Sample records for ice zone retreival

  1. 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.

  2. 36 CFR 13.1304 - Ice fall hazard zones.

    Code of Federal Regulations, 2014 CFR

    2014-07-01

    ... 36 Parks, Forests, and Public Property 1 2014-07-01 2014-07-01 false Ice fall hazard zones. 13.1304 Section 13.1304 Parks, Forests, and Public Property NATIONAL PARK SERVICE, DEPARTMENT OF THE... Provisions § 13.1304 Ice fall hazard zones. Entering an ice fall hazard zone is prohibited. These zones will...

  3. 36 CFR 13.1304 - Ice fall hazard zones.

    Code of Federal Regulations, 2010 CFR

    2010-07-01

    ... 36 Parks, Forests, and Public Property 1 2010-07-01 2010-07-01 false Ice fall hazard zones. 13.1304 Section 13.1304 Parks, Forests, and Public Property NATIONAL PARK SERVICE, DEPARTMENT OF THE... Provisions § 13.1304 Ice fall hazard zones. Entering an ice fall hazard zone is prohibited. These zones will...

  4. 36 CFR 13.1304 - Ice fall hazard zones.

    Code of Federal Regulations, 2011 CFR

    2011-07-01

    ... 36 Parks, Forests, and Public Property 1 2011-07-01 2011-07-01 false Ice fall hazard zones. 13.1304 Section 13.1304 Parks, Forests, and Public Property NATIONAL PARK SERVICE, DEPARTMENT OF THE... Provisions § 13.1304 Ice fall hazard zones. Entering an ice fall hazard zone is prohibited. These zones will...

  5. 36 CFR 13.1304 - Ice fall hazard zones.

    Code of Federal Regulations, 2013 CFR

    2013-07-01

    ... 36 Parks, Forests, and Public Property 1 2013-07-01 2013-07-01 false Ice fall hazard zones. 13.1304 Section 13.1304 Parks, Forests, and Public Property NATIONAL PARK SERVICE, DEPARTMENT OF THE... Provisions § 13.1304 Ice fall hazard zones. Entering an ice fall hazard zone is prohibited. These zones will...

  6. 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.

  7. Beaufort Sea ice zones as delineated by microwave imagery

    NASA Technical Reports Server (NTRS)

    Campbell, W. J.; Gloersen, P.; Webster, W. J.; Wilheit, T. T.; Ramseier, R. O.

    1976-01-01

    Microwave and infrared data were obtained from a research aircraft over the Beaufort Sea ice from the shoreline of Harrison Bay northward to a latitude of almost 81 deg N. The data acquired were compared with microwave data obtained on the surface at an approximate position of 75 deg N, 150 deg W. Over this north-south transect of the polar ice canopy it was discovered that the sea ice could be divided into five distinct zones. The shorefast sea ice was found to consist uniformly of first-year sea ice. The second zone was found to be a mixture of first-year sea ice, medium size multiyear floes, and many recently refrozen leads, polynyas, and open water; considerable shearing activity was evident in this zone. The third zone was a mixture of first-year and multiyear sea ice which had a uniform microwave signature. The fourth zone was found to be a mixture of first-year sea ice and medium-to-large size multiyear floes which was similar in composition to the second zone. The fifth zone was almost exclusively multiyear ice extending to the North Pole.

  8. 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.

  9. 76 FR 1362 - Safety Zone; Ice Conditions for the Baltimore Captain of Port Zone

    Federal Register 2010, 2011, 2012, 2013, 2014

    2011-01-10

    ...-AA00 Safety Zone; Ice Conditions for the Baltimore Captain of Port Zone AGENCY: Coast Guard, DHS... protect mariners from the hazards associated with ice in the navigable waterways. DATES: This rule is... necessary to protect persons and vessels against the hazards associated with ice on navigable waters. Such...

  10. 78 FR 12595 - Safety Zone for Ice Conditions; Baltimore Captain of the Port Zone

    Federal Register 2010, 2011, 2012, 2013, 2014

    2013-02-25

    ... 1625-AA00 Safety Zone for Ice Conditions; Baltimore Captain of the Port Zone AGENCY: Coast Guard, DHS... protect mariners from the hazards associated with ice in the navigable waterways. DATES: This rule has... vessels against the hazards associated with ice on navigable waters. Such hazards include vessels becoming...

  11. SIPEX--Exploring the Antarctic Sea Ice Zone

    ERIC Educational Resources Information Center

    Zicus, Sandra; Dobson, Jane; Worby, Anthony

    2008-01-01

    Sea ice in the polar regions plays a key role in both regulating global climate and maintaining marine ecosystems. The international Sea Ice Physics and Ecosystem eXperiment (SIPEX) explored the sea ice zone around Antarctica in September and October 2007, investigating relationships between the physical sea ice environment and the structure of…

  12. 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

  13. 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.

  14. 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

  15. Seasonal Ice Zone Reconnaissance Surveys Coordination

    DTIC Science & Technology

    2013-09-30

    of SIZRS are covered in separate reports. Our long-term goal is to track and understand the interplay among the ice, atmosphere, and ocean...OMB control number. 1. REPORT DATE 30 SEP 2013 2. REPORT TYPE 3. DATES COVERED 00-00-2013 to 00-00-2013 4. TITLE AND SUBTITLE Seasonal Ice Zone...sensing resources include MODIS visible and IR imagery, NSIDC ice extent charts based on a composite of passive microwave products (http://nsidc.org

  16. 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.

  17. 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

  18. 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.

  19. Contrasts in Sea Ice Deformation and Production in the Arctic Seasonal and Perennial Ice Zones

    NASA Technical Reports Server (NTRS)

    Kwok, K.

    2006-01-01

    Four years (1997-2000) of RADARSAT Geophysical Processor System (RGPS) data are used to contrast the sea ice deformation and production regionally, and in the seasonal (SIZ) and perennial (PIZ) ice zones. Ice production is of seasonal ice in openings during the winter. Three-day estimates of these quantities are provided within Lagrangian elements initially 10 km on a side. A distinct seasonal cycle is seen in both zones with these estimates highest in the late fall and with seasonal minimums in the midwinter. Regional divergence over the winter could be up to 30%. Spatially, the highest deformation is seen in the SIZ north of coastal Alaska. Both ice deformation and production are higher in the SIZ: deformation-related ice production in the SIZ (approx.0.5 m) is 1.5-2.3 times that of the PIZ (approx.0.3 m): this is connected to ice strength and thickness. Atmospheric forcing and boundary layer structure contribute to only the seasonal and interannual variability. Seasonal ice growth in ice fractures accounts for approx.25-40% of the total ice production of the Arctic Ocean. Uncertainties in these estimates are discussed. By itself, this deformation-ice production relationship could be considered a negative feedback when thickness is perturbed. However, the overall effect on ice production in the face of increasing seasonal and thinner/weaker ice coverage could be modified by local destabilization of the water column promoting overturning of warmer water due to increased brine rejection; and the upwelling of the pynocline associated with increased occurrence of large shear motion in sea ice. Divergence is shown to be negligibly correlated to cyclonic motion in summer and winter in both ice zones.

  20. 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.

  1. 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.

  2. Aircraft Surveys of the Beaufort Sea Seasonal Ice Zone

    NASA Astrophysics Data System (ADS)

    Morison, J.

    2016-02-01

    The Seasonal Ice Zone Reconnaissance Surveys (SIZRS) is a program of repeated ocean, ice, and atmospheric measurements across the Beaufort-Chukchi sea seasonal sea ice zone (SIZ) utilizing US Coast Guard Arctic Domain Awareness (ADA) flights of opportunity. The SIZ is the region between maximum winter sea ice extent and minimum summer sea ice extent. As such, it contains the full range of positions of the marginal ice zone (MIZ) where sea ice interacts with open water. The increasing size and changing air-ice-ocean properties of the SIZ are central to recent reductions in Arctic sea ice extent. The changes in the interplay among the atmosphere, ice, and ocean require a systematic SIZ observational effort of coordinated atmosphere, ice, and ocean observations covering up to interannual time-scales, Therefore, every year beginning in late Spring and continuing to early Fall, SIZRS makes monthly flights across the Beaufort Sea SIZ aboard Coast Guard C-130H aircraft from USCG Air Station Kodiak dropping Aircraft eXpendable CTDs (AXCTD) and Aircraft eXpendable Current Profilers (AXCP) for profiles of ocean temperature, salinity and shear, dropsondes for atmospheric temperature, humidity, and velocity profiles, and buoys for atmosphere and upper ocean time series. Enroute measurements include IR imaging, radiometer and lidar measurements of the sea surface and cloud tops. SIZRS also cooperates with the International Arctic Buoy Program for buoy deployments and with the NOAA Earth System Research Laboratory atmospheric chemistry sampling program on board the aircraft. Since 2012, SIZRS has found that even as SIZ extent, ice character, and atmospheric forcing varies year-to-year, the pattern of ocean freshening and radiative warming south of the ice edge is consistent. The experimental approach, observations and extensions to other projects will be discussed.

  3. Ocean Profile Measurements During the Seasonal Ice Zone Reconnaissance Surveys Ocean Profiles

    DTIC Science & Technology

    2017-01-01

    repeated ocean, ice, and atmospheric measurements across the Beaufort-Chukchi sea seasonal sea ice zone (SIZ) utilizing US Coast Guard Arctic Domain...contributing to the rapid decline in summer ice extent that has occurred in recent years. The SIZ is the region between maximum winter sea ice extent and...minimum summer sea ice extent. As such, it contains the full range of positions of the marginal ice zone (MIZ) where sea ice interacts with open water

  4. 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.

  5. 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.

  6. 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.

  7. 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.

  8. Contrasts in Sea Ice Formation and Production in the Arctic Seasonal and Perennial Ice Zones

    NASA Technical Reports Server (NTRS)

    Kwok, R.

    2006-01-01

    Four years (1997-2000) of RADARSAT Geophysical Processor System (RGPS) data are used to contrast the sea ice deformation and production regionally, and in the seasonal (SIZ) and perennial (PIZ) ice zones. Ice production is of seasonal ice in openings during the winter. 3-day estimates of these quantities are provided within Lagrangian elements initially 10 km on a side. A distinct seasonal cycle is seen in both zones with these estimates highest in the late fall and with seasonal minimums in the mid-winter. Regional divergence over the winter could be up to 30%. Spatially, the highest deformation is in the SIZ north of coastal Alaska. Both ice deformation and production are higher in the SIZ: deformation-related ice production in the SIZ (approx.0.5 m) is 1.5-2.3 times that of the PIZ (approx.0.3 m) - this is connected to ice strength and thickness. Atmospheric forcing and boundary layer structure contribute to only the seasonal and interannual variability. Seasonal ice growth in ice fractures accounts for approx.25-40% of the total ice production of the Arctic Ocean. By itself, this deformation-ice production relationship could be considered a negative feedback when thickness is perturbed. However, the overall effect on ice production in the face of increasing seasonal and thinner/weaker ice coverage could be modified by: local destabilization of the water column promoting overturning of warmer water due to increased brine rejection; and, the upwelling of the pynocline associated with increased occurrence of large shear motion in sea ice.

  9. Sediment features at the grounding zone and beneath Ekström Ice Shelf, East Antarctica, imaged using on-ice vibroseis.

    NASA Astrophysics Data System (ADS)

    Smith, Emma C.; Eisen, Olaf; Hofstede, Coen; Lambrecht, Astrid; Mayer, Christoph

    2017-04-01

    The grounding zone, where an ice sheet becomes a floating ice shelf, is known to be a key threshold region for ice flow and stability. A better understanding of ice dynamics and sediment transport across such zones will improve knowledge about contemporary and palaeo ice flow, as well as past ice extent. Here we present a set of seismic reflection profiles crossing the grounding zone and continuing to the shelf edge of Ekström Ice Shelf, East Antarctica. Using an on-ice vibroseis source combined with a snowstreamer we have imaged a range of sub-glacial and sub-shelf sedimentary and geomorphological features; from layered sediment deposits to elongated flow features. The acoustic properties of the features as well as their morphology allow us to draw conclusions as to their material properties and origin. These results will eventually be integrated with numerical models of ice dynamics to quantify past and present interactions between ice and the solid Earth in East Antarctica; leading to a better understanding of future contributions of this region to sea-level rise.

  10. 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.

  11. Ocean stratification reduces melt rates at the grounding zone of the Ross Ice Shelf

    NASA Astrophysics Data System (ADS)

    Begeman, C. B.; Tulaczyk, S. M.; Marsh, O.; Mikucki, J.; Stanton, T. P.; Hodson, T. O.; Siegfried, M. R.; Powell, R. D.; Christianson, K. A.; King, M. A.

    2017-12-01

    Ocean-driven melting of ice shelves is often invoked as the primary mechanism for triggering ice loss from Antarctica. However, due to the difficulty in accessing the sub-ice-shelf ocean cavity, the relationship between ice-shelf melt rates and ocean conditions is poorly understood, particularly near the transition from grounded to floating ice, known as the grounding zone. Here we present the first borehole oceanographic observations from the grounding zone of Antarctica's largest ice shelf. Contrary to predictions that tidal currents near grounding zones should mix the water column, driving high ice-shelf melt rates, we find a stratified sub-ice-shelf water column. The vertical salinity gradient dominates stratification over a weakly unstable vertical temperature gradient; thus, stratification takes the form of a double-diffusive staircase. These conditions limit vertical heat fluxes and lead to low melt rates in the ice-shelf grounding zone. While modern grounding zone melt rates may presently be overestimated in models that assume efficient tidal mixing, the high sensitivity of double-diffusive staircases to ocean freshening and warming suggests future melt rates may be underestimated, biasing projections of global sea-level rise.

  12. 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.

  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. 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.

  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. 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

  17. 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.

  18. Biologically-Oriented Processes in the Coastal Sea Ice Zone of the White Sea

    NASA Astrophysics Data System (ADS)

    Melnikov, I. A.

    2002-12-01

    The annual advance and retreat of sea ice is a major physical determinant of spatial and temporal changes in the structure and function of marine coastal biological communities. Sea ice biological data obtained in the tidal zone of Kandalaksha Gulf (White Sea) during 1996-2001 period will be presented. Previous observations in this area were mainly conducted during the ice-free summer season. However, there is little information on the ice-covered winter season (6-7 months duration), and, especially, on the sea-ice biology in the coastal zone within tidal regimes. During the January-May period time-series observations were conducted on transects along shorelines with coastal and fast ice. Trends in the annual extent of sea ice showed significant impacts on ice-associated biological communities. Three types of sea ice impact on kelps, balanoides, littorinas and amphipods are distinguished: (i) positive, when sea ice protects these populations from grinding (ii) negative, when ice grinds both fauna and flora, and (iii) a combined effect, when fast ice protects, but anchored ice grinds plant and animals. To understand the full spectrum of ecological problems caused by pollution on the coastal zone, as well as the problems of sea ice melting caused by global warming, an integrated, long-term study of the physical, chemical, and biological processes is needed.

  19. 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.

  20. Meltwater storage in low-density near-surface bare ice in the Greenland ice sheet ablation zone

    NASA Astrophysics Data System (ADS)

    Cooper, Matthew G.; Smith, Laurence C.; Rennermalm, Asa K.; Miège, Clément; Pitcher, Lincoln H.; Ryan, Jonathan C.; Yang, Kang; Cooley, Sarah W.

    2018-03-01

    We document the density and hydrologic properties of bare, ablating ice in a mid-elevation (1215 m a.s.l.) supraglacial internally drained catchment in the Kangerlussuaq sector of the western Greenland ice sheet. We find low-density (0.43-0.91 g cm-3, μ = 0.69 g cm-3) ice to at least 1.1 m depth below the ice sheet surface. This near-surface, low-density ice consists of alternating layers of water-saturated, porous ice and clear solid ice lenses, overlain by a thin (< 0.5 m), even lower density (0.33-0.56 g cm-3, μ = 0.45 g cm-3) unsaturated weathering crust. Ice density data from 10 shallow (0.9-1.1 m) ice cores along an 800 m transect suggest an average 14-18 cm of specific meltwater storage within this low-density ice. Water saturation of this ice is confirmed through measurable water levels (1-29 cm above hole bottoms, μ = 10 cm) in 84 % of cryoconite holes and rapid refilling of 83 % of 1 m drilled holes sampled along the transect. These findings are consistent with descriptions of shallow, depth-limited aquifers on the weathered surface of glaciers worldwide and confirm the potential for substantial transient meltwater storage within porous low-density ice on the Greenland ice sheet ablation zone surface. A conservative estimate for the ˜ 63 km2 supraglacial catchment yields 0.009-0.012 km3 of liquid meltwater storage in near-surface, porous ice. Further work is required to determine if these findings are representative of broader areas of the Greenland ice sheet ablation zone, and to assess the implications for sub-seasonal mass balance processes, surface lowering observations from airborne and satellite altimetry, and supraglacial runoff processes.

  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. 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. 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.

  4. 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.

  5. 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.

  6. Radon and radium in the ice-covered Arctic Ocean, and what they reveal about gas exchange in the sea ice zone.

    NASA Astrophysics Data System (ADS)

    Loose, B.; Kelly, R. P.; Bigdeli, A.; Moran, S. B.

    2014-12-01

    The polar sea ice zones are regions of high primary productivity and interior water mass formation. Consequently, the seasonal sea ice cycle appears important to both the solubility and biological carbon pumps. To estimate net CO2 transfer in the sea ice zone, we require accurate estimates of the air-sea gas transfer velocity. In the open ocean, the gas transfer velocity is driven by wind, waves and bubbles - all of which are strongly altered by the presence of sea ice, making it difficult to translate open ocean estimates of gas transfer to the ice zone. In this study, we present profiles of 222Rn and 226Ra throughout the mixed-layer and euphotic zone. Profiles were collected spanning a range of sea ice cover conditions from 40 to 100%. The profiles of Rn/Ra can be used to estimate the gas transfer velocity, but the 3.8 day half-life of 222Rn implies that mixed layer radon will have a memory of the past ~20 days of gas exchange forcing, which may include a range of sea ice cover conditions. Here, we compare individual estimates of the gas transfer velocity to the turbulent forcing conditions constrained from shipboard and regional reanalysis data to more appropriately capture the time history upper ocean Rn/Ra.

  7. A Microwave Technique for Mapping Ice Temperature in the Arctic Seasonal Sea Ice Zone

    NASA Technical Reports Server (NTRS)

    St.Germain, Karen M.; Cavalieri, Donald J.

    1997-01-01

    A technique for deriving ice temperature in the Arctic seasonal sea ice zone from passive microwave radiances has been developed. The algorithm operates on brightness temperatures derived from the Special Sensor Microwave/Imager (SSM/I) and uses ice concentration and type from a previously developed thin ice algorithm to estimate the surface emissivity. Comparisons of the microwave derived temperatures with estimates derived from infrared imagery of the Bering Strait yield a correlation coefficient of 0.93 and an RMS difference of 2.1 K when coastal and cloud contaminated pixels are removed. SSM/I temperatures were also compared with a time series of air temperature observations from Gambell on St. Lawrence Island and from Point Barrow, AK weather stations. These comparisons indicate that the relationship between the air temperature and the ice temperature depends on ice type.

  8. 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.

  9. 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.

  10. 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.

  11. 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.

  12. The structure and effect of suture zones in the Larsen C Ice Shelf, Antarctica

    NASA Astrophysics Data System (ADS)

    McGrath, Daniel; Steffen, Konrad; Holland, Paul R.; Scambos, Ted; Rajaram, Harihar; Abdalati, Waleed; Rignot, Eric

    2014-03-01

    Ice shelf fractures frequently terminate where they encounter suture zones, regions of material heterogeneity that form between meteoric inflows in ice shelves. This heterogeneity can consist of marine ice, meteoric ice with modified rheological properties, or the presence of fractures. Here, we use radar observations on the Larsen C Ice Shelf, Antarctica, to investigate (i) the termination of a 25 km long rift in the Churchill Peninsula suture zone, which was found to contain 60 m of accreted marine ice, and (ii) the along-flow evolution of a suture zone originating at Cole Peninsula. We determine a steady state field of basal melting/freezing rates and apply it to a flowline model to delineate the along-flow evolution of layers within the ice shelf. The thickening surface wedge of locally accumulated meteoric ice, which likely has limited lateral variation in its mechanical properties, accounts for 60% of the total ice thickness near the calving front. Thus, we infer that the lower 40% of the ice column and the material heterogeneities present there are responsible for resisting fracture propagation and thereby delaying tabular calving events, as demonstrated in the >40 year time series leading up to the 2004/2005 calving event for Larsen C. This likely represents a highly sensitive aspect of ice shelf stability, as changes in the oceanic forcing may lead to the loss of this heterogeneity.

  13. 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

  14. 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.

  15. Acquisition of Ice Thickness and Ice Surface Characteristics in the Seasonal Ice Zone by CULPIS-X during the US Coast Guard’s Arctic Domain Awareness Program

    DTIC Science & Technology

    2014-09-30

    OBJECTIVES • What is the volume of sea ice in the Beaufort Sea Seasonal Ice Zone (SIZ) and how does this evolve during summer as the ice edge...retreats? Recent observations suggest that the remaining ice in the Beaufort Sea is younger and thinner in recent years in part because even the oldest...surrounding ice . Recent analyses have indicated that ponds on thinner ice are often darker, accelerating the ice - albedo feedback over thin ice in summer

  16. 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

  17. An Examination of the Sea Ice Rheology for Seasonal Ice Zones Based on Ice Drift and Thickness Observations

    NASA Astrophysics Data System (ADS)

    Toyota, Takenobu; Kimura, Noriaki

    2018-02-01

    The validity of the sea ice rheological model formulated by Hibler (1979), which is widely used in present numerical sea ice models, is examined for the Sea of Okhotsk as an example of the seasonal ice zone (SIZ), based on satellite-derived sea ice velocity, concentration and thickness. Our focus was the formulation of the yield curve, the shape of which can be estimated from ice drift pattern based on the energy equation of deformation, while the strength of the ice cover that determines its magnitude was evaluated using ice concentration and thickness data. Ice drift was obtained with a grid spacing of 37.5 km from the AMSR-E 89 GHz brightness temperature using a maximum cross-correlation method. The ice thickness was obtained with a spatial resolution of 100 m from a regression of the PALSAR backscatter coefficients with ice thickness. To assess scale dependence, the ice drift data derived from a coastal radar covering a 70 km range in the southernmost Sea of Okhotsk were similarly analyzed. The results obtained were mostly consistent with Hibler's formulation that was based on the Arctic Ocean on both scales with no dependence on a time scale, and justify the treatment of sea ice as a plastic material, with an elliptical shaped yield curve to some extent. However, it also highlights the difficulty in parameterizing sub-grid scale ridging in the model because grid scale ice velocities reduce the deformation magnitude by half due to the large variation of the deformation field in the SIZ.

  18. 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

  19. 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.

  20. Micromechanics of sea ice gouge in shear zones

    NASA Astrophysics Data System (ADS)

    Sammonds, Peter; Scourfield, Sally; Lishman, Ben

    2015-04-01

    The deformation of sea ice is a key control on the Arctic Ocean dynamics. Shear displacement on all scales is an important deformation process in the sea cover. Shear deformation is a dominant mechanism from the scale of basin-scale shear lineaments, through floe-floe interaction and block sliding in ice ridges through to the micro-scale mechanics. Shear deformation will not only depend on the speed of movement of ice surfaces but also the degree that the surfaces have bonded during thermal consolidation and compaction. Recent observations made during fieldwork in the Barents Sea show that shear produces a gouge similar to a fault gouge in a shear zone in the crust. A range of sizes of gouge are exhibited. The consolidation of these fragments has a profound influence on the shear strength and the rate of the processes involved. We review experimental results in sea ice mechanics from mid-scale experiments, conducted in the Hamburg model ship ice tank, simulating sea ice floe motion and interaction and compare these with laboratory experiments on ice friction done in direct shear, and upscale to field measurement of sea ice friction and gouge deformation made during experiments off Svalbard. We find that consolidation, fragmentation and bridging play important roles in the overall dynamics and fit the model of Sammis and Ben-Zion, developed for understanding the micro-mechanics of rock fault gouge, to the sea ice problem.

  1. 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

  2. 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.

  3. Basal crevasses and suture zones in the Larsen C Ice Shelf, Antarctica: Implications for ice shelf stability in a warming climate

    NASA Astrophysics Data System (ADS)

    McGrath, Daniel J.

    Understanding ice shelf structure and processes is paramount to future predictions of sea level rise, as nearly 75% of the ice flux from the Antarctic Ice Sheet (AIS) passes through these gates. The breakup of an ice shelf removes the longitudinal back stress acting on the grounded inland ice and leads to flow acceleration, dynamic thinning and frontal retreat, processes that can be sustained for more than a decade. Increased ice discharge to the ocean contributes to global sea level rise. This dissertation investigates basal crevasses and suture zones, two key structural components of ice shelves, in order to understand how the structure of an ice shelf influences its stability in a warming climate. Ground penetrating radar, high-resolution satellite imagery and a variety of modeling approaches are utilized to assess these features on the Larsen C Ice Shelf but in a manner that considers their influence on ice shelf stability around the AIS. Basal crevasses are large-scale (~66% of ice thickness and ten's of kms in length) and abundant features that are significant structural weaknesses. The viscoplastic deformation of the ice shelf in response to the perturbed hydrostatic balance leads to the formation of both surface depressions and crevasses, hence weakening the ice shelf further. Basal crevasses increase the local ice-ocean interface by ~30%, thereby increasing basal roughness and altering ice-ocean interactions. Ice-shelf fractures frequently terminate where they encounter suture zones, regions of material heterogeneity that form at the lateral bounds of meteoric inflows to ice shelves. The termination of a 25 km-long rift in the Churchill Peninsula suture zone is investigated and found to contain ~60 m of accreted marine ice. Steady-state basal melting/freezing rates are determined for the ice shelf and applied to a flowline model to examine the along-flow evolution of ice shelf structure. The thickening surface wedge of locally accumulated meteoric ice

  4. 36 CFR 13.1304 - Ice fall hazard zones.

    Code of Federal Regulations, 2012 CFR

    2012-07-01

    ... 36 Parks, Forests, and Public Property 1 2012-07-01 2012-07-01 false Ice fall hazard zones. 13.1304 Section 13.1304 Parks, Forests, and Public Property NATIONAL PARK SERVICE, DEPARTMENT OF THE INTERIOR NATIONAL PARK SYSTEM UNITS IN ALASKA Special Regulations-Kenai Fjords National Park General...

  5. 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.

  6. POROSITY AND BAND-STRENGTH MEASUREMENTS OF MULTI-PHASE COMPOSITE ICES

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

    Bossa, Jean-Baptiste; Fransen, Coen; Cazaux, Stéphanie

    2015-11-20

    We use experimental mid-infrared optical constants and extended effective medium approximations to determine the porosity and the band strengths of multi-phase composite ices grown at 30 K. A set of porous H{sub 2}O:CH{sub 4} ices are taken as a prototypical example. As a benchmark and proof of concept, the stoichiometry of the ice constituents is retreived with good accuracy from the refractive indices and the extinction coefficients of the reference binary ice mixtures with known compositions. Accurate band strengths are then calculated from experimental mid-infrared spectra of complex ices. We notice that the presence of pores has only a smallmore » effect on the overall band strengths, whereas a water dilution can considerably alter them. Different levels of porosity are observed depending on the abundance of methane used as a gas contaminant premixed with water prior to background deposition. The absorption profiles are also found to vary with deposition rate. To explain this, we use Monte Carlo simulations and we observe that the deposition rate strongly affects the pore size distribution as well as the ice morphology through reorganization processes. Extrapolated to genuine interstellar ices, the methodology presented in this paper can be used to evaluate the porosity and to quantify the relative abundances from observational data.« less

  7. Aerial Surveys of the Beaufort Sea Seasonal Ice Zone in 2012-2014

    NASA Astrophysics Data System (ADS)

    Dewey, S.; Morison, J.; Andersen, R.; Zhang, J.

    2014-12-01

    Seasonal Ice Zone Reconnaissance Surveys (SIZRS) of the Beaufort Sea aboard U.S. Coast Guard Arctic Domain Awareness flights were made monthly from May 2012 to October 2012, June 2013 to August 2013, and June 2014 to October 2014. In 2012 sea ice extent reached a record minimum and the SIZRS sampling ranged from complete ice cover to open water; in addition to its large spatial coverage, the SIZRS program extends temporal coverage of the seasonal ice zone (SIZ) beyond the traditional season for ship-based observations, and is a good set of measurements for model validation and climatological comparison. The SIZ, where ice melts and reforms annually, encompasses the marginal ice zone (MIZ). Thus SIZRS tracks interannual MIZ conditions, providing a regional context for smaller-scale MIZ processes. Observations with Air eXpendable CTDs (AXCTDs) reveal two near-surface warm layers: a locally-formed surface seasonal mixed layer and a layer of Pacific origin at 50-60m. Temperatures in the latter differ from the freezing point by up to 2°C more than climatologies. To distinguish vertical processes of mixed layer formation from Pacific advection, vertical heat and salt fluxes are quantified using a 1-D Price-Weller-Pinkel (PWP) model adapted for ice-covered seas. This PWP simulates mixing processes in the top 100m of the ocean. Surface forcing fluxes are taken from the Marginal Ice Zone Modeling and Assimilation System MIZMAS. Comparison of SIZRS observations with PWP output shows that the ocean behaves one-dimensionally above the Pacific layer of the Beaufort Gyre. Despite agreement with the MIZMAS-forced PWP, SIZRS observations remain fresher to 100m than do outputs from MIZMAS and ECCO.2. The shapes of seasonal cycles in SIZRS salinity and temperature agree with MIZMAS and ECCO.2 model outputs despite differences in the values of each. However, the seasonal change of surface albedo is not high enough resolution to accurately drive the PWP. Use of ice albedo

  8. 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.

  9. 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.

  10. 22-year surface salinity changes in the Seasonal Ice Zone near 140°E off Antarctica

    NASA Astrophysics Data System (ADS)

    Morrow, Rosemary; Kestenare, Elodie

    2017-11-01

    Seasonal and interannual variations in sea surface salinity (SSS) are analyzed in the Sea Ice Zone south of 60°S, from a 22-year time series of observations near 140°E. In the northern sea-ice zone during the warming, melting cycle from October to March, waters warm by an average of 3.5 °C and become fresher by 0.1 to 0.25. In the southern sea-ice zone, the surface temperatures vary from - 1 to 1 °C over summer, and the maximal SSS range occurs in December, with a minimum SSS of 33.65 near the Southern Boundary of the ACC, reaching 34.4 in the shelf waters close to the coast. The main fronts, normally defined at subsurface, are shown to have more distinct seasonal characteristics in SSS than in SST. The interannual variations in SSS are more closely linked to variations in upstream sea-ice cover than surface forcing. SSS and sea-ice variations show distinct phases, with large biannual variations in the early 1990s, weaker variations in the 2000s and larger variations again from 2009 onwards. The calving of the Mertz Glacier Tongue in February 2010 leads to increased sea-ice cover and widespread freshening of the surface layers from 2011 onwards. Summer freshening in the northern sea-ice zone is 0.05-0.07 per decade, increasing to 0.08 per decade in the southern sea-ice zone, largely influenced by the Mertz Glacier calving event at the end of our time series. The summer time series of SSS on the shelf at 140°E is in phase but less variable than the SSS observed upstream in the Adélie Depression, and thus represents a spatially integrated index of the wider SSS variations.

  11. Atmospheric Profiles, Clouds and the Evolution of Sea Ice Cover in the Beaufort and Chukchi Seas: Atmospheric Observations and Modeling as Part of the Seasonal Ice Zone Reconnaissance Surveys

    DTIC Science & Technology

    2017-06-04

    Ice Zone Reconnai ssance Survey project (SIZRS). Combined with oceanographic and sea ice components of the SIZRS project. The projects i dentified...with clear , warm advection events . 1S. SUBJECT TERMS Sea i ce, atmosphere , sea ice retreat , Seasonal Ice Zone Reconnaissance Survey , SIZRS , model...Reconnaissance Surveys Axel Schweiger Applied Physics Laboratory, University of Washington, 1013 NE 40th St., Seattle, Wa. 98105 phone: (206) 543

  12. 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.

  13. A Comparison of Sea Ice Type, Sea Ice Temperature, and Snow Thickness Distributions in the Arctic Seasonal Ice Zones with the DMSP SSM/I

    NASA Technical Reports Server (NTRS)

    St.Germain, Karen; Cavalieri, Donald J.; Markus, Thorsten

    1997-01-01

    Global climate studies have shown that sea ice is a critical component in the global climate system through its effect on the ocean and atmosphere, and on the earth's radiation balance. Polar energy studies have further shown that the distribution of thin ice and open water largely controls the distribution of surface heat exchange between the ocean and atmosphere within the winter Arctic ice pack. The thickness of the ice, the depth of snow on the ice, and the temperature profile of the snow/ice composite are all important parameters in calculating surface heat fluxes. In recent years, researchers have used various combinations of DMSP SSMI channels to independently estimate the thin ice type (which is related to ice thickness), the thin ice temperature, and the depth of snow on the ice. In each case validation efforts provided encouraging results, but taken individually each algorithm gives only one piece of the information necessary to compute the energy fluxes through the ice and snow. In this paper we present a comparison of the results from each of these algorithms to provide a more comprehensive picture of the seasonal ice zone using passive microwave observations.

  14. Microphysical characteristics of squall-line stratiform precipitation and transition zones inferred using an ice particle property-evolving model

    NASA Astrophysics Data System (ADS)

    Jensen, A. A.; Harrington, J. Y.; Morrison, H.

    2017-12-01

    A quasi-idealized 3D squall line (based on a June 2007 Oklahoma case) is simulated using a novel bulk microphysics scheme called the Ice-Spheroids Habit Model with Aspect-ratio Evolution (ISHMAEL). In ISHMAEL, the evolution of ice particle properties, such as mass, shape, maximum diameter, density, and fall speed, are tracked as these properties evolve from vapor growth, sublimation, riming, and melting. Thus, ice properties evolve from various microphysical processes without needing separate unrimed and rimed ice categories. Simulation results show that ISHMAEL produces both a squall-line transition zone and an enhanced stratiform precipitation region. The ice particle properties produced in this simulation are analyzed and compared to observations to determine the characteristics of ice that lead to the development of these squall-line features. It is shown that rimed particles advected rearward from the convective region produce the enhanced stratiform precipitation region. The development of the transition zone results from hydrometer sorting: the evolution of ice particle properties in the convective region produces specific fall speeds that favor significant ice advecting rearward of the transition zone before reaching the melting level, causing a local minimum in precipitation rate and reflectivity there. Microphysical sensitivity studies, for example turning rime splintering off, that lead to changes in ice particle properties reveal that the fall speed of ice particles largely determines both the location of the enhanced stratiform precipitation region and whether or not a transition zone forms.

  15. 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.

  16. 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.

  17. Bimodal albedo distributions in the ablation zone of the southwestern Greenland Ice Sheet

    NASA Astrophysics Data System (ADS)

    Moustafa, S. E.; Rennermalm, A. K.; Smith, L. C.; Miller, M. A.; Mioduszewski, J. R.

    2014-09-01

    Surface albedo is a key variable controlling solar radiation absorbed at the Greenland Ice Sheet (GrIS) surface, and thus, meltwater production. Recent decline in surface albedo over the GrIS has been linked to enhanced snow grain metamorphic rates and amplified ice-albedo feedback from atmospheric warming. However, the importance of distinct surface types on ablation zone albedo and meltwater production is still relatively unknown, and excluded in surface mass balance models. In this study, we analyze albedo and ablation rates using in situ and remotely-sensed data. Observations include: (1) a new high-quality in situ spectral albedo dataset collected with an Analytical Spectral Devices (ASD) spectroradiometer measuring at 325-1075 nm, along a 1.25 km transect during three days in June 2013; (2) broadband albedo at two automatic weather stations; and (3) daily MODerate Resolution Imaging Spectroradiometer (MODIS) albedo (MOD10A1) between 31 May and 30 August. We find that seasonal ablation zone albedos have a bimodal distribution, with two alternate states. This suggests that an abrupt switch from high to low albedo can be triggered by a modest melt event, resulting in amplified surface ablation rates. Our results show that such a shift corresponds to an observed melt rate percent difference increase of 51.6% during peak melt season (between 10-14 and 20-24 July 2013). Furthermore, our findings demonstrate that seasonal changes in GrIS ablation zone albedo are not exclusively a function of a darkening surface from ice crystal growth, but rather are controlled by changes in the fractional coverage of snow, bare ice, and impurity-rich surface types. As the climate continues to warm, regional climate models should consider the seasonal evolution of ice surface types in Greenland's ablation zone to improve projections of mass loss contributions to sea level rise.

  18. Bimodal Albedo Distributions in the Ablation Zone of the Southwestern Greenland Ice Sheet

    NASA Astrophysics Data System (ADS)

    Moustafa, S.; Rennermalm, A. K.; Smith, L. C.; Miller, M. A.; Mioduszewski, J.; Koenig, L.

    2014-12-01

    Surface albedo is a key variable controlling solar radiation absorbed at the Greenland Ice Sheet (GrIS) surface, and thus meltwater production. Recent decline in surface albedo over the GrIS has been linked to enhanced snow grain metamorphic rates and amplified ice-albedo feedback from atmospheric warming. However, the importance of distinct surface types on ablation zone albedo and meltwater production is still relatively unknown, and excluded in surface mass balance models. In this study, we analyze albedo and ablation rates (m d-1) using in situ and remotely-sensed data. Observations include: 1) a new high-quality in situ spectral albedo dataset collected with an Analytical Spectral Devices (ASD) spectroradiometer measuring at 325-1075 nm, along a 1.25 km transect during three days in June 2013; 2) broadband albedo at two automatic weather stations; and 3) daily MODerate Resolution Imaging Spectroradiometer (MODIS) albedo (MOD10A1) between 31 May and 30 August. We find that seasonal ablation zone albedos have a bimodal distribution, with two alternate states. This suggests that an abrupt switch from high to low albedo can be triggered by a modest melt event, resulting in amplified ablation rates. Our results show that such a shift corresponds to an observed melt rate percent difference increase of 51.6% during peak melt season (between 10-14 July and 20-24 July, 2013). Furthermore, our findings demonstrate that seasonal changes in GrIS ablation zone albedo are not exclusively a function of a darkening surface from ice crystal growth, but rather are controlled by changes in the fractional coverage of snow, bare ice, and impurity-rich surface types. As the climate continues to warm, regional climate models should consider the seasonal evolution of ice surface types in Greenland's ablation zone to improve projections of mass loss contributions to sea level rise.

  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. Propagation of acoustic-gravity waves in arctic zones with elastic ice-sheets

    NASA Astrophysics Data System (ADS)

    Kadri, Usama; Abdolali, Ali; Kirby, James T.

    2017-04-01

    We present an analytical solution of the boundary value problem of propagating acoustic-gravity waves generated in the ocean by earthquakes or ice-quakes in arctic zones. At the surface, we assume elastic ice-sheets of a variable thickness, and show that the propagating acoustic-gravity modes have different mode shape than originally derived by Ref. [1] for a rigid ice-sheet settings. Computationally, we couple the ice-sheet problem with the free surface model by Ref. [2] representing shrinking ice blocks in realistic sea state, where the randomly oriented ice-sheets cause inter modal transition at the edges and multidirectional reflections. We then derive a depth-integrated equation valid for spatially slowly varying thickness of ice-sheet and water depth. Surprisingly, and unlike the free-surface setting, here it is found that the higher acoustic-gravity modes exhibit a larger contribution. These modes travel at the speed of sound in water carrying information on their source, e.g. ice-sheet motion or submarine earthquake, providing various implications for ocean monitoring and detection of quakes. In addition, we found that the propagating acoustic-gravity modes can result in orbital displacements of fluid parcels sufficiently high that may contribute to deep ocean currents and circulation, as postulated by Refs. [1, 3]. References [1] U. Kadri, 2016. Generation of Hydroacoustic Waves by an Oscillating Ice Block in Arctic Zones. Advances in Acoustics and Vibration, 2016, Article ID 8076108, 7 pages http://dx.doi.org/10.1155/2016/8076108 [2] A. Abdolali, J. T. Kirby and G. Bellotti, 2015, Depth-integrated equation for hydro-acoustic waves with bottom damping, J. Fluid Mech., 766, R1 doi:10.1017/jfm.2015.37 [3] U. Kadri, 2014. Deep ocean water transportation by acoustic?gravity waves. J. Geophys. Res. Oceans, 119, doi:10.1002/ 2014JC010234

  2. Ice erosion of a sea-floor knickpoint at the inner edge of the stamukhi zone, Beaufort Sea, Alaska

    USGS Publications Warehouse

    Barnes, P.W.; Asbury, J.L.; Rearic, D.M.; Ross, C.R.

    1987-01-01

    In 1981 and 1982, detailed bathymetric and side-scan sonar surveys were made of an area of the sea floor north of Prudhoe Bay, Alaska, to study the changing characteristics of the seabed at the inner boundary of the stamukhi zone, the coast-parallel zone of grounded ice ridges that occurs in water depths between 15 and 50 m in the arctic. The fathograms and sonographs resolved 10-cm features and electronic navigation gave relocations accurate to about 10 m. Year after year an ice boundary develops at the inner edge of the stamukhi zone where major shear and pressure deformation occur in about the same location. Associated with this ice boundary, the bathymetry shows a pronounced break in slope - the knickpoint - on the shelf profile at about 20 m depth. The 2-3 m-high knickpoint is cut in a consolidated gravelly mud of pre-Holocene age. A well-defined gravel and cobble shoal a few meters high usually occurs at the inshore edge of the knickpoint. The sonograph mosaic shows that seaward of the knickpoint, ice gouges saturate the sea floor and are well defined; inshore the gouges are fewer in number and are poorly defined on the records. Few gouges can be traced from the seaward side of the knickpoint across the shoals to the inshore side of the knickpoint. Studies of ice gouging rates in two seabed corridors that cross the stamukhi zone reveal the highest rates of gouging seaward of the knickpoint. We believe that the knickpoint results from ice erosion at the inner boundary of the stamukhi zone. Intensified currents associated with this boundary winnow away fine sediments. Ice bulldozing and currents shape the shoals, which perch atop the knickpoint. The knickpoint helps to limit ice forces on the seabed inshore of the stamukhi zone. ?? 1987.

  3. Atmospheric Profiles, Clouds and the Evolution of Sea Ice Cover in the Beaufort and Chukchi Seas: Atmospheric Observations and Modeling as Part of the Seasonal Ice Zone Reconnaissance Surveys

    DTIC Science & Technology

    2017-06-04

    Cover in the Beaufort and Chukchi Seas: Atmospheric Observations and Modeling as Part of the Seasonal Ice Zone Reconnaissance Surveys Axel...of the atmospheric component of the Seasonal Ice Zone Reconnaissance Survey project (SIZRS). Combined with oceanographic and sea ice components of...indicate cumulative probabilities. Vertical lines show median errors for forecast and climatology, respectively Figure 7 Correlation coefficient

  4. Thin Ice Area Extraction in the Seasonal Sea Ice Zones of the Northern Hemisphere Using Modis Data

    NASA Astrophysics Data System (ADS)

    Hayashi, K.; Naoki, K.; Cho, K.

    2018-04-01

    Sea ice has an important role of reflecting the solar radiation back into space. However, once the sea ice area melts, the area starts to absorb the solar radiation which accelerates the global warming. This means that the trend of global warming is likely to be enhanced in sea ice areas. In this study, the authors have developed a method to extract thin ice area using reflectance data of MODIS onboard Terra and Aqua satellites of NASA. The reflectance of thin sea ice in the visible region is rather low. Moreover, since the surface of thin sea ice is likely to be wet, the reflectance of thin sea ice in the near infrared region is much lower than that of visible region. Considering these characteristics, the authors have developed a method to extract thin sea ice areas by using the reflectance data of MODIS (NASA MYD09 product, 2017) derived from MODIS L1B. By using the scatter plots of the reflectance of Band 1 (620 nm-670 nm) and Band 2 (841 nm-876 nm)) of MODIS, equations for extracting thin ice area were derived. By using those equations, most of the thin ice areas which could be recognized from MODIS images were well extracted in the seasonal sea ice zones in the Northern Hemisphere, namely the Sea of Okhotsk, the Bering Sea and the Gulf of Saint Lawrence. For some limited areas, Landsat-8 OLI images were also used for validation.

  5. The winter pack-ice zone provides a sheltered but food-poor habitat for larval Antarctic krill.

    PubMed

    Meyer, Bettina; Freier, Ulrich; Grimm, Volker; Groeneveld, Jürgen; Hunt, Brian P V; Kerwath, Sven; King, Rob; Klaas, Christine; Pakhomov, Evgeny; Meiners, Klaus M; Melbourne-Thomas, Jessica; Murphy, Eugene J; Thorpe, Sally E; Stammerjohn, Sharon; Wolf-Gladrow, Dieter; Auerswald, Lutz; Götz, Albrecht; Halbach, Laura; Jarman, Simon; Kawaguchi, So; Krumpen, Thomas; Nehrke, Gernot; Ricker, Robert; Sumner, Michael; Teschke, Mathias; Trebilco, Rowan; Yilmaz, Noyan I

    2017-12-01

    A dominant Antarctic ecological paradigm suggests that winter sea ice is generally the main feeding ground for krill larvae. Observations from our winter cruise to the southwest Atlantic sector of the Southern Ocean contradict this view and present the first evidence that the pack-ice zone is a food-poor habitat for larval development. In contrast, the more open marginal ice zone provides a more favourable food environment for high larval krill growth rates. We found that complex under-ice habitats are, however, vital for larval krill when water column productivity is limited by light, by providing structures that offer protection from predators and to collect organic material released from the ice. The larvae feed on this sparse ice-associated food during the day. After sunset, they migrate into the water below the ice (upper 20 m) and drift away from the ice areas where they have previously fed. Model analyses indicate that this behaviour increases both food uptake in a patchy food environment and the likelihood of overwinter transport to areas where feeding conditions are more favourable in spring.

  6. 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.

  7. Atmospheric Profiles, Clouds, and the Evolution of Sea Ice Cover in the Beaufort and Chukchi Seas Atmospheric Observations and Modeling as Part of the Seasonal Ice Zone Reconnaissance Surveys

    DTIC Science & Technology

    2012-09-30

    Ice Cover in the Beaufort and Chukchi Seas Atmospheric Observations and Modeling as Part of the Seasonal Ice Zone Reconnaissance Surveys Axel...temperatures. These changes in turn will affect the evolution of the SIZ. An appropriate representation of this feedback loop in models is critical if we... modeling experiments as part of the atmospheric component of the Seasonal Ice Zone Reconnaissance Survey project (SIZRS). We will • Determine the role

  8. 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

  9. 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

  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. 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

  12. Mapping the grounding zone of Ross Ice Shelf using ICESat laser altimetry

    USGS Publications Warehouse

    Brunt, Kelly M.; Fricker, Helen A.; Padman, Laurie; Scambos, Ted A.; O'Neel, Shad

    2010-01-01

    We use laser altimetry from the Ice, Cloud, and land Elevation Satellite (ICESat) to map the grounding zone (GZ) of the Ross Ice Shelf, Antarctica, at 491 locations where ICESat tracks cross the grounding line (GL). Ice flexure in the GZ occurs as the ice shelf responds to short-term sea-level changes due primarily to tides. ICESat repeat-track analysis can be used to detect this region of flexure since each repeated pass is acquired at a different tidal phase; the technique provides estimates for both the landward limit of flexure and the point where the ice becomes hydrostatically balanced. We find that the ICESat-derived landward limits of tidal flexure are, in many places, offset by several km (and up to ∼60 km) from the GL mapped previously using other satellite methods. We discuss the reasons why different mapping methods lead to different GL estimates, including: instrument limitations; variability in the surface topographic structure of the GZ; and the presence of ice plains. We conclude that reliable and accurate mapping of the GL is most likely to be achieved when based on synthesis of several satellite datasets

  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. Some Results on Sea Ice Rheology for the Seasonal Ice Zone, Obtained from the Deformation Field of Sea Ice Drift Pattern

    NASA Astrophysics Data System (ADS)

    Toyota, T.; Kimura, N.

    2017-12-01

    Sea ice rheology which relates sea ice stress to the large-scale deformation of the ice cover has been a big issue to numerical sea ice modelling. At present the treatment of internal stress within sea ice area is based mostly on the rheology formulated by Hibler (1979), where the whole sea ice area behaves like an isotropic and plastic matter under the ordinary stress with the yield curve given by an ellipse with an aspect ratio (e) of 2, irrespective of sea ice area and horizontal resolution of the model. However, this formulation was initially developed to reproduce the seasonal variation of the perennial ice in the Arctic Ocean. As for its applicability to the seasonal ice zones (SIZ), where various types of sea ice are present, it still needs validation from observational data. In this study, the validity of this rheology was examined for the Sea of Okhotsk ice, typical of the SIZ, based on the AMSR-derived ice drift pattern in comparison with the result obtained for the Beaufort Sea. To examine the dependence on a horizontal scale, the coastal radar data operated near the Hokkaido coast, Japan, were also used. Ice drift pattern was obtained by a maximum cross-correlation method with grid spacings of 37.5 km from the 89 GHz brightness temperature of AMSR-E for the entire Sea of Okhotsk and the Beaufort Sea and 1.3 km from the coastal radar for the near-shore Sea of Okhotsk. The validity of this rheology was investigated from a standpoint of work rate done by deformation field, following the theory of Rothrock (1975). In analysis, the relative rates of convergence were compared between theory and observation to check the shape of yield curve, and the strain ellipse at each grid cell was estimated to see the horizontal variation of deformation field. The result shows that the ellipse of e=1.7-2.0 as the yield curve represents the observed relative conversion rates well for all the ice areas. Since this result corresponds with the yield criterion by Tresca and

  15. 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.

  16. 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.

  17. 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.

  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. 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

  20. 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.

  1. 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

  2. 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.

  3. 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.

  4. Fracture propagation and stability of ice shelves governed by ice shelf heterogeneity

    NASA Astrophysics Data System (ADS)

    Borstad, Chris; McGrath, Daniel; Pope, Allen

    2017-05-01

    Tabular iceberg calving and ice shelf retreat occurs after full-thickness fractures, known as rifts, propagate across an ice shelf. A quickly evolving rift signals a threat to the stability of Larsen C, the Antarctic Peninsula's largest ice shelf. Here we reveal the influence of ice shelf heterogeneity on the growth of this rift, with implications that challenge existing notions of ice shelf stability. Most of the rift extension has occurred in bursts after overcoming the resistance of suture zones that bind together neighboring glacier inflows. We model the stresses in the ice shelf to determine potential rift trajectories. Calving perturbations to ice flow will likely reach the grounding line. The stability of Larsen C may hinge on a single suture zone that stabilizes numerous upstream rifts. Elevated fracture toughness of suture zones may be the most important property that allows ice shelves to modulate Antarctica's contribution to sea level rise.

  5. 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

  6. 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

  7. Acoustic Gravity Waves Generated by an Oscillating Ice Sheet in Arctic Zone

    NASA Astrophysics Data System (ADS)

    Abdolali, A.; Kadri, U.; Kirby, J. T., Jr.

    2016-12-01

    ., 2015, Depth-integrated equation for hydro-acoustic waves with bottom damping, Journal of Fluid Mechanics, 766, R1 doi:10.1017/jfm.2015.37 Kadri, U., 2016, Generation of Hydroacoustic Waves by an Oscillating Ice Block in Arctic Zones, Advances in Acoustics and Vibration. 2016. doi:10.1155/2016/8076108

  8. 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.

  9. Understanding the Sea Ice Zone: Scientists and Communities Partnering to Archive, Analyze and Disseminate Local Ice Observations

    NASA Astrophysics Data System (ADS)

    Collins, J. A.; Oldenburg, J.; Liu, M.; Pulsifer, P. L.; Kaufman, M.; Eicken, H.; Parsons, M. A.

    2012-12-01

    Knowledge of sea ice is critical to the hunting, whaling, and cultural activities of many Indigenous communities in Northern and Western Alaska. Experienced hunters have monitored seasonal changes of the sea ice over many years, giving them a unique expertise in assessing the current state of the sea ice as well as any anomalies in seasonal sea ice conditions. The Seasonal Ice Zone Observing Network (SIZONet), in collaboration with the Exchange for Local Observations and Knowledge of the Arctic (ELOKA), has developed an online application for collecting, storing, and analyzing sea ice observations contributed by local experts from coastal Alaskan communities. Here we present the current iteration of the application, outline future plans and discuss how the development process and resulting system have improved our collective understanding of sea ice processes and changes. The SIZONet application design is based on the needs of the research scientists responsible for entering observation data into the database, the needs of local sea ice experts contributing their observations and knowledge, and the information needs of Alaska coastal communities. Entry forms provide a variety of input methods, including menus, check boxes, and free text input. Input options strive to balance flexibility in capturing concepts and details with the need for analytical consistency. Currently, research staff at the University of Alaska Fairbanks use the application to enter observations received via written or electronic communications from local sea ice experts. Observation data include current weather conditions, snow and ice quantity and quality, and wildlife sighted or taken. Future plans call for direct use of the SIZONet interface by local sea ice experts as well as students, both as contributors to the data collection and as users seeking meaning in the data. This functionality is currently available to a limited number of community members as we extend the application to support

  10. Atmospheric Profiles, Clouds, and the Evolution of Sea Ice Cover in the Beaufort and Chukchi Seas Atmospheric Observations and Modeling as Part of the Seasonal Ice Zone Reconnaissance Surveys

    DTIC Science & Technology

    2013-09-30

    Cover in the Beaufort and Chukchi Seas Atmospheric Observations and Modeling as Part of the Seasonal Ice Zone Reconnaissance Surveys Axel...how changes in sea ice and sea surface conditions in the SIZ affect changes in cloud properties and cover . • Determine the role additional atmospheric...REPORT TYPE 3. DATES COVERED 00-00-2013 to 00-00-2013 4. TITLE AND SUBTITLE Atmospheric Profiles, Clouds, and the Evolution of Sea Ice Cover in the

  11. Deterministic multi-zone ice accretion modeling

    NASA Technical Reports Server (NTRS)

    Yamaguchi, K.; Hansman, R. John, Jr.; Kazmierczak, Michael

    1991-01-01

    The focus here is on a deterministic model of the surface roughness transition behavior of glaze ice. The initial smooth/rough transition location, bead formation, and the propagation of the transition location are analyzed. Based on the hypothesis that the smooth/rough transition location coincides with the laminar/turbulent boundary layer transition location, a multizone model is implemented in the LEWICE code. In order to verify the effectiveness of the model, ice accretion predictions for simple cylinders calculated by the multizone LEWICE are compared to experimental ice shapes. The glaze ice shapes are found to be sensitive to the laminar surface roughness and bead thickness parameters controlling the transition location, while the ice shapes are found to be insensitive to the turbulent surface roughness.

  12. Gas exchange in the ice zone: the role of small waves and big animals

    NASA Astrophysics Data System (ADS)

    Loose, B.; Takahashi, A.; Bigdeli, A.

    2016-12-01

    The balance of air-sea gas exchange and net biological carbon fixation determine the transport and transformation of carbon dioxide and methane in the ocean. Air-sea gas exchange is mostly driven by upper ocean physics, but biology can also play a role. In the open ocean, gas exchange increases proportionate to the square of wind speed. When sea ice is present, this dependence breaks down in part because breaking waves and air bubble entrainment are damped out by interactions between sea ice and the wave field. At the same time, sea ice motions, formation, melt, and even sea ice-associated organisms can act to introduce turbulence and air bubbles into the upper ocean, thereby enhancing air-sea gas exchange. We take advantage of the knowledge advances of upper ocean physics including bubble dynamics to formulate a model for air-sea gas exchange in the sea ice zone. Here, we use the model to examine the role of small-scale waves and diving animals that trap air for insulation, including penguins, seals and polar bears. We compare these processes to existing parameterizations of wave and bubble dynamics in the open ocean, to observe how sea ice both mitigates and locally enhances air-sea gas transfer.

  13. 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

  14. Supraglacial Lakes in the Percolation Zone of the Western Greenland Ice Sheet: Formation and Development using Operation IceBridge Snow Radar and ATM (2009-2014)

    NASA Astrophysics Data System (ADS)

    Chen, C.; Howat, I. M.; de la Peña, S.

    2015-12-01

    Surface meltwater lakes on the Greenland Ice Sheet have appeared at higher elevations, extending well into the percolation zone, under recent warming, with the largest expansion occurring in the western Greenland Ice Sheet. The conditions that allow lakes to form atop firn are poorly constrained, but the formation of new lakes imply changes in the permeability of the firn at high elevations, promoting meltwater runoff. We explore the formation and evolution of new surface lakes in this region above 1500 meters, using a combination of satellite imagery and repeat Snow (2-6.5 GHz) radar echograms and LIDAR measurements from NASA's Operation IceBridge of 2009-2014. We identify conditions for surface lake formation at their farthest inland extent and suggest behaviors of persistence and lake drainage are due to differences in regional ice dynamics.

  15. Circulation and water properties in the landfast ice zone of the Alaskan Beaufort Sea

    NASA Astrophysics Data System (ADS)

    Weingartner, Thomas J.; Danielson, Seth L.; Potter, Rachel A.; Trefry, John H.; Mahoney, Andy; Savoie, Mark; Irvine, Cayman; Sousa, Leandra

    2017-09-01

    Moorings, hydrography, satellite-tracked drifters, and high-frequency radar data describe the annual cycle in circulation and water properties in the landfast ice zone (LIZ) of the Alaskan Beaufort Sea. Three seasons, whose duration and characteristics are controlled by landfast ice formation and ablation, define the LIZ: ;winter;, ;break-up;, and ;open-water;. Winter begins in October with ice formation and ends in June when rivers commence discharging. Winter LIZ ice velocities are zero, under-ice currents are weak ( 5 cm s-1), and poorly correlated with winds and local sea level. The along-shore momentum balance is between along-shore pressure gradients and bottom and ice-ocean friction. Currents at the landfast ice-edge are swift ( 35 cm s-1), wind-driven, with large horizontal shears, and potentially unstable. Weak cross-shore velocities ( 1 cm s-1) imply limited exchanges between the LIZ and the outer shelf in winter. The month-long break-up season (June) begins with the spring freshet and concludes when landfast ice detaches from the bottom. Cross-shore currents increase, and the LIZ hosts shallow ( 2 m), strongly-stratified, buoyant and sediment-laden, under-ice river plumes that overlie a sharp, 1 m thick, pycnocline across which salinity increases by 30. The plume salt balance is between entrainment and cross-shore advection. Break-up is followed by the 3-month long open-water season when currents are swift (≥20 cm s-1) and predominantly wind-driven. Winter water properties are initialized by fall advection and evolve slowly due to salt rejection from ice. Fall waters and ice within the LIZ derive from local rivers, the Mackenzie and/or Chukchi shelves, and the Arctic basin.

  16. Shallow methylmercury production in the marginal sea ice zone of the central Arctic Ocean

    PubMed Central

    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

    2015-01-01

    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 marginal sea ice 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 ice, extension of the seasonal sea ice zone, intensified surface ocean stratification and shifts in plankton ecodynamics, will likely lead to higher marine MeHg production. PMID:25993348

  17. Shallow methylmercury production in the marginal sea ice zone of the central Arctic Ocean.

    PubMed

    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

    2015-05-20

    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 marginal sea ice 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 ice, extension of the seasonal sea ice zone, intensified surface ocean stratification and shifts in plankton ecodynamics, will likely lead to higher marine MeHg production.

  18. The Ice Cap Zone: A Unique Habitable Zone for Ocean Worlds

    NASA Astrophysics Data System (ADS)

    Ramirez, Ramses M.; Levi, Amit

    2018-03-01

    Traditional definitions of the habitable zone assume that habitable planets contain a carbonate-silicate cycle that regulates CO2 between the atmosphere, surface, and the interior. Such theories have been used to cast doubt on the habitability of ocean worlds. However, Levi et al (2017) have recently proposed a mechanism by which CO2 is mobilized between the atmosphere and the interior of an ocean world. At high enough CO2 pressures, sea ice can become enriched in CO2 clathrates and sink after a threshold density is achieved. The presence of subpolar sea ice is of great importance for habitability in ocean worlds. It may moderate the climate and is fundamental in current theories of life formation in diluted environments. Here, we model the Levi et al. mechanism and use latitudinally-dependent non-grey energy balance and single-column radiative-convective models and find that this mechanism may be sustained on ocean worlds that rotate at least 3 times faster than the Earth. We calculate the circumstellar region in which this cycle may operate for G-M-stars (Teff = 2,600-5,800 K), extending from ˜1.23 - 1.65, 0.69 - 0.873, 0.38-0.528 AU, 0.219-0.308 AU, 0.146-0.206 AU, and 0.0428-0.0617 AU for G2, K3, M0, M3, M5, and M8 stars, respectively. However, unless planets are very young and not tidally-locked, our mechanism would be unlikely to apply to stars cooler than a ˜M3. We predict C/O ratios for our atmospheres (˜0.5) that can be verified by the JWST mission.

  19. The ice cap zone: a unique habitable zone for ocean worlds

    NASA Astrophysics Data System (ADS)

    Ramirez, Ramses M.; Levi, Amit

    2018-07-01

    Traditional definitions of the habitable zone assume that habitable planets contain a carbonate-silicate cycle that regulates CO2 between the atmosphere, surface, and the interior. Such theories have been used to cast doubt on the habitability of ocean worlds. However, Levi et al. have recently proposed a mechanism by which CO2 is mobilized between the atmosphere and the interior of an ocean world. At high enough CO2 pressures, sea ice can become enriched in CO2 clathrates and sink after a threshold density is achieved. The presence of subpolar sea ice is of great importance for habitability in ocean worlds. It may moderate the climate and is fundamental in current theories of life formation in diluted environments. Here, we model the Levi et al. mechanism and use latitudinally dependent non-grey energy balance and single-column radiative-convective climate models and find that this mechanism may be sustained on ocean worlds that rotate at least 3 times faster than the Earth. We calculate the circumstellar region in which this cycle may operate for G-M stars (Teff = 2600-5800 K), extending from ˜1.23-1.65, 0.69-0.954, 0.38-0.528, 0.219-0.308 , 0.146-0.206, and 0.0428-0.0617 au for G2, K2, M0, M3, M5, and M8 stars, respectively. However, unless planets are very young and not tidally locked, our mechanism would be unlikely to apply to stars cooler than a ˜M3. We predict C/O ratios for our atmospheres (˜0.5) that can be verified by the James Webb Space Telescope mission.

  20. Abundant Methanol Ice toward a Massive Young Stellar Object in the Central Molecular Zone

    NASA Astrophysics Data System (ADS)

    An, Deokkeun; Sellgren, Kris; Boogert, A. C. Adwin; Ramírez, Solange V.; Pyo, Tae-Soo

    2017-07-01

    Previous radio observations revealed widespread gas-phase methanol (CH3OH) in the Central Molecular Zone (CMZ) at the Galactic center (GC), but its origin remains unclear. Here, we report the discovery of CH3OH ice toward a star in the CMZ, based on a Subaru 3.4-4.0 μm spectrum, aided by NASA/IRTF L\\prime imaging and 2-4 μm spectra. The star lies ˜8000 au away in projection from a massive young stellar object (MYSO). Its observed high CH3OH ice abundance (17 % +/- 3 % relative to H2O ice) suggests that the 3.535 μm CH3OH ice absorption likely arises in the MYSO’s extended envelope. However, it is also possible that CH3OH ice forms with a higher abundance in dense clouds within the CMZ, compared to within the disk. Either way, our result implies that gas-phase CH3OH in the CMZ can be largely produced by desorption from icy grains. The high solid CH3OH abundance confirms the prominent 15.4 μm shoulder absorption observed toward GC MYSOs arises from CO2 ice mixed with CH3OH. Based in part on data collected at Subaru Telescope, which is operated by the National Astronomical Observatory of Japan.

  1. 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.

  2. Modeling ocean wave propagation under sea ice covers

    NASA Astrophysics Data System (ADS)

    Zhao, Xin; Shen, Hayley H.; Cheng, Sukun

    2015-02-01

    Operational ocean wave models need to work globally, yet current ocean wave models can only treat ice-covered regions crudely. The purpose of this paper is to provide a brief overview of ice effects on wave propagation and different research methodology used in studying these effects. Based on its proximity to land or sea, sea ice can be classified as: landfast ice zone, shear zone, and the marginal ice zone. All ice covers attenuate wave energy. Only long swells can penetrate deep into an ice cover. Being closest to open water, wave propagation in the marginal ice zone is the most complex to model. The physical appearance of sea ice in the marginal ice zone varies. Grease ice, pancake ice, brash ice, floe aggregates, and continuous ice sheet may be found in this zone at different times and locations. These types of ice are formed under different thermal-mechanical forcing. There are three classic models that describe wave propagation through an idealized ice 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 ice floes much smaller than the wavelength, thin elastic plate model is suitable for a continuous ice sheet, and the viscous layer model is suitable for grease ice. For different sea ice types we may need different wave ice 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 ice covers need to be implemented in the operational ocean wave models. In this review, we introduce the sea ice types, previous wave ice interaction models, wave attenuation mechanisms, the methods to calculate wave reflection and transmission between different ice covers, and the effect of ice floe breaking on shaping the sea ice morphology

  3. Modeling of surface roughness effects on glaze ice accretion

    NASA Technical Reports Server (NTRS)

    Hansman, R. John, Jr.; Yamaguchi, Keiko; Berkowitz, Brian M.; Potapczuk, Mark

    1990-01-01

    A series of experimental investigations focused on studying the cause and effect of roughness on accreting glaze ice surfaces were conducted. Detailed microvideo observations were made of glaze ice accretions on 1 to 4 inch diameter cylinders in three icing wind tunnels (the Data Products of New England six inch test facility, the NASA Lewis Icing Research Tunnel, and the B. F. Goodrich Ice Protection Research Facility). Infrared thermal video recordings were made of accreting ice surfaces in the Goodrich facility. Distinct zones of surface water behavior were observed; a smooth wet zone in the stagnation region with a uniform water film; a rough zone where surface tension effects caused coalescence of surface water into stationary beads; a horn zone where roughness elements grow into horn shapes; a runback zone where surface water ran back as rivulets; and a dry zone where rime feathers formed. The location of the transition from the smooth to the rough zone was found to migrate with time towards the stagnation point. The behavior of the transition appeared to be controlled by boundary layer transition and bead formation mechanisms at the interface between the smooth and rough zones. Regions of wet ice growth and enhanced heat transfer were clearly visible in the infrared video recordings of glaze ice surfaces. A simple multi-zone modification to the current glaze ice accretion model was proposed to include spatial variability in surface roughness.

  4. Unusual radar echoes from the Greenland ice sheet

    NASA Technical Reports Server (NTRS)

    Rignot, E. J.; Vanzyl, J. J.; Ostro, S. J.; Jezek, K. C.

    1993-01-01

    In June 1991, the NASA/Jet Propulsion Laboratory airborne synthetic-aperture radar (AIRSAR) instrument collected the first calibrated data set of multifrequency, polarimetric, radar observations of the Greenland ice sheet. At the time of the AIRSAR overflight, ground teams recorded the snow and firn (old snow) stratigraphy, grain size, density, and temperature at ice camps in three of the four snow zones identified by glaciologists to characterize four different degrees of summer melting of the Greenland ice sheet. The four snow zones are: (1) the dry-snow zone, at high elevation, where melting rarely occurs; (2) the percolation zone, where summer melting generates water that percolates down through the cold, porous, dry snow and then refreezes in place to form massive layers and pipes of solid ice; (3) the soaked-snow zone where melting saturates the snow with liquid water and forms standing lakes; and (4) the ablation zone, at the lowest elevations, where melting is vigorous enough to remove the seasonal snow cover and ablate the glacier ice. There is interest in mapping the spatial extent and temporal variability of these different snow zones repeatedly by using remote sensing techniques. The objectives of the 1991 experiment were to study changes in radar scattering properties across the different melting zones of the Greenland ice sheet, and relate the radar properties of the ice sheet to the snow and firn physical properties via relevant scattering mechanisms. Here, we present an analysis of the unusual radar echoes measured from the percolation zone.

  5. Physical and biological oceanographic interaction in the spring bloom at the Bering Sea marginal ice edge zone

    NASA Astrophysics Data System (ADS)

    Niebauer, H. J.; Alexander, Vera; Henrichs, Susan

    1990-12-01

    At the edge of the melting sea ice 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 ice 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 ice edge blooms from open water blooms where temperature gradients generate the stratification. Five cross-ice 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 ice edge zone are presented. In addition, meteorological and oceanographic conditions were observed that should have been conducive to ice edge up welling. While significant ice and water movement occurred, upwelling was not observed. Finally, the Bering Sea ice edge spring bloom is compared with other ice 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.

  6. Marine Ice Crevassing Imaged with Side-looking GPR: Implications for Stability within the McMurdo Shear Zone

    NASA Astrophysics Data System (ADS)

    Arcone, S. A.; Ray, L.; Lever, J.; Koons, P. O.; Kaluzienski, L. M.

    2017-12-01

    Shearing along ice shelf margins threatens shelf stability if crevassing results throughout the ice. We are investigating a 28 km2 section of the McMurdo Shear Zone (MSZ), which lies between the Ross Ice Shelf (RIS) and the McMurdo Ice Shelf (MIS). Our gridded transects are east-west, ice flow is nearly due north and the RIS compresses against the MIS from east to west. We find nearly synchronized firn and marine ice crevassing; the marine ice is stratified. However, the lack of any radar evidence for crevassing or fracture within the intermediate 120 m of meteoric ice is so far, enigmatic. The marine ice crevassing is interpreted from ground-penetrating radar (GPR) trace signatures within 100 m swaths of the interface between the meteoric and marine ice; thus the GPR performs like side-looking radar. Symmetric and deformed diffraction hyperbolas indicate crevasses oriented at 43-76 degrees relative to ice flow, as seen in the firn. Those near 45 degrees are interpreted as recently formed while those at greater angles are likely older and rotated. Many traces indicate crevasse warping, lateral faulting, and down-faulting. Traces nearly perpendicular to flow indicate possible wing cracks that grew from the tips of crevasses into the direction of compression from the RIS. We interpret the marine crevasses to have originated at the meteoric-marine interface, and to have extended to the shelf bottom because they appear filled with unstratified frozen seawater. In view of these observations, and that the intermediate meteoric ice must be under similar although not exactly the same stresses, the lack of fracturing within the meteoric ice may imply that suturing following brittle and ductile shear deformation provides stability for the MSZ and may result from this east-west compression of the RIS against the MIS.

  7. Modeling Primary Productivity in the Margin Ice Zone from Glider-Based Measurements of Chlorophyll and Light during the 2014 Miz Program

    NASA Astrophysics Data System (ADS)

    Perry, M. J.; Lee, C.; Rainville, L.; Cetinic, I.; Yang, E. J.; Kang, S. H.

    2016-02-01

    In late summer 2014 during the Marginal Ice Zone (MIZ) Experiment, an international project sponsored by ONR, four Seagliders transited open water, through the marginal ice zone, and under ice-covered regions in the Beaufort Sea, penetrating as far as 100 km into the ice pack. The gliders navigated either by GPS in open water or, when under the ice, 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 ice 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 ice, despite shorter days and reduce irradiation.

  8. Sea ice melting in the marginal ice zone.

    USGS Publications Warehouse

    Josberger, E.G.

    1983-01-01

    The heat and salt flux boundary conditions together with the freezing curve relationship are a necessary component of any ice- 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

  9. Air-Sea Interactions in the Marginal Ice Zone

    DTIC Science & Technology

    2016-03-31

    Arctic Ocean has increased with the significant retreat of the seasonal sea-ice extent. Here, we use wind, wave, turbulence, and ice measurements to...which has experienced a significant retreat of the seasonal ice extent (Comiso and Nishio, 2008; Comiso et al., 2008). Thomson and Rogers (2014) showed

  10. Investigation of surface water behavior during glaze ice accretion

    NASA Technical Reports Server (NTRS)

    Hansman, R. John, Jr.; Turnock, Stephen R.

    1990-01-01

    A series of experimental investigations that focused on isolating the primary factors that control the behavior of unfrozen surface water during glaze ice accretion were conducted. Detailed microvideo observations were made of glaze ice accretions on 2.54 cm diam cylinders in a closed-loop refrigerated wind tunnel. Distinct zones of surface water behavior were observed; a smooth wet zone in the stagnation region with a uniform water film, a rough zone where surface tension effects caused coalescence of surface water into stationary beads, and a zone where surface water ran back as rivulets. The location of the transition from the smooth to the rough zone was found to migrate towards the stagnation point with time. Comparative tests were conducted to study the effect of the substrate thermal and roughness properties on ice accretion. The importance of surface water behavior was evaluated by the addition of a surface tension reducing agent to the icing tunnel water supply, which significantly altered the accreted glaze ice shape. Measurements were made to determine the contact angle behavior of water droplets on ice. A simple multizone modification to current glaze ice accretion models was proposed to include the observed surface roughness behavior.

  11. Evolution of a Directional Wave Spectrum in a 3D Marginal Ice Zone with Random Floe Size Distribution

    NASA Astrophysics Data System (ADS)

    Montiel, F.; Squire, V. A.

    2013-12-01

    A new ocean wave/sea-ice interaction model is proposed that simulates how a directional wave spectrum evolves as it travels through a realistic marginal ice zone (MIZ), where wave/ice 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 ice edge. The data suggest that angular isotropy, arising from multiple scattering by ice 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 ice cover into adjacent infinite slabs of finite width parallel to the ice edge. Each slab contains an arbitrary (but finite) number of circular ice floes with randomly distributed properties. Ice 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

  12. Glacially-megalineated limestone terrain of Anticosti Island, Gulf of St. Lawrence, Canada; onset zone of the Laurentian Channel Ice Stream

    NASA Astrophysics Data System (ADS)

    Eyles, Nick; Putkinen, Niko

    2014-03-01

    Anticosti is a large elongate island (240 km long, 60 km wide) in eastern Canada within the northern part of a deep water trough (Gulf of St. Lawrence) that terminates at the Atlantic continental shelf edge. The island's Pleistocene glaciological significance is that its long axis lay transverse to ice from the Quebec and Labrador sectors of the Laurentide Ice Sheet moving south from the relatively high-standing Canadian Shield. Recent glaciological reconstructions place a fast-flowing ice stream along the axis of the Gulf of St. Lawrence but supporting geologic evidence in terms of recognizing its hard-bedded onset zone and downstream streamlined soft bed is limited. Anticosti Island consists of gently southward-dipping limestone plains composed of Ordovician and Silurian limestones (Vaureal, Becscie and Jupiter formations) with north-facing escarpments transverse to regional ice flow. Glacial deposits are largely absent and limestone plains in the higher central plateau of the island retain a relict apparently ‘preglacial’ drainage system consisting of deeply-incised dendritic bedrock valleys. In contrast, the bedrock geomorphology of the lower lying western and eastern limestone plains of the island is strikingly different having been extensively modified by glacial erosion. Escarpments are glacially megalineated with a distinct ‘zig-zag’ planform reflecting northward-projecting bullet-shaped ‘noses’ (identified as rock drumlins) up to 2 km wide at their base and 4 km in length with rare megagrooved upper surfaces. Drumlins are separated by southward-closing, funnel-shaped ‘through valleys’ where former dendritic valleys have been extensively altered by the streaming of basal ice through gaps in the escarpments. Glacially-megalineated bedrock terrain such as on the western and eastern flanks of Anticosti Island is elsewhere associated with the hard-bedded onset zones of fast flowing ice streams and provides important ground truth for the

  13. Evidence for ice-ocean albedo feedback in the Arctic Ocean shifting to a seasonal ice zone.

    PubMed

    Kashiwase, Haruhiko; Ohshima, Kay I; Nihashi, Sohey; Eicken, Hajo

    2017-08-15

    Ice-albedo feedback due to the albedo contrast between water and ice is a major factor in seasonal sea ice retreat, and has received increasing attention with the Arctic Ocean shifting to a seasonal ice cover. However, quantitative evaluation of such feedbacks is still insufficient. Here we provide quantitative evidence that heat input through the open water fraction is the primary driver of seasonal and interannual variations in Arctic sea ice retreat. Analyses of satellite data (1979-2014) and a simplified ice-upper ocean coupled model reveal that divergent ice motion in the early melt season triggers large-scale feedback which subsequently amplifies summer sea ice anomalies. The magnitude of divergence controlling the feedback has doubled since 2000 due to a more mobile ice cover, which can partly explain the recent drastic ice reduction in the Arctic Ocean.

  14. Arctic multiyear ice classification and summer ice cover using passive microwave satellite data

    NASA Astrophysics Data System (ADS)

    Comiso, J. C.

    1990-08-01

    The ability to classify and monitor Arctic multiyear sea ice cover using multispectral passive microwave data is studied. Sea ice concentration maps during several summer minima have been analyzed to obtain estimates of ice surviving the summer. The results are compared with multiyear ice concentrations derived from data the following winter, using an algorithm that assumes a certain emissivity for multiyear ice. The multiyear ice cover inferred from the winter data is approximately 25 to 40% less than the summer ice cover minimum, suggesting that even during winter when the emissivity of sea ice is most stable, passive microwave data may account for only a fraction of the total multiyear ice 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 ice floes in the Arctic, especially those near the summer marginal ice zone, have first-year ice or intermediate signatures in the subsequent winter. A likely mechanism for this is the intrusion of seawater into the snow-ice interface, which often occurs near the marginal ice 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 ice. Hence the multiyear ice data should be studied in conjunction with the previous summer ice data to obtain a more complete characterization of the state of the Arctic ice cover. The total extent and actual areas of the summertime Arctic pack ice 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 ice cover.

  15. MIZEX. A Program for Mesoscale Air-Ice-Ocean Interaction Experiments in Arctic Marginal Ice Zones. III. Modeling the Marginal Ice Zone,

    DTIC Science & Technology

    1984-04-01

    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 Ice OnlY Mod" D"’, 55*w F~tth Yea’ Ice 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

  16. ICESat: Ice, Cloud and Land Elevation Satellite

    NASA Technical Reports Server (NTRS)

    Zwally, Jay; Shuman, Christopher

    2002-01-01

    Ice exists in the natural environment in many forms. The Earth dynamic ice features shows that at high elevations and/or high latitudes,snow that falls to the ground can gradually build up tu form thick consolidated ice masses called glaciers. Glaciers flow downhill under the force of gravity and can extend into areas that are too warm to support year-round snow cover. The snow line, called the equilibrium line on a glacier or ice sheet, separates the ice areas that melt on the surface and become show free in summer (net ablation zone) from the ice area that remain snow covered during the entire year (net accumulation zone). Snow near the surface of a glacier that is gradually being compressed into solid ice is called firm.

  17. Marginal Ice Zone: Biogeochemical Sampling with Gliders

    DTIC Science & Technology

    2015-09-30

    chlorophyll primary productivity model to estimate and compare phytoplankton productivity under full ice cover, in the MIZ, and in open ice-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

  18. The seasonal sea-ice zone in the glacial Southern Ocean as a carbon sink.

    PubMed

    Abelmann, Andrea; Gersonde, Rainer; Knorr, Gregor; Zhang, Xu; Chapligin, Bernhard; Maier, Edith; Esper, Oliver; Friedrichsen, Hans; Lohmann, Gerrit; Meyer, Hanno; Tiedemann, Ralf

    2015-09-18

    Reduced surface-deep ocean exchange and enhanced nutrient consumption by phytoplankton in the Southern Ocean have been linked to lower glacial atmospheric CO2. However, identification of the biological and physical conditions involved and the related processes remains incomplete. Here we specify Southern Ocean surface-subsurface contrasts using a new tool, the combined oxygen and silicon isotope measurement of diatom and radiolarian opal, in combination with numerical simulations. Our data do not indicate a permanent glacial halocline related to melt water from icebergs. Corroborated by numerical simulations, we find that glacial surface stratification was variable and linked to seasonal sea-ice changes. During glacial spring-summer, the mixed layer was relatively shallow, while deeper mixing occurred during fall-winter, allowing for surface-ocean refueling with nutrients from the deep reservoir, which was potentially richer in nutrients than today. This generated specific carbon and opal export regimes turning the glacial seasonal sea-ice zone into a carbon sink.

  19. The seasonal sea-ice zone in the glacial Southern Ocean as a carbon sink

    PubMed Central

    Abelmann, Andrea; Gersonde, Rainer; Knorr, Gregor; Zhang, Xu; Chapligin, Bernhard; Maier, Edith; Esper, Oliver; Friedrichsen, Hans; Lohmann, Gerrit; Meyer, Hanno; Tiedemann, Ralf

    2015-01-01

    Reduced surface–deep ocean exchange and enhanced nutrient consumption by phytoplankton in the Southern Ocean have been linked to lower glacial atmospheric CO2. However, identification of the biological and physical conditions involved and the related processes remains incomplete. Here we specify Southern Ocean surface–subsurface contrasts using a new tool, the combined oxygen and silicon isotope measurement of diatom and radiolarian opal, in combination with numerical simulations. Our data do not indicate a permanent glacial halocline related to melt water from icebergs. Corroborated by numerical simulations, we find that glacial surface stratification was variable and linked to seasonal sea-ice changes. During glacial spring–summer, the mixed layer was relatively shallow, while deeper mixing occurred during fall–winter, allowing for surface-ocean refueling with nutrients from the deep reservoir, which was potentially richer in nutrients than today. This generated specific carbon and opal export regimes turning the glacial seasonal sea-ice zone into a carbon sink. PMID:26382319

  20. 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.

  1. Sudden disintegration of ice in the glacial-proglacial transition zone of the largest glacier in Austria

    NASA Astrophysics Data System (ADS)

    Kellerer-Pirklbauer, Andreas; Avian, Michael; Hirschmann, Simon; Lieb, Gerhard Karl; Seier, Gernot; Sulzer, Wolfgang; Wakonigg, Herwig

    2017-04-01

    Rapid deglaciation does not only reveal a landscape which is prone to rapid geomorphic changes and sediment reworking but also the glacier ice itself might be in a state of disintegration by ice melting, pressure relief, crevasse formation, ice collapse or changes in the glacier's hydrology. In this study we considered the sudden disintegration of glacier ice in the glacial-proglacial transition zone of Pasterze Glacier. Pasterze Glacier is a typical alpine valley glacier and covers currently some 16.5 km2 making it to the largest glacier in Austria. This glacier is an important site for alpine mass tourism in Austria related to a public high alpine road and a cable car which enable access to the glacier rather easily also for unexperienced mountaineers. Spatial focus in our research is given on two particular study areas where several ice-mass movement events occurred during the 2015- and 2016-melting seasons. The first study area is a crevasse field at the lower third of the glacier tongue. This lateral crevasse field has been substantially modified during the last two melting seasons particularly because of thermo-erosional effects of a glacial stream which changed at this site from subglacial (until 2015) to glacier-lateral revealing a several tens of meters high unstable ice cliff prone to ice falls of different magnitudes. The second study area is located at the proglacial area. At Pasterze Glacier the proglacial area is widely influenced by dead-ice bodies of various dimensions making this area prone to slow to sudden geomorphic changes caused by ice mass changes. A particular ice-mass movement event took place on 20.09.2016. Within less than one hour the surface of the proglacial area changed substantially by tilting, lateral shifting, and subsidence of the ground accompanied by complete ice disintegration of once-debris covered ice. To understand acting processes at both areas of interest and to quantify mass changes we used field observations, terrain

  2. 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/2017AGUFM.C51A0954S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C51A0954S"><span>Surface melt effects on Cryosat-2 elevation retrievals in the ablation <span class="hlt">zone</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>Slater, T.; McMillan, M.; Shepherd, A.; Leeson, A.; Cornford, S. L.; Hogg, A.; Gilbert, L.; Muir, A. S.; Briggs, K.</p> <p>2017-12-01</p> <p>Over the past two decades, there has been an acceleration in the rate of mass losses from the Greenland <span class="hlt">ice</span> sheet. This acceleration is, in part, attributed to an increasingly negative surface mass balance (SMB), linked to increasing melt water runoff rates due to enhanced surface melting. Understanding the past, present and future evolution in surface melting is central to ongoing monitoring of <span class="hlt">ice</span> sheet mass balance and, in turn, to building realistic future projections. Currently, regional climate models are commonly used for this purpose, because direct in-situ observations are spatially and temporally sparse due to the logistics and resources required to collect such data. In particular, modelled SMB is used to estimate the extent and magnitude of surface melting, which influences (1) many geodetic mass balance estimates, and (2) snowpack microwave scattering properties. The latter is poorly understood and introduces uncertainty into radar altimeter estimates of <span class="hlt">ice</span> sheet evolution. Here, we investigate the changes in CryoSat-2 waveforms and elevation measurements caused by the onset of surface melt in the summer months over the ablation <span class="hlt">zone</span> of the Greenland <span class="hlt">ice</span> sheet. Specifically, we use CryoSat-2 SARIn mode data acquired between 2011 and 2016, to characterise the effect of high variability in surface melt during this period, and to assess the associated impact on estimates of <span class="hlt">ice</span> mass balance.</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>Marginal <span class="hlt">Ice</span> <span class="hlt">Zone</span>: 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('https://pubs.er.usgs.gov/publication/70012473','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70012473"><span>Arctic continental shelf morphology related to sea-<span class="hlt">ice</span> zonation, Beaufort Sea, 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>Reimnitz, E.; Toimil, L.; Barnes, P.</p> <p>1978-01-01</p> <p>Landsat-1 and NOAA satellite imagery for the winter 1972-1973, and a variety of <span class="hlt">ice</span> and sea-floor data were used to study sea-<span class="hlt">ice</span> zonation and dynamics and their relation to bottom morphology and geology on the Beaufort Sea continental shelf of arctic Alaska. In early winter the location of the boundary between undeformed fast <span class="hlt">ice</span> and westward-drifting pack <span class="hlt">ice</span> of the Pacific Gyre is controlled by major coastal promontories. Pronounced linear pressure- and shear-ridges, as well as hummock fields, form along this boundary and are stabilized by grounding, generally between the 10- and 20-m isobaths. Slippage along this boundary occurs intermittently at or seaward of the grounded ridges, forming new grounded ridges in a widening <span class="hlt">zone</span>, the stamukhi <span class="hlt">zone</span>, which by late winter extends out to the 40-m isobath. Between intermittent events along the stamukhi <span class="hlt">zone</span>, pack-<span class="hlt">ice</span> drift and slippage is continuous along the shelf edge, at average rates of 3-10 km/day. Whether slippage occurs along the stamukhi <span class="hlt">zone</span> or along the shelf edge, it is restricted to a <span class="hlt">zone</span> several hundred meters wide, and <span class="hlt">ice</span> seaward of the slip face moves at uniform rates without discernible drag effects. A causal relationship is seen between the spatial distribution of major <span class="hlt">ice</span>-ridge systems and offshore shoals downdrift of major coastal promontories. The shoals appear to have migrated shoreward under the influence of <span class="hlt">ice</span> up to 400 m in the last 25 years. The sea floor seaward of these shoals within the stamukhi <span class="hlt">zone</span> shows high <span class="hlt">ice</span>-gouge density, large incision depths, and a high degree of disruption of internal sedimentary structures. The concentration of large <span class="hlt">ice</span> ridges and our sea floor data in the stamukhi <span class="hlt">zone</span> indicate that much of the available marine energy is expended here, while the inner shelf and coast, where the relatively undeformed fast <span class="hlt">ice</span> grows, are sheltered. There is evidence that anomalies in the overall arctic shelf profile are related to sea-<span class="hlt">ice</span> zonation, <span class="hlt">ice</span> dynamics, and bottom</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 Marginal <span class="hlt">Ice</span> <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2013-09-30</p> <p><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://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 marginal <span class="hlt">ice</span> <span class="hlt">zone</span></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 <span class="hlt">zone</span> was derived from pelagic primary production, but at 3 of 11 stations within the marginal <span class="hlt">ice</span> <span class="hlt">zone</span> (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('http://hdl.handle.net/2060/20140010302','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140010302"><span><span class="hlt">Ice</span>-Shelf Flexure and Tidal Forcing of Bindschadler <span class="hlt">Ice</span> Stream, West Antarctica</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Walker, Ryan T.; Parizek, Bryron R.; Alley, Richard B.; Brunt, Kelly M.; Anandakrishnan, Sridhar</p> <p>2014-01-01</p> <p>Viscoelastic models of <span class="hlt">ice</span>-shelf flexure and <span class="hlt">ice</span>-stream velocity perturbations are combined into a single efficient flowline model to study tidal forcing of grounded <span class="hlt">ice</span>. The magnitude and timing of icestream response to tidally driven changes in hydrostatic pressure and/or basal drag are found to depend significantly on bed rheology, with only a perfectly plastic bed allowing instantaneous velocity response at the grounding line. The model can reasonably reproduce GPS observations near the grounding <span class="hlt">zone</span> of Bindschadler <span class="hlt">Ice</span> Stream (formerly <span class="hlt">Ice</span> Stream D) on semidiurnal time scales; however, other forcings such as tidally driven <span class="hlt">ice</span>-shelf slope transverse to the flowline and flexurally driven till deformation must also be considered if diurnal motion is to be matched</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..44.6218R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..44.6218R"><span>How robust are in situ observations for validating satellite-derived albedo over the dark <span class="hlt">zone</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>Ryan, J. C.; Hubbard, A.; Irvine-Fynn, T. D.; Doyle, S. H.; Cook, J. M.; Stibal, M.; Box, J. E.</p> <p>2017-06-01</p> <p>Calibration and validation of satellite-derived <span class="hlt">ice</span> sheet albedo data require high-quality, in situ measurements commonly acquired by up and down facing pyranometers mounted on automated weather stations (AWS). However, direct comparison between ground and satellite-derived albedo can only be justified when the measured surface is homogeneous at the length-scale of both satellite pixel and in situ footprint. Here we use digital imagery acquired by an unmanned aerial vehicle to evaluate point-to-pixel albedo comparisons across the western, ablating margin of the Greenland <span class="hlt">Ice</span> Sheet. Our results reveal that in situ measurements overestimate albedo by up to 0.10 at the end of the melt season because the ground footprints of AWS-mounted pyranometers are insufficient to capture the spatial heterogeneity of the <span class="hlt">ice</span> surface as it progressively ablates and darkens. Statistical analysis of 21 AWS across the entire Greenland <span class="hlt">Ice</span> Sheet reveals that almost half suffer from this bias, including some AWS located within the wet snow <span class="hlt">zone</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C13F1015R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C13F1015R"><span>How robust are in situ observations for validating satellite-derived albedo over the dark <span class="hlt">zone</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>Ryan, J.; Hubbard, A., II; Irvine-Fynn, T. D.; Doyle, S. H.; Cook, J.; Stibal, M.; Smith, L. C.; Box, J. E.</p> <p>2017-12-01</p> <p>Calibration and validation of satellite-derived <span class="hlt">ice</span> sheet albedo data require high-quality, in situ measurements commonly acquired by up and down facing pyranometers mounted on automated weather stations (AWS). However, direct comparison between ground and satellite-derived albedo can only be justified when the measured surface is homogeneous at the length-scale of both satellite pixel and in situ footprint. We used digital imagery acquired by an unmanned aerial vehicle to evaluate point-to-pixel albedo comparisons across the western, ablating margin of the Greenland <span class="hlt">Ice</span> Sheet. Our results reveal that in situ measurements overestimate albedo by up to 0.10 at the end of the melt season because the ground footprints of AWS-mounted pyranometers are insufficient to capture the spatial heterogeneity of the <span class="hlt">ice</span> surface as it progressively ablates and darkens. Statistical analysis of 21 AWS across the entire Greenland <span class="hlt">Ice</span> Sheet reveals that almost half suffer from this bias, including some AWS located within the wet snow <span class="hlt">zone</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008E%26PSL.265..246N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008E%26PSL.265..246N"><span>Conditions for a steady <span class="hlt">ice</span> sheet <span class="hlt">ice</span> shelf junction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nowicki, S. M. J.; Wingham, D. J.</p> <p>2008-01-01</p> <p>This paper investigates the conditions under which a marine <span class="hlt">ice</span> sheet may adopt a steady profile. The <span class="hlt">ice</span> is treated as a linear viscous fluid caused to flow from a rigid base to and over water, treated as a denser but inviscid fluid. The solutions in the region around the point of flotation, or 'transition' <span class="hlt">zone</span>, are calculated numerically. In-flow and out-flow conditions appropriate to <span class="hlt">ice</span> sheet and <span class="hlt">ice</span> shelf flow are applied at the ends of the transition <span class="hlt">zone</span> and the rigid base is specified; the flow and steady free surfaces are determined as part of the solutions. The basal stress upstream, and the basal deflection downstream, of the flotation point are examined to determine which of these steady solutions satisfy 'contact' conditions that would prevent (i) the steady downstream basal deflection contacting the downstream base, and (ii) the upstream <span class="hlt">ice</span> commencing to float in the event it was melted at the base. In the case that the upstream bed is allowed to slide, we find only one mass flux that satisfies the contact conditions. When no sliding is allowed at the bed, however, we find a range of mass fluxes satisfy the contact conditions. The effect of 'backpressure' on the solutions is investigated, and is found to have no affect on the qualitative behaviour of the junctions. To the extent that the numerical, linearly viscous treatment may be applied to the case of <span class="hlt">ice</span> flowing out over the ocean, we conclude that when sliding is present, Weertman's 'instability' hypothesis holds.</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 <span class="hlt">zone</span> observed at the edge of the consolidated <span class="hlt">ice</span> area where are found the wave-fractured floes (i.e. marginal <span class="hlt">ice</span> <span class="hlt">zone</span> 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 <span class="hlt">zone</span>. 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 marginal <span class="hlt">ice</span> <span class="hlt">zone</span> 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('https://ntrs.nasa.gov/search.jsp?R=19780055834&hterms=fossils&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dfossils','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19780055834&hterms=fossils&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dfossils"><span>Possible fossil H2O liquid-<span class="hlt">ice</span> interfaces in the Martian crust</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Soderblom, L. A.; Wenner, D. B.</p> <p>1978-01-01</p> <p>The extensive chaotic and fretted terrains in the equatorial regions of Mars are explained on the basis of the vertical distribution of H2O liquid and <span class="hlt">ice</span> which once existed in the crust. This account assumes that below the permafrost containing water <span class="hlt">ice</span>, there was a second <span class="hlt">zone</span> in which liquid water resided for at least a time. Diagenetic alteration and cementation characterized the material in the subpermafrost <span class="hlt">zone</span>; above, pristine fragmented material with various <span class="hlt">ice</span> concentrations was found. Later, the <span class="hlt">ice</span>-laden <span class="hlt">zone</span> was stripped away by a number of erosional processes, exposing the former <span class="hlt">ice</span>-liquid water interface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004DSRI...51..307P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004DSRI...51..307P"><span>Geochemical particle fluxes in the Southern Indian Ocean seasonal <span class="hlt">ice</span> <span class="hlt">zone</span>: Prydz Bay region, 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>Pilskaln, C. H.; Manganini, S. J.; Trull, T. W.; Armand, L.; Howard, W.; Asper, V. L.; Massom, R.</p> <p>2004-02-01</p> <p>Time-series sediment traps were deployed between December 1998 and January 2000 and from March 2000 to February 2001 at two offshore Prydz Bay sites within the seasonal <span class="hlt">ice</span> <span class="hlt">zone</span> (SIZ) of the Southern Indian Ocean located between 62-63°S and 73-76°E to quantify seasonal biogeochemical particle fluxes. Samples were obtained from traps placed at 1400, 2400, and 3400 m during the first deployment year (PZB-1) and from 3300 m in the second deployment year (PZB-2). All geochemical export fluxes were highly seasonal with primary peaks occurring during the austral summer and relatively low fluxes prevailing through the winter months. Secondary flux peaks in mid-winter and in early spring were suggestive of small-scale, sea-<span class="hlt">ice</span> break-up events and the spring retreat of seasonal <span class="hlt">ice</span>, respectively. Biogenic silica represented over 70% (by weight) of the collected trap material and provided an annual opal export of 18 g m -2 to 1 km and 3-10 g m -2 to 3 km. POC fluxes supplied an annual export of approximately 1 g m -2, equal to the estimated ocean-wide average. Elevated particulate C org/C inorg and Si bio/C inorg molar ratios indicate a productive, diatom-dominated system, although consistently small fluxes of planktonic foraminifera and pteropod shells document a heterotrophic source of carbonate to deeper waters in the SIZ. The observation of high Si bio/C org ratios and the δ15N time-series data suggest enhanced rates of diatom-POC remineralization in the upper 1000 m relative to bioSiO 2. The occurrence in this region of a pronounced temperature minimum, associated with a strong pycnocline and subsurface particle maximum at 50-100 m, may represent a <span class="hlt">zone</span> where sinking, diatom-rich particulates temporarily accumulate and POC is remineralized.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.C53A..05S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.C53A..05S"><span>Discharge of New Subglacial Lake on Whillians <span class="hlt">Ice</span> Stream: Implication for <span class="hlt">Ice</span> Stream Flow Dynamics.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sergienko, O. V.; Fricker, H. A.; Bindschadler, R. A.; Vornberger, P. L.; Macayeal, D. R.</p> <p>2006-12-01</p> <p>One of the surprise discoveries made possible by the ICESat laser altimeter mission of 2004-2006 is the presence of a large subglacial lake below the grounding <span class="hlt">zone</span> of Whillians <span class="hlt">Ice</span> Stream (dubbed here `Lake Helen' after the discoverer, Helen Fricker). What is even more surprising is the fact that this lake discharged a substantial portion of its volume during the ICESat mission, and changes in lake volume and surface elevation of the <span class="hlt">ice</span> stream are documented in exquisite detail [Fricker et al., in press]. The presence and apparent dynamism of large subglacial lakes in the grounding <span class="hlt">zone</span> of a major <span class="hlt">ice</span> stream raises questions about their effects on <span class="hlt">ice</span>-stream dynamics. Being liquid and movable, water modifies basal friction spatially and temporally. Melting due to shear heating and geothermal flux reduces basal traction, making the <span class="hlt">ice</span> stream move fast. However, when water collects in a depression to form a lake, it potentially deprives the surrounding bed of lubricating water, and additionally makes the <span class="hlt">ice</span> surface flat, thereby locally decreasing the <span class="hlt">ice</span> stream driving stress. We study the effect of formation and discharge of a subglacial lake at the mouth of and <span class="hlt">ice</span> stream using a two dimensional, vertically integrated, <span class="hlt">ice</span>-stream model. The model is forced by the basal friction, <span class="hlt">ice</span> thickness and surface elevation. The basal friction is obtained by inversion of the <span class="hlt">ice</span> surface velocity, <span class="hlt">ice</span> thickness and surface elevation come from observations. To simulate the lake formation we introduce zero basal friction and "inflate" the basal elevation of the <span class="hlt">ice</span> stream at the site of the lake. Sensitivity studies of the response of the surrounding <span class="hlt">ice</span> stream and <span class="hlt">ice</span> shelf flow are performed to delineate the influence of near-grounding-line subglacial water storage for <span class="hlt">ice</span> streams in general.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.C13H..08C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.C13H..08C"><span>Accumulation Rates in the Dry Snow <span class="hlt">Zone</span> of the Greenland <span class="hlt">Ice</span> Sheet Inferred from L-band InSAR Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, A. C.; Zebker, H. A.</p> <p>2012-12-01</p> <p>The Greenland <span class="hlt">ice</span> sheet contains about 2.9 million km3 of <span class="hlt">ice</span> and would raise global sea levels by about 7.1 m if it melted completely. Two unusually large iceberg calving events at Petermann Glacier in the past several years, along with the unusually large extent of <span class="hlt">ice</span> sheet melt this summer point to the relevance of understanding the mass balance of the Greenland <span class="hlt">ice</span> sheet. In this study, we use data from the PALSAR instrument aboard the ALOS satellite to form L-band (23-centimeter carrier wavelength) InSAR images of the dry snow <span class="hlt">zone</span> of the Greenland <span class="hlt">ice</span> sheet. We form geocoded differential interferograms, using the <span class="hlt">ice</span> sheet elevation model produced by Howat et.al. [1]. By applying phase and radiometric calibration, we can examine interferograms formed between any pair of transmit and receive polarization channels. In co-polarized interferograms, the InSAR correlation ranges from about 0.35 at the summit (38.7 deg W, 73.0 deg N) where accumulation is about 20 cm w.e./yr to about 0.70 at the north-eastern part of the dry snow <span class="hlt">zone</span> (35.1 deg W, 77.1 deg N), where accumulation is about 11.7 cm w.e./yr. Cross-polarized interferograms show similar geographic variation with overall lower correlation. We compare our InSAR data with in-situ measurements published by Bales et.al. [2]. We examine the applicability of dense-medium radiative transfer electromagnetic scattering models for estimating accumulation rates from L-band InSAR data. The large number and broad coverage of ALOS scenes acquired between 2007 and 2009 with good InSAR coherence at 46-day repeat times and 21.5 degree incidence angles gives us the opportunity to examine the empirical relationship between in-situ accumulation rate observations and the polarimetric InSAR correlation and radar brightness at this particular imaging geometry. This helps us quantify the accuracy of accumulation rates estimated from InSAR data. In some regions, 46-day interferograms acquired in the winters of several consecutive</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25214629','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25214629"><span>Boundary condition of grounding lines prior to collapse, Larsen-B <span class="hlt">Ice</span> Shelf, Antarctica.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rebesco, M; Domack, E; Zgur, F; Lavoie, C; Leventer, A; Brachfeld, S; Willmott, V; Halverson, G; Truffer, M; Scambos, T; Smith, J; Pettit, E</p> <p>2014-09-12</p> <p>Grounding <span class="hlt">zones</span>, where <span class="hlt">ice</span> sheets transition between resting on bedrock to full floatation, help regulate <span class="hlt">ice</span> flow. Exposure of the sea floor by the 2002 Larsen-B <span class="hlt">Ice</span> Shelf collapse allowed detailed morphologic mapping and sampling of the embayment sea floor. Marine geophysical data collected in 2006 reveal a large, arcuate, complex grounding <span class="hlt">zone</span> sediment system at the front of Crane Fjord. Radiocarbon-constrained chronologies from marine sediment cores indicate loss of <span class="hlt">ice</span> contact with the bed at this site about 12,000 years ago. Previous studies and morphologic mapping of the fjord suggest that the Crane Glacier grounding <span class="hlt">zone</span> was well within the fjord before 2002 and did not retreat further until after the <span class="hlt">ice</span> shelf collapse. This implies that the 2002 Larsen-B <span class="hlt">Ice</span> Shelf collapse likely was a response to surface warming rather than to grounding <span class="hlt">zone</span> instability, strengthening the idea that surface processes controlled the disintegration of the Larsen <span class="hlt">Ice</span> Shelf. Copyright © 2014, American Association for the Advancement of Science.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C53B1038L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C53B1038L"><span>Spatial Variability of accumulation across the Western Greenland <span class="hlt">Ice</span> Sheet Percolation <span class="hlt">Zone</span> from ground-penetrating-radar and shallow firn cores</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lewis, G.; Osterberg, E. C.; Hawley, R. L.; Marshall, H. P.; Birkel, S. D.; Meehan, T. G.; Graeter, K.; Overly, T. B.; McCarthy, F.</p> <p>2017-12-01</p> <p>The mass balance of the Greenland <span class="hlt">Ice</span> Sheet (GrIS) in a warming climate is of critical interest to scientists and the general public in the context of future sea-level rise. Increased melting in the GrIS percolation <span class="hlt">zone</span> over the past several decades has led to increased mass loss at lower elevations due to recent warming. Uncertainties in mass balance are especially large in regions with sparse and/or outdated in situ measurements. This study is the first to calculate in situ accumulation over a large region of western Greenland since the Program for Arctic Regional Climate Assessment campaign during the 1990s. Here we analyze 5000 km of 400 MHz ground penetrating radar data and sixteen 25-33 m-long firn cores in the western GrIS percolation <span class="hlt">zone</span> to determine snow accumulation over the past 50 years. The cores and radar data were collected as part of the 2016-2017 Greenland Traverse for Accumulation and Climate Studies (GreenTrACS). With the cores and radar profiles we capture spatial accumulation gradients between 1850-2500 m a.s.l and up to Summit Station. We calculate accumulation rates and use them to validate five widely used regional climate models and to compare with <span class="hlt">Ice</span>Bridge snow and accumulation radars. Our results indicate that while the models capture most regional spatial climate patterns, they lack the small-scale spatial variability captured by in situ measurements. Additionally, we evaluate temporal trends in accumulation at <span class="hlt">ice</span> core locations and throughout the traverse. Finally, we use empirical orthogonal function and correlation analyses to investigate the principal drivers of radar-derived accumulation rates across the western GrIS percolation <span class="hlt">zone</span>, including major North Atlantic climate modes such as the North Atlantic Oscillation, Atlantic Multidecadal Oscillation, and Greenland Blocking Index.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19970009633','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19970009633"><span>Characterization of <span class="hlt">Ice</span> Roughness From Simulated <span class="hlt">Icing</span> Encounters</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Anderson, David N.; Shin, Jaiwon</p> <p>1997-01-01</p> <p>Detailed measurements of the size of roughness elements on <span class="hlt">ice</span> accreted on models in the NASA Lewis <span class="hlt">Icing</span> Research Tunnel (IRT) were made in a previous study. Only limited data from that study have been published, but included were the roughness element height, diameter and spacing. In the present study, the height and spacing data were found to correlate with the element diameter, and the diameter was found to be a function primarily of the non-dimensional parameters freezing fraction and accumulation parameter. The width of the smooth <span class="hlt">zone</span> which forms at the leading edge of the model was found to decrease with increasing accumulation parameter. Although preliminary, the success of these correlations suggests that it may be possible to develop simple relationships between <span class="hlt">ice</span> roughness and <span class="hlt">icing</span> conditions for use in <span class="hlt">ice</span>-accretion-prediction codes. These codes now require an <span class="hlt">ice</span>-roughness estimate to determine convective heat transfer. Studies using a 7.6-cm-diameter cylinder and a 53.3-cm-chord NACA 0012 airfoil were also performed in which a 1/2-min <span class="hlt">icing</span> spray at an initial set of conditions was followed by a 9-1/2-min spray at a second set of conditions. The resulting <span class="hlt">ice</span> shape was compared with that from a full 10-min spray at the second set of conditions. The initial <span class="hlt">ice</span> accumulation appeared to have no effect on the final <span class="hlt">ice</span> shape. From this result, it would appear the accreting <span class="hlt">ice</span> is affected very little by the initial roughness or shape features.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19840019240','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19840019240"><span>Satellite remote sensing over <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>Thomas, R. H.</p> <p>1984-01-01</p> <p>Satellite remote sensing provides unique opportunities for observing <span class="hlt">ice</span>-covered terrain. Passive-microwave data give information on snow extent on land, sea-<span class="hlt">ice</span> extent and type, and <span class="hlt">zones</span> of summer melting on the polar <span class="hlt">ice</span> sheets, with the potential for estimating snow-accumulation rates on these <span class="hlt">ice</span> sheets. All weather, high-resolution imagery of sea <span class="hlt">ice</span> is obtained using synthetic aperture radars, and <span class="hlt">ice</span>-movement vectors can be deduced by comparing sequential images of the same region. Radar-altimetry data provide highly detailed information on <span class="hlt">ice</span>-sheet topography, with the potential for deducing thickening/thinning rates from repeat surveys. The coastline of Antarctica can be mapped accurately using altimetry data, and the size and spatial distribution of icebergs can be monitored. Altimetry data also distinguish open ocean from pack <span class="hlt">ice</span> and they give an indication of sea-<span class="hlt">ice</span> characteristics.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_8 --> <div id="page_9" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="161"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19860043882&hterms=Antarctic+icebergs&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3DAntarctic%2Bicebergs','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19860043882&hterms=Antarctic+icebergs&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3DAntarctic%2Bicebergs"><span>Satellite remote sensing over <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>Thomas, R. H.</p> <p>1986-01-01</p> <p>Satellite remote sensing provides unique opportunities for observing <span class="hlt">ice</span>-covered terrain. Passive-microwave data give information on snow extent on land, sea-<span class="hlt">ice</span> extent and type, and <span class="hlt">zones</span> of summer melting on the polar <span class="hlt">ice</span> sheets, with the potential for estimating snow-accumulation rates on these <span class="hlt">ice</span> sheets. All weather, high-resolution imagery of sea <span class="hlt">ice</span> is obtained using synthetic aperture radars, and <span class="hlt">ice</span>-movement vectors can be deduced by comparing sequential images of the same region. Radar-altimetry data provide highly detailed information on <span class="hlt">ice</span>-sheet topography, with the potential for deducing thickening/thinning rates from repeat surveys. The coastline of Antarctica can be mapped accurately using altimetry data, and the size and spatial distribution of icebergs can be monitored. Altimetry data also distinguish open ocean from pack <span class="hlt">ice</span> and they give an indication of sea-<span class="hlt">ice</span> characteristics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120009100','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120009100"><span>The Annual Glaciohydrology Cycle in the Ablation <span class="hlt">Zone</span> of the Greenland <span class="hlt">Ice</span> Sheet: Part 1. Hydrology Model</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Colgan, William; Rajaram, Harihar; Anderson, Robert; Steffen. Konrad; Phillips, Thomas; Zwally, H. Jay; Abdalati, Waleed</p> <p>2012-01-01</p> <p>We apply a novel one-dimensional glacier hydrology model that calculates hydraulic head to the tidewater-terminating Sermeq Avannarleq flowline of the Greenland <span class="hlt">ice</span> sheet. Within a plausible parameter space, the model achieves a quasi-steady-state annual cycle in which hydraulic head oscillates close to flotation throughout the ablation <span class="hlt">zone</span>. Flotation is briefly achieved during the summer melt season along a approx.17 km stretch of the approx.50 km of flowline within the ablation <span class="hlt">zone</span>. Beneath the majority of the flowline, subglacial conduit storage closes (i.e. obtains minimum radius) during the winter and opens (i.e. obtains maximum radius) during the summer. Along certain stretches of the flowline, the model predicts that subglacial conduit storage remains open throughout the year. A calculated mean glacier water residence time of approx.2.2 years implies that significant amounts of water are stored in the glacier throughout the year. We interpret this residence time as being indicative of the timescale over which the glacier hydrologic system is capable of adjusting to external surface meltwater forcings. Based on in situ <span class="hlt">ice</span> velocity observations, we suggest that the summer speed-up event generally corresponds to conditions of increasing hydraulic head during inefficient subglacial drainage. Conversely, the slowdown during fall generally corresponds to conditions of decreasing hydraulic head during efficient subglacial drainage.</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 Marginal <span class="hlt">Ice</span> <span class="hlt">Zone</span> 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 Marginal <span class="hlt">Ice</span> <span class="hlt">Zone</span> (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 Marginal <span class="hlt">Ice</span> <span class="hlt">Zone</span> 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://www.dtic.mil/docs/citations/ADA572179','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA572179"><span>Mass Balance of Multiyear Sea <span class="hlt">Ice</span> in the Southern Beaufort Sea</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2012-09-30</p> <p>datasets. Table 1 lists the primary data sources to be used. To determine sources and sinks of MY <span class="hlt">ice</span>, we use a simple model of MY <span class="hlt">ice</span> circulation, which is...shown in Figure 1. In this model , we consider the Beaufort Sea to consist of four <span class="hlt">zones</span> defined by mean drift of sea <span class="hlt">ice</span> in summer and winter, such...Healy/Louis S. St. Laurant cruises 1 Seasonal <span class="hlt">Ice</span> <span class="hlt">Zone</span> Observing Network 2 Polar Airborne Measurements and Arctic Regional Climate Model</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 Marginal <span class="hlt">Zone</span>.</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('http://adsabs.harvard.edu/abs/2013AGUFM.A33C0234Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.A33C0234Y"><span>Minimalist model of <span class="hlt">ice</span> microphysics in mixed-phase stratiform clouds</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, F.; Ovchinnikov, M.; Shaw, R. A.</p> <p>2013-12-01</p> <p>The question of whether persistent <span class="hlt">ice</span> crystal precipitation from supercooled layer clouds can be explained by time-dependent, stochastic <span class="hlt">ice</span> nucleation is explored using an approximate, analytical model and a large-eddy simulation (LES) cloud model. The updraft velocity in the cloud defines an accumulation <span class="hlt">zone</span>, where small <span class="hlt">ice</span> particles cannot fall out until they are large enough, which will increase the residence time of <span class="hlt">ice</span> particles in the cloud. <span class="hlt">Ice</span> particles reach a quasi-steady state between growth by vapor deposition and fall speed at cloud base. The analytical model predicts that <span class="hlt">ice</span> water content (wi) has a 2.5 power-law relationship with <span class="hlt">ice</span> number concentration (ni). wi and ni from a LES cloud model with stochastic <span class="hlt">ice</span> nucleation confirm the 2.5 power-law relationship, and initial indications of the scaling law are observed in data from the Indirect and Semi-Direct Aerosol Campaign. The prefactor of the power law is proportional to the <span class="hlt">ice</span> nucleation rate and therefore provides a quantitative link to observations of <span class="hlt">ice</span> microphysical properties. <span class="hlt">Ice</span> water content (wi) and <span class="hlt">ice</span> number concentration (ni) relationship from LES. a and c: Accumulation <span class="hlt">zone</span> region; b and d: Selective accumulation <span class="hlt">zone</span> region. Black lines in c and d are best fitted 2.5 slope lines. Colors in Figures a and b represent updraft velocity, while colors in c and d represent altitude. The cloud base and top are at about 600 m and 800 m, respectively. <span class="hlt">Ice</span> water content (wi) and <span class="hlt">ice</span> number concentration (ni) relationship for two <span class="hlt">ice</span> nucleation rates. Blue points are from LES with low <span class="hlt">ice</span> nucleation rate and red points with high <span class="hlt">ice</span> nucleation rate. Solid and dashed lines are best fitted 2.5 slope lines.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C51A0955L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C51A0955L"><span>Sea <span class="hlt">ice</span> roughness: the key for predicting Arctic summer <span class="hlt">ice</span> albedo</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Landy, J.; Ehn, J. K.; Tsamados, M.; Stroeve, J.; Barber, D. G.</p> <p>2017-12-01</p> <p>Although melt ponds on Arctic sea <span class="hlt">ice</span> evolve in stages, <span class="hlt">ice</span> with smoother surface topography typically allows the pond water to spread over a wider area, reducing the <span class="hlt">ice</span>-albedo and accelerating further melt. Building on this theory, we simulated the distribution of meltwater on a range of statistically-derived topographies to develop a quantitative relationship between premelt sea <span class="hlt">ice</span> surface roughness and summer <span class="hlt">ice</span> albedo. Our method, previously applied to ICESat observations of the end-of-winter sea <span class="hlt">ice</span> roughness, could account for 85% of the variance in AVHRR observations of the summer <span class="hlt">ice</span>-albedo [Landy et al., 2015]. Consequently, an Arctic-wide reduction in sea <span class="hlt">ice</span> roughness over the ICESat operational period (from 2003 to 2008) explained a drop in <span class="hlt">ice</span>-albedo that resulted in a 16% increase in solar heat input to the sea <span class="hlt">ice</span> cover. Here we will review this work and present new research linking pre-melt sea <span class="hlt">ice</span> surface roughness observations from Cryosat-2 to summer sea <span class="hlt">ice</span> albedo over the past six years, examining the potential of winter roughness as a significant new source of sea <span class="hlt">ice</span> predictability. We will further evaluate the possibility for high-resolution (kilometre-scale) forecasts of summer sea <span class="hlt">ice</span> albedo from waveform-level Cryosat-2 roughness data in the landfast sea <span class="hlt">ice</span> <span class="hlt">zone</span> of the Canadian Arctic. Landy, J. C., J. K. Ehn, and D. G. Barber (2015), Albedo feedback enhanced by smoother Arctic sea <span class="hlt">ice</span>, Geophys. Res. Lett., 42, 10,714-10,720, doi:10.1002/2015GL066712.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70029435','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70029435"><span>Local response of a glacier to annual filling and drainage of an <span class="hlt">ice</span>-marginal 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.; Fountain, A.G.; Anderson, S.P.; Anderson, R. Scott; Malm, A.</p> <p>2006-01-01</p> <p><span class="hlt">Ice</span>-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 '<span class="hlt">ice</span> dam' (the glacier adjacent to the lake) move obliquely to the <span class="hlt">ice</span> margin and rise substantially. As the lake drains, <span class="hlt">ice</span> motion speeds up, becomes nearly perpendicular to the face of the <span class="hlt">ice</span> dam, and the <span class="hlt">ice</span> surface drops. Vertical movement of the <span class="hlt">ice</span> dam probably reflects growth and decay of a wedge of water beneath the <span class="hlt">ice</span> dam, in line with established ideas about jo??kulhlaup mechanics. However, the distribution of vertical <span class="hlt">ice</span> movement, with a narrow (50-100 m wide) <span class="hlt">zone</span> where the uplift rate decreases by 90%, cannot be explained by invoking flexure of the <span class="hlt">ice</span> dam in a fashion analogous to tidal flexure of a floating glacier tongue or <span class="hlt">ice</span> shelf. Rather, the <span class="hlt">zone</span> of large uplift-rate gradient is a fault <span class="hlt">zone</span>: <span class="hlt">ice</span>-dam deformation is dominated by movement along high-angle faults that cut the <span class="hlt">ice</span> dam through its entire thickness, with the sense of fault slip reversing as the lake drains. Survey targets spanning the <span class="hlt">zone</span> 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 <span class="hlt">zone</span>, 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 <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('http://www.dtic.mil/docs/citations/ADA124508','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA124508"><span>Reservoir Bank Erosion Caused and Influenced by <span class="hlt">Ice</span> Cover.</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1982-12-01</p> <p>8 8. Bank sediment deposited on shorefast <span class="hlt">ice</span> ------------ 9 9. Sediment frozen to the bottom of <span class="hlt">ice</span> laid down onto the reservoir bed...end of November 1979 during a storm with 45-mph northwesterly winds-- 17 16. <span class="hlt">Ice</span> and shore sediment uplifted where an <span class="hlt">ice</span> pres- sure ridge intersects...restarts at breakup when the <span class="hlt">ice</span> becomes mobile; the <span class="hlt">ice</span> scrapes, shoves and scours the shore or bank, and transports sediment away. Figure 1. Narrow <span class="hlt">zone</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3997805','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3997805"><span>Marine <span class="hlt">ice</span> regulates the future stability of a large Antarctic <span class="hlt">ice</span> shelf</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Kulessa, Bernd; Jansen, Daniela; Luckman, Adrian J.; King, Edward C.; Sammonds, Peter R.</p> <p>2014-01-01</p> <p>The collapses of the Larsen A and B <span class="hlt">ice</span> shelves on the Antarctic Peninsula in 1995 and 2002 confirm the impact of southward-propagating climate warming in this region. Recent mass and dynamic changes of Larsen B’s southern neighbour Larsen C, the fourth largest <span class="hlt">ice</span> shelf in Antarctica, may herald a similar instability. Here, using a validated <span class="hlt">ice</span>-shelf model run in diagnostic mode, constrained by satellite and in situ geophysical data, we identify the nature of this potential instability. We demonstrate that the present-day spatial distribution and orientation of the principal stresses within Larsen C <span class="hlt">ice</span> shelf are akin to those within pre-collapse Larsen B. When Larsen B’s stabilizing frontal portion was lost in 1995, the unstable remaining shelf accelerated, crumbled and ultimately collapsed. We hypothesize that Larsen C <span class="hlt">ice</span> shelf may suffer a similar fate if it were not stabilized by warm and mechanically soft marine <span class="hlt">ice</span>, entrained within narrow suture <span class="hlt">zones</span>. PMID:24751641</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009PhDT........67W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009PhDT........67W"><span><span class="hlt">Ice</span>-atmosphere interactions in the Canadian High Arctic: Implications for the thermo-mechanical evolution of terrestrial <span class="hlt">ice</span> masses</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wohlleben, Trudy M. H.</p> <p></p> <p>Canadian High Arctic terrestrial <span class="hlt">ice</span> masses and the polar atmosphere evolve codependently, and interactions between the two systems can lead to feedbacks, positive and negative. The two primary positive cryosphere-atmosphere feedbacks are: (1) The snow/<span class="hlt">ice</span>-albedo feedback (where area changes in snow and/or <span class="hlt">ice</span> cause changes in surface albedo and surface air temperatures, leading to further area changes in snow/<span class="hlt">ice</span>); and (2) The elevation - mass balance feedback (where thickness changes in terrestrial <span class="hlt">ice</span> masses cause changes to atmospheric circulation and precipitation patterns, leading to further <span class="hlt">ice</span> thickness changes). In this thesis, numerical experiments are performed to: (1) quantify the magnitudes of the two feedbacks for chosen Canadian High Arctic terrestrial <span class="hlt">ice</span> masses; and (2) to examine the direct and indirect consequences of surface air temperature changes upon englacial temperatures with implications for <span class="hlt">ice</span> flow, mass flux divergence, and topographic evolution. Model results show that: (a) for John Evans Glacier, Ellesmere Island, the magnitude of the terrestrial snow/<span class="hlt">ice</span>-albedo feedback can locally exceed that of sea <span class="hlt">ice</span> on less than decadal timescales, with implications for glacier response times to climate perturbations; (b) although historical air temperature changes might be the direct cause of measured englacial temperature anomalies in various glacier and <span class="hlt">ice</span> cap accumulation <span class="hlt">zones</span>, they can also be the indirect cause of their enhanced diffusive loss; (c) while the direct result of past air temperature changes has been to cool the interior of John Evans Glacier, and its bed, the indirect result has been to create and maintain warm (pressure melting point) basal temperatures in the ablation <span class="hlt">zone</span>; and (d) for Devon <span class="hlt">Ice</span> Cap, observed mass gains in the northwest sector of the <span class="hlt">ice</span> cap would be smaller without orographic precipitation and the mass balance---elevation feedback, supporting the hypothesis that this feedback is playing a role in the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRC..123..746B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123..746B"><span>Physical and Biological Drivers of Biogeochemical Tracers Within the Seasonal Sea <span class="hlt">Ice</span> <span class="hlt">Zone</span> of the Southern Ocean From Profiling Floats</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Briggs, Ellen M.; Martz, Todd R.; Talley, Lynne D.; Mazloff, Matthew R.; Johnson, Kenneth S.</p> <p>2018-02-01</p> <p>Here we present initial findings from nine profiling floats equipped with pH, O2, NO3-, and other biogeochemical sensors that were deployed in the seasonal <span class="hlt">ice</span> <span class="hlt">zone</span> (SIZ) of the Southern Ocean in 2014 and 2015 through the Southern Ocean Carbon and Climate Observations and Modelling (SOCCOM) project. A large springtime phytoplankton bloom was observed that coincided with sea <span class="hlt">ice</span> melt for all nine floats. We argue this bloom results from a shoaling of the mixed layer depth, increased vertical stability, and enhanced nutrient and light availability as the sea <span class="hlt">ice</span> melts. This interpretation is supported by the absence of a springtime bloom when one of the floats left the SIZ in the second year of observations. During the sea <span class="hlt">ice</span> covered period, net heterotrophic conditions were observed. The rate of uptake of O2 and release of dissolved inorganic carbon (derived from pH and estimated total alkalinity) and NO3- is reminiscent of biological respiration and is nearly Redfieldian for the nine floats. A simple model of mixed layer physics was developed to separate the physical and biological components of the signal in pH and O2 over one annual cycle for a float in the Ross Sea SIZ. The resulting annual net community production suggests that seasonal respiration during the <span class="hlt">ice</span> covered period of the year nearly balances the production in the euphotic layer of up to 5 mol C m-2 during the <span class="hlt">ice</span> free period leading to a net of near zero carbon exported to depth for this one float.</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 marginal <span class="hlt">ice</span> <span class="hlt">zone</span>, 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://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 Marginal <span class="hlt">Ice</span> <span class="hlt">Zone</span> 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('http://www.dtic.mil/docs/citations/ADA601788','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA601788"><span>Acquisition of <span class="hlt">Ice</span> Thickness and <span class="hlt">Ice</span> Surface Characteristics in the Seasonal <span class="hlt">Ice</span> <span class="hlt">Zone</span> by CULPIS-X During the US Coast Guard’s Arctic Domain Awareness Program</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>What is the volume of sea <span class="hlt">ice</span> in the Beaufort Sea SIZ and how does this evolve during summer as the <span class="hlt">ice</span> edge retreats? Recent observations...suggest that the remaining <span class="hlt">ice</span> in the Beaufort Sea is younger and thinner in recent years in part because even the oldest <span class="hlt">ice</span> advected into the region does...indicated that ponds on thinner <span class="hlt">ice</span> are often darker, accelerating the <span class="hlt">ice</span> - albedo feedback over thin <span class="hlt">ice</span> in summer. During winter, leads and very</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>Marginal <span class="hlt">Ice</span> <span class="hlt">Zone</span> (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=19860048367&hterms=marginal&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dmarginal','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19860048367&hterms=marginal&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dmarginal"><span>Weddell-Scotia sea marginal <span class="hlt">ice</span> <span class="hlt">zone</span> observations from space, October 1984</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.; Holt, B.; Martin, S.; Rothrock, D. A.; Mcnutt, L.</p> <p>1986-01-01</p> <p>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 <span class="hlt">ice</span> margin of the Weddell-Scotia Seas region. At the <span class="hlt">ice</span> edge, the <span class="hlt">ice</span> forms into bandlike aggregates of small <span class="hlt">ice</span> 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.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6648212-fire-beneath-ice','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6648212-fire-beneath-ice"><span>Fire beneath the <span class="hlt">ice</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Monastersky, R.</p> <p>1993-02-13</p> <p>A volcano discovered six years ago by researchers Blankenship and Bell under Antarctica poses questions about a potential climatic catastrophe. The researchers claim that the volcano is still active, erupting occasionally and growing. A circular depression on the surface of the <span class="hlt">ice</span> sheet has <span class="hlt">ice</span> flowing into it and is used to provide a portrait of the heat source. The volcano is on a critical transition <span class="hlt">zone</span> within West Antarctica with fast flowing <span class="hlt">ice</span> streams directly downhill. Work by Blankenship shows that a soft layer of water-logged sediments called till provide the lubricating layer on the underside of the icemore » streams. Volcanos may provide the source of this till. The <span class="hlt">ice</span> streams buffer the thick interior <span class="hlt">ice</span> from the ocean and no one know what will happen if the <span class="hlt">ice</span> streams continue to shorten. These researchers believe their results indicate that the stability of West Antarctica ultimately depends less on the current climate than on the location of heat and sediments under the <span class="hlt">ice</span> and the legacy of past climatic changes.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA617866','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA617866"><span>Seasonal <span class="hlt">Ice</span> <span class="hlt">Zone</span> Reconnaissance Surveys Coordination</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>profiler (AXCP) ocean velocity shear (Morison), UpTempO buoy measurements of sea surface temperature (SST), sea level atmospheric pressure ( SLP ), and...and prediction…. Steele UpTempO buoy drops for SLP , SST, SSS, & surface velocity Visible and Thermal Images of the SIZ from the Coast Guard...Expendable CTD, AXCP= Air Expendable Current Profiler, SLP = Sea Level atmospheric Pressure, SST= Seas Surface Temperature, A/C= aircraft, SIC=Sea <span class="hlt">Ice</span></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 margin 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 margin, in the ablation <span class="hlt">zone</span>, 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 margin 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 <span class="hlt">zone</span> 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 <span class="hlt">zone</span> 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 <span class="hlt">zone</span> 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> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_9 --> <div id="page_10" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="181"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013QSRv...79..168A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013QSRv...79..168A"><span>A review of sea <span class="hlt">ice</span> proxy information from polar <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>Abram, Nerilie J.; Wolff, Eric W.; Curran, Mark A. J.</p> <p>2013-11-01</p> <p>Sea <span class="hlt">ice</span> plays an important role in Earth's climate system. The lack of direct indications of past sea <span class="hlt">ice</span> coverage, however, means that there is limited knowledge of the sensitivity and rate at which sea <span class="hlt">ice</span> dynamics are involved in amplifying climate changes. As such, there is a need to develop new proxy records for reconstructing past sea <span class="hlt">ice</span> conditions. Here we review the advances that have been made in using chemical tracers preserved in <span class="hlt">ice</span> cores to determine past changes in sea <span class="hlt">ice</span> cover around Antarctica. <span class="hlt">Ice</span> core records of sea salt concentration show promise for revealing patterns of sea <span class="hlt">ice</span> extent particularly over glacial-interglacial time scales. In the coldest climates, however, the sea salt signal appears to lose sensitivity and further work is required to determine how this proxy can be developed into a quantitative sea <span class="hlt">ice</span> indicator. Methane sulphonic acid (MSA) in near-coastal <span class="hlt">ice</span> cores has been used to reconstruct quantified changes and interannual variability in sea <span class="hlt">ice</span> extent over shorter time scales spanning the last ˜160 years, and has potential to be extended to produce records of Antarctic sea <span class="hlt">ice</span> changes throughout the Holocene. However the MSA <span class="hlt">ice</span> core proxy also requires careful site assessment and interpretation alongside other palaeoclimate indicators to ensure reconstructions are not biased by non-sea <span class="hlt">ice</span> factors, and we summarise some recommended strategies for the further development of sea <span class="hlt">ice</span> histories from <span class="hlt">ice</span> core MSA. For both proxies the limited information about the production and transfer of chemical markers from the sea <span class="hlt">ice</span> <span class="hlt">zone</span> to the Antarctic <span class="hlt">ice</span> sheets remains an issue that requires further multidisciplinary study. Despite some exploratory and statistical work, the application of either proxy as an indicator of sea <span class="hlt">ice</span> change in the Arctic also remains largely unknown. As information about these new <span class="hlt">ice</span> core proxies builds, so too does the potential to develop a more comprehensive understanding of past changes in sea</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/638180','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/638180"><span>Separations on water-<span class="hlt">ice</span>. Final report</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Dasgupta, P.K.</p> <p>1998-07-01</p> <p>This report focuses on processes to separate water frozen into <span class="hlt">ice</span>. Research topics include the following: normal phase columnar chromatography; electrophoresis in a planar format; and <span class="hlt">zone</span> melting type separations on a solid column of <span class="hlt">ice</span>. Attempts were made to dope the emulsion with {beta}-cyclodextrin in order to separate commercially important chiral drugs such as Inderal.</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 marginal <span class="hlt">ice</span> <span class="hlt">zone</span> 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('http://adsabs.harvard.edu/abs/2015AGUFMOS11B..02B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMOS11B..02B"><span>Observing Physical and Biological Drivers of pH and O2 in a Seasonal <span class="hlt">Ice</span> <span class="hlt">Zone</span> in the Ross Sea Using Profiling Float Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Briggs, E.; Martz, T. R.; Talley, L. D.; Mazloff, M. R.</p> <p>2015-12-01</p> <p><span class="hlt">Ice</span> cover has strong influence over gas exchange, vertical stability, and biological production which are critical to understanding the Southern Ocean's central role in oceanic biogeochemical cycling and heat and carbon uptake under a changing climate. However the relative influence of physical versus biological processes in this hard-to-study region is poorly understood due to limited observations. Here we present new findings from a profiling float equipped with biogeochemical sensors in the seasonal <span class="hlt">ice</span> <span class="hlt">zone</span> of the Ross Sea capturing, for the first time, under-<span class="hlt">ice</span> pH profile data over a two year timespan from 2014 to the present. The relative influence of physical (e.g. vertical mixing and air-sea gas exchange) and biological (e.g. production and respiration) drivers of pH and O2 within the mixed layer are explored during the phases of <span class="hlt">ice</span> formation, <span class="hlt">ice</span> cover, and <span class="hlt">ice</span> melt over the two seasonal cycles. During the austral fall just prior to and during <span class="hlt">ice</span> formation, O2 increases as expected due to surface-layer undersaturation and enhanced gas exchange. A small increase in pH is also observed during this phase, but without a biological signal in accompanying profiling float chlorophyll data, which goes against common reasoning from both a biological and physical standpoint. During the phase of <span class="hlt">ice</span> cover, gas exchange is inhibited and a clear respiration signal is observed in pH and O2 data from which respiration rates are calculated. In the austral spring, <span class="hlt">ice</span> melt gives rise to substantial <span class="hlt">ice</span> edge phytoplankton blooms indicated by O2 supersaturation and corresponding increase in pH and large chlorophyll signal. The influence of the duration of <span class="hlt">ice</span> cover and mixed layer depth on the magnitude of the <span class="hlt">ice</span> edge blooms is explored between the two seasonal cycles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C41E0717L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C41E0717L"><span>Albedo Spatial Variability and Causes on the Western Greenland <span class="hlt">Ice</span> Sheet Percolation <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lewis, G.; Osterberg, E. C.; Hawley, R. L.; Koffman, B. G.; Marshall, H. P.; Birkel, S. D.; Dibb, J. E.</p> <p>2016-12-01</p> <p>Many recent studies have concluded that Greenland <span class="hlt">Ice</span> Sheet (GIS) mass loss has been accelerating over recent decades, but spatial and temporal variations in GIS mass balance remain poorly understood due to a complex relationship among precipitation and temperature changes, increasing melt and runoff, <span class="hlt">ice</span> discharge, and surface albedo. Satellite measurements from MODerate resolution Imaging Spectroradiometer (MODIS) indicate that albedo has been declining over the past decade, but the cause and extent of GIS albedo change remains poorly constrained by field data. As fresh snow (albedo > 0.85) warms and melts, its albedo decreases due to snow grain growth, promoting solar absorption, higher snowpack temperatures and further melt. However, dark impurities like soot and dust can also significantly reduce snow albedo, even in the dry snow <span class="hlt">zone</span>. While many regional climate models (e.g. the Regional Atmospheric Climate MOdel - RACMO2) calculate albedo spatial resolutions on the order of 10-30 km, and MODIS averages albedo over 500 m, surface features like sastrugi can affect albedo on much smaller scales. Here we assess the relative importance of grain size and shape vs. impurity concentrations on albedo in the western GIS percolation <span class="hlt">zone</span>. We collected broadband albedo measurements (300-2500 nm at 3-8 nm resolution) at 35 locations using an ASD FieldSpec4 spectroradiometer to simultaneously quantify radiative fluxes and spectral reflectance. Measurements were collected on 10 x 10 m, 1 x 1 km, 5 x 5 km, and 10 x 10 km grids to determine the spatial variability of albedo as part of the 850-km Greenland Traverse for Accumulation and Climate Studies (GreenTrACS) traverse from Raven/Dye 2 to Summit. Additionally, we collected shallow (0-50 cm) snow pit samples every 5 cm at ASD measurement sites to quantify black carbon and mineral dust concentrations and size distributions using a Single Particle Soot Photometer and Coulter Counter, respectively. Preliminary results</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/6091444','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/6091444"><span>Arctic <span class="hlt">ice</span> islands</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>Sackinger, W.M.; Jeffries, M.O.; Lu, M.C.</p> <p>1988-01-01</p> <p>The development of offshore oil and gas resources in the Arctic waters of Alaska requires offshore structures which successfully resist the lateral forces due to moving, drifting <span class="hlt">ice</span>. <span class="hlt">Ice</span> islands are floating, a tabular icebergs, up to 60 meters thick, of solid <span class="hlt">ice</span> throughout their thickness. The <span class="hlt">ice</span> islands are thus regarded as the strongest <span class="hlt">ice</span> features in the Arctic; fixed offshore structures which can directly withstand the impact of <span class="hlt">ice</span> islands are possible but in some locations may be so expensive as to make oilfield development uneconomic. The resolution of the <span class="hlt">ice</span> island problem requires two research steps: (1)more » calculation of the probability of interaction between an <span class="hlt">ice</span> island and an offshore structure in a given region; and (2) if the probability if sufficiently large, then the study of possible interactions between <span class="hlt">ice</span> island and structure, to discover mitigative measures to deal with the moving <span class="hlt">ice</span> island. The <span class="hlt">ice</span> island research conducted during the 1983-1988 interval, which is summarized in this report, was concerned with the first step. Monte Carlo simulations of <span class="hlt">ice</span> island generation and movement suggest that <span class="hlt">ice</span> island lifetimes range from 0 to 70 years, and that 85% of the lifetimes are less then 35 years. The simulation shows a mean value of 18 <span class="hlt">ice</span> islands present at any time in the Arctic Ocean, with a 90% probability of less than 30 <span class="hlt">ice</span> islands. At this time, approximately 34 <span class="hlt">ice</span> islands are known, from observations, to exist in the Arctic Ocean, not including the 10-meter thick class of <span class="hlt">ice</span> islands. Return interval plots from the simulation show that coastal <span class="hlt">zones</span> of the Beaufort and Chukchi Seas, already leased for oil development, have <span class="hlt">ice</span> island recurrences of 10 to 100 years. This implies that the <span class="hlt">ice</span> island hazard must be considered thoroughly, and appropriate safety measures adopted, when offshore oil production plans are formulated for the Alaskan Arctic offshore. 132 refs., 161 figs., 17 tabs.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.C53B0303S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.C53B0303S"><span>Characterizing Englacial Attenuation and Grounding <span class="hlt">Zone</span> Geometry Using Airborne Radar Sounding</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schroeder, D. M.; Grima, C.; Blankenship, D. D.</p> <p>2014-12-01</p> <p>The impact of warm ocean water on <span class="hlt">ice</span> sheet retreat and stability is a one of the primary drivers and sources of uncertainty for the rate of global sea level rise. One critical but challenging observation required to understand and model this impact is the location and extent of grounding <span class="hlt">ice</span> sheet <span class="hlt">zones</span>. However, existing surface topography based techniques do not directly detect the location where ocean water reaches (or breaches) grounded <span class="hlt">ice</span> at the bed, which can significantly affect <span class="hlt">ice</span> sheet stability. The primary geophysical tool for directly observing the basal properties of <span class="hlt">ice</span> sheets is airborne radar sounding. However, uncertainty in englacial attenuation from unknown <span class="hlt">ice</span> temperature and chemistry can lead to erroneous interpretation of subglacial conditions from bed echo strengths alone . Recently developed analysis techniques for radar sounding data have overcome this challenge by taking advantage of information in the angular distribution of bed echo energy and joint modeling of radar returns and water routing. We have developed similar approaches to analyze the spatial pattern and character of echoes to address the problems of improved characterization of grounding <span class="hlt">zone</span> geometry and englacial attenuation. The spatial signal of the transition from an <span class="hlt">ice</span>-bed interface to an <span class="hlt">ice</span>-ocean interface is an increase in bed echo strength. However, rapidly changing attenuation near the grounding <span class="hlt">zone</span> prevents the unambiguous interpretation of this signal in typical echo strength profiles and violates the assumptions of existing empirical attenuation correction techniques. We present a technique that treat bed echoes as continuous signals to take advantage of along-profile <span class="hlt">ice</span> thickness and echo strength variations to constrain the spatial pattern of attenuation and detect the grounding <span class="hlt">zone</span> transition. The transition from an <span class="hlt">ice</span>-bed interface to an <span class="hlt">ice</span>-ocean interface will also result in a change in the processes that determine basal interface morphology (e</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040035532&hterms=information+needs&qs=N%3D0%26Ntk%3DTitle%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dinformation%2Bneeds','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040035532&hterms=information+needs&qs=N%3D0%26Ntk%3DTitle%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dinformation%2Bneeds"><span>Pilots' Information Needs and Strategies for Operating in <span class="hlt">Icing</span> Conditions</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Vigeant-Langlois, Laurence N.; Hansman, R. John</p> <p>2003-01-01</p> <p>Pilot current use of <span class="hlt">icing</span> information, pilot encounters and strategies for dealing with in-flight aircraft structural <span class="hlt">icing</span> situations, and desired attributes of new <span class="hlt">icing</span> information systems were investigated through a survey of pilots of several operational categories. The survey identified important information elements and fiequently used information paths for obtaining <span class="hlt">icing</span>-related information. Free- response questions solicited descriptions of significant , <span class="hlt">icing</span> encounters, and probed key <span class="hlt">icing</span>-related decision and information criteria. Results indicated the information needs for the horizontal and vertical location of <span class="hlt">icing</span> conditions and the identification of <span class="hlt">icing</span>-free <span class="hlt">zones</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19820006693&hterms=marginal&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dmarginal','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19820006693&hterms=marginal&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dmarginal"><span>The Norwegian remote sensing experiment (Norsex) in a marginal <span class="hlt">ice</span> <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Farrelly, B.; Johannessen, J.; Johannessen, O. M.; Svendson, E.; Kloster, K.; Horjen, I.; Campbell, W. J.; Crawford, J.; Harrington, R.; Jones, L.</p> <p>1981-01-01</p> <p>Passive and active microwave measurements from surface based, airborne, and satellite instruments were obtained together with surface observations northwest of Svalbard. Emissivities of different <span class="hlt">ice</span> patches in the <span class="hlt">ice</span> 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 <span class="hlt">ice</span> classification. A variety of mesoscale features under different meteorological conditions is revealed by a 1.36 GHz synthetic aperture radar. <span class="hlt">Ice</span> edge location by Nimbus 7 scanning multifrequency microwave radiometer is shown accurate to 10 km when the 37 GHz horizontal polarized channel is used.</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 Marginal <span class="hlt">Ice</span> <span class="hlt">Zone</span> (MIZ). The problems, results and future potential of such observations are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20070016598&hterms=sea+ice+albedo&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dsea%2Bice%2Balbedo','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20070016598&hterms=sea+ice+albedo&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dsea%2Bice%2Balbedo"><span>Observational Evidence of a Hemispheric-wide <span class="hlt">Ice</span>-ocean Albedo Feedback Effect on Antarctic Sea-<span class="hlt">ice</span> Decay</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nihashi, Sohey; Cavalieri, Donald J.</p> <p>2007-01-01</p> <p>The effect of <span class="hlt">ice</span>-ocean albedo feedback (a kind of <span class="hlt">ice</span>-albedo feedback) on sea-<span class="hlt">ice</span> decay is demonstrated over the Antarctic sea-<span class="hlt">ice</span> <span class="hlt">zone</span> from an analysis of satellite-derived hemispheric sea <span class="hlt">ice</span> concentration and European Centre for Medium-Range Weather Forecasts (ERA-40) atmospheric data for the period 1979-2001. Sea <span class="hlt">ice</span> concentration in December (time of most active melt) correlates better with the meridional component of the wind-forced <span class="hlt">ice</span> drift (MID) in November (beginning of the melt season) than the MID in December. This 1 month lagged correlation is observed in most of the Antarctic sea-<span class="hlt">ice</span> covered ocean. Daily time series of <span class="hlt">ice</span> , concentration show that the <span class="hlt">ice</span> concentration anomaly increases toward the time of maximum sea-<span class="hlt">ice</span> melt. These findings can be explained by the following positive feedback effect: once <span class="hlt">ice</span> concentration decreases (increases) at the beginning of the melt season, solar heating of the upper ocean through the increased (decreased) open water fraction is enhanced (reduced), leading to (suppressing) a further decrease in <span class="hlt">ice</span> concentration by the oceanic heat. Results obtained fi-om a simple <span class="hlt">ice</span>-ocean coupled model also support our interpretation of the observational results. This positive feedback mechanism explains in part the large interannual variability of the sea-<span class="hlt">ice</span> cover in summer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930063983&hterms=photography&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DTitle%26N%3D0%26No%3D50%26Ntt%3Dphotography','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930063983&hterms=photography&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DTitle%26N%3D0%26No%3D50%26Ntt%3Dphotography"><span><span class="hlt">Ice</span> patterns and hydrothermal plumes, Lake Baikal, Russia - Insights from Space Shuttle hand-held photography</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Evans, Cynthia A.; Helfert, Michael R.; Helms, David R.</p> <p>1992-01-01</p> <p>Earth photography from the Space Shuttle is used to examine the <span class="hlt">ice</span> cover on Lake Baikal and correlate the patterns of weakened and melting <span class="hlt">ice</span> with known hydrothermal areas in the Siberian lake. Particular <span class="hlt">zones</span> of melted and broken <span class="hlt">ice</span> may be surface expressions of elevated heat flow in Lake Baikal. The possibility is explored that hydrothermal vents can introduce local convective upwelling and disrupt a stable water column to the extent that the melt <span class="hlt">zones</span> which are observed in the lake's <span class="hlt">ice</span> cover are produced. A heat flow map and photographs of the lake are overlaid to compare specific areas of thinned or broken <span class="hlt">ice</span> with the hot spots. The regions of known hydrothermal activity and high heat flow correlate extremely well with circular regions of thinned <span class="hlt">ice</span>, and <span class="hlt">zones</span> of broken and recrystallized <span class="hlt">ice</span>. Local and regional climate data and other sources of warm water, such as river inlets, are considered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('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 marginal <span class="hlt">ice</span> <span class="hlt">zone</span></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 active-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('http://hdl.handle.net/2060/19940019049','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940019049"><span>Characteristics of surface roughness associated with leading edge <span class="hlt">ice</span> accretion</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Shin, Jaiwon</p> <p>1994-01-01</p> <p>Detailed size measurements of surface roughness associated with leading edge <span class="hlt">ice</span> accretions are presented to provide information on characteristics of roughness and trends of roughness development with various <span class="hlt">icing</span> parameters. Data was obtained from <span class="hlt">icing</span> tests conducted in the <span class="hlt">Icing</span> Research Tunnel (IRT) at NASA Lewis Research Center (LeRC) using a NACA 0012 airfoil. Measurements include diameters, heights, and spacing of roughness elements along with chordwise <span class="hlt">icing</span> limits. Results confirm the existence of smooth and rough <span class="hlt">ice</span> <span class="hlt">zones</span> and that the boundary between the two <span class="hlt">zones</span> (surface roughness transition region) moves upstream towards stagnation region with time. The height of roughness grows as the air temperature and the liquid water content increase, however, the airspeed has little effect on the roughness height. Results also show that the roughness in the surface roughness transition region grows during a very early stage of accretion but reaches a critical height and then remains fairly constant. Results also indicate that a uniformly distributed roughness model is only valid at a very initial stage of the <span class="hlt">ice</span> accretion process.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19830044475&hterms=empiricism&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dempiricism','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19830044475&hterms=empiricism&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dempiricism"><span>'Scaling' analysis of the <span class="hlt">ice</span> accretion process on aircraft surfaces</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Keshock, E. G.; Tabrizi, A. H.; Missimer, J. R.</p> <p>1982-01-01</p> <p>A comprehensive set of scaling parameters is developed for the <span class="hlt">ice</span> accretion process by analyzing the energy equations of the dynamic freezing <span class="hlt">zone</span> and the already frozen <span class="hlt">ice</span> layer, the continuity equation associated with supercooled liquid droplets entering into and impacting within the dynamic freezing <span class="hlt">zone</span>, and energy equation of the <span class="hlt">ice</span> layer. No initial arbitrary judgments are made regarding the relative magnitudes of each of the terms. The method of intrinsic reference variables in employed in order to develop the appropriate scaling parameters and their relative significance in rime <span class="hlt">icing</span> conditions in an orderly process, rather than utilizing empiricism. The significance of these parameters is examined and the parameters are combined with scaling criteria related to droplet trajectory similitude.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22181553','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22181553"><span>Suppression of the water <span class="hlt">ice</span> and snow albedo feedback on planets orbiting red dwarf stars and the subsequent widening of the habitable <span class="hlt">zone</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Joshi, Manoj M; Haberle, Robert M</p> <p>2012-01-01</p> <p>M stars comprise 80% of main sequence stars, so their planetary systems provide the best chance for finding habitable planets, that is, those with surface liquid water. We have modeled the broadband albedo or reflectivity of water <span class="hlt">ice</span> and snow for simulated planetary surfaces orbiting two observed red dwarf stars (or M stars), using spectrally resolved data of Earth's cryosphere. The gradual reduction of the albedos of snow and <span class="hlt">ice</span> at wavelengths greater than 1 μm, combined with M stars emitting a significant fraction of their radiation at these same longer wavelengths, means that the albedos of <span class="hlt">ice</span> and snow on planets orbiting M stars are much lower than their values on Earth. Our results imply that the <span class="hlt">ice</span>/snow albedo climate feedback is significantly weaker for planets orbiting M stars than for planets orbiting G-type stars such as the Sun. In addition, planets with significant <span class="hlt">ice</span> and snow cover will have significantly higher surface temperatures for a given stellar flux if the spectral variation of cryospheric albedo is considered, which in turn implies that the outer edge of the habitable <span class="hlt">zone</span> around M stars may be 10-30% farther away from the parent star than previously thought.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A33M..02W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A33M..02W"><span>Upper-Tropospheric Cloud <span class="hlt">Ice</span> from <span class="hlt">Ice</span>Cube</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wu, D. L.</p> <p>2017-12-01</p> <p>, 2017 shows a clear distribution of the inter-tropical convergence <span class="hlt">zone</span> (ITCZ), as well as the classic Gill-model pattern over the Western Pacific and Indian monsoon regions. Like the ISS, the coverage of ICIR observations is limited to low-to-mid latitudes. More science results and <span class="hlt">Ice</span>Cube experiments with the cubesat operation will be discussed.</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 Marginal <span class="hlt">Ice</span> <span class="hlt">Zone</span>: 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('http://adsabs.harvard.edu/abs/2017AGUFM.C13F1014L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C13F1014L"><span>The Effect of Topographic Shadowing by <span class="hlt">Ice</span> on Irradiance in the Greenland <span class="hlt">Ice</span> Sheet Ablation <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Leidman, S. Z.; Rennermalm, A. K.; Ryan, J.; Cooper, M. G.; Smith, L. C.</p> <p>2017-12-01</p> <p>Accurately predicting runoff contributions to global sea level rise requires more refined surface mass balance (SMB) models of the Greenland <span class="hlt">Ice</span> Sheet (GrIS). Topographic shadowing has shown to be important in the SMB of snow-covered regions, yet SMB models for the GrIS generally ignore how surface topography affects spatial variability of incoming solar radiation on a surface. In the ablation <span class="hlt">zone</span> of Southwest Greenland, deeply incised supraglacial drainage features, fracturing, and large-scale bed deformation result in extensive areas of rough surface topography. This topography blocks direct radiation such that shadowed areas receive less energy for melting while other topographic features such as peaks recieve more energy. In this study, we quantify how shadowing from local topography features changes incoming solar radiation. We apply the ArcGIS Pro Solar Radiation Toolset to calculate the direct and diffuse irradiance in sunlit and shadowed areas by determining the sun's movement for every half hour increment of 2016. Multiple digital elevation models (DEMs) with spatial resolutions ranging from 0.06 to 5m were derived from fixed wing and quadcopter UAV imagery collected in summer 2016 and the ArcticDEM dataset. Our findings show that shadowing significantly decreases irradiance compared to smoothed surfaces where local topography is removed. This decrease is exponentially proportional to the DEM pixel sized with 5m DEMs only able to capture a small percentage of the effect. Applying these calculations to the ArcticDEM to cover a larger study area indicates that decreases in irradiance are nonlinearly proportional to elevation with highly crevassed areas showing a larger effect from shadowing. Even so, shading at higher elevations reduces irradiance enough to result in several centimeters snow water equivalence (SWE) per year of over-prediction of runoff in SMB models. Furthermore, analysis of solar radiation products shows that shadowing predicts albedo</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.C13D..06G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.C13D..06G"><span>The response of grounded <span class="hlt">ice</span> to ocean temperature forcing in a coupled <span class="hlt">ice</span> sheet-<span class="hlt">ice</span> shelf-ocean cavity model</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.</p> <p>2010-12-01</p> <p><span class="hlt">Ice</span> shelves provide a pathway for the heat content of the ocean to influence continental <span class="hlt">ice</span> sheets. Changes in the rate or location of basal melting can alter their geometry and effect changes in stress conditions at the grounding line, leading to a grounded <span class="hlt">ice</span> response. Recent observations of <span class="hlt">ice</span> streams and <span class="hlt">ice</span> shelves in the Amundsen Sea sector of West Antarctica have been consistent with this story. On the other hand, <span class="hlt">ice</span> dynamics in the grounding <span class="hlt">zone</span> control flux into the shelf and thus <span class="hlt">ice</span> shelf geometry, which has a strong influence on the circulation in the cavity beneath the shelf. Thus the coupling between the two systems, ocean and <span class="hlt">ice</span> sheet-<span class="hlt">ice</span> shelf, can be quite strong. We examine the response of the <span class="hlt">ice</span> sheet-<span class="hlt">ice</span> shelf-ocean cavity system to changes in ocean temperature using a recently developed coupled model. The coupled model consists a 3-D ocean model (GFDL's Generalized Ocean Layered Dynamics model, or GOLD) to a two-dimensional <span class="hlt">ice</span> sheet-<span class="hlt">ice</span> shelf model (Goldberg et al, 2009), and allows for changing cavity geometry and a migrating grounding line. Steady states of the coupled system are found even under considerable forcing. The <span class="hlt">ice</span> shelf morphology and basal melt rate patterns of the steady states exhibit detailed structure, and furthermore seem to be unique and robust. The relationship between temperature forcing and area-averaged melt rate is influenced by the response of <span class="hlt">ice</span> shelf morphology to thermal forcing, and is found to be sublinear in the range of forcing considered. However, results suggest that area-averaged melt rate is not the best predictor of overall system response, as grounding line stability depends on local aspects of the basal melt field. Goldberg, D N, D M Holland and C G Schoof, 2009. Grounding line movement and <span class="hlt">ice</span> shelf buttressing in marine <span class="hlt">ice</span> sheets, Journal of Geophysical Research-Earth Surfaces, 114, F04026.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_10 --> <div id="page_11" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="201"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1987AdSpR...7..125R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1987AdSpR...7..125R"><span>Europa, tidally heated oceans, and habitable <span class="hlt">zones</span> around giant planets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Reynolds, R. T.; McKay, C. P.; Kasting, J. F.</p> <p></p> <p>Tidal dissipation in the satellites of a giant planet may provide sufficient heating to maintain an environment favorable to life on the satellite surface or just below a thin <span class="hlt">ice</span> layer. Europa could have a liquid ocean which may occasionally receive sunlight through cracks in the overlying <span class="hlt">ice</span> shell. In such a case, sufficient solar energy could reach liquid water that organisms similar to those found under Antarctic <span class="hlt">ice</span> could grow. In other solar systems, larger satellites with more significant heat flow could represent environments that are stable over an order of eons and in which life could perhaps evolve. A <span class="hlt">zone</span> around a giant planet is defined in which such satellites could exist as a tidally-heated habitable <span class="hlt">zone</span>. This <span class="hlt">zone</span> can be compared to the habitable <span class="hlt">zone</span> which results from heating due to the radiation of a central star. In this solar system, this radiatively-heated habitable <span class="hlt">zone</span> contains the earth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19880032690&hterms=habitable+planet&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DA%2Bhabitable%2Bplanet','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19880032690&hterms=habitable+planet&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DA%2Bhabitable%2Bplanet"><span>Europa, tidally heated oceans, and habitable <span class="hlt">zones</span> around giant planets</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Reynolds, Ray T.; Mckay, Christopher P.; Kasting, James F.</p> <p>1987-01-01</p> <p>Tidal dissipation in the satellites of a giant planet may provide sufficient heating to maintain an environment favorable to life on the satellite surface or just below a thin <span class="hlt">ice</span> layer. Europa could have a liquid ocean which may occasionally receive sunlight through cracks in the overlying <span class="hlt">ice</span> shell. In such a case, sufficient solar energy could reach liquid water that organisms similar to those found under Antarctic <span class="hlt">ice</span> could grow. In other solar systems, larger satellites with more significant heat flow could represent environments that are stable over an order of eons and in which life could perhaps evolve. A <span class="hlt">zone</span> around a giant planet is defined in which such satellites could exist as a tidally-heated habitable <span class="hlt">zone</span>. This <span class="hlt">zone</span> can be compared to the habitable <span class="hlt">zone</span> which results from heating due to the radiation of a central star. In this solar system, this radiatively-heated habitable <span class="hlt">zone</span> contains the earth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11538217','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11538217"><span>Europa, tidally heated oceans, and habitable <span class="hlt">zones</span> around giant planets.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Reynolds, R T; McKay, C P; Kasting, J F</p> <p>1987-01-01</p> <p>Tidal dissipation in the satellites of a giant planet may provide sufficient heating to maintain an environment favorable to life on the satellite surface or just below a thin <span class="hlt">ice</span> layer. In our own solar system, Europa, one of the Galilean satellites of Jupiter, could have a liquid ocean which may occasionally receive sunlight through cracks in the overlying <span class="hlt">ice</span> shell. In such case, sufficient solar energy could reach liquid water that organisms similar to those found under Antarctic <span class="hlt">ice</span> could grow. In other solar systems, larger satellites with more significant heat flow could represent environments that are stable over an order of Aeons and in which life could perhaps evolve. We define a <span class="hlt">zone</span> around a giant planet in which such satellites could exist as a tidally-heated habitable <span class="hlt">zone</span>. This <span class="hlt">zone</span> can be compared to the habitable <span class="hlt">zone</span> which results from heating due to the radiation of a central star. In our solar system, this radiatively-heated habitable <span class="hlt">zone</span> contains the Earth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950038689&hterms=glacier+melt&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dglacier%2Bmelt','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950038689&hterms=glacier+melt&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dglacier%2Bmelt"><span>Radar measurements of melt <span class="hlt">zones</span> 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>Jezek, Kenneth C.; Gogineni, Prasad; Shanableh, M.</p> <p>1994-01-01</p> <p>Surface-based microwave radar measurements were performed at a location on the western flank of the Greenland <span class="hlt">Ice</span> Sheet. Here, firn metamorphasis is dominated by seasonal melt, which leads to marked contrasts in the vertical structure of winter and summer firn. This snow regime is also one of the brightest radar targets on Earth with an average backscatter coefficient of 0 dB at 5.3 GHz and an incidence angle of 25 deg. By combining detailed observations of firn physical properties with ranging radar measurements we find that the glaciological mechanism associated with this strong electromagnetic response is summer <span class="hlt">ice</span> lens formation within the previous winter's snow pack. This observation has important implications for monitoring and understanding changes in <span class="hlt">ice</span> sheet volume using spaceborne microwave sensors.</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 marginal <span class="hlt">ice</span> <span class="hlt">zone</span>. 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/2016APS..DFDE16002B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..DFDE16002B"><span>Dueling Mechanisms for Dry <span class="hlt">Zones</span> around Frozen Droplets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bisbano, Caitlin; Nath, Saurabh; Boreyko, Jonathan</p> <p>2016-11-01</p> <p><span class="hlt">Ice</span> acts as a local humidity sink, due to its depressed saturation pressure relative to that of supercooled water. Hygroscopic chemicals typically exhibit annular dry <span class="hlt">zones</span> of inhibited condensation; however, dry <span class="hlt">zones</span> do not tend to form around <span class="hlt">ice</span> because of inter-droplet frost growth to nearby liquid droplets that have already condensed on the chilled surface. Here, we use a humidity chamber with an embedded Peltier stage to initially suppress the growth of condensation on a chilled surface containing a single frozen droplet, in order to characterize the dry <span class="hlt">zone</span> around <span class="hlt">ice</span> for the first time. The length of the dry <span class="hlt">zone</span> was observed to vary by at least two orders of magnitude as a function of surface temperature, ambient humidity, and the size of the frozen droplet. The surface temperature and ambient humidity govern the magnitudes of the in-plane and out-of-plane gradients in vapor pressure, while the size of the frozen droplet effects the local thickness of the concentration boundary layer. We develop an analytical model that reveals two different types of dry <span class="hlt">zones</span> are possible: one in which nucleation is inhibited and one where the net growth of condensate is inhibited. Finally, a phase map was developed to predict the parameter space in which nucleation dry <span class="hlt">zones</span> versus flux dry <span class="hlt">zones</span> are dominant.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45.4899W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45.4899W"><span>Topographic Steering of Enhanced <span class="hlt">Ice</span> Flow at the Bottleneck Between East and 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>Winter, Kate; Ross, Neil; Ferraccioli, Fausto; Jordan, Tom A.; Corr, Hugh F. J.; Forsberg, René; Matsuoka, Kenichi; Olesen, Arne V.; Casal, Tania G.</p> <p>2018-05-01</p> <p>Hypothesized drawdown of the East Antarctic <span class="hlt">Ice</span> Sheet through the "bottleneck" <span class="hlt">zone</span> between East and West Antarctica would have significant impacts for a large proportion of the Antarctic <span class="hlt">Ice</span> Sheet. Earth observation satellite orbits and a sparseness of radio echo sounding data have restricted investigations of basal boundary controls on <span class="hlt">ice</span> flow in this region until now. New airborne radio echo sounding surveys reveal complex topography of high relief beneath the southernmost Weddell/Ross <span class="hlt">ice</span> divide, with three subglacial troughs connecting interior Antarctica to the Foundation and Patuxent <span class="hlt">Ice</span> Streams and Siple Coast <span class="hlt">ice</span> streams. These troughs route enhanced <span class="hlt">ice</span> flow through the interior of Antarctica but limit potential drawdown of the East Antarctic <span class="hlt">Ice</span> Sheet through the bottleneck <span class="hlt">zone</span>. In a thinning or retreating scenario, these topographically controlled corridors of enhanced flow could however drive <span class="hlt">ice</span> divide migration and increase mass discharge from interior West Antarctica to the Southern Ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018FrEaS...6...28W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018FrEaS...6...28W"><span>Unravelling InSAR observed Antarctic <span class="hlt">ice</span>-shelf flexure using 2-D elastic and viscoelastic modelling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wild, Christian T.; Marsh, Oliver J.; Rack, Wolfgang</p> <p>2018-04-01</p> <p><span class="hlt">Ice</span>-shelf grounding <span class="hlt">zones</span> link the Antarctic <span class="hlt">ice</span>-sheets to the ocean. Differential interferometric synthetic aperture radar (DInSAR) is commonly used to monitor grounding-line locations, but also contains information on grounding-<span class="hlt">zone</span> <span class="hlt">ice</span> thickness, <span class="hlt">ice</span> properties and tidal conditions beneath the <span class="hlt">ice</span> shelf. Here, we combine in-situ data with numerical modelling of <span class="hlt">ice</span>-shelf flexure to investigate 2-D controls on the tidal bending pattern on the Southern McMurdo <span class="hlt">Ice</span> Shelf. We validate our results with 9 double-differential TerraSAR-X interferograms. It is necessary to make adjustments to the tidal forcing to directly compare observations with model output and we find that when these adjustments are small (< 1.5 cm) a viscoelastic model matches better, while an elastic model is more robust overall. Within landward embayments, where lateral stresses from surrounding protrusions damp the flexural response, a 2-D model captures behaviour that is missed in simple 1-D models. We conclude that improvements in current tide models are required to allow for the full exploitation of DInSAR in grounding-<span class="hlt">zone</span> glaciology.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1208660-changes-firn-structure-western-greenland-ice-sheet-caused-recent-warming','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1208660-changes-firn-structure-western-greenland-ice-sheet-caused-recent-warming"><span>Changes in the firn structure of the western Greenland <span class="hlt">Ice</span> Sheet caused by recent warming</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>de la Peña, S.; Howat, I. M.; Nienow, P. W.; ...</p> <p>2015-06-11</p> <p>Atmospheric warming over the Greenland <span class="hlt">Ice</span> Sheet during the last 2 decades has increased the amount of surface meltwater production, resulting in the migration of melt and percolation regimes to higher altitudes and an increase in the amount of <span class="hlt">ice</span> content from refrozen meltwater found in the firn above the superimposed <span class="hlt">ice</span> <span class="hlt">zone</span>. Here we present field and airborne radar observations of buried <span class="hlt">ice</span> layers within the near-surface (0–20 m) firn in western Greenland, obtained from campaigns between 1998 and 2014. We find a sharp increase in firn-<span class="hlt">ice</span> content in the form of thick widespread layers in the percolation <span class="hlt">zone</span>,more » which decreases the capacity of the firn to store meltwater. The estimated total annual <span class="hlt">ice</span> content retained in the near-surface firn in areas with positive surface mass balance west of the <span class="hlt">ice</span> divide in Greenland reached a maximum of 74 ± 25 Gt in 2012, when compared to the 1958–1999 average of 13 ± 2 Gt, while the percolation <span class="hlt">zone</span> area more than doubled between 2003 and 2012. Increased melt and column densification resulted in surface lowering averaging -0.80 ± 0.39 m yr -1 between 1800 and 2800 m in the accumulation <span class="hlt">zone</span> of western Greenland. Since 2007, modeled annual melt and refreezing rates in the percolation <span class="hlt">zone</span> at elevations below 2100 m surpass the annual snowfall from the previous year, implying that mass gain in the region is retained after melt in the form of refrozen meltwater. Furthermore, if current melt trends over high elevation regions continue, subsequent changes in firn structure will have implications for the hydrology of the <span class="hlt">ice</span> sheet and related abrupt seasonal densification could become increasingly significant for altimetry-derived <span class="hlt">ice</span> sheet mass balance estimates.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016DPS....4830209L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016DPS....4830209L"><span>The Effect of Carbon Dioxide (CO 2) <span class="hlt">Ice</span> Cloud Condensation on the Habitable <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lincowski, Andrew; Meadows, Victoria; Robinson, Tyler D.; Crisp, David</p> <p>2016-10-01</p> <p>The currently accepted outer limit of the habitable <span class="hlt">zone</span> (OHZ) is defined by the "maximum greenhouse" limit, where Rayleigh scattering from additional CO2 gas overwhelms greenhouse warming. However, this long-standing definition neglects the radiative effects of CO2 clouds (Kopparapu, 2013); this omission was justified based on studies using the two-stream approximation, which found CO2 clouds to be highly likely to produce a net warming. However, recent comparisons of the radiative effect of CO2 clouds using both a two-stream and multi-stream radiative transfer model (Kitzmann et al, 2013; Kitzmann, 2016) found that the warming effect was reduced when the more sophisticated multi-stream models were used. In many cases CO2 clouds caused a cooling effect, meaning that their impact on climate could not be neglected when calculating the outer edge of the habitable <span class="hlt">zone</span>. To better understand the impact of CO2 <span class="hlt">ice</span> clouds on the OHZ, we have integrated CO2 cloud condensation into a versatile 1-D climate model for terrestrial planets (Robinson et al, 2012) that uses the validated multi-stream SMART radiative transfer code (Meadows & Crisp, 1996; Crisp, 1997) with a simple microphysical model. We present preliminary results on the habitable <span class="hlt">zone</span> with self-consistent CO2 clouds for a range of atmospheric masses, compositions and host star spectra, and the subsequent effect on surface temperature. In particular, we evaluate the habitable <span class="hlt">zone</span> for TRAPPIST-1d (Gillon et al, 2016) with a variety of atmospheric compositions and masses. We present reflectance and transit spectra of these cold terrestrial planets. We identify any consequences for the OHZ in general and TRAPPIST-1d in particular. This more comprehensive treatment of the OHZ could impact our understanding of the distribution of habitable planets in the universe, and provide better constraints for statistical target selection techniques, such as the habitability index (Barnes et al, 2015), for missions like JWST</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 marginal <span class="hlt">ice</span> <span class="hlt">zone</span>. 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/2015EGUGA..1715613W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1715613W"><span>The impacts of intense moisture transport on the deep and marginal sea-<span class="hlt">ice</span> <span class="hlt">zones</span> 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 marginal <span class="hlt">ice-zones</span> 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://www.dtic.mil/docs/citations/ADA602481','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA602481"><span>Marginal <span class="hlt">Ice</span> <span class="hlt">Zone</span>: 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://hdl.handle.net/2060/19930094532','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930094532"><span>Meteorological-physical Limitations of <span class="hlt">Icing</span> in the Atmosphere</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Findeisen, W</p> <p>1939-01-01</p> <p>The <span class="hlt">icing</span> hazard can, in most cases, be avoided by correct execution of the flights according to meteorological viewpoints and by meteorologically correct navigation (horizontal and, above all, vertical). The <span class="hlt">zones</span> of <span class="hlt">icing</span> hazard are usually narrowly confined. Their location can be ascertained with, in most cases, sufficient accuracy before take-off.</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 marginal <span class="hlt">ice</span> <span class="hlt">zone</span>, 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/2017TCry...11.2491T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017TCry...11.2491T"><span>Dark <span class="hlt">ice</span> dynamics of the south-west 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>Tedstone, Andrew J.; Bamber, Jonathan L.; Cook, Joseph M.; Williamson, Christopher J.; Fettweis, Xavier; Hodson, Andrew J.; Tranter, Martyn</p> <p>2017-11-01</p> <p>Runoff from the Greenland <span class="hlt">Ice</span> Sheet (GrIS) has increased in recent years due largely to changes in atmospheric circulation and atmospheric warming. Albedo reductions resulting from these changes have amplified surface melting. Some of the largest declines in GrIS albedo have occurred in the ablation <span class="hlt">zone</span> of the south-west sector and are associated with the development of dark <span class="hlt">ice</span> surfaces. Field observations at local scales reveal that a variety of light-absorbing impurities (LAIs) can be present on the surface, ranging from inorganic particulates to cryoconite materials and <span class="hlt">ice</span> algae. Meanwhile, satellite observations show that the areal extent of dark <span class="hlt">ice</span> has varied significantly between recent successive melt seasons. However, the processes that drive such large interannual variability in dark <span class="hlt">ice</span> extent remain essentially unconstrained. At present we are therefore unable to project how the albedo of bare <span class="hlt">ice</span> sectors of the GrIS will evolve in the future, causing uncertainty in the projected sea level contribution from the GrIS over the coming decades. Here we use MODIS satellite imagery to examine dark <span class="hlt">ice</span> dynamics on the south-west GrIS each year from 2000 to 2016. We quantify dark <span class="hlt">ice</span> in terms of its annual extent, duration, intensity and timing of first appearance. Not only does dark <span class="hlt">ice</span> extent vary significantly between years but so too does its duration (from 0 to > 80 % of June-July-August, JJA), intensity and the timing of its first appearance. Comparison of dark <span class="hlt">ice</span> dynamics with potential meteorological drivers from the regional climate model MAR reveals that the JJA sensible heat flux, the number of positive minimum-air-temperature days and the timing of bare <span class="hlt">ice</span> appearance are significant interannual synoptic controls. We use these findings to identify the surface processes which are most likely to explain recent dark <span class="hlt">ice</span> dynamics. We suggest that whilst the spatial distribution of dark <span class="hlt">ice</span> is best explained by outcropping of particulates from</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19890009374&hterms=bank+canada&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dbank%2Bcanada','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19890009374&hterms=bank+canada&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dbank%2Bcanada"><span>SAR imagery of the Grand Banks (Newfoundland) pack <span class="hlt">ice</span> pack and its relationship to surface features</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Argus, S. D.; Carsey, F. D.</p> <p>1988-01-01</p> <p>Synthetic Aperture Radar (SAR) data and aerial photographs were obtained over pack <span class="hlt">ice</span> off the East Coast of Canada in March 1987 as part of the Labrador <span class="hlt">Ice</span> Margin Experiment (LIMEX) pilot project. Examination of this data shows that although the pack <span class="hlt">ice</span> off the Canadian East Coast appears essentially homogeneous to visible light imagery, two clearly defined <span class="hlt">zones</span> of <span class="hlt">ice</span> are apparent on C-band SAR imagery. To identify factors that create the <span class="hlt">zones</span> seen on the radar image, aerial photographs were compared to the SAR imagery. Floe size data from the aerial photographs was compared to digital number values taken from SAR imagery of the same <span class="hlt">ice</span>. The SAR data of the inner <span class="hlt">zone</span> acquired three days apart over the melt period was also examined. The studies indicate that the radar response is governed by floe size and meltwater distribution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1911309W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1911309W"><span>Submarine melt rates under Greenland's <span class="hlt">ice</span> tongues</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wilson, Nat; Straneo, Fiametta; Heimbach, Patrick; Cenedese, Claudia</p> <p>2017-04-01</p> <p>The few remaining <span class="hlt">ice</span> tongues (<span class="hlt">ice</span>-shelf like extensions) of Greenland's glaciers are undergoing rapid changes with potential implications for the stability of the <span class="hlt">ice</span> sheet. Submarine melting is recognized as a major contributor to mass loss, yet the magnitude and spatial distribution of melt are poorly known or understood. Here, we use high resolution satellite imagery to infer the magnitude and spatial variability of melt rates under Greenland's largest remaining <span class="hlt">ice</span> tongues: Ryder Glacier, Petermann Glacier and Nioghalvfjerdsbræ (79 North Glacier). We find that submarine plus aerial melt approximately balance the <span class="hlt">ice</span> flux from the grounded <span class="hlt">ice</span> sheet for the first two while at Nioghalvfjerdsbræ the total melt flux exceeds the inflow of <span class="hlt">ice</span> indicating thinning of the <span class="hlt">ice</span> tongue. We also show that melt rates under the <span class="hlt">ice</span> tongues vary considerably, exceeding 60 m yr-1 near the grounding <span class="hlt">zone</span> and decaying rapidly downstream. Channels, likely originating from upstream subglacial channels, give rise to large melt variations across the <span class="hlt">ice</span> tongues. Using derived melt rates, we test simplified melt parameterizations appropriate for <span class="hlt">ice</span> sheet models and find the best agreement with those that incorporate <span class="hlt">ice</span> tongue geometry in the form of depth and slope.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014NatGe...7..762K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014NatGe...7..762K"><span>Evidence for subduction in the <span class="hlt">ice</span> shell of Europa</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kattenhorn, Simon A.; Prockter, Louise M.</p> <p>2014-10-01</p> <p>Jupiter’s icy moon Europa has one of the youngest planetary surfaces in the Solar System, implying rapid recycling by some mechanism. Despite ubiquitous extension and creation of new surface area at dilational bands that resemble terrestrial mid-ocean spreading <span class="hlt">zones</span>, there is little evidence of large-scale contraction to balance the observed extension or to recycle ageing terrains. We address this enigma by presenting several lines of evidence that subduction may be recycling surface material into the interior of Europa’s <span class="hlt">ice</span> shell. Using Galileo spacecraft images, we produce a tectonic reconstruction of geologic features across a 134,000 km2 region of Europa and find, in addition to dilational band spreading, evidence for transform motions along prominent strike-slip faults, as well as the removal of approximately 20,000 km2 of the surface along a discrete tabular <span class="hlt">zone</span>. We interpret this <span class="hlt">zone</span> as a subduction-like convergent boundary that abruptly truncates older geological features and is flanked by potential cryolavas on the overriding <span class="hlt">ice</span>. We propose that Europa’s <span class="hlt">ice</span> shell has a brittle, mobile, plate-like system above convecting warmer <span class="hlt">ice</span>. Hence, Europa may be the only Solar System body other than Earth to exhibit a system of plate tectonics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23705008','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23705008"><span>Change and variability in East antarctic sea <span class="hlt">ice</span> seasonality, 1979/80-2009/10.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Massom, Robert; Reid, Philip; Stammerjohn, Sharon; Raymond, Ben; Fraser, Alexander; Ushio, Shuki</p> <p>2013-01-01</p> <p>Recent analyses have shown that significant changes have occurred in patterns of sea <span class="hlt">ice</span> seasonality in West Antarctica since 1979, with wide-ranging climatic, biological and biogeochemical consequences. Here, we provide the first detailed report on long-term change and variability in annual timings of sea <span class="hlt">ice</span> advance, retreat and resultant <span class="hlt">ice</span> season duration in East Antarctica. These were calculated from satellite-derived <span class="hlt">ice</span> concentration data for the period 1979/80 to 2009/10. The pattern of change in sea <span class="hlt">ice</span> seasonality off East Antarctica comprises mixed signals on regional to local scales, with pockets of strongly positive and negative trends occurring in near juxtaposition in certain regions e.g., Prydz Bay. This pattern strongly reflects change and variability in different elements of the marine "icescape", including fast <span class="hlt">ice</span>, polynyas and the marginal <span class="hlt">ice</span> <span class="hlt">zone</span>. A trend towards shorter sea-<span class="hlt">ice</span> duration (of 1 to 3 days per annum) occurs in fairly isolated pockets in the outer pack from∼95-110°E, and in various near-coastal areas that include an area of particularly strong and persistent change near Australia's Davis Station and between the Amery and West <span class="hlt">Ice</span> Shelves. These areas are largely associated with coastal polynyas that are important as sites of enhanced sea <span class="hlt">ice</span> production/melt. Areas of positive trend in <span class="hlt">ice</span> season duration are more extensive, and include an extensive <span class="hlt">zone</span> from 160-170°E (i.e., the western Ross Sea sector) and the near-coastal <span class="hlt">zone</span> between 40-100°E. The East Antarctic pattern is considerably more complex than the well-documented trends in West Antarctica e.g., in the Antarctic Peninsula-Bellingshausen Sea and western Ross Sea sectors.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_11 --> <div id="page_12" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="221"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C42A..02G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C42A..02G"><span>Channelized melting drives thinning under Dotson <span class="hlt">ice</span> shelf, Western 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>Gourmelen, N.; Goldberg, D.; Snow, K.; Henley, S. F.; Bingham, R. G.; Kimura, S.; Hogg, A.; Shepherd, A.; Mouginot, J.; Lenaerts, J.; Ligtenberg, S.; Van De Berg, W. J.</p> <p>2017-12-01</p> <p>The majority of meteoric <span class="hlt">ice</span> that forms in West Antarctica leaves the <span class="hlt">ice</span> sheet through floating <span class="hlt">ice</span> shelves, many of which have been thinning substantially over the last 25 years. A significant proportion of <span class="hlt">ice</span>-shelf thinning has been driven by submarine melting facilitated by increased access of relatively warm (>0.6oC) modified Circumpolar Deep Water to sub-shelf cavities. <span class="hlt">Ice</span> shelves play a significant role in stabilising the <span class="hlt">ice</span> sheet from runaway retreat and regulating its contribution to sea level change. <span class="hlt">Ice</span>-shelf melting has also been implicated in sustaining high primary productivity in Antarctica's coastal seas. However, these processes vary regionally and are not fully understood. Under some <span class="hlt">ice</span> shelves, concentrated melting leads to the formation of inverted channels. These channels guide buoyant melt-laden outflow, which can lead to localised melting of the sea <span class="hlt">ice</span> cover. The channels may also potentially lead to heightened crevassing, which in turn affects <span class="hlt">ice</span>-shelf stability. Meanwhile, numerical studies suggest that buttressing loss is sensitive to the location of <span class="hlt">ice</span> removal within an <span class="hlt">ice</span>-shelf. Thus it is important that we observe spatial patterns, as well as magnitudes, of <span class="hlt">ice</span>-shelf thinning, in order to improve understanding of the ocean drivers of thinning and of their impacts on <span class="hlt">ice</span>-shelf stability. Here we show from high-resolution altimetry measurements acquired between 2010 to 2016 that Dotson <span class="hlt">Ice</span> Shelf, West Antarctica, thins in response to basal melting focussed along a single 5 km-wide and 60 km-long channel extending from the <span class="hlt">ice</span> shelf's grounding <span class="hlt">zone</span> to its calving front. The coupled effect of geostrophic circulation and <span class="hlt">ice</span>-shelf topography leads to the observed concentration of basal melting. Analysis of previous datasets suggests that this process has been ongoing for at least the last 25 years. If focused thinning continues at present rates, the channel would melt through within 40-50 years, almost two centuries before it is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19790069568&hterms=limnology&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dlimnology','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19790069568&hterms=limnology&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dlimnology"><span>Remote sensing of snow and <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>Rango, A.</p> <p>1979-01-01</p> <p>This paper reviews remote sensing of snow and <span class="hlt">ice</span>, techniques for improved monitoring, and incorporation of the new data into forecasting and management systems. The snowcover interpretation of visible and infrared data from satellites, automated digital methods, radiative transfer modeling to calculate the solar reflectance of snow, and models using snowcover input data and elevation <span class="hlt">zones</span> for calculating snowmelt are discussed. The use of visible and near infrared techniques for inferring snow properties, microwave monitoring of snowpack characteristics, use of Landsat images for collecting glacier data, monitoring of river <span class="hlt">ice</span> with visible imagery from NOAA satellites, use of sequential imagery for tracking <span class="hlt">ice</span> flow movement, and microwave studies of sea <span class="hlt">ice</span> are described. Applications of snow and <span class="hlt">ice</span> research to commercial use are examined, and it is concluded that a major problem to be solved is characterization of snow and <span class="hlt">ice</span> in nature, since assigning of the correct properties to a real system to be modeled has been difficult.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19980017810','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19980017810"><span>Measuring Geophysical Parameters of the Greenland <span class="hlt">Ice</span> Sheet using Airborne Radar Altimetry</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ferraro, Ellen J.; Swift. Calvin T.</p> <p>1995-01-01</p> <p>This paper presents radar-altimeter scattering models for each of the diagenetic <span class="hlt">zones</span> of the Greenland <span class="hlt">ice</span> sheet. AAFE radar- altimeter waveforms obtained during the 1991 and 1993 NASA multi-sensor airborne altimetry experiments over Greenland reveal that the Ku-band return pulse changes significantly with the different diagenetic <span class="hlt">zones</span>. These changes are due to varying amounts of surface and volume scattering in the return waveform. In the ablation and soaked <span class="hlt">zones</span>, where surface scattering dominates the AAFE return, geophysical parameters such as rms surface height and rms surface slope are obtained by fitting the waveforms to a surface-scattering model. Waveforms from the percolation <span class="hlt">zone</span> show that the sub-surface <span class="hlt">ice</span> features have a much more significant effect on the return pulse than the surrounding snowpack. Model percolation waveforms, created using a combined surface- and volume-scattering model and an <span class="hlt">ice</span>-feature distribution obtained during the 1993 field season, agree well with actual AAFE waveforms taken in the same time period. Using a combined surface- and volume-scattering model for the dry-snow-<span class="hlt">zone</span> return waveforms, the rms surface height and slope and the attenuation coefficient of the snowpack are obtained. These scattering models not only allow geophysical parameters of the <span class="hlt">ice</span> sheet to be measured but also help in the understanding of satellite radar-altimeter data.</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 marginal <span class="hlt">ice</span> <span class="hlt">zone</span>, 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('http://adsabs.harvard.edu/abs/2017AGUFMMR41D0438M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMMR41D0438M"><span>Microfabric and Structures in Glacial <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>Monz, M.; Hudleston, P. J.</p> <p>2017-12-01</p> <p>Similar to rocks in active orogens, glacial <span class="hlt">ice</span> develops both structures and fabrics that reflect deformation. Crystallographic preferred orientation (CPO), associated with mechanical anisotropy, develops as <span class="hlt">ice</span> deforms, and as in rock, directly reflects the conditions and mechanisms of deformation and influences the overall strength. This project aims to better constrain the rheologic properties of natural <span class="hlt">ice</span> through microstructural analysis and to establish the relationship of microfabric to macroscale structures. The focus is on enigmatic fabric patterns found in coarse grained, "warm" (T > -10oC) <span class="hlt">ice</span> deep in <span class="hlt">ice</span> sheets and in valley glaciers. Deformation mechanisms that produce such patterns are poorly understood. Detailed mapping of surface structures, including bedding, foliation, and blue bands (bubble-free veins of <span class="hlt">ice</span>), was done in the ablation <span class="hlt">zone</span> of Storglaciären, a polythermal valley glacier in northern Sweden. Microstructural studies on samples from a transect across the ablation <span class="hlt">zone</span> were carried out in a cold room. Crystal size was too large for use of electron backscattered diffraction to determine CPO, therefore a Rigsby universal stage, designed specifically for <span class="hlt">ice</span>, was used. In thick and thin sections, recrystallized grains are locally variable in both size (1mm-7cm in one thin section) and shape and clearly reflect recrystallization involving highly mobile grain boundaries. Larger crystals are often branching, and appear multiple times throughout one thin section. There is a clear shape preferred orientation that is generally parallel with foliation defined by bubble alignment and concentration. Locally, there appears to be an inverse correlation between bubble concentration and smoothness of grain boundaries. Fabric in samples that have undergone prolonged shear display roughly symmetrical multimaxima patterns centered around the pole to foliation. The angular distances between maxima suggest a possible twin relationship that may have</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA601203','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA601203"><span>Forecasting Future Sea <span class="hlt">Ice</span> Conditions in the MIZ: A Lagrangian Approach</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>www.mcgill.ca/meteo/people/tremblay LONG-TERM GOALS 1- Determine the source regions for sea <span class="hlt">ice</span> in the seasonally <span class="hlt">ice</span>-covered <span class="hlt">zones</span> (SIZs...distribution of sea <span class="hlt">ice</span> cover and transport pathways. 2- Improve our understanding of the strengths and/or limitations of GCM predictions of future...ocean currents, RGPS sea <span class="hlt">ice</span> deformation, Reanalysis surface wind , surface radiative fluxes, etc. Processing the large datasets involved is a tedious</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19990064620','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19990064620"><span>Parametric Experimental Study of the Formation of Glaze <span class="hlt">Ice</span> Shapes on Swept Wings</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Vargas, Mario; Reshotko, Eli</p> <p>1999-01-01</p> <p>An experiment was conducted to study the effect of velocity and sweep angle on the critical distance in <span class="hlt">ice</span> accretion formation on swept wings at glaze <span class="hlt">ice</span> conditions. The critical distance is defined as the distance from the attachment line to the beginning of the <span class="hlt">zone</span> where roughness elements develop into glaze <span class="hlt">ice</span> feathers. <span class="hlt">Icing</span> runs were performed on a NACA 00 1 2 swept wing tip at velocities of 75, 100, 150, and 200 miles per hour. At each velocity and tunnel condition, the sweep angle was changed from 0 deg to 45 deg at 5 deg increments. Casting data, <span class="hlt">ice</span> shape tracings, and close-up photographic data were obtained. The results showed that at given velocity and tunnel conditions, as the sweep angle is increased from 0 deg to 25 deg the critical distance slowly decreases. As the sweep angle is increased past 25 deg, the critical distance starts decreasing more rapidly. For 75 and 100 mph it reaches a value of 0 millimeters at 35 deg. For 150 and 200 mph it reaches a value of 0 millimeters at 40 deg. On the <span class="hlt">ice</span> accretion, as the sweep angle is increased from 0 deg to 25 deg, the extent of the attachment line <span class="hlt">zone</span> slowly decreases. In the glaze <span class="hlt">ice</span> feathers <span class="hlt">zone</span>, the angle that the preferred direction of growth of the feathers makes with respect to the attachment line direction increases. But overall, the <span class="hlt">ice</span> accretions remain similar to the 0 deg sweep angle case. As the sweep angle is increased above 25 deg, the extent of the attachment line <span class="hlt">zone</span> decreases rapidly and complete scallops form at 35 deg sweep angle for 75 and 100 mph, and at 40 deg for 150 and 200 mph.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/211927-transport-contaminants-arctic-sea-ice-surface-ocean-currents','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/211927-transport-contaminants-arctic-sea-ice-surface-ocean-currents"><span>Transport of contaminants by Arctic sea <span class="hlt">ice</span> and surface ocean currents</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>Pfirman, S.</p> <p>1995-12-31</p> <p>Sea <span class="hlt">ice</span> 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 <span class="hlt">ice</span> during suspension freezing on the shelves, and by atmospheric deposition during drift. <span class="hlt">Ice</span> releases its contaminant load through brinemore » drainage, surface runoff of snow and meltwater, and when the floe disintegrates. The marginal <span class="hlt">ice</span> <span class="hlt">zone</span>, a region of intense biological activity, may also be the site of major contaminant release. Potentially contaminated <span class="hlt">ice</span> from the Kara Sea is likely to influence the marginal <span class="hlt">ice</span> <span class="hlt">zones</span> of the Barents and Greenland seas. From studies conducted to date it appears that sea <span class="hlt">ice</span> from the Kara Sea does not typically enter the Beaufort Gyre, and thus is unlikely to affect the northern Canadian and Alaskan margins.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26932187','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26932187"><span>Colonization of maritime glacier <span class="hlt">ice</span> by bdelloid Rotifera.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Shain, Daniel H; Halldórsdóttir, Katrín; Pálsson, Finnur; Aðalgeirsdóttir, Guðfinna; Gunnarsson, Andri; Jónsson, Þorsteinn; Lang, Shirley A; Pálsson, Hlynur Skagfjörð; Steinþórssson, Sveinbjörn; Arnason, Einar</p> <p>2016-05-01</p> <p>Very few animal taxa are known to reside permanently in glacier <span class="hlt">ice</span>/snow. Here we report the widespread colonization of Icelandic glaciers and <span class="hlt">ice</span> fields by species of bdelloid Rotifera. Specimens were collected within the accumulation <span class="hlt">zones</span> of Langjökull and Vatnajökull <span class="hlt">ice</span> caps, among the largest European <span class="hlt">ice</span> masses. Rotifers reached densities up to ∼100 individuals per liter-equivalent of glacier <span class="hlt">ice</span>/snow, and were freeze-tolerant. Phylogenetic analyses indicate that glacier rotifers are polyphyletic, with independent ancestries occurring within the Pleistocene. Collectively, these data identify a previously undescribed environmental niche for bdelloid rotifers and suggest their presence in comparable habitats worldwide. Copyright © 2016 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060026203&hterms=sauber&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsauber','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060026203&hterms=sauber&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsauber"><span><span class="hlt">Ice</span> Mass Fluctuations and Earthquake Hazard</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sauber, J.</p> <p>2006-01-01</p> <p>In south central Alaska, tectonic strain rates are high in a region that includes large glaciers undergoing <span class="hlt">ice</span> wastage over the last 100-150 years [Sauber et al., 2000; Sauber and Molnia, 2004]. In this study we focus on the region referred to as the Yakataga segment of the Pacific-North American plate boundary <span class="hlt">zone</span> in Alaska. In this region, the Bering and Malaspina glacier ablation <span class="hlt">zones</span> have average <span class="hlt">ice</span> elevation decreases from 1-3 meters/year (see summary and references in Molnia, 2005). The elastic response of the solid Earth to this <span class="hlt">ice</span> mass decrease alone would cause several mm/yr of horizontal motion and uplift rates of up to 10-12 mm/yr. In this same region observed horizontal rates of tectonic deformation range from 10 to 40 mm/yr to the north-northwest and the predicted tectonic uplift rates range from -2 mm/year near the Gulf of Alaska coast to 12mm/year further inland [Savage and Lisowski, 1988; Ma et al, 1990; Sauber et al., 1997, 2000, 2004; Elliot et al., 2005]. The large <span class="hlt">ice</span> mass changes associated with glacial wastage and surges perturb the tectonic rate of deformation at a variety of temporal and spatial scales. The associated incremental stress change may enhance or inhibit earthquake occurrence. We report recent (seasonal to decadal) <span class="hlt">ice</span> elevation changes derived from data from NASA's ICESat satellite laser altimeter combined with earlier DEM's as a reference surface to illustrate the characteristics of short-term <span class="hlt">ice</span> elevation changes [Sauber et al., 2005, Muskett et al., 2005]. Since we are interested in evaluating the effect of <span class="hlt">ice</span> changes on faulting potential, we calculated the predicted surface displacement changes and incremental stresses over a specified time interval and calculated the change in the fault stability margin using the approach given by Wu and Hasegawa [1996]. Additionally, we explored the possibility that these <span class="hlt">ice</span> mass fluctuations altered the seismic rate of background seismicity. Although we primarily focus on</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017NatCC...7...58L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017NatCC...7...58L"><span>Meltwater produced by wind-albedo interaction stored in an East Antarctic <span class="hlt">ice</span> shelf</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lenaerts, J. T. M.; Lhermitte, S.; Drews, R.; Ligtenberg, S. R. M.; Berger, S.; Helm, V.; Smeets, C. J. P. P.; Broeke, M. R. Van Den; van de Berg, W. J.; van Meijgaard, E.; Eijkelboom, M.; Eisen, O.; Pattyn, F.</p> <p>2017-01-01</p> <p>Surface melt and subsequent firn air depletion can ultimately lead to disintegration of Antarctic <span class="hlt">ice</span> shelves causing grounded glaciers to accelerate and sea level to rise. In the Antarctic Peninsula, foehn winds enhance melting near the grounding line, which in the recent past has led to the disintegration of the most northerly <span class="hlt">ice</span> shelves. Here, we provide observational and model evidence that this process also occurs over an East Antarctic <span class="hlt">ice</span> shelf, where meltwater-induced firn air depletion is found in the grounding <span class="hlt">zone</span>. Unlike the Antarctic Peninsula, where foehn events originate from episodic interaction of the circumpolar westerlies with the topography, in coastal East Antarctica high temperatures are caused by persistent katabatic winds originating from the <span class="hlt">ice</span> sheet’s interior. Katabatic winds warm and mix the air as it flows downward and cause widespread snow erosion, explaining >3 K higher near-surface temperatures in summer and surface melt doubling in the grounding <span class="hlt">zone</span> compared with its surroundings. Additionally, these winds expose blue <span class="hlt">ice</span> and firn with lower surface albedo, further enhancing melt. The in situ observation of supraglacial flow and englacial storage of meltwater suggests that <span class="hlt">ice</span>-shelf grounding <span class="hlt">zones</span> in East Antarctica, like their Antarctic Peninsula counterparts, are vulnerable to hydrofracturing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011PhDT.......110D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011PhDT.......110D"><span>Alaska shorefast <span class="hlt">ice</span>: Interfacing geophysics with local sea <span class="hlt">ice</span> knowledge and use</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Druckenmiller, Matthew L.</p> <p></p> <p>This thesis interfaces geophysical techniques with local and traditional knowledge (LTK) of indigenous <span class="hlt">ice</span> experts to track and evaluate coastal sea <span class="hlt">ice</span> conditions over annual and inter-annual timescales. A novel approach is presented for consulting LTK alongside a systematic study of where, when, and how the community of Barrow, Alaska uses the <span class="hlt">ice</span> cover. The goal of this research is to improve our understanding of and abilities to monitor the processes that govern the state and dynamics of shorefast sea <span class="hlt">ice</span> in the Chukchi Sea and use of <span class="hlt">ice</span> by the community. Shorefast <span class="hlt">ice</span> stability and community strategies for safe hunting provide a framework for data collection and knowledge sharing that reveals how nuanced observations by Inupiat <span class="hlt">ice</span> experts relate to identifying hazards. In particular, shorefast <span class="hlt">ice</span> break-out events represent a significant threat to the lives of hunters. Fault tree analysis (FTA) is used to combine local and time-specific observations of <span class="hlt">ice</span> conditions by both geophysical instruments and local experts, and to evaluate how <span class="hlt">ice</span> features, atmospheric and oceanic forces, and local to regional processes interact to cause break-out events. Each year, the Barrow community builds trails across shorefast <span class="hlt">ice</span> for use during the spring whaling season. In collaboration with hunters, a systematic multi-year survey (2007--2011) was performed to map these trails and measure <span class="hlt">ice</span> thickness along them. Relationships between <span class="hlt">ice</span> conditions and hunter strategies that guide trail placement and risk assessment are explored. In addition, trail surveys provide a meaningful and consistent approach to monitoring the thickness distribution of shorefast <span class="hlt">ice</span>, while establishing a baseline for assessing future environmental change and potential impacts to the community. Coastal communities in the region have proven highly adaptive in their ability to safely and successfully hunt from sea <span class="hlt">ice</span> over the last 30 years as significant changes have been observed in the <span class="hlt">ice</span> <span class="hlt">zone</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007PhDT........29K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007PhDT........29K"><span>Arctic landfast 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>Konig, Christof S.</p> <p></p> <p>Landfast <span class="hlt">ice</span> is sea <span class="hlt">ice</span> which forms and remains fixed along a coast, where it is attached either to the shore, or held between shoals or grounded icebergs. Landfast <span class="hlt">ice</span> fundamentally modifies the momentum exchange between atmosphere and ocean, as compared to pack <span class="hlt">ice</span>. It thus affects the heat and freshwater exchange between air and ocean and impacts on the location of ocean upwelling and downwelling <span class="hlt">zones</span>. Further, the landfast <span class="hlt">ice</span> edge is essential for numerous Arctic mammals and Inupiat who depend on them for their subsistence. The current generation of sea <span class="hlt">ice</span> models is not capable of reproducing certain aspects of landfast <span class="hlt">ice</span> formation, maintenance, and disintegration even when the spatial resolution would be sufficient to resolve such features. In my work I develop a new <span class="hlt">ice</span> model that permits the existence of landfast sea <span class="hlt">ice</span> even in the presence of offshore winds, as is observed in mature. Based on viscous-plastic as well as elastic-viscous-plastic <span class="hlt">ice</span> dynamics I add tensile strength to the <span class="hlt">ice</span> rheology and re-derive the equations as well as numerical methods to solve them. Through numerical experiments on simplified domains, the effects of those changes are demonstrated. It is found that the modifications enable landfast <span class="hlt">ice</span> modeling, as desired. The elastic-viscous-plastic rheology leads to initial velocity fluctuations within the landfast <span class="hlt">ice</span> that weaken the <span class="hlt">ice</span> sheet and break it up much faster than theoretically predicted. Solving the viscous-plastic rheology using an implicit numerical method avoids those waves and comes much closer to theoretical predictions. Improvements in landfast <span class="hlt">ice</span> modeling can only verified in comparison to observed data. I have extracted landfast sea <span class="hlt">ice</span> data of several decades from several sources to create a landfast sea <span class="hlt">ice</span> climatology that can be used for that purpose. Statistical analysis of the data shows several factors that significantly influence landfast <span class="hlt">ice</span> distribution: distance from the coastline, ocean depth, as</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 marginal <span class="hlt">ice</span> <span class="hlt">zone</span> 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://ntrs.nasa.gov/search.jsp?R=19880034852&hterms=behavior+modification&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dbehavior%2Bmodification','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19880034852&hterms=behavior+modification&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dbehavior%2Bmodification"><span>Investigation of surface water behavior during glaze <span class="hlt">ice</span> accretion</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hansman, R. John, Jr.; Turnock, Stephen R.</p> <p>1988-01-01</p> <p>Microvideo observations of glaze <span class="hlt">ice</span> accretions on 1-in-diameter cylinders in a closed-loop refrigerated wind tunnel were obtained to study factors controlling the behavior of unfrozen surface water during glaze <span class="hlt">ice</span> accretion. Three <span class="hlt">zones</span> of surface water behavior were noted, each with a characteristic roughness. The effect of substrate thermal and roughness properties on <span class="hlt">ice</span> accretions was also studied. The contact angle and hysteresis were found to increase sharply at temperatures just below 0 C, explaining the high resistance to motion of water beads observed on accreting glaze <span class="hlt">ice</span> surfaces. Based on the results, a simple multizone modification to the current glaze <span class="hlt">ice</span> accretion model is proposed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140009626','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140009626"><span><span class="hlt">Ice</span>-Shelf Tidal Flexure and Subglacial Pressure Variations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Walker, Ryan T.; Parizek, Byron R.; Alley, Richard B.; Anandakrishnan, Sridhar; Riverman, Kiya L.; Christianson, Knut</p> <p>2013-01-01</p> <p>We develop a model of an <span class="hlt">ice</span> shelf-<span class="hlt">ice</span> stream system as a viscoelastic beam partially supported by an elastic foundation. When bed rock near the grounding line acts as a fulcrum, leverage from the <span class="hlt">ice</span> shelf dropping at low tide can cause significant (approx 1 cm) uplift in the first few kilometers of grounded <span class="hlt">ice</span>.This uplift and the corresponding depression at high tide lead to basal pressure variations of sufficient magnitude to influence subglacial hydrology.Tidal flexure may thus affect basal lubrication, sediment flow, and till strength, all of which are significant factors in <span class="hlt">ice</span>-stream dynamics and grounding-line stability. Under certain circumstances, our results suggest the possibility of seawater being drawn into the subglacial water system. The presence of sea water beneath grounded <span class="hlt">ice</span> would significantly change the radar reflectivity of the grounding <span class="hlt">zone</span> and complicate the interpretation of grounded versus floating <span class="hlt">ice</span> based on <span class="hlt">ice</span>-penetrating radar observations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010TCD.....4.1307M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010TCD.....4.1307M"><span>The Potsdam Parallel <span class="hlt">Ice</span> Sheet Model (PISM-PIK) - Part 2: Dynamic equilibrium simulation of the 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>Martin, M. A.; Winkelmann, R.; Haseloff, M.; Albrecht, T.; Bueler, E.; Khroulev, C.; Levermann, A.</p> <p>2010-08-01</p> <p>We present a dynamic equilibrium simulation of the <span class="hlt">ice</span> sheet-shelf system on Antarctica with the Potsdam Parallel <span class="hlt">Ice</span> Sheet Model (PISM-PIK). The simulation is initialized with present-day conditions for topography and <span class="hlt">ice</span> thickness and then run to steady state with constant present-day surface mass balance. Surface temperature and basal melt distribution are parameterized. Grounding lines and calving fronts are free to evolve, and their modeled equilibrium state is compared to observational data. A physically-motivated dynamic calving law based on horizontal spreading rates allows for realistic calving fronts for various types of shelves. Steady-state dynamics including surface velocity and <span class="hlt">ice</span> flux are analyzed for whole Antarctica and the Ronne-Filchner and Ross <span class="hlt">ice</span> shelf areas in particular. The results show that the different flow regimes in sheet and shelves, and the transition <span class="hlt">zone</span> between them, are captured reasonably well, supporting the approach of superposition of SIA and SSA for the representation of fast motion of grounded <span class="hlt">ice</span>. This approach also leads to a natural emergence of streams in this new 3-D marine <span class="hlt">ice</span> sheet model.</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 marginal <span class="hlt">ice</span> <span class="hlt">zone</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017TCry...11.2711H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017TCry...11.2711H"><span>Wave-induced stress and breaking of sea <span class="hlt">ice</span> in a coupled hydrodynamic discrete-element wave-<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>Herman, Agnieszka</p> <p>2017-11-01</p> <p>In this paper, a coupled sea <span class="hlt">ice</span>-wave model is developed and used to analyze wave-induced stress and breaking in sea <span class="hlt">ice</span> for a range of wave and <span class="hlt">ice</span> conditions. The sea <span class="hlt">ice</span> module is a discrete-element bonded-particle model, in which <span class="hlt">ice</span> is represented as cuboid <q>grains</q> floating on the water surface that can be connected to their neighbors by elastic joints. The joints may break if instantaneous stresses acting on them exceed their strength. The wave module is based on an open-source version of the Non-Hydrostatic WAVE model (NHWAVE). The two modules are coupled with proper boundary conditions for pressure and velocity, exchanged at every wave model time step. In the present version, the model operates in two dimensions (one vertical and one horizontal) and is suitable for simulating compact <span class="hlt">ice</span> in which heave and pitch motion dominates over surge. In a series of simulations with varying sea <span class="hlt">ice</span> properties and incoming wavelength it is shown that wave-induced stress reaches maximum values at a certain distance from the <span class="hlt">ice</span> edge. The value of maximum stress depends on both <span class="hlt">ice</span> properties and characteristics of incoming waves, but, crucially for <span class="hlt">ice</span> breaking, the location at which the maximum occurs does not change with the incoming wavelength. Consequently, both regular and random (Jonswap spectrum) waves break the <span class="hlt">ice</span> into floes with almost identical sizes. The width of the <span class="hlt">zone</span> of broken <span class="hlt">ice</span> depends on <span class="hlt">ice</span> strength and wave attenuation rates in the <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930022707&hterms=unicorn&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dunicorn','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930022707&hterms=unicorn&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dunicorn"><span>The role of the margins in <span class="hlt">ice</span> stream dynamics</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Echelmeyer, Keith; Harrison, William</p> <p>1993-01-01</p> <p>At first glance, it would appear that the bed of the active <span class="hlt">ice</span> 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 <span class="hlt">ice</span> stream is large (15:1 to 50:1). On the other hand, recent observations indicate that at least part of the <span class="hlt">ice</span> 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 <span class="hlt">ice</span> stream, across the chaotic shear margin, and onto the Unicorn, which is part of the slow-moving <span class="hlt">ice</span> 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 <span class="hlt">ice</span> must exhibit an increasing enhancement factor as the margins are approached (E equals 10 in the chaotic <span class="hlt">zone</span>), in keeping with laboratory measurements on <span class="hlt">ice</span> under prolonged shear strain. Also, there is either a narrow <span class="hlt">zone</span> of somewhat stiffer <span class="hlt">ice</span> (E</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_12 --> <div id="page_13" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="241"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1993wais.work...33E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1993wais.work...33E"><span>The role of the margins in <span class="hlt">ice</span> stream dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Echelmeyer, Keith; Harrison, William</p> <p>1993-07-01</p> <p>At first glance, it would appear that the bed of the active <span class="hlt">ice</span> 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 <span class="hlt">ice</span> stream is large (15:1 to 50:1). On the other hand, recent observations indicate that at least part of the <span class="hlt">ice</span> 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 <span class="hlt">ice</span> stream, across the chaotic shear margin, and onto the Unicorn, which is part of the slow-moving <span class="hlt">ice</span> 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 <span class="hlt">ice</span> must exhibit an increasing enhancement factor as the margins are approached (E equals 10 in the chaotic <span class="hlt">zone</span>), in keeping with laboratory measurements on <span class="hlt">ice</span> under prolonged shear strain. Also, there is either a narrow <span class="hlt">zone</span> of somewhat stiffer <span class="hlt">ice</span> (E</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 marginal <span class="hlt">ice</span> <span class="hlt">zone</span> 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://hdl.handle.net/2060/19820003852','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19820003852"><span>Evaluation of photogrammetric flight under <span class="hlt">icing</span> conditions on March 23, 1978</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fuchs, W.; Kaluza, J.</p> <p>1981-01-01</p> <p>In a double passage through a route laid out in a stagnation <span class="hlt">zone</span> of the Bavarian forest, it was found that the stagnation and attendant elevation increases the danger of <span class="hlt">icing</span>. Conversely, it turned out that formation of precipitation reduces the <span class="hlt">icing</span> intensity. A comparison of both factors showed: the reduction of <span class="hlt">ice</span> formation through precipitation equals the increase due to stagnation, or even exceeds it.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3660359','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3660359"><span>Change and Variability in East Antarctic Sea <span class="hlt">Ice</span> Seasonality, 1979/80–2009/10</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Massom, Robert; Reid, Philip; Stammerjohn, Sharon; Raymond, Ben; Fraser, Alexander; Ushio, Shuki</p> <p>2013-01-01</p> <p>Recent analyses have shown that significant changes have occurred in patterns of sea <span class="hlt">ice</span> seasonality in West Antarctica since 1979, with wide-ranging climatic, biological and biogeochemical consequences. Here, we provide the first detailed report on long-term change and variability in annual timings of sea <span class="hlt">ice</span> advance, retreat and resultant <span class="hlt">ice</span> season duration in East Antarctica. These were calculated from satellite-derived <span class="hlt">ice</span> concentration data for the period 1979/80 to 2009/10. The pattern of change in sea <span class="hlt">ice</span> seasonality off East Antarctica comprises mixed signals on regional to local scales, with pockets of strongly positive and negative trends occurring in near juxtaposition in certain regions e.g., Prydz Bay. This pattern strongly reflects change and variability in different elements of the marine “icescape”, including fast <span class="hlt">ice</span>, polynyas and the marginal <span class="hlt">ice</span> <span class="hlt">zone</span>. A trend towards shorter sea-<span class="hlt">ice</span> duration (of 1 to 3 days per annum) occurs in fairly isolated pockets in the outer pack from∼95–110°E, and in various near-coastal areas that include an area of particularly strong and persistent change near Australia's Davis Station and between the Amery and West <span class="hlt">Ice</span> Shelves. These areas are largely associated with coastal polynyas that are important as sites of enhanced sea <span class="hlt">ice</span> production/melt. Areas of positive trend in <span class="hlt">ice</span> season duration are more extensive, and include an extensive <span class="hlt">zone</span> from 160–170°E (i.e., the western Ross Sea sector) and the near-coastal <span class="hlt">zone</span> between 40–100°E. The East Antarctic pattern is considerably more complex than the well-documented trends in West Antarctica e.g., in the Antarctic Peninsula-Bellingshausen Sea and western Ross Sea sectors. PMID:23705008</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013LaPhy..23g5605B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013LaPhy..23g5605B"><span><span class="hlt">Ice</span> matrix in reconfigurable microfluidic systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bossi, A. M.; Vareijka, M.; Piletska, E. V.; Turner, A. P. F.; Meglinski, I.; Piletsky, S. A.</p> <p>2013-07-01</p> <p>Microfluidic devices find many applications in biotechnologies. Here, we introduce a flexible and biocompatible microfluidic <span class="hlt">ice</span>-based platform with tunable parameters and configuration of microfluidic patterns that can be changed multiple times during experiments. Freezing and melting of cavities, channels and complex relief structures created and maintained in the bulk of <span class="hlt">ice</span> by continuous scanning of an infrared laser beam are used as a valve action in microfluidic systems. We demonstrate that pre-concentration of samples and transport of ions and dyes through the open channels created can be achieved in <span class="hlt">ice</span> microfluidic patterns by IR laser-assisted <span class="hlt">zone</span> melting. The proposed approach can be useful for performing separation and sensing processes in flexible reconfigurable microfluidic devices.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017TCry...11.1553S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017TCry...11.1553S"><span>Sea-<span class="hlt">ice</span> deformation in a coupled ocean-sea-<span class="hlt">ice</span> model and in satellite remote sensing data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Spreen, Gunnar; Kwok, Ron; Menemenlis, Dimitris; Nguyen, An T.</p> <p>2017-07-01</p> <p>A realistic representation of sea-<span class="hlt">ice</span> deformation in models is important for accurate simulation of the sea-<span class="hlt">ice</span> mass balance. Simulated sea-<span class="hlt">ice</span> deformation from numerical simulations with 4.5, 9, and 18 km horizontal grid spacing and a viscous-plastic (VP) sea-<span class="hlt">ice</span> rheology are compared with synthetic aperture radar (SAR) satellite observations (RGPS, RADARSAT Geophysical Processor System) for the time period 1996-2008. All three simulations can reproduce the large-scale <span class="hlt">ice</span> deformation patterns, but small-scale sea-<span class="hlt">ice</span> deformations and linear kinematic features (LKFs) are not adequately reproduced. The mean sea-<span class="hlt">ice</span> total deformation rate is about 40 % lower in all model solutions than in the satellite observations, especially in the seasonal sea-<span class="hlt">ice</span> <span class="hlt">zone</span>. A decrease in model grid spacing, however, produces a higher density and more localized <span class="hlt">ice</span> deformation features. The 4.5 km simulation produces some linear kinematic features, but not with the right frequency. The dependence on length scale and probability density functions (PDFs) of absolute divergence and shear for all three model solutions show a power-law scaling behavior similar to RGPS observations, contrary to what was found in some previous studies. Overall, the 4.5 km simulation produces the most realistic divergence, vorticity, and shear when compared with RGPS data. This study provides an evaluation of high and coarse-resolution viscous-plastic sea-<span class="hlt">ice</span> simulations based on spatial distribution, time series, and power-law scaling metrics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70013376','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70013376"><span>SIMPLE MODEL OF <span class="hlt">ICE</span> SEGREGATION USING AN ANALYTIC FUNCTION TO MODEL HEAT AND SOIL-WATER FLOW.</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hromadka, T.V.; Guymon, G.L.</p> <p>1984-01-01</p> <p>This paper reports on the development of a simple two-dimensional model of coupled heat and soil-water flow in freezing or thawing soil. The model also estimates <span class="hlt">ice</span>-segregation (frost-heave) evolution. <span class="hlt">Ice</span> segregation in soil results from water drawn into a freezing <span class="hlt">zone</span> by hydraulic gradients created by the freezing of soil-water. Thus, with a favorable balance between the rate of heat extraction and the rate of water transport to a freezing <span class="hlt">zone</span>, segregated <span class="hlt">ice</span> lenses may form.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018QSRv..179...87E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018QSRv..179...87E"><span><span class="hlt">Ice</span> streams of the Late Wisconsin Cordilleran <span class="hlt">Ice</span> Sheet in western North America</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Eyles, Nick; Arbelaez Moreno, Lina; Sookhan, Shane</p> <p>2018-01-01</p> <p>The Late Wisconsin Cordilleran <span class="hlt">Ice</span> Sheet (CIS) of western North America is thought to have reached its maximum extent (∼2.5 × 106 km2) as late at c. 14.5 ka. Most (80%) of the <span class="hlt">ice</span> sheet's bed consists of high mountains but its 'core <span class="hlt">zone</span>' sited on plateaux of the Intermontane Belt of British Columbia and coterminous parts of the USA, shows broad swaths of subglacially-streamlined rock and sediment. Broad scale mapping from new digital imagery data identifies three subglacial bed types: 1) 'hard beds' of variably streamlined bedrock; 2) drumlinized 'soft beds' of deformation till reworked from antecedent sediment, and 3) 'mixed beds' of variably-streamlined bedrock protruding through drumlinized sediment. Drumlins on soft beds appear to be erosional features cut into till and antecedent sediments, and identify the catchment areas of paleo <span class="hlt">ice</span> streams expressed downglacier as flow sets of megascale glacial lineations (MSGLs). 'Grooved' and 'cloned' drumlins appear to record the transition from drumlins to MSGLs. The location of paleo <span class="hlt">ice</span> streams reflects topographic funneling of <span class="hlt">ice</span> from plateau surfaces through outlet valleys and a soft bed that sustained fast flow; rock-cut MSGLs are also present locally on the floors of outlet valleys. CIS disintegrated in <1000 years shortly after c. 13.0 ka releasing very large volumes of meltwater and sediment to the Pacific coast. Abrupt deglaciation may reflect unsustainable calving of marine-based <span class="hlt">ice</span> streams along the glacio-isostatically depressed coast; large deep 'fiord lakes' in the <span class="hlt">ice</span> sheet's interior may have played an analogous role. Mapping of the broad scale distribution of bed types across the Cordilleran <span class="hlt">Ice</span> Sheet provides key information for paleoglaciological modelling and also for understanding the beds of modern <span class="hlt">ice</span> masses such as the Greenland <span class="hlt">Ice</span> Sheet which is of a comparable topographic setting.</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 marginal 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 <span class="hlt">zone</span> of steep uplift gradient move relative to one another in a nearly reversible fashion as the lake fills and drains. Evidently, the <span class="hlt">zone</span> of steep uplift gradient is a fault <span class="hlt">zone</span>, 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://ntrs.nasa.gov/search.jsp?R=20080023352&hterms=sauber&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsauber','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20080023352&hterms=sauber&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsauber"><span>Rapid <span class="hlt">Ice</span> Mass Loss: Does It Have an Influence on Earthquake Occurrence in Southern Alaska?</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sauber, Jeanne M.</p> <p>2008-01-01</p> <p>The glaciers of southern Alaska are extensive, and many of them have undergone gigatons of <span class="hlt">ice</span> wastage on time scales on the order of the seismic cycle. Since the <span class="hlt">ice</span> loss occurs directly above a shallow main thrust <span class="hlt">zone</span> associated with subduction of the Pacific-Yakutat plate beneath continental Alaska, the region between the Malaspina and Bering Glaciers is an excellent test site for evaluating the importance of recent <span class="hlt">ice</span> wastage on earthquake faulting potential. We demonstrate the influence of cumulative glacial mass loss following the 1899 Yakataga earthquake (M=8.1) by using a two dimensional finite element model with a simple representation of <span class="hlt">ice</span> fluctuations to calculate the incremental stresses and change in the fault stability margin (FSM) along the main thrust <span class="hlt">zone</span> (MTZ) and on the surface. Along the MTZ, our results indicate a decrease in FSM between 1899 and the 1979 St. Elias earthquake (M=7.4) of 0.2 - 1.2 MPa over an 80 km region between the coast and the 1979 aftershock <span class="hlt">zone</span>; at the surface, the estimated FSM was larger but more localized to the lower reaches of glacial ablation <span class="hlt">zones</span>. The <span class="hlt">ice</span>-induced stresses were large enough, in theory, to promote the occurrence of shallow thrust earthquakes. To empirically test the influence of short-term <span class="hlt">ice</span> fluctuations on fault stability, we compared the seismic rate from a reference background time period (1988-1992) against other time periods (1993-2006) with variable <span class="hlt">ice</span> or tectonic change characteristics. We found that the frequency of small tectonic events in the Icy Bay region increased in 2002-2006 relative to the background seismic rate. We hypothesize that this was due to a significant increase in the rate of <span class="hlt">ice</span> wastage in 2002-2006 instead of the M=7.9, 2002 Denali earthquake, located more than 100km away.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C13D..08T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C13D..08T"><span>Grounding <span class="hlt">Zones</span>, Subglacial Lakes, and Dynamics of an Antarctic <span class="hlt">Ice</span> Stream: The WISSARD Glaciological Experiment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tulaczyk, S. M.; Schwartz, S. Y.; Fisher, A. T.; Powell, R. D.; Fricker, H. A.; Anandakrishnan, S.; Horgan, H. J.; Scherer, R. P.; Walter, J. I.; Siegfried, M. R.; Mikucki, J.; Christianson, K.; Beem, L.; Mankoff, K. D.; Carter, S. P.; Hodson, T. O.; Marsh, O.; Barcheck, C. G.; Branecky, C.; Neuhaus, S.; Jacobel, R. W.</p> <p>2015-12-01</p> <p>Interactions of West Antarctic <span class="hlt">ice</span> streams with meltwater at their beds, and with seawater at their grounding lines, are widely considered to be the primary drivers of <span class="hlt">ice</span> stream flow variability on different timescales. Understanding of processes controlling <span class="hlt">ice</span> flow variability is needed to build quantitative models of the Antarctic <span class="hlt">Ice</span> Sheet that can be used to help predict its future behavior and to reconstruct its past evolution. The <span class="hlt">ice</span> plain of Whillans <span class="hlt">Ice</span> Stream provides a natural glaciological laboratory for investigations of Antarctic <span class="hlt">ice</span> flow dynamics because of its highly variable flow rate modulated by tidal processes and fill-drain cycles of subglacial lakes. Moreover, this part of Antarctica has one of the longest time series of glaciological observations, which can be used to put recently acquired datasets in a multi-decadal context. Since 2007 Whillans <span class="hlt">Ice</span> Stream has been the focus of a regional glaciological experiment, which included surface GPS and passive-source seismic sensors, radar and seismic imaging of subglacial properties, as well as deep borehole geophysical sensors. This experiment was possible thanks to the NSF-funded multidisciplinary WISSARD project (Whillans <span class="hlt">Ice</span> Stream Subglacial Access Research Drilling). Here we will review the datasets collected during the WISSARD glaciological experiment and report on selected results pertaining to interactions of this <span class="hlt">ice</span> stream with water at its bed and its grounding line.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012IJCMS...150008G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012IJCMS...150008G"><span>Peculiarities of Vibration Characteristics of Amorphous <span class="hlt">Ices</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gets, Kirill V.; Subbotin, Oleg S.; Belosludov, Vladimir R.</p> <p>2012-03-01</p> <p>Dynamic properties of low (LDA), high (HDA) and very high (VHDA) density amorphous <span class="hlt">ices</span> were investigated within the approach based on Lattice Dynamics simulations. In this approach, we assume that the short-range molecular order mainly determines the dynamic and thermodynamic properties of amorphous <span class="hlt">ices</span>. Simulation cell of 512 water molecules with periodical boundary conditions and disordering allows us to study dynamical properties and dispersion curves in the Brillouin <span class="hlt">zone</span> of pseudo-crystal. Existence of collective phenomena in amorphous <span class="hlt">ices</span> which is usual for crystals but anomalous for disordered phase was confirmed in our simulations. Molecule amplitudes of delocalized (collective) as well as localized vibrations have been considered.</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 Marginal <span class="hlt">Ice</span> <span class="hlt">Zone</span> 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('https://www.osti.gov/biblio/1091494-minimalist-model-ice-microphysics-mixed-phase-stratiform-clouds','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1091494-minimalist-model-ice-microphysics-mixed-phase-stratiform-clouds"><span>Minimalist Model of <span class="hlt">Ice</span> Microphysics in Mixed-phase Stratiform Clouds</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Yang, F.; Ovchinnikov, Mikhail; Shaw, Raymond A.</p> <p></p> <p>The question of whether persistent <span class="hlt">ice</span> crystal precipitation from super cooled layer clouds can be explained by time-dependent, stochastic <span class="hlt">ice</span> nucleation is explored using an approximate, analytical model, and a large-eddy simulation (LES) cloud model. The updraft velocity in the cloud defines an accumulation <span class="hlt">zone</span>, where small <span class="hlt">ice</span> particles cannot fall out until they are large enough, which will increase the residence time of <span class="hlt">ice</span> particles in the cloud. <span class="hlt">Ice</span> particles reach a quasi-steady state between growth by vapor deposition and fall speed at cloud base. The analytical model predicts that <span class="hlt">ice</span> water content (wi) has a 2.5 power lawmore » relationship with <span class="hlt">ice</span> number concentration ni. wi and ni from a LES cloud model with stochastic <span class="hlt">ice</span> nucleation also confirm the 2.5 power law relationship. The prefactor of the power law is proportional to the <span class="hlt">ice</span> nucleation rate, and therefore provides a quantitative link to observations of <span class="hlt">ice</span> microphysical properties.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19850015283&hterms=permafrost&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dpermafrost','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19850015283&hterms=permafrost&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dpermafrost"><span>Permafrost and Subsurface <span class="hlt">Ice</span> in the Solar System</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Anderson, D. M.</p> <p>1985-01-01</p> <p>The properties and behavior of planetary permafrost are discussed with reference to the ability of such surfaces to sustain loads characteristics of spacecraft landing and planetary bases. In most occurrences, water <span class="hlt">ice</span> is in close proximity to, or in contact with, finely divided silicate mineral matter. When <span class="hlt">ice</span> contacts silicate mineral surfaces, a liquid-like, transition <span class="hlt">zone</span> is created. Its thickness ranges from several hundred Angstron units at temperatures near 0 degrees C to about three Angstrom units at -150 degrees C. When soluble substances are present, the resulting brine enlarges the interfacial <span class="hlt">zone</span>. When clays are involved, although the interfacial <span class="hlt">zone</span> may be small, its extent is large. The unfrozen, interfacial water may amount to 100% or more weight at a temperature of -5 degrees C. The presence of this interfacial unfrozen water acts to confer plasticity to permafrost, enabling it to exhibit creep at all imposed levels of stress. Nucleation processes and load-bearing capacity are examined.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011TCry....5..727M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011TCry....5..727M"><span>The Potsdam Parallel <span class="hlt">Ice</span> Sheet Model (PISM-PIK) - Part 2: Dynamic equilibrium simulation of the 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>Martin, M. A.; Winkelmann, R.; Haseloff, M.; Albrecht, T.; Bueler, E.; Khroulev, C.; Levermann, A.</p> <p>2011-09-01</p> <p>We present a dynamic equilibrium simulation of the <span class="hlt">ice</span> sheet-shelf system on Antarctica with the Potsdam Parallel <span class="hlt">Ice</span> Sheet Model (PISM-PIK). The simulation is initialized with present-day conditions for bed topography and <span class="hlt">ice</span> thickness and then run to steady state with constant present-day surface mass balance. Surface temperature and sub-shelf basal melt distribution are parameterized. Grounding lines and calving fronts are free to evolve, and their modeled equilibrium state is compared to observational data. A physically-motivated calving law based on horizontal spreading rates allows for realistic calving fronts for various types of shelves. Steady-state dynamics including surface velocity and <span class="hlt">ice</span> flux are analyzed for whole Antarctica and the Ronne-Filchner and Ross <span class="hlt">ice</span> shelf areas in particular. The results show that the different flow regimes in sheet and shelves, and the transition <span class="hlt">zone</span> between them, are captured reasonably well, supporting the approach of superposition of SIA and SSA for the representation of fast motion of grounded <span class="hlt">ice</span>. This approach also leads to a natural emergence of sliding-dominated flow in stream-like features in this new 3-D marine <span class="hlt">ice</span> sheet model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.3696L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.3696L"><span>How well does wind speed predict air-sea gas transfer in the sea <span class="hlt">ice</span> <span class="hlt">zone</span>? A synthesis of radon deficit profiles in the upper water column of the Arctic Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Loose, B.; Kelly, R. P.; Bigdeli, A.; Williams, W.; Krishfield, R.; Rutgers van der Loeff, M.; Moran, S. B.</p> <p>2017-05-01</p> <p>We present 34 profiles of radon-deficit from the <span class="hlt">ice</span>-ocean boundary layer of the Beaufort Sea. Including these 34, there are presently 58 published radon-deficit estimates of air-sea gas transfer velocity (k) in the Arctic Ocean; 52 of these estimates were derived from water covered by 10% sea <span class="hlt">ice</span> or more. The average value of k collected since 2011 is 4.0 ± 1.2 m d-1. This exceeds the quadratic wind speed prediction of weighted kws = 2.85 m d-1 with mean-weighted wind speed of 6.4 m s-1. We show how <span class="hlt">ice</span> cover changes the mixed-layer radon budget, and yields an "effective gas transfer velocity." We use these 58 estimates to statistically evaluate the suitability of a wind speed parameterization for k, when the ocean surface is <span class="hlt">ice</span> covered. Whereas the six profiles taken from the open ocean indicate a statistically good fit to wind speed parameterizations, the same parameterizations could not reproduce k from the sea <span class="hlt">ice</span> <span class="hlt">zone</span>. We conclude that techniques for estimating k in the open ocean cannot be similarly applied to determine k in the presence of sea <span class="hlt">ice</span>. The magnitude of k through gaps in the <span class="hlt">ice</span> may reach high values as <span class="hlt">ice</span> cover increases, possibly as a result of focused turbulence dissipation at openings in the free surface. These 58 profiles are presently the most complete set of estimates of k across seasons and variable <span class="hlt">ice</span> cover; as dissolved tracer budgets they reflect air-sea gas exchange with no impact from air-<span class="hlt">ice</span> gas exchange.</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> <span class="hlt">zone</span> 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 marginal 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/2017GeoRL..44.9796G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..44.9796G"><span>Channelized Melting Drives Thinning Under a Rapidly Melting Antarctic <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>Gourmelen, Noel; Goldberg, Dan N.; Snow, Kate; Henley, Sian F.; Bingham, Robert G.; Kimura, Satoshi; Hogg, Anna E.; Shepherd, Andrew; Mouginot, Jeremie; Lenaerts, Jan T. M.; Ligtenberg, Stefan R. M.; van de Berg, Willem Jan</p> <p>2017-10-01</p> <p><span class="hlt">Ice</span> shelves play a vital role in regulating loss of grounded <span class="hlt">ice</span> and in supplying freshwater to coastal seas. However, melt variability within <span class="hlt">ice</span> shelves is poorly constrained and may be instrumental in driving <span class="hlt">ice</span> shelf imbalance and collapse. High-resolution altimetry measurements from 2010 to 2016 show that Dotson <span class="hlt">Ice</span> Shelf (DIS), West Antarctica, thins in response to basal melting focused along a single 5 km-wide and 60 km-long channel extending from the <span class="hlt">ice</span> shelf's grounding <span class="hlt">zone</span> to its calving front. If focused thinning continues at present rates, the channel will melt through, and the <span class="hlt">ice</span> shelf collapse, within 40-50 years, almost two centuries before collapse is projected from the average thinning rate. Our findings provide evidence of basal melt-driven sub-<span class="hlt">ice</span> shelf channel formation and its potential for accelerating the weakening of <span class="hlt">ice</span> shelves.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12..761D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12..761D"><span>Compression experiments on artificial, alpine and marine <span class="hlt">ice</span>: implications for <span class="hlt">ice</span>-shelf/continental interactions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dierckx, Marie; Goossens, Thomas; Samyn, Denis; Tison, Jean-Louis</p> <p>2010-05-01</p> <p>Antarctic <span class="hlt">ice</span> shelves are important components of continental <span class="hlt">ice</span> dynamics, in that they control grounded <span class="hlt">ice</span> flow towards the ocean. As such, Antarctic <span class="hlt">ice</span> shelves are a key parameter to the stability of the Antarctic <span class="hlt">ice</span> sheet in the context of global change. Marine <span class="hlt">ice</span>, formed by sea water accretion beneath some <span class="hlt">ice</span> shelves, displays distinct physical (grain textures, bubble content, ...) and chemical (salinity, isotopic composition, ...) characteristics as compared to glacier <span class="hlt">ice</span> and sea <span class="hlt">ice</span>. The aim is to refine Glen's flow relation (generally used for <span class="hlt">ice</span> behaviour in deformation) under various parameters (temperature, salinity, debris, grain size ...) to improve deformation laws used in dynamic <span class="hlt">ice</span> shelf models, which would then give more accurate and / or realistic predictions on <span class="hlt">ice</span> shelf stability. To better understand the mechanical properties of natural <span class="hlt">ice</span>, deformation experiments were performed on <span class="hlt">ice</span> samples in laboratory, using a pneumatic compression device. To do so, we developed a custom built compression rig operated by pneumatic drives. It has been designed for performing uniaxial compression tests at constant load and under unconfined conditions. The operating pressure ranges from about 0.5 to 10 Bars. This allows modifying the experimental conditions to match the conditions found at the grounding <span class="hlt">zone</span> (in the 1 Bar range). To maintain the <span class="hlt">ice</span> at low temperature, the samples are immersed in a Silicone oil bath connected to an external refrigeration system. During the experiments, the vertical displacement of the piston and the applied force is measured by sensors which are connected to a digital acquisition system. We started our experiments with artificial <span class="hlt">ice</span> and went on with continental <span class="hlt">ice</span> samples from glaciers in the Alps. The first results allowed us to acquire realistic mechanical data for natural <span class="hlt">ice</span>. <span class="hlt">Ice</span> viscosity was calculated for different types of artificial <span class="hlt">ice</span>, using Glen's flow law, and showed the importance of impurities</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_13 --> <div id="page_14" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="261"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C41D0706A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C41D0706A"><span>Regional Patterns of Stress Transfer in the Ablation <span class="hlt">Zone</span> of the Western 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>Andrews, L. C.; Hoffman, M. J.; Neumann, T.; Catania, G. A.; Luethi, M. P.; Hawley, R. L.</p> <p>2016-12-01</p> <p>Current understanding of the subglacial system indicates that the seasonal evolution of <span class="hlt">ice</span> flow is strongly controlled by the gradual upstream progression of an inefficient - efficient transition within the subglacial hydrologic system followed by the reduction of melt and a downstream collapse of the efficient system. Using a spatiotemporally dense network of GPS-derived surface velocities from the Pâkitsoq Region of the western Greenland <span class="hlt">Ice</span> Sheet, we find that this pattern of subglacial development is complicated by heterogeneous bed topography, resulting in complex patterns of <span class="hlt">ice</span> flow. Following low elevation melt onset, early melt season strain rate anomalies are dominated by regional extension, which then gives way to spatially expansive compression. However, once daily minimum <span class="hlt">ice</span> velocities fall below the observed winter background velocities, an alternating spatial pattern of extension and compression prevails. This pattern of strain rate anomalies is correlated with changing basal topography and differences in the magnitude of diurnal surface <span class="hlt">ice</span> speeds. Along subglacial ridges, diurnal variability in <span class="hlt">ice</span> speed is large, suggestive of a mature, efficient subglacial system. In regions of subglacial lows, diurnal variability in <span class="hlt">ice</span> velocity is relatively low, likely associated with a less developed efficient subglacial system. The observed pattern suggests that borehole observations and modeling results demonstrating the importance of longitudinal stress transfer at a single field location are likely widely applicable in our study area and other regions of the Greenland <span class="hlt">Ice</span> Sheet with highly variable bed topography. Further, the complex pattern of <span class="hlt">ice</span> flow and evidence of spatially extensive longitudinal stress transfer add to the body of work indicating that the bed character plays an important role in the development of the subglacial system; closely matching diurnal <span class="hlt">ice</span> velocity patterns with subglacial models may be difficult without coupling these</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 margin 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 <span class="hlt">zones</span> (Oi1-Oi2, Mi1-Mi6). Benthic foraminiferal δ18O increases which are associated with the bases of <span class="hlt">Zones</span> 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 <span class="hlt">Zones</span> 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 <span class="hlt">Zone</span> Mi4 (circa 12.6 Ma) and Mi6 (circa 9</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA601787','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA601787"><span>Mass Balance of Multiyear Sea <span class="hlt">Ice</span> in the Southern Beaufort Sea</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>model of MY <span class="hlt">ice</span> circulation, which is shown in Figure 1. In this model , we consider the Beaufort Sea to consist of four <span class="hlt">zones</span> defined by mean drift...Arctic Regional Climate Model Simulation Project 3 International Arctic Buoy Program 4 Sea <span class="hlt">ice</span> Experiment - Dynamic Nature of the Arctic 5Cold...2 Table 2: Datasets compiled to date Geophysical data type Source Time period acquired Buoy tracks IABP 12 hrly position data 1978-2012 <span class="hlt">Ice</span></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 marginal 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-<span class="hlt">zone</span> processes, ocean-<span class="hlt">ice</span> interactions, and the numerical representation of all three.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C21E..06L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C21E..06L"><span>Atmospheric forcing of sea <span class="hlt">ice</span> leads in the Beaufort Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lewis, B. J.; Hutchings, J.; Mahoney, A. R.; Shapiro, L. H.</p> <p>2016-12-01</p> <p>Leads in sea <span class="hlt">ice</span> play an important role in the polar marine environment where they allow heat and moisture transfer between the oceans and atmosphere and act as travel pathways for both marine mammals and ships. Examining AVHRR thermal imagery of the Beaufort Sea, collected between 1994 and 2010, sea <span class="hlt">ice</span> leads appear in repeating patterns and locations (Eicken et al 2005). The leads, resolved by AVHRR, are at least 250m wide (Mahoney et al 2012), thus the patterns described are for lead systems that extend up to hundreds of kilometers across the Beaufort Sea. We describe how these patterns are associated with the location of weather systems relative to the coastline. Mean sea level pressure and 10m wind fields from ECMWF ERA-Interim reanalysis are used to identify if particular lead patterns can be uniquely forecast based on the location of weather systems. <span class="hlt">Ice</span> drift data from the NSIDC's Polar Pathfinder Daily 25km EASE-Grid Sea <span class="hlt">Ice</span> Motion Vectors indicates the role shear along leads has on the motion of <span class="hlt">ice</span> in the Beaufort Gyre. Lead formation is driven by 4 main factors: (i) coastal features such as promontories and islands influence the origin of leads by concentrating stresses within the <span class="hlt">ice</span> pack; (ii) direction of the wind forcing on the <span class="hlt">ice</span> pack determines the type of fracture, (iii) the location of the anticyclone (or cyclone) center determines the length of the fracture for certain patterns; and (iv) duration of weather conditions affects the width of the <span class="hlt">ice</span> fracture <span class="hlt">zones</span>. Movement of the <span class="hlt">ice</span> pack on the leeward side of leads originating at promontories and islands increases, creating shear <span class="hlt">zones</span> that control <span class="hlt">ice</span> transport along the Alaska coast in winter. . Understanding how atmospheric conditions influence the large-scale motion of the <span class="hlt">ice</span> pack is needed to design models that predict variability of the gyre and export of multi-year <span class="hlt">ice</span> to lower latitudes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Geomo.297...20K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Geomo.297...20K"><span>Degradation and stabilization of <span class="hlt">ice</span> wedges: Implications for assessing risk of thermokarst in northern Alaska</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kanevskiy, Mikhail; Shur, Yuri; Jorgenson, Torre; Brown, Dana R. N.; Moskalenko, Nataliya; Brown, Jerry; Walker, Donald A.; Raynolds, Martha K.; Buchhorn, Marcel</p> <p>2017-11-01</p> <p>Widespread degradation of <span class="hlt">ice</span> wedges has been observed during the last decades in numerous areas within the continuous permafrost <span class="hlt">zone</span> of Eurasia and North America. To study <span class="hlt">ice</span>-wedge degradation, we performed field investigations at Prudhoe Bay and Barrow in northern Alaska during 2011-2016. In each study area, a 250-m transect was established with plots representing different stages of <span class="hlt">ice</span>-wedge degradation/stabilization. Field work included surveying ground- and water-surface elevations, thaw-depth measurements, permafrost coring, vegetation sampling, and ground-based LiDAR scanning. We described cryostratigraphy of frozen soils and stable isotope composition, analyzed environmental characteristics associated with <span class="hlt">ice</span>-wedge degradation and stabilization, evaluated the vulnerability and resilience of <span class="hlt">ice</span> wedges to climate change and disturbances, and developed new conceptual models of <span class="hlt">ice</span>-wedge dynamics that identify the main factors affecting <span class="hlt">ice</span>-wedge degradation and stabilization and the main stages of this quasi-cyclic process. We found significant differences in the patterns of <span class="hlt">ice</span>-wedge degradation and stabilization between the two areas, and the patterns were more complex than those previously described because of the interactions of changing topography, water redistribution, and vegetation/soil responses that can interrupt or reinforce degradation. Degradation of <span class="hlt">ice</span> wedges is usually triggered by an increase in the active-layer thickness during exceptionally warm and wet summers or as a result of flooding or disturbance. Vulnerability of <span class="hlt">ice</span> wedges to thermokarst is controlled by the thickness of the intermediate layer of the upper permafrost, which overlies <span class="hlt">ice</span> wedges and protects them from thawing. In the continuous permafrost <span class="hlt">zone</span>, degradation of <span class="hlt">ice</span> wedges rarely leads to their complete melting; and in most cases wedges eventually stabilize and can then resume growing, indicating a somewhat cyclic and reversible process. Stabilization of <span class="hlt">ice</span> wedges</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>Active and passive microwave and physical properties of Arctic sea <span class="hlt">ice</span> in the marginal <span class="hlt">ice</span> <span class="hlt">zone</span> 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 actively between 5 and 10 GHz. Significant information about the state of melt of snow and <span class="hlt">ice</span> is contained in the active and passive microwave signatures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150018794','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150018794"><span>Convective Enhancement of <span class="hlt">Icing</span> Roughness Elements in Stagnation Region Flows</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hughes, Michael T.; McClain, Stephen T.; Vargas, Mario; Broeren, Andy</p> <p>2015-01-01</p> <p>To improve existing <span class="hlt">ice</span> accretion simulation codes, more data regarding <span class="hlt">ice</span> roughness and its effects on convective heat transfer are required. To build on existing research on this topic, this study used the Vertical <span class="hlt">Icing</span> Studies Tunnel (VIST) at NASA Glenn Research to model realistic <span class="hlt">ice</span> roughness in the stagnation region of a NACA 0012 airfoil. Using the VIST, a test plate representing the leading 2% chord of the airfoil was subjected to flows of 7.62 m/s (25 ft/s), 12.19 m/s (40 ft/s), and 16.76 m/s (55 ft/s). The test plate was fitted with 3 surfaces, each with a different representation of <span class="hlt">ice</span> roughness: 1) a control surface with no <span class="hlt">ice</span> roughness, 2) a surface with <span class="hlt">ice</span> roughness with element height scaled by 10x and streamwise rough <span class="hlt">zone</span> width from the stagnation point scaled by 10x, and 3) a surface with <span class="hlt">ice</span> roughness with element height scaled by 10x and streamwise rough <span class="hlt">zone</span> width from the stagnation point scaled by 25x. Temperature data from the tests were recorded using an infrared camera and thermocouples imbedded in the test plate. From the temperature data, a convective heat transfer coefficient map was created for each case. Additional testing was also performed to validate the VIST's flow quality. These tests included five-hole probe and hot-wire probe velocity traces to provide flow visualization and to study boundary layer formation on the various test surfaces. The knowledge gained during the experiments will help improve <span class="hlt">ice</span> accretion codes by providing heat transfer coefficient validation data and by providing flow visualization data helping understand current and future experiments performed in the VIST.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C13F1009C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C13F1009C"><span>Significance of Thermal Fluvial Incision and Bedrock Transfer due to <span class="hlt">Ice</span> Advection on Greenland <span class="hlt">Ice</span> Sheet Topography</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Crozier, J. A.; Karlstrom, L.; Yang, K.</p> <p>2017-12-01</p> <p><span class="hlt">Ice</span> sheet surface topography reflects a complicated combination of processes that act directly upon the surface and that are products of <span class="hlt">ice</span> advection. Using recently-available high resolution <span class="hlt">ice</span> velocity, imagery, <span class="hlt">ice</span> surface elevation, and bedrock elevation data sets, we seek to determine the domain of significance of two important processes - thermal fluvial incision and transfer of bedrock topography through the <span class="hlt">ice</span> sheet - on controlling surface topography in the ablation <span class="hlt">zone</span>. Evaluating such controls is important for understanding how melting of the GIS surface during the melt season may be directly imprinted in topography through supraglacial drainage networks, and indirectly imprinted through its contribution to basal sliding that affects bedrock transfer. We use methods developed by (Karlstrom and Yang, 2016) to identify supraglacial stream networks on the GIS, and use high resolution surface digital elevation models as well as gridded <span class="hlt">ice</span> velocity and melt rate models to quantify surface processes. We implement a numerically efficient Fourier domain bedrock transfer function (Gudmundsson, 2003) to predict surface topography due to <span class="hlt">ice</span> advection over bedrock topography obtained from radar. Despite a number of simplifying assumptions, the bedrock transfer function predicts the observed <span class="hlt">ice</span> sheet surface in most regions of the GIS with ˜90% accuracy, regardless of the presence or absence of supraglacial drainage networks. This supports the hypothesis that bedrock is the most significant driver of <span class="hlt">ice</span> surface topography on wavelengths similar to <span class="hlt">ice</span> thickness. <span class="hlt">Ice</span> surface topographic asymmetry on the GIS is common, with slopes in the direction of <span class="hlt">ice</span> flow steeper than those faced opposite to <span class="hlt">ice</span> flow, consistent with bedrock transfer theory. At smaller wavelengths, topography consistent with fluvial erosion by surface hydrologic features is evident. We quantify the effect of <span class="hlt">ice</span> advection versus fluvial thermal erosion on supraglacial longitudinal stream</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013GeoRL..40.3756Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013GeoRL..40.3756Y"><span>Minimalist model of <span class="hlt">ice</span> microphysics in mixed-phase stratiform clouds</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, Fan; Ovchinnikov, Mikhail; Shaw, Raymond A.</p> <p>2013-07-01</p> <p>The question of whether persistent <span class="hlt">ice</span> crystal precipitation from supercooled layer clouds can be explained by time-dependent, stochastic <span class="hlt">ice</span> nucleation is explored using an approximate, analytical model and a large-eddy simulation (LES) cloud model. The updraft velocity in the cloud defines an accumulation <span class="hlt">zone</span>, where small <span class="hlt">ice</span> particles cannot fall out until they are large enough, which will increase the residence time of <span class="hlt">ice</span> particles in the cloud. <span class="hlt">Ice</span> particles reach a quasi-steady state between growth by vapor deposition and fall speed at cloud base. The analytical model predicts that <span class="hlt">ice</span> water content (wi) has a 2.5 power-law relationship with <span class="hlt">ice</span> number concentration (ni). wi and ni from a LES cloud model with stochastic <span class="hlt">ice</span> nucleation confirm the 2.5 power-law relationship, and initial indications of the scaling law are observed in data from the Indirect and Semi-Direct Aerosol Campaign. The prefactor of the power law is proportional to the <span class="hlt">ice</span> nucleation rate and therefore provides a quantitative link to observations of <span class="hlt">ice</span> microphysical properties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16782611','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16782611"><span>Numerical modelling and data assimilation of the Larsen B <span class="hlt">ice</span> shelf, Antarctic Peninsula.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Vieli, Andreas; Payne, Antony J; Du, Zhijun; Shepherd, Andrew</p> <p>2006-07-15</p> <p>In this study, the flow and rheology of pre-collapse Larsen B <span class="hlt">ice</span> shelf are investigated by using a combination of flow modelling and data assimilation. Observed shelf velocities from satellite interferometry are used to constrain an <span class="hlt">ice</span> shelf model by using a data assimilation technique based on the control method. In particular, the <span class="hlt">ice</span> rheology field and the velocities at the inland shelf boundary are simultaneously optimized to get a modelled flow and stress field that is consistent with the observed flow. The application to the Larsen B <span class="hlt">ice</span> shelf shows that a strong weakening of the <span class="hlt">ice</span> in the shear <span class="hlt">zones</span>, mostly along the margins, is necessary to fit the observed shelf flow. This pattern of bands with weak <span class="hlt">ice</span> is a very robust feature of the inversion, whereas the <span class="hlt">ice</span> rheology within the main shelf body is found to be not well constrained. This suggests that these weak <span class="hlt">zones</span> play a major role in the control of the flow of the Larsen B <span class="hlt">ice</span> shelf and may be the key to understanding the observed pre-collapse thinning and acceleration of Larsen B. Regarding the sensitivity of the stress field to rheology, the consistency of the model with the observed flow seems crucial for any further analysis such as the application of fracture mechanics or perturbation model experiments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.7117S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.7117S"><span>Warm water and life beneath the grounding <span class="hlt">zone</span> of an Antarctic outlet glacier</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sugiyama, Shin; Sawagaki, Takanobu; Fukuda, Takehiro</p> <p>2013-04-01</p> <p><span class="hlt">Ice</span>-ocean interaction plays a key role in rapidly changing Antarctic <span class="hlt">ice</span> sheet margins. Recent studies demonstrated that warming ocean is eroding floating part of the <span class="hlt">ice</span> sheet, resulting in thinning, retreat and acceleration of <span class="hlt">ice</span> shelves and outlet glaciers. Field data are necessary to understand such processes, but direct observations at the interface of <span class="hlt">ice</span> and the ocean are lacking, particularly beneath the grounding <span class="hlt">zone</span>. To better understand the interaction of Antarctic <span class="hlt">ice</span> sheet and the ocean, we performed subglacial measurements through boreholes drilled in the grounding <span class="hlt">zone</span> of Langhovde Glacier, an outlet glacier in East Antarctica. Langhovde Glacier is located at 69°12'S, 39°48'E, approximately 20 km south of a Japanese research station Syowa. The glacier discharges <span class="hlt">ice</span> into Lützow-holm Bay through a 3-km-wide floating terminus at a rate of 130 m a-1. Fast flowing feature is confined by bedrock to the west and slow moving <span class="hlt">ice</span> to the east, and it extends about 10 km upglacier from the calving front. In 2011/12 austral summer season, we operated a hot water drilling system to drill through the glacier at 2.5 and 3 km from the terminus. Inspections of the boreholes revealed the <span class="hlt">ice</span> was underlain by a shallow saline water layer. <span class="hlt">Ice</span> and water column thicknesses were found to be 398 and 24 m at the first site, and 431 and 10 m at the second site. Judging from <span class="hlt">ice</span> surface and bed elevations, the drilling sites were situated at within a several hundred meters from the grounding line. Sensors were lowered into the boreholes to measure temperature, salinity and current within the subglacial water layer. Salinity and temperature from the two sites were fairly uniform (34.25±0.05 PSU and -1.45±0.05°C), indicating vertical and horizontal mixing in the layer. The measured temperature was >0.7°C warmer than the in-situ freezing point, and very similar to the values measured in the open ocean near the glacier front. Subglacial current was up to 3 cm/s, which</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('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 active gas flares—across a previously glaciated Arctic margin with <span class="hlt">ice</span>-sheet thermomechanical and gas hydrate stability <span class="hlt">zone</span> 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 <span class="hlt">zone</span>. 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('http://hdl.handle.net/2060/20050160462','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050160462"><span>Grounding <span class="hlt">Zone</span> and Tidal Response of the Amery <span class="hlt">Ice</span> Shelf, East Antarctica</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fricker, Helen A.; Sandwell, David; Coleman, Richard; Minster, Bernard</p> <p>2005-01-01</p> <p>This report summarizes the main findings of the research project. Unfortunately, it turned out that there was not a great deal of SAR data over the Amery <span class="hlt">Ice</span> Shelf that we were able to work with on the project; nevertheless, we did make considerable progress on this project, with both the existing SAR data and new field measurements that were collected under this grant. In total we had constructed two SAR interferograms (SSIs), and four SSIs. The latter were combined them to construct two differential SAR interferograms (DSIs;). DSIs are useful because the contribution to the SAR phase from horizontal <span class="hlt">ice</span> motion is eliminated, since the time difference between the first and second pass within both image pairs used to make the DSI is the same for each pair. The SSIs and DSIs have revealed several interesting glaciological features, and have added to our knowledge of the Amery <span class="hlt">Ice</span> Shelf (AIS).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/237955-structure-internal-stresses-uncompacted-ice-cover','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/237955-structure-internal-stresses-uncompacted-ice-cover"><span>The structure of internal stresses in the uncompacted <span class="hlt">ice</span> cover</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>Sukhorukov, K.K.</p> <p>1995-12-31</p> <p>Interactions between engineering structures and sea <span class="hlt">ice</span> cover are associated with an inhomogeneous space/time field of internal stresses. Field measurements (e.g., Coon, 1989; Tucker, 1992) have revealed considerable local stresses depending on the regional stress field and <span class="hlt">ice</span> structure. These stresses appear in different time and space scales and depend on rheologic properties of the <span class="hlt">ice</span>. To estimate properly the stressed state a knowledge of a connection between internal stress components in various regions of the <span class="hlt">ice</span> cover is necessary. To develop reliable algorithms for estimates of <span class="hlt">ice</span> action on engineering structures new experimental data are required to take intomore » account both microscale (comparable with local <span class="hlt">ice</span> inhomogeneities) and small-scale (kilometers) inhomogeneities of the <span class="hlt">ice</span> cover. Studies of compacted <span class="hlt">ice</span> (concentration N is nearly 1) are mostly important. This paper deals with the small-scale spatial distribution of internal stresses in the interaction <span class="hlt">zone</span> between the <span class="hlt">ice</span> covers of various concentrations and icebergs. The experimental conditions model a situation of the interaction between a wide structure and the <span class="hlt">ice</span> cover. Field data on a drifting <span class="hlt">ice</span> were collected during the Russian-US experiment in Antarctica WEDDELL-I in 1992.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3721118','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3721118"><span>Diatom assemblages promote <span class="hlt">ice</span> formation in large lakes</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>D'souza, N A; Kawarasaki, Y; Gantz, J D; Lee, R E; Beall, B F N; Shtarkman, Y M; Koçer, Z A; Rogers, S O; Wildschutte, H; Bullerjahn, G S; McKay, R M L</p> <p>2013-01-01</p> <p>We present evidence for the directed formation of <span class="hlt">ice</span> by planktonic communities dominated by filamentous diatoms sampled from the <span class="hlt">ice</span>-covered Laurentian Great Lakes. We hypothesize that <span class="hlt">ice</span> formation promotes attachment of these non-motile phytoplankton to overlying <span class="hlt">ice</span>, thereby maintaining a favorable position for the diatoms in the photic <span class="hlt">zone</span>. However, it is unclear whether the diatoms themselves are responsible for <span class="hlt">ice</span> nucleation. Scanning electron microscopy revealed associations of bacterial epiphytes with the dominant diatoms of the phytoplankton assemblage, and bacteria isolated from the phytoplankton showed elevated temperatures of crystallization (Tc) as high as −3 °C. <span class="hlt">Ice</span> nucleation-active bacteria were identified as belonging to the genus Pseudomonas, but we could not demonstrate that they were sufficiently abundant to incite the observed freezing. Regardless of the source of <span class="hlt">ice</span> nucleation activity, the resulting production of frazil <span class="hlt">ice</span> may provide a means for the diatoms to be recruited to the overlying lake <span class="hlt">ice</span>, thereby increasing their fitness. Bacterial epiphytes are likewise expected to benefit from their association with the diatoms as recipients of organic carbon excreted by their hosts. This novel mechanism illuminates a previously undescribed stage of the life cycle of the meroplanktonic diatoms that bloom in Lake Erie and other Great Lakes during winter and offers a model relevant to aquatic ecosystems having seasonal <span class="hlt">ice</span> cover around the world. PMID:23552624</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 marginal <span class="hlt">ice</span> <span class="hlt">zone</span> 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://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> Margin Experiment (LIMEX), conducted on the marginal <span class="hlt">ice</span> <span class="hlt">zone</span> (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('https://www.ncbi.nlm.nih.gov/pubmed/11701924','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11701924"><span>Thickness of a Europan <span class="hlt">ice</span> shell from impact crater simulations.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Turtle, E P; Pierazzo, E</p> <p>2001-11-09</p> <p>Several impact craters on Jupiter's satellite Europa exhibit central peaks. On the terrestrial planets, central peaks consist of fractured but competent rock uplifted during cratering. Therefore, the observation of central peaks on Europa indicates that an <span class="hlt">ice</span> layer must be sufficiently thick that the impact events did not completely penetrate it. We conducted numerical simulations of vapor and melt production during cratering of water <span class="hlt">ice</span> layers overlying liquid water to estimate the thickness of Europa's icy crust. Because impacts disrupt material well beyond the <span class="hlt">zone</span> of partial melting, our simulations put a lower limit on <span class="hlt">ice</span> thickness at the locations and times of impact. We conclude that the <span class="hlt">ice</span> must be more than 3 to 4 kilometers thick.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140008938','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140008938"><span>The Annual Glaciohydrology Cycle in the Ablation <span class="hlt">Zone</span> of the Greenland <span class="hlt">Ice</span> Sheet: Part 2. Observed and Modeled <span class="hlt">Ice</span> Flow</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Colgan, William Terence; Rajaram, Harihar; Anderson, Robert S.; Steffen, Konrad; Zwally, H. Jay; Phillips, Thomas; Abdalati, Waleed</p> <p>2012-01-01</p> <p><span class="hlt">Ice</span> velocities observed in 2005/06 at three GPS stations along the Sermeq Avannarleq flowline, West Greenland, are used to characterize an observed annual velocity cycle. We attempt to reproduce this annual <span class="hlt">ice</span> velocity cycle using a 1-D <span class="hlt">ice</span>-flow model with longitudinal stresses coupled to a 1-D hydrology model that governs an empirical basal sliding rule. Seasonal basal sliding velocity is parameterized as a perturbation of prescribed winter sliding velocity that is proportional to the rate of change of glacier water storage. The coupled model reproduces the broad features of the annual basal sliding cycle observed along this flowline, namely a summer speed-up event followed by a fall slowdown event. We also evaluate the hypothesis that the observed annual velocity cycle is due to the annual calving cycle at the terminus. We demonstrate that the <span class="hlt">ice</span> acceleration due to a catastrophic calving event takes an order of magnitude longer to reach CU/ETH ('Swiss') Camp (46km upstream of the terminus) than is observed. The seasonal acceleration observed at Swiss Camp is therefore unlikely to be the result of velocity perturbations propagated upstream via longitudinal coupling. Instead we interpret this velocity cycle to reflect the local history of glacier water balance.</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://www.dtic.mil/docs/citations/AD1013713','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1013713"><span>Seasonal <span class="hlt">Ice</span> <span class="hlt">Zone</span> Reconnaissance Surveys Coordination and Ocean Profiles</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>Morison), UpTempO buoy measurements of sea surface temperature (SST), sea level atmospheric pressure ( SLP ), and velocity (Steele), and dropsonde...dropsondes, micro-aircraft), cloud top/base heights UpTempO buoys for understanding and prediction…. Steele UpTempO buoy drops for SLP , SST, SSS...Air Expendable Current Profiler, SLP = Sea Level atmospheric Pressure, SST= Seas Surface Temperature, A/C= aircraft, SIC=Sea <span class="hlt">Ice</span> Concentration We</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.P34A..06B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.P34A..06B"><span>Breaking <span class="hlt">Ice</span> 2: A rift system on the Ross <span class="hlt">Ice</span> Shelf as an analog for tidal tectonics on icy moons</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brunt, K. M.; Hurford, T., Jr.; Schmerr, N. C.; Sauber, J. M.; MacAyeal, D. R.</p> <p>2016-12-01</p> <p><span class="hlt">Ice</span> shelves are the floating regions of the polar <span class="hlt">ice</span> sheets. Outside of the influence of the narrow region of their grounding <span class="hlt">zone</span>, they are fully hydrostatic and strongly influenced by the ocean tides. Recent observational and modeling studies have assessed the effect of tides on <span class="hlt">ice</span> shelves, including: the tidal influence on the <span class="hlt">ice</span>-shelf surface height, which changes by as much as 6 to 7 m on the southern extreme of the Ronne-Filchner <span class="hlt">Ice</span> Shelf; the tidal modulation of the <span class="hlt">ice</span>-shelf horizontal flow velocities, which changes the mean <span class="hlt">ice</span>-flow rate by as much as two fold on the Ross <span class="hlt">Ice</span> Shelf; and the tidal contribution to fracture and rift propagation, which eventually leads to iceberg calving. Here, we present the analysis of 16 days of continuous GPS data from a rift system near the front of the Ross <span class="hlt">Ice</span> Shelf. While the GPS sites were installed for a different scientific investigation, and not optimized to assess tidal rifting mechanics, they provide a first-order sense of the tidal evolution of the rift system. These analyses can be used as a terrestrial analog for tidal activity on icy satellites, such as Europa and Enceladus, moons of Jupiter and Saturn, respectively. Using remote sensing and modeling of the Ross <span class="hlt">Ice</span> Shelf rift system, we can investigate the geological processes observed on icy satellites and advance modeling efforts of their tidal-tectonic evolution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JGRC..120..777M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JGRC..120..777M"><span>Invisible polynyas: Modulation of fast <span class="hlt">ice</span> thickness by ocean heat flux on the Canadian polar shelf</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Melling, Humfrey; Haas, Christian; Brossier, Eric</p> <p>2015-02-01</p> <p>Although the Canadian polar shelf is dominated by thick fast <span class="hlt">ice</span> in winter, areas of young <span class="hlt">ice</span> or open water do recur annually at locations within and adjacent to the fast <span class="hlt">ice</span>. These polynyas are detectable by eye and sustained by wind or tide-driven <span class="hlt">ice</span> divergence and ocean heat flux. Our <span class="hlt">ice</span>-thickness surveys by drilling and towed electromagnetic sounder reveal that visible polynyas comprise only a subset of thin-<span class="hlt">ice</span> coverage. Additional area in the coastal <span class="hlt">zone</span>, in shallow channels and in fjords is covered by thin <span class="hlt">ice</span> which is too thick to be discerned by eye. Our concurrent surveys by CTD reveal correlation between thin fast <span class="hlt">ice</span> and above-freezing seawater beneath it. We use winter time series of air and ocean temperatures and <span class="hlt">ice</span> and snow thicknesses to calculate the ocean-to-<span class="hlt">ice</span> heat flux as 15 and 22 W/m2 at locations with thin <span class="hlt">ice</span> in Penny Strait and South Cape Fjord, respectively. Near-surface seawater above freezing is not a sufficient condition for ocean heat to reach the <span class="hlt">ice</span>; kinetic energy is needed to overcome density stratification. The ocean's isolation from wind under fast <span class="hlt">ice</span> in winter leaves tides as the only source. Two tidal mechanisms driving ocean heat flux are discussed: diffusion via turbulence generated by shear at the under-<span class="hlt">ice</span> and benthic boundaries, and the internal hydraulics of flow over topography. The former appears dominant in channels and the coastal <span class="hlt">zone</span> and the latter in some silled fjords where and when the layering of seawater density permits hydraulically critical flow.</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 marginal <span class="hlt">zone</span> 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/2017AGUFMGC53E0944A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC53E0944A"><span>Record low lake <span class="hlt">ice</span> thickness and bedfast <span class="hlt">ice</span> extent on Alaska's Arctic Coastal Plain in 2017 exemplify the value of monitoring freshwater <span class="hlt">ice</span> to understand sea-<span class="hlt">ice</span> forcing and predict permafrost dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Arp, C. D.; Alexeev, V. A.; Bondurant, A. C.; Creighton, A.; Engram, M. J.; Jones, B. M.; Parsekian, A.</p> <p>2017-12-01</p> <p>The winter of 2016/2017 was exceptionally warm and snowy along the coast of Arctic Alaska partly due to low fall sea <span class="hlt">ice</span> extent. Based on several decades of field measurements, we documented a new record low maximum <span class="hlt">ice</span> thickness (MIT) for lakes on the Barrow Peninsula, averaging 1.2 m. This is in comparison to a long-term average MIT of 1.7 m stretching back to 1962 with a maximum of 2.1 m in 1970 and previous minimum of 1.3 m in 2014. The relevance of thinner lake <span class="hlt">ice</span> in arctic coastal lowlands, where thermokarst lakes cover greater than 20% of the land area, is that permafrost below lakes with bedfast <span class="hlt">ice</span> is typically preserved. Lakes deeper than the MIT warm and thaw sub-lake permafrost forming taliks. Remote sensing analysis using synthetic aperture radar (SAR) is a valuable tool for scaling the field observations of MIT to the entire freshwater landscape to map bedfast <span class="hlt">ice</span>. A new, long-term time-series of late winter multi-platform SAR from 1992 to 2016 shows a large dynamic range of bedfast <span class="hlt">ice</span> extent, 29% of lake area or 6% of the total land area over this period, and adding 2017 to this record is expected to extend this range further. Empirical models of lake mean annual bed temperature suggest that permafrost begins to thaw at depths less than 60% of MIT. Based on this information and knowledge of average lake <span class="hlt">ice</span> growth trajectories, we suggest that future SAR analysis of lake <span class="hlt">ice</span> should focus on mid-winter (January) to evaluate the extent of bedfast <span class="hlt">ice</span> and corresponding <span class="hlt">zones</span> of sub-lake permafrost thaw. Tracking changes in these areas from year to year in mid-winter may provide the best landscape-scale evaluation of changing permafrost conditions in lake-rich arctic lowlands. Because observed changes in MIT coupled with mid-winter bedfast <span class="hlt">ice</span> extent provide much information on permafrost stability, we suggest that these measurements can serve as Essential Climate Variables (EVCs) to indicate past and future changes in lake-rich arctic regions. The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.9552K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.9552K"><span>Palaeo-<span class="hlt">ice</span> stream pathways in the easternmost Amundsen Sea Embayment, 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>Klages, Johann P.; Kuhn, Gerhard; Graham, Alastair G. C.; Smith, James A.; Hillenbrand, Claus-Dieter; Nitsche, Frank O.; Larter, Rob D.; Gohl, Karsten</p> <p>2015-04-01</p> <p>Multibeam swath bathymetry datasets collected over the past two decades have been compiled to identify palaeo-<span class="hlt">ice</span> stream pathways in the easternmost Amundsen Sea Embayment. We mapped 3010 glacial landforms to reconstruct palaeo-<span class="hlt">ice</span> flow in the ~250 km-long Abbot Glacial Trough that was occupied by a large palaeo-<span class="hlt">ice</span> stream, fed by two tributaries (Cosgrove and Abbot) that reached the continental shelf edge during the last maximum <span class="hlt">ice</span>-sheet advance. The mapping has enabled a clear differentiation between glacial landforms interpreted as indicative of wet- (e.g. mega-scale glacial lineations) and cold-based <span class="hlt">ice</span> (e.g. hill-hole pairs) during the last glaciation of the continental shelf. Both the regions of fast palaeo-<span class="hlt">ice</span> flow within the palaeo-<span class="hlt">ice</span> stream troughs, and the regions of slow palaeo-<span class="hlt">ice</span> flow on adjacent seafloor highs (referred to as inter-<span class="hlt">ice</span> stream ridges) additionally record glacial landforms such as grounding-<span class="hlt">zone</span> wedges and recessional moraines that indicate grounding line stillstands of the <span class="hlt">ice</span> sheet during the last deglaciation from the shelf. As the palaeo-<span class="hlt">ice</span> stream flowed along a trough with variable geometry and variable subglacial substrate, it appears that trough sections characterized by constrictions and outcropping hard substrate that changes the bed gradient, led the pace of grounding-line retreat to slow and subsequently pause, resulting in the deposition of grounding-<span class="hlt">zone</span> wedges. The stepped retreat recorded within the Abbot Glacial Trough corresponds well to post-glacial stepped retreat interpreted for the neighbouring Pine Island-Thwaites Palaeo-<span class="hlt">Ice</span> Stream trough, thus suggesting a uniform pattern of episodic retreat across the eastern Amundsen Sea Embayment. The correlation of episodic retreat features with geological boundaries further emphasises the significance of subglacial geology in steering <span class="hlt">ice</span> stream flow. Our new geomorphological map of the easternmost Amundsen Sea Embayment resolves the pathways of palaeo-<span class="hlt">ice</span> streams that</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADB805737','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADB805737"><span><span class="hlt">Icing</span> <span class="hlt">Zones</span> in a Warm Front System with General Precipitation</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1947-07-01</p> <p>to the Bergeron- Findeisen theory of the forma- tion of precipitation; any large are& of cbntinuouti grecipita-. tion is characterized by the...Journal. of Xeteorology, vol. no. 3, September 194-6, pp. 57-77. 3,’ Findeisen , V. : Meteorologic.K&Physical Lfmitntions of <span class="hlt">Icing</span> in 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 marginal <span class="hlt">ice</span> <span class="hlt">zone</span>, 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/2016AGUFMPP51A2283T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMPP51A2283T"><span>Spatial Variability of Climate Signatures Recorded in an Array of Shallow Firn Cores from the Western Greenland Percolation <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thundercloud, Z. R.; Osterberg, E. C.; Ferris, D. G.; Graeter, K.; Lewis, G.; Hawley, R. L.; Marshall, H. P.</p> <p>2016-12-01</p> <p>Greenland <span class="hlt">ice</span> cores provide seasonally to annually resolved proxy records of past temperature, accumulation and atmospheric circulation. Most Greenland <span class="hlt">ice</span> cores have been collected from the dry snow <span class="hlt">zone</span> at elevations greater than 2500 m to produce records of North Atlantic paleoclimate over the last full glacial cycle. <span class="hlt">Ice</span> cores collected from more costal regions, however, provide the opportunity to develop regional-scale records of climate conditions along <span class="hlt">ice</span> sheet margins where recent temperature and precipitation changes have been larger than those in the <span class="hlt">ice</span> sheet interior. These cores are more readily comparable to lake sediment and landscape (i.e. moraine) records from the <span class="hlt">ice</span> sheet margin, and are potentially more sensitive to sea-<span class="hlt">ice</span> variability due to the proximity to the coast. Here we present major ion and stable isotope records from an array of firn cores (40-55 year records) collected in the western Greenland percolation <span class="hlt">zone</span>, and assess the spatial variability of <span class="hlt">ice</span> core statistical relationships with the North Atlantic Oscillation (NAO) and Baffin Bay sea <span class="hlt">ice</span> extent. Seven cores were collected from elevations of 2100-2500 m along a 400-km segment of the <span class="hlt">ice</span> sheet from Dye-2 to Milcent as part of the Greenland Traverse for Accumulation and Climate Studies (GreenTrACS) project from May-June 2016. They were sampled by a continuous melter system at Dartmouth College, and analyzed using Dionex ion chromatographs and a Picarro L2130-i laser ring-down spectrometer. We focus on the signature of the NAO and Baffin Bay sea <span class="hlt">ice</span> extent in the sea-salt, dust, deuterium excess (d-excess), and methanesulfonic acid (MSA) firn core records, and assess the special variability of these climate-<span class="hlt">ice</span> core relationships across the study area. Climate reanalysis data indicate that NAO-<span class="hlt">ice</span> core correlations should be stronger at lower elevation in the percolation <span class="hlt">zone</span> than high in the dry snow <span class="hlt">zone</span>. Our results will provide valuable insight into the sensitivity of</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 marginal <span class="hlt">ice</span> <span class="hlt">zone</span> (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> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..11.1261G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..11.1261G"><span>Buttressing and stability of marine <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>Goldberg, D.; Holland, D. M.; Schoof, C.</p> <p>2009-04-01</p> <p>The West Antarctic <span class="hlt">Ice</span> Sheet is marine in nature, meaning most of its base is below sea level. At the grounding line (where it becomes thin enough to float), its outlet streams flow into large <span class="hlt">ice</span> shelves. Gravitational stress in the shelf is transmitted back to the grounding line, and largely balanced by basal friction in the transition <span class="hlt">zone</span>. The details of this force balance control the evolution of both the thickness and grounded extent of the <span class="hlt">ice</span> sheet, and can lead to Weertman's (1974) Marine Instability for a foredeepened bedrock (one that deepens inland). However, the presence of rigid sidewalls and locally grounded regions in the shelf can reduce the longitudinal stresses felt at the grounding line (a phenomenon called buttressing). Thomas (1979) and others pointed out that Marine Instability may be lessened or reversed by <span class="hlt">ice</span> shelf buttressing. When modelling marine <span class="hlt">ice</span> sheets numerically, the physics of the grounded-to-floating transition must be represented and the associated small length scales must be resolved (Schoof, 2007). Failing to do so can result in nonphysical or numerically inconsistent behavior (Vieli and Payne, 2005). While several methods have been developed to treat these issues (Vieli and Payne, 2005; Pattyn et al, 2006; Schoof, 2007) they are limited to flowline models. We present a model that represents the physics of the grounded-to-floating transition in a time-dependent three-dimensional marine <span class="hlt">ice</span> sheet, using mesh adaption to resolve the transition <span class="hlt">zone</span>. We show that in the special case of a two-dimensional sheet our model reproduces the theoretical results of the MISMIP experiments, and that it produces robust results when both horizontal dimensions are resolved. In idealized experiments in a channel with rigid sidewalls and a foredeepened bed, we narrow the channel to determine whether buttressing is sufficient to reverse instability. We find that for strong beds (high friction coefficients), while the timescales and dynamics are</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.9286O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.9286O"><span>The influence of climate change on the intensity of <span class="hlt">ice</span> gouging at the Kara Sea bottom by hummocky formations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ogorodov, Stanislav; Arkhipov, Vasily; Kokin, Osip; Natalia, Shabanova</p> <p>2016-04-01</p> <p>Sea <span class="hlt">ice</span> as a zonal factor is an important passive and active relief-forming agent in the coastal-shelf <span class="hlt">zone</span> of the Arctic and other freezing seas. The most dangerous process in relation to the hydrotechnical facilities is <span class="hlt">ice</span> gouging - destructive mechanical impact of the <span class="hlt">ice</span> of the ground, connected with the dynamics of the <span class="hlt">ice</span> cover, formation of hummocks and stamukhas under the influence of hydrometeorologic factors and of the relief of the coastal-shelf <span class="hlt">zone</span>. Underestimation of the <span class="hlt">ice</span> gouging intensity can lead to damage of the engineering facilities, while excessive deepening increases the expenses of the construction. Finding the optimal variant and, by this, decreasing the risks of extreme situations is a relevant task of the science and practice. This task is complicated by the fact that the oil and gas infrastructure within the coastal and shelf areas of the freezing seas is currently being developed in the conditions of global climate change. In the present work, several results of the repeated sounding of bottom <span class="hlt">ice</span> gouging microrelief within the area of the underwater pipeline crossing of the Baydaratskaya Bay, Kara Sea, are presented. Based on the results of the monitoring, as well as the analysis of literature sources and modeling it has been established that under the conditions of climate warming and sea <span class="hlt">ice</span> reduction, the <span class="hlt">zone</span> of the most intensive <span class="hlt">ice</span> gouging is shifted landwards, on shallower water areas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C32A..01M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C32A..01M"><span>Microbial processes at the beds of glaciers and <span class="hlt">ice</span> sheets: a look at life below the Whillans <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>Mikucki, J.; Campen, R.; Vancleave, S.; Scherer, R. P.; Coenen, J. J.; Powell, R. D.; Tulaczyk, S. M.</p> <p>2017-12-01</p> <p>Groundwater, saturated sediments and hundreds of subglacial lakes exist below the <span class="hlt">ice</span> sheets of Antarctica. The few Antarctic subglacial environments sampled to date all contain viable microorganisms. This is a significant finding because microbes are known to be key in mediating biogeochemical cycles. In sediments, microbial metabolic activity can also result in byproducts or direct interactions with sediment particles that influence the physical and geochemical characteristics of the matrix they inhabit. Subglacial Lake Whillans (SLW), a fresh water lake under the Whillans <span class="hlt">Ice</span> Stream that drains into the Ross Sea at its grounding <span class="hlt">zone</span>, was recently sampled as part of the NSF-funded Whillans <span class="hlt">Ice</span> Stream Subglacial Access Research Drilling (WISSARD) project. Sediments from both SLW and its grounding <span class="hlt">zone</span> contain microbial taxa related to iron, sulfur, nitrogen and methane oxidizers. In addition to molecular data, biogeochemical measurements and culture based experiments on Whillans sediments support the notion that the system is chemosynthetic with energy derived in part by cycling inorganic compounds. Etch pitting and mineral precipitates on fossil sponge spicules suggest that spicules may also provide microbial nutrients in these environments. Perhaps the most widespread microbial process that affects sediment structure and mineral weathering is the production of extra polymeric substances (EPS). Several phylogenetic groups detected in Whillans sediments are known to produce EPS and we have observed its production in pure cultures enriched directly from these sediments. Our data sheds light on how microbial life persists below the Antarctic <span class="hlt">Ice</span> Sheet despite extended isolation in icy darkness, and how these microbes may be shaping their environment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..DFDE12003S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DFDE12003S"><span>A Bridge Too Far: Suppressing Frost Using an Out-of-Plane Dry <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Spohn, Corey; Ahmadi, Farzad; Nath, Saurabh; Boreyko, Jonathan</p> <p>2017-11-01</p> <p>It has recently been shown that <span class="hlt">ice</span> can suppress the formation of any nearby condensation or frost on a substrate. However, these in-plane dry <span class="hlt">zones</span> require the hygroscopic <span class="hlt">ice</span> features to be placed on the same surface they are helping to keep dry, which makes it impossible to achieve complete anti-frosting. Here, we create an out-of-plane dry <span class="hlt">zone</span> by holding two aluminum surfaces parallel to each other, where a uniform sheet of frost was grown on one surface to keep the other surface completely dry. The critical separation required to keep the test surface dry was found to be a function of the ambient supersaturation. We also show that inter-droplet <span class="hlt">ice</span> bridging, now known to be a primary mechanism for in-plane frost growth, can be similarly extended to an out-of-plane configuration. We freeze a droplet on a hydrophobic surface and suspend a water droplet above it, such that an <span class="hlt">ice</span> bridge grows toward the water droplet. More generally, these findings show that the recently discovered phenomena of dry <span class="hlt">zones</span> and <span class="hlt">ice</span> bridging can be extended to out-of-plane scenarios, which could lead to a better understanding of the behavior of mixed-phase systems. This work was supported by the National Science Foundation (CBET-1604272) and by the 3M Company (Non-Tenured Faculty Award).</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 marginal <span class="hlt">ice</span> <span class="hlt">zone</span> 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('http://adsabs.harvard.edu/abs/2012PhDT.......190H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012PhDT.......190H"><span>The influence of sea <span class="hlt">ice</span> on Antarctic <span class="hlt">ice</span> core sulfur chemistry and on the future evolution of Arctic snow depth: Investigations using global models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hezel, Paul J.</p> <p></p> <p>Observational studies have examined the relationship between methanesulfonic acid (MSA) measured in Antarctic <span class="hlt">ice</span> cores and sea <span class="hlt">ice</span> extent measured by satellites with the aim of producing a proxy for past sea <span class="hlt">ice</span> extent. MSA is an oxidation product of dimethylsulfide (DMS) and is potentially linked to sea <span class="hlt">ice</span> based on observations of very high surface seawater DMS in the sea <span class="hlt">ice</span> <span class="hlt">zone</span>. Using a global chemical transport model, we present the first modeling study that specifically examines this relationship on interannual and on glacial-interglacial time scales. On interannual time scales, the model shows no robust relationship between MSA deposited in Antarctica and sea <span class="hlt">ice</span> extent. We show that lifetimes of MSA and DMS are longer in the high latitudes than in the global mean, interannual variability of sea <span class="hlt">ice</span> is small (<25%) as a fraction of sea <span class="hlt">ice</span> area, and sea <span class="hlt">ice</span> determines only a fraction of the variability (<30%) of DMS emissions from the ocean surface. A potentially larger fraction of the variability in DMS emissions is determined by surface wind speed (up to 46%) via the parameterization for ocean-to-atmosphere gas exchange. Furthermore, we find that a significant fraction (up to 74%) of MSA deposited in Antarctica originates from north of 60°S, north of the seasonal sea <span class="hlt">ice</span> <span class="hlt">zone</span>. We then examine the deposition of MSA and non-sea-salt sulfate (nss SO2-4 ) on glacial-interglacial time scales. <span class="hlt">Ice</span> core observations on the East Antarctic Plateau suggest that MSA increases much more than nss SO2-4 during the last glacial maximum (LGM) compared to the modern period. It has been suggested that high MSA during the LGM is indicative of higher primary productivity and DMS emissions in the LGM compared to the modern day. Studies have also shown that MSA is subject to post-depositional volatilization, especially during the modern period. Using the same chemical transport model driven by meteorology from a global climate model, we examine the sensitivity of MSA and nss</p> </li> <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 Marginal <span class="hlt">Ice</span> <span class="hlt">Zone</span> 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://ntrs.nasa.gov/search.jsp?R=19940015961&hterms=glacier+melt&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dglacier%2Bmelt','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19940015961&hterms=glacier+melt&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dglacier%2Bmelt"><span>Radar backscattering from snow facies of the Greenland <span class="hlt">ice</span> sheet: Results from the AIRSAR 1991 campaign</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rignot, Eric; Jezek, K.; Vanzyl, J. J.; Drinkwater, Mark R.; Lou, Y. L.</p> <p>1993-01-01</p> <p>In June 1991, the NASA/JPL airborne SAR (AIRSAR) acquired C- (lambda = 5.6cm), L- (lambda = 24cm), and P- (lambda = 68m) band polarimetric SAR data over the Greenland <span class="hlt">ice</span> sheet. These data are processed using version 3.55 of the AIRSAR processor which provides radiometrically and polarimetrically calibrated images. The internal calibration of the AIRSAR data is cross-checked using the radar response from corner reflectors deployed prior to flight in one of the scenes. In addition, a quantitative assessment of the noise power level at various frequencies and polarizations is made in all the scenes. Synoptic SAR data corresponding to a swath width of about 12 by 50 km in length (compared to the standard 12 x 12 km size of high-resolution scenes) are also processed and calibrated to study transitions in radar backscatter as a function of snow facies at selected frequencies and polarizations. The snow facies on the Greenland <span class="hlt">ice</span> sheet are traditionally categorized based on differences in melting regime during the summer months. The interior of Greenland corresponds to the dry snow <span class="hlt">zone</span> where terrain elevation is the highest and no snow melt occurs. The lowest elevation boundary of the dry snow <span class="hlt">zone</span> is known traditionally as the dry snow line. Beneath it is the percolation <span class="hlt">zone</span> where melting occurs in the summer and water percolates through the snow freezing at depth to form massive <span class="hlt">ice</span> lenses and <span class="hlt">ice</span> pipes. At the downslope margin of this <span class="hlt">zone</span> is the wet snow line. Below it, the wet snow <span class="hlt">zone</span> corresponds to the lowest elevations where snow remains at the end of the summer. Ablation produces enough meltwater to create areas of snow saturated with water, together with ponds and lakes. The lowest altitude <span class="hlt">zone</span> of ablation sees enough summer melt to remove all traces of seasonal snow accumulation, such that the surface comprises bare glacier <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19780017559','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19780017559"><span>LANDSAT survey of near-shore <span class="hlt">ice</span> conditions along the Arctic coast of Alaska</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stringer, W. J. (Principal Investigator); Barrett, S. A.</p> <p>1978-01-01</p> <p>The author has identified the following significant results. Winter and spring near-shore <span class="hlt">ice</span> conditions were analyzed for the Beaufort Sea 1973-77, and the Chukchi Sea 1973-76. LANDSAT imagery was utilized to map major <span class="hlt">ice</span> features related to regional <span class="hlt">ice</span> morphology. Significant features from individual LANDSAT image maps were combined to yield regional maps of major <span class="hlt">ice</span> ridge systems for each year of study and maps of flaw lead systems for representative seasons during each year. These regional maps were, in turn, used to prepare seasonal <span class="hlt">ice</span> morphology maps. These maps showed, in terms of a zonal analysis, regions of statistically uniform <span class="hlt">ice</span> behavior. The behavioral characteristics of each <span class="hlt">zone</span> were described in terms of coastal processes and bathymetric configuration.</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 marginal <span class="hlt">ice</span> <span class="hlt">zone</span> 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> </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/2016AGUFM.C53C0732W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C53C0732W"><span>Iceberg Ploughmarks Indicate Past Rapid Iceberg Calving and Retreat of Pine Island-Thwaites <span class="hlt">Ice</span> Stream due to Marine <span class="hlt">Ice</span>-Cliff Instability Processes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wise, M.; Dowdeswell, J. A.; Larter, R. D.; Jakobsson, M.</p> <p>2016-12-01</p> <p>Seafloor ploughmarks provide evidence of past and present iceberg dimensions and drift direction. Today, Pine Island and Thwaites glaciers, which account for 35% of mass loss from the West Antarctic <span class="hlt">Ice</span> Sheet (WAIS), calve mainly large, tabular icebergs, which, when grounded, produce `toothcomb-like' multi-keeled ploughmarks. High-resolution multi-beam swath bathymetry of the mid-shelf Pine Island Trough and adjacent banks, reveals many linear-curvilinear depressions interpreted as iceberg-keel ploughmarks, the majority of which are single-keeled in form. From measurements of ploughmark planform and cross-sections, we find iceberg calving from the palaeo-Pine Island-Thwaites <span class="hlt">Ice</span> Stream was not characterised by small numbers of large, tabular icebergs, but instead, by a large number of `smaller' icebergs with v-shaped keels. Geological evidence of ploughmark form and water-depth distribution indicates calving-margin thicknesses ( 950 m) and subaerial <span class="hlt">ice</span>-cliff elevations ( 100 m) equivalent to the theoretical threshold recently predicted to trigger <span class="hlt">ice</span>-cliff structural collapse through Marine <span class="hlt">Ice</span> Cliff Instability (MICI) processes. Significantly, our proposed period of iceberg ploughing predates the early Holocene climate optimum, and likely occurred in an absence of widespread surface melt. We therefore provide the first observational evidence of rapid retreat of the Palaeo-Pine Island-Thwaites <span class="hlt">ice</span> stream from the crest of a large, mid-shelf sedimentary depocentre or grounding-<span class="hlt">zone</span> wedge, to a restabilising position 112 km offshore of the December 2013 calving line, driven by MICI processes commencing 12.3 cal. ka BP. We emphasise the effective operation of MICI processes without extensive surface melt and induced hydrofracture, and conclude that such processes are unlikely to be confined to the past, given the steep, retrograde bed-slope which the modern grounding lines of Pine Island and Thwaites Glaciers are approaching, and the absence of any discernible</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.S52A..06B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.S52A..06B"><span>Teleseismic Earthquake Signals Observed on an <span class="hlt">Ice</span> Shelf</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Baker, M. G.; Aster, R. C.; Anthony, R. E.; Wiens, D.; Nyblade, A.; Bromirski, P. D.; Stephen, R. A.; Gerstoft, P.</p> <p>2015-12-01</p> <p>The West Antarctic Rift System (WARS) is one of Earth's largest continental extension <span class="hlt">zones</span>. Study of the WARS is complicated by the presence of the West Antarctic <span class="hlt">Ice</span> Sheet, the Ross <span class="hlt">Ice</span> Shelf, and the Ross Sea. Recent deployments of broadband seismographs in the POLENET project have allowed passive seismic techniques, such as receiver function analysis and surface wave dispersion, to be widely utilized to infer crustal and mantle velocity structure across much of the WARS and West Antarctica. However, a large sector of the WARS lies beneath the Ross <span class="hlt">Ice</span> Shelf. In late 2014, 34 broadband seismographs were deployed atop the <span class="hlt">ice</span> shelf to jointly study deep Earth structure and the dynamics of the <span class="hlt">ice</span> shelf. <span class="hlt">Ice</span> shelf conditions present strong challenges to broadband teleseismic imaging: 1) The presence of complicating signals in the microseism through long-period bands due to the influence of ocean gravity waves; 2) The strong velocity contrasts at the <span class="hlt">ice</span>-water and water-sediment interfaces on either side of the water layer give rise to large amplitude reverberations; 3) The water layer screens S-waves or P-to-S phases originating from below the water layer. We present an initial analysis of the first teleseismic earthquake arrivals collected on the <span class="hlt">ice</span> shelf at the end of the 2014 field season from a limited subset of these stations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140017431','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140017431"><span>Spatially Mapped Reductions in the Length of the Arctic Sea <span class="hlt">Ice</span> Season</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parkinson, Claire L.</p> <p>2014-01-01</p> <p>Satellite data are used to determine the number of days having sea <span class="hlt">ice</span> coverage in each year 1979-2013 and to map the trends in these <span class="hlt">ice</span>-season lengths. Over the majority of the Arctic seasonal sea <span class="hlt">ice</span> <span class="hlt">zone</span>, the <span class="hlt">ice</span> season shortened at an average rate of at least 5 days/decade between 1979 and 2013, and in a small area in the northeastern Barents Sea the rate of shortening reached over 65 days/decade. The only substantial non-coastal area with lengthening sea <span class="hlt">ice</span> seasons is the Bering Sea, where the <span class="hlt">ice</span> season lengthened by 5-15 days/decade. Over the Arctic as a whole, the area with <span class="hlt">ice</span> seasons shortened by at least 5 days/decade is 12.4 × 10(exp 6) square kilimeters, while the area with <span class="hlt">ice</span> seasons lengthened by at least 5 days/decade is only 1.1 × 10(exp 6) square kilometers. The contrast is even greater, percentage-wise, for higher rates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19890025240&hterms=wind+monitor&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dwind%2Bmonitor','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19890025240&hterms=wind+monitor&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dwind%2Bmonitor"><span>Wind, current and swell influences on the <span class="hlt">ice</span> extent and flux in the Grand Banks-Labrador sea area as observed in the LIMEX '87 experiment</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Argus, Susan Digby; Carsey, Frank; Holt, Benjamin</p> <p>1988-01-01</p> <p>This paper presents data collected by airborne and satellite instruments during the Labrador <span class="hlt">Ice</span> Margin Experiment, that demonstrate the effects of oceanic and atmospheric processes on the <span class="hlt">ice</span> conditions in the Grand Banks-Labrador sea area. Special consideration is given to the development of algorithms for extracting information from SAR data. It is shown that SAR data can be used to monitor <span class="hlt">ice</span> extent, determine <span class="hlt">ice</span> motion, locate shear <span class="hlt">zones</span>, monitor the penetration of swell into the <span class="hlt">ice</span>, estimate floe sizes, and establish the dimensions of the <span class="hlt">ice</span> velocity <span class="hlt">zones</span>. It is also shown that the complex interaction of the <span class="hlt">ice</span> cover with winds, currents, swell, and coastlines is similar to the dynamics established for a number of sites in both polar regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFMAE33B0282F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFMAE33B0282F"><span><span class="hlt">Ice</span> in Volcanic Clouds</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Few, A. A.</p> <p>2010-12-01</p> <p>It is widely recognized that lightning activity in thunderstorm clouds is associated with <span class="hlt">ice</span> in the clouds. In volcanic plumes the lower electrical discharges near the vent are clearly not associated with <span class="hlt">ice</span>; however, the electrical discharges from the upper volcanic clouds very likely are associated with <span class="hlt">ice</span>. There is ample water in volcanic plumes and clouds. The explosive volcanic eruption is produced by volatile components in the rising magma. Researchers estimate that the water content of the volatiles is up to 99% by mole; other gases are mainly sulfur and chlorine species. These volatiles carry with them a wide range of hot magma melts and solids, importantly silicate particles and tephra. The more massive components fall out near the vent carrying with them much of the heat from the plume; these large components are not in thermodynamic equilibrium with the gases, ash, and lapilli; thus the heat removed does not lower the temperature of the materials carried aloft in the plume. Upward motion is initially provided by the thrust from the volcanic eruption, then by buoyancy of the hot plume. The rising plume is cooled by entrainment of environmental air, which contains water, and by adiabatic expansion; the plume transitions into a volcanic cloud. Further lifting and cooling produces supercooled water droplets (T ~ -5 C) in a limited <span class="hlt">zone</span> (z ~ 9 km) before the fast updraft (~ 60 m/s) rapidly transforms them into <span class="hlt">ice</span>. Computer models of volcanic clouds that include water and <span class="hlt">ice</span> microphysics indicate that the latent heat of condensation is not significant in cloud dynamics because it occurs in a region where buoyancy is provided by the original hot plume material. The latent heat of <span class="hlt">ice</span> formation occurs at higher and colder levels and seems to contribute to the final lifting of the cloud top by ~1.5km. Laboratory results indicate that the fine silicate ash particles, which are abundant, are good <span class="hlt">ice</span> nuclei, IN. Because of the abundance of the silicate ash</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 marginal <span class="hlt">ice</span> <span class="hlt">zones</span> 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('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 Marginal <span class="hlt">Ice</span> <span class="hlt">Zones</span>. II. A Science Plan for a Summer Marginal <span class="hlt">Ice</span> <span class="hlt">Zone</span> 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/2015AGUFM.C11B0758J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C11B0758J"><span>Imaging Basal Crevasses at the Grounding Line of Whillans <span class="hlt">Ice</span> Stream, 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>Jacobel, R. W.; Dawson, E. C.; Christianson, K.</p> <p>2015-12-01</p> <p>We acquired gridded ground-based radar data at the WIS grounding <span class="hlt">zone</span> where the transition from limited- or no-slip conditions at the base of grounded <span class="hlt">ice</span> to free-slip conditions beneath floating <span class="hlt">ice</span> occurs across a region only a few kilometers wide. This transition is either an elastic-flexural transition from bedrock to hydrostatically-supported elevations (often tidally influenced), a transition from thicker to thinner <span class="hlt">ice</span> over a flat bed, or some combination of these. In either case, the stress field of the <span class="hlt">ice</span> changes as it flows across the grounding <span class="hlt">zone</span>, often resulting in brittle deformation, which is manifested as basal crevassing at the <span class="hlt">ice</span>-sheet base and sometimes as strand cracks at the surface. The position and morphology of these features reveal important information about the stress state across this transition where <span class="hlt">ice</span> and ocean interact. Our surveys indicate a complex pattern of basal crevassing with many imaged in two or more profile segments as a linear feature at the bed, usually trending oblique to flow and often extending for several kilometers. Due to the wide beam pattern of our antennas, we image many of the crevasses from off-nadir reflections. Thus their arrival times are later than the primary basal reflection and segments of the crevasse appear "below" the bed, when in fact they are merely trending oblique to the profile. Often these returns have a reversed phase relative to the bed echo because the high dielectric contrast of seawater and a favorable geometry enable reflections with little loss (but a second phase reversal) from the <span class="hlt">ice</span>-water interface near the crevasse base. In a few cases, these crevasse echoes from targets trending oblique to the profile appear to mimic the geometry of a sub-<span class="hlt">ice</span> sediment "wedge", while in reality the radar never penetrates below the basal interface. Only about 25% of the crevasses appear to extend any significant distance upward into the basal <span class="hlt">ice</span>, typically at low angles. A subset of these are</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> margin during warm intervals of the Oligocene-Miocene. Flat-lying bedrock plateaus are indicative of an <span class="hlt">ice</span> sheet margin positioned >400-500 km inland of the modern grounding <span class="hlt">zone</span> for extended periods of the Oligocene-Miocene, equivalent to a 2-m rise in global sea level. Our findings imply that if major EAIS retreat occurs in the future, isostatic rebound will enable the plateau surfaces to act as seeding points for extensive <span class="hlt">ice</span> rises, thus limiting extensive <span class="hlt">ice</span> margin retreat of the scale seen during the early EAIS.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C42A..07R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C42A..07R"><span>Bending the law: tidal bending and its effects on <span class="hlt">ice</span> viscosity and flow</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rosier, S.; Gudmundsson, G. H.</p> <p>2017-12-01</p> <p>Many <span class="hlt">ice</span> shelves are subject to strong ocean tides and, in order to accommodate this vertical motion, the <span class="hlt">ice</span> must bend within the grounding <span class="hlt">zone</span>. This tidal bending generates large stresses within the <span class="hlt">ice</span>, changing its effective viscosity. For a confined <span class="hlt">ice</span> shelf, this is particularly relevant because the tidal bending stresses occur along the sidewalls, which play an important role in the overall flow regime of the <span class="hlt">ice</span> shelf. Hence, tidal bending stresses will affect both the mean and time-varying components of <span class="hlt">ice</span> shelf flow. GPS measurements reveal strong variations in horizontal <span class="hlt">ice</span> shelf velocities at a variety of tidal frequencies. We show, using full-Stokes viscoelastic modelling, that inclusion of tidal bending within the model accounts for much of the observed tidal modulation of horizontal <span class="hlt">ice</span> shelf flow. Furthermore, our model shows that in the absence of a vertical tidal forcing, the mean flow of the <span class="hlt">ice</span> shelf is reduced considerably.</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 marginal <span class="hlt">ice</span> <span class="hlt">zone</span> 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('https://ntrs.nasa.gov/search.jsp?R=PIA00291&hterms=europa+ice&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Deuropa%2Bice','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=PIA00291&hterms=europa+ice&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Deuropa%2Bice"><span>Europa's Broken <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></p> <p>1996-01-01</p> <p>Jupiter's moon Europa, as seen in this image taken June 27, 1996 by NASA's Galileo spacecraft, displays features in some areas resembling <span class="hlt">ice</span> floes seen in Earth's polar seas. Europa, about the size of Earth's moon, has an icy crust that has been severely fractured, as indicated by the dark linear, curved, and wedged-shaped bands seen here. These fractures have broken the crust into plates as large as 30 kilometers (18.5 miles) across. Areas between the plates are filled with material that was probably icy slush contaminated with rocky debris. Some individual plates were separated and rotated into new positions. Europa's density indicates that it has a shell of water <span class="hlt">ice</span> as thick as 100 kilometers (about 60 miles), parts of which could be liquid. Currently, water <span class="hlt">ice</span> could extend from the surface down to the rocky interior, but the features seen in this image suggest that motion of the disrupted icy plates was lubricated by soft <span class="hlt">ice</span> or liquid water below the surface at the time of disruption. This image covers part of the equatorial <span class="hlt">zone</span> of Europa and was taken from a distance of 156,000 kilometers (about 96,300 miles) by the solid-state imager camera on the Galileo spacecraft. North is to the right and the sun is nearly directly overhead. The area shown is about 360 by 770 kilometers (220-by-475 miles or about the size of Nebraska), and the smallest visible feature is about 1.6 kilometers (1 mile) across. The Jet Propulsion Laboratory manages the Galileo mission for NASA's Office of Space Science.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/984088-modeling-fracture-ice-sheets-parallel-computers','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/984088-modeling-fracture-ice-sheets-parallel-computers"><span>Modeling the fracture of <span class="hlt">ice</span> sheets on parallel computers.</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>Waisman, Haim; Bell, Robin; Keyes, David</p> <p>2010-03-01</p> <p>The objective of this project is to investigate the complex fracture of <span class="hlt">ice</span> and understand its role within larger <span class="hlt">ice</span> sheet simulations and global climate change. At the present time, <span class="hlt">ice</span> fracture is not explicitly considered within <span class="hlt">ice</span> sheet models due in part to large computational costs associated with the accurate modeling of this complex phenomena. However, fracture not only plays an extremely important role in regional behavior but also influences <span class="hlt">ice</span> dynamics over much larger <span class="hlt">zones</span> in ways that are currently not well understood. Dramatic illustrations of fracture-induced phenomena most notably include the recent collapse of <span class="hlt">ice</span> shelves inmore » Antarctica (e.g. partial collapse of the Wilkins shelf in March of 2008 and the diminishing extent of the Larsen B shelf from 1998 to 2002). Other fracture examples include <span class="hlt">ice</span> calving (fracture of icebergs) which is presently approximated in simplistic ways within <span class="hlt">ice</span> sheet models, and the draining of supraglacial lakes through a complex network of cracks, a so called <span class="hlt">ice</span> sheet plumbing system, that is believed to cause accelerated <span class="hlt">ice</span> sheet flows due essentially to lubrication of the contact surface with the ground. These dramatic changes are emblematic of the ongoing change in the Earth's polar regions and highlight the important role of fracturing <span class="hlt">ice</span>. To model <span class="hlt">ice</span> fracture, a simulation capability will be designed centered around extended finite elements and solved by specialized multigrid methods on parallel computers. In addition, appropriate dynamic load balancing techniques will be employed to ensure an approximate equal amount of work for each processor.« less</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 marginal <span class="hlt">ice</span> <span class="hlt">zone</span> (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/2013AGUFM.C53B0574L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.C53B0574L"><span><span class="hlt">Ice</span> Shelf-Ocean Interactions Near <span class="hlt">Ice</span> Rises and <span class="hlt">Ice</span> Rumples</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lange, M. A.; Rückamp, M.; Kleiner, T.</p> <p>2013-12-01</p> <p>The stability of <span class="hlt">ice</span> shelves depends on the existence of embayments and is largely influenced by <span class="hlt">ice</span> rises and <span class="hlt">ice</span> rumples, which act as 'pinning-points' for <span class="hlt">ice</span> shelf movement. Of additional critical importance are interactions between <span class="hlt">ice</span> shelves and the water masses underlying them in <span class="hlt">ice</span> shelf cavities, particularly melting and refreezing processes. The present study aims to elucidate the role of <span class="hlt">ice</span> rises and <span class="hlt">ice</span> rumples in the context of climate change impacts on Antarctic <span class="hlt">ice</span> shelves. However, due to their smaller spatial extent, <span class="hlt">ice</span> rumples react more sensitively to climate change than <span class="hlt">ice</span> rises. Different forcings are at work and need to be considered separately as well as synergistically. In order to address these issues, we have decided to deal with the following three issues explicitly: oceanographic-, cryospheric and general topics. In so doing, we paid particular attention to possible interrelationships and feedbacks in a coupled <span class="hlt">ice</span>-shelf-ocean system. With regard to oceanographic issues, we have applied the ocean circulation model ROMBAX to ocean water masses adjacent to and underneath a number of idealized <span class="hlt">ice</span> shelf configurations: wide and narrow as well as laterally restrained and unrestrained <span class="hlt">ice</span> shelves. Simulations were performed with and without small <span class="hlt">ice</span> rises located close to the calving front. For larger configurations, the impact of the <span class="hlt">ice</span> rises on melt rates at the <span class="hlt">ice</span> shelf base is negligible, while for smaller configurations net melting rates at the <span class="hlt">ice</span>-shelf base differ by a factor of up to eight depending on whether <span class="hlt">ice</span> rises are considered or not. We employed the thermo-coupled <span class="hlt">ice</span> flow model TIM-FD3 to simulate the effects of several <span class="hlt">ice</span> rises and one <span class="hlt">ice</span> rumple on the dynamics of <span class="hlt">ice</span> shelf flow. We considered the complete un-grounding of the <span class="hlt">ice</span> shelf in order to investigate the effect of pinning points of different characteristics (interior or near calving front, small and medium sized) on the resulting flow and stress fields</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.ars.usda.gov/research/publications/publication/?seqNo115=307925','TEKTRAN'); return false;" href="http://www.ars.usda.gov/research/publications/publication/?seqNo115=307925"><span>Field test and sensitivity analysis of a sensible heat balance method to determine <span class="hlt">ice</span> contents</span></a></p> <p><a target="_blank" href="https://www.ars.usda.gov/research/publications/find-a-publication/">USDA-ARS?s Scientific Manuscript database</a></p> <p></p> <p></p> <p>Soil <span class="hlt">ice</span> content impacts winter vadose <span class="hlt">zone</span> hydrology. It may be possible to estimate changes in soil <span class="hlt">ice</span> content with a sensible heat balance (SHB) method, using measurements from heat pulse (HP) sensors. Feasibility of the SHB method is unknown because of difficulties in measuring soil thermal pro...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C53B1037M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C53B1037M"><span>Continuous Estimates of Surface Density and Annual Snow Accumulation with Multi-Channel Snow/Firn Penetrating Radar in the Percolation <span class="hlt">Zone</span>, Western 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>Meehan, T.; Marshall, H. P.; Bradford, J.; Hawley, R. L.; Osterberg, E. C.; McCarthy, F.; Lewis, G.; Graeter, K.</p> <p>2017-12-01</p> <p>A priority of <span class="hlt">ice</span> sheet surface mass balance (SMB) prediction is ascertaining the surface density and annual snow accumulation. These forcing data can be supplied into firn compaction models and used to tune Regional Climate Models (RCM). RCMs do not accurately capture subtle changes in the snow accumulation gradient. Additionally, leading RCMs disagree among each other and with accumulation studies in regions of the Greenland <span class="hlt">Ice</span> Sheet (GrIS) over large distances and temporal scales. RCMs tend to yield inconsistencies over GrIS because of sparse and outdated validation data in the reanalysis pool. Greenland Traverse for Accumulation and Climate Studies (GreenTrACS) implemented multi-channel 500 MHz Radar in multi-offset configuration throughout two traverse campaigns totaling greater than 3500 km along the western percolation <span class="hlt">zone</span> of GrIS. The multi-channel radar has the capability of continuously estimating snow depth, average density, and annual snow accumulation, expressed at 95% confidence (+-) 0.15 m, (+-) 17 kgm-3, (+-) 0.04 m w.e. respectively, by examination of the primary reflection return from the previous year's summer surface.</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 marginal <span class="hlt">ice</span> <span class="hlt">zone</span>. 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('https://www.ncbi.nlm.nih.gov/pubmed/28708127','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28708127"><span>An active bacterial community linked to high chl-a concentrations in 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 active throughout the winter period and thus possible future warming of sea <span class="hlt">ice</span> and consequent increase in bacterial production may lead to changes in bacteria-mediated processes in the Antarctic sea-<span class="hlt">ice</span> <span class="hlt">zone</span>.</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 marginal <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 Marginal <span class="hlt">Ice</span> <span class="hlt">Zone</span> (MIZ) and show a robust distinction of <span class="hlt">ice</span> and water.</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/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> aggregating there. As a result, much of the Southern Ocean pelagic whaling was concentrated at the edge of the marginal <span class="hlt">ice</span> <span class="hlt">zone</span>. The extent and duration of sea <span class="hlt">ice</span> fluctuate periodically under the influence of global climatic phenomena including the El Niño Southern Oscillation. Life cycles of some associated species may reflect this periodicity. With evidence for climatic warming in some regions of Antarctica, there is concern that ecosystem change may be induced by changes in sea-<span class="hlt">ice</span> extent. The relative abundance of krill and salps appears to change interannually with sea-<span class="hlt">ice</span> extent, and in warm years, when salps proliferate, krill are scarce and dependent predators suffer severely. Further research on the Southern Ocean sea-<span class="hlt">ice</span> system is required, not only to further our basic understanding of the ecology, but also to provide ecosystem managers with the information necessary for the development of strategies in response to short- and medium-term environmental changes in Antarctica. Technological advances are delivering new sampling platforms such as autonomous underwater vehicles that are improving vastly our ability to sample the Antarctic under sea-<span class="hlt">ice</span> environment. Data from such platforms will enhance greatly our understanding of the globally important Southern Ocean sea-<span class="hlt">ice</span> ecosystem.</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 marginal <span class="hlt">zone</span> 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/2016EGUGA..18.4115C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.4115C"><span>Antarctic <span class="hlt">ice</span> shelf thickness from CryoSat-2 radar altimetry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chuter, Stephen; Bamber, Jonathan</p> <p>2016-04-01</p> <p>The Antarctic <span class="hlt">ice</span> shelves provide buttressing to the inland grounded <span class="hlt">ice</span> sheet, and therefore play a controlling role in regulating <span class="hlt">ice</span> dynamics and mass imbalance. Accurate knowledge of <span class="hlt">ice</span> shelf thickness is essential for input-output method mass balance calculations, sub-<span class="hlt">ice</span> shelf ocean models and buttressing parameterisations in <span class="hlt">ice</span> sheet models. <span class="hlt">Ice</span> shelf thickness has previously been inferred from satellite altimetry elevation measurements using the assumption of hydrostatic equilibrium, as direct measurements of <span class="hlt">ice</span> thickness do not provide the spatial coverage necessary for these applications. The sensor limitations of previous radar altimeters have led to poor data coverage and a lack of accuracy, particularly the grounding <span class="hlt">zone</span> where a break in slope exists. We present a new <span class="hlt">ice</span> shelf thickness dataset using four years (2011-2014) of CryoSat-2 elevation measurements, with its SARIn dual antennae mode of operation alleviating the issues affecting previous sensors. These improvements and the dense across track spacing of the satellite has resulted in ˜92% coverage of the <span class="hlt">ice</span> shelves, with substantial improvements, for example, of over 50% across the Venable and Totten <span class="hlt">Ice</span> Shelves in comparison to the previous dataset. Significant improvements in coverage and accuracy are also seen south of 81.5° for the Ross and Filchner-Ronne <span class="hlt">Ice</span> Shelves. Validation of the surface elevation measurements, used to derive <span class="hlt">ice</span> thickness, against NASA ICESat laser altimetry data shows a mean bias of less than 1 m (equivalent to less than 9 m in <span class="hlt">ice</span> thickness) and a fourfold decrease in standard deviation in comparison to the previous continental dataset. Importantly, the most substantial improvements are found in the grounding <span class="hlt">zone</span>. Validation of the derived thickness data has been carried out using multiple Radio Echo Sounding (RES) campaigns across the continent. Over the Amery <span class="hlt">ice</span> shelf, where extensive RES measurements exist, the mean difference between the datasets is 3</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMPA31D..08N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMPA31D..08N"><span>Transnational Sea-<span class="hlt">Ice</span> Transport in a Warmer, More Mobile Arctic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Newton, R.; Tremblay, B.; Pfirman, S. L.; DeRepentigny, P.</p> <p>2015-12-01</p> <p>As the Arctic sea <span class="hlt">ice</span> thins, summer <span class="hlt">ice</span> continues to shrink in its area, and multi-year <span class="hlt">ice</span> becomes rarer, winter <span class="hlt">ice</span> is not disappearing from the Arctic Basin. Rather, it is ever more dominated by first year <span class="hlt">ice</span>. And each summer, as the total coverage withdraws, the first year <span class="hlt">ice</span> is able travel faster and farther, carrying any <span class="hlt">ice</span>-rafted material with it. Micro-organisms, sediments, pollutants and river runoff all move across the Arctic each summer and are deposited hundreds of kilometers from their origins. Analyzing Arctic sea <span class="hlt">ice</span> drift patterns in the context of the exclusive economic <span class="hlt">zones</span> (EEZs) of the Arctic nations raises concerns about the changing fate of "alien" <span class="hlt">ice</span> which forms within one country's EEZ, then drifts and melts in another country's EEZ. We have developed a new data set from satellite-based <span class="hlt">ice</span>-drift data that allows us to track groups of <span class="hlt">ice</span> "pixels" forward from their origin to their destination, or backwards from their melting location to their point of formation. The software has been integrated with model output to extend the tracking of sea <span class="hlt">ice</span> to include climate projections. Results indicate, for example, that Russian sea <span class="hlt">ice</span> dominates "imports" to the EEZ of Norway, as expected, but with increasing <span class="hlt">ice</span> mobility it is also is exported into the EEZs of other countries, including Canada and the United States. Regions of potential conflict are identified, including several national borders with extensive and/or changing transboundary sea <span class="hlt">ice</span> transport. These data are a starting point for discussion of transborder questions raised by "alien" <span class="hlt">ice</span> and the material it may import from one nation's EEZ to another's.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C41E0719G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C41E0719G"><span>Surface Melt and Firn Density Evolution in the Western Greenland Percolation <span class="hlt">Zone</span> Over the Past 50 Years</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Graeter, K.; Osterberg, E. C.; Hawley, R. L.; Thundercloud, Z. R.; Marshall, H. P.; Ferris, D. G.; Lewis, G.</p> <p>2016-12-01</p> <p>Predictions of the Greenland <span class="hlt">Ice</span> Sheet's (GIS) contribution to sea-level rise in a warming climate depend on our ability to model the surface mass balance (SMB) processes occurring across the <span class="hlt">ice</span> sheet. These processes are poorly constrained in the percolation <span class="hlt">zone</span>, the region of the <span class="hlt">ice</span> sheet where surface melt refreezes in the firn, thus preventing that melt from directly contributing to GIS mass loss. In this way, the percolation <span class="hlt">zone</span> serves as a buffer to higher temperatures increasing mass loss. However, it is unknown how the percolation <span class="hlt">zone</span> is evolving in a changing climate and to what extent the region will continue to serve as a buffer to future runoff. We collected seven shallow ( 22-30 m) firn cores from the Western Greenland percolation <span class="hlt">zone</span> in May-June 2016 as part of the Greenland Traverse for Accumulation and Climate Studies (GreenTrACS) project. Here we present data on melt layer stratigraphy, density, and annual accumulation for each core to determine: (1) the temporal and spatial accumulation and melt refreeze patterns in the percolation <span class="hlt">zone</span> of W. Greenland over the past 40 - 55 years, and (2) the impacts of changing melt and refreeze patterns on the near-surface density profile of the percolation <span class="hlt">zone</span>. Three of the GreenTrACS firn cores re-occupy firn core sites collected in the 1970's-1990's, allowing us to more accurately quantify the evolution of the percolation <span class="hlt">zone</span> surface melt and firn density during the most recent decades of summertime warming. This work is the basis for broader investigations into how changes in W. Greenland summertime climate are impacting the SMB of the Greenland <span class="hlt">Ice</span> Sheet.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040079837&hterms=ice+antarctica&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dice%2Bantarctica','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040079837&hterms=ice+antarctica&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dice%2Bantarctica"><span>Validation of EOS Aqua AMSR Sea <span class="hlt">Ice</span> Products for East Antarctica</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Massom, Rob; Lytle, Vicky; Allison, Ian; Worby, Tony; Markus, Thorsten; Scambos, Ted; Haran, Terry; Enomoto, Hiro; Tateyama, Kazu; Pfaffling, Andi</p> <p>2004-01-01</p> <p>This paper presents results from AMSR-E validation activities during a collaborative international cruise onboard the RV Aurora Australis to the East Antarctic sea <span class="hlt">ice</span> <span class="hlt">zone</span> (64-65 deg.S, 110-120 deg.E) in the early Austral spring of 2003. The validation strategy entailed an IS-day survey of the statistical characteristics of sea <span class="hlt">ice</span> and snowcover over a Lagrangian grid 100 x 50 km in size (demarcated by 9 drifting <span class="hlt">ice</span> beacons) i.e. at a scale representative of Ah4SR pixels. <span class="hlt">Ice</span> conditions ranged h m consolidated first-year <span class="hlt">ice</span> to a large polynya offshore from Casey Base. Data sets collected include: snow depth and snow-<span class="hlt">ice</span> interface temperatures on 24 (?) randomly-selected floes in grid cells within a 10 x 50 km area (using helicopters); detailed snow and <span class="hlt">ice</span> measurements at 13 dedicated <span class="hlt">ice</span> stations, one of which lasted for 4 days; time-series measurements of snow temperature and thickness at selected sites; 8 aerial photography and thermal-IR radiometer flights; other satellite products (SAR, AVHRR, MODIS, MISR, ASTER and Envisat MERIS); <span class="hlt">ice</span> drift data; and ancillary meteorological (ship-based, meteorological buoys, twice-daily radiosondes). These data are applied to a validation of standard AMSR-E <span class="hlt">ice</span> concentration, snowcover thickness and <span class="hlt">ice</span>-temperature products. In addition, a validation is carried out of <span class="hlt">ice</span>-surface skin temperature products h m the NOAA AVHRR and EOS MODIS datasets.</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 marginal <span class="hlt">ice</span> <span class="hlt">zone</span>, 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> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.C51B0477B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.C51B0477B"><span>Surface mass balance of Greenland mountain glaciers and <span class="hlt">ice</span> caps</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Benson, R. J.; Box, J. E.; Bromwich, D. H.; Wahr, J. M.</p> <p>2009-12-01</p> <p>Mountain glaciers and <span class="hlt">ice</span> caps contribute roughly half of eustatic sea-level rise. Greenland has thousands of small mountain glaciers and several <span class="hlt">ice</span> caps > 1000 sq. km that have not been included in previous mass balance calculations. To include small glaciers and <span class="hlt">ice</span> caps in our study, we use Polar WRF, a next-generation regional climate data assimilation model is run at grid resolution less than 10 km. WRF provides surface mass balance data at sufficiently high resolution to resolve not only the narrow <span class="hlt">ice</span> sheet ablation <span class="hlt">zone</span>, but provides information useful in downscaling melt and accumulation rates on mountain glaciers and <span class="hlt">ice</span> caps. In this study, we refine Polar WRF to simulate a realistic surface energy budget. Surface melting is calculated in-line from surface energy budget closure. Blowing snow sublimation is computed in-line. Melt water re-freeze is calculated using a revised scheme. Our results are compared with NASA's Gravity Recovery and Climate Experiment (GRACE) and associated error is calculated on a regional and local scale with validation from automated weather stations (AWS), snow pits and <span class="hlt">ice</span> core data from various regions along the Greenland <span class="hlt">ice</span> sheet.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1010890','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1010890"><span>Modeling Relevant to Safe Operations of U.S. Navy Vessels in Arctic Conditions: Physical Modeling of <span class="hlt">Ice</span> Loads</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><span class="hlt">zones</span> with <span class="hlt">ice</span> concentrations up to 40%. To achieve this goal, the Navy must determine safe operational speeds as a function of <span class="hlt">ice</span> concen- tration...and full-scale experience with <span class="hlt">ice</span>-capable hull forms that have shallow entry angles to promote flexural <span class="hlt">ice</span> failure preferentially over crushing...plan view) of the proposed large-scale ice–hull impact experiment to be conducted in CRREL’s refrigerated towing basin. Shown here is a side-panel</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 marginal <span class="hlt">ice</span> <span class="hlt">zone</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16..324M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16..324M"><span>Disintegration of a marine-based <span class="hlt">ice</span> stream - evidence from the Norwegian Channel, north-eastern North Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Morén, Björn M.; Petter Sejrup, Hans; Hjelstuen, Berit O.; Haflidason, Haflidi; Schäuble, Cathrina; Borge, Marianne</p> <p>2014-05-01</p> <p>The Norwegian Channel <span class="hlt">Ice</span> Stream repeatedly drained large part of the Fennoscandian <span class="hlt">Ice</span> Sheet through Mid and Late Pleistocene glacial stages. During parts of Marine Isotope Stages 2 and 3, glacial <span class="hlt">ice</span> from Fennoscandia and the British Isles coalesced in the central North Sea and the Norwegian Channel <span class="hlt">Ice</span> Stream reached the shelf edge on multiple occasions. Through the last decades a large amount of acoustic and sediment core data have been collected from the Norwegian Channel, providing a good background for studies focussing on stability- and development-controlling parameters for marine-based <span class="hlt">ice</span> streams, the retreat rate of the Norwegian Channel <span class="hlt">Ice</span> Stream, and the behaviour of the Fennoscandian <span class="hlt">Ice</span> Sheet. Further, this improved understanding can be used to develop more accurate numerical climate models and models which can be used to model <span class="hlt">ice</span>-sheet behaviour of the past as well as the future. This study presents new acoustic records and data from sediment cores which contribute to a better understanding of the retreat pattern and the retreat rate of the last <span class="hlt">ice</span> stream that occupied the Norwegian Channel. From bathymetric and TOPAS seismic data, mega-scale glacial lineations, grounding-<span class="hlt">zone</span> wedges, and end moraines have been mapped, thereby allowing us to reconstruct the pro- and subglacial conditions at the time of the creation of these landforms. It is concluded that the whole Norwegian Channel was deglaciated in just over 1 000 years and that for most of this time the <span class="hlt">ice</span> margin was located at positions reflected by depositional grounding-<span class="hlt">zone</span> wedges. Further work will explore the influence of channel shape and feeding of <span class="hlt">ice</span> from western Norwegian fjords on this retreat pattern through numerical modelling.</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 margins, 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 <span class="hlt">zone</span>; 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/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, marginal sea <span class="hlt">ice</span> <span class="hlt">zone</span> 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('http://adsabs.harvard.edu/abs/2017EGUGA..1919527R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1919527R"><span>Variability of the volume and thickness of sea <span class="hlt">ice</span> in the Bay of Bothnia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ronkainen, Iina; Lehtiranta, Jonni; Lensu, Mikko; Rinne, Eero; Hordoir, Robinson; Haapala, Jari</p> <p>2017-04-01</p> <p>Variability of the volume and thickness of sea <span class="hlt">ice</span> in the Bay of Bothnia In our study, we want to quantify the variability of sea <span class="hlt">ice</span> volume and thickness in the Bay of Bothnia and to introduce the drivers of the observed variability. There has been similar studies, but only for fast <span class="hlt">ice</span>. We use various different data sets: in-situ <span class="hlt">ice</span> thickness data, remote sensing data, model data and <span class="hlt">ice</span> charts. In-situ data is from the regular monitoring stations in the coastal fast <span class="hlt">ice</span> <span class="hlt">zone</span> and from field campaigns. The remote sensing data is helicopter-borne and ship-borne electromagnetic data. The models we use are HELMI and NEMO-Nordic. We analyze the different data sets and compare them to each other to solve the inter-annual variability and to discuss the ratio of level and deformed <span class="hlt">ice</span>.</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 Marginal <span class="hlt">Ice</span> <span class="hlt">Zone</span> 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('http://adsabs.harvard.edu/abs/2016AGUFM.C53A0693M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C53A0693M"><span>Multi-channel <span class="hlt">Ice</span> Penetrating Radar Traverse for Estimates of Firn Density in the Percolation <span class="hlt">Zone</span>, Western 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>Meehan, T.; Osterberg, E. C.; Lewis, G.; Overly, T. B.; Hawley, R. L.; Bradford, J.; Marshall, H. P.</p> <p>2016-12-01</p> <p>To better predict the response of the Greenland <span class="hlt">Ice</span> Sheet (GrIS) to future warming, leading edge Regional Climate Models (RCM) must be calibrated with in situ measurements of recent accumulation and melt. Mass balance estimates averaged across the entire Greenland <span class="hlt">Ice</span> Sheet (GrIS) vary between models by more than 30 percent, and regional comparisons of mass balance reconstructions in Greenland vary by 100 percent or more. Greenland Traverse for Accumulation and Climate Studies (GreenTrACS) is a multi-year and multi-disciplinary 1700 km science traverse from Raven/Dye2 in SW Greenland, to Summit Station. Multi-offset radar measurements can provide high accuracy electromagnetic (EM) velocity estimates of the firn to within (+-) 0.002 to 0.003 m/ns. EM velocity, in turn, can be used to estimate bulk firn density. Using a mixing equation such as the CRIM Equation we use the measured EM velocity, along with the known EM velocity in air and <span class="hlt">ice</span>, to estimate bulk density. During spring 2016, we used multi-channel 500MHz radar in a multi-offset configuration to survey more than 800 km from Raven towards summit. Preliminary radar-derived snow density estimates agree with density estimates from a firn core measurement ( 50 kg/m3), despite the lateral heterogeneity of the firn across the length of the antenna array (12 m).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C41B1213T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C41B1213T"><span>Ultra-Wideband Radiometry Remote Sensing of Polar <span class="hlt">Ice</span> Sheet Temperature Profile, Sea <span class="hlt">Ice</span> and Terrestrial Snow Thickness: Forward Modeling and Data Analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tsang, L.; Tan, S.; Sanamzadeh, M.; Johnson, J. T.; Jezek, K. C.; Durand, M. T.</p> <p>2017-12-01</p> <p>The recent development of an ultra-wideband software defined radiometer (UWBRAD) operating over the unprotected spectrum of 0.5 2.0 GHz using radio-frequency interference suppression techniques offers new methodologies for remote sensing of the polar <span class="hlt">ice</span> sheets, sea <span class="hlt">ice</span>, and terrestrial snow. The instrument was initially designed for remote sensing of the intragalcial temperature profile of the <span class="hlt">ice</span> sheet, where a frequency dependent penetration depth yields a frequency dependent brightness temperature (Tb) spectrum that can be linked back to the temperature profile of the <span class="hlt">ice</span> sheet. The instrument was tested during a short flight over Northwest Greenland in September, 2016. Measurements were successfully made over the different snow facies characteristic of Greenland including the ablation, wet snow and percolation facies, and ended just west of Camp Century during the approach to the dry snow <span class="hlt">zone</span>. Wide-band emission spectra collected during the flight have been processed and analyzed. Results show that the spectra are highly sensitive to the facies type with scattering from <span class="hlt">ice</span> lenses being the dominant reason for low Tbs in the percolation <span class="hlt">zone</span>. Inversion of Tb to physical temperature at depth was conducted on the measurements near Camp Century, achieving a -1.7K ten-meter error compared to borehole measurements. However, there is a relatively large uncertainty in the lower part possibly due to the large scattering near the surface. Wideband radiometry may also be applicable to sea <span class="hlt">ice</span> and terrestrial snow thickness retrieval. Modeling studies suggest that the UWBRAD spectra reduce ambiguities inherent in other sea <span class="hlt">ice</span> thickness retrievals by utilizing coherent wave interferences that appear in the Tb spectrum. When applied to a lossless medium such as terrestrial snow, this coherent oscillation turns out to be the single key signature that can be used to link back to snow thickness. In this paper, we report our forward modeling findings in support of instrument</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>Active microwave measurements were made of various sea <span class="hlt">ice</span> forms in March and April 1987 during the Marginal <span class="hlt">Ice</span> <span class="hlt">Zone</span> 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('http://adsabs.harvard.edu/abs/2017Icar..297..160F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Icar..297..160F"><span>Inhibition of ordinary and diffusive convection in the water condensation <span class="hlt">zone</span> of the <span class="hlt">ice</span> giants and implications for their thermal evolution</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Friedson, A. James; Gonzales, Erica J.</p> <p>2017-11-01</p> <p>We explore the conditions under which ordinary and double-diffusive thermal convection may be inhibited by water condensation in the hydrogen atmospheres of the <span class="hlt">ice</span> giants and examine the consequences. The saturation of vapor in the condensation layer induces a vertical gradient in the mean molecular weight that stabilizes the layer against convective instability when the abundance of vapor exceeds a critical value. In this instance, the layer temperature gradient can become superadiabatic and heat must be transported vertically by another mechanism. On Uranus and Neptune, water is inferred to be sufficiently abundant for inhibition of ordinary convection to take place in their respective condensation <span class="hlt">zones</span>. We find that suppression of double-diffusive convection is sensitive to the ratio of the sedimentation time scale of the condensates to the buoyancy period in the condensation layer. In the limit of rapid sedimentation, the layer is found to be stable to diffusive convection. In the opposite limit, diffusive convection can occur. However, if the fluid remains saturated, then layered convection is generally suppressed and the motion is restricted in form to weak, homogeneous, oscillatory turbulence. This form of diffusive convection is a relatively inefficient mechanism for transporting heat, characterized by low Nusselt numbers. When both ordinary and layered convection are suppressed, the condensation <span class="hlt">zone</span> acts effectively as a thermal insulator, with the heat flux transported across it only slightly greater than the small value that can be supported by radiative diffusion. This may allow a large superadiabatic temperature gradient to develop in the layer over time. Once the layer has formed, however, it is vulnerable to persistent erosion by entrainment of fluid into the overlying convective envelope of the cooling planet, potentially leading to its collapse. We discuss the implications of our results for thermal evolution models of the <span class="hlt">ice</span> giants, for</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C24C..06F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C24C..06F"><span>Optical Benson: Following the Impact of Melt Season Progression Using Landsat and Sentinel 2 - Snow <span class="hlt">Zone</span> Formation Imaged</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fahnestock, M. A.; Shuman, C. A.; Alley, K. E.</p> <p>2017-12-01</p> <p>Snow pit observations on a glaciologically-focussed surface traverse in Greenland allowed Benson [1962, SIPRE (now CRREL) Research Report 70] to define a series of snow <span class="hlt">zones</span> based on the extent of post-depositional diagenesis of the snowpack. At high elevations, Benson found fine-grained "dry snow" where melt (at that time) was absent year-round, followed down-elevation by a "percolation <span class="hlt">zone</span>" where surface melt penetrated the snowpack, then a "wet snow <span class="hlt">zone</span>" where firn became saturated during the peak of the melt season, and finally "superimposed <span class="hlt">ice</span>" and "bare <span class="hlt">ice</span>" <span class="hlt">zones</span> where refrozen surface melt and glacier <span class="hlt">ice</span> were exposed in the melt season. These snow <span class="hlt">zones</span> can be discriminated in winter synthetic aperture radar (SAR) imagery of the <span class="hlt">ice</span> sheet (e.g. Fahnestock et al. 2001), but summer melt reduces radar backscatter and makes it difficult to follow the progression of diagenesis beyond the initial indications of surface melting. While some of the impacts of surface melt (especially bands of blue water-saturated firn) are observed from time to time in optical satellite imagery, it has only become possible to map effects of melt over the course of a summer season with the advent of large-data analysis tools such as Google Earth Engine and the inclusion of Landsat and Sentinel-2 data streams in these tools. A map of the maximum extent of this blue saturated <span class="hlt">zone</span> through the 2016 melt season is shown in the figure. This image is a true color (RGB) composite, but each pixel in the image shows the color of the surface when the "blueness" of the pixel was at a maximum. This means each pixel can be from a different satellite image acquisition than adjacent pixels - but it also means that the maximum extent of the saturated firn (Benson's wet snow <span class="hlt">zone</span>) is visible. Also visible are percolation, superimposed and bare <span class="hlt">ice</span> <span class="hlt">zones</span>. This analysis, using Landsat 8 Operational Land Imager data, was performed using Google Earth Engine to access and analyze the entire melt</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('http://adsabs.harvard.edu/abs/2017AGUFM.A22E..01H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A22E..01H"><span>On The Importance of Connecting Laboratory Measurements of <span class="hlt">Ice</span> Crystal Growth with Model Parameterizations: Predicting <span class="hlt">Ice</span> Particle Properties</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Harrington, J. Y.</p> <p>2017-12-01</p> <p> lines show a substantial influence to predicted particle properties: The more natural evolution of <span class="hlt">ice</span> crystals during riming produces graupel-like particles with size and fall-speeds required for the formation of a classic transition <span class="hlt">zone</span> and extended stratiform precipitation region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1911372D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1911372D"><span>Towards multi-decadal to multi-millennial <span class="hlt">ice</span> core records from coastal west Greenland <span class="hlt">ice</span> caps</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Das, Sarah B.; Osman, Matthew B.; Trusel, Luke D.; McConnell, Joseph R.; Smith, Ben E.; Evans, Matthew J.; Frey, Karen E.; Arienzo, Monica; Chellman, Nathan</p> <p>2017-04-01</p> <p>The Arctic region, and Greenland in particular, is undergoing dramatic change as characterized by atmospheric warming, decreasing sea <span class="hlt">ice</span>, shifting ocean circulation patterns, and rapid <span class="hlt">ice</span> sheet mass loss, but longer records are needed to put these changes into context. <span class="hlt">Ice</span> core records from the Greenland <span class="hlt">ice</span> sheet have yielded invaluable insight into past climate change both regionally and globally, and provided important constraints on past surface mass balance more directly, but these <span class="hlt">ice</span> cores are most often from the interior <span class="hlt">ice</span> sheet accumulation <span class="hlt">zone</span>, at high altitude and hundreds of kilometers from the coast. Coastal <span class="hlt">ice</span> caps, situated around the margins of Greenland, have the potential to provide novel high-resolution records of local and regional maritime climate and sea surface conditions, as well as contemporaneous glaciological changes (such as accumulation and surface melt history). But obtaining these records is extremely challenging. Most of these <span class="hlt">ice</span> caps are unexplored, and thus their thickness, age, stratigraphy, and utility as sites of new and unique paleoclimate records is largely unknown. Access is severely limited due to their high altitude, steep relief, small surface area, and inclement weather. Furthermore, their relatively low elevation and marine moderated climate can contribute to significant surface melting and degradation of the <span class="hlt">ice</span> stratigraphy. We recently targeted areas near the Disko Bay region of central west Greenland where maritime <span class="hlt">ice</span> caps are prevalent but unsampled, as potential sites for new multi-decadal to multi-millennial <span class="hlt">ice</span> core records. In 2014 & 2015 we identified two promising <span class="hlt">ice</span> caps, one on Disko Island (1250 m. asl) and one on Nuussuaq Peninsula (1980 m. asl) based on airborne and ground-based geophysical observations and physical and glaciochemical stratigraphy from shallow firn cores. In spring 2015 we collected <span class="hlt">ice</span> cores at both sites using the Badger-Eclipse electromechanical drill, transported by a medley</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26339489','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26339489"><span><span class="hlt">Ice</span> swimming - '<span class="hlt">Ice</span> Mile' and '1 km <span class="hlt">Ice</span> event'.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Knechtle, Beat; Rosemann, Thomas; Rüst, Christoph A</p> <p>2015-01-01</p> <p><span class="hlt">Ice</span> swimming for 1 mile and 1 km is a new discipline in open-water swimming since 2009. This study examined female and male performances in swimming 1 mile ('<span class="hlt">Ice</span> Mile') and 1 km ('1 km <span class="hlt">Ice</span> event') in water of 5 °C or colder between 2009 and 2015 with the hypothesis that women would be faster than men. Between 2009 and 2015, 113 men and 38 women completed one '<span class="hlt">Ice</span> Mile' and 26 men and 13 completed one '1 km <span class="hlt">Ice</span> event' in water colder than +5 °C following the rules of International <span class="hlt">Ice</span> Swimming Association (IISA). Differences in performance between women and men were determined. Sex difference (%) was calculated using the equation ([time for women] - [time for men]/[time for men] × 100). For '<span class="hlt">Ice</span> Mile', a mixed-effects regression model with interaction analyses was used to investigate the influence of sex and environmental conditions on swimming speed. The association between water temperature and swimming speed was assessed using Pearson correlation analyses. For '<span class="hlt">Ice</span> Mile' and '1 km <span class="hlt">Ice</span> event', the best men were faster than the best women. In '<span class="hlt">Ice</span> Mile', calendar year, number of attempts, water temperature and wind chill showed no association with swimming speed for both women and men. For both women and men, water temperature was not correlated to swimming speed in both '<span class="hlt">Ice</span> Mile' and '1 km <span class="hlt">Ice</span> event'. In water colder than 5 °C, men were faster than women in '<span class="hlt">Ice</span> Mile' and '1 km <span class="hlt">Ice</span> event'. Water temperature showed no correlation to swimming speed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..1511771L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..1511771L"><span>The northern Uummannaq <span class="hlt">Ice</span> Stream System, West Greenland: <span class="hlt">ice</span> dynamics and and controls upon deglaciation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lane, Timothy; Roberts, David; Rea, Brice; Cofaigh, Colm Ó.; Vieli, Andreas</p> <p>2013-04-01</p> <p>At the Last Glacial Maximum (LGM), the Uummannaq <span class="hlt">Ice</span> 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 <span class="hlt">Ice</span> Sheet. Geomorphological mapping, terrestrial cosmogenic nuclide (TCN) exposure dating, and radiocarbon dating constrain warm-based <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> flow, forcing it south through Igdlorssuit Sund, and into the Uummannaq Trough. Here it coalesced with <span class="hlt">ice</span> from the south, forming the trunk <span class="hlt">zone</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..1113700S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..1113700S"><span>Nature and History of Cenozoic Polar <span class="hlt">Ice</span> Covers: The Case 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>Spielhagen, R.; Thiede, J.</p> <p>2009-04-01</p> <p>The nature of the modern climate System is characterized by steep temperature gradients between the tropical and polar climatic <span class="hlt">zones</span> and finds its most spectacular expression in the formation of <span class="hlt">ice</span> caps in high Northern and Southern latitudes. While polar regions of Planet Earth have been glaciated repeatedly in the long course of their geological history, the Cenozoic transition from a „greenhouse" to an „icehouse" has in fact produced a unique climatic scenario with bipolar glacation, different from all previous glacial events. The Greenland <span class="hlt">ice</span> sheet is a remainder of the Northern Hemisphere last glacial maximum <span class="hlt">ice</span> sheets and represents hence a spectacular anomaly. Geological records from Tertiary and Quaternary terrestrial and oceanic sections have documented the presence of <span class="hlt">ice</span> caps and sea <span class="hlt">ice</span> covers both on the Southern as well on the Northern hemisphere since Eocene times, aqpprox. 45 Mio. years ago. While this was well known in the case of Antarctica already for some time, previous ideas about the origin of Northern hemisphere glaciation during Pliocene times (approx. 2-3 Mio. years ago) have been superceded by the dramatic findings of coarse, terrigenous <span class="hlt">ice</span> rafted detritus in Eocene sediments from Lomonosov Ridge (close to the North Pole) apparently slightly older than the oldest Antarctic records of <span class="hlt">ice</span> rafting.The histories of the onset of Cenozoic glaciation in high Northern and Southern latitudes remain enigmatic and are presently subjects of international geological drilling projects, with prospects to reveal some of their secrets over the coming decades. By virtue of the physical porperties of <span class="hlt">ice</span> and the processes controlling the dynamics of the turn-over of the <span class="hlt">ice</span>-sheets only young records of glacial <span class="hlt">ice</span> caps on Antarctica and on Greemnland have been preserved, on Greenland with <span class="hlt">ice</span> probably not older than a few hundred thousand years, on Antarctica potentially as old as 1.5-2 Mio. years. Deep-sea cores with their records od <span class="hlt">ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-200910220008HQ.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-200910220008HQ.html"><span><span class="hlt">Ice</span> Bridge Antarctic Sea <span class="hlt">Ice</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2009-10-21</p> <p>Sea <span class="hlt">ice</span> is seen out the window of NASA's DC-8 research aircraft as it flies 2,000 feet above the Bellingshausen Sea in West Antarctica on Wednesday, Oct., 21, 2009. This was the fourth science flight of NASA’s Operation <span class="hlt">Ice</span> Bridge airborne Earth science mission to study Antarctic <span class="hlt">ice</span> sheets, sea <span class="hlt">ice</span>, and <span class="hlt">ice</span> shelves. Photo Credit: (NASA/Jane Peterson)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014TCry....8.1469R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014TCry....8.1469R"><span>Temporal dynamics of ikaite in experimental 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>Rysgaard, S.; Wang, F.; Galley, R. J.; Grimm, R.; Notz, D.; Lemes, M.; Geilfus, N.-X.; Chaulk, A.; Hare, A. A.; Crabeck, O.; Else, B. G. T.; Campbell, K.; Sørensen, L. L.; Sievers, J.; Papakyriakou, T.</p> <p>2014-08-01</p> <p>Ikaite (CaCO3 · 6H2O) is a metastable phase of calcium carbonate that normally forms in a cold environment and/or under high pressure. Recently, ikaite crystals have been found in sea <span class="hlt">ice</span>, and it has been suggested that their precipitation may play an important role in air-sea CO2 exchange in <span class="hlt">ice</span>-covered seas. Little is known, however, of the spatial and temporal dynamics of ikaite in sea <span class="hlt">ice</span>. Here we present evidence for highly dynamic ikaite precipitation and dissolution in sea <span class="hlt">ice</span> grown at an outdoor pool of the Sea-<span class="hlt">ice</span> Environmental Research Facility (SERF) in Manitoba, Canada. During the experiment, ikaite precipitated in sea <span class="hlt">ice</span> when temperatures were below -4 °C, creating three distinct <span class="hlt">zones</span> of ikaite concentrations: (1) a millimeter-to-centimeter-thin surface layer containing frost flowers and brine skim with bulk ikaite concentrations of >2000 μmol kg-1, (2) an internal layer with ikaite concentrations of 200-400 μmol kg-1, and (3) a bottom layer with ikaite concentrations of <100 μmol kg-1. Snowfall events caused the sea <span class="hlt">ice</span> to warm and ikaite crystals to dissolve. Manual removal of the snow cover allowed the sea <span class="hlt">ice</span> to cool and brine salinities to increase, resulting in rapid ikaite precipitation. The observed ikaite concentrations were on the same order of magnitude as modeled by FREZCHEM, which further supports the notion that ikaite concentration in sea <span class="hlt">ice</span> increases with decreasing temperature. Thus, varying snow conditions may play a key role in ikaite precipitation and dissolution in sea <span class="hlt">ice</span>. This could have a major implication for CO2 exchange with the atmosphere and ocean that has not been accounted for previously.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EaFut...5..633N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EaFut...5..633N"><span>Increasing transnational sea-<span class="hlt">ice</span> exchange in a changing 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>Newton, Robert; Pfirman, Stephanie; Tremblay, Bruno; DeRepentigny, Patricia</p> <p>2017-06-01</p> <p>The changing Arctic sea-<span class="hlt">ice</span> cover is likely to impact the trans-border exchange of sea <span class="hlt">ice</span> between the exclusive economic <span class="hlt">zones</span> (EEZs) of the Arctic nations, affecting the risk of <span class="hlt">ice</span>-rafted contamination. We apply the Lagrangian <span class="hlt">Ice</span> Tracking System (LITS) to identify sea-<span class="hlt">ice</span> formation events and track sea <span class="hlt">ice</span> to its melt locations. Most <span class="hlt">ice</span> (52%) melts within 100 km of where it is formed; ca. 21% escapes from its EEZ. Thus, most contaminants will be released within an <span class="hlt">ice</span> parcel's originating EEZ, while material carried by over 1 00,000 km2 of ice—an area larger than France and Germany combined—will be released to other nations' waters. Between the periods 1988-1999 and 2000-2014, sea-<span class="hlt">ice</span> formation increased by ˜17% (roughly 6 million km2 vs. 5 million km2 annually). Melting peaks earlier; freeze-up begins later; and the central Arctic Ocean is more prominent in both formation and melt in the later period. The total area of <span class="hlt">ice</span> transported between EEZs increased, while transit times decreased: for example, Russian <span class="hlt">ice</span> reached melt locations in other nations' EEZs an average of 46% faster while North American <span class="hlt">ice</span> reached destinations in Eurasian waters an average of 37% faster. Increased trans-border exchange is mainly a result of increased speed (˜14% per decade), allowing first-year <span class="hlt">ice</span> to escape the summer melt front, even as the front extends further north. Increased trans-border exchange over shorter times is bringing the EEZs of the Arctic nations closer together, which should be taken into account in policy development—including establishment of marine-protected areas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16..634C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16..634C"><span>A laboratory experiment assessing the effect of sea <span class="hlt">ice</span> on wave dumping</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cavaliere, Claudio; Alberello, Alberto; Bennetts, Luke; Meylan, Mike; Babanin, Alexander; Malavasi, Stefano; Toffoli, Alessandro</p> <p>2014-05-01</p> <p>Wave-<span class="hlt">ice</span> interaction is a critical factor in the dynamics of the marginal <span class="hlt">ice</span> <span class="hlt">zone</span> (MIZ), the region between open ocean and an expanse of <span class="hlt">ice</span> floes of varying size and shape. This interaction works both ways: while waves cause the fractures of <span class="hlt">ice</span> floes, the presence of <span class="hlt">ice</span> floes affects waves through scattering and various dissipative processes. In order to assess the latter, a laboratory experiment has been carried out in the coastal directional basin at Plymouth University. Sea <span class="hlt">ice</span> has been simulated with two deformable plates: 1mX1m plastic sheet with variable thickness of polypropylene, which holds the same density (~0.9 g/cm3) of <span class="hlt">ice</span>, and PVC Forex, which hold the same mechanical property of <span class="hlt">ice</span>. Experiments have been conducted using monochromatic as well as random wave fields with different steepness and wavelengths (both shorter and larger than the floe). The wave field has been monitored before and after the simulated <span class="hlt">ice</span> floe with a number of wave probes deployed along the basin, including a 6-probe array to track directional properties. On the whole, results show a substantial scattering and dissipation of the wave field, which appears to be dependent on the amount of overwash on the <span class="hlt">ice</span> floe.</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-<span class="hlt">zone</span> wedges, iceberg scours, and a lateral shear margin 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 margin 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/2016QSRv..140..101P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016QSRv..140..101P"><span>Sedimentology and chronology of the advance and retreat of the last British-Irish <span class="hlt">Ice</span> Sheet on the continental shelf west of Ireland</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 L.; Benetti, Sara; Dunlop, Paul; Ó Cofaigh, Colm; Moreton, Steven G.; Wheeler, Andrew J.; Clark, Christopher D.</p> <p>2016-05-01</p> <p>The last British-Irish <span class="hlt">Ice</span> Sheet (BIIS) had extensive marine-terminating margins and was drained by multiple large <span class="hlt">ice</span> streams and is thus a useful analogue for marine-based areas of modern <span class="hlt">ice</span> sheets. However, despite recent advances from investigating the offshore record of the BIIS, the dynamic history of its marine margins, which would have been sensitive to external forcing(s), remain inadequately understood. This study is the first reconstruction of the retreat dynamics and chronology of the western, marine-terminating, margin of the last (Late Midlandian) BIIS. Analyses of shelf geomorphology and core sedimentology and chronology enable a reconstruction of the Late Midlandian history of the BIIS west of Ireland, from initial advance to final retreat onshore. Five AMS radiocarbon dates from marine cores constrain the timing of retreat and associated readvances during deglaciation. The BIIS advanced without streaming or surging, depositing a bed of highly consolidated subglacial traction till, and reached to within ∼20 km of the shelf break by ∼24,000 Cal BP. <span class="hlt">Ice</span> margin retreat was likely preceded by thinning, grounding <span class="hlt">zone</span> retreat and <span class="hlt">ice</span> shelf formation on the outer shelf by ∼22,000 Cal BP. This <span class="hlt">ice</span> shelf persisted for ≤2500 years, while retreating at a minimum rate of ∼24 m/yr and buttressing a >150-km long, 20-km wide, bathymetrically-controlled grounding <span class="hlt">zone</span>. A large (∼150 km long), arcuate, flat-topped grounding-<span class="hlt">zone</span> wedge, termed here the Galway Lobe Grounding-<span class="hlt">Zone</span> Wedge (GLGZW), was deposited below this <span class="hlt">ice</span> shelf and records a significant stillstand in BIIS retreat. Geomorphic relationships indicate that the BIIS experienced continued thinning during its retreat across the shelf, which led to increased topographic influence on its flow dynamics following <span class="hlt">ice</span> shelf break up and grounding <span class="hlt">zone</span> retreat past the GLGZW. At this stage of retreat the western BIIS was comprised of several discrete, asynchronous lobes that underwent several</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.1637W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.1637W"><span>Increased future <span class="hlt">ice</span> discharge from Antarctica owing to higher snowfall</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Winkelmann, Ricarda; Levermann, Anders; Martin, Maria A.; Frieler, Katja</p> <p>2013-04-01</p> <p>Anthropogenic climate change is likely to cause continuing global sea-level rise, but some processes within the Earth system may mitigate the magnitude of the projected effect. Regional and global climate models simulate enhanced snowfall over Antarctica, which would provide a direct offset of the future contribution to global sea level rise from cryospheric mass loss and ocean expansion. Uncertainties exist in modelled snowfall, but even larger uncertainties exist in the potential changes of dynamic <span class="hlt">ice</span> discharge from Antarctica. Here we show that snowfall and discharge are not independent, but that future <span class="hlt">ice</span> discharge will increase by up to three times as a result of additional snowfall under global warming. Our results, based on an <span class="hlt">ice</span>-sheet model forced by climate simulations through to the end of 2500, show that the enhanced discharge effect exceeds the effect of surface warming as well as that of basal <span class="hlt">ice</span>-shelf melting, and is due to the difference in surface elevation change caused by snowfall on grounded versus floating <span class="hlt">ice</span>. Although different underlying forcings drive <span class="hlt">ice</span> loss from basal melting versus increased snowfall, similar <span class="hlt">ice</span> dynamical processes are nonetheless at work in both; therefore results are relatively independent of the specific representation of the transition <span class="hlt">zone</span>. In an ensemble of simulations designed to capture <span class="hlt">ice</span>-physics uncertainty, the additional dynamic <span class="hlt">ice</span> loss along the coastline compensates between 30 and 65 per cent of the <span class="hlt">ice</span> gain due to enhanced snowfall over the entire continent. This results in a dynamic <span class="hlt">ice</span> loss of up to 1.25 metres in the year 2500 for the strongest warming scenario.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=PIA04933&hterms=Age+earth&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DAge%2Bearth','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=PIA04933&hterms=Age+earth&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DAge%2Bearth"><span>Mars <span class="hlt">Ice</span> Age, Simulated</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>2003-01-01</p> <p><p/>December 17, 2003<p/>This simulated view shows Mars as it might have appeared during the height of a possible <span class="hlt">ice</span> age in geologically recent time.<p/>Of all Solar System planets, Mars has the climate most like that of Earth. Both are sensitive to small changes in orbit and tilt. During a period about 2.1 million to 400,000 years ago, increased tilt of Mars' rotational axis caused increased solar heating at the poles. A new study using observations from NASA's Mars Global Surveyor and Mars Odyssey orbiters concludes that this polar warming caused mobilization of water vapor and dust into the atmosphere, and buildup of a surface deposit of <span class="hlt">ice</span> and dust down to about 30 degrees latitude in both hemispheres. That is the equivalent of the southern Unites States or Saudi Arabia on Earth. Mars has been in an interglacial period characterized by less axial tilt for about the last 300,000 years. The <span class="hlt">ice</span>-rich surface deposit has been degrading in the latitude <span class="hlt">zone</span> of 30 degrees to 60 degrees as water-<span class="hlt">ice</span> returns to the poles.<p/>In this illustration prepared for the December 18, 2003, cover of the journal Nature, the simulated surface deposit is superposed on a topography map based on altitude measurements by Global Surveyor and images from NASA's Viking orbiters of the 1970s.<p/>Mars Global Surveyor and Mars Odyssey are managed by NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology, Pasadena, for the NASA Office of Space Science, Washington.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.C13E0656L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.C13E0656L"><span>Long-Endurance, <span class="hlt">Ice</span>-capable Autonomous Seagliders</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lee, C. M.; Gobat, J. I.; Shilling, G.; Curry, B.</p> <p>2012-12-01</p> <p>. The first successful section across the <span class="hlt">ice</span>-covered Davis Strait occurred in 2006, while the first full mission took place September - February 2008. Mission duration was 25 weeks, with over 800 km of under-<span class="hlt">ice</span> transit over 51 days. The glider was able to identify and surface through leads 10 times during under-<span class="hlt">ice</span> operations. Most recently, a pair of successful missions collected continuous sections across Davis Strait from October 2010 through June 2011, including operations between January and June, when the strait was nearly entirely <span class="hlt">ice</span>-covered and the glider rarely gained access to the surface. These missions provide the first year-round time series of high-resolution sections across Davis Strait. In the Antarctic, <span class="hlt">ice</span>-capable Seagliders successfully transited beneath a 40-km <span class="hlt">ice</span> bridge and self-extracted after being carried beneath the Ross <span class="hlt">ice</span> shelf during missions conducted without the support of an acoustic navigation array. <span class="hlt">Ice</span>-capable Seagliders can provide sustainable, continuous occupation of critical sections in <span class="hlt">ice</span>-covered regions, including the marginal <span class="hlt">ice</span> <span class="hlt">zone</span>, with typical horizontal resolution of 3 km and routine sampling of the important, but hazardous, region near the <span class="hlt">ice</span>-ocean interface. Future directions include development of basin-scale acoustic navigation ('underwater GPS' for the Arctic) and use of existing high-frequency acoustic communications for short-range data transfer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.3986L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.3986L"><span>Long-Endurance, <span class="hlt">Ice</span>-capable Autonomous Seagliders</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lee, Craig; Gobat, Jason; Shilling, Geoff; Curry, Beth</p> <p>2013-04-01</p> <p>. The first successful section across the <span class="hlt">ice</span>-covered Davis Strait occurred in 2006, while the first full mission took place September - February 2008. Mission duration was 25 weeks, with over 800 km of under-<span class="hlt">ice</span> transit over 51 days. The glider was able to identify and surface through leads 10 times during under-<span class="hlt">ice</span> operations. Most recently, a pair of successful missions collected continuous sections across Davis Strait from October 2010 through June 2011, including operations between January and June, when the strait was nearly entirely <span class="hlt">ice</span>-covered and the glider rarely gained access to the surface. These missions provide the first year-round time series of high-resolution sections across Davis Strait. In the Antarctic, <span class="hlt">ice</span>-capable Seagliders successfully transited beneath a 40-km <span class="hlt">ice</span> bridge and self-extracted after being carried beneath the Ross <span class="hlt">ice</span> shelf during missions conducted without the support of an acoustic navigation array. <span class="hlt">Ice</span>-capable Seagliders can provide sustainable, continuous occupation of critical sections in <span class="hlt">ice</span>-covered regions, including the marginal <span class="hlt">ice</span> <span class="hlt">zone</span>, with typical horizontal resolution of 3 km and routine sampling of the important, but hazardous, region near the <span class="hlt">ice</span>-ocean interface. Future directions include development of basin-scale acoustic navigation ('underwater GPS' for the Arctic) and use of existing high-frequency acoustic communications for short-range data transfer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70012586','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70012586"><span>Possible fossil H2O liquid-<span class="hlt">ice</span> interfaces in the Martian crust</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Soderblom, L.A.; Wenner, D.B.</p> <p>1978-01-01</p> <p>Throughout the northern equatorial region of Mars, extensive areas have been uniformly stripped, roughly to a constant depth. These terrains vary widely in their relative ages. A model is described here to explain this phenomenon as reflecting the vertical distribution of H2O liquid and <span class="hlt">ice</span> in the crust. Under present conditions the Martian equatorial regions are stratified in terms of the stability of water <span class="hlt">ice</span> and liquid water. This arises because the temperature of the upper 1 or 2 km is below the melting point of <span class="hlt">ice</span> and liquid is stable only at greater depth. It is suggested here that during planetary outgassing earlier in Martian history H2O was injected into the upper few kilometers of the crust by subsurface and surface volcanic eruption and lateral migration of the liquid and vapor. As a result, a discontinuity in the physical state of materials developed in the Martian crust coincident with the depth of H2O liquid-<span class="hlt">ice</span> phase boundary. Material above the boundary remained pristine; material below underwent diagenetic alteration and cementation. Subsequently, sections of the <span class="hlt">ice</span>-laden <span class="hlt">zone</span> were erosionally stripped by processes including eolian deflation, gravitational slump and collapse, and fluvial transport due to geothermal heating and melting of the <span class="hlt">ice</span>. The youngest plains which display this uniform stripping may provide a minimum stratigraphic age for the major period of outgassing of the planet. Viking results suggest that the total amount of H2O outgassed is less than half that required to fill the <span class="hlt">ice</span> layer, hence any residual liquid eventually found itself in the upper permafrost <span class="hlt">zone</span> or stored in the polar regions. Erosion stopped at the old liquid-<span class="hlt">ice</span> interface due to increased resistance of subjacent material and/or because melting of <span class="hlt">ice</span> was required to mobilize the debris. Water <span class="hlt">ice</span> may remain in uneroded regions, the overburden of debris preventing its escape to the atmosphere. Numerous morphological examples shown in Viking and Mariner 9</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20000025583','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20000025583"><span>LWC and Temperature Effects on <span class="hlt">Ice</span> Accretion Formation on Swept Wings at Glaze <span class="hlt">Ice</span> Conditions</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Vargas, Mario; Reshotko, Eli</p> <p>2000-01-01</p> <p>An experiment was conducted to study the effect of liquid water content and temperature on the critical distance in <span class="hlt">ice</span> accretion formation on swept wings at glaze <span class="hlt">ice</span> conditions. The critical distance is defined as the distance from the attachment line to tile beginning of the <span class="hlt">zone</span> where roughness elements develop into glaze <span class="hlt">ice</span> feathers. A baseline case of 150 mph, 25 F, 0.75 g/cu m. Cloud Liquid Water Content (LWC) and 20 micrometers in Water Droplet Median Volume Diameter (MVD) was chosen. <span class="hlt">Icing</span> runs were performed on a NACA 0012 swept wing tip at 150 mph and MVD of 20 micrometers for liquid water contents of 0.5 g/cu m, 0.75 g/cu m, and 1.0 g/cu m, and for total temperatures of 20 F, 25 F and 30 F. At each tunnel condition, the sweep angle was changed from 0 deg to 45 deg in 5 deg increments. Casting data, <span class="hlt">ice</span> shape tracings, and close-up photographic data were obtained. The results showed that decreasing the LWC to 0.5 g/cu m decreases the value of the critical distance at a given sweep angle compared to the baseline case, and starts the formation of complete scallops at 30 sweep angle. Increasing the LWC to 1.0 g/cu m increases the value of the critical distance compared to the baseline case, the critical distance remains always above 0 millimeters and complete scallops are not formed. Decreasing the total temperature to 20 F decreases the critical distance with respect to the baseline case and formation of complete scallops begins at 25 deg sweep angle. When the total temperature is increased to 30 F, bumps covered with roughness elements appear on the <span class="hlt">ice</span> accretion at 25 deg and 30 deg sweep angles, large <span class="hlt">ice</span> structures appear at 35 deg and 40 deg sweep angles, and complete scallops are formed at 45 deg sweep angle.</p> </li> <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 activities have been conducted internal to NASA and through collaboration efforts with industry, academia, and other government agencies. The details of the research activities 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 activities have been conducted internal to NASA and through collaboration efforts with industry, academia, and other government agencies. The details of the research activities 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('https://www.ncbi.nlm.nih.gov/pubmed/12712582','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12712582"><span>[Dynamics of ecological-biochemical characteristics of the sea <span class="hlt">ice</span> in the coastal <span class="hlt">zone</span> of the White sea].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mel'nikov, I A; Korneeva, G A; zhitina, L S; Shanin, S S</p> <p>2003-01-01</p> <p>The distribution of salinity, silicon and phosphorus contents, and hydrolytic enzyme activities along a sea-coast transect was studied in melted <span class="hlt">ice</span> cores and water samples taken from under the <span class="hlt">ice</span> cover in the periods of active <span class="hlt">ice</span> formation and melting in the Kandalaksha Bay, White Sea. The species list of identified algae was compiled, which included 170 species and varieties (90% of them belonged to diatoms). Strong correlations were revealed between the salinity of water samples and the content of silicon, protease activity, and the species composition of algae. Preliminary estimations of the rate of photosynthetic processes in individual cells of algae belonging to the mass species of the <span class="hlt">ice</span> flora are discussed.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_18 --> <div id="page_19" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="361"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19850042373&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=19850042373&hterms=glacier+melt&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dglacier%2Bmelt"><span><span class="hlt">Ice</span> sheet margins and <span class="hlt">ice</span> shelves</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Thomas, R. H.</p> <p>1984-01-01</p> <p>The effect of climate warming on the size of <span class="hlt">ice</span> 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 <span class="hlt">ice</span> sheets and <span class="hlt">ice</span> shelves. For sufficiently large warming (5-10C) the delayed effects would include the breakup of the <span class="hlt">ice</span> shelves by an increase in <span class="hlt">ice</span> drainage rates, particularly from the <span class="hlt">ice</span> sheets. On the basis of published data for periodic changes in the thickness and melting rates of the marine <span class="hlt">ice</span> sheets and fjord glaciers in Greenland and Antarctica, it is shown that the rate of retreat (or advance) of an <span class="hlt">ice</span> sheet is primarily determined by: bedrock topography; the basal conditions of the grounded <span class="hlt">ice</span> sheet; and the <span class="hlt">ice</span> shelf condition downstream of the grounding line. A program of satellite and ground measurements to monitor the state of <span class="hlt">ice</span> sheet equilibrium is recommended.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=PIA00578&hterms=europa+ice&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Deuropa%2Bice','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=PIA00578&hterms=europa+ice&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Deuropa%2Bice"><span>Europa <span class="hlt">Ice</span> Floes</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1997-01-01</p> <p>Jupiter's moon Europa, as seen in this image taken June 27, 1996 by NASA's Galileo spacecraft, displays features in some areas resembling <span class="hlt">ice</span> floes seen in Earth's polar seas. Europa, about the size of Earth's moon, has an icy crust that has been severely fractured, as indicated by the dark linear, curved, and wedged-shaped bands seen here. These fractures have broken the crust into plates as large as 30 kilometers (18.5 miles) across. Areas between the plates are filled with material that was probably icy slush contaminated with rocky debris. Some individual plates were separated and rotated into new positions. Europa's density indicates that it has a shell of water <span class="hlt">ice</span> thicker than 100 kilometers (about 60 miles), parts of which could be liquid. Currently, water <span class="hlt">ice</span> could extend from the surface down to the rocky interior, but the features seen in this image suggest that motion of the disrupted icy plates was lubricated by soft <span class="hlt">ice</span> or liquid water below the surface at the time of disruption. This image covers part of the equatorial <span class="hlt">zone</span> of Europa and was taken from a distance of 156,000 kilometers (about 96,300 miles) by the Solid-state Imaging Subsystem on the Galileo spacecraft. North is to the right and the sun is nearly directly overhead. The area shown is about 510 by 989 kilometers (310-by-600 miles), and the smallest visible feature is about 1.6 kilometers (1 mile) across.<p/>The Jet Propulsion Laboratory manages the Galileo mission for NASA's Office of Space Science, Washington, DC.<p/>This image and other images and data received from Galileo are posted on the World Wide Web Galileo mission home page at http://galileo.jpl.nasa.gov. Background information and educational context for the images can be found at http:// www.jpl.nasa.gov/galileo/sepo.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA01786.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA01786.html"><span>Space Radar Image of Weddell Sea <span class="hlt">Ice</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>1999-04-15</p> <p> growth perhaps 5 to 10 centimeters (2 to 4 inches) thick. The more extensive dark <span class="hlt">zones</span> are covered by a slightly thicker layer of smooth, level <span class="hlt">ice</span> up to 70 centimeters (28 inches) thick. http://photojournal.jpl.nasa.gov/catalog/PIA01786</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1919299M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1919299M"><span>Flow structure at an <span class="hlt">ice</span>-covered river confluence</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Martel, Nancy; Biron, Pascale; Buffin-Bélanger, Thomas</p> <p>2017-04-01</p> <p>River confluences are known to exhibit complex relationships between flow structure, sediment transport and bed-form development. Flow structure at these sites is influenced by the junction angle, the momentum flux ratio (Mr) and bed morphology. In cold regions where an <span class="hlt">ice</span> cover is present for most of the winter period, the flow structure is also likely affected by the roughness effect of the <span class="hlt">ice</span>. However, very few studies have examined the impact of an <span class="hlt">ice</span> cover on the flow structure at a confluence. The aims of this study are (1) to describe the evolution of an <span class="hlt">ice</span> cover at a river confluence and (2) to characterize and compare the flow structure at a river confluence with and without an <span class="hlt">ice</span> cover. The field site is a medium-sized confluence (around 40 m wide) between the Mit is and Neigette Rivers in the Bas-Saint-Laurent region, Quebec (Canada). The confluence was selected because a thick <span class="hlt">ice</span> cover is present for most of the winter allowing for safe field work. Two winter field campaigns were conducted in 2015 and 2016 to obtain <span class="hlt">ice</span> cover measurements in addition to hydraulic and morphological measurements. Daily monitoring of the evolution of the <span class="hlt">ice</span> cover was made with a Reconyx camera. Velocity profiles were collected with an acoustic Doppler current profiler (ADCP) to reconstruct the three-dimensional flow structure. Time series of photographs allow the evolution of the <span class="hlt">ice</span> cover to be mapped, linking the processes leading to the formation of the primary <span class="hlt">ice</span> cover for each year. The time series suggests that these processes are closely related with both confluence flow <span class="hlt">zones</span> and hydro-climatic conditions. Results on the thickness of the <span class="hlt">ice</span> cover from in situ measurements reveal that the <span class="hlt">ice</span> thickness tends to be thinner at the center of the confluence where high turbulent exchanges take place. Velocity measurements reveal that the <span class="hlt">ice</span> cover affects velocity profiles by moving the highest velocities towards the center of the profiles. A spatio</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.C53B..07A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.C53B..07A"><span>Summer Sea <span class="hlt">ice</span> in the Pacific Arctic sector from the CHINARE-2010 cruise</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ackley, S. F.; Xie, H.; Lei, R.; Huang, W.; Chinare 2010 Arctic Sea Ice Group</p> <p>2010-12-01</p> <p>The Fourth Chinese National Arctic Research Expedition (CHINARE) from July 1 to Sep. 23, 2010, the last Chinese campaign in Arctic Ocean contributing to the fourth International Polar Year (IPY), conducted comprehensive scientific studies on ocean-<span class="hlt">ice</span>-atmosphere interaction and the marine ecosystem’s response to climatic change in Arctic. This paper presents an overview on sea <span class="hlt">ice</span> (<span class="hlt">ice</span> concentration, floe size, melt pond coverage, sea <span class="hlt">ice</span> and snow thickness) of the Pacific Arctic sector, in particular between 150°W to 180°W to 86°N, based on: (1) underway visual observations of sea <span class="hlt">ice</span> at half-hourly and automatic cameras recording (both side looking from the icebreaker R.V. Xuelong) every 10 to 15 seconds; (2) a downward-looking video mounted on the left side of the vessel at a height of 7 m above waterline recording overturning of <span class="hlt">ice</span> floes; (3) on-site measurements of snow and <span class="hlt">ice</span> thickness using drilling and electromagnetic instrument EM31 (9.8 kHz) at eight short-term (~3 hours each) and one 12-day <span class="hlt">ice</span> stations; (4) six flights of aerial photogrammetry from helicopter, and (5) Satellite data (AMSE-E <span class="hlt">ice</span> concentration and ENVISAT ASAR) and NIC <span class="hlt">ice</span> charts) that extended the observations/measurements along beyond the ship track and airborne flights. In the northward leg, the largest <span class="hlt">ice</span> concentration <span class="hlt">zone</span> was in the area starting from ~75°N (July 29), with <span class="hlt">ice</span> concentration of 60-90% (mean ~80%), <span class="hlt">ice</span> thickness of 1.5-2m, melt ponds of 10-50% of <span class="hlt">ice</span>, ridged <span class="hlt">ice</span> of 10-30% of <span class="hlt">ice</span>, and floe size of 100’s meters to kms. The 12-day <span class="hlt">ice</span> station (from Aug 7-19), started at 86.92°N/178.88°W and moved a total of 175.7km, was on an <span class="hlt">ice</span> floe over 100 km2 in size and ~2 m in mean thickness. There were two heavy and several slight snowfall events in the period (July 29 to Aug 19). Snow thickness varies from 5cm to 15 cm, and melted about 5cm during the 12-day <span class="hlt">ice</span> camp. In the southward leg, the largest sea <span class="hlt">ice</span> concentration <span class="hlt">zone</span> was in the area between 87°N to 80</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017FrEaS...5...20S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017FrEaS...5...20S"><span>Inferring Firn Permeability from Pneumatic Testing: A Case Study on 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>Sommers, Aleah N.; Rajaram, Harihar; Weber, Eliezer P.; MacFerrin, Michael J.; Colgan, William T.; Stevens, C. Max</p> <p>2017-03-01</p> <p>Across the accumulation <span class="hlt">zone</span> of the Greenland <span class="hlt">ice</span> sheet, summer temperatures can be sufficiently warm to cause widespread melting, as was the case in July 2012 when the entire <span class="hlt">ice</span> sheet experienced a brief episode of enhanced surface ablation. The resulting meltwater percolates into the firn and refreezes, to create <span class="hlt">ice</span> lenses and layers within the firn column. This is an important process to consider when estimating the surface mass balance of the <span class="hlt">ice</span> sheet. The rate of meltwater percolation depends on the permeability of the firn, a property that is not well constrained in the presence of refrozen <span class="hlt">ice</span> layers and lenses. We present a novel, inexpensive method for measuring in-situ firn permeability using pneumatic testing, a well-established technique used in environmental engineering and hydrology. To illustrate the capabilities of this method, we estimate both horizontal and vertical permeability from pilot tests at six sites on the Greenland <span class="hlt">ice</span> sheet: KAN-U, DYE-2, EKT, NASA-SE, Saddle, and EastGRIP. These sites cover a range of conditions from mostly dry firn (EastGRIP), to firn with several <span class="hlt">ice</span> layers and lenses from refrozen meltwater (Saddle, NASA-SE, EKT), to firn with extensive <span class="hlt">ice</span> layers (DYE-2 and KAN-U). The estimated permeability in firn without refrozen <span class="hlt">ice</span> layers at EastGRIP agrees well with the range previously reported using an air permeameter to measure permeability through firn core samples at Summit, Greenland. At sites with <span class="hlt">ice</span> lenses or layers, we find high degrees of anisotropy, with vertical permeability much lower than horizontal permeability. Pneumatic testing is a promising and low-cost technique for measuring firn permeability, particularly as meltwater production increases in the accumulation <span class="hlt">zone</span> and <span class="hlt">ice</span> layers and lenses from refrozen melt layers become more prevalent. In these initial proof-of-concept tests, the estimated permeabilities represent effective permeability at the meter scale. With appropriately higher vacuum pressures</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23235878','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23235878"><span>Increased future <span class="hlt">ice</span> discharge from Antarctica owing to higher snowfall.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Winkelmann, R; Levermann, A; Martin, M A; Frieler, K</p> <p>2012-12-13</p> <p>Anthropogenic climate change is likely to cause continuing global sea level rise, but some processes within the Earth system may mitigate the magnitude of the projected effect. Regional and global climate models simulate enhanced snowfall over Antarctica, which would provide a direct offset of the future contribution to global sea level rise from cryospheric mass loss and ocean expansion. Uncertainties exist in modelled snowfall, but even larger uncertainties exist in the potential changes of dynamic <span class="hlt">ice</span> discharge from Antarctica and thus in the ultimate fate of the precipitation-deposited <span class="hlt">ice</span> mass. Here we show that snowfall and discharge are not independent, but that future <span class="hlt">ice</span> discharge will increase by up to three times as a result of additional snowfall under global warming. Our results, based on an <span class="hlt">ice</span>-sheet model forced by climate simulations through to the end of 2500 (ref. 8), show that the enhanced discharge effect exceeds the effect of surface warming as well as that of basal <span class="hlt">ice</span>-shelf melting, and is due to the difference in surface elevation change caused by snowfall on grounded versus floating <span class="hlt">ice</span>. Although different underlying forcings drive <span class="hlt">ice</span> loss from basal melting versus increased snowfall, similar <span class="hlt">ice</span> dynamical processes are nonetheless at work in both; therefore results are relatively independent of the specific representation of the transition <span class="hlt">zone</span>. In an ensemble of simulations designed to capture <span class="hlt">ice</span>-physics uncertainty, the additional dynamic <span class="hlt">ice</span> loss along the coastline compensates between 30 and 65 per cent of the <span class="hlt">ice</span> gain due to enhanced snowfall over the entire continent. This results in a dynamic <span class="hlt">ice</span> loss of up to 1.25 metres in the year 2500 for the strongest warming scenario. The reported effect thus strongly counters a potential negative contribution to global sea level by the Antarctic <span class="hlt">Ice</span> Sheet.</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 activities 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 activities 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 activities, survey results from teachers who have used the material, and other suggested material that can be used before and after the activities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16044598','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16044598"><span>Radiative habitable <span class="hlt">zones</span> in martian polar environments.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Córdoba-Jabonero, Carmen; Zorzano, María-Paz; Selsis, Franck; Patel, Manish R; Cockell, Charles S</p> <p>2005-06-01</p> <p>The biologically damaging solar ultraviolet (UV) radiation (quantified by the DNA-weighted dose) reaches the martian surface in extremely high levels. Searching for potentially habitable UV-protected environments on Mars, we considered the polar <span class="hlt">ice</span> caps that consist of a seasonally varying CO2 <span class="hlt">ice</span> cover and a permanent H2O <span class="hlt">ice</span> layer. It was found that, though the CO2 <span class="hlt">ice</span> is insufficient by itself to screen the UV radiation, at approximately 1 m depth within the perennial H2O <span class="hlt">ice</span> the DNA-weighted dose is reduced to terrestrial levels. This depth depends strongly on the optical properties of the H2O <span class="hlt">ice</span> layers (for instance snow-like layers). The Earth-like DNA-weighted dose and Photosynthetically Active Radiation (PAR) requirements were used to define the upper and lower limits of the northern and southern polar Radiative Habitable <span class="hlt">Zone</span> (RHZ) for which a temporal and spatial mapping was performed. Based on these studies we conclude that photosynthetic life might be possible within the <span class="hlt">ice</span> layers of the polar regions. The thickness varies along each martian polar spring and summer between approximately 1.5 and 2.4 m for H2O <span class="hlt">ice</span>-like layers, and a few centimeters for snow-like covers. These martian Earth-like radiative habitable environments may be primary targets for future martian astrobiological missions. Special attention should be paid to planetary protection, since the polar RHZ may also be subject to terrestrial contamination by probes. c2004 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRC..123...90L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123...90L"><span>Under-<span class="hlt">Ice</span> Phytoplankton Blooms Inhibited by Spring Convective Mixing in Refreezing Leads</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lowry, Kate E.; Pickart, Robert S.; Selz, Virginia; Mills, Matthew M.; Pacini, Astrid; Lewis, Kate M.; Joy-Warren, Hannah L.; Nobre, Carolina; van Dijken, Gert L.; Grondin, Pierre-Luc; Ferland, Joannie; Arrigo, Kevin R.</p> <p>2018-01-01</p> <p>Spring phytoplankton growth in polar marine ecosystems is limited by light availability beneath <span class="hlt">ice</span>-covered waters, particularly early in the season prior to snowmelt and melt pond formation. Leads of open water increase light transmission to the <span class="hlt">ice</span>-covered ocean and are sites of air-sea exchange. We explore the role of leads in controlling phytoplankton bloom dynamics within the sea <span class="hlt">ice</span> <span class="hlt">zone</span> of the Arctic Ocean. Data are presented from spring measurements in the Chukchi Sea during the Study of Under-<span class="hlt">ice</span> Blooms In the Chukchi Ecosystem (SUBICE) program in May and June 2014. We observed that fully consolidated sea <span class="hlt">ice</span> supported modest under-<span class="hlt">ice</span> blooms, while waters beneath sea <span class="hlt">ice</span> with leads had significantly lower phytoplankton biomass, despite high nutrient availability. Through an analysis of hydrographic and biological properties, we attribute this counterintuitive finding to springtime convective mixing in refreezing leads of open water. Our results demonstrate that waters beneath loosely consolidated sea <span class="hlt">ice</span> (84-95% <span class="hlt">ice</span> concentration) had weak stratification and were frequently mixed below the critical depth (the depth at which depth-integrated production balances depth-integrated respiration). These findings are supported by theoretical model calculations of under-<span class="hlt">ice</span> light, primary production, and critical depth at varied lead fractions. The model demonstrates that under-<span class="hlt">ice</span> blooms can form even beneath snow-covered sea <span class="hlt">ice</span> in the absence of mixing but not in more deeply mixed waters beneath sea <span class="hlt">ice</span> with refreezing leads. Future estimates of primary production should account for these phytoplankton dynamics in <span class="hlt">ice</span>-covered waters.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.C21D0685B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.C21D0685B"><span>Influence of the sea-<span class="hlt">ice</span> edge on the Arctic nearshore environment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barnhart, K. R.; Overeem, I.; Anderson, R. S.</p> <p>2013-12-01</p> <p>Coasts form the dynamic interface of the terrestrial and oceanic systems. In the Arctic, and in much of the world, the coast is a <span class="hlt">zone</span> of relatively high population, infrastructure, biodiversity, and ecosystem services. A significant difference between Arctic and temperate coasts is the presence of sea <span class="hlt">ice</span>. Sea <span class="hlt">ice</span> influences Arctic coasts in two main ways: (1) the length of the sea <span class="hlt">ice</span>-free season controls the length of time over which nearshore water can interact with the land, and (2) the sea <span class="hlt">ice</span> edge controls the fetch over which storm winds can blow over open water, resulting in changes in nearshore water level and wave field. The resulting nearshore hydrodynamic environment impacts all aspects of the coastal system. Here, we use satellite records of sea <span class="hlt">ice</span> along with a simple model for wind-driven storm surge and waves to document how changes in the length and character of the sea <span class="hlt">ice</span>-free season have impacted the nearshore hydrodynamic environment. For our sea <span class="hlt">ice</span> analysis we primarily use the Bootstrap Sea <span class="hlt">Ice</span> Concentrations from Nimbus-7 SMMR and DMSP SSM/I-SSMIS. We make whole-Arctic maps of sea <span class="hlt">ice</span> change in the coastal <span class="hlt">zone</span>. In addition to evaluating changes in length of the sea <span class="hlt">ice</span>-free season at the coast, we look at changes segmented by azimuth. This allows us to consider changes in the sea <span class="hlt">ice</span> in the context of the wind field. For our storm surge and wave field analysis we focus on the Beaufort Sea region. This region has experienced some of the greatest changes in both sea <span class="hlt">ice</span> cover and coastal erosion rates in the Arctic and is anticipated to experience significant change in the future. In addition, the NOAA ESRL GMD has observed the wind field at Barrow since extends to 1977. In our past work on the rapid and accelerating coastal erosion, we have shown that one may model storm surge with a 2D numerical bathystrophic model, and that waves are well represented by the Shore Protection Manual methods for shallow-water fetch-limited waves. We use</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010PhDT........54T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010PhDT........54T"><span>Analysis of scale effect in compressive <span class="hlt">ice</span> failure and implications for design</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Taylor, Rocky Scott</p> <p></p> <p>The main focus of the study was the analysis of scale effect in local <span class="hlt">ice</span> pressure resulting from probabilistic (spalling) fracture and the relationship between local and global loads due to the averaging of pressures across the width of a structure. A review of fundamental theory, relevant <span class="hlt">ice</span> mechanics and a critical analysis of data and theory related to the scale dependent pressure behavior of <span class="hlt">ice</span> were completed. To study high pressure <span class="hlt">zones</span> (hpzs), data from small-scale indentation tests carried out at the NRC-IOT were analyzed, including small-scale <span class="hlt">ice</span> block and <span class="hlt">ice</span> sheet tests. Finite element analysis was used to model a sample <span class="hlt">ice</span> block indentation event using a damaging, viscoelastic material model and element removal techniques (for spalling). Medium scale tactile sensor data from the Japan Ocean Industries Association (JOIA) program were analyzed to study details of hpz behavior. The averaging of non-simultaneous hpz loads during an <span class="hlt">ice</span>-structure interaction was examined using local panel pressure data. Probabilistic averaging methodology for extrapolating full-scale pressures from local panel pressures was studied and an improved correlation model was formulated. Panel correlations for high speed events were observed to be lower than panel correlations for low speed events. Global pressure estimates based on probabilistic averaging were found to give substantially lower average errors in estimation of load compared with methods based on linear extrapolation (no averaging). Panel correlations were analyzed for Molikpaq and compared with JOIA results. From this analysis, it was shown that averaging does result in decreasing pressure for increasing structure width. The relationship between local pressure and <span class="hlt">ice</span> thickness for a panel of unit width was studied in detail using full-scale data from the STRICE, Molikpaq, Cook Inlet and Japan Ocean Industries Association (JOIA) data sets. A distinct trend of decreasing pressure with increasing <span class="hlt">ice</span> thickness</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018DokES.478..228O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018DokES.478..228O"><span>The Influence of Climate Change on the Intensity of <span class="hlt">Ice</span> Gouging of the Bottom by Hummocky Formations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ogorodov, S. A.; Arkhipov, V. V.; Baranskaya, A. V.; Kokin, O. V.; Romanov, A. O.</p> <p>2018-02-01</p> <p>In the present work, several results of repeated sounding of bottom <span class="hlt">ice</span> gouging microrelief within the area of the underwater pipeline crossing of the Baydaratskaya Bay, Kara Sea, are presented. Based on the results of the monitoring, as well as the analysis of literature sources and modeling it has been established that under the conditions of climate warming and sea <span class="hlt">ice</span> reduction, the <span class="hlt">zone</span> of the most intensive <span class="hlt">ice</span> gouging is shifted landwards, on shallower water areas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120002543','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120002543"><span>Links Between Acceleration, Melting, and Supraglacial Lake Drainage of the Western 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>Hoffman, M. J.; Catania, G. A.; Newmann, T. A.; Andrews, L. C.; Rumrill, J. A.</p> <p>2012-01-01</p> <p>The impact of increasing summer melt on the dynamics and stability of the Greenland <span class="hlt">Ice</span> Sheet is not fully understood. Mounting evidence suggests seasonal evolution of subglacial drainage mitigates or counteracts the ability of surface runoff to increase basal sliding. Here, we compare subdaily <span class="hlt">ice</span> velocity and uplift derived from nine Global Positioning System stations in the upper ablation <span class="hlt">zone</span> in west Greenland to surface melt and supraglacial lake drainage during summer 2007. Starting around day 173, we observe speedups of 6-41% above spring velocity lasting approximately 40 days accompanied by sustained surface uplift at most stations, followed by a late summer slowdown. After initial speedup, we see a spatially uniform velocity response across the ablation <span class="hlt">zone</span> and strong diurnal velocity variations during periods of melting. Most lake drainages were undetectable in the velocity record, and those that were detected only perturbed velocities for approximately 1 day, suggesting preexisting drainage systems could efficiently drain large volumes of water. The dynamic response to melt forcing appears to 1) be driven by changes in subglacial storage of water that is delivered in diurnal and episodic pulses, and 2) decrease over the course of the summer, presumably as the subglacial drainage system evolves to greater efficiency. The relationship between hydrology and <span class="hlt">ice</span> dynamics observed is similar to that observed on mountain glaciers, suggesting that seasonally large water pressures under the <span class="hlt">ice</span> sheet largely compensate for the greater <span class="hlt">ice</span> thickness considered here. Thus, increases in summer melting may not guarantee faster seasonal <span class="hlt">ice</span> flow.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20120015198&hterms=glacier+melt&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dglacier%2Bmelt','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20120015198&hterms=glacier+melt&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dglacier%2Bmelt"><span>Links Between Acceleration, Melting, and Supraglacial Lake Drainage of the Western 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>Hoffman, M. J.; Catania, G. A.; Neumann, T. A.; Andrews, L. C.; Rumrill, J. A.</p> <p>2011-01-01</p> <p>The impact of increasing summer melt on the dynamics and stability of the Greenland <span class="hlt">Ice</span> Sheet is not fully understood. Mounting evidence suggests seasonal evolution of subglacial drainage mitigates or counteracts the ability of surface runoff to increase basal sliding. Here, we compare subdaily <span class="hlt">ice</span> velocity and uplift derived from nine Global Positioning System stations in the upper ablation <span class="hlt">zone</span> in west Greenland to surface melt and supraglacial lake drainage during summer 2007. Starting around day 173, we observe speedups of 6-41% above spring velocity lasting 40 days accompanied by sustained surface uplift at most stations, followed by a late summer slowdown. After initial speedup, we see a spatially uniform velocity response across the ablation <span class="hlt">zone</span> and strong diurnal velocity variations during periods of melting. Most lake drainages were undetectable in the velocity record, and those that were detected only perturbed velocities for approx 1 day, suggesting preexisting drainage systems could efficiently drain large volumes of water. The dynamic response to melt forcing appears to (1) be driven by changes in subglacial storage of water that is delivered in diurnal and episodic pulses, and (2) decrease over the course of the summer, presumably as the subglacial drainage system evolves to greater efficiency. The relationship between hydrology and <span class="hlt">ice</span> dynamics observed is similar to that observed on mountain glaciers, suggesting that seasonally large water pressures under the <span class="hlt">ice</span> sheet largely compensate for the greater <span class="hlt">ice</span> thickness considered here. Thus, increases in summer melting may not guarantee faster seasonal <span class="hlt">ice</span> flow.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26887494','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26887494"><span><span class="hlt">Ice</span> stream activity scaled to <span class="hlt">ice</span> sheet volume during Laurentide <span class="hlt">Ice</span> Sheet deglaciation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Stokes, C R; Margold, M; Clark, C D; Tarasov, L</p> <p>2016-02-18</p> <p>The contribution of the Greenland and West Antarctic <span class="hlt">ice</span> sheets to sea level has increased in recent decades, largely owing to the thinning and retreat of outlet glaciers and <span class="hlt">ice</span> streams. This dynamic loss is a serious concern, with some modelling studies suggesting that the collapse of a major <span class="hlt">ice</span> 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 <span class="hlt">ice</span>-sheet scale, it is unclear how the entire drainage network of <span class="hlt">ice</span> streams evolves over longer timescales. This represents one of the largest sources of uncertainty when predicting the contributions of <span class="hlt">ice</span> sheets to sea-level rise. A key question is whether <span class="hlt">ice</span> 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 <span class="hlt">ice</span> streams that operated at various times during deglaciation of the Laurentide <span class="hlt">Ice</span> 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 <span class="hlt">ice</span> sheet perimeter and their total discharge decreased. The underlying geology and topography clearly influenced <span class="hlt">ice</span> stream activity, but--at the <span class="hlt">ice</span>-sheet scale--their drainage network adjusted and was linked to changes in <span class="hlt">ice</span> sheet volume. It is unclear whether these findings can be directly translated to modern <span class="hlt">ice</span> sheets. However, contrary to the view that sees <span class="hlt">ice</span> streams as unstable entities that can accelerate <span class="hlt">ice</span>-sheet deglaciation, we conclude that <span class="hlt">ice</span> streams exerted progressively less influence on <span class="hlt">ice</span> sheet mass balance during the retreat of the Laurentide <span class="hlt">Ice</span> Sheet.</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 margin 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 <span class="hlt">zones</span> (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 <span class="hlt">Zones</span> 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 <span class="hlt">Zone</span> 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('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 margins. 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-<span class="hlt">zone</span> 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 margin 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://pubs.er.usgs.gov/publication/70012710','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70012710"><span><span class="hlt">Ice</span>-lubricated gravity spreading of the Olympus Mons aureole 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>Tanaka, K.L.</p> <p>1985-01-01</p> <p>Gravity sliding and spreading at low strain rates can account for the general morphology and structure of the aureoles and basal scarp of Olympus Mons. Detachment sliding could have occurred around the volcano if either pore-fluid pressures were exceptionally high (greater than 90%) or the rocks had very low resistance to shear (about 1 ?? 105 Pa or 1 bar). Because of the vast areal extent and probable shallow depth of the detachment <span class="hlt">zone</span>, development of ubiquitous, high pore-fluid pressures beneath aureole-forming material was unlikely. However, a <span class="hlt">zone</span> of sufficiently weak material consisting of about 10% interstitial or interbedded <span class="hlt">ice</span> could have been present. If so, a simple rheologic model for the aureole deposits can be applied that consists of a thin ductile layer overlain by a thicker brittle layer. According to this model, extensional deformation would have occurred near the shield and compressional deformation in its distal parts. Proximal grabens and distal corrugations on aureole surfaces support this model. A submarine slide at Kitimat Arm, British Columbia, is a valid qualitative analogy for the observed features and inferred emplacement style of the aureole deposits. Ground-<span class="hlt">ice</span> processes have been considered the cause of many geologic features on Mars; a 3% average concentration of ground <span class="hlt">ice</span> in the regolith is predicted by theoretical models for the <span class="hlt">ice</span> budget and cryosphere. <span class="hlt">Ice</span> may have been deposited in higher concentrations below the aureole-forming material; the source of the <span class="hlt">ice</span> could have been juvenile water circulated hydrothermally by Olympus Mons volcanism. The basal scarp of Olympus Mons apparently demarcates the transition between the upper, stable part of the shield and its lower part that decoupled and formed the aureole deposits. This transition may reflect a change in the bulk shear strength of the shield, caused either by a radial dependence in the abundance of <span class="hlt">ice</span> or fluid in the shield materials or by the concentration of intrusive</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..11.8790H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..11.8790H"><span>Study of elevation changes along a profile crossing 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>Hvidegaard, S. M.; Sandberg, L.</p> <p>2009-04-01</p> <p>In recent years much research has focused on determining how the Greenland <span class="hlt">Ice</span> Sheet is responding to the observed climate changes. There is wide agreement on the fact that the <span class="hlt">Ice</span> Sheet is currently loosing mass, and studies have shown that the mass loss is found near the <span class="hlt">ice</span> edge and that no significant changes are found in the central part of the <span class="hlt">Ice</span> Sheet. As a part of European Space Agency's CryoSat Validation Experiment (CryoVEx) running from 2004 to 2008, the National Space Institute (DTU Space) measured the elevations along a profile crossing the Greenland <span class="hlt">Ice</span> Sheet. The elevation observations were carried out in 2004, 2006 and 2008 using airborne laser altimetry from a Twin Otter aircraft. The observed profile follows the old EGIG line (Expédition Glaciologique au Groenland, measured in the 1950's) situated between 69-71N, heading nearly east-west. This unique dataset gives the opportunity to study elevation changes along the profile crossing the <span class="hlt">ice</span> sheet. With this work, we outline the observed elevation changes from the different <span class="hlt">zones</span> of the <span class="hlt">ice</span> sheet. We furthermore compare elevation changes based on coincident ICESat and airborne laser altimeter data.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_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://www.dtic.mil/docs/citations/AD1013707','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1013707"><span>Evolution of the Marginal <span class="hlt">Ice</span> <span class="hlt">Zone</span>: 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/2017PrOce.156...17L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PrOce.156...17L"><span>Under the sea <span class="hlt">ice</span>: Exploring the relationship between sea <span class="hlt">ice</span> and the foraging behaviour of southern elephant seals in 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>Labrousse, Sara; Sallée, Jean-Baptiste; Fraser, Alexander D.; Massom, Robert A.; Reid, Phillip; Sumner, Michael; Guinet, Christophe; Harcourt, Robert; McMahon, Clive; Bailleul, Frédéric; Hindell, Mark A.; Charrassin, Jean-Benoit</p> <p>2017-08-01</p> <p> diurnal vertical migration) in the pack <span class="hlt">ice</span> region, likely attracted by an <span class="hlt">ice</span> algal autumn bloom that sustains an under-<span class="hlt">ice</span> ecosystem. In contrast, male foraging effort increased when they remained deep within the sea <span class="hlt">ice</span> (420-960 km from the <span class="hlt">ice</span> edge) over the shelf. Males had a longer foraging activity (i) in the lowest sea <span class="hlt">ice</span> concentration at their position, and (ii) when there were more patches of low concentration sea <span class="hlt">ice</span> around their position (either in time or in space; 30 days & 50 km) presumably in polynyas or flaw leads between land fast and pack <span class="hlt">ice</span>. This provides access to <span class="hlt">zones</span> of enhanced resources in autumn or in early spring such as polynyas, the Antarctic shelf and slope. Our results suggest that some seals utilized a highly sea <span class="hlt">ice</span> covered environment, which is key for their foraging effort, sustaining or concentrating resources during winter.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4242568','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4242568"><span>Effects of <span class="hlt">ice</span> and floods on vegetation in streams in cold regions: implications for climate change</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Lind, Lovisa; Nilsson, Christer; Weber, Christine</p> <p>2014-01-01</p> <p>Riparian <span class="hlt">zones</span> support some of the most dynamic and species-rich plant communities in cold regions. A common conception among plant ecologists is that flooding during the season when plants are dormant generally has little effect on the survival and production of riparian vegetation. We show that winter floods may also be of fundamental importance for the composition of riverine vegetation. We investigated the effects of <span class="hlt">ice</span> formation on riparian and in-stream vegetation in northern Sweden using a combination of experiments and observations in 25 reaches, spanning a gradient from <span class="hlt">ice</span>-free to <span class="hlt">ice</span>-rich reaches. The <span class="hlt">ice</span>-rich reaches were characterized by high production of frazil and anchor <span class="hlt">ice</span>. In a couple of experiments, we exposed riparian vegetation to experimentally induced winter flooding, which reduced the dominant dwarf-shrub cover and led to colonization of a species-rich forb-dominated vegetation. In another experiment, natural winter floods caused by anchor-<span class="hlt">ice</span> formation removed plant mimics both in the in-stream and in the riparian <span class="hlt">zone</span>, further supporting the result that anchor <span class="hlt">ice</span> maintains dynamic plant communities. With a warmer winter climate, <span class="hlt">ice</span>-induced winter floods may first increase in frequency because of more frequent shifts between freezing and thawing during winter, but further warming and shortening of the winter might make them less common than today. If <span class="hlt">ice</span>-induced winter floods become reduced in number because of a warming climate, an important disturbance agent for riparian and in-stream vegetation will be removed, leading to reduced species richness in streams and rivers in cold regions. Given that such regions are expected to have more plant species in the future because of immigration from the south, the distribution of species richness among habitats can be expected to show novel patterns. PMID:25505542</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25505542','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25505542"><span>Effects of <span class="hlt">ice</span> and floods on vegetation in streams in cold regions: implications for climate change.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lind, Lovisa; Nilsson, Christer; Weber, Christine</p> <p>2014-11-01</p> <p>Riparian <span class="hlt">zones</span> support some of the most dynamic and species-rich plant communities in cold regions. A common conception among plant ecologists is that flooding during the season when plants are dormant generally has little effect on the survival and production of riparian vegetation. We show that winter floods may also be of fundamental importance for the composition of riverine vegetation. We investigated the effects of <span class="hlt">ice</span> formation on riparian and in-stream vegetation in northern Sweden using a combination of experiments and observations in 25 reaches, spanning a gradient from <span class="hlt">ice</span>-free to <span class="hlt">ice</span>-rich reaches. The <span class="hlt">ice</span>-rich reaches were characterized by high production of frazil and anchor <span class="hlt">ice</span>. In a couple of experiments, we exposed riparian vegetation to experimentally induced winter flooding, which reduced the dominant dwarf-shrub cover and led to colonization of a species-rich forb-dominated vegetation. In another experiment, natural winter floods caused by anchor-<span class="hlt">ice</span> formation removed plant mimics both in the in-stream and in the riparian <span class="hlt">zone</span>, further supporting the result that anchor <span class="hlt">ice</span> maintains dynamic plant communities. With a warmer winter climate, <span class="hlt">ice</span>-induced winter floods may first increase in frequency because of more frequent shifts between freezing and thawing during winter, but further warming and shortening of the winter might make them less common than today. If <span class="hlt">ice</span>-induced winter floods become reduced in number because of a warming climate, an important disturbance agent for riparian and in-stream vegetation will be removed, leading to reduced species richness in streams and rivers in cold regions. Given that such regions are expected to have more plant species in the future because of immigration from the south, the distribution of species richness among habitats can be expected to show novel patterns.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.S52A..01B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.S52A..01B"><span>Chilean Tsunami Rocks 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>Bromirski, P. D.; Gerstoft, P.; Chen, Z.; Stephen, R. A.; Diez, A.; Arcas, D.; Wiens, D.; Aster, R. C.; Nyblade, A.</p> <p>2016-12-01</p> <p>The response of the Ross <span class="hlt">Ice</span> Shelf (RIS) to the September 16, 2015 9.3 Mb Chilean earthquake tsunami (> 75 s period) and infragravity (IG) waves (50 - 300 s period) were recorded by a broadband seismic array deployed on the RIS from November 2014 to November 2015. The array included two linear transects, one approximately orthogonal to the shelf front extending 430 km southward toward the grounding <span class="hlt">zone</span>, and an east-west transect spanning the RIS roughly parallel to the front about 100 km south of the <span class="hlt">ice</span> edge (https://scripps.ucsd.edu/centers/iceshelfvibes/). Signals generated by both the tsunami and IG waves were recorded at all stations on floating <span class="hlt">ice</span>, with little ocean wave-induced energy reaching stations on grounded <span class="hlt">ice</span>. Cross-correlation and dispersion curve analyses indicate that tsunami and IG wave-generated signals propagate across the RIS at gravity wave speeds (about 70 m/s), consistent with coupled water-<span class="hlt">ice</span> flexural-gravity waves propagating through the <span class="hlt">ice</span> shelf from the north. Gravity wave excitation at periods > 100 s is continuously observed during the austral winter, providing mechanical excitation of the RIS throughout the year. Horizontal displacements are typically about 3 times larger than vertical displacements, producing extensional motions that could facilitate expansion of existing fractures. The vertical and horizontal spectra in the IG band attenuate exponentially with distance from the front. Tsunami model data are used to assess variability of excitation of the RIS by long period gravity waves. Substantial variability across the RIS roughly parallel to the front is observed, likely resulting from a combination of gravity wave amplitude variability along the front, signal attenuation, incident angle of the wave forcing at the front that depends on wave generation location as well as bathymetry under and north of the shelf, and water layer and <span class="hlt">ice</span> shelf thickness and properties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C32A..08D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C32A..08D"><span>Greenland deep boreholes inform on sliding and deformation of the basal <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>Dahl-Jensen, D.</p> <p>2017-12-01</p> <p>Repeated measurements of the deformation of the deep boreholes on the Greenland <span class="hlt">ice</span> sheet informs on the basal sliding, near basal deformation and in general on the horizontal velocity through the <span class="hlt">ice</span>. Results of the logging of the boreholes at Dye3, GRIP, NGRIP, NEEM and Camp Century through the last 40 years by the Danish <span class="hlt">Ice</span> and Climate group will be presented and discussed. The results on the flow will be compared with the information on <span class="hlt">ice</span> properties, impurity load and bedrock entrained material from the deep <span class="hlt">ice</span> cores and the radio echo sounding images near the drill sites.The results show that the basal movement often happens in an impurity rich <span class="hlt">zone</span> above the bedrock while pure basal sliding is limited even in the presence of basal water and significant basal melt.Most of the deep <span class="hlt">ice</span> core sites are located close to <span class="hlt">ice</span> divides where the surface velocity is limited so significant basal sliding is not expected. Exceptions are the surface velocities at Camp Century and Dye 3, both being 13 m/yr.Finally, the ongoing deep drilling at EGRIP will shortly be presented where we are drilling in the center of the North East Greenland <span class="hlt">Ice</span> Stream (NEGIS).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010TellB..62..621J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010TellB..62..621J"><span>Rapid changes in surface water carbonate chemistry during Antarctic sea <span class="hlt">ice</span> melt</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jones, Elizabeth M.; Bakker, Dorothee C. E.; Venables, Hugh J.; Whitehouse, Michael J.; Korb, Rebecca E.; Watson, Andrew J.</p> <p>2010-11-01</p> <p>ABSTRACT The effect of sea <span class="hlt">ice</span> melt on the carbonate chemistry of surface waters in the Weddell-Scotia Confluence, Southern Ocean, was investigated during January 2008. Contrasting concentrations of dissolved inorganic carbon (DIC), total alkalinity (TA) and the fugacity of carbon dioxide (fCO2) were observed in and around the receding sea <span class="hlt">ice</span> edge. The precipitation of carbonate minerals such as ikaite (CaCO3.6H2O) in sea <span class="hlt">ice</span> brine has the net effect of decreasing DIC and TA and increasing the fCO2 in the brine. Deficits in DIC up to 12 +/- 3 μmol kg-1 in the marginal <span class="hlt">ice</span> <span class="hlt">zone</span> (MIZ) were consistent with the release of DIC-poor brines to surface waters during sea <span class="hlt">ice</span> melt. Biological utilization of carbon was the dominant processes and accounted for 41 +/- 1 μmol kg-1 of the summer DIC deficit. The data suggest that the combined effects of biological carbon uptake and the precipitation of carbonates created substantial undersaturation in fCO2 of 95 μatm in the MIZ during summer sea <span class="hlt">ice</span> melt. Further work is required to improve the understanding of ikaite chemistry in Antarctic sea <span class="hlt">ice</span> and its importance for the sea <span class="hlt">ice</span> carbon pump.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-200910220009HQ.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-200910220009HQ.html"><span><span class="hlt">Ice</span> Bridge Antarctic Sea <span class="hlt">Ice</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2009-10-21</p> <p>An iceberg is seen out the window of NASA's DC-8 research aircraft as it flies 2,000 feet above the Amundsen Sea in West Antarctica on Wednesday, Oct., 21, 2009. This was the fourth science flight of NASA‚Äôs Operation <span class="hlt">Ice</span> Bridge airborne Earth science mission to study Antarctic <span class="hlt">ice</span> sheets, sea <span class="hlt">ice</span>, and <span class="hlt">ice</span> shelves. Photo Credit: (NASA/Jane Peterson)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C41C1245L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C41C1245L"><span>Impact of Basal Hydrology Near Grounding Lines: Results from the MISMIP-3D and MISMIP+ Experiments Using 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>Leguy, G.; Lipscomb, W. H.; Asay-Davis, X.</p> <p>2017-12-01</p> <p><span class="hlt">Ice</span> sheets and <span class="hlt">ice</span> shelves are linked by the transition <span class="hlt">zone</span>, the region where the grounded <span class="hlt">ice</span> lifts off the bedrock and begins to float. Adequate resolution of the transition <span class="hlt">zone</span> is necessary for numerically accurate <span class="hlt">ice</span> sheet-<span class="hlt">ice</span> shelf simulations. In previous work we have shown that by using a simple parameterization of the basal hydrology, a smoother transition in basal water pressure between floating and grounded <span class="hlt">ice</span> improves the numerical accuracy of a one-dimensional vertically integrated fixed-grid model. We used a set of experiments based on the Marine <span class="hlt">Ice</span> Sheet Model Intercomparison Project (MISMIP) to show that reliable grounding-line dynamics at resolutions 1 km is achievable. In this presentation we use the Community <span class="hlt">Ice</span> Sheet Model (CISM) to demonstrate how the representation of basal lubrication impacts three-dimensional models using the MISMIP-3D and MISMIP+ experiments. To this end we will compare three different Stokes approximations: the Shallow Shelf Approximation (SSA), a depth-integrated higher-order approximation, and the Blatter-Pattyn model. The results from our one-dimensional model carry over to the 3-D models; a resolution of 1 km (and in some cases 2 km) remains sufficient to accurately simulate grounding-line dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.V11B4717I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.V11B4717I"><span>Phreatomagmatic eruptions under the West Antarctic <span class="hlt">Ice</span> Sheet: potential hazard for <span class="hlt">ice</span> sheet stability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Iverson, N. A.; Dunbar, N. W.; Lieb-Lappen, R.; Kim, E. J.; Golden, E. J.; Obbard, R. W.</p> <p>2014-12-01</p> <p>Volcanic tephra layers have been seen in most <span class="hlt">ice</span> cores in Antarctica. These tephra layers are deposited almost instantaneously across wide areas of <span class="hlt">ice</span> sheets, creating horizons that can provide "pinning points" to adjust <span class="hlt">ice</span> time scales that may otherwise be lacking detailed chronology. A combination of traditional particle morphology characterization by SEM with new non-destructive X-ray micro-computed tomography (Micro-CT) has been used to analyze selected coarse grained tephra in the West Antarctica <span class="hlt">Ice</span> Sheet (WAIS) Divide WDC06A <span class="hlt">ice</span> core. Micro-CT has the ability to image particles as small as 50µm in length (15µm resolution), quantifying both particle shape and size. The WDC06A contains hundreds of dusty layers of which 36 have so far been identified as primary tephra layers. Two of these tephra layers have been characterized as phreatomagmatic eruptions based on SEM imagery and are blocky and platy in nature, with rare magmatic particles. These layers are strikingly different in composition from the typical phonolitic and trachytic tephra produced from West Antarctic volcanoes. These two layers are coarser in grain size, with many particles (including feldspar crystals) exceeding 100µm in length. One tephra layer found at 3149.138m deep in the <span class="hlt">ice</span> core is a coarse ~1mm thick basanitic tephra layer with a WDC06-7 <span class="hlt">ice</span> core age of 45,381±2000yrs. The second layer is a ~1.3 cm thick <span class="hlt">zoned</span> trachyandesite to trachydacite tephra found at 2569.205m deep with an <span class="hlt">ice</span> core age 22,470±835yrs. Micro-CT analysis shows that WDC06A-3149.138 has normal grading with the largest particles at the bottom of the sample (~160μm). WDC06A-2569.205 has a bimodal distribution of particles with large particles at the top and bottom of the layer. These large particles are more spherical in shape at the base and become more irregular and finer grained higher in the layer, likely showing changes in eruption dynamics. The distinct chemistry as well as the blocky and large grain size</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSME12B..03L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSME12B..03L"><span>Under the Sea <span class="hlt">Ice</span>: Exploration of the Relationships Between Sea <span class="hlt">Ice</span> Patterns and Foraging Movements of a Marine Predator in 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>Labrousse, S.; Sallee, J. B.; Fraser, A. D.; Massom, R. A.; Reid, P.; Sumner, M.; Guinet, C.; Harcourt, R.; Bailleul, F.; Hindell, M.; Charrassin, J. B.</p> <p>2016-02-01</p> <p> probably gave them access to <span class="hlt">zones</span> of enhanced resources in early spring such as polynyas, the Antarctic Slope Front, or the Antarctic shelf while avoiding the constraint of sea <span class="hlt">ice</span>. Over years, males foraging activity were not affected by anomalies of sea <span class="hlt">ice</span> advance, however negative SIC anomalies were profitable allowing them to use remote areas within sea <span class="hlt">ice</span>.</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 marginal sea <span class="hlt">ice</span> <span class="hlt">zone</span> 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 marginal sea <span class="hlt">ice</span> <span class="hlt">zone</span> 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('https://www.ncbi.nlm.nih.gov/pubmed/21396663','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21396663"><span>Large-scale oil-in-<span class="hlt">ice</span> experiment in the Barents Sea: monitoring of oil in water and MetOcean interactions.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Faksness, Liv-Guri; Brandvik, Per Johan; Daae, Ragnhild L; Leirvik, Frode; Børseth, Jan Fredrik</p> <p>2011-05-01</p> <p>A large-scale field experiment took place in the marginal <span class="hlt">ice</span> <span class="hlt">zone</span> in the Barents Sea in May 2009. Fresh oil (7000 L) was released uncontained between the <span class="hlt">ice</span> floes to study oil weathering and spreading in <span class="hlt">ice</span> and surface water. A detailed monitoring of oil-in-water and <span class="hlt">ice</span> interactions was performed throughout the six-day experiment. In addition, meteorological and oceanographic data were recorded for monitoring of the wind speed and direction, air temperature, currents and <span class="hlt">ice</span> floe movements. The monitoring showed low concentrations of dissolved hydrocarbons and the predicted acute toxicity indicated that the acute toxicity was low. The <span class="hlt">ice</span> field drifted nearly 80 km during the experimental period, and although the oil drifted with the <span class="hlt">ice</span>, it remained contained between the <span class="hlt">ice</span> floes. Copyright © 2011 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017SciDr..22...29N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017SciDr..22...29N"><span>Facility for testing <span class="hlt">ice</span> drills</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nielson, Dennis L.; Delahunty, Chris; Goodge, John W.; Severinghaus, Jeffery P.</p> <p>2017-05-01</p> <p>The Rapid Access <span class="hlt">Ice</span> Drill (RAID) is designed for subsurface scientific investigations in Antarctica. Its objectives are to drill rapidly through <span class="hlt">ice</span>, to core samples of the transition <span class="hlt">zone</span> and bedrock, and to leave behind a borehole observatory. These objectives required the engineering and fabrication of an entirely new drilling system that included a modified mining-style coring rig, a unique fluid circulation system, a rod skid, a power unit, and a workshop with areas for the storage of supplies and consumables. An important milestone in fabrication of the RAID was the construction of a North American Test (NAT) facility where we were able to test drilling and fluid processing functions in an environment that is as close as possible to that expected in Antarctica. Our criteria for site selection was that the area should be cold during the winter months, be located in an area of low heat flow, and be at relatively high elevation. We selected a site for the facility near Bear Lake, Utah, USA. The general design of the NAT well (NAT-1) started with a 27.3 cm (10.75 in.) outer casing cemented in a 152 m deep hole. Within that casing, we hung a 14 cm (5.5 in.) casing string, and, within that casing, a column of <span class="hlt">ice</span> was formed. The annulus between the 14 and 27.3 cm casings provided the path for circulation of a refrigerant. After in-depth study, we chose to use liquid CO2 to cool the hole. In order to minimize the likelihood of the casing splitting due to the volume increase associated with freezing water, the hole was first cooled and then <span class="hlt">ice</span> was formed in increments from the bottom upward. First, <span class="hlt">ice</span> cubes were placed in the inner liner and then water was added. Using this method, a column of <span class="hlt">ice</span> was incrementally prepared for drilling tests. The drilling tests successfully demonstrated the functioning of the RAID system. Reproducing such a facility for testing of other <span class="hlt">ice</span> drilling systems could be advantageous to other research programs in the future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMPP41F..08W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMPP41F..08W"><span>Polar <span class="hlt">Ice</span> Sheets Drive Paleohydroclimate Affecting Terrestrial Plant Distribution and CO2 Exchange Potential during the Upper Carboniferous</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>White, J. D.; Poulsen, C. J.; Montanez, I. P.; McElwain, J.; Wilson, J. P.; Hren, M. T.</p> <p>2016-12-01</p> <p>Variation in atmospheric CO2 concentration and presence or absence of polar <span class="hlt">ice</span> sheets simulated for 310 mya using the GENESIS model show changes in terrestrial temperature, precipitation, and potential evapotranspiration at mid and lower latitudes. Classifying the data into Holdridge life <span class="hlt">zones</span> for simulations with 280, 560, and 1120 ppm CO2, in the presence of a southern Gondwanan <span class="hlt">ice</span> sheet resulted in progressive increase of cool temperate, humid-to-subhumid and tropical subhumid <span class="hlt">zones</span>. Without the <span class="hlt">ice</span> sheet, subtropical subhumid to semiarid <span class="hlt">zones</span> expanded. Simulation results show that approximately 50% of the land area was classified as polar or tundra followed by 35 to 42%, depending on the scenario, classified as sub-tropical semiarid-to-subhumid. Only 5-8% were classified as temperate humid-to-subhumid or tropical humid-to-perhumid. Also, the absence of <span class="hlt">ice</span> sheets reduced the moister sub-climates, such as within the tropical climate <span class="hlt">zone</span>. Because different plant assemblages dominated each climate <span class="hlt">zone</span>, for example cordaitaleans in the subtropical and medullosans and lycophytes in the tropics, physiological differences in these plants may have resulted in unequal CO2 exchange feedbacks to the atmosphere during climate shifts. Previous physiological modeling based on plant foliar traits indicates that late Paleozoic plant species differed in CO2 uptake capacity with highest sensitivity to water availability during periods with low atmospheric CO2 concentration. This implies that vegetation climate feedbacks during this period may have been non-uniform during climate change events. Inference of plant contribution to climate forcing must rely on understanding geographic distribution of affected vegetation, inherent vegetation physiological properties, and antecedent atmospheric CO2 concentrations. Our results indicate that seasonally dry climates prevailed in the low-latitude land area, and that slightly cooler temperatures than today must be considered. This</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.P53C2215H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.P53C2215H"><span>The Western Noachis Terra Chloride Deposits: An Improved Characterization of the Proposed Human Exploration <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hill, J. R.; Plaut, J. J.; Christensen, P. R.</p> <p>2016-12-01</p> <p>At the First Landing Site and Exploration <span class="hlt">Zone</span> Workshop for Human Missions to the Surface of Mars (Oct 27-30, 2015, Houston, TX), planetary scientists, students and members of the public proposed forty-seven sites that meet the engineering requirements for a human mission and would also allow astronauts to investigate important scientific questions while on the surface. The chloride deposits in western Noachis Terra at -37.2°N, 350.5°E were proposed as a potential exploration <span class="hlt">zone</span> due to their proximity to craters containing glacier-like forms and imperfectly-formed concentric crater fill. The high astrobiological preservation potential of the chloride deposits exposed on the surface would allow astronauts to investigate the past habitability of a well-preserved Noachian fluvial system, while the subsurface <span class="hlt">ice</span> features suggest astronauts would have relatively easy access to enough water to meet the requirements of NASA's current baseline mission architecture. Since the workshop, the proposed exploration <span class="hlt">zone</span> has been further characterized using additional datasets, as well as new data collected by the Mars Reconnaissance Orbiter as part of the exploration <span class="hlt">zone</span> data acquisition effort organized by NASA's Human Landing Sites Study (HLS2) team. First, SHARAD radar data were used to constrain the subsurface structure of the imperfectly-formed concentric crater fill within the two large craters, which makes a more accurate assessment of the potential subsurface water <span class="hlt">ice</span> resources possible. Second, newly acquired HiRISE images were used to better assess the traversability of the terrain between the habitation <span class="hlt">zone</span> and the primary resource and science regions-of-interest (ROIs). And third, the exploration <span class="hlt">zone</span> was shifted in order to place the central landing site closer to potential subsurface water <span class="hlt">ice</span> resources. Although this would require crews to travel further to investigate the chloride deposits, it reduces the distance between the subsurface water <span class="hlt">ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29291835','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29291835"><span><span class="hlt">Ice</span> cream structure modification by <span class="hlt">ice</span>-binding proteins.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kaleda, Aleksei; Tsanev, Robert; Klesment, Tiina; Vilu, Raivo; Laos, Katrin</p> <p>2018-04-25</p> <p><span class="hlt">Ice</span>-binding proteins (IBPs), also known as antifreeze proteins, were added to <span class="hlt">ice</span> cream to investigate their effect on structure and texture. <span class="hlt">Ice</span> recrystallization inhibition was assessed in the <span class="hlt">ice</span> cream mixes using a novel accelerated microscope assay and the <span class="hlt">ice</span> cream microstructure was studied using an <span class="hlt">ice</span> crystal dispersion method. It was found that adding recombinantly produced fish type III IBPs at a concentration 3 mg·L -1 made <span class="hlt">ice</span> cream hard and crystalline with improved shape preservation during melting. <span class="hlt">Ice</span> creams made with IBPs (both from winter rye, and type III IBP) had aggregates of <span class="hlt">ice</span> crystals that entrapped pockets of the <span class="hlt">ice</span> cream mixture in a rigid network. Larger individual <span class="hlt">ice</span> crystals and no entrapment in control <span class="hlt">ice</span> creams was observed. Based on these results a model of <span class="hlt">ice</span> crystals aggregates formation in the presence of IBPs was proposed. Copyright © 2017 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C33C1203F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C33C1203F"><span>Fragmentation and melting of the seasonal sea <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>Feltham, D. L.; Bateson, A.; Schroeder, D.; Ridley, J. K.; Aksenov, Y.</p> <p>2017-12-01</p> <p>Recent years have seen a rapid reduction in the summer extent of Arctic sea <span class="hlt">ice</span>. This trend has implications for navigation, oil exploration, wildlife, and local communities. Furthermore the Arctic sea <span class="hlt">ice</span> cover impacts the exchange of heat and momentum between the ocean and atmosphere with significant teleconnections across the climate system, particularly mid to low latitudes in the Northern Hemisphere. The treatment of melting and break-up processes of the seasonal sea <span class="hlt">ice</span> cover within climate models is currently limited. In particular floes are assumed to have a uniform size which does not evolve with time. Observations suggest however that floe sizes can be modelled as truncated power law distributions, with different exponents for smaller and larger floes. This study aims to examine factors controlling the floe size distribution in the seasonal and marginal <span class="hlt">ice</span> <span class="hlt">zone</span>. This includes lateral melting, wave induced break-up of floes, and the feedback between floe size and the mixed ocean layer. These results are then used to quantify the proximate mechanisms of seasonal sea <span class="hlt">ice</span> reduction in a sea ice—ocean mixed layer model. Observations are used to assess and calibrate the model. The impacts of introducing these processes to the model will be discussed and the preliminary results of sensitivity and feedback studies will also be presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1810447B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1810447B"><span>Rate and style of <span class="hlt">ice</span> stream retreat constrained by new surface-exposure ages: The Minch, NW Scotland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bradwell, Tom; Small, David; Fabel, Derek; Dove, Dayton; Cofaigh, Colm O.; Clark, Chris; Consortium, Britice-Chrono</p> <p>2016-04-01</p> <p>Chronologically constrained studies of former <span class="hlt">ice</span>-sheet extents and dynamics are important for understanding past cryospheric responses and modelling future <span class="hlt">ice</span>-sheet and sea-level change. As part of the BRITICE-CHRONO project, we present new geomorphological and chronological data from a marine-terminating <span class="hlt">ice</span> stream system in NW Europe that operated during the Late Weichselian Glaciation. A suite of 51 cosmogenic-nuclide exposure ages from <span class="hlt">ice</span> sheet moraines and glacially transported boulders constrain the maximum extent of the <span class="hlt">ice</span> sheet on the continental shelf (~28 ka BP) and its subsequent retreat, between ~27 and 16 ka BP, into a large marine embayment (ca. 7000 km2; the Minch, NW Scotland). Recently acquired swath bathymetry and acoustic sub-bottom profiler data reveal several large transverse grounding-<span class="hlt">zone</span> wedges up to 40 m thick and 5 km wide with diagnostic acoustic-facies architecture. These seabed sediment wedges mark former quasi-stable positions of grounded marine-terminating <span class="hlt">ice</span>-stream fronts; their size and thickness suggest long-lived stillstands of the order of centuries. Statistically significant clusters of exposure ages from glacial deposits on islands and intervening headlands shed important new light on the age of these marine grounding-<span class="hlt">zone</span> wedges and, by inference, the rate and timing of Minch palaeo-<span class="hlt">ice</span> stream retreat. We find strong evidence for episodic <span class="hlt">ice</span> stream retreat on the continental shelf between ~28-24 ka BP, in the outer Minch between ~24-22 ka BP, and in the central Minch between 22-18.5 ka BP. In contrast, final <span class="hlt">ice</span> stream deglaciation (<18 ka) across the deepest parts of the inner Minch embayment, was probably rapid and uninterrupted - with the <span class="hlt">ice</span> sheet margin at or close to the present-day coastline in NW Scotland by 16.1 ka BP. It is hoped that these results will form the empirical basis for future <span class="hlt">ice</span>-sheet modelling of this dynamically sensitive sector of the British-Irish <span class="hlt">Ice</span> Sheet.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27812435','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27812435"><span>Loitering of the retreating sea <span class="hlt">ice</span> edge in the Arctic Seas.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Steele, Michael; Ermold, Wendy</p> <p>2015-12-01</p> <p>Each year, the arctic sea <span class="hlt">ice</span> edge retreats from its winter maximum extent through the Seasonal <span class="hlt">Ice</span> <span class="hlt">Zone</span> (SIZ) to its summer minimum extent. On some days, this retreat happens at a rapid pace, while on other days, parts of the pan-arctic <span class="hlt">ice</span> edge hardly move for periods of days up to 1.5 weeks. We term this stationary behavior "<span class="hlt">ice</span> edge loitering," and identify areas that are more prone to loitering than others. Generally, about 20-25% of the SIZ area experiences loitering, most often only one time at any one location during the retreat season, but sometimes two or more times. The main mechanism controlling loitering is an interaction between surface winds and warm sea surface temperatures in areas from which the <span class="hlt">ice</span> has already retreated. When retreat happens early enough to allow atmospheric warming of this open water, winds that force <span class="hlt">ice</span> floes into this water cause melting. Thus, while individual <span class="hlt">ice</span> floes are moving, the <span class="hlt">ice</span> edge as a whole appears to loiter. The time scale of loitering is then naturally tied to the synoptic time scale of wind forcing. Perhaps surprisingly, the area of loitering in the arctic seas has not changed over the past 25 years, even as the SIZ area has grown. This is because rapid <span class="hlt">ice</span> retreat happens most commonly late in the summer, when atmospheric warming of open water is weak. We speculate that loitering may have profound effects on both physical and biological conditions at the <span class="hlt">ice</span> edge during the retreat season.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_20 --> <div id="page_21" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="401"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C51B0973H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C51B0973H"><span>Ground-penetrating radar evidence of refrozen meltwater in the firn column of Larsen C <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>Hubbard, B. P.; Booth, A. D.; Sevestre, H.; Kulessa, B.; Bevan, S. L.; Luckman, A. J.; Kuipers Munneke, P.; Buzzard, S. C.; Ashmore, D. W.; O'Leary, M.</p> <p>2017-12-01</p> <p>Firn densification, which has been strongly implicated in <span class="hlt">ice</span> shelf collapse, can occur rapidly by the percolation and refreezing of surface meltwater. This process reduces the permeability of the firn column, potentially establishing a positive feedback between densification and the occurrence of surface meltwater ponds, and may ultimately facilitate fracturing associated with shelf collapse. Meltwater ponds on Larsen C's Cabinet (CI) and Whirlwind (WI) inlets form where foehn winds reach and influence the shelf surface. While associated <span class="hlt">zones</span> of refrozen meltwater are strongly evidenced in borehole optical televiewing (OPTV) and seismic refraction data, the sparsity of these observations limits insight into the dimensions of these <span class="hlt">zones</span>. Here, we present highlights from an 800-km archive of ground-penetrating radar (GPR) profiles acquired by the MIDAS project on CI and WI during November-December 2015. In the upstream reaches of CI and WI, stratified firn layers are abruptly truncated by <span class="hlt">zones</span> of diminished GPR reflectivity. These initiate 5 m beneath the surface and extend to a depth of 30 m. Volumes appear to exceed 6 km3 (CI) and 1 km3 (WI); these are underestimates, established only where there is GPR control. The horizontal distribution of these <span class="hlt">zones</span> correlates with the pattern of reduced backscatter in SAR images, supporting their association with meltwater ponds. GPR reflectivity models, derived from OPTV density trends, suggest reduced GPR wavespeeds (as do GPR velocity analyses) and dielectric contrasts consistent with homogenised and densified firn. A firn density model supports the ability of meltwater ponds to form periodically in Cabinet Inlet and subsequently homogenise the density of the firn column. Our observations suggest that <span class="hlt">ice</span> shelves affected by surface melt and ponding can contain spatially extensive bodies of <span class="hlt">ice</span> that are warmer and denser than assumed so far, with significant implications for <span class="hlt">ice</span> shelf flow and fracturing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.B13A0432K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.B13A0432K"><span>Microorganisms Trapped Within Permafrost <span class="hlt">Ice</span> In The Fox Permafrost Tunnel, Alaska</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Katayama, T.; Tanaka, M.; Douglas, T. A.; Cai, Y.; Tomita, F.; Asano, K.; Fukuda, M.</p> <p>2008-12-01</p> <p>Several different types of massive <span class="hlt">ice</span> are common in permafrost. <span class="hlt">Ice</span> wedges are easily recognized by their shape and foliated structure. They grow syngenetically or epigenetically as a result of repeated cycles of frost cracking followed by the infiltration of snow, melt water, soil or other material into the open frost cracks. Material incorporated into <span class="hlt">ice</span> wedges becomes frozen and preserved. Pool <span class="hlt">ice</span>, another massive <span class="hlt">ice</span> type, is formed by the freezing of water resting on top of frozen thermokarst sediment or melting wedges and is not foliated. The Fox Permafrost Tunnel in Fairbanks was excavated within the discontinuous permafrost <span class="hlt">zone</span> of central Alaska and it contains permafrost, <span class="hlt">ice</span> wedges, and pool <span class="hlt">ice</span> preserved at roughly -3°C. We collected samples from five <span class="hlt">ice</span> wedges and three pool <span class="hlt">ice</span> structures in the Fox Permafrost Tunnel. If the microorganisms were incorporated into the <span class="hlt">ice</span> during its formation, a community analysis of the microorganisms could elucidate the environment in which the <span class="hlt">ice</span> was formed. Organic material from sediments in the tunnel was radiocarbon-dated between 14,000 and 30,000 years BP. However, it is still not clear when the <span class="hlt">ice</span> wedges were formed or subsequently deformed because they are only partially exposed and their upper surfaces are above the tunnel walls. The objectives of our study were to determine the biogeochemical conditions during massive <span class="hlt">ice</span> formation and to analyze the microbial community within the <span class="hlt">ices</span> by incubation-based and DNA-based analyses. The geochemical profile and the PCR-DGGE band patterns of bacteria among five <span class="hlt">ice</span> wedge and 3 portions of pool <span class="hlt">ice</span> samples were markedly different. The DGGE band patterns of fungi were simple with a few bands of fungi or yeast. The dominant bands of <span class="hlt">ice</span> wedge and pool <span class="hlt">ice</span> samples were affiliated with the genus Geomyces and Doratomyces, respectively. Phylogenetic analysis using rRNA gene ITS regions indicated isolates of Geomyces spp. from different <span class="hlt">ice</span> wedges were affiliated</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27206961','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27206961"><span>Experimental provocation of '<span class="hlt">ice</span>-cream headache' by <span class="hlt">ice</span> cubes and <span class="hlt">ice</span> water.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mages, Stephan; Hensel, Ole; Zierz, Antonia Maria; Kraya, Torsten; Zierz, Stephan</p> <p>2017-04-01</p> <p>Background There are various studies on experimentally provoked '<span class="hlt">ice</span>-cream headache' or 'headache attributed to ingestion or inhalation of a cold stimulus' (HICS) using different provocation protocols. The aim of this study was to compare two provocation protocols. Methods <span class="hlt">Ice</span> cubes pressed to the palate and fast ingestion of <span class="hlt">ice</span> water were used to provoke HICS and clinical features were compared. Results The <span class="hlt">ice</span>-water stimulus provoked HICS significantly more often than the <span class="hlt">ice</span>-cube stimulus (9/77 vs. 39/77). <span class="hlt">Ice</span>-water-provoked HICS had a significantly shorter latency (median 15 s, range 4-97 s vs. median 68 s, range 27-96 s). There was no difference in pain localisation. Character after <span class="hlt">ice</span>-cube stimulation was predominantly described as pressing and after <span class="hlt">ice</span>-water stimulation as stabbing. A second HICS followed in 10/39 (26%) of the headaches provoked by <span class="hlt">ice</span> water. Lacrimation occurred significantly more often in volunteers with than in those without HICS. Discussion HICS provoked by <span class="hlt">ice</span> water was more frequent, had a shorter latency, different pain character and higher pain intensity than HICS provoked by <span class="hlt">ice</span> cubes. The finding of two subsequent HICS attacks in the same volunteers supports the notion that two types of HICS exist. Lacrimation during HICS indicates involvement of the trigeminal-autonomic reflex.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1995JGR...10014269P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1995JGR...10014269P"><span>Coupled energy-balance/<span class="hlt">ice</span>-sheet model simulations of the glacial cycle: A possible connection between terminations and terrigenous dust</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Peltier, W. Richard; Marshall, Shawn</p> <p>1995-07-01</p> <p>We apply a coupled energy-balance/<span class="hlt">ice</span>-sheet climate model in an investigation of northern hemisphere <span class="hlt">ice</span>-sheet advance and retreat over the last glacial cycle. When driven only by orbital insolation variations, the model predicts <span class="hlt">ice</span>-sheet advances over the continents of North America and Eurasia that are in good agreement with geological reconstructions in terms of the timescale of advance and the spatial positioning of the main <span class="hlt">ice</span> masses. The orbital forcing alone, however, is unable to induce the observed rapid <span class="hlt">ice</span>-sheet retreat, and we conclude that additional climatic feedbacks not explicitly included in the basic model must be acting. In the analyses presented here we have parameterized a number of potentially important effects in order to test their relative influence on the process of glacial termination. These include marine instability, thermohaline circulation effects, carbon dioxide variations, and snow albedo changes caused by dust loading during periods of high atmospheric aerosol concentration. For the purpose of these analyses the temporal changes in the latter two variables were inferred from <span class="hlt">ice</span> core records. Of these various influences, our analyses suggest that the albedo variations in the <span class="hlt">ice</span>-sheet ablation <span class="hlt">zone</span> caused by dust loading may represent an extremely important ablation mechanism. Using our parameterization of "dirty" snow in the ablation <span class="hlt">zone</span> we find glacial retreat to be strongly accelerated, such that complete collapse of the otherwise stable Laurentide <span class="hlt">ice</span> sheet ensues. The last glacial maximum configurations of the Laurentide and Fennoscandian complexes are also brought into much closer accord with the <span class="hlt">ICE</span>-3G reconstruction of Tushingham and Peltier (1991,1992) and the <span class="hlt">ICE</span>-4G reconstruction of Peltier (1994) when this effect is reasonably introduced.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910031227&hterms=TYPES+RADAR&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DTYPES%2BOF%2BRADAR','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910031227&hterms=TYPES+RADAR&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DTYPES%2BOF%2BRADAR"><span><span class="hlt">Ice</span>-type classifications from airborne pulse-limited radar altimeter return waveform characteristics</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fedor, L. S.; Hayne, G. S.; Walsh, E. J.</p> <p>1989-01-01</p> <p>During mid-March 1978, the NASA C-130 aircraft was deployed to Eielson Air Force Base in Fairbanks, Alaska, to make a series of flights over <span class="hlt">ice</span> in the Beaufort Sea. The radar altimeter data analyzed were obtained northeast of Mackenzie Bay on March 14th in the vicinity of 69.9 deg N, 134.2 deg W. The data were obtained with a 13.9 GHz radar altimeter developed under the NASA Advanced Applications Flight Experiments (AAFE) Program. This airborne radar was built as a forerunner of the Seasat radar altimeter, and utilized the same pulse compression technique. Pulse-limited radar data taken with the altimeter from 1500-m altitude over sea <span class="hlt">ice</span> are registered to high-quality photography. The backscattered power is statistically related the surface conductivity and to the number of facets whose surface normal is directed towards the radar. The variations of the radar return waveform shape and signal level are correlated with the variation of the <span class="hlt">ice</span> type determined from photography. The AAFE altimeter has demonstrated that the return waveform shape and signal level of an airborne pulse-limited altimeter at 13.9 GHz respond to sea <span class="hlt">ice</span> type. The signal level responded dramatically to even a very small fracture in the <span class="hlt">ice</span>, as long as it occurred directly at the altimeter nadir point. Shear <span class="hlt">zones</span> and regions of significant compression ridging consistently produced low signal levels. The return waveforms frequently evidenced the characteristics of both specular and diffuse scattering, and there was an indication that the power backscattered at 3 deg off-nadir in a shear <span class="hlt">zone</span> was actually somewhat higher than that from nadir.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1013705','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1013705"><span>Use of Declassified High-Resolution Imagery and Coincident Data Sets for Characterizing the Changing Arctic <span class="hlt">Ice</span> Cover, and Collaboration with SIZRS</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>Meter-Scale Sea <span class="hlt">Ice</span> Properties Karen E. Frey, Christopher Polashenski The Seasonal Evolution of Sea <span class="hlt">Ice</span> Floe Size Distribution Jacqueline A...Richter-Menge and Donald K. Perovich 3 Monitoring of Arctic Conditions from a Virtual Constellation of Synthetic Aperture Radar Hans C. Graber, Peter...Jennifer K. Hutchings, Jacqueline A. Richter-Menge Seasonal <span class="hlt">Ice</span> <span class="hlt">Zone</span> Reconnaissance Surveys Coordination James Morison REFERENCES Kwok, R., and N</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=STS048-152-007&hterms=5S&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3D5S','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=STS048-152-007&hterms=5S&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3D5S"><span>Breakup of Pack <span class="hlt">Ice</span>, Antarctic <span class="hlt">Ice</span> Shelf</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1991-01-01</p> <p>Breakup of Pack <span class="hlt">Ice</span> along the periphery of the Antarctic <span class="hlt">Ice</span> Shelf (53.5S, 3.0E) produced this mosaic of <span class="hlt">ice</span> floes off the Antarctic <span class="hlt">Ice</span> Shelf. Strong offshore winds, probably associated with strong katabatic downdrafts from the interior of the continent, are seen peeling off the edges of the <span class="hlt">ice</span> shelf into long filamets of sea <span class="hlt">ice</span>, icebergs, bergy bits and growlers to flow northward into the South Atlantic Ocean. 53.5S, 3.0E</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010BGD.....7.1167A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010BGD.....7.1167A"><span>Differences in community composition of bacteria in four deep <span class="hlt">ice</span> sheets in western China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>An, L.; Chen, Y.; Xiang, S.-R.; Shang, T.-C.; Tian, L.-De</p> <p>2010-02-01</p> <p>Microbial community patterns vary in glaciers world wide, presenting unique responses to global climatic and environmental changes. Four bacterial clone libraries were established by 16S rRNA gene amplification from four <span class="hlt">ice</span> layers along the 42-m-long <span class="hlt">ice</span> core MuztB drilled from the Muztag Ata Glacier. A total of 152 bacterial sequences obtained from the <span class="hlt">ice</span> core MuztB were phylogenetically compared with the 71 previously reported sequences from three <span class="hlt">ice</span> cores extracted from <span class="hlt">ice</span> caps Malan, Dunde, and Puruoganri. The six functional clusters Flavisolibacter, Flexibacter (Bacteroidetes), Acinetobacter, Enterobacter (Gammaproteobacteria), Planococcus/Anoxybacillus (Firmicutes), and Propionibacter/Luteococcus (Actinobacteria) frequently occurred along the Muztag Ata Glacier profile. Sequence analysis showed that most of the sequences from the <span class="hlt">ice</span> core clustered with those from cold environments, and the sequences from the same glacier formed a distinct cluster. Moreover, bacterial communities from the same location or similarly aged <span class="hlt">ice</span> formed a cluster, and were clearly separate from those from other geographically isolated glaciers. In a summary, the findings provide preliminary evidence of <span class="hlt">zone</span> distribution of microbial community, support our hypothesis of the spatial and temporal biogeography of microorganisms in glacial <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.5786B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.5786B"><span>Tsunami and infragravity waves impacting Antarctic <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>Bromirski, P. D.; Chen, Z.; Stephen, R. A.; Gerstoft, P.; Arcas, D.; Diez, A.; Aster, R. C.; Wiens, D. A.; Nyblade, A.</p> <p>2017-07-01</p> <p>The responses of the Ross <span class="hlt">Ice</span> Shelf (RIS) to the 16 September 2015 8.3 (Mw) Chilean earthquake tsunami (>75 s period) and to oceanic infragravity (IG) waves (50-300 s period) were recorded by a broadband seismic array deployed on the RIS from November 2014 to November 2016. Here we show that tsunami and IG-generated signals within the RIS propagate at gravity wave speeds (˜70 m/s) as water-<span class="hlt">ice</span> coupled flexural-gravity waves. IG band signals show measureable attenuation away from the shelf front. The response of the RIS to Chilean tsunami arrivals is compared with modeled tsunami forcing to assess <span class="hlt">ice</span> shelf flexural-gravity wave excitation by very long period (VLP; >300 s) gravity waves. Displacements across the RIS are affected by gravity wave incident direction, bathymetry under and north of the shelf, and water layer and <span class="hlt">ice</span> shelf thicknesses. Horizontal displacements are typically about 10 times larger than vertical displacements, producing dynamical extensional motions that may facilitate expansion of existing fractures. VLP excitation is continuously observed throughout the year, with horizontal displacements highest during the austral winter with amplitudes exceeding 20 cm. Because VLP flexural-gravity waves exhibit no discernable attenuation, this energy must propagate to the grounding <span class="hlt">zone</span>. Both IG and VLP band flexural-gravity waves excite mechanical perturbations of the RIS that likely promote tabular iceberg calving, consequently affecting <span class="hlt">ice</span> shelf evolution. Understanding these ocean-excited mechanical interactions is important to determine their effect on <span class="hlt">ice</span> shelf stability to reduce uncertainty in the magnitude and rate of global sea level rise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Natur.550..506W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Natur.550..506W"><span>Evidence of marine <span class="hlt">ice</span>-cliff instability in Pine Island Bay from iceberg-keel plough marks</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wise, Matthew G.; Dowdeswell, Julian A.; Jakobsson, Martin; Larter, Robert D.</p> <p>2017-10-01</p> <p>Marine <span class="hlt">ice</span>-cliff instability (MICI) processes could accelerate future retreat of the Antarctic <span class="hlt">Ice</span> Sheet if <span class="hlt">ice</span> shelves that buttress grounding lines more than 800 metres below sea level are lost. The present-day grounding <span class="hlt">zones</span> of the Pine Island and Thwaites glaciers in West Antarctica need to retreat only short distances before they reach extensive retrograde slopes. When grounding <span class="hlt">zones</span> of glaciers retreat onto such slopes, theoretical considerations and modelling results indicate that the retreat becomes unstable (marine <span class="hlt">ice</span>-sheet instability) and thus accelerates. It is thought that MICI is triggered when this retreat produces <span class="hlt">ice</span> cliffs above the water line with heights approaching about 90 metres. However, observational evidence confirming the action of MICI has not previously been reported. Here we present observational evidence that rapid deglacial <span class="hlt">ice</span>-sheet retreat into Pine Island Bay proceeded in a similar manner to that simulated in a recent modelling study, driven by MICI. Iceberg-keel plough marks on the sea-floor provide geological evidence of past and present iceberg morphology, keel depth and drift direction. From the planform shape and cross-sectional morphologies of iceberg-keel plough marks, we find that iceberg calving during the most recent deglaciation was not characterized by small numbers of large, tabular icebergs as is observed today, which would produce wide, flat-based plough marks or toothcomb-like multi-keeled plough marks. Instead, it was characterized by large numbers of smaller icebergs with V-shaped keels. Geological evidence of the form and water-depth distribution of the plough marks indicates calving-margin thicknesses equivalent to the threshold that is predicted to trigger <span class="hlt">ice</span>-cliff structural collapse as a result of MICI. We infer rapid and sustained <span class="hlt">ice</span>-sheet retreat driven by MICI, commencing around 12,300 years ago and terminating before about 11,200 years ago, which produced large numbers of icebergs smaller than the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMGC31D1210T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMGC31D1210T"><span>Interannual variability of high <span class="hlt">ice</span> cloud properties over the tropics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tamura, S.; Iwabuchi, H.</p> <p>2015-12-01</p> <p>The El Niño/Southern Oscillation (ENSO) affects atmospheric conditions and cloud physical properties such as cloud fraction (CF) and cloud top height (CTH). However, an impact of the ENSO on physical properties in high-<span class="hlt">ice</span> cloud is not well known. Therefore, this study attempts to reveal relationship between variability of <span class="hlt">ice</span> cloud physical properties and ENSO. <span class="hlt">Ice</span> clouds are inferred with the multiband IR method in this study. <span class="hlt">Ice</span> clouds are categorized in terms of cloud optical thickness (COT) as thin (0.1< COT <0.3), opaque (0.3< COT <3.6), thick (3.6< COT <11), and deep convective (DC) (11< COT) clouds, and relationship between ENSO and interannual variability of cloud physical properties is investigated for each category during the period from January 2003 to December 2014. The deseasonalized anomalies of CF and CTH in all categories correlate well with Niño3.4 index, with positive anomaly over the eastern Pacific and negative anomaly over the western Pacific during El Niño condition. However, the global distribution of these correlation coefficients is different by cloud categories. For example, CF of DC correlates well with Niño3.4 index over the convergence <span class="hlt">zone</span>, while, that of thin cloud shows high correlation extending to high latitude from convergence <span class="hlt">zone</span>, suggesting a connection with cloud formation. The global distributions of average rate of change differ by cloud category, because the different associate with ENSO and gradual trend toward La Niña condition had occurred over the analysis period. In this conference, detailed results and relationship between variability of cloud physical properties and atmospheric conditions will be shown.</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-<span class="hlt">zones</span> 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 active subglacial hydrologic and geological systems or at the marine margin 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 active 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('https://www.ncbi.nlm.nih.gov/pubmed/27025155','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27025155"><span><span class="hlt">Ice</span>-shell purification of <span class="hlt">ice</span>-binding proteins.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Marshall, Craig J; Basu, Koli; Davies, Peter L</p> <p>2016-06-01</p> <p><span class="hlt">Ice</span>-affinity purification is a simple and efficient method of purifying to homogeneity both natural and recombinant <span class="hlt">ice</span>-binding proteins. The purification involves the incorporation of <span class="hlt">ice</span>-binding proteins into slowly-growing <span class="hlt">ice</span> and the exclusion of other proteins and solutes. In previous approaches, the <span class="hlt">ice</span> was grown around a hollow brass finger through which coolant was circulated. We describe here an easily-constructed apparatus that employs <span class="hlt">ice</span> affinity purification that not only shortens the time for purification from 1-2 days to 1-2 h, but also enhances yield and purity. In this apparatus, the surface area for the separation was increased by extracting the <span class="hlt">ice</span>-binding proteins into an <span class="hlt">ice</span>-shell formed inside a rotating round-bottom flask partially submerged in a sub-zero bath. In principle, any <span class="hlt">ice</span>-binding compound can be recovered from liquid solution, and the method is readily scalable. Copyright © 2016 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5599042-airborne-gravity-measurement-over-sea-ice-western-weddel-sea','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5599042-airborne-gravity-measurement-over-sea-ice-western-weddel-sea"><span>Airborne gravity measurement over sea-<span class="hlt">ice</span>: The western Weddel Sea</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>Brozena, J.; Peters, M.; LaBrecque, J.</p> <p>1990-10-01</p> <p>An airborne gravity study of the western Weddel Sea, east of the Antarctic Peninsula, has shown that floating pack-<span class="hlt">ice</span> provides a useful radar altimetric reference surface for altitude and vertical acceleration corrections surface for alititude and vertical acceleration corrections to airborne gravimetry. Airborne gravimetry provides an important alternative to satellite altimetry for the sea-<span class="hlt">ice</span> covered regions of the world since satellite alimeters are not designed or intended to provide accurate geoidal heights in areas where significant sea-<span class="hlt">ice</span> is present within the radar footprint. Errors in radar corrected airborne gravimetry are primarily sensitive to the variations in the second derivative ofmore » the sea-<span class="hlt">ice</span> reference surface in the frequency pass-band of interest. With the exception of imbedded icebergs the second derivative of the pack-<span class="hlt">ice</span> surface closely approximates that of the mean sea-level surface at wavelengths > 10-20 km. With the airborne method the percentage of <span class="hlt">ice</span> coverage, the mixture of first and multi-year <span class="hlt">ice</span> and the existence of leads and pressure ridges prove to be unimportant in determining gravity anomalies at scales of geophysical and geodetic interest, provided that the <span class="hlt">ice</span> is floating and not grounded. In the Weddell study an analysis of 85 crosstrack miss-ties distributed over 25 data tracks yields an rms error of 2.2 mGals. Significant structural anomalies including the continental shelf and offsets and lineations interpreted as fracture <span class="hlt">zones</span> recording the early spreading directions within the Weddell Sea are observed in the gravity map.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030068097','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030068097"><span>Quantification of <span class="hlt">Ice</span> Accretions for <span class="hlt">Icing</span> Scaling Evaluations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ruff, Gary A.; Anderson, David N.</p> <p>2003-01-01</p> <p>The comparison of <span class="hlt">ice</span> accretion characteristics is an integral part of aircraft <span class="hlt">icing</span> research. It is often necessary to compare an <span class="hlt">ice</span> accretion obtained from a flight test or numerical simulation to one produced in an <span class="hlt">icing</span> wind tunnel or for validation of an <span class="hlt">icing</span> scaling method. Traditionally, this has been accomplished by overlaying two-dimensional tracings of <span class="hlt">ice</span> accretion shapes. This paper addresses the basic question of how to compare <span class="hlt">ice</span> accretions using more quantitative methods. For simplicity, geometric characteristics of the <span class="hlt">ice</span> accretions are used for the comparison. One method evaluated is a direct comparison of the percent differences of the geometric measurements. The second method inputs these measurements into a fuzzy inference system to obtain a single measure of the goodness of the comparison. The procedures are demonstrated by comparing <span class="hlt">ice</span> shapes obtained in the <span class="hlt">Icing</span> Research Tunnel at NASA Glenn Research Center during recent <span class="hlt">icing</span> scaling tests. The results demonstrate that this type of analysis is useful in quantifying the similarity of <span class="hlt">ice</span> accretion shapes and that the procedures should be further developed by expanding the analysis to additional <span class="hlt">icing</span> data sets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Sci...359.1136T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Sci...359.1136T"><span><span class="hlt">Ice</span>-VII inclusions in diamonds: Evidence for aqueous fluid in Earth’s deep mantle</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tschauner, O.; Huang, S.; Greenberg, E.; Prakapenka, V. B.; Ma, C.; Rossman, G. R.; Shen, A. H.; Zhang, D.; Newville, M.; Lanzirotti, A.; Tait, K.</p> <p>2018-03-01</p> <p>Water-rich regions in Earth’s deeper mantle are suspected to play a key role in the global water budget and the mobility of heat-generating elements. We show that <span class="hlt">ice</span>-VII occurs as inclusions in natural diamond and serves as an indicator for such water-rich regions. <span class="hlt">Ice</span>-VII, the residue of aqueous fluid present during growth of diamond, crystallizes upon ascent of the host diamonds but remains at pressures as high as 24 gigapascals; it is now recognized as a mineral by the International Mineralogical Association. In particular, <span class="hlt">ice</span>-VII in diamonds points toward fluid-rich locations in the upper transition <span class="hlt">zone</span> and around the 660-kilometer boundary.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMPP11E..02G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMPP11E..02G"><span>Simulating a Dynamic Antarctic <span class="hlt">Ice</span> Sheet in the Early to Middle Miocene</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gasson, E.; DeConto, R.; Pollard, D.; Levy, R. H.</p> <p>2015-12-01</p> <p>There are a variety of sources of geological data that suggest major variations in the volume and extent of the Antarctic <span class="hlt">ice</span> sheet during the early to middle Miocene. Simulating such variability using coupled climate-<span class="hlt">ice</span> sheet models is problematic due to a strong hysteresis effect caused by height-mass balance feedback and albedo feedback. This results in limited retreat of the <span class="hlt">ice</span> sheet once it has reached the continental size, as likely occurred prior to the Miocene. Proxy records suggest a relatively narrow range of atmospheric CO2 during the early to middle Miocene, which exacerbates this problem. We use a new climate forcing which accounts for <span class="hlt">ice</span> sheet-climate feedbacks through an asynchronous GCM-RCM coupling, which is able to better resolve the narrow Antarctic ablation <span class="hlt">zone</span> in warm climate simulations. When combined with recently suggested mechanisms for retreat into subglacial basins due to <span class="hlt">ice</span> shelf hydrofracture and <span class="hlt">ice</span> cliff failure, we are able to simulate large-scale variability of the Antarctic <span class="hlt">ice</span> sheet in the Miocene. This variability is equivalent to a seawater oxygen isotope signal of ~0.5 ‰, or a sea level equivalent change of ~35 m, for a range of atmospheric CO2 between 280 - 500 ppm.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20000044552','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20000044552"><span><span class="hlt">Ice</span> Accretions and <span class="hlt">Icing</span> Effects for Modern Airfoils</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Addy, Harold E., Jr.</p> <p>2000-01-01</p> <p><span class="hlt">Icing</span> tests were conducted to document <span class="hlt">ice</span> shapes formed on three different two-dimensional airfoils and to study the effects of the accreted <span class="hlt">ice</span> on aerodynamic performance. The models tested were representative of airfoil designs in current use for each of the commercial transport, business jet, and general aviation categories of aircraft. The models were subjected to a range of <span class="hlt">icing</span> conditions in an <span class="hlt">icing</span> wind tunnel. The conditions were selected primarily from the Federal Aviation Administration's Federal Aviation Regulations 25 Appendix C atmospheric <span class="hlt">icing</span> conditions. A few large droplet <span class="hlt">icing</span> conditions were included. To verify the aerodynamic performance measurements, molds were made of selected <span class="hlt">ice</span> shapes formed in the <span class="hlt">icing</span> tunnel. Castings of the <span class="hlt">ice</span> were made from the molds and placed on a model in a dry, low-turbulence wind tunnel where precision aerodynamic performance measurements were made. Documentation of all the <span class="hlt">ice</span> shapes and the aerodynamic performance measurements made during the <span class="hlt">icing</span> tunnel tests is included in this report. Results from the dry, low-turbulence wind tunnel tests are also presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA601068','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA601068"><span>Sunlight, Sea <span class="hlt">Ice</span>, and the <span class="hlt">Ice</span> Albedo Feedback in a Changing Arctic Sea <span class="hlt">Ice</span> Cover</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2013-09-30</p> <p>Sea <span class="hlt">Ice</span> , and the <span class="hlt">Ice</span> Albedo Feedback in a...COVERED 00-00-2013 to 00-00-2013 4. TITLE AND SUBTITLE Sunlight, Sea <span class="hlt">Ice</span> , and the <span class="hlt">Ice</span> Albedo Feedback in a Changing Arctic Sea <span class="hlt">Ice</span> Cover 5a...during a period when incident solar irradiance is large increasing solar heat input to the <span class="hlt">ice</span> . Seasonal sea <span class="hlt">ice</span> typically has a smaller albedo</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018TCry...12.1957A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018TCry...12.1957A"><span>Microtopographic control on the ground thermal regime in <span class="hlt">ice</span> wedge polygons</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Abolt, Charles J.; Young, Michael H.; Atchley, Adam L.; Harp, Dylan R.</p> <p>2018-06-01</p> <p>The goal of this research is to constrain the influence of <span class="hlt">ice</span> wedge polygon microtopography on near-surface ground temperatures. <span class="hlt">Ice</span> wedge polygon microtopography is prone to rapid deformation in a changing climate, and cracking in the <span class="hlt">ice</span> wedge depends on thermal conditions at the top of the permafrost; therefore, feedbacks between microtopography and ground temperature can shed light on the potential for future <span class="hlt">ice</span> wedge cracking in the Arctic. We first report on a year of sub-daily ground temperature observations at 5 depths and 9 locations throughout a cluster of low-centered polygons near Prudhoe Bay, Alaska, and demonstrate that the rims become the coldest <span class="hlt">zone</span> of the polygon during winter, due to thinner snowpack. We then calibrate a polygon-scale numerical model of coupled thermal and hydrologic processes against this dataset, achieving an RMSE of less than 1.1 °C between observed and simulated ground temperature. Finally, we conduct a sensitivity analysis of the model by systematically manipulating the height of the rims and the depth of the troughs and tracking the effects on <span class="hlt">ice</span> wedge temperature. The results indicate that winter temperatures in the <span class="hlt">ice</span> wedge are sensitive to both rim height and trough depth, but more sensitive to rim height. Rims act as preferential outlets of subsurface heat; increasing rim size decreases winter temperatures in the <span class="hlt">ice</span> wedge. Deeper troughs lead to increased snow entrapment, promoting insulation of the <span class="hlt">ice</span> wedge. The potential for <span class="hlt">ice</span> wedge cracking is therefore reduced if rims are destroyed or if troughs subside, due to warmer conditions in the <span class="hlt">ice</span> wedge. These findings can help explain the origins of secondary <span class="hlt">ice</span> wedges in modern and ancient polygons. The findings also imply that the potential for re-establishing rims in modern thermokarst-affected terrain will be limited by reduced cracking activity in the <span class="hlt">ice</span> wedges, even if regional air temperatures stabilize.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_21 --> <div id="page_22" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="421"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..1514188K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..1514188K"><span>Arctic Warming and Sea <span class="hlt">Ice</span> Diminution Herald Changing Glacier and Cryospheric Hazard Regimes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kargel, Jeffrey; Bush, Andrew; Leonard, Gregory</p> <p>2013-04-01</p> <p>The recent expansion of summertime melt <span class="hlt">zones</span> in both Greenland and some Arctic <span class="hlt">ice</span> caps, and the clearing of perennial sea <span class="hlt">ice</span> from much of the Arctic, may presage more rapid shifts in mass balances of land <span class="hlt">ice</span> than glaciologists had generally expected. The summer openings of vast stretches of open water in the Arctic, particularly in straits and the Arctic Ocean shores of the Queen Elizabeth Islands and along some Greenland coastal <span class="hlt">zones</span>, must have a large impact on summer and early autumn temperatures and precipitation now that the surface boundary condition is no longer limited by the triple-point temperature and water-vapor pressure of H2O. This state change in the Arctic probably is part of the explanation for the expanded melt <span class="hlt">zones</span> high in the Greenland <span class="hlt">ice</span> sheet. However, Greenland and the Canadian Arctic are vast regions subject to climatic influences of multiple marine bodies, and the situation with sea <span class="hlt">ice</span> and climate change remains heterogeneous, and so the local climate feedbacks from sea <span class="hlt">ice</span> diminution remain patchy. Projected forward just a few decades, it is likely that sea <span class="hlt">ice</span> will play a significant role in the Queen Elizabeth Islands and around Greenland only in the winter months. The region is in the midst of a dramatic climate change that is affecting the mass balances of the Arctic's <span class="hlt">ice</span> bodies; some polar-type glaciers must be transforming to polythermal, and polythermal ones to maritime-temperate types. Attendant with these shifts, glacier response times will shorten, the distribution and sizes of glacier lakes will change, unconsolidated debris will be debuttressed, and hazards-related dynamics will shift. Besides changes to outburst flood, debris flow, and rock avalanche occurrences, the tsunami hazard (with <span class="hlt">ice</span> and debris landslide/avalanche triggers) in glacierized fjords and the surge behaviors of many glaciers is apt to increase or shift locations. For any given location, the past is no longer the key to the present, and the present</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.C11C..05F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.C11C..05F"><span>A Decade of Arctic Sea <span class="hlt">Ice</span> Thickness Change from Airborne and Satellite Altimetry (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Farrell, S. L.; Richter-Menge, J.; Kurtz, N. T.; McAdoo, D. C.; Newman, T.; Zwally, H.; Ruth, J.</p> <p>2013-12-01</p> <p>Altimeters on both airborne and satellite platforms provide direct measurements of sea <span class="hlt">ice</span> freeboard from which sea <span class="hlt">ice</span> thickness may be calculated. Satellite altimetry observations of Arctic sea <span class="hlt">ice</span> from ICESat and CryoSat-2 indicate a significant decline in <span class="hlt">ice</span> thickness, and volume, over the last decade. During this time the <span class="hlt">ice</span> pack has experienced a rapid change in its composition, transitioning from predominantly thick, multi-year <span class="hlt">ice</span> to thinner, increasingly seasonal <span class="hlt">ice</span>. We will discuss the regional trends in <span class="hlt">ice</span> thickness derived from ICESat and <span class="hlt">Ice</span>Bridge altimetry between 2003 and 2013, contrasting observations of the multi-year <span class="hlt">ice</span> pack with seasonal <span class="hlt">ice</span> <span class="hlt">zones</span>. ICESat ceased operation in 2009, and the final, reprocessed data set became available recently. We extend our analysis to April 2013 using data from the <span class="hlt">Ice</span>Bridge airborne mission, which commenced operations in 2009. We describe our current efforts to more accurately convert from freeboard to <span class="hlt">ice</span> thickness, with a modified methodology that corrects for range errors, instrument biases, and includes an enhanced treatment of snow depth, with respect to <span class="hlt">ice</span> type. With the planned launch by NASA of ICESat-2 in 2016 we can expect continuity of the sea <span class="hlt">ice</span> thickness time series through the end of this decade. Data from the ICESat-2 mission, together with ongoing observations from CryoSat-2, will allow us to understand both the decadal trends and inter-annual variability in the Arctic sea <span class="hlt">ice</span> thickness record. We briefly present the status of planned ICESat-2 sea <span class="hlt">ice</span> data products, and demonstrate the utility of micro-pulse, photon-counting laser altimetry over sea <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2657028','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2657028"><span>Comparisons of Cubed <span class="hlt">Ice</span>, Crushed <span class="hlt">Ice</span>, and Wetted <span class="hlt">Ice</span> on Intramuscular and Surface Temperature 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>Dykstra, Joseph H; Hill, Holly M; Miller, Michael G; Cheatham, Christopher C; Michael, Timothy J; Baker, Robert J</p> <p>2009-01-01</p> <p>Context: Many researchers have investigated the effectiveness of different types of cold application, including cold whirlpools, <span class="hlt">ice</span> packs, and chemical packs. However, few have investigated the effectiveness of different types of <span class="hlt">ice</span> used in <span class="hlt">ice</span> packs, even though <span class="hlt">ice</span> is one of the most common forms of cold application. Objective: To evaluate and compare the cooling effectiveness of <span class="hlt">ice</span> packs made with cubed, crushed, and wetted <span class="hlt">ice</span> on intramuscular and skin surface temperatures. Design: Repeated-measures counterbalanced design. Setting: Human performance research laboratory. Patients or Other Participants: Twelve healthy participants (6 men, 6 women) with no history of musculoskeletal disease and no known preexisting inflammatory conditions or recent orthopaedic injuries to the lower extremities. Intervention(s): <span class="hlt">Ice</span> packs made with cubed, crushed, or wetted <span class="hlt">ice</span> were applied to a standardized area on the posterior aspect of the right gastrocnemius for 20 minutes. Each participant was given separate <span class="hlt">ice</span> pack treatments, with at least 4 days between treatment sessions. Main Outcome Measure(s): Cutaneous and intramuscular (2 cm plus one-half skinfold measurement) temperatures of the right gastrocnemius were measured every 30 seconds during a 20-minute baseline period, a 20-minute treatment period, and a 120-minute recovery period. Results: Differences were observed among all treatments. Compared with the crushed-<span class="hlt">ice</span> treatment, the cubed-<span class="hlt">ice</span> and wetted-<span class="hlt">ice</span> treatments produced lower surface and intramuscular temperatures. Wetted <span class="hlt">ice</span> produced the greatest overall temperature change during treatment and recovery, and crushed <span class="hlt">ice</span> produced the smallest change. Conclusions: As administered in our protocol, wetted <span class="hlt">ice</span> was superior to cubed or crushed <span class="hlt">ice</span> at reducing surface temperatures, whereas both cubed <span class="hlt">ice</span> and wetted <span class="hlt">ice</span> were superior to crushed <span class="hlt">ice</span> at reducing intramuscular temperatures. PMID:19295957</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.C23C0631H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.C23C0631H"><span>The kinematic response of Petermann Glacier, Greenland to <span class="hlt">ice</span> shelf perturbation</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.; Box, J. E.; Bates, R.; Nick, F.; Luckman, A. J.; van de Wal, R.; Doyle, S. H.</p> <p>2010-12-01</p> <p>The acceleration and dynamic thinning of interior <span class="hlt">zones</span> of the polar <span class="hlt">ice</span> sheets due to outlet/<span class="hlt">ice</span> shelf retreat has been identified as a factor hastening their demise and contribution to global sea-level rise. The detachment of a 275 square km area of the Petermann Glacier <span class="hlt">ice</span> shelf in August, 2010 presents a natural experiment to investigate the timing, mechanisms and efficacy of upstream dynamic feedbacks resulting from a singular but potentially significant frontal perturbation. In 2009, a permanent geodetic/differential GPS strain network logging every 10 seconds was deployed along a 200 km longitudinal profile from the <span class="hlt">ice</span> front across the grounding line extending into the interior of Petermann Glacier to characterize the system’s state before, during and after any such event. We present an overview of the geophysical measurements conducted and analyze the kinematics of the shelf detachment in relation to local environmental forcing. Finally, we discuss the postulated instantaneous and ongoing evolution in force-balance and concomitant dynamic response resulting from the perturbation along with its implications for Petermann's ongoing stability. Petermann Glacier GNSS base & telemetric GPS facility: community AA & rehab meet point. On <span class="hlt">ice</span> geodetic-GPS station flat out & reading 0 Volts</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017SPIE10466E..4ZP','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017SPIE10466E..4ZP"><span>Diurnal dynamics of the CO2 concentration in water of the coastal <span class="hlt">zone</span> of lake Baikal in the <span class="hlt">ice</span> period (testing of the DIEL - CO2 method for assessment of lake metabolic rate)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Panchenko, M. V.; Domysheva, V. M.; Pestunov, D. A.; Sakirko, M. V.; Ivanov, V. G.; Shamrin, A. M.</p> <p>2017-11-01</p> <p>Results of three long cycles of 24-hour measurements of the carbon dioxide content in the surface and bottom water in the <span class="hlt">ice</span> period of 2014-2016 in the Baikal coastal <span class="hlt">zone</span> are analyzed. The diurnal dynamics of the CO2 concentration in the subglacial water, in which photosynthesis plays the leading role, is described. It is found that, in comparison with the surface subglacial water (that is, directly adjacent to the <span class="hlt">ice</span> bottom), the more pronounced diurnal rhythm of CO2 is observed in the bottom layer in all realizations. This rhythm is well correlated with pyranometer readings. The data on the diurnal dynamics of CO2 are used to estimate the gross primary production in the bottom water with the DIEL method based on the analysis of temporal variability of the carbon dioxide concentration in water in situ.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA617621','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA617621"><span>Wave-<span class="hlt">Ice</span> and Air-<span class="hlt">Ice</span>-Ocean Interaction During the Chukchi Sea <span class="hlt">Ice</span> Edge Advance</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>During cruise CU-B UAF UW Airborne expendable <span class="hlt">Ice</span> Buoy (AXIB) Ahead, at and inside <span class="hlt">ice</span> edge Surface meteorology T, SLP ~1 year CU-B UW...Balance (IMB) buoys Inside <span class="hlt">ice</span> edge w/ >50cm thickness <span class="hlt">Ice</span> mass balance T in snow-<span class="hlt">ice</span>-ocean, T, SLP at surface ~1 year WHOI CRREL (SeaState DRI</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C24B..04Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C24B..04Z"><span>Sea <span class="hlt">Ice</span> Concentration Estimation Using Active and Passive Remote Sensing Data Fusion</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.; Zhu, T.</p> <p>2017-12-01</p> <p>In this abstract, a decision-level fusion method by utilizing SAR and passive microwave remote sensing data for sea <span class="hlt">ice</span> concentration estimation is investigated. Sea <span class="hlt">ice</span> concentration product from passive microwave concentration retrieval methods has large uncertainty within thin <span class="hlt">ice</span> <span class="hlt">zone</span>. Passive microwave data including SSM/I, AMSR-E, and AMSR-2 provide daily and long time series observations covering whole polar sea <span class="hlt">ice</span> scene, and SAR images provide rich sea <span class="hlt">ice</span> details with high spatial resolution including deformation and polarimetric features. In the proposed method, the merits from passive microwave data and SAR data are considered. Sea <span class="hlt">ice</span> concentration products from ASI and sea <span class="hlt">ice</span> category label derived from CRF framework in SAR imagery are calibrated under least distance protocol. For SAR imagery, incident angle and azimuth angle were used to correct backscattering values from slant range to ground range in order to improve geocoding accuracy. The posterior probability distribution between category label from SAR imagery and passive microwave sea <span class="hlt">ice</span> concentration product is modeled and integrated under Bayesian network, where Gaussian statistical distribution from ASI sea <span class="hlt">ice</span> concentration products serves as the prior term, which represented as an uncertainty of sea <span class="hlt">ice</span> concentration. Empirical model based likelihood term is constructed under Bernoulli theory, which meets the non-negative and monotonically increasing conditions. In the posterior probability estimation procedure, final sea <span class="hlt">ice</span> concentration is obtained using MAP criterion, which equals to minimize the cost function and it can be calculated with nonlinear iteration method. The proposed algorithm is tested on multiple satellite SAR data sets including GF-3, Sentinel-1A, RADARSAT-2 and Envisat ASAR. Results show that the proposed algorithm can improve the accuracy of ASI sea <span class="hlt">ice</span> concentration products and reduce the uncertainty along the <span class="hlt">ice</span> edge.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20170009008&hterms=sea&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsea','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20170009008&hterms=sea&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsea"><span>Variability and Trends in the Arctic Sea <span class="hlt">Ice</span> Cover: Results from Different Techniques</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.; Meier, Walter N.; Gersten, Robert</p> <p>2017-01-01</p> <p>Variability and trend studies of sea <span class="hlt">ice</span> in the Arctic have been conducted using products derived from the same raw passive microwave data but by different groups using different algorithms. This study provides consistency assessment of four of the leading products, namely, Goddard Bootstrap (SB2), Goddard NASA Team (NT1), EUMETSAT Ocean and Sea <span class="hlt">Ice</span> Satellite Application Facility (OSI-SAF 1.2), and Hadley HadISST 2.2 data in evaluating variability and trends in the Arctic sea <span class="hlt">ice</span> cover. All four provide generally similar <span class="hlt">ice</span> patterns but significant disagreements in <span class="hlt">ice</span> concentration distributions especially in the marginal <span class="hlt">ice</span> <span class="hlt">zone</span> and adjacent regions in winter and meltponded areas in summer. The discrepancies are primarily due to different ways the four techniques account for occurrences of new <span class="hlt">ice</span> and meltponding. However, results show that the different products generally provide consistent and similar representation of the state of the Arctic sea <span class="hlt">ice</span> cover. Hadley and NT1 data usually provide the highest and lowest monthly <span class="hlt">ice</span> extents, respectively. The Hadley data also show the lowest trends in <span class="hlt">ice</span> extent and <span class="hlt">ice</span> area at negative 3.88 percent decade and negative 4.37 percent decade, respectively, compared to an average of negative 4.36 percent decade and negative 4.57 percent decade for all four. Trend maps also show similar spatial distribution for all four with the largest negative trends occurring at the Kara/Barents Sea and Beaufort Sea regions, where sea <span class="hlt">ice</span> has been retreating the fastest. The good agreement of the trends especially with updated data provides strong confidence in the quantification of the rate of decline in the Arctic sea <span class="hlt">ice</span> cover.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=PIA04300&hterms=sea+world&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dsea%2Bworld','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=PIA04300&hterms=sea+world&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dsea%2Bworld"><span><span class="hlt">Ice</span> Types in the Beaufort Sea, Alaska</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>2003-01-01</p> <p><p/> Determining the amount and type of sea <span class="hlt">ice</span> in the polar oceans is crucial to improving our knowledge and understanding of polar weather and long term climate fluctuations. These views from two satellite remote sensing instruments; the synthetic aperture radar (SAR) on board the RADARSAT satellite and the Multi-angle Imaging SpectroRadiometer (MISR), illustrate different methods that may be used to assess sea <span class="hlt">ice</span> type. Sea <span class="hlt">ice</span> in the Beaufort Sea off the north coast of Alaska was classified and mapped in these concurrent images acquired March 19, 2001 and mapped to the same geographic area.<p/>To identify sea <span class="hlt">ice</span> types, the National Oceanic and Atmospheric Administration (NOAA) National <span class="hlt">Ice</span> Center constructs <span class="hlt">ice</span> charts using several data sources including RADARSAT SAR images such as the one shown at left. SAR classifies sea <span class="hlt">ice</span> types primarily by how the surface and subsurface roughness influence radar backscatter. In the SAR image, white lines delineate different sea <span class="hlt">ice</span> <span class="hlt">zones</span> as identified by the National <span class="hlt">Ice</span> Center. Regions of mostly multi-year <span class="hlt">ice</span> (A) are separated from regions with large amounts of first year and younger <span class="hlt">ice</span> (B-D), and the dashed white line at bottom marks the coastline. In general, sea <span class="hlt">ice</span> types that exhibit increased radar backscatter appear bright in SAR and are identified as rougher, older <span class="hlt">ice</span> types. Younger, smoother <span class="hlt">ice</span> types appear dark to SAR. Near the top of the SAR image, however, red arrows point to bright areas in which large, crystalline 'frost flowers' have formed on young, thin <span class="hlt">ice</span>, causing this young <span class="hlt">ice</span> type to exhibit an increased radar backscatter. Frost flowers are strongly backscattering at radar wavelengths (cm) due to both surface roughness and the high salinity of frost flowers, which causes them to be highly reflective to radar energy.<p/>Surface roughness is also registered by MISR, although the roughness observed is at a different spatial scale. Older, rougher <span class="hlt">ice</span> areas are predominantly backward scattering to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA17281.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA17281.html"><span><span class="hlt">Ice</span> Front at Venable <span class="hlt">Ice</span> Shelf</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2013-06-13</p> <p>This photo, taken onboard the Chilean Navy P3 aircraft, shows the <span class="hlt">ice</span> front of Venable <span class="hlt">Ice</span> Shelf, West Antarctica, in October 2008. It is an example of a small-size <span class="hlt">ice</span> shelf that is a large melt water producer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSHE14A1392Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSHE14A1392Z"><span>Seasonal and Interannual Variability of the Arctic Sea <span class="hlt">Ice</span>: A Comparison between AO-FVCOM and Observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Y.; Chen, C.; Beardsley, R. C.; Gao, G.; Qi, J.; Lin, H.</p> <p>2016-02-01</p> <p>A high-resolution (up to 2 km), unstructured-grid, fully <span class="hlt">ice</span>-sea coupled Arctic Ocean Finite-Volume Community Ocean Model (AO-FVCOM) was used to simulate the Arctic sea <span class="hlt">ice</span> over the period 1978-2014. Good agreements were found between simulated and observed sea <span class="hlt">ice</span> extent, concentration, drift velocity and thickness, indicating that the AO-FVCOM captured not only the seasonal and interannual variability but also the spatial distribution of the sea <span class="hlt">ice</span> in the Arctic in the past 37 years. Compared with other six Arctic Ocean models (ECCO2, GSFC, INMOM, ORCA, NAME and UW), the AO-FVCOM-simulated <span class="hlt">ice</span> thickness showed a higher correlation coefficient and a smaller difference with observations. An effort was also made to examine the physical processes attributing to the model-produced bias in the sea <span class="hlt">ice</span> simulation. The error in the direction of the <span class="hlt">ice</span> drift velocity was sensitive to the wind turning angle; smaller when the wind was stronger, but larger when the wind was weaker. This error could lead to the bias in the near-surface current in the fully or partially <span class="hlt">ice</span>-covered <span class="hlt">zone</span> where the <span class="hlt">ice</span>-sea interfacial stress was a major driving force.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C21A0698B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C21A0698B"><span>Looking Into and Through the Ross <span class="hlt">Ice</span> Shelf - ROSETTA-<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>Bell, R. E.</p> <p>2015-12-01</p> <p>Our current understanding of the structure and stability of the Ross <span class="hlt">Ice</span> Shelf is based on satellite studies of the <span class="hlt">ice</span> surface and the 1970's RIGGS program. The study of the flowlines evident in the MODIS imagery combined with surface geophysics has revealed a complex history with <span class="hlt">ice</span> streams Mercer, Whillans and Kamb changing velocity over the past 1000 years. Here, we present preliminary <span class="hlt">Ice</span>Pod and <span class="hlt">Ice</span>Bridge radar data acquired in December 2014 and November 2013 across the Ross <span class="hlt">Ice</span> Shelf that show clearly, for the first time, the structure of the <span class="hlt">ice</span> shelf and provide insights into <span class="hlt">ice</span>-ocean interaction. The three major layers of the <span class="hlt">ice</span> shelf are (1) the continental meteoric <span class="hlt">ice</span> layer), <span class="hlt">ice</span> formed on the grounded <span class="hlt">ice</span> sheet that entered the <span class="hlt">ice</span> shelf where <span class="hlt">ice</span> streams and outlet glaciers crossed the grounding line (2) the locally accumulating meteoric <span class="hlt">ice</span> layer, <span class="hlt">ice</span> and snow that forms from snowfall on the floating <span class="hlt">ice</span> shelf and (3) a basal marine <span class="hlt">ice</span> layer. The locally accumulating meteoric <span class="hlt">ice</span> layer contains well-defined internal layers that are generally parallel to the <span class="hlt">ice</span> surface and thickens away from the grounding line and reaches a maximum thickness of 220m along the line crossing Roosevelt Island. The continental meteoric layer is located below a broad irregular internal reflector, and is characterized by irregular internal layers. These internal layers are often folded, likely a result of deformation as the <span class="hlt">ice</span> flowed across the grounding line. The basal marine <span class="hlt">ice</span> layer, up to 50m thick, is best resolved in locations where basal crevasses are present, and appears to thicken along the flow at rates of decimeters per year. Each individual flowband of the <span class="hlt">ice</span> shelf contains layers that are distinct in their structure. For example, the thickness of the locally accumulated layer is a function of both the time since crossing the grounding line and the thickness of the incoming <span class="hlt">ice</span>. Features in the meteoric <span class="hlt">ice</span>, such as distinct folds, can be traced between</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040171503','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040171503"><span>Elevation Changes of <span class="hlt">Ice</span> Caps in the Canadian Arctic Archipelago</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Abdalati, W.; Krabill, W.; Frederick, E.; Manizade, S.; Martin, C.; Sonntag, J.; Swift, R.; Thomas, R.; Yungel, J.; Koerner, R.</p> <p>2004-01-01</p> <p>Precise repeat airborne laser surveys were conducted over the major <span class="hlt">ice</span> caps in the Canadian Arctic Archipelago in the spring of 1995 and 2000 in order to measure elevation changes in the region. Our measurements reveal thinning at lower elevations (below 1600 m) on most of the <span class="hlt">ice</span> caps and glaciers, but either very little change or thickening at higher elevations in the <span class="hlt">ice</span> cap accumulation <span class="hlt">zones</span>. Recent increases in precipitation in the area can account for the slight thickening where it was observed, but not for the thinning at lower elevations. For the northern <span class="hlt">ice</span> caps on the Queen Elizabeth Islands, thinning was generally less than 0.5 m/yr , which is consistent with what would be expected from the warm temperature anomalies in the region for the 5-year period between surveys and appears to be a continuation of a trend that began in the mid 1980s. Further south, however, on the Barnes and Penny <span class="hlt">ice</span> caps on Baffin Island, this thinning was much more pronounced at over 1 m/yr in the lower elevations. Here temperature anomalies were very small, and the thinning at low elevations far exceeds any associated enhanced ablation. The observations on Barnes, and perhaps Penny are consistent with the idea that the observed thinning is part of a much longer term deglaciation, as has been previously suggested for Barnes <span class="hlt">Ice</span> Cap. Based on the regional relationships between elevation and elevation-change in our data, the 1995-2000 mass balance for the region is estimated to be 25 cu km/yr of <span class="hlt">ice</span>, which corresponds to a sea level increase of 0.064 mm/ yr . This places it among the more significant sources of eustatic sea level rise, though not as substantial as Greenland <span class="hlt">ice</span> sheet, Alaskan glaciers, or the Patagonian <span class="hlt">ice</span> fields.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMED33D0965N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMED33D0965N"><span>Validation of the Antarctic Snow Accumulation and <span class="hlt">Ice</span> Discharge Basal Stress Boundary in the South Eastern Region of the Ross <span class="hlt">Ice</span> Shelf, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nelson, C. B.; King, K.</p> <p>2015-12-01</p> <p>The largest <span class="hlt">ice</span> shelf in Antarctic, Ross <span class="hlt">Ice</span> Shelf, was investigated over the years of (1970-2015). Near the basal stress boundary between the <span class="hlt">ice</span> shelf and the West Antarctic <span class="hlt">ice</span> sheet, <span class="hlt">ice</span> velocity ranges from a few meters per year to several hundred meters per year in <span class="hlt">ice</span> streams. Most of the drainage from West Antarctica into the Ross <span class="hlt">Ice</span> Shelf flows down two major <span class="hlt">ice</span> streams, each of which discharges more than 20 km3 of <span class="hlt">ice</span> each year. Along with velocity changes, the warmest water below parts of the Ross <span class="hlt">Ice</span> Shelf resides in the lowest portion of the water column because of its high salinity. Vertical mixing caused by tidal stirring can thus induce ablation by lifting the warm water into contact with the <span class="hlt">ice</span> shelf. This process can cause melting over a period of time and eventually cause breakup of <span class="hlt">ice</span> shelf. With changes occurring over many years a validation is needed for the Antarctic Snow Accumulation and <span class="hlt">Ice</span> Discharge (ASAID) basal stress boundary created in 2003. After the 2002 Larsen B <span class="hlt">Ice</span> Shelf disintegration, nearby glaciers in the Antarctic Peninsula accelerated up to eight times their original speed over the next 18 months. Similar losses of <span class="hlt">ice</span> tongues in Greenland have caused speed-ups of two to three times the flow rates in just one year. Rapid changes occurring in regions surrounding Antarctica are causing concern in the polar science community to research changes occurring in coastal <span class="hlt">zones</span> over time. During the research, the team completed study on the Ross <span class="hlt">Ice</span> Shelf located on the south western coast of the Antarctic. The study included a validation of the ABSB vs. the natural basal stress boundary (NBSB) along the Ross <span class="hlt">Ice</span> Shelf. The ASAID BSB was created in 2003 by a team of researchers headed by National Aeronautics and Space Administration Goddard Space Flight Center (NASA GSFC), with an aim of studying coastal deviations as it pertains to the mass balance of the entire continent. The point data file was aimed at creating a replica of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C21D..08R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C21D..08R"><span>Extensive massive basal-<span class="hlt">ice</span> structures in West Antarctica relate to <span class="hlt">ice</span>-sheet anisotropy and <span class="hlt">ice</span>-flow</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ross, N.; Bingham, R. G.; Corr, H. F. J.; Siegert, M. J.</p> <p>2016-12-01</p> <p>Complex structures identified within both the East Antarctic and Greenland <span class="hlt">ice</span> sheets are thought to be generated by the action of basal water freezing to the <span class="hlt">ice</span>-sheet base, evolving under <span class="hlt">ice</span> flow. Here, we use <span class="hlt">ice</span>-penetrating radar to image an extensive series of similarly complex basal <span class="hlt">ice</span> facies in West Antarctica, revealing a thick (>500 m) tectonised unit in an area of cold-based and relatively slow-flowing <span class="hlt">ice</span>. We show that major folding and overturning of the unit perpendicular to <span class="hlt">ice</span> flow elevates deep, warm <span class="hlt">ice</span> into the mid <span class="hlt">ice</span>-sheet column. Fold axes align with present <span class="hlt">ice</span> flow, and axis amplitudes increase down-<span class="hlt">ice</span>, suggesting long-term consistency in the direction and convergence of flow. In the absence of basal water, and the draping of the tectonised unit over major subglacial mountain ranges, the formation of the unit must be solely through the deformation of meteoric <span class="hlt">ice</span>. Internal layer radar reflectivity is consistently greater parallel to flow compared with the perpendicular direction, revealing <span class="hlt">ice</span>-sheet crystal anisotropy is associated with the folding. By linking layers to the Byrd <span class="hlt">ice</span>-core site, we show the basal <span class="hlt">ice</span> dates to at least the last glacial cycle and may be as old as the last interglacial. Deformation of deep-<span class="hlt">ice</span> in this sector of WAIS, and potentially elsewhere in Antarctica, may be caused by differential shearing at interglacial-glacial boundaries, in a process analogous to that proposed for interior Greenland. The scale and heterogeneity of the englacial structures, and their subsequent impact on <span class="hlt">ice</span> sheet rheology, means that the nature of <span class="hlt">ice</span> flow across the bulk of West Antarctica must be far more complex that is currently accounted for by any numerical <span class="hlt">ice</span> sheet model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19980017788','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19980017788"><span>Comparison of Retracking Algorithms Using Airborne Radar and Laser Altimeter Measurements 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>Ferraro, Ellen J.; Swift, Calvin T.</p> <p>1995-01-01</p> <p>This paper compares four continental <span class="hlt">ice</span> sheet radar altimeter retracking algorithms using airborne radar and laser altimeter data taken over the Greenland <span class="hlt">ice</span> sheet in 1991. The refurbished Advanced Application Flight Experiment (AAFE) airborne radar altimeter has a large range window and stores the entire return waveform during flight. Once the return waveforms are retracked, or post-processed to obtain the most accurate altitude measurement possible, they are compared with the high-precision Airborne Oceanographic Lidar (AOL) altimeter measurements. The AAFE waveforms show evidence of varying degrees of both surface and volume scattering from different regions of the Greenland <span class="hlt">ice</span> sheet. The AOL laser altimeter, however, obtains a return only from the surface of the <span class="hlt">ice</span> sheet. Retracking altimeter waveforms with a surface scattering model results in a good correlation with the laser measurements in the wet and dry-snow <span class="hlt">zones</span>, but in the percolation region of the <span class="hlt">ice</span> sheet, the deviation between the two data sets is large due to the effects of subsurface and volume scattering. The Martin et al model results in a lower bias than the surface scattering model, but still shows an increase in the noise level in the percolation <span class="hlt">zone</span>. Using an Offset Center of Gravity algorithm to retrack altimeter waveforms results in measurements that are only slightly affected by subsurface and volume scattering and, despite a higher bias, this algorithm works well in all regions of the <span class="hlt">ice</span> sheet. A cubic spline provides retracked altitudes that agree with AOL measurements over all regions of Greenland. This method is not sensitive to changes in the scattering mechanisms of the <span class="hlt">ice</span> sheet and it has the lowest noise level and bias of all the retracking methods presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150002346','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150002346"><span><span class="hlt">Ice</span> Roughness in Short Duration SLD <span class="hlt">Icing</span> Events</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>McClain, Stephen T.; Reed, Dana; Vargas, Mario; Kreeger, Richard E.; Tsao, Jen-Ching</p> <p>2014-01-01</p> <p><span class="hlt">Ice</span> accretion codes depend on models of roughness parameters to account for the enhanced heat transfer during the <span class="hlt">ice</span> accretion process. While mitigating supercooled large droplet (SLD or Appendix O) <span class="hlt">icing</span> is a significant concern for manufacturers seeking future vehicle certification due to the pending regulation, historical <span class="hlt">ice</span> roughness studies have been performed using Appendix C <span class="hlt">icing</span> clouds which exhibit mean volumetric diameters (MVD) much smaller than SLD clouds. Further, the historical studies of roughness focused on extracting parametric representations of <span class="hlt">ice</span> roughness using multiple images of roughness elements. In this study, the <span class="hlt">ice</span> roughness developed on a 21-in. NACA 0012 at 0deg angle of attack exposed to short duration SLD <span class="hlt">icing</span> events was measured in the <span class="hlt">Icing</span> Research Tunnel at the NASA Glenn Research Center. The MVD's used in the study ranged from 100 micrometer to 200 micrometers, in a 67 m/s flow, with liquid water contents of either 0.6 gm/cubic meters or 0.75 gm/cubic meters. The <span class="hlt">ice</span> surfaces were measured using a Romer Absolute Arm laser scanning system. The roughness associated with each surface point cloud was measured using the two-dimensional self-organizing map approach developed by McClain and Kreeger (2013) resulting in statistical descriptions of the <span class="hlt">ice</span> roughness.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C11A0898S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C11A0898S"><span>The feasibility of imaging subglacial hydrology beneath <span class="hlt">ice</span> streams with ground-based electromagnetics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Siegfried, M. R.; Key, K.</p> <p>2017-12-01</p> <p>Subglacial hydrologic systems in Antarctica and Greenland play a fundamental role in <span class="hlt">ice</span>-sheet dynamics, yet critical aspects of these systems remain poorly understood due to a lack of observations. Ground-based electromagnetic (EM) geophysical methods are established for mapping groundwater in many environments, but have never been applied to imaging lakes beneath <span class="hlt">ice</span> sheets. Here we study the feasibility of passive and active source EM imaging for quantifying the nature of subglacial water systems beneath <span class="hlt">ice</span> streams, with an emphasis on the interfaces between <span class="hlt">ice</span> and basal meltwater, as well as deeper groundwater in the underlying sediments. Specifically, we look at the passive magnetotelluric method and active-source EM methods that use a large loop transmitter and receivers that measure either frequency-domain or transient soundings. We describe a suite of model studies that exam the data sensitivity as a function of <span class="hlt">ice</span> thickness, water conductivity and hydrologic system geometry for models representative of a subglacial lake and a grounding <span class="hlt">zone</span> estuary. We show that EM data are directly sensitive to groundwater and can image its lateral and depth extent. By combining the conductivity obtained from EM data with <span class="hlt">ice</span> thickness and geological structure from conventional geophysical techniques such as ground-penetrating radar and active seismic techniques, EM data have the potential to provide new insights on the interaction between <span class="hlt">ice</span>, rock, and water at critical <span class="hlt">ice</span>-sheet boundaries.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2575336','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2575336"><span>Southern Ocean frontal structure and sea-<span class="hlt">ice</span> formation rates revealed by elephant seals</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Charrassin, J.-B.; Hindell, M.; Rintoul, S. R.; Roquet, F.; Sokolov, S.; Biuw, M.; Costa, D.; Boehme, L.; Lovell, P.; Coleman, R.; Timmermann, R.; Meijers, A.; Meredith, M.; Park, Y.-H.; Bailleul, F.; Goebel, M.; Tremblay, Y.; Bost, C.-A.; McMahon, C. R.; Field, I. C.; Fedak, M. A.; Guinet, C.</p> <p>2008-01-01</p> <p>Polar regions are particularly sensitive to climate change, with the potential for significant feedbacks between ocean circulation, sea <span class="hlt">ice</span>, and the ocean carbon cycle. However, the difficulty in obtaining in situ data means that our ability to detect and interpret change is very limited, especially in the Southern Ocean, where the ocean beneath the sea <span class="hlt">ice</span> remains almost entirely unobserved and the rate of sea-<span class="hlt">ice</span> formation is poorly known. Here, we show that southern elephant seals (Mirounga leonina) equipped with oceanographic sensors can measure ocean structure and water mass changes in regions and seasons rarely observed with traditional oceanographic platforms. In particular, seals provided a 30-fold increase in hydrographic profiles from the sea-<span class="hlt">ice</span> <span class="hlt">zone</span>, allowing the major fronts to be mapped south of 60°S and sea-<span class="hlt">ice</span> formation rates to be inferred from changes in upper ocean salinity. Sea-<span class="hlt">ice</span> production rates peaked in early winter (April–May) during the rapid northward expansion of the pack <span class="hlt">ice</span> and declined by a factor of 2 to 3 between May and August, in agreement with a three-dimensional coupled ocean–sea-<span class="hlt">ice</span> model. By measuring the high-latitude ocean during winter, elephant seals fill a “blind spot” in our sampling coverage, enabling the establishment of a truly global ocean-observing system. PMID:18695241</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20090035004&hterms=rate+sensitivity+ice&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Drate%2Bsensitivity%2Bice','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20090035004&hterms=rate+sensitivity+ice&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Drate%2Bsensitivity%2Bice"><span>Understanding <span class="hlt">Ice</span> Supersaturation, Particle Growth, and Number Concentration in Cirrus Clouds</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Comstock, Jennifer M.; Lin, Ruei-Fong; Starr, David O'C.; Yang, Ping</p> <p>2008-01-01</p> <p>Many factors control the <span class="hlt">ice</span> supersaturation and microphysical properties in cirrus clouds. We explore the effects of dynamic forcing, <span class="hlt">ice</span> nucleation mechanisms, and <span class="hlt">ice</span> crystal growth rate on the evolution and distribution of water vapor and cloud properties in nighttime cirrus clouds using a one-dimensional cloud model with bin microphysics and remote sensing measurements obtained at the Department of Energy's Atmospheric Radiation Measurement (ARM) Climate Research Facility located near Lamont, OK. We forced the model using both large-scale vertical ascent and, for the first time, mean mesoscale velocity derived from radar Doppler velocity measurements. Both heterogeneous and homogeneous nucleation processes are explored, where a classical theory heterogeneous scheme is compared with empirical representations. We evaluated model simulations by examining both bulk cloud properties and distributions of measured radar reflectivity, lidar extinction, and water vapor profiles, as well as retrieved cloud microphysical properties. Our results suggest that mesoscale variability is the primary mechanism needed to reproduce observed quantities. Model sensitivity to the <span class="hlt">ice</span> growth rate is also investigated. The most realistic simulations as compared with observations are forced using mesoscale waves, include fast <span class="hlt">ice</span> crystal growth, and initiate <span class="hlt">ice</span> by either homogeneous or heterogeneous nucleation. Simulated <span class="hlt">ice</span> crystal number concentrations (tens to hundreds particles per liter) are typically two orders of magnitude smaller than previously published results based on aircraft measurements in cirrus clouds, although higher concentrations are possible in isolated pockets within the nucleation <span class="hlt">zone</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://www.dtic.mil/docs/citations/AD1013703','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1013703"><span>Quantifying the Role of Atmospheric Forcing in <span class="hlt">Ice</span> Edge Retreat and Advance Including Wind-Wave Coupling</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>Quantifying the Role of Atmospheric Forcing in <span class="hlt">Ice</span> Edge Retreat and Advance Including Wind- Wave Coupling Peter S. Guest (NPS Technical Contact) Naval...surface fluxes and ocean waves in coupled models in the Beaufort and Chukchi Seas. 2. Understand the physics of heat and mass transfer from the ocean...to the atmosphere. 3. Improve forecasting of waves on the open ocean and in the marginal <span class="hlt">ice</span> <span class="hlt">zone</span>. 2 OBJECTIVES 1. Quantifying the open-ocean</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C41E0726K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C41E0726K"><span>Quantifying Local Ablation Rates for the Greenland <span class="hlt">Ice</span> Sheet Using Terrestrial LIDAR</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kershner, C. M.; Pitcher, L. H.; LeWinter, A.; Finnegan, D. C.; Overstreet, B. T.; Miège, C.; Cooper, M. G.; Smith, L. C.; Rennermalm, A. K.</p> <p>2016-12-01</p> <p>Quantifying accurate <span class="hlt">ice</span> surface ablation or melt rates for the Greenland <span class="hlt">Ice</span> Sheet is important for calibrating and validating surface mass balance models and constraining sea level rise estimates. Common practice is to monitor surface ablation at defined points by manually measuring <span class="hlt">ice</span> surface lowering in relation to stakes inserted into the <span class="hlt">ice</span> / snow. However, this method does not account for the effects of local topography, solar zenith angle, and local variations in <span class="hlt">ice</span> surface albedo/impurities on ablation rates. To directly address these uncertainties, we use a commercially available terrestrial LIDAR scanner (TLS) to monitor daily melt rates in the ablation <span class="hlt">zone</span> of the Greenland <span class="hlt">Ice</span> Sheet for 7 consecutive days in July 2016. Each survey is registered to previous scans using retroreflective cylinders and is georeferenced using static GPS measurements. Bulk ablation will be calculated using multi-temporal differential LIDAR techniques, and difficulties in referencing scans and collecting high quality surveys in this dynamic environment will be discussed, as well as areas for future research. We conclude that this novel application of TLS technology provides a spatially accurate, higher fidelity measurements of ablation across a larger area with less interpolation and less time spent than using traditional manual point based methods alone. Furthermore, this sets the stage for direct calibration, validation and cross-comparison with existing airborne (e.g. NASA's Airborne Topographic Mapper - ATM - onboard Operation <span class="hlt">Ice</span>Bridge and NASA's Land, Vegetation & <span class="hlt">Ice</span> Sensor - LVIS) and forthcoming spaceborne sensors (e.g. NASA's ICESat-2).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1013732','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1013732"><span>Wave-<span class="hlt">Ice</span> and Air-<span class="hlt">Ice</span>-Ocean Interaction During the Chukchi Sea <span class="hlt">Ice</span> Edge Advance</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>1 DISTRIBUTION STATEMENT A. Approved for public release; distribution is unlimited. Wave -<span class="hlt">Ice</span> and Air-<span class="hlt">Ice</span>-Ocean Interaction During the...Chukchi Sea in the late summer have potentially changed the impact of fall storms by creating wave fields in the vicinity of the advancing <span class="hlt">ice</span> edge. A...first) wave -<span class="hlt">ice</span> interaction field experiment that adequately documents the relationship of a growing pancake <span class="hlt">ice</span> cover with a time and space varying</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=67181&keyword=LAKE+AND+ICE&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=67181&keyword=LAKE+AND+ICE&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>SIMULATED CLIMATE CHANGE EFFECTS ON DISSOLVED OXYGEN CHARACTERISTICS IN <span class="hlt">ICE</span>-COVERED LAKES. (R824801)</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>A deterministic, one-dimensional model is presented which simulates daily dissolved oxygen (DO) profiles and associated water temperatures, <span class="hlt">ice</span> covers and snow covers for dimictic and polymictic lakes of the temperate <span class="hlt">zone</span>. The lake parameters required as model input are surface ...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990071137&hterms=ice+mechanics&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dice%2Bmechanics','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990071137&hterms=ice+mechanics&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dice%2Bmechanics"><span><span class="hlt">Ice</span> Flow in the North East Greenland <span class="hlt">Ice</span> Stream</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Joughin, Ian; Kwok, Ron; Fahnestock, M.; MacAyeal, Doug</p> <p>1999-01-01</p> <p>Early observations with ERS-1 SAR image data revealed a large <span class="hlt">ice</span> stream in North East Greenland (Fahnestock 1993). The <span class="hlt">ice</span> stream has a number of the characteristics of the more closely studied <span class="hlt">ice</span> streams in Antarctica, including its large size and gross geometry. The onset of rapid flow close to the <span class="hlt">ice</span> divide and the evolution of its flow pattern, however, make this <span class="hlt">ice</span> stream unique. These features can be seen in the balance velocities for the <span class="hlt">ice</span> stream (Joughin 1997) and its outlets. The <span class="hlt">ice</span> stream is identifiable for more than 700 km, making it much longer than any other flow feature in Greenland. Our research goals are to gain a greater understanding of the <span class="hlt">ice</span> flow in the northeast Greenland <span class="hlt">ice</span> stream and its outlet glaciers in order to assess their impact on the past, present, and future mass balance of the <span class="hlt">ice</span> sheet. We will accomplish these goals using a combination of remotely sensed data and <span class="hlt">ice</span> sheet models. We are using satellite radar interferometry data to produce a complete maps of velocity and topography over the entire <span class="hlt">ice</span> stream. We are in the process of developing methods to use these data in conjunction with existing <span class="hlt">ice</span> sheet models similar to those that have been used to improve understanding of the mechanics of flow in Antarctic <span class="hlt">ice</span> streams.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C32B..06D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C32B..06D"><span>Discrete-element simulation of sea-<span class="hlt">ice</span> mechanics: Contact mechanics and granular jamming</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Damsgaard, A.; Adcroft, A.; Sergienko, O. V.; Stern, A. A.</p> <p>2017-12-01</p> <p>Lagrangian models of sea-<span class="hlt">ice</span> dynamics offer several advantages to Eulerian continuum methods. Spatial discretization on the <span class="hlt">ice</span>-floe scale is natural for Lagrangian models, which additionally offer the convenience of being able to handle arbitrary sea-<span class="hlt">ice</span> concentrations. This is likely to improve model performance in <span class="hlt">ice</span>-marginal <span class="hlt">zones</span> with strong advection. Furthermore, phase transitions in granular rheology around the jamming limit, such as observed when sea <span class="hlt">ice</span> moves through geometric confinements, includes sharp thresholds in effective viscosity which are typically ignored in Eulerian models. Granular jamming is a stochastic process dependent on having the right grains in the right place at the right time, and the jamming likelihood over time can be described by a probabilistic model. Difficult to parameterize in continuum formulations, jamming occurs naturally in dense granular systems simulated in a Lagrangian framework, and is a very relevant process controlling sea-<span class="hlt">ice</span> transport through narrow straits. We construct a flexible discrete-element framework for simulating Lagrangian sea-<span class="hlt">ice</span> dynamics at the <span class="hlt">ice</span>-floe scale, forced by ocean and atmosphere velocity fields. Using this framework, we demonstrate that frictionless contact models based on compressive stiffness alone are unlikely to jam, and describe two different approaches based on friction and tensile strength which both result in increased bulk shear strength of the granular assemblage. The frictionless but cohesive contact model, with certain tensile strength values, can display jamming behavior which on the large scale is very similar to a more complex and realistic model with contact friction and <span class="hlt">ice</span>-floe rotation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1996JGR...10120809K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1996JGR...10120809K"><span>Atmospheric and oceanic forcing of Weddell Sea <span class="hlt">ice</span> motion</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kottmeier, C.; Sellmann, Lutz</p> <p>1996-09-01</p> <p>The data from sea <span class="hlt">ice</span> buoys, which were deployed during the Winter Weddell Sea Project 1986, the Winter Weddell Gyre Studies 1989 and 1992, the <span class="hlt">Ice</span> Station Weddell in 1992, the Antarctic <span class="hlt">Zone</span> Flux Experiment in 1994, and several ship cruises in Austral summers, are uniformly reanalyzed by the same objective methods. Geostrophic winds are derived after matching of the buoy pressure data with the surface pressure fields of the European Centre for Medium Range Weather Forecasts. The ratio between <span class="hlt">ice</span> drift and geostrophic wind speeds is reduced when winds and currents oppose each other, when the atmospheric surface layer is stably stratified, and when the <span class="hlt">ice</span> is under pressure near coasts. Over the continental shelves, the spatial inhomogeneity of tidal and inertial motion effectively controls the variability of divergence for periods below 36 hours. Far from coasts, speed ratios, which presumably reflect internal stress variations in the <span class="hlt">ice</span> cover, are independent of drift divergence on the spatial scale of 100 km. To study basin-scale <span class="hlt">ice</span> dynamics, all <span class="hlt">ice</span> drift data are related to the geostrophic winds based on the complex linear model [Thorndike and Colony, 1982] for daily averaged data. The composite patterns of mean <span class="hlt">ice</span> motion, geostrophic winds, and geostrophic surface currents document cyclonic basin-wide circulations. Geostrophic ocean currents are generally small in the Weddell Sea. Significant features are the coastal current near the southeastern coasts and the bands of larger velocities of ≈6 cm s-1 following the northward and eastward orientation of the continental shelf breaks in the western and northwestern Weddell Sea. In the southwestern Weddell Sea the mean <span class="hlt">ice</span> drift speed is reduced to less than 0.5% of the geostrophic wind speed and increases rather continuously to 1.5% in the northern, central, and eastern Weddell Sea. The linear model accounts for less than 50% of the total variance of drift speeds in the southwestern Weddell Sea and up to 80</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010DyAtO..49..215W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010DyAtO..49..215W"><span>On the estimation of <span class="hlt">ice</span> thickness from scattering observations</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. D.; Squire, V. A.</p> <p>2010-04-01</p> <p>This paper is inspired by the proposition that it may be possible to extract descriptive physical parameters - in particular the <span class="hlt">ice</span> thickness, of a sea-<span class="hlt">ice</span> field from ocean wave information. The motivation is that mathematical theory describing wave propagation in such media has reached a point where the inherent heterogeneity, expressed as pressure ridge keels and sails, leads, thickness variations and changes of material property and draught, can be fully assimilated exactly or through approximations whose limitations are understood. On the basis that leads have the major wave scattering effect for most sea-<span class="hlt">ice</span> [Williams, T.D., Squire, V.A., 2004. Oblique scattering of plane flexural-gravity waves by heterogeneities in sea <span class="hlt">ice</span>. Proc. R. Soc. Lon. Ser.-A 460 (2052), 3469-3497], a model two dimensional sea-<span class="hlt">ice</span> sheet composed of a large number of such features, randomly dispersed, is constructed. The wide spacing approximation is used to predict how wave trains of different period will be affected, after first establishing that this produces results that are very close to the exact solution. Like Kohout and Meylan [Kohout, A.L., Meylan, M.H., 2008. An elastic plate model for wave attenuation and <span class="hlt">ice</span> floe breaking in the marginal <span class="hlt">ice</span> <span class="hlt">zone</span>. J. Geophys. Res. 113, C09016, doi:10.1029/2007JC004434], we find that on average the magnitude of a wave transmitted by a field of leads decays exponentially with the number of leads. Then, by fitting a curve based on this assumption to the data, the thickness of the <span class="hlt">ice</span> sheet is obtained. The attenuation coefficient can always be calculated numerically by ensemble averaging but in some cases more rapidly computed approximations work extremely well. Moreover, it is found that the underlying thickness can be determined to good accuracy by the method as long as Archimedean draught is correctly provided for, suggesting that waves can indeed be effective as a remote sensing agent to measure <span class="hlt">ice</span> thickness in areas where pressure ridges</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.C21B0322Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.C21B0322Z"><span>Sensing the bed-rock movement due to <span class="hlt">ice</span> unloading from space using InSAR time-series</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhao, W.; Amelung, F.; Dixon, T. H.; Wdowinski, S.</p> <p>2014-12-01</p> <p><span class="hlt">Ice</span>-sheets in the Arctic region are retreating rapidly since late 1990s. Typical <span class="hlt">ice</span> loss rates are 0.5 - 1 m/yr at the Canadian Arctic Archipelago, ~ 1 m/yr at the Icelandic <span class="hlt">ice</span> sheets, and several meters per year at the edge of Greenland <span class="hlt">ice</span> sheet. Such load decreasing causes measurable (several millimeter per year) deformation of the Earth's crust from Synthetic Aperture Radar Interferometry (InSAR). Using small baseline time-series analysis, this signal is retrieved after noises such as orbit error, atmospheric delay and DEM error being removed. We present results from Vatnajokull <span class="hlt">ice</span> cap, Petermann glacier and Barnes <span class="hlt">ice</span> cap using ERS, Envisat and TerraSAR-X data. Up to 2 cm/yr relative radar line-of-sight displacement is detected. The pattern of deformation matches the shape of <span class="hlt">ice</span> sheet very well. The result in Iceland was used to develop a new model for the <span class="hlt">ice</span> mass balance estimation from 1995 to 2010. Other applications of this kind of technique include validation of ICESat or GRACE based <span class="hlt">ice</span> sheet model, Earth's rheology (Young's modulus, viscosity and so on). Moreover, we find a narrow (~ 1km) uplift <span class="hlt">zone</span> close to the periglacial area of Petermann glacier which may due to a special rheology under the <span class="hlt">ice</span> stream.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19850009740','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19850009740"><span><span class="hlt">Icing</span> flight research: Aerodynamic effects of <span class="hlt">ice</span> and <span class="hlt">ice</span> shape documentation with stereo photography</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mikkelsen, K. L.; Mcknight, R. C.; Ranaudo, R. J.; Perkins, P. J., Jr.</p> <p>1985-01-01</p> <p>Aircraft <span class="hlt">icing</span> flight research was performed in natural <span class="hlt">icing</span> conditions. A data base consisting of <span class="hlt">icing</span> cloud measurements, <span class="hlt">ice</span> shapes, and aerodynamic measurements is being developed. During research <span class="hlt">icing</span> encounters the <span class="hlt">icing</span> cloud was continuously measured. After the encounter, the <span class="hlt">ice</span> accretion shapes on the wing were documented with a stereo camera system. The increase in wing section drag was measured with a wake survey probe. The overall aircraft performance loss in terms of lift and drag coefficient changes was obtained by steady level speed/power measurements. Selective deicing of the airframe components was performed to determine their contributions to the total drag increase. Engine out capability in terms of power available was analyzed for the <span class="hlt">iced</span> aircraft. It was shown that the stereo photography system can be used to document <span class="hlt">ice</span> shapes in flight and that the wake survey probe can measure increases in wing section drag caused by <span class="hlt">ice</span>. On one flight, the wing section drag coefficient (c sub d) increased approximately 120 percent over the uniced baseline at an aircraft angle of attack of 6 deg. On another flight, the aircraft darg coefficient (c sub d) increased by 75 percent over the uniced baseline at an aircraft lift coefficient (C sub d) of 0.5.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19850048041&hterms=photography&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DTitle%26N%3D0%26No%3D90%26Ntt%3Dphotography','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19850048041&hterms=photography&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DTitle%26N%3D0%26No%3D90%26Ntt%3Dphotography"><span><span class="hlt">Icing</span> flight research - Aerodynamic effects of <span class="hlt">ice</span> and <span class="hlt">ice</span> shape documentation with stereo photography</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mikkelsen, K. L.; Mcknight, R. C.; Ranaudo, R. J.; Perkins, P. J., Jr.</p> <p>1985-01-01</p> <p>Aircraft <span class="hlt">icing</span> flight research was performed in natural <span class="hlt">icing</span> conditions. A data base consisting of <span class="hlt">icing</span> cloud measurements, <span class="hlt">ice</span> shapes, and aerodynamic measurements is being developed. During research <span class="hlt">icing</span> encounters the <span class="hlt">icing</span> cloud was continuously measured. After the encounter, the <span class="hlt">ice</span> accretion shapes on the wing were documented with a stereo camera system. The increase in wing section drag was measured with a wake survey probe. The overall aircraft performance loss in terms of lift and drag coefficient changes were obtained by steady level speed/power measurements. Selective deicing of the airframe components was performed to determine their contributions to the total drag increase. Engine out capability in terms of power available was analyzed for the <span class="hlt">iced</span> aircraft. It was shown that the stereo photography system can be used to document <span class="hlt">ice</span> shapes in flight and that the wake survey probe can measure increases in wing section drag caused by <span class="hlt">ice</span>. On one flight, the wing section drag coefficient (c sub d) increased approximately 120 percent over the uniced baseline at an aircraft angle of attack of 6 deg. On another flight, the aircraft drag coefficient (c sub d) increased by 75 percent over the uniced baseline at an aircraft lift coefficient (c sub d) of 0.5.</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 activity 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 <span class="hlt">zone</span> 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 margin, as did both cell numbers and activity rates before reaching a peak (photosynthesis) or a plateau (respiration, abundance) between 10 and 20 km from the margin. 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 <span class="hlt">zones</span>', confirmed by a redundancy analysis (RDA) using physical data as predictors. RDA using data from the largest 'bare <span class="hlt">ice</span> <span class="hlt">zone</span>' 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('http://adsabs.harvard.edu/abs/2017EGUGA..1915875W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1915875W"><span>SAR <span class="hlt">ice</span> thickness mapping in the Beaufort Sea during autumn 2015 using wave dispersion in pancake <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>Wadhams, Peter; Aulicino, Giuseppe; Parmiggiani, Flavio</p> <p>2017-04-01</p> <p>Pancake and frazil <span class="hlt">ice</span> represent an important component of the Arctic and Antarctic cryosphere, especially in the Marginal <span class="hlt">Ice</span> <span class="hlt">Zones</span>. In particular, pancake <span class="hlt">ice</span> is the result of a freezing process that takes place in turbulent surface conditions, typically associated with wind and wave fields. The retrieval of its thickness by remote sensing is, in general, a very difficult task. This study presents our ongoing work in the EU SPICES project, in which we aim to use the results of theory and observations developed so far in order to refine a processing system for routinely deriving <span class="hlt">ice</span> thicknesses in frazil-pancake regions of the Arctic and Antarctic. The change in dispersion of ocean waves as they penetrate into pancake icefield is analyzed in order to derive <span class="hlt">ice</span> thickness estimation. The spectral changes in wave spectra from imagery provided by space-borne SAR systems (mainly Cosmo-SkyMed and Sentinel-1 satellites) is used to retrieve pancake <span class="hlt">ice</span> thickness run trough by the R/V Sikuliaq research cruise in the Beaufort Sea (October-November 2015). During several experiments, a line of wave buoys was deployed along a pre-declared line, which could thus be covered by simultaneous overhead Cosmo-SkyMed images. The inversion procedures was then applied to SAR images, the final goal being the comparison between the <span class="hlt">ice</span> thicknesses measured in situ and those inferred from SAR wave number analysis with the application of a viscous theory. Results show a broad agreement between observed thicknesses and those retrieved from the SAR, the latter slightly overestimating the former in several case studies. In the case of November 1, for example, the agreement is excellent (SAR retrievals 4.9, 5.0, 6.5 cm; observed mean 6.7 cm); on October 11 the agreement is also very good between the SAR retriveal (21 cm) and the output from an along-track EM-sounder; on October 23-24 the SAR retrieval of 18.1 cm is double the observed pancake thickness of 8.7 cm, but this difference can be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23135470','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23135470"><span>Greenland <span class="hlt">ice</span>-sheet contribution to sea-level rise buffered by meltwater storage in firn.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Harper, J; Humphrey, N; Pfeffer, W T; Brown, J; Fettweis, X</p> <p>2012-11-08</p> <p>Surface melt on the Greenland <span class="hlt">ice</span> sheet has shown increasing trends in areal extent and duration since the beginning of the satellite era. Records for melt were broken in 2005, 2007, 2010 and 2012. Much of the increased surface melt is occurring in the percolation <span class="hlt">zone</span>, a region of the accumulation area that is perennially covered by snow and firn (partly compacted snow). The fate of melt water in the percolation <span class="hlt">zone</span> is poorly constrained: some may travel away from its point of origin and eventually influence the <span class="hlt">ice</span> sheet's flow dynamics and mass balance and the global sea level, whereas some may simply infiltrate into cold snow or firn and refreeze with none of these effects. Here we quantify the existing water storage capacity of the percolation <span class="hlt">zone</span> of the Greenland <span class="hlt">ice</span> sheet and show the potential for hundreds of gigatonnes of meltwater storage. We collected in situ observations of firn structure and meltwater retention along a roughly 85-kilometre-long transect of the melting accumulation area. Our data show that repeated infiltration events in which melt water penetrates deeply (more than 10 metres) eventually fill all pore space with water. As future surface melt intensifies under Arctic warming, a fraction of melt water that would otherwise contribute to sea-level rise will fill existing pore space of the percolation <span class="hlt">zone</span>. We estimate the lower and upper bounds of this storage sink to be 322 ± 44 gigatonnes and  1,289(+388)(-252) gigatonnes, respectively. Furthermore, we find that decades are required to fill this pore space under a range of plausible future climate conditions. Hence, routing of surface melt water into filling the pore space of the firn column will delay expansion of the area contributing to sea-level rise, although once the pore space is filled it cannot quickly be regenerated.</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 activity 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 activity 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 activity 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/2018JGRC..123.1586G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123.1586G"><span>Atmosphere-<span class="hlt">Ice</span>-Ocean-Ecosystem Processes in a Thinner Arctic Sea <span class="hlt">Ice</span> Regime: The Norwegian Young Sea <span class="hlt">ICE</span> (N-<span class="hlt">ICE</span>2015) Expedition</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Granskog, Mats A.; Fer, Ilker; Rinke, Annette; Steen, Harald</p> <p>2018-03-01</p> <p>Arctic sea <span class="hlt">ice</span> has been in rapid decline the last decade and the Norwegian young sea <span class="hlt">ICE</span> (N-<span class="hlt">ICE</span>2015) expedition sought to investigate key processes in a thin Arctic sea <span class="hlt">ice</span> regime, with emphasis on atmosphere-snow-<span class="hlt">ice</span>-ocean dynamics and sea <span class="hlt">ice</span> associated ecosystem. The main findings from a half-year long campaign are collected into this special section spanning the Journal of Geophysical Research: Atmospheres, Journal of Geophysical Research: Oceans, and Journal of Geophysical Research: Biogeosciences and provide a basis for a better understanding of processes in a thin sea <span class="hlt">ice</span> regime in the high Arctic. All data from the campaign are made freely available to the research community.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..DFDE12001O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DFDE12001O"><span>Using <span class="hlt">Ice</span> Nucleating Particles to Enable Desublimation on Chilled Substrates</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>O'Brien, Julia; Failor, Kevin; Bisbano, Caitlin; Mulroe, Megan; Nath, Saurabh; Vinatzer, Boris; Boreyko, Jonathan</p> <p>2017-11-01</p> <p>On a subfreezing surface, nucleating embryos usually form as supercooled condensate that later freeze into <span class="hlt">ice</span>, as opposed to desublimation. <span class="hlt">Ice</span> nucleating particles (INPs) have been widely used to freeze existing water; however, nobody has studied how they might affect the initial mode of nucleation. Here, we show that INPs deposited on a substrate can switch the mode of embryo nucleation to desublimation, rather than supercooled condensation. Deposition was achieved by evaporating a water droplet containing INPs on a hydrophobic silicon wafer. A Peltier stage was used to cool the wafer down inside of a controlled humidity chamber, such that the desired set point temperature correlated with the dew point and onset of nucleation. Beneath a critical surface temperature, microscopy indicated that desublimation occurred on the circular patch of deposited INPs, compared to supercooled condensation outside the circle. The hydrophobic surface was then patterned with hydrophilic stripe arrays, which facilitated the deposition of stripes of INPs via the same evaporation method. The resulting array of desublimating <span class="hlt">ice</span> stripes created dry <span class="hlt">zones</span> free of condensation or frost in the intermediate areas, as the hygroscopic <span class="hlt">ice</span> stripes served as overlapping humidity sinks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28429262','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28429262"><span>Movement of a female polar bear (Ursus maritimus) in the Kara Sea during the summer sea-<span class="hlt">ice</span> break-up.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rozhnov, V V; Platonov, N G; Naidenko, S V; Mordvintsev, I N; Ivanov, E A</p> <p>2017-01-01</p> <p>The polar bear movement trajectory in relation to onset date of the sea-<span class="hlt">ice</span> break-up was studied in the coastal <span class="hlt">zone</span> of the Taimyr Peninsula, eastern part of the Kara Sea, using as an example a female polar bear tagged by a radio collar with an Argos satellite transmitter. Analysis of the long-term pattern of <span class="hlt">ice</span> melting and tracking, by means of satellite telemetry, of the female polar bear who followed the <span class="hlt">ice</span>-edge outgoing in the north-eastern direction (in summer 2012) suggests that direction of the polar bear movement depends precisely on the direction of the sea-<span class="hlt">ice</span> cover break-up.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1917155B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1917155B"><span>Sea <span class="hlt">ice</span> type dynamics in the Arctic based on Sentinel-1 Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Babiker, Mohamed; Korosov, Anton; Park, Jeong-Won</p> <p>2017-04-01</p> <p>Sea <span class="hlt">ice</span> observation from satellites has been carried out for more than four decades and is one of the most important applications of EO data in operational monitoring as well as in climate change studies. Several sensors and retrieval methods have been developed and successfully utilized to measure sea <span class="hlt">ice</span> area, concentration, drift, type, thickness, etc [e.g. Breivik et al., 2009]. Today operational sea <span class="hlt">ice</span> monitoring and analysis is fully dependent on use of satellite data. However, new and improved satellite systems, such as multi-polarisation Synthetic Apperture Radar (SAR), require further studies to develop more advanced and automated sea <span class="hlt">ice</span> monitoring methods. In addition, the unprecedented volume of data available from recently launched Sentinel missions provides both challenges and opportunities for studying sea <span class="hlt">ice</span> dynamics. In this study we investigate sea <span class="hlt">ice</span> type dynamics in the Fram strait based on Sentinel-1 A, B SAR data. Series of images for the winter season are classified into 4 <span class="hlt">ice</span> types (young <span class="hlt">ice</span>, first year <span class="hlt">ice</span>, multiyear <span class="hlt">ice</span> and leads) using the new algorithm developed by us for sea <span class="hlt">ice</span> classification, which is based on segmentation, GLCM calculation, Haralick texture feature extraction, unsupervised and supervised classifications and Support Vector Machine (SVM) [Zakhvatkina et al., 2016; Korosov et al., 2016]. This algorithm is further improved by applying thermal and scalloping noise removal [Park et al. 2016]. Sea <span class="hlt">ice</span> drift is retrieved from the same series of Sentinel-1 images using the newly developed algorithm based on combination of feature tracking and pattern matching [Mukenhuber et al., 2016]. Time series of these two products (sea <span class="hlt">ice</span> type and sea <span class="hlt">ice</span> drift) are combined in order to study sea <span class="hlt">ice</span> deformation processes at small scales. <span class="hlt">Zones</span> of sea <span class="hlt">ice</span> convergence and divergence identified from sea <span class="hlt">ice</span> drift are compared with ridges and leads identified from texture features. That allows more specific interpretation of SAR</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29023825','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29023825"><span>Gen<span class="hlt">Ice</span>: Hydrogen-Disordered <span class="hlt">Ice</span> Generator.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Matsumoto, Masakazu; Yagasaki, Takuma; Tanaka, Hideki</p> <p>2018-01-05</p> <p>Gen<span class="hlt">Ice</span> is an efficient and user-friendly tool to generate hydrogen-disordered <span class="hlt">ice</span> structures. It makes <span class="hlt">ice</span> and clathrate hydrate structures in various file formats. More than 100 kinds of structures are preset. Users can install their own crystal structures, guest molecules, and file formats as plugins. The algorithm certifies that the generated structures are completely randomized hydrogen-disordered networks obeying the <span class="hlt">ice</span> rule with zero net polarization. © 2017 The Authors. Journal of Computational Chemistry Published by Wiley Periodicals, Inc. © 2017 The Authors. Journal of Computational Chemistry Published by Wiley Periodicals, Inc.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_23 --> <div id="page_24" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="461"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70033550','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70033550"><span>Observations of the north polar water <span class="hlt">ice</span> annulus on Mars using THEMIS and TES</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Wagstaff, K.L.; Titus, T.N.; Ivanov, A.B.; Castano, R.; Bandfield, J.L.</p> <p>2008-01-01</p> <p>The Martian seasonal CO2 <span class="hlt">ice</span> caps advance and retreat each year. In the spring, as the CO2 cap gradually retreats, it leaves behind an extensive defrosting <span class="hlt">zone</span> from the solid CO2 cap to the location where all CO2 frost has sublimated. We have been studying this phenomenon in the north polar region using data from the THermal EMission Imaging System (THEMIS), a visible and infra-red (IR) camera on the Mars Odyssey spacecraft, and the Thermal Emission Spectrometer (TES) on Mars Global Surveyor. Recently, we discovered that some THEMIS images of the CO2 defrosting <span class="hlt">zone</span> contain evidence for a distinct defrosting phenomenon: some areas just south of the CO2 cap edge are too bright in visible wavelengths to be defrosted terrain, but too warm in the IR to be CO2 <span class="hlt">ice</span>. We hypothesize that we are seeing evidence for a seasonal annulus of water <span class="hlt">ice</span> (frost) that recedes with the seasonal CO2 cap, as predicted by previous workers. In this paper, we describe our observations with THEMIS and compare them to simultaneous observations by TES and OMEGA. All three instruments find that this phenomenon is distinct from the CO2 cap and most likely composed of water <span class="hlt">ice</span>. We also find strong evidence that the annulus widens as it recedes. Finally, we show that this annulus can be detected in the raw THEMIS data as it is collected, enabling future long-term onboard monitoring. ?? 2007.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015GeoRL..42.5442L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015GeoRL..42.5442L"><span>Observed platelet <span class="hlt">ice</span> distributions in Antarctic sea <span class="hlt">ice</span>: An index for ocean-<span class="hlt">ice</span> shelf heat flux</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Langhorne, P. J.; Hughes, K. G.; Gough, A. J.; Smith, I. J.; Williams, M. J. M.; Robinson, N. J.; Stevens, C. L.; Rack, W.; Price, D.; Leonard, G. H.; Mahoney, A. R.; Haas, C.; Haskell, T. G.</p> <p>2015-07-01</p> <p>Antarctic sea <span class="hlt">ice</span> that has been affected by supercooled <span class="hlt">Ice</span> Shelf Water (ISW) has a unique crystallographic structure and is called platelet <span class="hlt">ice</span>. In this paper we synthesize platelet <span class="hlt">ice</span> observations to construct a continent-wide map of the winter presence of ISW at the ocean surface. The observations demonstrate that, in some regions of coastal Antarctica, supercooled ISW drives a negative oceanic heat flux of -30 Wm-2 that persists for several months during winter, significantly affecting sea <span class="hlt">ice</span> thickness. In other regions, particularly where the thinning of <span class="hlt">ice</span> shelves is believed to be greatest, platelet <span class="hlt">ice</span> is not observed. Our new data set includes the longest <span class="hlt">ice</span>-ocean record for Antarctica, which dates back to 1902 near the McMurdo <span class="hlt">Ice</span> Shelf. These historical data indicate that, over the past 100 years, any change in the volume of very cold surface outflow from this <span class="hlt">ice</span> shelf is less than the uncertainties in the measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19840025845&hterms=marginal&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dmarginal','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19840025845&hterms=marginal&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dmarginal"><span>Observation of variations in the composition of sea <span class="hlt">ice</span> in the Greenland MIZ during early summer 1983 with the Nimbus-7 SMMR. [Marginal <span class="hlt">Ice</span> <span class="hlt">Zone</span> (MIZ); Scanning Multichannel Microwave radiometer (SMMR)</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gloersen, P.; Campbell, W. J.</p> <p>1984-01-01</p> <p>Data acquired with the Scanning Multichannel Microwave Radiometer (SMMR) on board the Nimbus-7 Satellite for a six-week period in Fram Strait were analyzed with a procedure for calculating sea <span class="hlt">ice</span> concentration, multiyear fraction, and <span class="hlt">ice</span> temperature. Calculations were compared with independent observations made on the surface and from aircraft to check the validity of the calculations based on SMMR data. The calculation of multiyear fraction, which was known to be invalid near the melting point of sea <span class="hlt">ice</span>, is discussed. The indication of multiyear <span class="hlt">ice</span> is found to disappear a number of times, presumably corresponding to freeze/thaw cycles which occurred in this time period.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhDT........48D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhDT........48D"><span>Arctic Sea <span class="hlt">Ice</span> Trafficability - New Strategies for a Changing Icescape</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dammann, Dyre Oliver</p> <p></p> <p> substantial thickness variability results in the need to raise thickness thresholds by 50%. If sea <span class="hlt">ice</span> is thick enough for safe travel, then the efficiency of travel is relevant and is influenced by the roughness of the <span class="hlt">ice</span> surface. Here, I develop a technique to derive trafficability measures from <span class="hlt">ice</span> roughness using polarimetric and interferometric synthetic aperture radar (SAR). Validated using Structure-from-Motion analysis of imagery obtained from an unmanned aerial system near Utqiagvik, Alaska, I demonstrate the ability of these SAR techniques to map both topography and roughness with potential to guide trail construction efforts towards more trafficable <span class="hlt">ice</span>. Even when the <span class="hlt">ice</span> is sufficiently thick to ensure safe travel, potential for fracturing can be a serious hazard through the ability of cracks to compromise load-bearing capacity. Therefore, I have created a state-of-the-art technique using interferometric SAR to assess <span class="hlt">ice</span> stability with capability of assessing internal <span class="hlt">ice</span> stress and potential for failure. In an analysis of <span class="hlt">ice</span> deformation and potential hazards for the Northstar Island <span class="hlt">ice</span> road near Prudhoe Bay on Alaska's North Slope I have identified a <span class="hlt">zone</span> of high relative fracture intensity potential that conformed with road inspections and hazard assessments by the operator. Through this work I have investigated the intersection between <span class="hlt">ice</span> use and geophysics, demonstrating that quantitative evaluation of a given region in the <span class="hlt">ice</span> use assessment framework developed here can aid in tactical routing of <span class="hlt">ice</span> trails and roads as well as help inform long-term strategic decision-making regarding the future of Arctic operations on or near sea <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP43B1345K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP43B1345K"><span>Antarctic Circumpolar Current Dynamics and Their Relation to Antarctic <span class="hlt">Ice</span> Sheet and Perennial Sea-<span class="hlt">Ice</span> Variability in the Central Drake Passage During the Last Climate Cycle</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kuhn, G.; Wu, S.; Hass, H. C.; Klages, J. P.; Zheng, X.; Arz, H. W.; Esper, O.; Hillenbrand, C. D.; Lange, C.; Lamy, F.; Lohmann, G.; Müller, J.; McCave, I. N. N.; Nürnberg, D.; Roberts, J.; Tiedemann, R.; Timmermann, A.; Titschack, J.; Zhang, X.</p> <p>2017-12-01</p> <p>The evolution of the Antarctic <span class="hlt">Ice</span> Sheet during the last climate cycle and the interrelation to global atmospheric and ocean circulation remains controversial and plays an important role for our understanding of <span class="hlt">ice</span> sheet response to modern global warming. The timing and sequence of deglacial warming is relevant for understanding the variability and sensitivity of the Antarctic <span class="hlt">Ice</span> Sheet to climatic changes, and the continuing rise of atmospheric greenhouse gas concentrations. The Antarctic <span class="hlt">Ice</span> Sheet is a pivotal component of the global water budget. Freshwater fluxes from the <span class="hlt">ice</span> sheet may affect the Antarctic Circumpolar Current (ACC), which is strongly impacted by the westerly wind belt in the Southern Hemisphere (SHWW) and constricted to its narrowest extent in the Drake Passage. The flow of ACC water masses through Drake Passage is, therefore, crucial for advancing our understanding of the Southern Ocean's role in global meridional overturning circulation and global climate change. In order to address orbital and millennial-scale variability of the Antarctic <span class="hlt">ice</span> sheet and the ACC, we applied a multi-proxy approach on a sediment core from the central Drake Passage including grain size, iceberg-rafted debris, mineral dust, bulk chemical and mineralogical composition, and physical properties. In combination with already published and new sediment records from the Drake Passage and Scotia Sea, as well as high-resolution data from Antarctic <span class="hlt">ice</span> cores (WDC, EDML), we now have evidence that during glacial times a more northerly extent of the perennial sea-<span class="hlt">ice</span> <span class="hlt">zone</span> decreased ACC current velocities in the central Drake Passage. During deglaciation the SHWW shifted southwards due to a decreasing temperature gradient between subtropical and polar latitudes caused by sea <span class="hlt">ice</span> and <span class="hlt">ice</span> sheet decline. This in turn caused Southern Hemisphere warming, a more vigorous ACC, stronger Southern Ocean ventilation, and warm Circumpolar Deep Water (CDW) upwelling on Antarctic shelves</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930022699&hterms=stream+box&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dstream%2Bbox','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930022699&hterms=stream+box&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dstream%2Bbox"><span>The mass balance of the <span class="hlt">ice</span> plain of <span class="hlt">Ice</span> Stream B and Crary <span class="hlt">Ice</span> Rise</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bindschadler, Robert</p> <p>1993-01-01</p> <p>The region in the mouth of <span class="hlt">Ice</span> Stream B (the <span class="hlt">ice</span> plain) and that in the vicinity of Crary <span class="hlt">Ice</span> Rise are experiencing large and rapid changes. Based on velocity, <span class="hlt">ice</span> thickness, and accumulation rate data, the patterns of net mass balance in these regions were calculated. Net mass balance, or the rate of <span class="hlt">ice</span> thickness change, was calculated as the residual of all mass fluxes into and out of subregions (or boxes). Net mass balance provides a measure of the state of health of the <span class="hlt">ice</span> sheet and clues to the current dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016TCry...10.2361N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016TCry...10.2361N"><span>A daily, 1 km resolution data set of downscaled Greenland <span class="hlt">ice</span> sheet surface mass balance (1958-2015)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Noël, Brice; van de Berg, Willem Jan; Machguth, Horst; Lhermitte, Stef; Howat, Ian; Fettweis, Xavier; van den Broeke, Michiel R.</p> <p>2016-10-01</p> <p>This study presents a data set of daily, 1 km resolution Greenland <span class="hlt">ice</span> sheet (GrIS) surface mass balance (SMB) covering the period 1958-2015. Applying corrections for elevation, bare <span class="hlt">ice</span> albedo and accumulation bias, the high-resolution product is statistically downscaled from the native daily output of the polar regional climate model RACMO2.3 at 11 km. The data set includes all individual SMB components projected to a down-sampled version of the Greenland <span class="hlt">Ice</span> Mapping Project (GIMP) digital elevation model and <span class="hlt">ice</span> mask. The 1 km mask better resolves narrow ablation <span class="hlt">zones</span>, valley glaciers, fjords and disconnected <span class="hlt">ice</span> caps. Relative to the 11 km product, the more detailed representation of isolated glaciated areas leads to increased precipitation over the southeastern GrIS. In addition, the downscaled product shows a significant increase in runoff owing to better resolved low-lying marginal glaciated regions. The combined corrections for elevation and bare <span class="hlt">ice</span> albedo markedly improve model agreement with a newly compiled data set of ablation measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.3528R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.3528R"><span>New insights into West Greenland <span class="hlt">ice</span> sheet/stream dynamics during the last glacial cycle.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roberts, David; Lane, Tim; Rea, Brice; Cofaigh, Colm O.; Jamieson, Stewart; Vieli, Andreas; Rodes, Angel</p> <p>2015-04-01</p> <p>Onshore and offshore geomorphological mapping and deglacial chronologies from West Greenland constrain the nature and magnitude of <span class="hlt">ice</span> advance and decay of the Greenland <span class="hlt">Ice</span> Sheet (GrIS) during the last glacial cycle. Several <span class="hlt">ice</span> stream troughs are known to have fed <span class="hlt">ice</span> to the shelf edge during the last glacial cycle. Their offshore expression suggests that many were coalescent systems fed by smaller outlet glaciers and <span class="hlt">ice</span> streams onshore but their central flow pathways were also controlled by geology and preglacial topography. The bed morphology of these large <span class="hlt">ice</span> streams shows they operated over soft, deforming beds with drumlins, mega-scale glacial lineations and grounding <span class="hlt">zone</span> wedges marking an offshore transition from predominant areal scour onshore. Records of offshore deglacial chronology remain sparse but the Uummannaq and Disko Bugt <span class="hlt">ice</span> stream corridors are now well constrained. The Uummannaq <span class="hlt">ice</span> stream (UIS) completely deglaciated from the continental shelf between 14.8 ka and 11.0 ka in response to rising air temperatures, increasing JJA solar radiation and sea-level rise, but temporary standstills and the asynchronous retreat history of its feeder <span class="hlt">zones</span> suggest that topography/bathymetry strongly modulated retreat rates as <span class="hlt">ice</span> became 'locked' back into the coastal fjord system. Initial reconstructions of behaviour UIS discounted an oceanic role in early deglaciation and favoured retreat from the mid-shelf and inner-shelf prior to the Younger Dryas but both these concepts remain under investigation. In Disko Bugt, Jakobshavn Isbrae deglaciated later than the UIS and remained on the outer shelf during the Younger Dyras stadial (12.8 - 11.7 cal. kyrs BP) only reaching in the inner coast fjords at approximately 10.0 ka. The later deglaciation of the Disko system (despite similar external forcing mechanisms) was controlled by regional topographic/bathymetric contrasts in their respective trough morphologies. This hypothesis is supported by recent model</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016Natur.529..519C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016Natur.529..519C"><span>No iron fertilization in the equatorial Pacific Ocean during the last <span class="hlt">ice</span> age</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Costa, K. M.; McManus, J. F.; Anderson, R. F.; Ren, H.; Sigman, D. M.; Winckler, G.; Fleisher, M. Q.; Marcantonio, F.; Ravelo, A. C.</p> <p>2016-01-01</p> <p>The equatorial Pacific Ocean is one of the major high-nutrient, low-chlorophyll regions in the global ocean. In such regions, the consumption of the available macro-nutrients such as nitrate and phosphate is thought to be limited in part by the low abundance of the critical micro-nutrient iron. Greater atmospheric dust deposition could have fertilized the equatorial Pacific with iron during the last <span class="hlt">ice</span> age—the Last Glacial Period (LGP)—but the effect of increased <span class="hlt">ice</span>-age dust fluxes on primary productivity in the equatorial Pacific remains uncertain. Here we present meridional transects of dust (derived from the 232Th proxy), phytoplankton productivity (using opal, 231Pa/230Th and excess Ba), and the degree of nitrate consumption (using foraminifera-bound δ15N) from six cores in the central equatorial Pacific for the Holocene (0-10,000 years ago) and the LGP (17,000-27,000 years ago). We find that, although dust deposition in the central equatorial Pacific was two to three times greater in the LGP than in the Holocene, productivity was the same or lower, and the degree of nitrate consumption was the same. These biogeochemical findings suggest that the relatively greater <span class="hlt">ice</span>-age dust fluxes were not large enough to provide substantial iron fertilization to the central equatorial Pacific. This may have been because the absolute rate of dust deposition in the LGP (although greater than the Holocene rate) was very low. The lower productivity coupled with unchanged nitrate consumption suggests that the subsurface major nutrient concentrations were lower in the central equatorial Pacific during the LGP. As these nutrients are today dominantly sourced from the Subantarctic <span class="hlt">Zone</span> of the Southern Ocean, we propose that the central equatorial Pacific data are consistent with more nutrient consumption in the Subantarctic <span class="hlt">Zone</span>, possibly owing to iron fertilization as a result of higher absolute dust fluxes in this region. Thus, <span class="hlt">ice</span>-age iron fertilization in the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26819045','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26819045"><span>No iron fertilization in the equatorial Pacific Ocean during the last <span class="hlt">ice</span> age.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Costa, K M; McManus, J F; Anderson, R F; Ren, H; Sigman, D M; Winckler, G; Fleisher, M Q; Marcantonio, F; Ravelo, A C</p> <p>2016-01-28</p> <p>The equatorial Pacific Ocean is one of the major high-nutrient, low-chlorophyll regions in the global ocean. In such regions, the consumption of the available macro-nutrients such as nitrate and phosphate is thought to be limited in part by the low abundance of the critical micro-nutrient iron. Greater atmospheric dust deposition could have fertilized the equatorial Pacific with iron during the last <span class="hlt">ice</span> age--the Last Glacial Period (LGP)--but the effect of increased <span class="hlt">ice</span>-age dust fluxes on primary productivity in the equatorial Pacific remains uncertain. Here we present meridional transects of dust (derived from the (232)Th proxy), phytoplankton productivity (using opal, (231)Pa/(230)Th and excess Ba), and the degree of nitrate consumption (using foraminifera-bound δ(15)N) from six cores in the central equatorial Pacific for the Holocene (0-10,000 years ago) and the LGP (17,000-27,000 years ago). We find that, although dust deposition in the central equatorial Pacific was two to three times greater in the LGP than in the Holocene, productivity was the same or lower, and the degree of nitrate consumption was the same. These biogeochemical findings suggest that the relatively greater <span class="hlt">ice</span>-age dust fluxes were not large enough to provide substantial iron fertilization to the central equatorial Pacific. This may have been because the absolute rate of dust deposition in the LGP (although greater than the Holocene rate) was very low. The lower productivity coupled with unchanged nitrate consumption suggests that the subsurface major nutrient concentrations were lower in the central equatorial Pacific during the LGP. As these nutrients are today dominantly sourced from the Subantarctic <span class="hlt">Zone</span> of the Southern Ocean, we propose that the central equatorial Pacific data are consistent with more nutrient consumption in the Subantarctic <span class="hlt">Zone</span>, possibly owing to iron fertilization as a result of higher absolute dust fluxes in this region. Thus, <span class="hlt">ice</span>-age iron fertilization in the</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 activities (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('http://hdl.handle.net/2060/20120002071','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120002071"><span>Analysis of Antarctic <span class="hlt">Ice</span>-Sheet Mass Balance from ICESat Measurements</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zwally, H. Jay; Li, Jun; Robbins, John; Saba, Jack L.; Yi, Donghui</p> <p>2011-01-01</p> <p>If protoplanets formed from 10 to 20 kilometer diameter planetesimals in a runaway accretion process prior to their oligarchic growth into the terrestrial planets, it is only logical to ask where these planetesimals may have formed in order to assess the initial composition of the Earth. We have used Weidenschilling's model for the formation of comets (1997) to calculate an efficiency factor for the formation of planetesimals from the solar nebula, then used this factor to calculate the feeding <span class="hlt">zones</span> that contribute to material contained within 10, 15 and 20 kilometer diameter planetesimals at 1 A.V. as a function of nebular mass. We find that for all reasonable nebular masses, these planetesimals contain a minimum of 3% water as <span class="hlt">ice</span> by mass. The fraction of <span class="hlt">ice</span> increases as the planetesimals increase in size and as the nebular mass decreases, since both factors increase the feeding <span class="hlt">zones</span> from which solids in the final planetesimals are drawn. Is there really a problem with the current accretion scenario that makes the Earth too dry, or is it possible that the nascent Earth lost significant quantities of water in the final stages of accretion?</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1817781A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1817781A"><span>Providing Real-time Sea <span class="hlt">Ice</span> Modeling Support to the U.S. Coast Guard</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Allard, Richard; Dykes, James; Hebert, David; Posey, Pamela; Rogers, Erick; Wallcraft, Alan; Phelps, Michael; Smedstad, Ole Martin; Wang, Shouping; Geiszler, Dan</p> <p>2016-04-01</p> <p>The Naval Research Laboratory (NRL) supported the U.S. Coast Guard Research Development Center (RDC) through a demonstration project during the summer and autumn of 2015. Specifically, a modeling system composed of a mesoscale atmospheric model, regional sea <span class="hlt">ice</span> model, and regional wave model were loosely coupled to provide real-time 72-hr forecasts of environmental conditions for the Beaufort/Chukchi Seas. The system components included a 2-km regional Community <span class="hlt">Ice</span> CodE (CICE) sea <span class="hlt">ice</span> model, 15-km Coupled Ocean Atmosphere Mesoscale Prediction System (COAMPS) atmospheric model, and a 5-km regional WAVEWATCH III wave model. The wave model utilized modeled sea <span class="hlt">ice</span> concentration fields to incorporate the effects of sea <span class="hlt">ice</span> on waves. The other modeling components assimilated atmosphere, ocean, and <span class="hlt">ice</span> observations available from satellite and in situ sources. The modeling system generated daily 72-hr forecasts of synoptic weather (including visibility), <span class="hlt">ice</span> drift, <span class="hlt">ice</span> thickness, <span class="hlt">ice</span> concentration and <span class="hlt">ice</span> strength for missions within the economic exclusion <span class="hlt">zone</span> off the coast of Alaska and a transit to the North Pole in support of the National Science Foundation GEOTRACES cruise. Model forecasts graphics were shared on a common web page with selected graphical products made available via ftp for bandwidth limited users. Model <span class="hlt">ice</span> thickness and <span class="hlt">ice</span> drift show very good agreement compared with Cold Regions Research and Engineering Laboratory (CRREL) <span class="hlt">Ice</span> Mass Balance buoys. This demonstration served as a precursor to a fully coupled atmosphere-ocean-wave-<span class="hlt">ice</span> modeling system under development. National <span class="hlt">Ice</span> Center (NIC) analysts used these model data products (CICE and COAMPS) along with other existing model and satellite data to produce the predicted 48-hr position of the <span class="hlt">ice</span> edge. The NIC served as a liaison with the RDC and NRL to provide feedback on the model predictions. This evaluation provides a baseline analysis of the current models for future comparison studies</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27862807','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27862807"><span>Microbial processes of the carbon and sulfur cycles in an <span class="hlt">ice</span>-covered, iron-rich meromictic lake Svetloe (Arkhangelsk region, Russia).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Savvichev, Alexander S; Kokryatskaya, Natalia M; Zabelina, Svetlana A; Rusanov, Igor I; Zakharova, Elena E; Veslopolova, Elena F; Lunina, Olga N; Patutina, Ekaterina O; Bumazhkin, Boris K; Gruzdev, Denis S; Sigalevich, Pavel A; Pimenov, Nikolay V; Kuznetsov, Boris B; Gorlenko, Vladimir M</p> <p>2017-02-01</p> <p>Biogeochemical, isotope geochemical and microbiological investigation of Lake Svetloe (White Sea basin), a meromictic freshwater was carried out in April 2014, when <span class="hlt">ice</span> thickness was ∼0.5 m, and the <span class="hlt">ice</span>-covered water column contained oxygen to 23 m depth. Below, the anoxic water column contained ferrous iron (up to 240 μμM), manganese (60 μM), sulfide (up to 2 μM) and dissolved methane (960 μM). The highest abundance of microbial cells revealed by epifluorescence microscopy was found in the chemocline (redox <span class="hlt">zone</span>) at 23-24.5 m. Oxygenic photosynthesis exhibited two peaks: the major one (0.43 μmol C L -1  day -1 ) below the <span class="hlt">ice</span> and the minor one in the chemocline <span class="hlt">zone</span>, where cyanobacteria related to Synechococcus rubescens were detected. The maximum of anoxygenic photosynthesis (0.69 μmol C L -1  day -1 ) at the oxic/anoxic interface, for which green sulfur bacteria Chlorobium phaeoclathratiforme were probably responsible, exceeded the value for oxygenic photosynthesis. Bacterial sulfate reduction peaked (1.5 μmol S L -1  day -1 ) below the chemocline <span class="hlt">zone</span>. The rates of methane oxidation were as high as 1.8 μmol CH 4  L -1  day -1 at the oxi/anoxic interface and much lower in the oxic <span class="hlt">zone</span>. Small phycoerythrin-containing Synechococcus-related cyanobacteria were probably involved in accumulation of metal oxides in the redox <span class="hlt">zone</span>. © 2016 Society for Applied Microbiology and John Wiley & Sons Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050179461','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050179461"><span>Sea <span class="hlt">Ice</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parkinson, Claire L.; Cavalieri, Donald J.</p> <p>2005-01-01</p> <p>Sea <span class="hlt">ice</span> covers vast areas of the polar oceans, with <span class="hlt">ice</span> extent in the Northern Hemisphere ranging from approximately 7 x 10(exp 6) sq km in September to approximately 15 x 10(exp 6) sq km in March and <span class="hlt">ice</span> extent in the Southern Hemisphere ranging from approximately 3 x 10(exp 6) sq km in February to approximately 18 x 10(exp 6) sq km in September. These <span class="hlt">ice</span> covers have major impacts on the atmosphere, oceans, and ecosystems of the polar regions, and so as changes occur in them there are potential widespread consequences. Satellite data reveal considerable interannual variability in both polar sea <span class="hlt">ice</span> covers, and many studies suggest possible connections between the <span class="hlt">ice</span> and various oscillations within the climate system, such as the Arctic Oscillation, North Atlantic Oscillation, and Antarctic Oscillation, or Southern Annular Mode. Nonetheless, statistically significant long-term trends are also apparent, including overall trends of decreased <span class="hlt">ice</span> coverage in the Arctic and increased <span class="hlt">ice</span> coverage in the Antarctic from late 1978 through the end of 2003, with the Antarctic <span class="hlt">ice</span> increases following marked decreases in the Antarctic <span class="hlt">ice</span> during the 1970s. For a detailed picture of the seasonally varying <span class="hlt">ice</span> cover at the start of the 21st century, this chapter includes <span class="hlt">ice</span> concentration maps for each month of 2001 for both the Arctic and the Antarctic, as well as an overview of what the satellite record has revealed about the two polar <span class="hlt">ice</span> covers from the 1970s through 2003.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://rosap.ntl.bts.gov/view/dot/26945','DOTNTL'); return false;" href="https://rosap.ntl.bts.gov/view/dot/26945"><span>Fast determination of soil behavior in the capillary <span class="hlt">zone</span> using simple laboratory tests.</span></a></p> <p><a target="_blank" href="http://ntlsearch.bts.gov/tris/index.do">DOT National Transportation Integrated Search</a></p> <p></p> <p>2012-12-01</p> <p>Frost heave and thaw weakening are typical problems for engineers building in northern regions. These unsaturated-soil behaviors are : caused by water flowing through the capillary <span class="hlt">zone</span> to a freezing front, where it forms <span class="hlt">ice</span> lenses. Although suction...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1919528K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1919528K"><span><span class="hlt">Ice</span> fall streaks in a warm front . An S-band polarimetric radar study</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Keppas, Stavros; Crosier, Jonathan; Choularton, Thomas; Bower, Keith</p> <p>2017-04-01</p> <p>On 21st January 2009, a maturing low pressure system approached the UK along with several associated systems. An observational research flight (part of the APPRAISE-Clouds project) took place in southern England, sampling the leading warm front of this system. During the flight, the Warm Conveyor Belt (WCB) was well depicted by the radar Doppler velocity parameter. Simultaneously, extensive <span class="hlt">ice</span> fall streaks appeared on ZDR RHI scans as long slanted <span class="hlt">zones</span> of high ZDR. It seems that there is a connection between the WCB activity and the formation and structure of the <span class="hlt">ice</span> fall streaks. The Kelvin-Helmholtz instability caused by the WCB played a key role on their formation. Moreover, in-situ measurements showed that the <span class="hlt">ice</span> fall streaks had a very specific substance and they can affect the surface precipitation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29590042','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29590042"><span><span class="hlt">Ice</span>-VII inclusions in diamonds: Evidence for aqueous fluid in Earth's deep mantle.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tschauner, O; Huang, S; Greenberg, E; Prakapenka, V B; Ma, C; Rossman, G R; Shen, A H; Zhang, D; Newville, M; Lanzirotti, A; Tait, K</p> <p>2018-03-09</p> <p>Water-rich regions in Earth's deeper mantle are suspected to play a key role in the global water budget and the mobility of heat-generating elements. We show that <span class="hlt">ice</span>-VII occurs as inclusions in natural diamond and serves as an indicator for such water-rich regions. <span class="hlt">Ice</span>-VII, the residue of aqueous fluid present during growth of diamond, crystallizes upon ascent of the host diamonds but remains at pressures as high as 24 gigapascals; it is now recognized as a mineral by the International Mineralogical Association. In particular, <span class="hlt">ice</span>-VII in diamonds points toward fluid-rich locations in the upper transition <span class="hlt">zone</span> and around the 660-kilometer boundary. Copyright © 2018 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26582841','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26582841"><span>Predictions replaced by facts: a keystone species' behavioural responses to declining 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>Hamilton, Charmain D; Lydersen, Christian; Ims, Rolf A; Kovacs, Kit M</p> <p>2015-11-01</p> <p>Since the first documentation of climate-warming induced declines in arctic sea-<span class="hlt">ice</span>, predictions have been made regarding the expected negative consequences for endemic marine mammals. But, several decades later, little hard evidence exists regarding the responses of these animals to the ongoing environmental changes. Herein, we report the first empirical evidence of a dramatic shift in movement patterns and foraging behaviour of the arctic endemic ringed seal (Pusa hispida), before and after a major collapse in sea-<span class="hlt">ice</span> in Svalbard, Norway. Among other changes to the <span class="hlt">ice</span>-regime, this collapse shifted the summer position of the marginal <span class="hlt">ice</span> <span class="hlt">zone</span> from over the continental shelf, northward to the deep Arctic Ocean Basin. Following this change, which is thought to be a 'tipping point', subadult ringed seals swam greater distances, showed less area-restricted search behaviour, dived for longer periods, exhibited shorter surface intervals, rested less on sea-<span class="hlt">ice</span> and did less diving directly beneath the <span class="hlt">ice</span> during post-moulting foraging excursions. In combination, these behavioural changes suggest increased foraging effort and thus also likely increases in the energetic costs of finding food. Continued declines in sea-<span class="hlt">ice</span> are likely to result in distributional changes, range reductions and population declines in this keystone arctic species. © 2015 The Author(s).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C42A..05C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C42A..05C"><span><span class="hlt">Ice</span> shelf melt rates in Greenland and Antarctica using time-tagged digital imagery from World View and TanDEM-X</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Charolais, A.; Rignot, E. J.; Milillo, P.; Scheuchl, B.; Mouginot, J.</p> <p>2017-12-01</p> <p>The floating extensions of glaciers, or <span class="hlt">ice</span> shelves, melt vigorously in contact with ocean waters. Melt is non uniform, with the highest melt taking place in the deepest part of the cavity, where thermal forcing is the greatest because of 1) the pressure dependence of the freezing point of the seawater/<span class="hlt">ice</span> mixture and 2) subglacial water injects fresh, buoyant, cold melt water to fuel stronger <span class="hlt">ice</span>-ocean interactions. Melt also forms along preferential channels, which are not stationary, and create lines of weakness in the shelf. <span class="hlt">Ice</span> shelf melt rates have been successfully measured from space over the entire Antarctic continent and on the <span class="hlt">ice</span> shelves in Greenland using an Eulerian approach that combines <span class="hlt">ice</span> thickness, <span class="hlt">ice</span> velocity vectors, surface mass balance data, and measurements of <span class="hlt">ice</span> thinning rates. The Eulerian approach is limited by the precision of the thickness gradients, typically of a few km, and requires significant spatial averaging to remove advection effects. A Lagrangian approach has been shown to be robust to advection effects and provides higher resolution details. We implemented a Lagrangian methodology for time-tagged World View DEMs by the Polar Geoscience Center (PGS) at the University of Minnesota and time-tagged TanDEM-X DEMs separated by one year. We derive melt rates on a 300-m grid with a precision of a few m/yr. Melt is strongest along grounding lines and along preferred channels. Channels are non-stationary because melt is not the same on opposite sides of the channels. Examining time series of data and comparing with the time-dependent grounding line positions inferred from satellite radar interferometry, we evaluate the magnitude of melt near the grounding line and even within the grounding <span class="hlt">zone</span>. A non-zero melt rate in the grounding <span class="hlt">zone</span> has vast implications for <span class="hlt">ice</span> sheet modeling. This work is funded by a grant from NASA Cryosphere Program.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_24 --> <div id="page_25" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="481"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19900017841','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19900017841"><span>Applications of ISES for coastal <span class="hlt">zone</span> studies</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bartlett, D. S.</p> <p>1990-01-01</p> <p>In contrast to the discipline- and process-oriented topics addressed, coastal <span class="hlt">zone</span> studies are defined geographically by the special circumstances inherent in the interface between land and water. The characteristics of coastal <span class="hlt">zones</span> which make them worthy of separate consideration are: (1) the dynamic nature of natural and anthropogenic processes taking place; (2) the relatively restricted spatial domain of the narrow land/water interface; and (3) the large proportion of the Earth's population living within coastal <span class="hlt">zones</span>, and the resulting extreme pressure on natural and human resources. These characteristics place special constraints and priorities on remote sensing applications, even though the applications themselves bear close relation to those addressed by other elements of this report (e.g., oceans, <span class="hlt">ice</span>, vegetation/land use). The discussion which follows first describes the suite of remote sensing activities relevant to coastal <span class="hlt">zone</span> studies. Potential Information Sciences Experiment System (ISES) experiments will then be addressed within two general categories: applications of real-time data transmission and applications of onboard data acquisition and processing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1912222G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1912222G"><span>Basal friction evolution and crevasse distribution during the surge of Basin 3, Austfonna <span class="hlt">ice</span>-cap - offline coupling between a continuum <span class="hlt">ice</span> dynamic model and a discrete element model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gong, Yongmei; Zwinger, Thomas; Åström, Jan; Gladstone, Rupert; Schellenberger, Thomas; Altena, Bas; Moore, John</p> <p>2017-04-01</p> <p>The outlet glacier at Basin 3, Austfonna <span class="hlt">ice</span>-cap entered its active surge phase in autumn 2012. We assess the evolution of the basal friction during the surge through inverse modelling of basal friction coefficients using recent velocity observation from 2012 to 2014 in a continuum <span class="hlt">ice</span> dynamic model Elmer/<span class="hlt">ice</span>. The obtained basal friction coefficient distributions at different time instances are further used as a boundary condition in a discrete element model (HiDEM) that is capable of computing fracturing of <span class="hlt">ice</span>. The inverted basal friction coefficient evolution shows a gradual 'unplugging' of the stagnant frontal area and northwards and inland expansion of the fast flowing region in the southern basin. The validation between the modeled crevasses distribution and the satellite observation in August 2013 shows a good agreement in shear <span class="hlt">zones</span> inland and at the frontal area. Crevasse distributions of the summer before and after the glacier reached its maximum velocity in January 2013 (August 2012 and August 2014, respectively) are also evaluated. Previous studies suggest the triggering and development of the surge are linked to surface melt water penetrating through <span class="hlt">ice</span> to form an efficient basal hydrology system thereby triggering a hydro- thermodynamic feedback. This preliminary offline coupling between a continuum <span class="hlt">ice</span> dynamic model and a discrete element model will give a hint on future model development of linking supra-glacial to sub-glacial hydrology system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018QSRv..185..244E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018QSRv..185..244E"><span>On the use of δ18Oatm for <span class="hlt">ice</span> core dating</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Extier, Thomas; Landais, Amaelle; Bréant, Camille; Prié, Frédéric; Bazin, Lucie; Dreyfus, Gabrielle; Roche, Didier M.; Leuenberger, Markus</p> <p>2018-04-01</p> <p>Deep <span class="hlt">ice</span> core chronologies have been improved over the past years through the addition of new age constraints. However, dating methods are still associated with large uncertainties for <span class="hlt">ice</span> cores from the East Antarctic plateau where layer counting is not possible. Indeed, an uncertainty up to 6 ka is associated with AICC2012 chronology of EPICA Dome C (EDC) <span class="hlt">ice</span> core, which mostly arises from uncertainty on the delay between changes recorded in δ18Oatm and in June 21st insolation variations at 65°N used for <span class="hlt">ice</span> core orbital dating. Consequently, we need to enhance the knowledge of this delay to improve <span class="hlt">ice</span> core chronologies. We present new high-resolution EDC δ18Oatm record (153-374 ka) and δO2/N2 measurements (163-332 ka) performed on well-stored <span class="hlt">ice</span> to provide continuous records of δ18Oatm and δO2/N2 between 100 and 800 ka. The comparison of δ18Oatm with the δ18Ocalcite from East Asian speleothems shows that both signals present similar orbital and millennial variabilities, which may represent shifts in the InterTropical Convergence <span class="hlt">Zone</span> position, themselves associated with Heinrich events. We thus propose to use the δ18Ocalcite as target for δ18Oatm orbital dating. Such a tuning method improves the <span class="hlt">ice</span> core chronology of the last glacial inception compared to AICC2012 by reconciling NGRIP and mid-latitude climatic records. It is especially marked during Dansgaard-Oeschger 25 where the proposed chronology is 2.2 ka older than AICC2012. This δ18Oatm - δ18Ocalcite alignment method applied between 100 and 640 ka improves the EDC <span class="hlt">ice</span> core chronology, especially over MIS 11, and leads to lower <span class="hlt">ice</span> age uncertainties compared to AICC2012.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12..847S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12..847S"><span>Subglacial conditions under the Weichselian <span class="hlt">Ice</span> Sheet (Central-WesternPoland)</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</p> <p>2010-05-01</p> <p>The bed underlying the last Scandinavian <span class="hlt">Ice</span> Sheet in Poland consisted of an unlithified material susceptible under appropriate subglacial conditions to active deformations under the normal and the driving stress. The thermodynamics at the <span class="hlt">ice</span>-sediment contact <span class="hlt">zone</span> had a significant influence for the <span class="hlt">ice</span> movement character, especially velocity and the <span class="hlt">ice</span> cap longitudinal profile. Clues of those paleoglaciological processes are recorded in structures and textures of subglacial sediments and the deformation structures are one of the most useful indicator for processes interpretation in basal environment The research area is placed in the Great Poland Lowland in the central-western part of Poland. Detailed investigations were carried out in several outcrops situated within the range of maximal Leszno (Brandenburger) phase extent and recessional Poznan phase (Frankfurter) of the Weichselian <span class="hlt">Ice</span> Sheet. Those glacial events are not sufficiently dated however, it is known, that they probably took place between 20 000 and 16 000 BP in this region. The purpose of this study is to propose a model of subglacial conditions during till deposition under advancing Weichselian <span class="hlt">Ice</span> Sheet using the lithofacies analysis as a main tool. Sedimentological analysis in each of the places of investigation was carried out by the means of a macroscopic evidence of deposits texture and structure together with the detailed identification of contact boundaries between individual lithofacies, till fabric measurements on the basis of at least 30 elongated clasts, the calculation of eigenvectors and eigenvalues and laboratory analysis of grain-size distribution using wet and dry (mechanical) sieving techniques. Results show that the fabric characteristics of subglacial tills and underlying sediments are significantly diversified. In general three types of subglacial tills were recognized - lodgement, deformation and melt-out till. Some of vertical profiles showed complexes of lithofacies, and the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C22A..06R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C22A..06R"><span>Spatiotemporal Variability of Meltwater Refreezing in Southwest Greenland <span class="hlt">Ice</span> Sheet Firn</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rennermalm, A. K.; Hock, R.; Tedesco, M.; Corti, G.; Covi, F.; Miège, C.; Kingslake, J.; Leidman, S. Z.; Munsell, S.</p> <p>2017-12-01</p> <p>A substantial fraction of the summer meltwater formed on the surface of the Greenland <span class="hlt">ice</span> sheet is retained in firn, while the remaining portion runs to the ocean through surface and subsurface channels. Refreezing of meltwater in firn can create impenetrable <span class="hlt">ice</span> lenses, hence being a crucial process in the redistribution of surface runoff. To quantify the impact of refreezing on runoff and current and future Greenland surface mass balance, a three year National Science Foundation funded project titled "Refreezing in the firn of the Greenland <span class="hlt">ice</span> sheet: Spatiotemporal variability and implications for <span class="hlt">ice</span> sheet mass balance" started this past year. Here we present an overview of the project and some initial results from the first field season in May 2017 conducted in proximity of the DYE-2 site in the percolation <span class="hlt">zone</span> of the Southwest Greenland <span class="hlt">ice</span> sheet at elevations between 1963 and 2355 m a.s.l.. During this fieldwork two automatic weather stations were deployed, outfitted with surface energy balance sensors and 16 m long thermistor strings, over 300 km of ground penetrating radar data were collected, and five 20-26 m deep firn cores were extracted and analyzed for density and stratigraphy. Winter snow accumulation was measured along the radar tracks. Preliminary work on the firn-core data reveals increasing frequency and thickness of <span class="hlt">ice</span> lenses at lower <span class="hlt">ice</span>-sheet elevations, in agreement with other recent work in the area. Data collected within this project will facilitate advances in our understanding of the spatiotemporal variability of firn refreezing and its role in the hydrology and surface mass balance of the Greenland <span class="hlt">Ice</span> Sheet.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMOS41A1182C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMOS41A1182C"><span>Visible and thermal imaging of sea <span class="hlt">ice</span> and open water from Coast Guard Arctic Domain Awareness flights</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chickadel, C. C.; Lindsay, R. W.; Clark, D.</p> <p>2014-12-01</p> <p>An uncooled thermal camera (microbolometer) and RGB camera were mounted in the tail section of a US Coast Guard HC-130 to observe sea <span class="hlt">ice</span>, open water, and cloud tops through the open rear cargo doors during routine Arctic Domain Awareness (ADA) flights. Recent flights were conducted over the Beaufort Sea in June, July, and August of 2014, with flights planned for September and October. Thermal and visible images were collected at low altitude (100m) during times when the cargo doors were open and recorded high resolution information on <span class="hlt">ice</span> floes, melt ponds, and surface temperature variability associated with the marginal <span class="hlt">ice</span> <span class="hlt">zone</span> (MIZ). These observations of sea <span class="hlt">ice</span> conditions and surface water temperatures will be used to characterize floe size development and the temperature and albedo of <span class="hlt">ice</span> ponds and leads. This information will allow for a detailed characterization of sea <span class="hlt">ice</span> that can be used in process studies and for model evaluation, calibration of satellite remote sensing products, and initialization of sea <span class="hlt">ice</span> prediction schemes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14.3174F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.3174F"><span>Validation and Interpretation of a new sea <span class="hlt">ice</span> Glob<span class="hlt">Ice</span> dataset using buoys and the CICE 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>Flocco, D.; Laxon, S. W.; Feltham, D. L.; Haas, C.</p> <p>2012-04-01</p> <p>The Glob<span class="hlt">Ice</span> project has provided high resolution sea <span class="hlt">ice</span> product datasets over the Arctic derived from SAR data in the ESA archive. The products are validated sea <span class="hlt">ice</span> motion, deformation and fluxes through straits. Glob<span class="hlt">Ice</span> sea <span class="hlt">ice</span> velocities, deformation data and sea <span class="hlt">ice</span> concentration have been validated using buoy data provided by the International Arctic Buoy Program (IABP). Over 95% of the Glob<span class="hlt">Ice</span> and buoy data analysed fell within 5 km of each other. The Glob<span class="hlt">Ice</span> Eulerian image pair product showed a high correlation with buoy data. The sea <span class="hlt">ice</span> concentration product was compared to SSM/I data. An evaluation of the validity of the Glob<span class="hlt">ICE</span> data will be presented in this work. Glob<span class="hlt">ICE</span> sea <span class="hlt">ice</span> velocity and deformation were compared with runs of the CICE sea <span class="hlt">ice</span> model: in particular the mass fluxes through the straits were used to investigate the correlation between the winter behaviour of sea <span class="hlt">ice</span> and the sea <span class="hlt">ice</span> state in the following summer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-GSFC_20171208_Archive_e001932.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-GSFC_20171208_Archive_e001932.html"><span><span class="hlt">Ice</span> Stars</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><span class="hlt">Ice</span> Stars - August 4th, 2002 Description: Like distant galaxies amid clouds of interstellar dust, chunks of sea <span class="hlt">ice</span> drift through graceful swirls of grease <span class="hlt">ice</span> in the frigid waters of Foxe Basin near Baffin Island in the Canadian Arctic. Sea <span class="hlt">ice</span> often begins as grease <span class="hlt">ice</span>, a soupy slick of tiny <span class="hlt">ice</span> crystals on the ocean's surface. As the temperature drops, grease <span class="hlt">ice</span> thickens and coalesces into slabs of more solid <span class="hlt">ice</span>. Credit: USGS/NASA/Landsat 7 To learn more about the Landsat satellite go to: landsat.gsfc.nasa.gov/ NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. Follow us on Twitter Join us on Facebook</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.C31A0574J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.C31A0574J"><span>Geological control of flow in the Institute and Möller <span class="hlt">Ice</span> Streams, 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>Jordan, T. A.; Ferraccioli, F.; Ross, N.; Corr, H.; Bingham, R. G.; Rippin, D. M.; Le Brocq, A.; Siegert, M. J.</p> <p>2012-12-01</p> <p>The conditions at the base of an <span class="hlt">ice</span> sheet influence its flow, and reflect the ongoing interaction between moving <span class="hlt">ice</span> and the underlying geology. Critical influences on <span class="hlt">ice</span> flow include subglacial topography, bed lithology, and geothermal heat flux. These factors are influenced either directly by local geology, or by the regional tectonic setting. Geophysical methods have been used in many parts of Antarctica, such as the Siple Coast, to reveal the role subglacial geology plays in influencing <span class="hlt">ice</span> flow. Until recently, however, the Institute and Möller <span class="hlt">Ice</span> Streams, which drain ~20% of the West Antarctic <span class="hlt">Ice</span> Sheet into the Weddell Sea, were only covered by sparse airborne radar (~50 km line spacing), and reconnaissance aeromagnetic data, limiting our understanding of the geological template for this sector of the West Antarctic <span class="hlt">Ice</span> Sheet. Here we present our geological interpretation of the first integrated aerogeophysical survey over the catchments of the Institute and Möller <span class="hlt">Ice</span> Streams, which collected ~25,000 km of new aerogeophysical data during the 2010/11 field season. These new airborne radar, magnetic and gravity data reveals both the subglacial topography, and the subglacial geology. Our maps show the fastest flowing coastal part of the Institute <span class="hlt">Ice</span> Stream crosses a sedimentary basin underlain by thinned continental crust. Further inland two distinct <span class="hlt">ice</span> flow provinces are recognised: the Pagano <span class="hlt">Ice</span> Flow Province, which follows the newly identified, ~75 km wide, sinistral strike-slip Pagano Fault <span class="hlt">Zone</span> at the boundary between East and West Antarctica; and the Ellsworth <span class="hlt">Ice</span> Flow Province, which is controlled by the Permo-Triassic structural grain of folded Middle Cambrian-Permian meta-sediments, and Jurassic granitic rocks which form significant subglacial highlands. Our new data highlight the importance of understanding subglacial geology when explaining the complex pattern of <span class="hlt">ice</span> flow observed in the <span class="hlt">ice</span> sheet interior.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017TCry...11.2543S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017TCry...11.2543S"><span><span class="hlt">Ice</span> shelf fracture parameterization in an <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>Sun, Sainan; Cornford, Stephen L.; Moore, John C.; Gladstone, Rupert; Zhao, Liyun</p> <p>2017-11-01</p> <p>Floating <span class="hlt">ice</span> shelves exert a stabilizing force onto the inland <span class="hlt">ice</span> sheet. However, this buttressing effect is diminished by the fracture process, which on large scales effectively softens the <span class="hlt">ice</span>, accelerating its flow, increasing calving, and potentially leading to <span class="hlt">ice</span> shelf breakup. We add a continuum damage model (CDM) to the BISICLES <span class="hlt">ice</span> sheet model, which is intended to model the localized opening of crevasses under stress, the transport of those crevasses through the <span class="hlt">ice</span> sheet, and the coupling between crevasse depth and the <span class="hlt">ice</span> flow field and to carry out idealized numerical experiments examining the broad impact on large-scale <span class="hlt">ice</span> sheet and shelf dynamics. In each case we see a complex pattern of damage evolve over time, with an eventual loss of buttressing approximately equivalent to halving the thickness of the <span class="hlt">ice</span> shelf. We find that it is possible to achieve a similar <span class="hlt">ice</span> flow pattern using a simple rule of thumb: introducing an enhancement factor ˜ 10 everywhere in the model domain. However, spatially varying damage (or equivalently, enhancement factor) fields set at the start of prognostic calculations to match velocity observations, as is widely done in <span class="hlt">ice</span> sheet simulations, ought to evolve in time, or grounding line retreat can be slowed by an order of magnitude.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28598345','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28598345"><span>Microbiological quality of <span class="hlt">ice</span> and <span class="hlt">ice</span> machines used in food establishments.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hampikyan, Hamparsun; Bingol, Enver Baris; Cetin, Omer; Colak, Hilal</p> <p>2017-06-01</p> <p>The <span class="hlt">ice</span> used in the food industry has to be safe and the water used in <span class="hlt">ice</span> production should have the quality of drinking water. The consumption of contaminated <span class="hlt">ice</span> directly or indirectly may be a vehicle for transmission of pathogenic bacteria to humans producing outbreaks of gastrointestinal diseases. The objective of this study was to monitor the microbiological quality of <span class="hlt">ice</span>, the water used in producing <span class="hlt">ice</span> and the hygienic conditions of <span class="hlt">ice</span> making machines in various food enterprises. Escherichia coli was detected in seven (6.7%) <span class="hlt">ice</span> and 23 (21.9%) <span class="hlt">ice</span> chest samples whereas E. coli was negative in all examined water samples. Psychrophilic bacteria were detected in 83 (79.0%) of 105 <span class="hlt">ice</span> chest and in 68 (64.7%) of 105 <span class="hlt">ice</span> samples, whereas Enterococci were detected only in 13 (12.4%) <span class="hlt">ice</span> samples. Coliforms were detected in 13 (12.4%) water, 71 (67.6%) <span class="hlt">ice</span> chest and 54 (51.4%) <span class="hlt">ice</span> samples. In order to improve the microbiological quality of <span class="hlt">ice</span>, the maintenance, cleaning and disinfecting of <span class="hlt">ice</span> machines should be carried out effectively and periodically. Also, high quality water should be used for <span class="hlt">ice</span> production.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C34B..02B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C34B..02B"><span>Constraining <span class="hlt">ice</span> sheet history in the Weddell Sea, West Antarctica, using <span class="hlt">ice</span> fabric at Korff <span class="hlt">Ice</span> Rise</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brisbourne, A.; Smith, A.; Kendall, J. M.; Baird, A. F.; Martin, C.; Kingslake, J.</p> <p>2017-12-01</p> <p>The grounding history of <span class="hlt">ice</span> rises (grounded area of independent flow regime within a floating <span class="hlt">ice</span> shelf) can be used to constrain large scale <span class="hlt">ice</span> sheet history: <span class="hlt">ice</span> fabric, resulting from the preferred orientation of <span class="hlt">ice</span> crystals due to the stress regime, can be used to infer this grounding history. With the aim of measuring the present day <span class="hlt">ice</span> fabric at Korff <span class="hlt">Ice</span> Rise, West Antarctica, a multi-azimuth wide-angle seismic experiment was undertaken. Three wide-angle common-midpoint gathers were acquired centred on the apex of the <span class="hlt">ice</span> rise, at azimuths of 60 degrees to one another, to measure variation in seismic properties with offset and azimuth. Both vertical and horizontal receivers were used to record P and S arrivals including converted phases. Measurements of the variation with offset and azimuth of seismic traveltimes, seismic attenuation and shear wave splitting have been used to quantify seismic anisotropy in the <span class="hlt">ice</span> column. The observations cannot be reproduced using an isotropic <span class="hlt">ice</span> column model. Anisotropic ray tracing has been used to test likely models of <span class="hlt">ice</span> fabric by comparison with the data. A model with a weak girdle fabric overlying a strong cluster fabric provides the best fit to the observations. Fabric of this nature is consistent with Korff <span class="hlt">Ice</span> Rise having been stable for the order of 10,000 years without any ungrounding or significant change in the <span class="hlt">ice</span> flow configuration across the <span class="hlt">ice</span> rise for this period. This observation has significant implications for the <span class="hlt">ice</span> sheet history of the Weddell Sea sector.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017TCry...11.1851P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017TCry...11.1851P"><span>Sea-level response to melting of Antarctic <span class="hlt">ice</span> shelves on multi-centennial timescales with the fast Elementary Thermomechanical <span class="hlt">Ice</span> Sheet model (f.ETISh v1.0)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pattyn, Frank</p> <p>2017-08-01</p> <p>The magnitude of the Antarctic <span class="hlt">ice</span> sheet's contribution to global sea-level rise is dominated by the potential of its marine sectors to become unstable and collapse as a response to ocean (and atmospheric) forcing. This paper presents Antarctic sea-level response to sudden atmospheric and oceanic forcings on multi-centennial timescales with the newly developed fast Elementary Thermomechanical <span class="hlt">Ice</span> Sheet (f.ETISh) model. The f.ETISh model is a vertically integrated hybrid <span class="hlt">ice</span> sheet-<span class="hlt">ice</span> shelf model with vertically integrated thermomechanical coupling, making the model two-dimensional. Its marine boundary is represented by two different flux conditions, coherent with power-law basal sliding and Coulomb basal friction. The model has been compared to existing benchmarks. Modelled Antarctic <span class="hlt">ice</span> sheet response to forcing is dominated by sub-<span class="hlt">ice</span> shelf melt and the sensitivity is highly dependent on basal conditions at the grounding line. Coulomb friction in the grounding-line transition <span class="hlt">zone</span> leads to significantly higher mass loss in both West and East Antarctica on centennial timescales, leading to 1.5 m sea-level rise after 500 years for a limited melt scenario of 10 m a-1 under freely floating <span class="hlt">ice</span> shelves, up to 6 m for a 50 m a-1 scenario. The higher sensitivity is attributed to higher <span class="hlt">ice</span> fluxes at the grounding line due to vanishing effective pressure. Removing the <span class="hlt">ice</span> shelves altogether results in a disintegration of the West Antarctic <span class="hlt">ice</span> sheet and (partially) marine basins in East Antarctica. After 500 years, this leads to a 5 m and a 16 m sea-level rise for the power-law basal sliding and Coulomb friction conditions at the grounding line, respectively. The latter value agrees with simulations by DeConto and Pollard (2016) over a similar period (but with different forcing and including processes of hydrofracturing and cliff failure). The chosen parametrizations make model results largely independent of spatial resolution so that f.ETISh can potentially be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140003875','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140003875"><span>Modeling Commercial Turbofan Engine <span class="hlt">Icing</span> Risk With <span class="hlt">Ice</span> Crystal Ingestion</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jorgenson, Philip C. E.; Veres, Joseph P.</p> <p>2013-01-01</p> <p>The occurrence of <span class="hlt">ice</span> accretion within commercial high bypass aircraft turbine engines has been reported under certain atmospheric conditions. Engine anomalies have taken place at high altitudes that have been attributed to <span class="hlt">ice</span> crystal ingestion, partially melting, and <span class="hlt">ice</span> accretion on the compression system components. The result was degraded engine performance, and one or more of the following: loss of thrust control (roll back), compressor surge or stall, and flameout of the combustor. As <span class="hlt">ice</span> crystals are ingested into the fan and low pressure compression system, the increase in air temperature causes a portion of the <span class="hlt">ice</span> crystals to melt. It is hypothesized that this allows the <span class="hlt">ice</span>-water mixture to cover the metal surfaces of the compressor stationary components which leads to <span class="hlt">ice</span> accretion through evaporative cooling. <span class="hlt">Ice</span> accretion causes a blockage which subsequently results in the deterioration in performance of the compressor and engine. The focus of this research is to apply an engine <span class="hlt">icing</span> computational tool to simulate the flow through a turbofan engine and assess the risk of <span class="hlt">ice</span> accretion. The tool is comprised of an engine system thermodynamic cycle code, a compressor flow analysis code, and an <span class="hlt">ice</span> particle melt code that has the capability of determining the rate of sublimation, melting, and evaporation through the compressor flow path, without modeling the actual <span class="hlt">ice</span> accretion. A commercial turbofan engine which has previously experienced <span class="hlt">icing</span> events during operation in a high altitude <span class="hlt">ice</span> crystal environment has been tested in the Propulsion Systems Laboratory (PSL) altitude test facility at NASA Glenn Research Center. The PSL has the capability to produce a continuous <span class="hlt">ice</span> cloud which are ingested by the engine during operation over a range of altitude conditions. The PSL test results confirmed that there was <span class="hlt">ice</span> accretion in the engine due to <span class="hlt">ice</span> crystal ingestion, at the same simulated altitude operating conditions as experienced previously in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015GPC...129...56K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015GPC...129...56K"><span>Increased precipitation drives mega slump development and destabilization of <span class="hlt">ice</span>-rich permafrost terrain, northwestern Canada</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kokelj, S. V.; Tunnicliffe, J.; Lacelle, D.; Lantz, T. C.; Chin, K. S.; Fraser, R.</p> <p>2015-06-01</p> <p>It is anticipated that an increase in rainfall will have significant impacts on the geomorphology of permafrost landscapes. Field observations, remote sensing and historical climate data were used to investigate the drivers, processes and feedbacks that perpetuate the growth of large retrogressive thaw slumps. These "mega slumps" (5-40 ha) are now common in formerly glaciated, fluvially incised, <span class="hlt">ice</span>-cored terrain of the Peel Plateau, NW Canada. Individual thaw slumps can persist for decades and their enlargement due to ground <span class="hlt">ice</span> thaw can displace up to 106 m3 of materials from slopes to valley bottoms reconfiguring slope morphology and drainage networks. Analysis of Landsat images (1985-2011) indicate that the number and size of active slumps and debris tongue deposits has increased significantly with the recent intensification of rainfall. The analyses of high resolution climatic and photographic time-series for summers 2010 and 2012 shows strong linkages amongst temperature, precipitation and the downslope sediment flux from active slumps. Ground <span class="hlt">ice</span> thaw supplies meltwater and sediments to the slump scar <span class="hlt">zone</span> and drives diurnal pulses of surficial flow. Coherence in the timing of down valley debris tongue deposition and fine-scaled observations of sediment flux indicate that heavy rainfall stimulates major mass flow events. Evacuation of sediments from the slump scar <span class="hlt">zone</span> can help to maintain a headwall of exposed ground <span class="hlt">ice</span>, perpetuating slump growth and leading to larger disturbances. The development of debris tongue deposits divert streams and increase thermoerosion to initiate adjacent slumps. We conclude that higher rainfall can intensify thaw slump activity and rapidly alter the slope-sediment cascade in regions of <span class="hlt">ice</span>-cored glaciogenic deposits.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23862786','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23862786"><span>Under-<span class="hlt">ice</span> ambient noise in Eastern Beaufort Sea, Canadian Arctic, and its relation to environmental forcing.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kinda, G Bazile; Simard, Yvan; Gervaise, Cédric; Mars, Jérome I; Fortier, Louis</p> <p>2013-07-01</p> <p>This paper analyzes an 8-month time series (November 2005 to June 2006) of underwater noise recorded at the mouth of the Amundsen Gulf in the marginal <span class="hlt">ice</span> <span class="hlt">zone</span> of the western Canadian Arctic when the area was >90% <span class="hlt">ice</span> covered. The time-series of the ambient noise component was computed using an algorithm that filtered out transient acoustic events from 7-min hourly recordings of total ocean noise over a [0-4.1] kHz frequency band. Under-<span class="hlt">ice</span> ambient noise did not respond to thermal changes, but showed consistent correlations with large-scale regional <span class="hlt">ice</span> drift, wind speed, and measured currents in upper water column. The correlation of ambient noise with <span class="hlt">ice</span> drift peaked for locations at ranges of ~300 km off the mouth of the Amundsen Gulf. These locations are within the multi-year <span class="hlt">ice</span> plume that extends westerly along the coast in the Eastern Beaufort Sea due to the large Beaufort Gyre circulation. These results reveal that ambient noise in Eastern Beaufort Sea in winter is mainly controlled by the same meteorological and oceanographic forcing processes that drive the <span class="hlt">ice</span> drift and the large-scale circulation in this part of the Arctic Ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C21B1120W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C21B1120W"><span>Autonomous <span class="hlt">Ice</span> Mass Balance Buoys for Seasonal 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>Whitlock, J. D.; Planck, C.; Perovich, D. K.; Parno, J. T.; Elder, B. C.; Richter-Menge, J.; Polashenski, C. M.</p> <p>2017-12-01</p> <p>The <span class="hlt">ice</span> mass-balance represents the integration of all surface and ocean heat fluxes and attributing the impact of these forcing fluxes on the <span class="hlt">ice</span> cover can be accomplished by increasing temporal and spatial measurements. Mass balance information can be used to understand the ongoing changes in the Arctic sea <span class="hlt">ice</span> cover and to improve predictions of future <span class="hlt">ice</span> conditions. Thinner seasonal <span class="hlt">ice</span> in the Arctic necessitates the deployment of Autonomous <span class="hlt">Ice</span> Mass Balance buoys (IMB's) capable of long-term, in situ data collection in both <span class="hlt">ice</span> and open ocean. Seasonal IMB's (SIMB's) are free floating IMB's that allow data collection in thick <span class="hlt">ice</span>, thin <span class="hlt">ice</span>, during times of transition, and even open water. The newest generation of SIMB aims to increase the number of reliable IMB's in the Arctic by leveraging inexpensive commercial-grade instrumentation when combined with specially developed monitoring hardware. Monitoring tasks are handled by a custom, expandable data logger that provides low-cost flexibility for integrating a large range of instrumentation. The SIMB features ultrasonic sensors for direct measurement of both snow depth and <span class="hlt">ice</span> thickness and a digital temperature chain (DTC) for temperature measurements every 2cm through both snow and <span class="hlt">ice</span>. Air temperature and pressure, along with GPS data complete the Arctic picture. Additionally, the new SIMB is more compact to maximize deployment opportunities from multiple types of platforms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013fss..book..383B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013fss..book..383B"><span>Spin <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>Bramwell, Steven T.; Gingras, Michel J. P.; Holdsworth, Peter C. W.</p> <p>2013-03-01</p> <p>Pauling's model of hydrogen disorder in water <span class="hlt">ice</span> represents the prototype of a frustrated system. Over the years it has spawned several analogous models, including Anderson's model antiferromagnet and the statistical "vertex" models. Spin <span class="hlt">Ice</span> is a sixteen vertex model of "ferromagnetic frustration" that is approximated by real materials, most notably the rare earth pyrochlores Ho2Ti2O7, Dy2Ti2O7 and Ho2Sn2O7. These "spin <span class="hlt">ice</span> materials" have the Pauling zero point entropy and in all respects represent almost ideal realisations of Pauling's model. They provide experimentalists with unprecedented access to a wide variety of novel magnetic states and phase transitions that are located in different regions of the field-temperature phase diagram. They afford theoreticians the opportunity to explore many new features of the magnetic interactions and statistical mechanics of frustrated systems. This chapter is a comprehensive review of the physics -- both experimental and theoretical -- of spin <span class="hlt">ice</span>. It starts with a discussion of the historic problem of water <span class="hlt">ice</span> and its relation to spin <span class="hlt">ice</span> and other frustrated magnets. The properties of spin <span class="hlt">ice</span> are then discussed in three sections that deal with the zero field spin <span class="hlt">ice</span> state, the numerous field-induced states (including the recently identified "kagomé <span class="hlt">ice</span>") and the magnetic dynamics. Some materials related to spin <span class="hlt">ice</span> are briefly described and the chapter is concluded with a short summary of spin <span class="hlt">ice</span> physics.</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>Active 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 Active 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> <span class="hlt">zones</span> 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('https://www.ncbi.nlm.nih.gov/pubmed/25399173','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25399173"><span>Vapor deposition of water on graphitic surfaces: formation of amorphous <span class="hlt">ice</span>, bilayer <span class="hlt">ice</span>, <span class="hlt">ice</span> I, and liquid water.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lupi, Laura; Kastelowitz, Noah; Molinero, Valeria</p> <p>2014-11-14</p> <p>Carbonaceous surfaces are a major source of atmospheric particles and could play an important role in the formation of <span class="hlt">ice</span>. Here we investigate through molecular simulations the stability, metastability, and molecular pathways of deposition of amorphous <span class="hlt">ice</span>, bilayer <span class="hlt">ice</span>, and <span class="hlt">ice</span> I from water vapor on graphitic and atomless Lennard-Jones surfaces as a function of temperature. We find that bilayer <span class="hlt">ice</span> is the most stable <span class="hlt">ice</span> polymorph for small cluster sizes, nevertheless it can grow metastable well above its region of thermodynamic stability. In agreement with experiments, the simulations predict that on increasing temperature the outcome of water deposition is amorphous <span class="hlt">ice</span>, bilayer <span class="hlt">ice</span>, <span class="hlt">ice</span> I, and liquid water. The deposition nucleation of bilayer <span class="hlt">ice</span> and <span class="hlt">ice</span> I is preceded by the formation of small liquid clusters, which have two wetting states: bilayer pancake-like (wetting) at small cluster size and droplet-like (non-wetting) at larger cluster size. The wetting state of liquid clusters determines which <span class="hlt">ice</span> polymorph is nucleated: bilayer <span class="hlt">ice</span> nucleates from wetting bilayer liquid clusters and <span class="hlt">ice</span> I from non-wetting liquid clusters. The maximum temperature for nucleation of bilayer <span class="hlt">ice</span> on flat surfaces, T(B)(max) is given by the maximum temperature for which liquid water clusters reach the equilibrium melting line of bilayer <span class="hlt">ice</span> as wetting bilayer clusters. Increasing water-surface attraction stabilizes the pancake-like wetting state of liquid clusters leading to larger T(B)(max) for the flat non-hydrogen bonding surfaces of this study. The findings of this study should be of relevance for the understanding of <span class="hlt">ice</span> formation by deposition mode on carbonaceous atmospheric particles, including soot.</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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