water column productivity by reducing light or nutrient supply, provide a habitat for <span class="hlt">ice</span> algae and condition the <span class="hlt">marginal</span> <span class="hlt">ice</span> zone (MIZ) for phytoplankton blooms on its seasonal retreat. The relative importance of three different carbon sources (sea <span class="hlt">ice</span> derived, sea <span class="hlt">ice</span> conditioned, non-sea-<span class="hlt">ice</span> associated) for the polar food web is not well understood, partly due to the lack of methods that enable their unambiguous distinction. Here we analysed two highly branched isoprenoid (HBI) biomarkers to trace sea-<span class="hlt">ice</span>-derived and sea-<span class="hlt">ice</span>-conditioned carbon in Antarctic krill (Euphausia superba) and relate their concentrations to the grazers' body reserves, growth and recruitment. During our sampling in January-February 2003, the proxy for sea <span class="hlt">ice</span> diatoms (a di-unsaturated HBI termed IPSO25, δ13C = -12.5 ± 3.3 ‰) occurred in open waters of the western Scotia Sea, where seasonal <span class="hlt">ice</span> retreat was slow. In suspended matter from surface waters, IPSO25 was present at a few stations close to the <span class="hlt">ice</span> edge, but in krill the marker was widespread. Even at stations that had been <span class="hlt">ice</span>-free for several weeks, IPSO25 was found in krill stomachs, suggesting that they gathered the <span class="hlt">ice</span>-derived algae from below the upper mixed layer. Peak abundances of the proxy for MIZ diatoms (a tri-unsaturated HBI termed HBI III, δ13C = -42.2 ± 2.4 ‰) occurred in regions of fast sea <span class="hlt">ice</span> retreat and persistent salinity-driven stratification in the eastern Scotia Sea. Krill sampled in the area defined by the <span class="hlt">ice</span> edge bloom likewise contained high amounts of HBI III. As indicators for the grazer's performance we used the mass-length ratio, size of digestive gland and growth rate for krill, and recruitment for the biomass-dominant calanoid copepods Calanoides acutus and Calanus propinquus. These indices consistently point to blooms in the MIZ as an important feeding ground for pelagic grazers. Even though <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_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_22 --> <div id="page_23" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="441"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C43B0756M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C43B0756M"><span>Laboratory Studies of Sea-<span class="hlt">Ice</span>-Wave Interactions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Monty, J.; Meylan, M. H.; Babanin, A. V.; Toffoli, A.; Bennetts, L.</p> <p>2016-12-01</p> <p>A world-first facility for studying the <span class="hlt">Marginal</span> <span class="hlt">Ice</span> Zone has been constructed in the Michell Hydrodynamics Laboratory at the University of Melbourne. A 14m long wave tank (0.75m wide, 0.6m deep) resides in a freezer, where air temperature can be controlled down to -15C. This permits the freezing of the water surface. Large stainless steel <span class="hlt">ice</span>-making trays (up to 4 m long) are also available to create <span class="hlt">ice</span> of desired thickness and microstructure, which can be lowered onto the water surface. A computer controlled wave generator is capable of creating waves of any desired form. The temperature of the water in the tank can also be controlled between 2 and 30C. The tank frame is constructed of marine-treated wood and the entire tank is glass and acrylic, permitting the use of corrosive fluids, such as salt water. Here we present the first laboratory experiments of break-up of a controlled thickness, fresh water <span class="hlt">ice</span> sheet impacted by regular and JONSWAP spectrum surface waves. The geometry of the resultant <span class="hlt">ice</span>-floes is measured with high-resolution, time-resolved imaging, providing the crucial data of floe size distribution. Initial observations show that, in the case of high steepness waves, the primary mechanisms of <span class="hlt">ice</span> break-up at the <span class="hlt">ice</span> edge are overwash and rafting, both of which put weight on the <span class="hlt">ice</span> interior to the <span class="hlt">ice</span>-water interface. This additional weight (and impact in the case of rafting) breaks more <span class="hlt">ice</span>, which allows overwash and rafting deeper into the <span class="hlt">ice</span> sheet, breaking more <span class="hlt">ice</span> and so on. For lower steepness waves, overwash and rafting are still present but far less significant. Finally, results of vertical <span class="hlt">ice</span> movement using laser height gauges will be presented showing the attenuation of waves into an <span class="hlt">ice</span> sheet and through a pack of <span class="hlt">ice</span> floes. These results are compared with field data and theory available (e.g. Squire & Moore, Nature, 1980 and Kohout et al., Nature, 2014).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29515117','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29515117"><span><span class="hlt">Ice</span>-volume-forced erosion of the Chinese Loess Plateau global Quaternary stratotype site.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Stevens, T; Buylaert, J-P; Thiel, C; Újvári, G; Yi, S; Murray, A S; Frechen, M; Lu, H</p> <p>2018-03-07</p> <p>The International Commission on Stratigraphy (ICS) utilises benchmark chronostratigraphies to divide geologic time. The reliability of these records is fundamental to understand past global change. Here we use the most detailed luminescence dating age model yet published to show that the ICS chronology for the Quaternary terrestrial type section at Jingbian, desert <span class="hlt">marginal</span> Chinese Loess Plateau, is inaccurate. There are large hiatuses and depositional changes expressed across a dynamic gully landform at the site, which demonstrates rapid environmental shifts at the East Asian desert <span class="hlt">margin</span>. We propose a new independent age model and reconstruct monsoon climate and desert expansion/contraction for the last ~250 ka. Our record demonstrates the dominant influence of <span class="hlt">ice</span> volume on desert expansion, dust dynamics and sediment preservation, and further shows that East Asian Summer Monsoon (EASM) variation closely matches that of <span class="hlt">ice</span> volume, but lags insolation by ~5 ka. These observations show that the EASM at the monsoon <span class="hlt">margin</span> does not respond directly to precessional forcing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16347871','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16347871"><span>Diel Variation in Population Size and <span class="hlt">Ice</span> Nucleation <span class="hlt">Activity</span> of Pseudomonas syringae on Snap Bean Leaflets.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hirano, S S; Upper, C D</p> <p>1989-03-01</p> <p>The extent to which diel changes in the physical environment affect changes in population size and <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> of Pseudomonas syringae on snap bean leaflets was determined under field conditions. To estimate bacterial population size and <span class="hlt">ice</span> nucleation <span class="hlt">activity</span>, bean leaflets were harvested at 2-h intervals during each of three 26-h periods. A tube nucleation test was used to assay individual leaflets for <span class="hlt">ice</span> nuclei. Population sizes of P. syringae were determined by dilution plating of leaflet homogenates. The overall diel changes in P. syringae population sizes differed during each of the 26-h periods. In one 26-h period, there was a continuous increase in the logarithm of P. syringae population size despite intense solar radiation, absence of free moisture on leaf surfaces, and low relative humidity during the day. A mean doubling time of approximately 4.9 h was estimated for the 28-fold increase in P. syringae population size that occurred from 0900 to 0900 h during the 26-h period. However, doubling times of 3.3 and 1.9 h occurred briefly during this period from 1700 to 2300 h and from 0100 to 0700 h, respectively. Thus, growth rates of P. syringae in association with leaves in the field were of the same order of magnitude as optimal rates measured in the laboratory. The frequency with which leaflets bore <span class="hlt">ice</span> nuclei <span class="hlt">active</span> at -2.0, -2.2, and -2.5 degrees C varied greatly within each 26-h period. These large diel changes were inversely correlated primarily with the diel changes in air temperature and reflected changes in nucleation frequency rather than changes in population size of P. syringae. Thus, the response of bacterial <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> to the physical environment was distinct from the changes in population size of <span class="hlt">ice</span> nucleation-<span class="hlt">active</span> P. syringae.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSHE24A1425S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSHE24A1425S"><span>Maiden Voyage of the Under-<span class="hlt">Ice</span> Float</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shcherbina, A.; D'Asaro, E. A.; Light, B.; Deming, J. W.; Rehm, E.</p> <p>2016-02-01</p> <p>The Under-<span class="hlt">Ice</span> Float (UIF) is a new autonomous platform for sea <span class="hlt">ice</span> and upper ocean observations in the <span class="hlt">marginal</span> <span class="hlt">ice</span> zone (MIZ). UIF is based on the Mixed Layer Lagrangian Float design, inheriting its accurate buoyancy control and relatively heavy payload capability. A major challenge for sustained autonomous observations in the MIZ is detection of open water for navigation and telemetry surfacings. UIF employs the new surface classification algorithm based on the spectral analysis of surface roughness sensed by an upward-looking sonar. A prototype UIF was deployed in the MIZ of the central Arctic Ocean in late August 2015. The main payload of the first UIF was a bio-optical suit consisting of upward- and downward hyperspectral radiometers; temperature, salinity, chlorophyll, turbidity, and dissolved oxygen sensors, and a high-definition photo camera. In the early stages of its mission, the float successfully avoided <span class="hlt">ice</span>, detected leads, surfaced in open water, and transmitted data and photographs. We will present the analysis of these observations from the full UIF mission extending into the freeze-up season.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011MsT.........18M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011MsT.........18M"><span>Quantification of Changes for the Milne <span class="hlt">Ice</span> Shelf, Nunavut, Canada, 1950 -- 2009</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mortimer, Colleen Adel</p> <p></p> <p>This study presents a comprehensive overview of the current state of the Milne <span class="hlt">Ice</span> Shelf and how it has changed over the last 59 years. The 205 +/-1 km2 <span class="hlt">ice</span> shelf experienced a 28% (82 +/-0.8 km 2) reduction in area between 1950 -- 2009, and a 20% (2.5 +/-0.9km 3 water equivalent (w.e.)) reduction in volume between 1981 -- 2008/2009, suggesting a long-term state of negative mass balance. Comparison of mean annual specific mass balances (up to -0.34 m w.e. yr-1) with surface mass balance measurements for the nearby Ward Hunt <span class="hlt">Ice</span> Shelf suggest that basal melt is a key contributor to total <span class="hlt">ice</span> shelf thinning. The development and expansion of new and existing surface cracks, as well as <span class="hlt">ice-marginal</span> and epishelf lake development, indicate significant <span class="hlt">ice</span> shelf weakening. Over the next few decades it is likely that the Milne <span class="hlt">Ice</span> Shelf will continue to deteriorate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014ESSDD...7..419L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014ESSDD...7..419L"><span>Sea <span class="hlt">ice</span> in the Baltic Sea - revisiting BASIS <span class="hlt">ice</span>, a~historical data set covering the period 1960/1961-1978/1979</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Löptien, U.; Dietze, H.</p> <p>2014-06-01</p> <p>The Baltic Sea is a seasonally <span class="hlt">ice</span>-covered, <span class="hlt">marginal</span> sea, situated in central northern Europe. It is an essential waterway connecting highly industrialised countries. Because ship traffic is intermittently hindered by sea <span class="hlt">ice</span>, the local weather services have been monitoring sea <span class="hlt">ice</span> conditions for decades. In the present study we revisit a historical monitoring data set, covering the winters 1960/1961. This data set, dubbed Data Bank for Baltic Sea <span class="hlt">Ice</span> and Sea Surface Temperatures (BASIS) <span class="hlt">ice</span>, is based on hand-drawn maps that were collected and then digitised 1981 in a joint project of the Finnish Institute of Marine Research (today Finish Meteorological Institute (FMI)) and the Swedish Meteorological and Hydrological Institute (SMHI). BASIS <span class="hlt">ice</span> was designed for storage on punch cards and all <span class="hlt">ice</span> information is encoded by five digits. This makes the data hard to access. Here we present a post-processed product based on the original five-digit code. Specifically, we convert to standard <span class="hlt">ice</span> quantities (including information on <span class="hlt">ice</span> types), which we distribute in the current and free Network Common Data Format (NetCDF). Our post-processed data set will help to assess numerical <span class="hlt">ice</span> models and provide easy-to-access unique historical reference material for sea <span class="hlt">ice</span> in the Baltic Sea. In addition we provide statistics showcasing the data quality. The website <a href="www.baltic-ocean.org"target="_blank">www.baltic-ocean.org<a/> hosts the post-prossed data and the conversion code. The data are also archived at the Data Publisher for Earth & Environmental Science PANGEA (<a href="http://dx.doi.org/"target="_blank">doi:10.1594/PANGEA.832353<a/>).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19801462','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19801462"><span>Low salinity and high-level UV-B radiation reduce single-cell <span class="hlt">activity</span> in antarctic sea <span class="hlt">ice</span> bacteria.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Martin, Andrew; Hall, Julie; Ryan, Ken</p> <p>2009-12-01</p> <p>Experiments simulating the sea <span class="hlt">ice</span> cycle were conducted by exposing microbes from Antarctic fast <span class="hlt">ice</span> to saline and irradiance regimens associated with the freeze-thaw process. In contrast to hypersaline conditions (<span class="hlt">ice</span> formation), the simulated release of bacteria into hyposaline seawater combined with rapid exposure to increased UV-B radiation significantly reduced metabolic <span class="hlt">activity</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPA13C0243T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPA13C0243T"><span>The practicality of defensive <span class="hlt">ice</span> walls: How would the great <span class="hlt">ice</span> wall in Game of Thrones hold up?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Truffer, M.</p> <p>2017-12-01</p> <p>The Game of Thrones great <span class="hlt">ice</span> wall is a colossal feature stretching several hundred miles and over 200 m high. Its purpose is to defend the realm from the wildlings. It is generally pictured as a near vertical wall. An <span class="hlt">ice</span> wall of these proportions poses interesting challenges, mainly because <span class="hlt">ice</span> acts as a non-linear shear-thinning fluid. A 200 m high vertical wall would create a large effective stress near its base of almost 1.8 MPa. Typical stresses responsible for <span class="hlt">ice</span> flow in glaciers and <span class="hlt">ice</span> sheets are more than a magnitude lower (0.1 MPa). Extrapolating a commonly used flow law for temperate <span class="hlt">ice</span> to such high stresses would lead to strain rates at the bottom of the wall in excess of 1/day, meaning the wall would rapidly collapse and spread laterally under its own weight. To keep the wall stable, it would help to cool it significantly, as the flow of <span class="hlt">ice</span> is also very temperature dependent. Cooling to a chilly -40 C would reduce strain rates by two orders of magnitude, but this still leads to significant slumping of the wall within just a few weeks. A time-dependent similarity solution for simplified <span class="hlt">ice</span> flow equations that describe the evolving shape of the <span class="hlt">ice</span> wall was provided by Halfar (1981), and demonstrates the rapid decay of the wall. A simple estimate can be derived by assuming that <span class="hlt">ice</span> is a perfectly plastic fluid, able to maintain a basal shear stress of about 0.1 MPa. A stable <span class="hlt">ice</span> wall would then spread laterally to about 4 km width. The resulting slope would only be steep at the very <span class="hlt">margin</span> and the <span class="hlt">ice</span> wall would loose much of its defensive capabilities. I conclude that the <span class="hlt">ice</span> wall as proposed would not be a practicable defense under typical Earth conditions, and special magical powers would be necessary to maintain its shape, even for just a few days.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20050139766&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=20050139766&hterms=balance+sheet&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dbalance%2Bsheet"><span>Recent Observations of Increased Thinning of the Greenland <span class="hlt">Ice</span> Sheet Measured by Aircraft GPS and Laser Altimetry</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Krabill, William B.</p> <p>2004-01-01</p> <p>The Arctic <span class="hlt">Ice</span> Mapping group (Project AIM) at the NASA Goddard Space Flight Center Wallops Flight Facility has been conducting systematic topographic surveys of the Greenland <span class="hlt">Ice</span> Sheet (GIs) since 1993, using scanning airborne laser altimeters combined with Global Positioning System (GPS) technology onboard NASA's P-3 aircraft. Flight lines have covered all major <span class="hlt">ice</span> drainage basins, with repeating surveys after a 5-year interval during the decade of the 90's. Analysis of this data documented significant thinning in many areas near the <span class="hlt">ice</span> sheet <span class="hlt">margins</span> and an overall negative mass balance of the GIS (Science, 2000). In 2001, 2002, and 2003 many of these flight lines were re-surveyed, providing evidence of continued or accelerated thinning in all observed areas around the <span class="hlt">margin</span> of the GIs. Additionally, however, a highly-anomalous snowfall was observed between 2002 and 2003 in SE Greenland - perhaps an indicator of a shift in the regional climate?</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.B44B..03C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.B44B..03C"><span>Quantifying ocean and <span class="hlt">ice</span> sheet contributions to nutrient fluxes in Sermilik Fjord, Southeast Greenland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cape, M. R.; Straneo, F.; Beaird, N.; Bundy, R.; Charette, M. A.</p> <p>2016-12-01</p> <p>Meltwater discharged at the <span class="hlt">margins</span> of the Greenland <span class="hlt">Ice</span> Sheet (GrIS) represents a potential source of nutrients to biological communities downstream. In Greenland's glacial fjords, this discharge occurs at depth below and along the face of deeply grounded marine-terminating glaciers. This process drives vigorous circulation and mixing between melt and ambient waters at the <span class="hlt">ice</span>-ocean <span class="hlt">margins</span>, giving rise to a new glacially modified water mass (GMW) which constitutes the primary vehicle for transport of meltwater in the marine environment. While previous field studies have noted nutrient enrichment in GMW with respect to unmodified waters along the shelf, the source of this enrichment, whether due to entrainment of deep ambient waters or input by meltwater, remains poorly understood. This knowledge is however critical in order to evaluate the current and future contributions of the GrIS to marine biogeochemical cycling. Here we shed light on the distribution, composition, and properties of GMW along the GrIS <span class="hlt">margin</span> by analyzing integrated physical and chemical measurements collected in August 2015 in Sermilik Fjord, a major glacial freshwater export pathway. Our results document up to a doubling of nutrient concentrations (nitrate, silicate, phosphate, and iron) in GMW, which is distributed in the top 300 m of the water column throughout the fjord. Partitioning of ocean and <span class="hlt">ice</span> sheet contributions to GMW nutrient load demonstrates that upwelled waters are the primary source of macro-nutrients to GMW. We expand on these results to discuss the magnitude of fluxes in context of previous observations along the GrIS <span class="hlt">margins</span>, export pathways of GMW to the shelf, and knowledge gaps needed to be addressed to better constrain <span class="hlt">ice</span> sheet contributions to marine ecosystem processes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013BGeo...10.8083P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013BGeo...10.8083P"><span>Spores of many common airborne fungi reveal no <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> in oil immersion freezing experiments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pummer, B. G.; Atanasova, L.; Bauer, H.; Bernardi, J.; Druzhinina, I. S.; Fröhlich-Nowoisky, J.; Grothe, H.</p> <p>2013-12-01</p> <p>Fungal spores are ubiquitous biological aerosols, which are considered to act as <span class="hlt">ice</span> nuclei. In this study the <span class="hlt">ice</span> nucleation (IN) <span class="hlt">activity</span> of spores harvested from 29 fungal strains belonging to 21 different species was tested in the immersion freezing mode by microscopic observation of water-in-oil emulsions. Spores of 8 of these strains were also investigated in a microdroplet freezing array instrument. The focus was laid on species of economical, ecological or sanitary significance. Besides common molds (Ascomycota), some representatives of the widespread group of mushrooms (Basidiomycota) were also investigated. Fusarium avenaceum was the only sample showing IN <span class="hlt">activity</span> at relatively high temperatures (about 264 K), while the other investigated fungal spores showed no freezing above 248 K. Many of the samples indeed froze at homogeneous <span class="hlt">ice</span> nucleation temperatures (about 237 K). In combination with other studies, this suggests that only a limited number of species may act as atmospheric <span class="hlt">ice</span> nuclei. This would be analogous to what is already known for the bacterial <span class="hlt">ice</span> nuclei. Apart from that, we selected a set of fungal strains from different sites and exposed them to occasional freezing stress during their cultivation. This was in order to test if the exposure to a cold environment encourages the expression of <span class="hlt">ice</span> nuclei during growth as a way of adaptation. Although the total protein expression was altered by this treatment, it had no significant impact on the IN <span class="hlt">activity</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19880003322','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19880003322"><span>Analysis of the <span class="hlt">ICE</span> combiner for multiple antenna arraying</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Foster, C.; Marina, M.</p> <p>1987-01-01</p> <p>The passage of the International Cometary Explorer (<span class="hlt">ICE</span>) through the tail of comet Giacobini-Zinner took place on September 11, 1985, at approximately 11:04 GMT. The signal-to-noise ratio of the data received from the <span class="hlt">ICE</span> spacecraft during the comet encounter was improved by arraying the 64-m antenna channels A and B (RCP and LCP) with the two 34-m antennas. Specially designed combiners were built to combine the signals received by the three antennas at the different DSN sites to ensure that the spacecraft's weak signal was received. Although the <span class="hlt">ICE</span> spacecraft was built with a 5-W transmitter and with a small antenna designed to provide data from no farther than 1 million miles, these combiners provided enough signal <span class="hlt">margin</span> during the encounter to receive the <span class="hlt">ICE</span> transmitted data from within the tail of comet Giacobini-Zinner, 44 million miles from earth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20070035024','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20070035024"><span>Arctic Sea <span class="hlt">Ice</span> Parameters from AMSR-E Data using Two Techniques, and Comparisons with Sea <span class="hlt">Ice</span> from SSM</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.; Parkinson, Claire L.</p> <p>2007-01-01</p> <p>We use two algorithms to process AMSR-E data in order to determine algorithm dependence, if any, on the estimates of sea <span class="hlt">ice</span> concentration, <span class="hlt">ice</span> extent and area, and trends and to evaluate how AMSR-E data compare with historical SSM/I data. The monthly <span class="hlt">ice</span> concentrations derived from the two algorithms from AMSR-E data (the AMSR-E Bootstrap Algorithm, or ABA, and the enhanced NASA Team algorithm, or NT2) differ on average by about 1 to 3%, with data from the consolidated <span class="hlt">ice</span> region being generally comparable for ABA and NT2 retrievals while data in the <span class="hlt">marginal</span> <span class="hlt">ice</span> zones and thin <span class="hlt">ice</span> regions show higher values when the NT2 algorithm is used. The <span class="hlt">ice</span> extents and areas derived separately from AMSR-E using these two algorithms are, however, in good agreement, with the differences (ABA-NT2) being about 6.6 x 10(exp 4) square kilometers on average for <span class="hlt">ice</span> extents and -6.6 x 10(exp 4) square kilometers for <span class="hlt">ice</span> area which are small compared to mean seasonal values of 10.5 x 10(exp 6) and 9.8 x 10(exp 6) for <span class="hlt">ice</span> extent and area: respectively. Likewise, extents and areas derived from the same algorithm but from AMSR-E and SSM/I data are consistent but differ by about -24.4 x 10(exp 4) square kilometers and -13.9 x 10(exp 4) square kilometers, respectively. The discrepancies are larger with the estimates of extents than area mainly because of differences in channel selection and sensor resolutions. Trends in extent during the AMSR-E era were also estimated and results from all three data sets are shown to be in good agreement (within errors).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/fs/2012/3131/pdf/fs20123131.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/fs/2012/3131/pdf/fs20123131.pdf"><span>Polar bear and walrus response to the rapid decline in Arctic sea <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>Oakley, K.; Whalen, M.; Douglas, David C.; Udevitz, Mark S.; Atwood, Todd C.; Jay, C.</p> <p>2012-01-01</p> <p>The Arctic is warming faster than other regions of the world due to positive climate feedbacks associated with loss of snow and <span class="hlt">ice</span>. One highly visible consequence has been a rapid decline in Arctic sea <span class="hlt">ice</span> over the past 3 decades - a decline projected to continue and result in <span class="hlt">ice</span>-free summers likely as soon as 2030. The polar bear (Ursus maritimus) and the Pacific walrus (Odobenus rosmarus divergens) are dependent on sea <span class="hlt">ice</span> over the continental shelves of the Arctic Ocean's <span class="hlt">marginal</span> seas. The continental shelves are shallow regions with high biological productivity, supporting abundant marine life within the water column and on the sea floor. Polar bears use sea <span class="hlt">ice</span> as a platform for hunting <span class="hlt">ice</span> seals; walruses use sea <span class="hlt">ice</span> as a resting platform between dives to forage for clams and other bottom-dwelling invertebrates. How have sea <span class="hlt">ice</span> changes affected polar bears and walruses? How will anticipated changes affect them in the future?</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150014255','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150014255"><span>Sustained High Basal Motion of the Greenland <span class="hlt">Ice</span> Sheet Revealed by Borehole Deformation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ryser, Claudia; Luthi, Martin P.; Andrews, Lauren C.; Hoffman, Matthew, J.; Catania, Ginny A.; Hawley, Robert L.; Neumann, Thomas A.; Kristensen, Steen S.</p> <p>2014-01-01</p> <p><span class="hlt">Ice</span> deformation and basal motion characterize the dynamical behavior of the Greenland <span class="hlt">ice</span> sheet (GrIS). We evaluate the contribution of basal motion from <span class="hlt">ice</span> deformation measurements in boreholes drilled to the bed at two sites in the western <span class="hlt">marginal</span> zone of the GrIS. We find a sustained high amount of basal motion contribution to surface velocity of 44-73 percent in winter, and up to 90 percent in summer. Measured <span class="hlt">ice</span> deformation rates show an unexpected variation with depth that can be explained with the help of an <span class="hlt">ice</span>-flow model as a consequence of stress transfer from slippery to sticky areas. This effect necessitates the use of high-order <span class="hlt">ice</span>-flow models, not only in regions of fast-flowing <span class="hlt">ice</span> streams but in all temperate-based areas of the GrIS. The agreement between modeled and measured deformation rates confirms that the recommended values of the temperature-dependent flow rate factor A are a good choice for <span class="hlt">ice</span>-sheet models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.C41D..08M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.C41D..08M"><span>Ocean wave generation by collapsing <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>Macayeal, D. R.; Bassis, J. N.; Okal, E. A.; Aster, R. C.; Cathles, L. M.</p> <p>2008-12-01</p> <p>The 28-29 February, 2008, break-up of the Wilkins <span class="hlt">Ice</span> Shelf, Antarctica, exemplifies the now-familiar, yet largely unexplained pattern of explosive <span class="hlt">ice</span>-shelf break-up. While environmental warming is a likely ultimate cause of explosive break-up, several key aspects of their short-term behavior need to be explained: (1) The abrupt, near-simultaneous onset of iceberg calving across long spans of the <span class="hlt">ice</span> front <span class="hlt">margin</span>; (2) High outward drift velocity (about 0.3 m/s) of a leading phalanx of tabular icebergs that originate from the seaward edge of the intact <span class="hlt">ice</span> shelf prior to break-up; (3) Rapid coverage of the ocean surface in the wake of this leading phalanx by small, capsized and dismembered tabular icebergs; (4) Extremely large gravitational potential energy release rates, e.g., up to 3 × 1010 W; (5) Lack of proximal iceberg-calving triggers that control the timing of break-up onset and that maintain the high break-up calving rates through to the conclusion of the event. Motivated by seismic records obtained from icebergs and the Ross <span class="hlt">Ice</span> Shelf that show hundreds of micro- tsunamis emanating from near the <span class="hlt">ice</span> shelf front, we re-examine the basic dynamic features of <span class="hlt">ice</span>- shelf/ocean-wave interaction and, in particular, examine the possibility that collapsing <span class="hlt">ice</span> shelves themselves are a source of waves that stimulate the disintegration process. We propose that <span class="hlt">ice</span>-shelf generated surface-gravity waves associated with initial calving at an arbitrary seed location produce stress perturbations capable of triggering the onset of calving on the entire <span class="hlt">ice</span> front. Waves generated by parting detachment rifts, iceberg capsize and break-up act next to stimulate an inverted submarine landslide (<span class="hlt">ice</span>- slide) process, where gravitational potential energy released by upward movement of buoyant <span class="hlt">ice</span> is radiated as surface gravity waves in the wake of the advancing phalanx of tabular icebergs. We conclude by describing how field research and remote sensing can be used to test the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014ACPD...1417359D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014ACPD...1417359D"><span>Integrating laboratory and field data to quantify the immersion freezing <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> of mineral dust particles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>DeMott, P. J.; Prenni, A. J.; McMeeking, G. R.; Sullivan, R. C.; Petters, M. D.; Tobo, Y.; Niemand, M.; Möhler, O.; Snider, J. R.; Wang, Z.; Kreidenweis, S. M.</p> <p>2014-06-01</p> <p>Data from both laboratory studies and atmospheric measurements are used to develop a simple parametric description for the immersion freezing <span class="hlt">activity</span> of natural mineral dust particles. Measurements made with the Colorado State University (CSU) continuous flow diffusion chamber (CFDC) when processing mineral dust aerosols at a nominal 105% relative humidity with respect to water (RHw) are taken to approximate the immersion freezing nucleation <span class="hlt">activity</span> of particles. <span class="hlt">Ice</span> <span class="hlt">active</span> frozen fractions vs. temperature for dusts representative of Saharan and Asian desert sources were consistent with similar measurements in atmospheric dust plumes for a limited set of comparisons available. The parameterization developed follows the form of one suggested previously for atmospheric particles of non-specific composition in quantifying <span class="hlt">ice</span> nucleating particle concentrations as functions of temperature and the total number concentration of particles larger than 0.5 μm diameter. Such an approach does not explicitly account for surface area and time dependencies for <span class="hlt">ice</span> nucleation, but sufficiently encapsulates the <span class="hlt">activation</span> properties for potential use in regional and global modeling simulations, and possible application in developing remote sensing retrievals for <span class="hlt">ice</span> nucleating particles. A correction factor is introduced to account for the apparent underestimate (by approximately 3, on average) of the immersion freezing fraction of mineral dust particles for CSU CFDC data processed at an RHw of 105% vs. maximum fractions <span class="hlt">active</span> at higher RHw. Instrumental factors that affect <span class="hlt">activation</span> behavior vs. RHw in CFDC instruments remain to be fully explored in future studies. Nevertheless, the use of this correction factor is supported by comparison to <span class="hlt">ice</span> <span class="hlt">activation</span> data obtained for the same aerosols from Aerosol Interactions and Dynamics of the Atmosphere (AIDA) expansion chamber cloud parcel experiments. Further comparison of the new parameterization to the immersion freezing</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015ACP....15..393D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015ACP....15..393D"><span>Integrating laboratory and field data to quantify the immersion freezing <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> of mineral dust particles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>DeMott, P. J.; Prenni, A. J.; McMeeking, G. R.; Sullivan, R. C.; Petters, M. D.; Tobo, Y.; Niemand, M.; Möhler, O.; Snider, J. R.; Wang, Z.; Kreidenweis, S. M.</p> <p>2015-01-01</p> <p>Data from both laboratory studies and atmospheric measurements are used to develop an empirical parameterization for the immersion freezing <span class="hlt">activity</span> of natural mineral dust particles. Measurements made with the Colorado State University (CSU) continuous flow diffusion chamber (CFDC) when processing mineral dust aerosols at a nominal 105% relative humidity with respect to water (RHw) are taken as a measure of the immersion freezing nucleation <span class="hlt">activity</span> of particles. <span class="hlt">Ice</span> <span class="hlt">active</span> frozen fractions vs. temperature for dusts representative of Saharan and Asian desert sources were consistent with similar measurements in atmospheric dust plumes for a limited set of comparisons available. The parameterization developed follows the form of one suggested previously for atmospheric particles of non-specific composition in quantifying <span class="hlt">ice</span> nucleating particle concentrations as functions of temperature and the total number concentration of particles larger than 0.5 μm diameter. Such an approach does not explicitly account for surface area and time dependencies for <span class="hlt">ice</span> nucleation, but sufficiently encapsulates the <span class="hlt">activation</span> properties for potential use in regional and global modeling simulations, and possible application in developing remote sensing retrievals for <span class="hlt">ice</span> nucleating particles. A calibration factor is introduced to account for the apparent underestimate (by approximately 3, on average) of the immersion freezing fraction of mineral dust particles for CSU CFDC data processed at an RHw of 105% vs. maximum fractions <span class="hlt">active</span> at higher RHw. Instrumental factors that affect <span class="hlt">activation</span> behavior vs. RHw in CFDC instruments remain to be fully explored in future studies. Nevertheless, the use of this calibration factor is supported by comparison to <span class="hlt">ice</span> <span class="hlt">activation</span> data obtained for the same aerosols from Aerosol Interactions and Dynamics of the Atmosphere (AIDA) expansion chamber cloud parcel experiments. Further comparison of the new parameterization, including calibration</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990064613&hterms=Parkinsons&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DParkinsons','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990064613&hterms=Parkinsons&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DParkinsons"><span>Variability of Arctic Sea <span class="hlt">Ice</span> as Determined from Satellite Observations</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>1999-01-01</p> <p>The compiled, quality-controlled satellite multichannel passive-microwave record of polar sea <span class="hlt">ice</span> now spans over 18 years, from November 1978 through December 1996, and is revealing considerable information about the Arctic sea <span class="hlt">ice</span> cover and its variability. The information includes data on <span class="hlt">ice</span> concentrations (percent areal coverages of <span class="hlt">ice</span>), <span class="hlt">ice</span> extents, <span class="hlt">ice</span> melt, <span class="hlt">ice</span> velocities, the seasonal cycle of the <span class="hlt">ice</span>, the interannual variability of the <span class="hlt">ice</span>, the frequency of <span class="hlt">ice</span> coverage, and the length of the sea <span class="hlt">ice</span> season. The data reveal marked regional and interannual variabilities, as well as some statistically significant trends. For the north polar <span class="hlt">ice</span> cover as a whole, maximum <span class="hlt">ice</span> extents varied over a range of 14,700,000 - 15,900,000 sq km, while individual regions experienced much greater percent variations, for instance, with the Greenland Sea having a range of 740,000 - 1,110,000 sq km in its yearly maximum <span class="hlt">ice</span> coverage. In spite of the large variations from year to year and region to region, overall the Arctic <span class="hlt">ice</span> extents showed a statistically significant, 2.80% / decade negative trend over the 18.2-year period. <span class="hlt">Ice</span> season lengths, which vary from only a few weeks near the <span class="hlt">ice</span> <span class="hlt">margins</span> to the full year in the large region of perennial <span class="hlt">ice</span> coverage, also experienced interannual variability, along with spatially coherent overall trends. Linear least squares trends show the sea <span class="hlt">ice</span> season to have lengthened in much of the Bering Sea, Baffin Bay, the Davis Strait, and the Labrador Sea, but to have shortened over a much larger area, including the Sea of Okhotsk, the Greenland Sea, the Barents Sea, and the southeastern Arctic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014GeoRL..41.1035T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014GeoRL..41.1035T"><span>Seasonal to interannual Arctic sea <span class="hlt">ice</span> predictability in current 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>Tietsche, S.; Day, J. J.; Guemas, V.; Hurlin, W. J.; Keeley, S. P. E.; Matei, D.; Msadek, R.; Collins, M.; Hawkins, E.</p> <p>2014-02-01</p> <p>We establish the first intermodel comparison of seasonal to interannual predictability of present-day Arctic climate by performing coordinated sets of idealized ensemble predictions with four state-of-the-art global climate models. For Arctic sea <span class="hlt">ice</span> extent and volume, there is potential predictive skill for lead times of up to 3 years, and potential prediction errors have similar growth rates and magnitudes across the models. Spatial patterns of potential prediction errors differ substantially between the models, but some features are robust. Sea <span class="hlt">ice</span> concentration errors are largest in the <span class="hlt">marginal</span> <span class="hlt">ice</span> zone, and in winter they are almost zero away from the <span class="hlt">ice</span> edge. Sea <span class="hlt">ice</span> thickness errors are amplified along the coasts of the Arctic Ocean, an effect that is dominated by sea <span class="hlt">ice</span> advection. These results give an upper bound on the ability of current global climate models to predict important aspects of Arctic climate.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_23 --> <div id="page_24" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="461"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999PalOc..14..211K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999PalOc..14..211K"><span>Mid-Wisconsin Laurentide <span class="hlt">Ice</span> Sheet growth and decay: Implications for Heinrich events 3 and 4</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kirby, Matthew E.; Andrews, John T.</p> <p>1999-04-01</p> <p>A close look at the sedimentology of Heinrich event 4 from the northwest Labrador Sea indicates that an extended <span class="hlt">ice</span> <span class="hlt">margin</span>, perhaps greater than before Heinrich events 1 or 2 (H-1 and H-2), existed in the Hudson Strait region pre-Heinrich event 4 (H-4) and, that on the basis of characteristics of the sediment unit, Heinrich event-4 was different than Heinrich events 1 or 2 (i.e., larger <span class="hlt">ice</span> sheet collapse(?), longer duration(?), "dirtier" icebergs(?)). Other data from across the southern and eastern <span class="hlt">margin</span> of the Laurentide <span class="hlt">Ice</span> Sheet, as well as Greenland and the North Atlantic, support this interpretation, possibly indicating a relative mid-Wisconsin glacial maximum pre-Heinrich event 4. Many of these data also indicate that Heinrich event 4 (35 ka) resulted in serious climatic and oceanographic reorganizations. We suggest that Heinrich event 4 gutted the Hudson Strait, leaving it devoid of <span class="hlt">ice</span> for Heinrich event 3. We further hypothesize that Heinrich event 3 did not originate from axial <span class="hlt">ice</span> transport along the Hudson Strait; thus Heinrich event 3 may be more analogous to the proposed northward advancing <span class="hlt">ice</span> from Ungava Bay during Heinrich event 0 than to the more typical down-the-strait flow during H-1, H-2, and H-4. Consequently, the climatic and oceanographic impacts resulting from Heinrich events are highly susceptible to the type, origin, and magnitude of <span class="hlt">ice</span> sheet collapse, something which varied per Heinrich event during the last glacial period.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2014-title14-vol3/pdf/CFR-2014-title14-vol3-sec121-321.pdf','CFR2014'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2014-title14-vol3/pdf/CFR-2014-title14-vol3-sec121-321.pdf"><span>14 CFR 121.321 - Operations in <span class="hlt">icing</span>.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2014&page.go=Go">Code of Federal Regulations, 2014 CFR</a></p> <p></p> <p>2014-01-01</p> <p>.... (1) The airplane must be equipped with a certificated primary airframe <span class="hlt">ice</span> detection system. (i) The airframe <span class="hlt">ice</span> protection system must be <span class="hlt">activated</span> automatically, or manually by the flightcrew, when the primary <span class="hlt">ice</span> detection system indicates <span class="hlt">activation</span> is necessary. (ii) When the airframe <span class="hlt">ice</span> protection...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMOS23E..04C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMOS23E..04C"><span>Tracking small mountainous river derived terrestrial organic carbon across the <span class="hlt">active</span> <span class="hlt">margin</span> marine environment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Childress, L. B.; Blair, N. E.; Orpin, A. R.</p> <p>2015-12-01</p> <p><span class="hlt">Active</span> <span class="hlt">margins</span> are particularly efficient in the burial of organic carbon due to the close proximity of highland sources to marine sediment sinks and high sediment transport rates. Compared with passive <span class="hlt">margins</span>, <span class="hlt">active</span> <span class="hlt">margins</span> are dominated by small mountainous river systems, and play a unique role in marine and global carbon cycles. Small mountainous rivers drain only approximately 20% of land, but deliver approximately 40% of the fluvial sediment to the global ocean. Unlike large passive <span class="hlt">margin</span> systems where riverine organic carbon is efficiently incinerated on continental shelves, small mountainous river dominated systems are highly effective in the burial and preservation of organic carbon due to the rapid and episodic delivery of organic carbon sourced from vegetation, soil, and rock. To investigate the erosion, transport, and burial of organic carbon in <span class="hlt">active</span> <span class="hlt">margin</span> small mountainous river systems we use the Waipaoa River, New Zealand. The Waipaoa River, and adjacent marine depositional environment, is a system of interest due to a large sediment yield (6800 tons km-2 yr-1) and extensive characterization. Previous studies have considered the biogeochemistry of the watershed and tracked the transport of terrestrially derived sediment and organics to the continental shelf and slope by biogeochemical proxies including stable carbon isotopes, lignin phenols, n-alkanes, and n-fatty acids. In this work we expand the spatial extent of investigation to include deep sea sediments of the Hikurangi Trough. Located in approximately 3000 m water depth 120 km from the mouth of the Waipaoa River, the Hikurangi Trough is the southern extension of the Tonga-Kermadec-Hikurangi subduction system. Piston core sediments collected by the National Institute of Water and Atmospheric Research (NIWA, NZ) in the Hikurangi Trough indicate the presence of terrestrially derived material (lignin phenols), and suggest a continuum of deposition, resuspension, and transport across the <span class="hlt">margin</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1991JGR....96.4531F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1991JGR....96.4531F"><span>Strain in shore fast <span class="hlt">ice</span> due to incoming ocean waves and swell</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fox, Colin; Squire, Vernon A.</p> <p>1991-03-01</p> <p>Using a development from the theoretical model presented by Fox and Squire (1990), this paper investigates the strain field generated in shore fast <span class="hlt">ice</span> by normally incident ocean waves and swell. After a brief description of the model and its convergence, normalized absolute strain (relative to a 1-m incident wave) is found as a function of distance from the <span class="hlt">ice</span> edge for various wave periods, <span class="hlt">ice</span> thicknesses, and water depths. The squared transfer function, giving the relative ability of incident waves of different periods to generate strain in the <span class="hlt">ice</span>, is calculated, and its consequences are discussed. The <span class="hlt">ice</span> is then forced with a Pierson-Moskowitz spectrum, and the consequent strain spectra are plotted as a function of penetration into the <span class="hlt">ice</span> sheet. Finally, rms strain, computed as the incoherent sum of the strains resulting from energy in the open water spectrum, is found. The results have implications to the breakup of shore fast <span class="hlt">ice</span> and hence to the floe size distribution of the <span class="hlt">marginal</span> <span class="hlt">ice</span> zone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP21E..05Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP21E..05Y"><span>Heinrich events and sea level changes: records from uplifted coral terraces and <span class="hlt">marginal</span> seas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yokoyama, Y.; Esat, T. M.; Suga, H.; Obrochta, S.; Ohkouchi, N.</p> <p>2017-12-01</p> <p>Repeated major <span class="hlt">ice</span> discharge events spaced every ca.7,000 years during the last <span class="hlt">ice</span> age was first detected in deep sea sediments from North Atlantic. Characterized as lithic layers, these Heinrich Events (Heinrich, 1988 QR) correspond to rapid climate changes attributed to weakened ocean circulation (eg., Broecker, 1994 Nature; Alley, 1998 Nature) as shown by a number of different proxies. A better understanding of the overall picture of Heinrich events would benefit from determining the total amount of <span class="hlt">ice</span> involved each event, which is still under debate. Sea level records are the most direct means for that, and uranium series dated corals can constrain the timing precisely. However, averaged global sea level during the time of interest was around -70m, hindering study from tectonically stable regions. Using uplifted coral terraces that extend 80 km along the Huon Peninsula, Papua New Guinea, the magnitude of sea level change during Heinrich Events was successfully reconstructed (Yokoyama et al., 2001 EPSL; Chappell et al., 1996 EPSL; Cutler et al., 2003). The H3 and H5 events are also well correlated with continuous sea level reconstructions using Red Sea oxygen isotope records (Siddall et al., 2003 Nature; Yokoyama and Esat, 2011Oceanography). Global <span class="hlt">ice</span> sheet growth after 30 ka complicates interpretation of the Huon Peninsula record. However oxygen isotope data from the Japan Sea, a restricted <span class="hlt">margin</span> sea with a shallow sill depth similar to the Red Sea, clearly captures the episode of H2 sea level change. The timing of these sea level excursions correlate well to the DSDP Site 609 detrital layers that are anchored in the latest Greenland <span class="hlt">ice</span> core chronology (Obrochta et al., 2012 QSR). In the presentation, Antarctic <span class="hlt">ice</span> sheet behavior during the H2 event will also be discussed using <span class="hlt">marginal</span> seas oxygen records.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C24B..02K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C24B..02K"><span>C-band Joint <span class="hlt">Active</span>/Passive Dual Polarization Sea <span class="hlt">Ice</span> Detection</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Keller, M. R.; Gifford, C. M.; Winstead, N. S.; Walton, W. C.; Dietz, J. E.</p> <p>2017-12-01</p> <p>A technique for synergistically-combining high-resolution SAR returns with like-frequency passive microwave emissions to detect thin (<30 cm) <span class="hlt">ice</span> under the difficult conditions of late melt and freeze-up is presented. As the Arctic sea <span class="hlt">ice</span> cover thins and shrinks, the algorithm offers an approach to adapting existing sensors monitoring thicker <span class="hlt">ice</span> to provide continuing coverage. Lower resolution (10-26 km) <span class="hlt">ice</span> detections with spaceborne radiometers and scatterometers are challenged by rapidly changing thin <span class="hlt">ice</span>. Synthetic Aperture Radar (SAR) is high resolution (5-100m) but because of cross section ambiguities automated algorithms have had difficulty separating thin <span class="hlt">ice</span> types from water. The radiometric emissivity of thin <span class="hlt">ice</span> versus water at microwave frequencies is generally unambiguous in the early stages of <span class="hlt">ice</span> growth. The method, developed using RADARSAT-2 and AMSR-E data, uses higher-ordered statistics. For the SAR, the COV (coefficient of variation, ratio of standard deviation to mean) has fewer ambiguities between <span class="hlt">ice</span> and water than cross sections, but breaking waves still produce <span class="hlt">ice</span>-like signatures for both polarizations. For the radiometer, the PRIC (polarization ratio <span class="hlt">ice</span> concentration) identifies areas that are unambiguously water. Applying cumulative statistics to co-located COV levels adaptively determines an <span class="hlt">ice</span>/water threshold. Outcomes from extensive testing with Sentinel and AMSR-2 data are shown in the results. The detection algorithm was applied to the freeze-up in the Beaufort, Chukchi, Barents, and East Siberian Seas in 2015 and 2016, spanning mid-September to early November of both years. At the end of the melt, 6 GHz PRIC values are 5-10% greater than those reported by radiometric algorithms at 19 and 37 GHz. During freeze-up, COV separates grease <span class="hlt">ice</span> (<5 cm thick) from water. As the <span class="hlt">ice</span> thickens, the COV is less reliable, but adding a mask based on either the PRIC or the cross-pol/co-pol SAR ratio corrects for COV deficiencies. In general</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011TRACE...5..143O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011TRACE...5..143O"><span><span class="hlt">Ice</span>-Nucleating Bacteria</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Obata, Hitoshi</p> <p></p> <p>Since the discovery of <span class="hlt">ice</span>-nucleating bacteria in 1974 by Maki et al., a large number of studies on the biological characteristics, <span class="hlt">ice</span>-nucleating substance, <span class="hlt">ice</span> nucleation gene and frost damage etc. of the bacteria have been carried out. <span class="hlt">Ice</span>-nucleating bacteria can cause the freezing of water at relatively warm temperature (-2.3°C). Tween 20 was good substrates for <span class="hlt">ice</span>-nucleating <span class="hlt">activity</span> of Pseudomonas fluorescens KUIN-1. Major fatty acids of Isolate (Pseudomonas fluorescens) W-11 grown at 30°C were palmitic, cis-9-hexadecenoic and cis-11-octadecenoic which amounted to 90% of the total fatty acids. Sequence analysis shows that an <span class="hlt">ice</span> nucleation gene from Pseudomonas fluorescens is related to the gene of Pseudomonas syringae.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24204642','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24204642"><span>Floating <span class="hlt">ice</span>-algal aggregates below melting arctic 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>Assmy, Philipp; Ehn, Jens K; Fernández-Méndez, Mar; Hop, Haakon; Katlein, Christian; Sundfjord, Arild; Bluhm, Katrin; Daase, Malin; Engel, Anja; Fransson, Agneta; Granskog, Mats A; Hudson, Stephen R; Kristiansen, Svein; Nicolaus, Marcel; Peeken, Ilka; Renner, Angelika H H; Spreen, Gunnar; Tatarek, Agnieszka; Wiktor, Jozef</p> <p>2013-01-01</p> <p>During two consecutive cruises to the Eastern Central Arctic in late summer 2012, we observed floating algal aggregates in the melt-water layer below and between melting <span class="hlt">ice</span> floes of first-year pack <span class="hlt">ice</span>. The macroscopic (1-15 cm in diameter) aggregates had a mucous consistency and were dominated by typical <span class="hlt">ice</span>-associated pennate diatoms embedded within the mucous matrix. Aggregates maintained buoyancy and accumulated just above a strong pycnocline that separated meltwater and seawater layers. We were able, for the first time, to obtain quantitative abundance and biomass estimates of these aggregates. Although their biomass and production on a square metre basis was small compared to <span class="hlt">ice</span>-algal blooms, the floating <span class="hlt">ice</span>-algal aggregates supported high levels of biological <span class="hlt">activity</span> on the scale of the individual aggregate. In addition they constituted a food source for the <span class="hlt">ice</span>-associated fauna as revealed by pigments indicative of zooplankton grazing, high abundance of naked ciliates, and <span class="hlt">ice</span> amphipods associated with them. During the Arctic melt season, these floating aggregates likely play an important ecological role in an otherwise impoverished near-surface sea <span class="hlt">ice</span> environment. Our findings provide important observations and measurements of a unique aggregate-based habitat during the 2012 record sea <span class="hlt">ice</span> minimum year.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3804104','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3804104"><span>Floating <span class="hlt">Ice</span>-Algal Aggregates below Melting Arctic Sea <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>Assmy, Philipp; Ehn, Jens K.; Fernández-Méndez, Mar; Hop, Haakon; Katlein, Christian; Sundfjord, Arild; Bluhm, Katrin; Daase, Malin; Engel, Anja; Fransson, Agneta; Granskog, Mats A.; Hudson, Stephen R.; Kristiansen, Svein; Nicolaus, Marcel; Peeken, Ilka; Renner, Angelika H. H.; Spreen, Gunnar; Tatarek, Agnieszka; Wiktor, Jozef</p> <p>2013-01-01</p> <p>During two consecutive cruises to the Eastern Central Arctic in late summer 2012, we observed floating algal aggregates in the melt-water layer below and between melting <span class="hlt">ice</span> floes of first-year pack <span class="hlt">ice</span>. The macroscopic (1-15 cm in diameter) aggregates had a mucous consistency and were dominated by typical <span class="hlt">ice</span>-associated pennate diatoms embedded within the mucous matrix. Aggregates maintained buoyancy and accumulated just above a strong pycnocline that separated meltwater and seawater layers. We were able, for the first time, to obtain quantitative abundance and biomass estimates of these aggregates. Although their biomass and production on a square metre basis was small compared to <span class="hlt">ice</span>-algal blooms, the floating <span class="hlt">ice</span>-algal aggregates supported high levels of biological <span class="hlt">activity</span> on the scale of the individual aggregate. In addition they constituted a food source for the <span class="hlt">ice</span>-associated fauna as revealed by pigments indicative of zooplankton grazing, high abundance of naked ciliates, and <span class="hlt">ice</span> amphipods associated with them. During the Arctic melt season, these floating aggregates likely play an important ecological role in an otherwise impoverished near-surface sea <span class="hlt">ice</span> environment. Our findings provide important observations and measurements of a unique aggregate-based habitat during the 2012 record sea <span class="hlt">ice</span> minimum year. PMID:24204642</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1815778H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1815778H"><span>3D-seismic observations of Late Pleistocene glacial dynamics on the central West Greenland <span class="hlt">margin</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hofmann, Julia; Knutz, Paul; Cofaigh, Colm Ó.</p> <p>2016-04-01</p> <p>Fast-flowing <span class="hlt">ice</span> streams and outlet glaciers exert a major control on glacial discharge from contemporary and palaeo <span class="hlt">ice</span> sheets. Improving our understanding of the extent and dynamic behaviour of these palaeo-<span class="hlt">ice</span> streams is therefore crucial for predictions of the response of <span class="hlt">ice</span> sheets to present and future climate warming and the associated implications for global sea level. This poster presents results from two 3D-seismic surveys located on the shelf adjoining the Disko Bay trough-mouth fan (TMF), one of the largest glacial outlet systems in Greenland. Located at the seaward terminus of the c. 370 km long cross-shelf Disko Trough, the Disko Bay TMF was generated by highly efficient subglacial sediment delivery onto the continental slopes during repeated <span class="hlt">ice</span>-stream advances. A variety of submarine glacial landform assemblages are recognised on the seabed reflecting past <span class="hlt">ice</span>-stream <span class="hlt">activity</span> presumably related to glacial-interglacial cycles. The 3D-seismic volumes cover the shallow banks located north and south of the Disko Trough. The focus of this study is the seabed and the uppermost stratigraphic interval associated with the Late Stage of TMF development, presumably covering the late Pleistocene (Hofmann et al., submitted). Seabed morphologies include multiple sets of ridges up to 20 m high that extend in NW-SE direction for c. 30 km, and cross-cutting curvilinear furrows with maximum lengths of c. 9 km and average depths of c. 4.5 m. Back-stepping, arcuate scarps facing NW define the shelf break on the northern survey, comprising average widths of c. 4.5 km and incision depths of c. 27.5 m. The large transverse ridge features on the southern survey are likely <span class="hlt">ice-marginal</span> and are interpreted as terminal moraine ridges recording the existence of a shelf-edge terminating, grounded Late Weichselian <span class="hlt">ice</span> sheet. The furrows, most prominent on the outer shelf adjoining the shallow banks and partly incising the moraine ridges, are interpreted as iceberg ploughmarks</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4928901','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4928901"><span>Pan–<span class="hlt">ice</span>-sheet glacier terminus change in East Antarctica reveals sensitivity of Wilkes Land to sea-<span class="hlt">ice</span> changes</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Miles, Bertie W. J.; Stokes, Chris R.; Jamieson, Stewart S. R.</p> <p>2016-01-01</p> <p>The dynamics of ocean-terminating outlet glaciers are an important component of <span class="hlt">ice</span>-sheet mass balance. Using satellite imagery for the past 40 years, we compile an approximately decadal record of outlet-glacier terminus position change around the entire East Antarctic <span class="hlt">Ice</span> Sheet (EAIS) marine <span class="hlt">margin</span>. We find that most outlet glaciers retreated during the period 1974–1990, before switching to advance in every drainage basin during the two most recent periods, 1990–2000 and 2000–2012. The only exception to this trend was in Wilkes Land, where the majority of glaciers (74%) retreated between 2000 and 2012. We hypothesize that this anomalous retreat is linked to a reduction in sea <span class="hlt">ice</span> and associated impacts on ocean stratification, which increases the incursion of warm deep water toward glacier termini. Because Wilkes Land overlies a large marine basin, it raises the possibility of a future sea level contribution from this sector of East Antarctica. PMID:27386519</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27386519','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27386519"><span>Pan-<span class="hlt">ice</span>-sheet glacier terminus change in East Antarctica reveals sensitivity of Wilkes Land to sea-<span class="hlt">ice</span> changes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Miles, Bertie W J; Stokes, Chris R; Jamieson, Stewart S R</p> <p>2016-05-01</p> <p>The dynamics of ocean-terminating outlet glaciers are an important component of <span class="hlt">ice</span>-sheet mass balance. Using satellite imagery for the past 40 years, we compile an approximately decadal record of outlet-glacier terminus position change around the entire East Antarctic <span class="hlt">Ice</span> Sheet (EAIS) marine <span class="hlt">margin</span>. We find that most outlet glaciers retreated during the period 1974-1990, before switching to advance in every drainage basin during the two most recent periods, 1990-2000 and 2000-2012. The only exception to this trend was in Wilkes Land, where the majority of glaciers (74%) retreated between 2000 and 2012. We hypothesize that this anomalous retreat is linked to a reduction in sea <span class="hlt">ice</span> and associated impacts on ocean stratification, which increases the incursion of warm deep water toward glacier termini. Because Wilkes Land overlies a large marine basin, it raises the possibility of a future sea level contribution from this sector of East Antarctica.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5610426','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5610426"><span>Plume <span class="hlt">Activity</span> and Tidal Deformation on Enceladus Influenced by Faults and Variable <span class="hlt">Ice</span> Shell Thickness</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Souček, Ondřej; Hron, Jaroslav; Čadek, Ondřej</p> <p>2017-01-01</p> <p>Abstract We investigated the effect of variations in <span class="hlt">ice</span> shell thickness and of the tiger stripe fractures crossing Enceladus' south polar terrain on the moon's tidal deformation by performing finite element calculations in three-dimensional geometry. The combination of thinning in the polar region and the presence of faults has a synergistic effect that leads to an increase of both the displacement and stress in the south polar terrain by an order of magnitude compared to that of the traditional model with a uniform shell thickness and without faults. Assuming a simplified conductive heat transfer and neglecting the heat sources below the <span class="hlt">ice</span> shell, we computed the global heat budget of the <span class="hlt">ice</span> shell. For the inelastic properties of the shell described by a Maxwell viscoelastic model, we show that unrealistically low average viscosity of the order of 1013 Pa s is necessary for preserving the volume of the ocean, suggesting the important role of the heat sources in the deep interior. Similarly, low viscosity is required to predict the observed delay of the plume <span class="hlt">activity</span>, which hints at other delaying mechanisms than just the viscoelasticity of the <span class="hlt">ice</span> shell. The presence of faults results in large spatial and temporal heterogeneity of geysering <span class="hlt">activity</span> compared to the traditional models without faults. Our model contributes to understanding the physical mechanisms that control the fault <span class="hlt">activity</span>, and it provides potentially useful information for future missions that will sample the plume for evidence of life. Key Words: Enceladus—Tidal deformation—Faults—Variable <span class="hlt">ice</span> shell thickness—Tidal heating—Plume <span class="hlt">activity</span> and timing. Astrobiology 17, 941–954. PMID:28816521</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1376012','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1376012"><span>Delayed deglaciation or extreme Arctic conditions 21-16 cal. kyr at southeastern Laurentide <span class="hlt">Ice</span> Sheet <span class="hlt">margin</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>Peteet, D. M.; Beh, M.; Orr, C.</p> <p></p> <p>The conventionally accepted ages of the Last Glacial Maximum (LGM) retreat of the southeastern Laurentide <span class="hlt">Ice</span> Sheet (LIS) are 26–21 cal. kyr (derived from bulk-sediment radiocarbon ages) and 28–23 cal. kyr (varve estimates). By utilizing accelerator mass spectrometry (AMS) 14C dating of earliest macrofossils in 13 lake/bog inorganic clays, we find that vegetation first appeared on the landscape at 16–15 cal. kyr, suggesting <span class="hlt">ice</span> had not retreated until that time. The gap between previous age estimates and ours is significant and has large implications for our understanding of ocean-atmosphere linkages. Older ages imply extreme Arctic conditions for 9–5 cal kyr;more » a landscape with no <span class="hlt">ice</span>, yet no deposition in lakes. Also, our new AMS chronology of LIS retreat is consistent with marine evidence of deglaciation from the N. Atlantic, showing significant freshwater input and sea level rise only after 19 cal kyr with a cold meltwater lid, perhaps delaying <span class="hlt">ice</span> melt.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1376012-delayed-deglaciation-extreme-arctic-conditions-cal-kyr-southeastern-laurentide-ice-sheet-margin','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1376012-delayed-deglaciation-extreme-arctic-conditions-cal-kyr-southeastern-laurentide-ice-sheet-margin"><span>Delayed deglaciation or extreme Arctic conditions 21-16 cal. kyr at southeastern Laurentide <span class="hlt">Ice</span> Sheet <span class="hlt">margin</span>?</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Peteet, D. M.; Beh, M.; Orr, C.; ...</p> <p>2012-06-15</p> <p>The conventionally accepted ages of the Last Glacial Maximum (LGM) retreat of the southeastern Laurentide <span class="hlt">Ice</span> Sheet (LIS) are 26–21 cal. kyr (derived from bulk-sediment radiocarbon ages) and 28–23 cal. kyr (varve estimates). By utilizing accelerator mass spectrometry (AMS) 14C dating of earliest macrofossils in 13 lake/bog inorganic clays, we find that vegetation first appeared on the landscape at 16–15 cal. kyr, suggesting <span class="hlt">ice</span> had not retreated until that time. The gap between previous age estimates and ours is significant and has large implications for our understanding of ocean-atmosphere linkages. Older ages imply extreme Arctic conditions for 9–5 cal kyr;more » a landscape with no <span class="hlt">ice</span>, yet no deposition in lakes. Also, our new AMS chronology of LIS retreat is consistent with marine evidence of deglaciation from the N. Atlantic, showing significant freshwater input and sea level rise only after 19 cal kyr with a cold meltwater lid, perhaps delaying <span class="hlt">ice</span> melt.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013TCry....7.1161B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013TCry....7.1161B"><span>Data assimilation and prognostic whole <span class="hlt">ice</span> sheet modelling with the variationally derived, higher order, open source, and fully parallel <span class="hlt">ice</span> sheet model VarGlaS</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brinkerhoff, D. J.; Johnson, J. V.</p> <p>2013-07-01</p> <p>We introduce a novel, higher order, finite element <span class="hlt">ice</span> sheet model called VarGlaS (Variational Glacier Simulator), which is built on the finite element framework FEniCS. Contrary to standard procedure in <span class="hlt">ice</span> sheet modelling, VarGlaS formulates <span class="hlt">ice</span> sheet motion as the minimization of an energy functional, conferring advantages such as a consistent platform for making numerical approximations, a coherent relationship between motion and heat generation, and implicit boundary treatment. VarGlaS also solves the equations of enthalpy rather than temperature, avoiding the solution of a contact problem. Rather than include a lengthy model spin-up procedure, VarGlaS possesses an automated framework for model inversion. These capabilities are brought to bear on several benchmark problems in <span class="hlt">ice</span> sheet modelling, as well as a 500 yr simulation of the Greenland <span class="hlt">ice</span> sheet at high resolution. VarGlaS performs well in benchmarking experiments and, given a constant climate and a 100 yr relaxation period, predicts a mass evolution of the Greenland <span class="hlt">ice</span> sheet that matches present-day observations of mass loss. VarGlaS predicts a thinning in the interior and thickening of the <span class="hlt">margins</span> of the <span class="hlt">ice</span> sheet.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.A13B0319S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.A13B0319S"><span>Highly <span class="hlt">Active</span> <span class="hlt">Ice</span> Nuclei from Tree Leaf Litters Retain <span class="hlt">Activity</span> for Decades</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schnell, R. C.; Hill, T. C. J.</p> <p>2015-12-01</p> <p>Biogenic <span class="hlt">ice</span> nuclei (IN) studied since the 1960s were first observed in tree leaf litters, in a few bacteria species and later in fungi and lichens. Recently, viable IN bacteria in precipitation have been used as a metric of their possible role in precipitation formation. Although bacterial IN <span class="hlt">activity</span> is deactivated by a variety of common environmental stresses, we present data showing that IN found in a potpourri of decayed plant leaves, bacteria, molds and fungi etc. in plant litters are exceptionally stable and <span class="hlt">active</span> over decades while in storage. As such, their atmospheric IN potential is worthy of further study due to their environmental persistence. In August 1970 litter collected in a grove of deciduous trees near Red Deer, AB, Canada was tested for IN (drop freezing technique). The sample initiated <span class="hlt">ice</span> at -4C with 109 IN per gram of litter <span class="hlt">active</span> at -10C. A few kilograms were stored in a plastic bag and tested every few years for IN content; the IN <span class="hlt">activity</span> remained essentially unchanged over 40 years. In 2011, litter collected in the same grove had the same IN <span class="hlt">activity</span> as the sample tested over the intervening 40 years. Boiling a gram sample of this litter in 100 grams of water deactivated 99 % of the IN <span class="hlt">activity</span> down to -13C. None of 88 different bacteria cultures several of which appeared to Pseudomonads (common IN producing bacteria) from the fresh litter produced any <span class="hlt">active</span> IN. A sample of the litter was placed on the top of a 15 cm column of laboratory grade kaolin and water dripped onto the litter. Ten days later the water reached the bottom of the column. The kaolin was dried and tested for IN. The prior essentially IN free kaolin now exhibited IN <span class="hlt">activity</span> at -4C with 105 IN <span class="hlt">active</span> at -10C. The litter exposed kaolin retained the IN <span class="hlt">activity</span> for 25 years. Baking the kaolin removed the <span class="hlt">active</span> IN. This suggests that IN <span class="hlt">activity</span> attributed to kaolin particles sometimes seen at the nucleus of snow crystals could be of biological origin.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/20020695-arctic-sea-ice-variability-context-recent-atmospheric-circulation-trends','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/20020695-arctic-sea-ice-variability-context-recent-atmospheric-circulation-trends"><span>Arctic sea <span class="hlt">ice</span> variability in the context of recent atmospheric circulation trends</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>Deser, C.; Walsh, J.E.; Timlin, M.S.</p> <p></p> <p>Sea <span class="hlt">ice</span> is a sensitive component of the climate system, influenced by conditions in both the atmosphere and ocean. Variations in sea <span class="hlt">ice</span> may in turn modulate climate by altering the surface albedo; the exchange of heat, moisture, and momentum between the atmosphere and ocean; and the upper ocean stratification in areas of deep water formation. The surface albedo effect is considered to be one of the dominant factors in the poleward amplification of global warming due to increased greenhouse gas concentrations simulated in many climate models. Forty years (1958--97) of reanalysis products and corresponding sea <span class="hlt">ice</span> concentration data aremore » used to document Arctic sea <span class="hlt">ice</span> variability and its association with surface air temperature (SAT) and sea level pressure (SLP) throughout the Northern Hemisphere extratropics. The dominant mode of winter (January-March) sea <span class="hlt">ice</span> variability exhibits out-of-phase fluctuations between the western and eastern North Atlantic, together with a weaker dipole in the North Pacific. The time series of this mode has a high winter-to-winter autocorrelation (0.69) and is dominated by decadal-scale variations and a longer-term trend of diminishing <span class="hlt">ice</span> cover east of Greenland and increasing <span class="hlt">ice</span> cover west of Greenland. Associated with the dominant pattern of winter sea <span class="hlt">ice</span> variability are large-scale changes in SAT and SLP that closely resemble the North Atlantic oscillation. The associated SAT and surface sensible and latent heat flux anomalies are largest over the portions of the <span class="hlt">marginal</span> sea <span class="hlt">ice</span> zone in which the trends of <span class="hlt">ice</span> coverage have been greatest, although the well-documented warming of the northern continental regions is also apparent. the temporal and spatial relationships between the SLP and <span class="hlt">ice</span> anomaly fields are consistent with the notion that atmospheric circulation anomalies force the sea <span class="hlt">ice</span> variations. However, there appears to be a local response of the atmospheric circulation to the changing sea <span class="hlt">ice</span> variations. However</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29735675','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29735675"><span>Polypentagonal <span class="hlt">ice</span>-like water networks emerge solely in an <span class="hlt">activity</span>-improved variant of <span class="hlt">ice</span>-binding protein.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mahatabuddin, Sheikh; Fukami, Daichi; Arai, Tatsuya; Nishimiya, Yoshiyuki; Shimizu, Rumi; Shibazaki, Chie; Kondo, Hidemasa; Adachi, Motoyasu; Tsuda, Sakae</p> <p>2018-05-22</p> <p>Polypentagonal water networks were recently observed in a protein capable of binding to <span class="hlt">ice</span> crystals, or <span class="hlt">ice</span>-binding protein (IBP). To examine such water networks and clarify their role in <span class="hlt">ice</span>-binding, we determined X-ray crystal structures of a 65-residue defective isoform of a Zoarcidae -derived IBP (wild type, WT) and its five single mutants (A20L, A20G, A20T, A20V, and A20I). Polypentagonal water networks composed of ∼50 semiclathrate waters were observed solely on the strongest A20I mutant, which appeared to include a tetrahedral water cluster exhibiting a perfect position match to the [Formula: see text] first prism plane of a single <span class="hlt">ice</span> crystal. Inclusion of another symmetrical water cluster in the polypentagonal network showed a perfect complementarity to the waters constructing the [Formula: see text] pyramidal <span class="hlt">ice</span> plane. The order of <span class="hlt">ice</span>-binding strength was A20L < A20G < WT < A20T < A20V < A20I, where the top three mutants capable of binding to the first prism and the pyramidal <span class="hlt">ice</span> planes commonly contained a bifurcated γ-CH 3 group. These results suggest that a fine-tuning of the surface of Zoarcidae -derived IBP assisted by a side-chain group regulates the holding property of its polypentagonal water network, the function of which is to freeze the host protein to specific <span class="hlt">ice</span> planes. Copyright © 2018 the Author(s). Published by PNAS.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2012-05-09/pdf/2012-11129.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2012-05-09/pdf/2012-11129.pdf"><span>77 FR 27254 - Self-Regulatory Organizations; <span class="hlt">ICE</span> Clear Europe Limited; Order Approving Proposed Rule Change To...</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2012-05-09</p> <p>... SECURITIES AND EXCHANGE COMMISSION [Release No. 34-66911; File No. SR-ICEEU-2012-05] Self-Regulatory Organizations; <span class="hlt">ICE</span> Clear Europe Limited; Order Approving Proposed Rule Change To Amend the <span class="hlt">ICE</span> Clear Europe Limited CDS Procedures, Finance Procedures, and Rules With Respect to the Calculation and Payment of Interest on Mark-To-Market <span class="hlt">Margin</span> on...</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_24 --> <div id="page_25" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="481"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16346129','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16346129"><span>Plants as sources of airborne bacteria, including <span class="hlt">ice</span> nucleation-<span class="hlt">active</span> bacteria.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lindemann, J; Constantinidou, H A; Barchet, W R; Upper, C D</p> <p>1982-11-01</p> <p>Vertical wind shear and concentration gradients of viable, airborne bacteria were used to calculate the upward flux of viable cells above bare soil and canopies of several crops. Concentrations at soil or canopy height varied from 46 colony-forming units per m over young corn and wet soil to 663 colony-forming units per m over dry soil and 6,500 colony-forming units per m over a closed wheat canopy. In simultaneous samples, concentrations of viable bacteria in the air 10 m inside an alfalfa field were fourfold higher than those over a field with dry, bare soil immediately upwind. The upward flux of viable bacteria over alfalfa was three- to fourfold greater than over dry soil. Concentrations of <span class="hlt">ice</span> nucleation-<span class="hlt">active</span> bacteria were higher over plants than over soil. Thus, plant canopies may constitute a major source of bacteria, including <span class="hlt">ice</span> nucleation-<span class="hlt">active</span> bacteria, in the air.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28247129','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28247129"><span>Habitat degradation affects the summer <span class="hlt">activity</span> of polar bears.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ware, Jasmine V; Rode, Karyn D; Bromaghin, Jeffrey F; Douglas, David C; Wilson, Ryan R; Regehr, Eric V; Amstrup, Steven C; Durner, George M; Pagano, Anthony M; Olson, Jay; Robbins, Charles T; Jansen, Heiko T</p> <p>2017-05-01</p> <p>Understanding behavioral responses of species to environmental change is critical to forecasting population-level effects. Although climate change is significantly impacting species' distributions, few studies have examined associated changes in behavior. Polar bear (Ursus maritimus) subpopulations have varied in their near-term responses to sea <span class="hlt">ice</span> decline. We examined behavioral responses of two adjacent subpopulations to changes in habitat availability during the annual sea <span class="hlt">ice</span> minimum using <span class="hlt">activity</span> data. Location and <span class="hlt">activity</span> sensor data collected from 1989 to 2014 for 202 adult female polar bears in the Southern Beaufort Sea (SB) and Chukchi Sea (CS) subpopulations were used to compare <span class="hlt">activity</span> in three habitat types varying in prey availability: (1) land; (2) <span class="hlt">ice</span> over shallow, biologically productive waters; and (3) <span class="hlt">ice</span> over deeper, less productive waters. Bears varied <span class="hlt">activity</span> across and within habitats with the highest <span class="hlt">activity</span> at 50-75% sea <span class="hlt">ice</span> concentration over shallow waters. On land, SB bears exhibited variable but relatively high <span class="hlt">activity</span> associated with the use of subsistence-harvested bowhead whale carcasses, whereas CS bears exhibited low <span class="hlt">activity</span> consistent with minimal feeding. Both subpopulations had fewer observations in their preferred shallow-water sea <span class="hlt">ice</span> habitats in recent years, corresponding with declines in availability of this substrate. The substantially higher use of <span class="hlt">marginal</span> habitats by SB bears is an additional mechanism potentially explaining why this subpopulation has experienced negative effects of sea <span class="hlt">ice</span> loss compared to the still-productive CS subpopulation. Variability in <span class="hlt">activity</span> among, and within, habitats suggests that bears alter their behavior in response to habitat conditions, presumably in an attempt to balance prey availability with energy costs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014Icar..237..315S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014Icar..237..315S"><span>Volcano-<span class="hlt">ice</span> interactions in the Arsia Mons tropical mountain glacier deposits</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Scanlon, Kathleen E.; Head, James W.; Wilson, Lionel; Marchant, David R.</p> <p>2014-07-01</p> <p>Fan-shaped deposits (FSD) superposed on the sides of the Tharsis Montes volcanic edifices are widely interpreted to have been formed by cold-based glaciation during the Late Amazonian, a period when the Tharsis Montes were volcanically <span class="hlt">active</span>. We survey the ∼166,000 km2 Arsia Mons FSD using new, high-resolution image and topography data and describe numerous landforms indicative of volcano-<span class="hlt">ice</span> interactions. These include (1) steep-sided mounds, morphologically similar to terrestrial tindar that form by subglacial eruptions under low confining pressure; (2) steep-sided, leveed flow-like landforms with depressed centers, interpreted to be subglacial lava flows with chilled <span class="hlt">margins</span>; (3) digitate flows that we interpret as having resulted from lava flow interaction with glacial <span class="hlt">ice</span> at the upslope <span class="hlt">margin</span> of the glacier; (4) a plateau with the steep sides and smooth capping flow of a basaltic tuya, a class of feature formed when subglacial eruptions persist long enough to melt through the overlying <span class="hlt">ice</span>; and (5) low, areally extensive mounds that we interpret as effusions of pillow lava, formed by subglacial eruptions under high confining pressure. Together, these eruptions involved hundreds of cubic kilometers of subglacially erupted lava; thermodynamic relationships indicate that this amount of lava would have produced a similar volume of subglacial liquid meltwater, some of which carved fluvial features in the FSD. Landforms in the FSD also suggest that glaciovolcanic heat transfer induced local wet-based flow in some parts of the glacier. Glaciovolcanic environments are important microbial habitats on Earth, and the evidence for widespread liquid water in the Amazonian-aged Arsia Mons FSD makes it one of the most recent potentially habitable environments on Mars. Such environments could have provided refugia for any life that developed on Mars and survived on its surface until the Amazonian.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1994GeoRu..83..743S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1994GeoRu..83..743S"><span>Early Paleozoic paleogeography of the northern Gondwana <span class="hlt">margin</span>: new evidence for Ordovician-Silurian glaciation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Semtner, A.-K.; Klitzsch, E.</p> <p>1994-12-01</p> <p>During the Early Paleozoic, transgressions and the distribution of sedimentary facies on the northern Gondwana <span class="hlt">margin</span> were controlled by a regional NNW-SSE to almost north-south striking structural relief. In Early Silurian times, a eustatic highstand enabled the sea to reach its maximum southward extent. The counterclockwise rotation of Gondwana during the Cambrian and Early Ordovician caused the northern Gondwana <span class="hlt">margin</span> to shift from intertropical to southern polar latitudes in Ordovician times. Glacial and periglacial deposits are reported from many localities in Morocco, Algeria, Niger, Libya, Chad, Sudan, Jordan and Saudi Arabia. The Late Ordovician glaciation phase was followed by a period of a major glacioeustatic sea-level rise in the Early Silurian due to the retreat of the <span class="hlt">ice</span>-cap. As a consequence of the decreasing water circulation in the basin centers (Central Arabia, Murzuk- and Ghadames basins), highly bituminous euxinic shales were deposited. These shales are considered to be the main source rock of Paleozoic oil and gas deposits in parts of Saudi Arabia, Libya and Algeria. The following regression in the southern parts of the Early Silurian sea was probably caused by a second glacial advance, which was mainly restricted to areas in Chad, Sudan and Niger. Evidence for glacial <span class="hlt">activity</span> and fluvioglacial sedimentation is available from rocks overlying the basal Silurian shale in north-east Chad and north-west Sudan. The Early Silurian <span class="hlt">ice</span> advance is considered to be responsible for the termination of euxinic shale deposition in the basin centers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26553559','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26553559"><span><span class="hlt">Ice</span> nucleation <span class="hlt">active</span> particles are efficiently removed by precipitating clouds.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Stopelli, Emiliano; Conen, Franz; Morris, Cindy E; Herrmann, Erik; Bukowiecki, Nicolas; Alewell, Christine</p> <p>2015-11-10</p> <p><span class="hlt">Ice</span> nucleation in cold clouds is a decisive step in the formation of rain and snow. Observations and modelling suggest that variations in the concentrations of <span class="hlt">ice</span> nucleating particles (INPs) affect timing, location and amount of precipitation. A quantitative description of the abundance and variability of INPs is crucial to assess and predict their influence on precipitation. Here we used the hydrological indicator δ(18)O to derive the fraction of water vapour lost from precipitating clouds and correlated it with the abundance of INPs in freshly fallen snow. Results show that the number of INPs <span class="hlt">active</span> at temperatures ≥ -10 °C (INPs-10) halves for every 10% of vapour lost through precipitation. Particles of similar size (>0.5 μm) halve in number for only every 20% of vapour lost, suggesting effective microphysical processing of INPs during precipitation. We show that INPs <span class="hlt">active</span> at moderate supercooling are rapidly depleted by precipitating clouds, limiting their impact on subsequent rainfall development in time and space.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009JVGR..185..298L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009JVGR..185..298L"><span>Fracture patterns at lava-<span class="hlt">ice</span> contacts on Kokostick Butte, OR, and Mazama Ridge, Mount Rainier, WA: Implications for flow emplacement and cooling histories</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lodge, Robert W. D.; Lescinsky, David T.</p> <p>2009-09-01</p> <p>Cooling lava commonly develop polygonal joints that form equant hexagonal columns. Such fractures are formed by thermal contraction resulting in an isotropic tensional stress regime. However, certain linear cooling fracture patterns observed at some lava-<span class="hlt">ice</span> contacts do not appear to fit the model for formation of cooling fractures and columns because of their preferred orientations. These fracture types include sheet-like (ladder-like rectangular fracture pattern), intermediate (pseudo-aligned individual column-bounding fractures), and pseudopillow (straight to arcuate fractures with perpendicular secondary fractures caused by water infiltration) fractures that form the edges of multiple columns along a single linear fracture. Despite the relatively common occurrence of these types of fractures at lava-<span class="hlt">ice</span> contacts, their significance and mode of formation have not been fully explored. This study investigates the stress regimes responsible for producing these unique fractures and their significance for interpreting cooling histories at lava-<span class="hlt">ice</span> contacts. Data was collected at Kokostick Butte dacite flow at South Sister, OR, and Mazama Ridge andesite flow at Mount Rainier, WA. Both of these lava flows have been interpreted as being emplaced into contact with <span class="hlt">ice</span> and linear fracture types have been observed on their <span class="hlt">ice</span>-contacted <span class="hlt">margins</span>. Two different mechanisms are proposed for the formation of linear fracture networks. One possible mechanism for the formation of linear fracture patterns is <span class="hlt">marginal</span> bulging. Melting of confining <span class="hlt">ice</span> walls will create voids into which flowing lava can deform resulting in <span class="hlt">margin</span>-parallel tension causing <span class="hlt">margin</span>-perpendicular fractures. If viewed from the <span class="hlt">ice</span>-wall, these fractures would be steeply dipping, linear fractures. Another possible mechanism for the formation of linear fracture types is gravitational settling. Pure shear during compression and settling can result in a tensional environment with similar consequences as</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C41C1229S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C41C1229S"><span>Simulating <span class="hlt">Ice</span> Dynamics in the Amundsen Sea Sector</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schwans, E.; Parizek, B. R.; Morlighem, M.; Alley, R. B.; Pollard, D.; Walker, R. T.; Lin, P.; St-Laurent, P.; LaBirt, T.; Seroussi, H. L.</p> <p>2017-12-01</p> <p>Thwaites and Pine Island Glaciers (TG; PIG) exhibit patterns of dynamic retreat forced from their floating <span class="hlt">margins</span>, and could act as gateways for destabilization of deep marine basins in the West Antarctic <span class="hlt">Ice</span> Sheet (WAIS). Poorly constrained basal conditions can cause model predictions to diverge. Thus, there is a need for efficient simulations that account for shearing within the <span class="hlt">ice</span> column, and include adequate basal sliding and <span class="hlt">ice</span>-shelf melting parameterizations. To this end, UCI/NASA JPL's <span class="hlt">Ice</span> Sheet System Model (ISSM) with coupled SSA/higher-order physics is used in the Amundsen Sea Embayment (ASE) to examine threshold behavior of TG and PIG, highlighting areas particularly vulnerable to retreat from oceanic warming and <span class="hlt">ice</span>-shelf removal. These moving-front experiments will aid in targeting critical areas for additional data collection in ASE as well as for weighting accuracy in further melt parameterization development. Furthermore, a sub-shelf melt parameterization, resulting from Regional Ocean Modeling System (ROMS; St-Laurent et al., 2015) and coupled ISSM-Massachusetts Institute of Technology general circulation model (MITgcm; Seroussi et al., 2017) output, is incorporated and initially tested in ISSM. Data-guided experiments include variable basal conditions and <span class="hlt">ice</span> hardness, and are also forced with constant modern climate in ISSM, providing valuable insight into i) effects of different basal friction parameterizations on <span class="hlt">ice</span> dynamics, illustrating the importance of constraining the variable bed character beneath TG and PIG; ii) the impact of including vertical shear in <span class="hlt">ice</span> flow models of outlet glaciers, confirming its role in capturing complex feedbacks proximal to the grounding zone; and iii) ASE's sensitivity to sub-shelf melt and <span class="hlt">ice</span>-front retreat, possible thresholds, and how these affect <span class="hlt">ice</span>-flow evolution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1818434P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1818434P"><span>A new model for the development of the <span class="hlt">active</span> Afar volcanic <span class="hlt">margin</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pik, Raphaël; Stab, Martin; Bellahsen, Nicolas; Leroy, Sylvie</p> <p>2016-04-01</p> <p>Volcanic passive <span class="hlt">margins</span>, that represent more than the three quarters of continental <span class="hlt">margins</span> worldwide, are privileged witnesses of the lithospheric extension processes thatform new oceanic basins. They are characterized by voluminous amounts of underplated, intruded and extruded magmas, under the form of massive lavas prisms (seaward-dipping reflectors, or SDR) during the course of thinning and stretching of the lithosphere, that eventually form the ocean-continent transition. The origin and mechanisms of formation of these objects are still largely debated today. We have focussed our attention in the last few years on the Afar volcanic province which represents an <span class="hlt">active</span> analogue of such volcanic <span class="hlt">margins</span>. We explored the structural and temporal relationships that exist between the development of the major thinning and stretching structures and the magmatic production in Central Afar. Conjugate precise fieldwork analysis along with lavas geochronology allowed us to revisit the timing and style of the rift formation, since the early syn-rift period of time in the W-Afar <span class="hlt">marginal</span> area to present days. Extension is primarily accommodated over a wide area at the surface since the very initial periods of extension (~ 25 Ma) following the emplacement of Oligocene CFBs. We propose in our reconstruction of central Afar <span class="hlt">margin</span> history that extension has been associated with important volumes of underplated mafic material that compensate crustal thinning. This has been facilitated by major crustal-scale detachments that help localize the thinning and underplating at depth. In line with this 'magmatic wide-rift' mode of extension, we demonstrate that episodic extension steps alternate with more protracted magmatic phases. The production of syn-rift massive flood basalts (~ 4 Ma) occurs after early thinning of both the crust and the lithosphere, which suggests that SDR formation, is controlled by previous tectonic event. We determined how the melting regime evolved in</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 Antarctic 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 Antarctic sea-<span class="hlt">ice</span> coverage, coeval with thinning West Antarctic <span class="hlt">Ice</span> Sheet (WAIS) <span class="hlt">ice</span> shelves and the rapid freshening of surface and bottom waters along the Antarctic <span class="hlt">margin</span>. 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 Antarctic <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://adsabs.harvard.edu/abs/2016AGUFM.C21A0650P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C21A0650P"><span>Sea <span class="hlt">Ice</span> Summer Camp: Bringing Together Arctic Sea <span class="hlt">Ice</span> Modelers and Observers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Perovich, D. K.; Holland, M. M.</p> <p>2016-12-01</p> <p>The Arctic sea <span class="hlt">ice</span> has undergone dramatic change and numerical models project this to continue for the foreseeable future. Understanding the mechanisms behind sea <span class="hlt">ice</span> loss and its consequences for the larger Arctic and global systems is of critical importance if we are to anticipate and plan for the future. One impediment to progress is a disconnect between the observational and modeling communities. A sea <span class="hlt">ice</span> summer camp was held in Barrow Alaska from 26 May to 1 June 2016 to overcome this impediment and better integrate the sea <span class="hlt">ice</span> community. The 25 participants were a mix of modelers and observers from 13 different institutions at career stages from graduate student to senior scientist. The summer camp provided an accelerated program on sea <span class="hlt">ice</span> observations and models and also fostered future collaborative interdisciplinary <span class="hlt">activities</span>. Each morning was spent in the classroom with a daily lecture on an aspect of modeling or remote sensing followed by practical exercises. Topics included using models to assess sensitivity, to test hypotheses and to explore sources of uncertainty in future Arctic sea <span class="hlt">ice</span> loss. The afternoons were spent on the <span class="hlt">ice</span> making observations. There were four observational <span class="hlt">activities</span>; albedo observations, <span class="hlt">ice</span> thickness measurements, <span class="hlt">ice</span> coring and physical properties, and <span class="hlt">ice</span> morphology surveys. The last field day consisted of a grand challenge where the group formulated a hypothesis, developed an observational and modeling strategy to test the hypothesis, and then integrated the observations and model results. The impacts of changing sea <span class="hlt">ice</span> are being felt today in Barrow Alaska. We opened a dialog with Barrow community members to further understand these changes. This included an evening discussion with two Barrow sea <span class="hlt">ice</span> experts and a community presentation of our work in a public lecture at the Inupiat Heritage Center.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C21G1192Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C21G1192Z"><span>Under Sea <span class="hlt">Ice</span> phytoplankton bloom detection and contamination in Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zeng, C.; Zeng, T.; Xu, H.</p> <p>2017-12-01</p> <p>Previous researches reported compelling sea <span class="hlt">ice</span> phytoplankton bloom in Arctic, while seldom reports studied about Antarctic. Here, lab experiment showed sea <span class="hlt">ice</span> increased the visible light albedo of the water leaving radiance. Even a new formed sea <span class="hlt">ice</span> of 10cm thickness increased water leaving radiance up to 4 times of its original bare water. Given that phytoplankton preferred growing and accumulating under the sea <span class="hlt">ice</span> with thickness of 10cm-1m, our results showed that the changing rate of OC4 estimated [Chl-a] varied from 0.01-0.5mg/m3 to 0.2-0.3mg/m3, if the water covered by 10cm sea <span class="hlt">ice</span>. Going further, varying thickness of sea <span class="hlt">ice</span> modulated the changing rate of estimating [Chl-a] non-linearly, thus current routine OC4 model cannot estimate under sea <span class="hlt">ice</span> [Chl-a] appropriately. Besides, <span class="hlt">marginal</span> sea <span class="hlt">ice</span> zone has a large amount of mixture regions containing sea <span class="hlt">ice</span>, water and snow, where is favorable for phytoplankton. We applied 6S model to estimate the sea <span class="hlt">ice</span>/snow contamination on sub-pixel water leaving radiance of 4.25km spatial resolution ocean color products. Results showed that sea <span class="hlt">ice</span>/snow scale effectiveness overestimated [Chl-a] concentration based on routine band ratio OC4 model, which contamination increased with the rising fraction of sea <span class="hlt">ice</span>/snow within one pixel. Finally, we analyzed the under sea <span class="hlt">ice</span> bloom in Antarctica based on the [Chl-a] concentration trends during 21 days after sea <span class="hlt">ice</span> retreating. Regardless of those overestimation caused by sea <span class="hlt">ice</span>/snow sub scale contamination, we still did not see significant under sea <span class="hlt">ice</span> blooms in Antarctica in 2012-2017 compared with Arctic. This research found that Southern Ocean is not favorable for under sea <span class="hlt">ice</span> blooms and the phytoplankton bloom preferred to occur in at least 3 weeks after sea <span class="hlt">ice</span> retreating.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1227764-integrating-laboratory-field-data-quantify-immersion-freezing-ice-nucleation-activity-mineral-dust-particles','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1227764-integrating-laboratory-field-data-quantify-immersion-freezing-ice-nucleation-activity-mineral-dust-particles"><span>Integrating laboratory and field data to quantify the immersion freezing <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> of mineral dust particles</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>DeMott, P. J.; Prenni, A. J.; McMeeking, G. R.; ...</p> <p>2014-06-27</p> <p>Data from both laboratory studies and atmospheric measurements are used to develop a simple parametric description for the immersion freezing <span class="hlt">activity</span> of natural mineral dust particles. Measurements made with the Colorado State University (CSU) continuous flow diffusion chamber (CFDC) when processing mineral dust aerosols at a nominal 105% relative humidity with respect to water (RH w) are taken to approximate the immersion freezing nucleation <span class="hlt">activity</span> of particles. <span class="hlt">Ice</span> <span class="hlt">active</span> frozen fractions vs. temperature for dusts representative of Saharan and Asian desert sources were consistent with similar measurements in atmospheric dust plumes for a limited set of comparisons available. The parameterizationmore » developed follows the form of one suggested previously for atmospheric particles of non-specific composition in quantifying <span class="hlt">ice</span> nucleating particle concentrations as functions of temperature and the total number concentration of particles larger than 0.5 μm diameter. Such an approach does not explicitly account for surface area and time dependencies for <span class="hlt">ice</span> nucleation, but sufficiently encapsulates the <span class="hlt">activation</span> properties for potential use in regional and global modeling simulations, and possible application in developing remote sensing retrievals for <span class="hlt">ice</span> nucleating particles. A correction factor is introduced to account for the apparent underestimate (by approximately 3, on average) of the immersion freezing fraction of mineral dust particles for CSU CFDC data processed at an RH w of 105% vs. maximum fractions <span class="hlt">active</span> at higher RH w. Instrumental factors that affect <span class="hlt">activation</span> behavior vs. RH w in CFDC instruments remain to be fully explored in future studies. Nevertheless, the use of this correction factor is supported by comparison to <span class="hlt">ice</span> <span class="hlt">activation</span> data obtained for the same aerosols from Aerosol Interactions and Dynamics of the Atmosphere (AIDA) expansion chamber cloud parcel experiments. Further comparison of the new parameterization to the immersion</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1227905-integrating-laboratory-field-data-quantify-immersion-freezing-ice-nucleation-activity-mineral-dust-particles','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1227905-integrating-laboratory-field-data-quantify-immersion-freezing-ice-nucleation-activity-mineral-dust-particles"><span>Integrating laboratory and field data to quantify the immersion freezing <span class="hlt">ice</span> nucleation <span class="hlt">activity</span> of mineral dust particles</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>DeMott, P. J.; Prenni, A. J.; McMeeking, G. R.; ...</p> <p>2015-01-13</p> <p>Data from both laboratory studies and atmospheric measurements are used to develop an empirical parameterization for the immersion freezing <span class="hlt">activity</span> of natural mineral dust particles. Measurements made with the Colorado State University (CSU) continuous flow diffusion chamber (CFDC) when processing mineral dust aerosols at a nominal 105% relative humidity with respect to water (RH w) are taken as a measure of the immersion freezing nucleation <span class="hlt">activity</span> of particles. <span class="hlt">Ice</span> <span class="hlt">active</span> frozen fractions vs. temperature for dusts representative of Saharan and Asian desert sources were consistent with similar measurements in atmospheric dust plumes for a limited set of comparisons available. Themore » parameterization developed follows the form of one suggested previously for atmospheric particles of non-specific composition in quantifying <span class="hlt">ice</span> nucleating particle concentrations as functions of temperature and the total number concentration of particles larger than 0.5 μm diameter. Such an approach does not explicitly account for surface area and time dependencies for <span class="hlt">ice</span> nucleation, but sufficiently encapsulates the <span class="hlt">activation</span> properties for potential use in regional and global modeling simulations, and possible application in developing remote sensing retrievals for <span class="hlt">ice</span> nucleating particles. A calibration factor is introduced to account for the apparent underestimate (by approximately 3, on average) of the immersion freezing fraction of mineral dust particles for CSU CFDC data processed at an RH w of 105% vs. maximum fractions <span class="hlt">active</span> at higher RH w. Instrumental factors that affect <span class="hlt">activation</span> behavior vs. RH w in CFDC instruments remain to be fully explored in future studies. Nevertheless, the use of this calibration factor is supported by comparison to <span class="hlt">ice</span> <span class="hlt">activation</span> data obtained for the same aerosols from Aerosol Interactions and Dynamics of the Atmosphere (AIDA) expansion chamber cloud parcel experiments. Further comparison of the new parameterization, including</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24579057','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24579057"><span>Bacterial <span class="hlt">ice</span> crystal controlling proteins.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lorv, Janet S H; Rose, David R; Glick, Bernard R</p> <p>2014-01-01</p> <p>Across the world, many <span class="hlt">ice</span> <span class="hlt">active</span> bacteria utilize <span class="hlt">ice</span> crystal controlling proteins for aid in freezing tolerance at subzero temperatures. <span class="hlt">Ice</span> crystal controlling proteins include both antifreeze and <span class="hlt">ice</span> nucleation proteins. Antifreeze proteins minimize freezing damage by inhibiting growth of large <span class="hlt">ice</span> crystals, while <span class="hlt">ice</span> nucleation proteins induce formation of embryonic <span class="hlt">ice</span> crystals. Although both protein classes have differing functions, these proteins use the same <span class="hlt">ice</span> binding mechanisms. Rather than direct binding, it is probable that these protein classes create an <span class="hlt">ice</span> surface prior to <span class="hlt">ice</span> crystal surface adsorption. Function is differentiated by molecular size of the protein. This paper reviews the similar and different aspects of bacterial antifreeze and <span class="hlt">ice</span> nucleation proteins, the role of these proteins in freezing tolerance, prevalence of these proteins in psychrophiles, and current mechanisms of protein-<span class="hlt">ice</span> interactions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMPP14A..04L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMPP14A..04L"><span>Retreat of the Southwest Labrador Sector of the Laurentide <span class="hlt">Ice</span> Sheet During the Last Termination</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lowell, T. V.; Kelly, M. A.; Fisher, T. G.; Barnett, P. J.; Howley, J. A.; Zimmerman, S. R. H.</p> <p>2016-12-01</p> <p>Large <span class="hlt">ice</span> sheets are suspected to have played a major role in forcing the transitions from glacial to interglacial conditions, known as terminations. To improve the understanding of the role of the Laurentide <span class="hlt">Ice</span> Sheet in the last termination, we present a chronology of <span class="hlt">ice</span> sheet recession from just subsequent to end of the Last Glacial Maximum (LGM) to the early Holocene. We focus on the retreat of the southwest Labrador Sector of the <span class="hlt">ice</span> sheet in northern Minnesota and adjacent Ontario. Multiple moraines in this region mark an overall pattern of <span class="hlt">ice</span> recession interrupted by stillstands and/or minor readvances. Radiocarbon and 10Be ages from 50 sites along this 400 km-long transect indicate that the oldest moraine complex, the Vermillion moraine, formed at 17.0 ka. Subsequently, the <span class="hlt">ice</span> <span class="hlt">margin</span> retreated with minor standstills until the Dog Lake moraine was deposited between 12.7 and 12.3 ka. Recession from the Dog Lake moraine began by 12.3 ka the <span class="hlt">ice</span> <span class="hlt">margin</span> receded 150 km to the north-northeast by 10.7 ka. In general, the radiocarbon and 10Be ages define a pattern of near-continuous <span class="hlt">ice</span> sheet retreat. Deposition of the Vermillion and Dog Lake moraines occurred at the beginning of Heinrich stadials 1 ( 17.5-14.5 ka) and 0 ( 12.9-11.7 ka), respectively, but <span class="hlt">ice</span> recession occurred throughout the remainder of these stadials. This pattern is different from climate conditions registered by Greenland <span class="hlt">ice</span> cores which show cold conditions from the end of the LGM until the Bølling warming at 14.5 ka, and throughout the Younger Dryas ( 12.9-11.7 ka). We suggest that the pattern of <span class="hlt">ice</span> sheet recession is more similar to mountain glaciers in the southern mid-latitudes and tropics, and that Heinrich stadials may have been characterized by warming at least in the summertime that influenced near global <span class="hlt">ice</span> recession.</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 Antarctic 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 Antarctic 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 Antarctic 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 Antarctic is 23,800 km2/yr (2.1 %/decade). For all 12 months, trends are negative in the Arctic and positive in the Antarctic, 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 Antarctic 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> covers, 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 <span class="hlt">marginal</span> <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 Antarctic sea <span class="hlt">ice</span> coverage was not widely anticipated and explaining it remains an area of <span class="hlt">active</span> research by many scientists exploring a variety of potential explanations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMGC33G..07C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMGC33G..07C"><span>Measured Two-Dimensional <span class="hlt">Ice</span>-Wedge Polygon Thermal and <span class="hlt">Active</span> Layer Dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cable, W.; Romanovsky, V. E.; Busey, R.</p> <p>2016-12-01</p> <p><span class="hlt">Ice</span>-wedge polygons are perhaps the most dominant permafrost related features in the arctic landscape. The microtopography of these features, that includes rims, troughs, and high and low polygon centers, alters the local hydrology. During winter, wind redistribution of snow leads to an increased snowpack depth in the low areas, while the slightly higher areas often have very thin snow cover, leading to differences across the landscape in vegetation communities and soil moisture between higher and lower areas. To investigate the effect of microtopographic caused variation in surface conditions on the ground thermal regime, we established temperature transects, composed of five vertical array thermistor probes (VATP), across four different development stages of <span class="hlt">ice</span>-wedge polygons near Barrow, Alaska. Each VATP had 16 thermistors from the surface to a depth of 1.5 m, for a total of 80 temperature measurements per polygon. We found snow cover, timing and depth, and <span class="hlt">active</span> layer soil moisture to be major controlling factors in the observed thermal regimes. In troughs and in the centers of low-centered polygons, the combined effect of typically saturated soils and increased snow accumulation resulted in the highest mean annual ground temperatures (MAGT) and latest freezeback dates. While the centers of high-centered polygons, with thinner snow cover and a dryer <span class="hlt">active</span> layer, had the lowest MAGT, earliest freezeback dates, and shallowest <span class="hlt">active</span> layer. Refreezing of the <span class="hlt">active</span> layer initiated at nearly the same time for all locations and polygons however, we found large differences in the proportion of downward versus upward freezing and the length of time required to complete the refreezing process between polygon types and locations. Using our four polygon stages as a space for time substitution, we conclude that <span class="hlt">ice</span>-wedge degradation resulting in surface subsidence and trough deepening can lead to overall drying of the <span class="hlt">active</span> layer and increased skewedness of snow</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70035407','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70035407"><span>A ground penetrating radar investigation of a glacial-marine <span class="hlt">ice</span>- contact delta, Pineo Ridge, eastern coastal Maine</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Tary, A.K.; Duncan, M. FitzGerald; Weddle, T.K.</p> <p>2007-01-01</p> <p>In eastern coastal Maine, many flat-topped landforms, often identified as glacial-marine deltas, are cultivated for blueberry production. These agriculturally valuable features are not exploited for aggregate resources, severely limiting stratigraphic exposure. Coring is often forbidden; where permissible, coarse-grained surficial sediments make coring and sediment retrieval difficult. Ground penetrating radar (GPR) has become an invaluable tool in an ongoing study of the otherwise inaccessible subsurface morphology in this region and provides a means of detailing the large-scale sedimentary structures comprising these features. GPR studies allow us to reassess previous depositional interpretations and to develop alternative developmental models. The work presented here focuses on Pineo Ridge, a large, flat-topped <span class="hlt">ice-marginal</span> glacial-marine delta complex with a strong linear trend and two distinct landform zones, informally termed East Pineo and West Pineo. Previous workers have described each zone separately due to local morphological variation. Our GPR work further substantiates this geomorphic differentiation. East Pineo developed as a series of deltaic lobes prograding southward from an <span class="hlt">ice</span>-contact <span class="hlt">margin</span> during the local marine highstand. GPR data do not suggest postdepositional modification by <span class="hlt">ice-margin</span> re-advance. We suggest that West Pineo has a more complex, two-stage depositional history. The southern section of the feature consists of southward-prograding deltaic lobes deposited during retreat of the Laurentide <span class="hlt">ice</span> <span class="hlt">margin</span>, with later erosional modification during marine regression. The northern section of West Pineo formed as a series of northward-prograd- ing deltaic lobes as sediment-laden meltwater may have been diverted by the existing deposits of the southern section of West Pineo. ?? 2007 The Geological Society of America. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C14A..01W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C14A..01W"><span>Oceans Melting Greenland (OMG): 2017 Observations and the First Look at Yearly Ocean/<span class="hlt">Ice</span> Changes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Willis, J. K.; Rignot, E. J.; Fenty, I. G.; Khazendar, A.; Moller, D.; Tinto, K. J.; Morison, J.; Schodlok, M.; Thompson, A. F.; Fukumori, I.; Holland, D.; Forsberg, R.; Jakobsson, M.; Dinardo, S. J.</p> <p>2017-12-01</p> <p>Oceans Melting Greenland (OMG) is an airborne NASA Mission to investigate the role of the oceans in <span class="hlt">ice</span> loss around the <span class="hlt">margins</span> of the Greenland <span class="hlt">Ice</span> Sheet. A five-year campaign, OMG will directly measure ocean warming and glacier retreat around all of Greenland. By relating these two, we will explore one of the most pressing open questions about how climate change drives sea level rise: How quickly are the warming oceans melting the Greenland <span class="hlt">Ice</span> Sheet from the edges? This year, OMG collected its second set of both elevation maps of marine terminating glaciers and ocean temperature and salinity profiles around all of Greenland. This give us our first look at year-to-year changes in both <span class="hlt">ice</span> volume at the <span class="hlt">margins</span>, as well as the volume and extent of warm, salty Atlantic water present on the continental shelf. In addition, we will compare recent data in east Greenland waters with historical ocean observations that suggest a long-term warming trend there. Finally, we will briefly review the multi-beam sonar and airborne gravity campaigns—both of which were completed last year—and the dramatic improvement they had on bathymetry maps over the continental shelf around Greenland.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.T12A..05Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.T12A..05Y"><span>Geoologic controls on the architecture of the Antarctic <span class="hlt">Ice</span> Sheet's basal interface: New results from West and East Antarctica from long range geophysics (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Young, D. A.; Blankenship, D. D.; Greenbaum, J. S.; Richter, T.; Aitken, A.; Siegert, M. J.; Roberts, J. L.</p> <p>2013-12-01</p> <p>The <span class="hlt">ice</span>-rock interface underlying the Antarctic <span class="hlt">Ice</span> Sheet was shaped by interactions between underlying gondwanan geology and the overlying <span class="hlt">ice</span> sheet. The <span class="hlt">ice</span> sheet now preserves from sedimentary infill an incredibly rugged terrain which now plays a critical role in shaping subglacial hydrology, and thus shape <span class="hlt">ice</span> sheet behavior. This terrain can by imaged through aerogeophysical means, in particular through <span class="hlt">ice</span> penetrating radar, while airborne potential fields measurements provide insight into the geological framework that controlled erosion. Over the post IPY era, the density of airborne coverage is only now reaching the point where small scale structure can be identified and placed in context. Of particular importance is understanding the formation of focused erosional valleys, 30-50 km wide, representing now buried subglacial fjords. After initial data from the GIMBLE project in West Antarctica, and five years of sustained long range ICECAP surveys over East Antarctica , we now have a better view of the diversity of these features. The local erosion of these valleys, often cutting through significant topographic barriers, irregularly samples the underlying geology, provided a complex story in the sediment to the Antarctic <span class="hlt">margin</span>. These valleys now provide the subglacial conduits for significant <span class="hlt">ice</span> sheet catchments, in particular for subglacial water, including the inland catchments of DeVicq, Thwaites, and Pine Island Glaciers in West Antarctica, and Denman Glacier, Totten Glacier, Byrd Glacier and Cook <span class="hlt">Ice</span> Shelf in East Antarctica. We find that these features, now sometimes hundreds of kilometers inland of the modern grounding line, often nucleate on or are aligned with structure inherited from the assembly of the Antarctic continent. While many of these features currently host <span class="hlt">active</span> outlet glaciers or their tributaries, some do not, implying avenues for <span class="hlt">ice</span> sheet change. In West Antarctica, we find a new deep connection between the coast and interior basin</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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