Sample records for ice mass variations

  1. Measuring Greenland Ice Mass Variation With Gravity Recovery and the Climate Experiment Gravity and GPS

    NASA Technical Reports Server (NTRS)

    Wu, Xiao-Ping

    1999-01-01

    The response of the Greenland ice sheet to climate change could significantly alter sea level. The ice sheet was much thicker at the last glacial maximum. To gain insight into the global change process and the future trend, it is important to evaluate the ice mass variation as a function of time and space. The Gravity Recovery and Climate Experiment (GRACE) mission to fly in 2001 for 5 years will measure gravity changes associated with the current ice variation and the solid earth's response to past variations. Our objective is to assess the separability of different change sources, accuracy and resolution in the mass variation determination by the new gravity data and possible Global Positioning System (GPS) bedrock uplift measurements. We use a reference parameter state that follows a dynamic ice model for current mass variation and a variant of the Tushingham and Peltier ICE-3G deglaciation model for historical deglaciation. The current linear trend is also assumed to have started 5 kyr ago. The Earth model is fixed as preliminary reference Earth model (PREM) with four viscoelastic layers. A discrete Bayesian inverse algorithm is developed employing an isotropic Gaussian a priori covariance function over the ice sheet and time. We use data noise predicted by the University of Texas and JPL for major GRACE error sources. A 2 mm/yr uplift uncertainty is assumed for GPS occupation time of 5 years. We then carry out covariance analysis and inverse simulation using GRACE geoid coefficients up to degree 180 in conjunction with a number of GPS uplift rates. Present-day ice mass variation and historical deglaciation are solved simultaneously over 146 grids of roughly 110 km x 110 km and with 6 time increments of 3 kyr each, along with a common starting epoch of the current trend. For present-day ice thickness change, the covariance analysis using GRACE geoid data alone results in a root mean square (RMS) posterior root variance of 2.6 cm/yr, with fairly large a priori

  2. Bedrock displacements in Greenland manifest ice mass variations, climate cycles and climate change

    PubMed Central

    Bevis, Michael; Wahr, John; Khan, Shfaqat A.; Madsen, Finn Bo; Brown, Abel; Willis, Michael; Kendrick, Eric; Knudsen, Per; Box, Jason E.; van Dam, Tonie; Caccamise, Dana J.; Johns, Bjorn; Nylen, Thomas; Abbott, Robin; White, Seth; Miner, Jeremy; Forsberg, Rene; Zhou, Hao; Wang, Jian; Wilson, Terry; Bromwich, David; Francis, Olivier

    2012-01-01

    The Greenland GPS Network (GNET) uses the Global Positioning System (GPS) to measure the displacement of bedrock exposed near the margins of the Greenland ice sheet. The entire network is uplifting in response to past and present-day changes in ice mass. Crustal displacement is largely accounted for by an annual oscillation superimposed on a sustained trend. The oscillation is driven by earth’s elastic response to seasonal variations in ice mass and air mass (i.e., atmospheric pressure). Observed vertical velocities are higher and often much higher than predicted rates of postglacial rebound (PGR), implying that uplift is usually dominated by the solid earth’s instantaneous elastic response to contemporary losses in ice mass rather than PGR. Superimposed on longer-term trends, an anomalous ‘pulse’ of uplift accumulated at many GNET stations during an approximate six-month period in 2010. This anomalous uplift is spatially correlated with the 2010 melting day anomaly. PMID:22786931

  3. Short-term variations of Icelandic ice cap mass inferred from cGPS coordinate time series

    NASA Astrophysics Data System (ADS)

    Compton, Kathleen; Bennett, Richard A.; Hreinsdóttir, Sigrún; van Dam, Tonie; Bordoni, Andrea; Barletta, Valentina; Spada, Giorgio

    2017-06-01

    As the global climate changes, understanding short-term variations in water storage is increasingly important. Continuously operating Global Positioning System (cGPS) stations in Iceland record annual periodic motion—the elastic response to winter accumulation and spring melt seasons—with peak-to-peak vertical amplitudes over 20 mm for those sites in the Central Highlands. Here for the first time for Iceland, we demonstrate the utility of these cGPS-measured displacements for estimating seasonal and shorter-term ice cap mass changes. We calculate unit responses to each of the five largest ice caps in central Iceland at each of the 62 cGPS locations using an elastic half-space model and estimate ice mass variations from the cGPS time series using a simple least squares inversion scheme. We utilize all three components of motion, taking advantage of the seasonal motion recorded in the horizontal. We remove secular velocities and accelerations and explore the impact that seasonal motions due to atmospheric, hydrologic, and nontidal ocean loading have on our inversion results. Our results match available summer and winter mass balance measurements well, and we reproduce the seasonal stake-based observations of loading and melting within the 1σ confidence bounds of the inversion. We identify nonperiodic ice mass changes associated with interannual variability in precipitation and other processes such as increased melting due to reduced ice surface albedo or decreased melting due to ice cap insulation in response to tephra deposition following volcanic eruptions, processes that are not resolved with once or twice-yearly stake measurements.

  4. Greenland Ice Sheet Mass Balance

    NASA Technical Reports Server (NTRS)

    Reeh, N.

    1984-01-01

    Mass balance equation for glaciers; areal distribution and ice volumes; estimates of actual mass balance; loss by calving of icebergs; hydrological budget for Greenland; and temporal variations of Greenland mass balance are examined.

  5. Estimates of Ice Sheet Mass Balance from Satellite Altimetry: Past and Future

    NASA Technical Reports Server (NTRS)

    Zwally, H. Jay; Zukor, Dorothy J. (Technical Monitor)

    2001-01-01

    A major uncertainty in predicting sea level rise is the sensitivity of ice sheet mass balance to climate change, as well as the uncertainty in present mass balance. Since the annual water exchange is about 8 mm of global sea level equivalent, the 20% uncertainty in current mass balance corresponds to 1.6 mm/yr in sea level change. Furthermore, estimates of the sensitivity of the mass balance to temperature change range from perhaps as much as - 10% to + 10% per K. A principal purpose of obtaining ice sheet elevation changes from satellite altimetry has been estimation of the current ice sheet mass balance. Limited information on ice sheet elevation change and their implications about mass balance have been reported by several investigators from radar altimetry (Seasat, Geosat, ERS-1&2). Analysis of ERS-1&2 data over Greenland for 7 years from 1992 to 1999 shows mixed patterns of ice elevation increases and decreases that are significant in terms of regional-scale mass balances. Observed seasonal and interannual variations in ice surface elevation are larger than previously expected because of seasonal and interannUal variations in precipitation, melting, and firn compaction. In the accumulation zone, the variations in firn compaction are modeled as a function of temperature leaving variations in precipitation and the mass balance trend. Significant interannual variations in elevation in some locations, in particular the difference in trends from 1992 to 1995 compared to 1995 to 1999, can be explained by changes in precipitation over Greenland. Over the 7 years, trends in elevation are mostly positive at higher elevations and negative at lower elevations. In addition, trends for the winter seasons (from a trend analysis through the average winter elevations) are more positive than the corresponding trends for the summer. At lower elevations, the 7-year trends in some locations are strongly negative for summer and near zero or slightly positive for winter. These

  6. Detecting high spatial variability of ice shelf basal mass balance, Roi Baudouin Ice Shelf, Antarctica

    NASA Astrophysics Data System (ADS)

    Berger, Sophie; Drews, Reinhard; Helm, Veit; Sun, Sainan; Pattyn, Frank

    2017-11-01

    Ice shelves control the dynamic mass loss of ice sheets through buttressing and their integrity depends on the spatial variability of their basal mass balance (BMB), i.e. the difference between refreezing and melting. Here, we present an improved technique - based on satellite observations - to capture the small-scale variability in the BMB of ice shelves. As a case study, we apply the methodology to the Roi Baudouin Ice Shelf, Dronning Maud Land, East Antarctica, and derive its yearly averaged BMB at 10 m horizontal gridding. We use mass conservation in a Lagrangian framework based on high-resolution surface velocities, atmospheric-model surface mass balance and hydrostatic ice-thickness fields (derived from TanDEM-X surface elevation). Spatial derivatives are implemented using the total-variation differentiation, which preserves abrupt changes in flow velocities and their spatial gradients. Such changes may reflect a dynamic response to localized basal melting and should be included in the mass budget. Our BMB field exhibits much spatial detail and ranges from -14.7 to 8.6 m a-1 ice equivalent. Highest melt rates are found close to the grounding line where the pressure melting point is high, and the ice shelf slope is steep. The BMB field agrees well with on-site measurements from phase-sensitive radar, although independent radar profiling indicates unresolved spatial variations in firn density. We show that an elliptical surface depression (10 m deep and with an extent of 0.7 km × 1.3 km) lowers by 0.5 to 1.4 m a-1, which we tentatively attribute to a transient adaptation to hydrostatic equilibrium. We find evidence for elevated melting beneath ice shelf channels (with melting being concentrated on the channel's flanks). However, farther downstream from the grounding line, the majority of ice shelf channels advect passively (i.e. no melting nor refreezing) toward the ice shelf front. Although the absolute, satellite-based BMB values remain uncertain, we have

  7. Long term ice sheet mass change rates and inter-annual variability from GRACE gravimetry.

    NASA Astrophysics Data System (ADS)

    Harig, C.

    2017-12-01

    The GRACE time series of gravimetry now stretches 15 years since its launch in 2002. Here we use Slepian functions to estimate the long term ice mass trends of Greenland, Antarctica, and several glaciated regions. The spatial representation shows multi-year to decadal regional shifts in accelerations, in agreement with increases in radar derived ice velocity. Interannual variations in ice mass are of particular interest since they can directly link changes in ice sheets to the drivers of change in the polar ocean and atmosphere. The spatial information retained in Slepian functions provides a tool to determine how this link varies in different regions within an ice sheet. We present GRACE observations of the 2013-2014 slowdown in mass loss of the Greenland ice sheet, which was concentrated in specific parts of the ice sheet and in certain months of the year. We also discuss estimating the relative importance of climate factors that control ice mass balance, as a function of location of the glacier/ice cap as well as the spatial variation within an ice sheet by comparing gravimetry with observations of surface air temperature, ocean temperature, etc. as well as model data from climate reanalysis products.

  8. Glaciological constraints on current ice mass changes from modelling the ice sheets over the glacial cycles

    NASA Astrophysics Data System (ADS)

    Huybrechts, P.

    2003-04-01

    The evolution of continental ice sheets introduces a long time scale in the climate system. Large ice sheets have a memory of millenia, hence the present-day ice sheets of Greenland and Antarctica are still adjusting to climatic variations extending back to the last glacial period. This trend is separate from the direct response to mass-balance changes on decadal time scales and needs to be correctly accounted for when assessing current and future contributions to sea level. One way to obtain estimates of current ice mass changes is to model the past history of the ice sheets and their underlying beds over the glacial cycles. Such calculations assist to distinguish between the longer-term ice-dynamic evolution and short-term mass-balance changes when interpreting altimetry data, and are helpful to isolate the effects of postglacial rebound from gravity and altimetry trends. The presentation will discuss results obtained from 3-D thermomechanical ice-sheet/lithosphere/bedrock models applied to the Antarctic and Greenland ice sheets. The simulations are forced by time-dependent boundary conditions derived from sediment and ice core records and are constrained by geomorphological and glacial-geological data of past ice sheet and sea-level stands. Current simulations suggest that the Greenland ice sheet is close to balance, while the Antarctic ice sheet is still losing mass, mainly due to incomplete grounding-line retreat of the West Antarctic ice sheet since the LGM. The results indicate that altimetry trends are likely dominated by ice thickness changes but that the gravitational signal mainly reflects postglacial rebound.

  9. Greenland Ice Sheet seasonal and spatial mass variability from model simulations and GRACE (2003-2012)

    NASA Astrophysics Data System (ADS)

    Alexander, Patrick M.; Tedesco, Marco; Schlegel, Nicole-Jeanne; Luthcke, Scott B.; Fettweis, Xavier; Larour, Eric

    2016-06-01

    Improving the ability of regional climate models (RCMs) and ice sheet models (ISMs) to simulate spatiotemporal variations in the mass of the Greenland Ice Sheet (GrIS) is crucial for prediction of future sea level rise. While several studies have examined recent trends in GrIS mass loss, studies focusing on mass variations at sub-annual and sub-basin-wide scales are still lacking. At these scales, processes responsible for mass change are less well understood and modeled, and could potentially play an important role in future GrIS mass change. Here, we examine spatiotemporal variations in mass over the GrIS derived from the Gravity Recovery and Climate Experiment (GRACE) satellites for the January 2003-December 2012 period using a "mascon" approach, with a nominal spatial resolution of 100 km, and a temporal resolution of 10 days. We compare GRACE-estimated mass variations against those simulated by the Modèle Atmosphérique Régionale (MAR) RCM and the Ice Sheet System Model (ISSM). In order to properly compare spatial and temporal variations in GrIS mass from GRACE with model outputs, we find it necessary to spatially and temporally filter model results to reproduce leakage of mass inherent in the GRACE solution. Both modeled and satellite-derived results point to a decline (of -178.9 ± 4.4 and -239.4 ± 7.7 Gt yr-1 respectively) in GrIS mass over the period examined, but the models appear to underestimate the rate of mass loss, especially in areas below 2000 m in elevation, where the majority of recent GrIS mass loss is occurring. On an ice-sheet-wide scale, the timing of the modeled seasonal cycle of cumulative mass (driven by summer mass loss) agrees with the GRACE-derived seasonal cycle, within limits of uncertainty from the GRACE solution. However, on sub-ice-sheet-wide scales, some areas exhibit significant differences in the timing of peaks in the annual cycle of mass change. At these scales, model biases, or processes not accounted for by models related

  10. One hundred years of Arctic ice cover variations as simulated by a one-dimensional, ice-ocean model

    NASA Astrophysics Data System (ADS)

    Hakkinen, S.; Mellor, G. L.

    1990-09-01

    A one-dimensional ice-ocean model consisting of a second moment, turbulent closure, mixed layer model and a three-layer snow-ice model has been applied to the simulation of Arctic ice mass and mixed layer properties. The results for the climatological seasonal cycle are discussed first and include the salt and heat balance in the upper ocean. The coupled model is then applied to the period 1880-1985, using the surface air temperature fluctuations from Hansen et al. (1983) and from Wigley et al. (1981). The analysis of the simulated large variations of the Arctic ice mass during this period (with similar changes in the mixed layer salinity) shows that the variability in the summer melt determines to a high degree the variability in the average ice thickness. The annual oceanic heat flux from the deep ocean and the maximum freezing rate and associated nearly constant minimum surface salinity flux did not vary significantly interannually. This also implies that the oceanic influence on the Arctic ice mass is minimal for the range of atmospheric variability tested.

  11. Antarctic Ice Mass Balance from GRACE

    NASA Astrophysics Data System (ADS)

    Boening, C.; Firing, Y. L.; Wiese, D. N.; Watkins, M. M.; Schlegel, N.; Larour, E. Y.

    2014-12-01

    The Antarctic ice mass balance and rates of change of ice mass over the past decade are analyzed based on observations from the Gravity Recovery and Climate Experiment (GRACE) satellites, in the form of JPL RL05M mascon solutions. Surface mass balance (SMB) fluxes from ERA-Interim and other atmospheric reanalyses successfully account for the seasonal GRACE-measured mass variability, and explain 70-80% of the continent-wide mass variance at interannual time scales. Trends in the residual (GRACE mass - SMB accumulation) mass time series in different Antarctic drainage basins are consistent with time-mean ice discharge rates based on radar-derived ice velocities and thicknesses. GRACE also resolves accelerations in regional ice mass change rates, including increasing rates of mass gain in East Antarctica and accelerating ice mass loss in West Antarctica. The observed East Antarctic mass gain is only partially explained by anomalously large SMB events in the second half of the record, potentially implying that ice discharge rates are also decreasing in this region. Most of the increasing mass loss rate in West Antarctica, meanwhile, is explained by decreasing SMB (principally precipitation) over this time period, part of the characteristic decadal variability in regional SMB. The residual acceleration of 2+/-1 Gt/yr, which is concentrated in the Amundsen Sea Embayment (ASE) basins, represents the contribution from increasing ice discharge rates. An Ice Sheet System Model (ISSM) run with constant ocean forcing and stationary grounding lines both underpredicts the largest trends in the ASE and produces negligible acceleration or interannual variability in discharge, highlighting the potential importance of ocean forcing for setting ice discharge rates at interannual to decadal time scales.

  12. Determination of Interannual to Decadal Changes in Ice Sheet Mass Balance from Satellite Altimetry

    NASA Technical Reports Server (NTRS)

    Zwally, H. Jay; Busalacchi, Antonioa J. (Technical Monitor)

    2001-01-01

    A major uncertainty in predicting sea level rise is the sensitivity of ice sheet mass balance to climate change, as well as the uncertainty in present mass balance. Since the annual water exchange is about 8 mm of global sea level equivalent, the +/- 25% uncertainty in current mass balance corresponds to +/- 2 mm/yr in sea level change. Furthermore, estimates of the sensitivity of the mass balance to temperature change range from perhaps as much as - 10% to + 10% per K. Although the overall ice mass balance and seasonal and inter-annual variations can be derived from time-series of ice surface elevations from satellite altimetry, satellite radar altimeters have been limited in spatial coverage and elevation accuracy. Nevertheless, new data analysis shows mixed patterns of ice elevation increases and decreases that are significant in terms of regional-scale mass balances. In addition, observed seasonal and interannual variations in elevation demonstrate the potential for relating the variability in mass balance to changes in precipitation, temperature, and melting. From 2001, NASA's ICESat laser altimeter mission will provide significantly better elevation accuracy and spatial coverage to 86 deg latitude and to the margins of the ice sheets. During 3 to 5 years of ICESat-1 operation, an estimate of the overall ice sheet mass balance and sea level contribution will be obtained. The importance of continued ice monitoring after the first ICESat is illustrated by the variability in the area of Greenland surface melt observed over 17-years and its correlation with temperature. In addition, measurement of ice sheet changes, along with measurements of sea level change by a series of ocean altimeters, should enable direct detection of ice level and global sea level correlations.

  13. The mass balance of the ice plain of Ice Stream B and Crary Ice Rise

    NASA Technical Reports Server (NTRS)

    Bindschadler, Robert

    1993-01-01

    The region in the mouth of Ice Stream B (the ice plain) and that in the vicinity of Crary Ice Rise are experiencing large and rapid changes. Based on velocity, ice thickness, and accumulation rate data, the patterns of net mass balance in these regions were calculated. Net mass balance, or the rate of ice 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 ice sheet and clues to the current dynamics.

  14. Modeling of Firn Compaction for Estimating Ice-Sheet Mass Change from Observed Ice-Sheet Elevation Change

    NASA Technical Reports Server (NTRS)

    Li, Jun; Zwally, H. Jay

    2011-01-01

    Changes in ice-sheet surface elevation are caused by a combination of ice-dynamic imbalance, ablation, temporal variations in accumulation rate, firn compaction and underlying bedrock motion. Thus, deriving the rate of ice-sheet mass change from measured surface elevation change requires information on the rate of firn compaction and bedrock motion, which do not involve changes in mass, and requires an appropriate firn density to associate with elevation changes induced by recent accumulation rate variability. We use a 25 year record of surface temperature and a parameterization for accumulation change as a function of temperature to drive a firn compaction model. We apply this formulation to ICESat measurements of surface elevation change at three locations on the Greenland ice sheet in order to separate the accumulation-driven changes from the ice-dynamic/ablation-driven changes, and thus to derive the corresponding mass change. Our calculated densities for the accumulation-driven changes range from 410 to 610 kg/cu m, which along with 900 kg/cu m for the dynamic/ablation-driven changes gives average densities ranging from 680 to 790 kg/cu m. We show that using an average (or "effective") density to convert elevation change to mass change is not valid where the accumulation and the dynamic elevation changes are of opposite sign.

  15. Autonomous Ice Mass Balance Buoys for Seasonal Sea Ice

    NASA Astrophysics Data System (ADS)

    Whitlock, J. D.; Planck, C.; Perovich, D. K.; Parno, J. T.; Elder, B. C.; Richter-Menge, J.; Polashenski, C. M.

    2017-12-01

    The ice mass-balance represents the integration of all surface and ocean heat fluxes and attributing the impact of these forcing fluxes on the ice 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 ice cover and to improve predictions of future ice conditions. Thinner seasonal ice in the Arctic necessitates the deployment of Autonomous Ice Mass Balance buoys (IMB's) capable of long-term, in situ data collection in both ice and open ocean. Seasonal IMB's (SIMB's) are free floating IMB's that allow data collection in thick ice, thin ice, 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 ice thickness and a digital temperature chain (DTC) for temperature measurements every 2cm through both snow and ice. 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.

  16. Ice-sheet mass balance and climate change.

    PubMed

    Hanna, Edward; Navarro, Francisco J; Pattyn, Frank; Domingues, Catia M; Fettweis, Xavier; Ivins, Erik R; Nicholls, Robert J; Ritz, Catherine; Smith, Ben; Tulaczyk, Slawek; Whitehouse, Pippa L; Zwally, H Jay

    2013-06-06

    Since the 2007 Intergovernmental Panel on Climate Change Fourth Assessment Report, new observations of ice-sheet mass balance and improved computer simulations of ice-sheet response to continuing climate change have been published. Whereas Greenland is losing ice mass at an increasing pace, current Antarctic ice loss is likely to be less than some recently published estimates. It remains unclear whether East Antarctica has been gaining or losing ice mass over the past 20 years, and uncertainties in ice-mass change for West Antarctica and the Antarctic Peninsula remain large. We discuss the past six years of progress and examine the key problems that remain.

  17. Characterization of Ice Roughness Variations in Scaled Glaze Icing Conditions

    NASA Technical Reports Server (NTRS)

    McClain, Stephen T.; Vargas, Mario; Tsao, Jen-Ching

    2016-01-01

    Because of the significant influence of surface tension in governing the stability and breakdown of the liquid film in flooded stagnation regions of airfoils exposed to glaze icing conditions, the Weber number is expected to be a significant parameter governing the formation and evolution of ice roughness. To investigate the influence of the Weber number on roughness formation, 53.3-cm (21-in.) and 182.9-cm (72-in.) NACA 0012 airfoils were exposed to flow conditions with essentially the same Weber number and varying stagnation collection efficiency to illuminate similarities of the ice roughness created on the different airfoils. The airfoils were exposed to icing conditions in the Icing Research Tunnel (IRT) at the NASA Glenn Research Center. Following exposure to the icing event, the airfoils were then scanned using a ROMER Absolute Arm scanning system. The resulting point clouds were then analyzed using the self-organizing map approach of McClain and Kreeger (2013) to determine the spatial roughness variations along the surfaces of the iced airfoils. The roughness characteristics on each airfoil were then compared using the relative geometries of the airfoil. The results indicate that features of the ice shape and roughness such as glaze-ice plateau limits and maximum airfoil roughness were captured well by Weber number and collection efficiency scaling of glaze icing conditions. However, secondary ice roughness features relating the instability and waviness of the liquid film on the glaze-ice plateau surface are scaled based on physics that were not captured by the local collection efficiency variations.

  18. Mass Gains of the Antarctic Ice Sheet Exceed Losses

    NASA Technical Reports Server (NTRS)

    Zwally, H. Jay; Li, Jun; Robbins, John; Saba, Jack L.; Yi, Donghui; Brenner, Anita; Bromwich, David

    2012-01-01

    During 2003 to 2008, the mass gain of the Antarctic ice sheet from snow accumulation exceeded the mass loss from ice discharge by 49 Gt/yr (2.5% of input), as derived from ICESat laser measurements of elevation change. The net gain (86 Gt/yr) over the West Antarctic (WA) and East Antarctic ice sheets (WA and EA) is essentially unchanged from revised results for 1992 to 2001 from ERS radar altimetry. Imbalances in individual drainage systems (DS) are large (-68% to +103% of input), as are temporal changes (-39% to +44%). The recent 90 Gt/yr loss from three DS (Pine Island, Thwaites-Smith, and Marie-Bryd Coast) of WA exceeds the earlier 61 Gt/yr loss, consistent with reports of accelerating ice flow and dynamic thinning. Similarly, the recent 24 Gt/yr loss from three DS in the Antarctic Peninsula (AP) is consistent with glacier accelerations following breakup of the Larsen B and other ice shelves. In contrast, net increases in the five other DS of WA and AP and three of the 16 DS in East Antarctica (EA) exceed the increased losses. Alternate interpretations of the mass changes driven by accumulation variations are given using results from atmospheric-model re-analysis and a parameterization based on 5% change in accumulation per degree of observed surface temperature change. A slow increase in snowfall with climate waRMing, consistent with model predictions, may be offsetting increased dynamic losses.

  19. Regional variations in the stability and diffusion of water-ice in the Martian regolith

    NASA Technical Reports Server (NTRS)

    Mellon, Michael T.; Jakosky, Bruce M.

    1992-01-01

    Geologic evidence suggests subsurface water-ice has played an important role in the formation of Martian landforms. Forms of mass-wasting such as debris aprons and flow patterns on valley floors suggest creep deformation of ice-laden soil, while thermokarst and chaotic terrain suggest once extensive deposits of ground ice that were later removed. The global distribution of ice-related morphology was mapped. The mapping showed regional variation, in both latitude and longitude, in the distribution of debris aprons, concentric fill craters, and 'softened' crater profiles.

  20. Diurnal Variation of Tropical Ice Cloud Microphysics inferred from Global Precipitation Measurement Microwave Imager (GPM-GMI)'s Polarimetric Measurement

    NASA Astrophysics Data System (ADS)

    Gong, J.; Zeng, X.; Wu, D. L.; Li, X.

    2017-12-01

    Diurnal variation of tropical ice cloud has been well observed and examined in terms of the area of coverage, occurring frequency, and total mass, but rarely on ice microphysical parameters (habit, size, orientation, etc.) because of lack of direct measurements of ice microphysics on a high temporal and spatial resolutions. This accounts for a great portion of the uncertainty in evaluating ice cloud's role on global radiation and hydrological budgets. The design of Global Precipitation Measurement (GPM) mission's procession orbit gives us an unprecedented opportunity to study the diurnal variation of ice microphysics on the global scale for the first time. Dominated by cloud ice scattering, high-frequency microwave polarimetric difference (PD, namely the brightness temperature difference between vertically- and horizontally-polarized paired channel measurements) from the GPM Microwave Imager (GMI) has been proven by our previous study to be very valuable to infer cloud ice microphysical properties. Using one year of PD measurements at 166 GHz, we found that cloud PD exhibits a strong diurnal cycle in the tropics (25S-25N). The peak PD amplitude varies as much as 35% over land, compared to only 6% over ocean. The diurnal cycle of the peak PD value is strongly anti-correlated with local ice cloud occurring frequency and the total ice mass with a leading period of 3 hours for the maximum correlation. The observed PD diurnal cycle can be explained by the change of ice crystal axial ratio. Using a radiative transfer model, we can simulate the observed 166 GHz PD-brightness temperature curve as well as its diurnal variation using different axial ratio values, which can be caused by the diurnal variation of ice microphysical properties including particle size, percentage of horizontally-aligned non-spherical particles, and ice habit. The leading of the change of PD ahead of ice cloud mass and occurring frequency implies the important role microphysics play in the

  1. Transient ice mass variations over Greenland detected by the combination of GPS and GRACE data

    NASA Astrophysics Data System (ADS)

    Zhang, B.; Liu, L.; Khan, S. A.; van Dam, T. M.; Zhang, E.

    2017-12-01

    Over the past decade, the Greenland Ice Sheet (GrIS) has been undergoing significant warming and ice mass loss. Such mass loss was not always a steady process but had substantial temporal and spatial variabilities. Here we apply multi-channel singular spectral analysis to crustal deformation time series measured at about 50 Global Positioning System (GPS) stations mounted on bedrock around the Greenland coast and mass changes inferred from Gravity Recovery and Climate Experiment (GRACE) to detect transient changes in ice mass balance over the GrIS. We detect two transient anomalies: one is a negative melting anomaly (Anomaly 1) that peaked around 2010; the other is a positive melting anomaly (Anomaly 2) that peaked between 2012 and 2013. The GRACE data show that both anomalies caused significant mass changes south of 74°N but negligible changes north of 74°N. Both anomalies caused the maximum mass change in southeast GrIS, followed by in west GrIS near Jakobshavn. Our results also show that the mass change caused by Anomaly 1 first reached the maximum in late 2009 in the southeast GrIS and then migrated to west GrIS. However, in Anomaly 2, the southeast GrIS was the last place that reached the maximum mass change in early 2013 and the west GrIS near Jakobshavn was the second latest place that reached the maximum mass change. Most of the GPS data show similar spatiotemporal patterns as those obtained from the GRACE data. However, some GPS time series show discrepancies in either space or time, because of data gaps and different sensitivities of mass loading change. Namely, loading deformation measured by GPS can be significantly affected by local dynamical mass changes, which, yet, has little impact on GRACE observations.

  2. Mass balance of the Antarctic ice sheet.

    PubMed

    Wingham, D J; Shepherd, A; Muir, A; Marshall, G J

    2006-07-15

    The Antarctic contribution to sea-level rise has long been uncertain. While regional variability in ice dynamics has been revealed, a picture of mass changes throughout the continental ice sheet is lacking. Here, we use satellite radar altimetry to measure the elevation change of 72% of the grounded ice sheet during the period 1992-2003. Depending on the density of the snow giving rise to the observed elevation fluctuations, the ice sheet mass trend falls in the range -5-+85Gtyr-1. We find that data from climate model reanalyses are not able to characterise the contemporary snowfall fluctuation with useful accuracy and our best estimate of the overall mass trend-growth of 27+/-29Gtyr-1-is based on an assessment of the expected snowfall variability. Mass gains from accumulating snow, particularly on the Antarctic Peninsula and within East Antarctica, exceed the ice dynamic mass loss from West Antarctica. The result exacerbates the difficulty of explaining twentieth century sea-level rise.

  3. A century of variation in the dependence of Greenland iceberg calving on ice sheet surface mass balance and regional climate change.

    PubMed

    Bigg, G R; Wei, H L; Wilton, D J; Zhao, Y; Billings, S A; Hanna, E; Kadirkamanathan, V

    2014-06-08

    Iceberg calving is a major component of the total mass balance of the Greenland ice sheet (GrIS). A century-long record of Greenland icebergs comes from the International Ice Patrol's record of icebergs (I48N) passing latitude 48° N, off Newfoundland. I48N exhibits strong interannual variability, with a significant increase in amplitude over recent decades. In this study, we show, through a combination of nonlinear system identification and coupled ocean-iceberg modelling, that I48N's variability is predominantly caused by fluctuation in GrIS calving discharge rather than open ocean iceberg melting. We also demonstrate that the episodic variation in iceberg discharge is strongly linked to a nonlinear combination of recent changes in the surface mass balance (SMB) of the GrIS and regional atmospheric and oceanic climate variability, on the scale of the previous 1-3 years, with the dominant causal mechanism shifting between glaciological (SMB) and climatic (ocean temperature) over time. We suggest that this is a change in whether glacial run-off or under-ice melting is dominant, respectively. We also suggest that GrIS calving discharge is episodic on at least a regional scale and has recently been increasing significantly, largely as a result of west Greenland sources.

  4. Inter-annual Variations in Snow/Firn Density over the Greenland Ice Sheet by Combining GRACE gravimetry and Envisat Altimetry

    NASA Astrophysics Data System (ADS)

    Su, X.; Shum, C. K.; Guo, J.; Howat, I.; Jezek, K. C.; Luo, Z.; Zhou, Z.

    2017-12-01

    Satellite altimetry has been used to monitor elevation and volume change of polar ice sheets since the 1990s. In order to derive mass change from the measured volume change, different density assumptions are commonly used in the research community, which may cause discrepancies on accurately estimating ice sheets mass balance. In this study, we investigate the inter-annual anomalies of mass change from GRACE gravimetry and elevation change from Envisat altimetry during years 2003-2009, with the objective of determining inter-annual variations of snow/firn density over the Greenland ice sheet (GrIS). High positive correlations (0.6 or higher) between these two inter-annual anomalies at are found over 93% of the GrIS, which suggests that both techniques detect the same geophysical process at the inter-annual timescale. Interpreting the two anomalies in terms of near surface density variations, over 80% of the GrIS, the inter-annual variation in average density is between the densities of snow and pure ice. In particular, at the Summit of Central Greenland, we validate the satellite data estimated density with the in situ data available from 75 snow pits and 9 ice cores. This study provides constraints on the currently applied density assumptions for the GrIS.

  5. Balance Mass Flux and Velocity Across the Equilibrium Line in Ice Drainage Systems of Greenland

    NASA Technical Reports Server (NTRS)

    Zwally, H. Jay; Giovinetto, Mario B.; Koblinsky, Chester J. (Technical Monitor)

    2001-01-01

    Estimates of balance mass flux and the depth-averaged ice velocity through the cross-section aligned with the equilibrium line are produced for each of six drainage systems in Greenland. (The equilibrium line, which lies at approximately 1200 m elevation on the ice sheet, is the boundary between the area of net snow accumulation at higher elevations and the areas of net melting at lower elevations around the ice sheet.) Ice drainage divides and six major drainage systems are delineated using surface topography from ERS (European Remote Sensing) radar altimeter data. The net accumulation rate in the accumulation zone bounded by the equilibrium line is 399 Gt/yr and net ablation rate in the remaining area is 231 Gt/yr. (1 GigaTon of ice is 1090 kM(exp 3). The mean balance mass flux and depth-averaged ice velocity at the cross-section aligned with the modeled equilibrium line are 0.1011 Gt kM(exp -2)/yr and 0.111 km/yr, respectively, with little variation in these values from system to system. The ratio of the ice mass above the equilibrium line to the rate of mass output implies an effective exchange time of approximately 6000 years for total mass exchange. The range of exchange times, from a low of 3 ka in the SE drainage system to 14 ka in the NE, suggests a rank as to which regions of the ice sheet may respond more rapidly to climate fluctuations.

  6. Greenland ice sheet mass balance: a review.

    PubMed

    Khan, Shfaqat A; Aschwanden, Andy; Bjørk, Anders A; Wahr, John; Kjeldsen, Kristian K; Kjær, Kurt H

    2015-04-01

    Over the past quarter of a century the Arctic has warmed more than any other region on Earth, causing a profound impact on the Greenland ice sheet (GrIS) and its contribution to the rise in global sea level. The loss of ice can be partitioned into processes related to surface mass balance and to ice discharge, which are forced by internal or external (atmospheric/oceanic/basal) fluctuations. Regardless of the measurement method, observations over the last two decades show an increase in ice loss rate, associated with speeding up of glaciers and enhanced melting. However, both ice discharge and melt-induced mass losses exhibit rapid short-term fluctuations that, when extrapolated into the future, could yield erroneous long-term trends. In this paper we review the GrIS mass loss over more than a century by combining satellite altimetry, airborne altimetry, interferometry, aerial photographs and gravimetry data sets together with modelling studies. We revisit the mass loss of different sectors and show that they manifest quite different sensitivities to atmospheric and oceanic forcing. In addition, we discuss recent progress in constructing coupled ice-ocean-atmosphere models required to project realistic future sea-level changes.

  7. Seasonal origins of air masses transported to Mount Wrangell, Alaska, and comparison with the past atmospheric dust and tritium variations in its ice core

    NASA Astrophysics Data System (ADS)

    Yasunari, T. J.; Shiraiwa, T.; Kanamori, S.; Fujii, Y.; Igarashi, M.; Yamazaki, K.; Benson, C. S.; Hondoh, T.

    2006-12-01

    The North Pacific region is subject to various climatic phenomena such as the Pacific Decadal Oscillation (PDO), the El Niño-Southern Oscillation (ENSO), and the Arctic Oscillation (AO), significantly affecting the ocean and the atmosphere. Additionally, material circulation is also very active in this region such as spring dust storms in the desert and arid regions of East Asia and forest fires in Siberia and Alaska. Understanding the complex connections among the climatic phenomena and the material circulation would help in attempts to predict future climate changes. For this subject, we drilled a 50-m ice core at the summit of Mount Wrangell, which is located near the coast of Alaska (62°162'170"162°171'N, 144°162'170"162;°171'W, and 4100-m). We analyzed dust particle number density, tritium concentration, and 171 171 171 171 170 162 171 D in the core. The ice core spanned the years from 1992 to 2002 and we finally divided the years into five parts (early-spring; late-spring; summer; fall; winter). Dust and tritium amounts varied annually and intra-annually. For further understanding of the factors on those variations, we should know the origins of the seasonal dust and tritium. Hence, we examined their origins by the calculation of everyday 10-days backward trajectory analysis from January 1992 to August 2002 with 3-D wind data of the European Center for Medium-Range Weather Forecast (ECMWF). In early spring, the air mass from East Asia increased and it also explained dust increases in springtime, although the air contribution in winter increased too. In late spring, the air mass from the stratosphere increased, and it also corresponded to the stratospheric tritium increase in the ice core. The air masses from Siberia and the North Pacific in the mid-latitude always significantly contributed to Mount Wrangell, although those maximum contributions were fall and summer, respectively. The air mass originating in the interior of Alaska and North America did

  8. Changes in ice dynamics and mass balance of the Antarctic ice sheet.

    PubMed

    Rignot, Eric

    2006-07-15

    The concept that the Antarctic ice sheet changes with eternal slowness has been challenged by recent observations from satellites. Pronounced regional warming in the Antarctic Peninsula triggered ice shelf collapse, which led to a 10-fold increase in glacier flow and rapid ice sheet retreat. This chain of events illustrated the vulnerability of ice shelves to climate warming and their buffering role on the mass balance of Antarctica. In West Antarctica, the Pine Island Bay sector is draining far more ice into the ocean than is stored upstream from snow accumulation. This sector could raise sea level by 1m and trigger widespread retreat of ice in West Antarctica. Pine Island Glacier accelerated 38% since 1975, and most of the speed up took place over the last decade. Its neighbour Thwaites Glacier is widening up and may double its width when its weakened eastern ice shelf breaks up. Widespread acceleration in this sector may be caused by glacier ungrounding from ice shelf melting by an ocean that has recently warmed by 0.3 degrees C. In contrast, glaciers buffered from oceanic change by large ice shelves have only small contributions to sea level. In East Antarctica, many glaciers are close to a state of mass balance, but sectors grounded well below sea level, such as Cook Ice Shelf, Ninnis/Mertz, Frost and Totten glaciers, are thinning and losing mass. Hence, East Antarctica is not immune to changes.

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

    NASA Astrophysics Data System (ADS)

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

    2017-12-01

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

  10. Diurnal Variation of Tropical Ice Cloud Microphysics: Evidence from Global Precipitation Measurement Microwave Imager Polarimetric Measurements

    NASA Astrophysics Data System (ADS)

    Gong, Jie; Zeng, Xiping; Wu, Dong L.; Li, Xiaowen

    2018-01-01

    The diurnal variation of tropical ice clouds has been well observed and examined in terms of the occurring frequency and total mass but rarely from the viewpoint of ice microphysical parameters. It accounts for a large portion of uncertainties in evaluating ice clouds' role on global radiation and hydrological budgets. Owing to the advantage of precession orbit design and paired polarized observations at a high-frequency microwave band that is particularly sensitive to ice particle microphysical properties, 3 years of polarimetric difference (PD) measurements using the 166 GHz channel of Global Precipitation Measurement Microwave Imager (GPM-GMI) are compiled to reveal a strong diurnal cycle over tropical land (30°S-30°N) with peak amplitude varying up to 38%. Since the PD signal is dominantly determined by ice crystal size, shape, and orientation, the diurnal cycle observed by GMI can be used to infer changes in ice crystal properties. Moreover, PD change is found to lead the diurnal changes of ice cloud occurring frequency and total ice mass by about 2 h, which strongly implies that understanding ice microphysics is critical to predict, infer, and model ice cloud evolution and precipitation processes.

  11. Ice Mass Fluctuations and Earthquake Hazard

    NASA Technical Reports Server (NTRS)

    Sauber, J.

    2006-01-01

    In south central Alaska, tectonic strain rates are high in a region that includes large glaciers undergoing ice 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 zone in Alaska. In this region, the Bering and Malaspina glacier ablation zones have average ice elevation decreases from 1-3 meters/year (see summary and references in Molnia, 2005). The elastic response of the solid Earth to this ice 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 ice 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) ice 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 ice elevation changes [Sauber et al., 2005, Muskett et al., 2005]. Since we are interested in evaluating the effect of ice 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 ice mass fluctuations altered the seismic rate of background seismicity. Although we primarily focus on

  12. Improving Surface Mass Balance Over Ice Sheets and Snow Depth on Sea Ice

    NASA Technical Reports Server (NTRS)

    Koenig, Lora Suzanne; Box, Jason; Kurtz, Nathan

    2013-01-01

    Surface mass balance (SMB) over ice sheets and snow on sea ice (SOSI) are important components of the cryosphere. Large knowledge gaps remain in scientists' abilities to monitor SMB and SOSI, including insufficient measurements and difficulties with satellite retrievals. On ice sheets, snow accumulation is the sole mass gain to SMB, and meltwater runoff can be the dominant single loss factor in extremely warm years such as 2012. SOSI affects the growth and melt cycle of the Earth's polar sea ice cover. The summer of 2012 saw the largest satellite-recorded melt area over the Greenland ice sheet and the smallest satellite-recorded Arctic sea ice extent, making this meeting both timely and relevant.

  13. Spatiotemporal Patterns of Ice Mass Variations and the Local Climatic Factors in the Riparian Zone of Central Valley, California

    NASA Astrophysics Data System (ADS)

    Inamdar, P.; Ambinakudige, S.

    2016-12-01

    Californian icefields are natural basins of fresh water. They provide irrigation water to the farms in the central valley. We analyzed the ice mass loss rates, air temperature and land surface temperature (LST) in Sacramento and San Joaquin basins in California. The digital elevation models from Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) were used to calculate ice mass loss rate between the years 2002 and 2015. Additionally, Landsat TIR data were used to extract the land surface temperature. Data from local weather stations were analyzed to understand the spatiotemporal trends in air temperature. The results showed an overall mass recession of -0.8 ± 0.7 m w.e.a-1. We also noticed an about 60% loss in areal extent of the glaciers in the study basins between 2000 and 2015. Local climatic factors, along with the global climate patterns might have influenced the negative trends in the ice mass loss. Overall, there was an increase in the air temperature by 0.07± 0.02 °C in the central valley between 2000 and 2015. Furthermore, LST increased by 0.34 ± 0.4 °C and 0.55± 0.1 °C in the Sacramento and San Joaquin basins. Our preliminary results show the decrease in area and mass of ice mass in the basins, and changing agricultural practices in the valley.

  14. Estimating the rates of mass change, ice volume change and snow volume change in Greenland from ICESat and GRACE data

    NASA Astrophysics Data System (ADS)

    Slobbe, D. C.; Ditmar, P.; Lindenbergh, R. C.

    2009-01-01

    The focus of this paper is on the quantification of ongoing mass and volume changes over the Greenland ice sheet. For that purpose, we used elevation changes derived from the Ice, Cloud, and land Elevation Satellite (ICESat) laser altimetry mission and monthly variations of the Earth's gravity field as observed by the Gravity Recovery and Climate Experiment (GRACE) mission. Based on a stand alone processing scheme of ICESat data, the most probable estimate of the mass change rate from 2003 February to 2007 April equals -139 +/- 68 Gtonyr-1. Here, we used a density of 600+/-300 kgm-3 to convert the estimated elevation change rate in the region above 2000m into a mass change rate. For the region below 2000m, we used a density of 900+/-300 kgm-3. Based on GRACE gravity models from half 2002 to half 2007 as processed by CNES, CSR, DEOS and GFZ, the estimated mass change rate for the whole of Greenland ranges between -128 and -218Gtonyr-1. Most GRACE solutions show much stronger mass losses as obtained with ICESat, which might be related to a local undersampling of the mass loss by ICESat and uncertainties in the used snow/ice densities. To solve the problem of uncertainties in the snow and ice densities, two independent joint inversion concepts are proposed to profit from both GRACE and ICESat observations simultaneously. The first concept, developed to reduce the uncertainty of the mass change rate, estimates this rate in combination with an effective snow/ice density. However, it turns out that the uncertainties are not reduced, which is probably caused by the unrealistic assumption that the effective density is constant in space and time. The second concept is designed to convert GRACE and ICESat data into two totally new products: variations of ice volume and variations of snow volume separately. Such an approach is expected to lead to new insights in ongoing mass change processes over the Greenland ice sheet. Our results show for different GRACE solutions a snow

  15. The Ice Sheet Mass Balance Inter-comparison Exercise

    NASA Astrophysics Data System (ADS)

    Shepherd, A.; Ivins, E. R.

    2015-12-01

    Fluctuations in the mass of ice stored in Antarctica and Greenland are of considerable societal importance. The Ice Sheet Mass Balance Inter-Comparison Exercise (IMBIE) is a joint-initiative of ESA and NASA aimed at producing a single estimate of the global sea level contribution to polar ice sheet losses. Within IMBIE, estimates of ice sheet mass balance are developed from a variety of satellite geodetic techniques using a common spatial and temporal reference frame and a common appreciation of the contributions due to external signals. The project brings together the laboratories and space agencies that have been instrumental in developing independent estimates of ice sheet mass balance to date. In its first phase, IMBIE involved 27 science teams, and delivered a first community assessment of ice sheet mass imbalance to replace 40 individual estimates. The project established that (i) there is good agreement between the three main satellite-based techniques for estimating ice sheet mass balance, (ii) combining satellite data sets leads to significant improvement in certainty, (iii) the polar ice sheets contributed 11 ± 4 mm to global sea levels between 1992 and 2012, and (iv) that combined ice losses from Antarctica and Greenland have increased over time, rising from 10% of the global trend in the early 1990's to 30% in the late 2000's. Demand for an updated assessment has grown, and there are now new satellite missions, new geophysical corrections, new techniques, and new teams producing data. The period of overlap between independent satellite techniques has increased from 5 to 12 years, and the full period of satellite data over which an assessment can be performed has increased from 19 to 40 years. It is also clear that multiple satellite techniques are required to confidently separate mass changes associated with snowfall and ice dynamical imbalance - information that is of critical importance for climate modelling. This presentation outlines the approach

  16. Ice Mass Change in Greenland and Antarctica Between 1993 and 2013 from Satellite Gravity Measurements

    NASA Technical Reports Server (NTRS)

    Talpe, Matthieu J.; Nerem, R. Steven; Forootan, Ehsan; Schmidt, Michael; Lemoine, Frank G.; Enderlin, Ellyn M.; Landerer, Felix W.

    2017-01-01

    We construct long-term time series of Greenland and Antarctic ice sheet mass change from satellite gravity measurements. A statistical reconstruction approach is developed based on a principal component analysis (PCA) to combine high-resolution spatial modes from the Gravity Recovery and Climate Experiment (GRACE) mission with the gravity information from conventional satellite tracking data. Uncertainties of this reconstruction are rigorously assessed; they include temporal limitations for short GRACE measurements, spatial limitations for the low-resolution conventional tracking data measurements, and limitations of the estimated statistical relationships between low- and high-degree potential coefficients reflected in the PCA modes. Trends of mass variations in Greenland and Antarctica are assessed against a number of previous studies. The resulting time series for Greenland show a higher rate of mass loss than other methods before 2000, while the Antarctic ice sheet appears heavily influenced by interannual variations.

  17. Deglaciation-induced uplift and seasonal variations patterns of bedrock displacement in Greenland ice sheet margin observed from GPS, GRACE and InSAR

    NASA Astrophysics Data System (ADS)

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

    2017-12-01

    The Greenland ice sheet is rapidly shrinking with the fastest retreat and thinning occurring at the ice sheet margin and near the outlet glaciers. The changes of the ice mass cause an elastic response of the bedrock. Theoretically, ice mass loss during the summer melting season is associated with bedrock uplift, whereas increasing ice mass during the winter months is associated with bedrock subsidence. Here we examine the annual changes of the vertical displacements measured at 37 GPS stations and compare the results with Greenland drainage basins' gravity from GRACE. We use both Fourier Series (FS) analysis and Cubic Smoothing Spline (CSS) method to estimate the phases and amplitudes of seasonal variations. Both methods show significant differences seasonal behaviors in southern and northern Greenland. The average amplitude of bedrock displacements (3.29±0.02mm) in south Greenland is about 2 times larger than the north (1.65±0.02mm). The phase of bedrock maximum uplift (November) is considerably consistent with the time of minimum ice mass load in south Greenland (October). However, the phase of bedrock maximum uplift in north Greenland (February) is 4 months later than the minimum ice mass load in north Greenland basins (October). In addition, we present ground deformation near several famous glaciers in Greenland such as Petermann glacier and Jakobshavn glacier. We process InSAR data from TerraSAR-X and Sentinel satellite, based on small baseline interferograms. We observed rapid deglaciation-induced uplift and seasonal variations on naked bedrock near the glacier ice margin.

  18. Data assimilation and prognostic whole ice sheet modelling with the variationally derived, higher order, open source, and fully parallel ice sheet model VarGlaS

    NASA Astrophysics Data System (ADS)

    Brinkerhoff, D. J.; Johnson, J. V.

    2013-07-01

    We introduce a novel, higher order, finite element ice sheet model called VarGlaS (Variational Glacier Simulator), which is built on the finite element framework FEniCS. Contrary to standard procedure in ice sheet modelling, VarGlaS formulates ice sheet motion as the minimization of an energy functional, conferring advantages such as a consistent platform for making numerical approximations, a coherent relationship between motion and heat generation, and implicit boundary treatment. VarGlaS also solves the equations of enthalpy rather than temperature, avoiding the solution of a contact problem. Rather than include a lengthy model spin-up procedure, VarGlaS possesses an automated framework for model inversion. These capabilities are brought to bear on several benchmark problems in ice sheet modelling, as well as a 500 yr simulation of the Greenland ice sheet at high resolution. VarGlaS performs well in benchmarking experiments and, given a constant climate and a 100 yr relaxation period, predicts a mass evolution of the Greenland ice sheet that matches present-day observations of mass loss. VarGlaS predicts a thinning in the interior and thickening of the margins of the ice sheet.

  19. Satellite-derived submarine melt rates and mass balance (2011-2015) for Greenland's largest remaining ice tongues

    NASA Astrophysics Data System (ADS)

    Wilson, Nat; Straneo, Fiammetta; Heimbach, Patrick

    2017-12-01

    Ice-shelf-like floating extensions at the termini of Greenland glaciers are undergoing rapid changes with potential implications for the stability of upstream glaciers and the ice sheet as a whole. While submarine melting is recognized as a major contributor to mass loss, the spatial distribution of submarine melting and its contribution to the total mass balance of these floating extensions is incompletely known and understood. Here, we use high-resolution WorldView satellite imagery collected between 2011 and 2015 to infer the magnitude and spatial variability of melt rates under Greenland's largest remaining ice tongues - Nioghalvfjerdsbræ (79 North Glacier, 79N), Ryder Glacier (RG), and Petermann Glacier (PG). Submarine melt rates under the ice tongues vary considerably, exceeding 50 m a-1 near the grounding zone and decaying rapidly downstream. Channels, likely originating from upstream subglacial channels, give rise to large melt variations across the ice tongues. We compare the total melt rates to the influx of ice to the ice tongue to assess their contribution to the current mass balance. At Petermann Glacier and Ryder Glacier, we find that the combined submarine and aerial melt approximately balances the ice flux from the grounded ice sheet. At Nioghalvfjerdsbræ the total melt flux (14.2 ± 0.96 km3 a-1 w.e., water equivalent) exceeds the inflow of ice (10.2 ± 0.59 km3 a-1 w.e.), indicating present thinning of the ice tongue.

  20. High Artic Glaciers and Ice Caps Ice Mass Change from GRACE, Regional Climate Model Output and Altimetry.

    NASA Astrophysics Data System (ADS)

    Ciraci, E.; Velicogna, I.; Fettweis, X.; van den Broeke, M. R.

    2016-12-01

    The Arctic hosts more than the 75% of the ice covered regions outside from Greenland and Antarctica. Available observations show that increased atmospheric temperatures during the last century have contributed to a substantial glaciers retreat in all these regions. We use satellite gravimetry by the NASA's Gravity Recovery and Climate Experiment (GRACE), and apply a least square fit mascon approach to calculate time series of ice mass change for the period 2002-2016. Our estimates show that arctic glaciers have constantly contributed to the sea level rise during the entire observation period with a mass change of -170+/-20 Gt/yr equivalent to the 80% of the total ice mass change from the world Glacier and Ice Caps (GIC) excluding the Ice sheet peripheral GIC, which we calculated to be -215+/-32 GT/yr, with an acceleration of 9+/-4 Gt/yr2. The Canadian Archipelago is the main contributor to the total mass depletion with an ice mass trend of -73+/-9 Gt/yr and a significant acceleration of -7+/-3 Gt/yr2. The increasing mass loss is mainly determined by melting glaciers located in the northern part of the archipelago.In order to investigate the physical processes driving the observed ice mass loss we employ satellite altimetry and surface mass balance (SMB) estimates from Regional climate model outputs available for the same time period covered by the gravimetry data. We use elevation data from the NASA ICESat (2003-2009) and ESA CryoSat-2 (2010-2016) missions to estimate ice elevation changes. We compare GRACE ice mass estimates with time series of surface mass balance from the Regional Climate Model (RACMO-2) and the Modèle Atmosphérique Régional (MAR) and determine the portion of the total mass change explained by the SMB signal. We find that in Iceland and in the and the Canadian Archipelago the SMB signal explains most of the observed mass changes, suggesting that ice discharge may play a secondary role here. In other region, e.g. in Svalbar, the SMB signal

  1. Measurements of sea ice mass redistribution during ice deformation event in Arctic winter

    NASA Astrophysics Data System (ADS)

    Itkin, P.; Spreen, G.; King, J.; Rösel, A.; Skourup, H.; Munk Hvidegaard, S.; Wilkinson, J.; Oikkonen, A.; Granskog, M. A.; Gerland, S.

    2016-12-01

    Sea-ice growth during high winter is governed by ice dynamics. The highest growth rates are found in leads that open under divergent conditions, where exposure to the cold atmosphere promotes thermodynamic growth. Additionally ice thickens dynamically, where convergence causes rafting and ridging. We present a local study of sea-ice growth and mass redistribution between two consecutive airborne measurements, on 19 and 24 April 2015, during the N-ICE2015 expedition in the area north of Svalbard. Between the two overflights an ice deformation event was observed. Airborne laser scanner (ALS) measurements revisited the same sea-ice area of approximately 3x3 km. By identifying the sea surface within the ALS measurements as a reference the sea ice plus snow freeboard was obtained with a spatial resolution of 5 m. By assuming isostatic equilibrium of level floes, the freeboard heights can be converted to ice thickness. The snow depth is estimated from in-situ measurements. Sea ice thickness measurements were made in the same area as the ALS measurements by electromagnetic sounding from a helicopter (HEM), and with a ground-based device (EM31), which allows for cross-validation of the sea-ice thickness estimated from all 3 procedures. Comparison of the ALS snow freeboard distributions between the first and second overflight shows a decrease in the thin ice classes and an increase of the thick ice classes. While there was no observable snowfall and a very low sea-ice growth of older level ice during this period, an autonomous buoy array deployed in the surroundings of the area measured by the ALS shows first divergence followed by convergence associated with shear. To quantify and link the sea ice deformation with the associated sea-ice thickness change and mass redistribution we identify over 100 virtual buoys in the ALS data from both overflights. We triangulate the area between the buoys and calculate the strain rates and freeboard change for each individual triangle

  2. Seasonal and Interannual Variations of Sea Ice Mass Balance From the Central Arctic to the Greenland Sea

    NASA Astrophysics Data System (ADS)

    Lei, Ruibo; Cheng, Bin; Heil, Petra; Vihma, Timo; Wang, Jia; Ji, Qing; Zhang, Zhanhai

    2018-04-01

    The seasonal evolution of sea ice mass balance between the Central Arctic and Fram Strait, as well as the underlying driving forces, remain largely unknown because of a lack of observations. In this study, two and three buoys were deployed in the Central Arctic during the summers of 2010 and 2012, respectively. It was established that basal ice growth commenced between mid-October and early December. Annual basal ice growth, ranging from 0.21 to 1.14 m, was determined mainly by initial ice thickness, air temperature, and oceanic heat flux during winter. An analytic thermodynamic model indicated that climate warming reduces the winter growth rate of thin ice more than for thick ice because of the weak thermal inertia of the former. Oceanic heat flux during the freezing season was 2-4 W m-2, which accounted for 18-31% of the basal ice energy balance. We identified two mechanisms that modified the oceanic heat flux, i.e., solar energy absorbed by the upper ocean during summer, and interaction with warm waters south of Fram Strait; the latter resulted in basal ice melt, even in winter. In summer 2010, ice loss in the Central Arctic was considerable, which led to increased oceanic heat flux into winter and delayed ice growth. The Transpolar Drift Stream was relatively weak in summer 2013. This reduced sea ice advection out of the Arctic Ocean, and it restrained ice melt because of the cool atmospheric conditions, weakened albedo feedback, and relatively small oceanic heat flux in the north.

  3. Ice-atmosphere interactions in the Canadian High Arctic: Implications for the thermo-mechanical evolution of terrestrial ice masses

    NASA Astrophysics Data System (ADS)

    Wohlleben, Trudy M. H.

    Canadian High Arctic terrestrial ice 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/ice-albedo feedback (where area changes in snow and/or ice cause changes in surface albedo and surface air temperatures, leading to further area changes in snow/ice); and (2) The elevation - mass balance feedback (where thickness changes in terrestrial ice masses cause changes to atmospheric circulation and precipitation patterns, leading to further ice thickness changes). In this thesis, numerical experiments are performed to: (1) quantify the magnitudes of the two feedbacks for chosen Canadian High Arctic terrestrial ice masses; and (2) to examine the direct and indirect consequences of surface air temperature changes upon englacial temperatures with implications for ice flow, mass flux divergence, and topographic evolution. Model results show that: (a) for John Evans Glacier, Ellesmere Island, the magnitude of the terrestrial snow/ice-albedo feedback can locally exceed that of sea ice 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 ice cap accumulation zones, 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 zone; and (d) for Devon Ice Cap, observed mass gains in the northwest sector of the ice 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

  4. Investigating ice shelf mass loss processes from continuous satellite altimetry

    NASA Astrophysics Data System (ADS)

    Fricker, H. A.

    2017-12-01

    The Antarctic Ice Sheet continually gains mass through snowfall over its large area and, to remain approximately in equilibrium, it sheds most of this excess mass through two processes, basal melting and iceberg calving, that both occur in the floating ice shelves surrounding the continent. Small amounts of mass are also lost by surface melting, which occurs on many ice shelves every summer to varying degrees, and has been linked to ice-shelf collapse via hydrofracture on ice shelves that have been pre-weakened. Ice shelves provide mechanical support to `buttress' seaward flow of grounded ice, so that ice-shelf thinning and retreat result in enhanced ice discharge to the ocean. Ice shelves are susceptible to changes in forcing from both the atmosphere and the ocean, which both change on a broad range of timescales to modify mass gains and losses at the surface and base, and from internal instabilities of the ice sheet itself. Mass loss from iceberg calving is episodic, with typical intervals between calving events on the order of decades. Since ice shelves are so vast, the only viable way to monitor them is with satellites. Here, we discuss results from satellite radar and laser altimeter data from one NASA satellite (ICESat), and four ESA satellites (ERS-1, ERS-2, Envisat, CryoSat-2) to obtain estimates of ice-shelf surface height since the early 1990s. The continuous time series show accelerated losses in total Antarctic ice-shelf volume from 1994 to 2017, and allow us to investigate the processes causing ice-shelf mass change. For Larsen C, much of the variability comes from changing atmospheric conditions affecting firn state. In the Amundsen Sea, the rapid thinning is a combination of accelerated ocean-driven thinning and ice dynamics. This long-term thinning signal is, however, is strongly modulated by ENSO-driven interannual variability. However, observations of ocean variability around Antarctica are sparse, since these regions are often covered in sea ice

  5. Recent Changes in Ices Mass Balance of the Amundsen Sea Sector

    NASA Astrophysics Data System (ADS)

    Sutterley, T. C.; Velicogna, I.; Rignot, E. J.; Mouginot, J.; Flament, T.; van den Broeke, M. R.; van Wessem, M.; Reijmer, C.

    2014-12-01

    The glaciers flowing into the Amundsen Sea Embayment (ASE) sector of West Antarctica were confirmed in the Ice Sheet Mass Balance Inter-comparison Exercise (IMBIE) to be the dominant contributors to the current Antarctic ice mass loss, and recently recognized to be undergoing marine ice sheet instability. Here, we investigate their regional ice mass balance using a time series of satellite and airborne data combined with model output products from the Regional Atmospheric and Climate Model (RACMO). Our dataset includes laser altimetry from NASA's ICESat-1 satellite mission and from Operation IceBridge (OIB) airborne surveys, satellite radar altimetry data from ESA's Envisat mission, time-variable gravity data from NASA/DLR's GRACE mission, surface mass balance products from RACMO, ice velocity from a combination of international synthetic aperture radar satellites and ice thickness data from OIB. We find a record of ice mass balance for the ASE where all the analyzed techniques agree remarkably in magnitude and temporal variability. The mass loss of the region has been increasing continuously since 1992, with no indication of a slow down. The mass loss during the common period averaged 91 Gt/yr and accelerated 20 Gt/yr2. In 1992-2013, the ASE contributed 4.5 mm global sea level rise. Overall, our results demonstrate the synergy of multiple analysis techniques for examining Antarctic Ice Sheet mass balance at the regional scale. This work was performed at UCI and JPL under a contract with NASA.

  6. Southern Alaska Glaciers: Spatial and Temporal Variations in Ice Volume

    NASA Astrophysics Data System (ADS)

    Sauber, J.; Molnia, B. F.; Luthcke, S.; Rowlands, D.; Harding, D.; Carabajal, C.; Hurtado, J. M.; Spada, G.

    2004-12-01

    footprint returns to estimate glacier ice elevations and surface characteristics. To obtain the optimal ICESat results, we are reprocessing the ICESat data from Alaska to provide a well-calibrated regional ICESat solution. We anticipate that our ICESat results combined with earlier data will provide new constraints on the temporal and spatial variations in ice volume of individual Alaskan mountain ranges. These results allow us to address how recent melting of the southern Alaska glaciers contribute to short-term sea-level rise. Our results will also enable us to quantify crustal stress changes due to ice mass fluctuations and to assess the influence of ice mass changes on the seismically active southern Alaskan plate boundary zone.

  7. Clouds enhance Greenland ice sheet mass loss

    NASA Astrophysics Data System (ADS)

    Van Tricht, Kristof; Gorodetskaya, Irina V.; L'Ecuyer, Tristan; Lenaerts, Jan T. M.; Lhermitte, Stef; Noel, Brice; Turner, David D.; van den Broeke, Michiel R.; van Lipzig, Nicole P. M.

    2015-04-01

    Clouds have a profound influence on both the Arctic and global climate, while they still represent one of the key uncertainties in climate models, limiting the fidelity of future climate projections. The potentially important role of thin liquid-containing clouds over Greenland in enhancing ice sheet melt has recently gained interest, yet current research is spatially and temporally limited, focusing on particular events, and their large scale impact on the surface mass balance remains unknown. We used a combination of satellite remote sensing (CloudSat - CALIPSO), ground-based observations and climate model (RACMO) data to show that liquid-containing clouds warm the Greenland ice sheet 94% of the time. High surface reflectivity (albedo) for shortwave radiation reduces the cloud shortwave cooling effect on the absorbed fluxes, while not influencing the absorption of longwave radiation. Cloud warming over the ice sheet therefore dominates year-round. Only when albedo values drop below ~0.6 in the coastal areas during summer, the cooling effect starts to overcome the warming effect. The year-round excess of energy due to the presence of liquid-containing clouds has an extensive influence on the mass balance of the ice sheet. Simulations using the SNOWPACK snow model showed not only a strong influence of these liquid-containing clouds on melt increase, but also on the increased sublimation mass loss. Simulations with the Community Earth System Climate Model for the end of the 21st century (2080-2099) show that Greenland clouds contain more liquid water path and less ice water path. This implies that cloud radiative forcing will be further enhanced in the future. Our results therefore urge the need for improving cloud microphysics in climate models, to improve future projections of ice sheet mass balance and global sea level rise.

  8. Firn Thickness Changes (1982-2015) Driven by SMB from MERRA-2, RACMO2.3, ERA-Int and AVHRR Surface Temperature and the Impacts to Greenland Ice Sheet Mass Balance

    NASA Astrophysics Data System (ADS)

    Li, J.; Medley, B.; Neumann, T.; Smith, B. E.; Luthcke, S. B.; Zwally, H. J.

    2016-12-01

    Surface mass balance (SMB) data are essential in the derivation of ice sheet mass balance. This is because ice sheet mass change consists of short-term and long-term variations. The short-term variations are directly given by the SMB data. For altimetry based ice sheet mass balance studies, these short-term mass changes are converted to firn thickness changes by using a firn densification-elevation model, and then the variations are subtracted from the altimetry measurements to give the long-term ice thickness changes that are associated with the density of ice. So far various SMB data sets such as ERA-Interim, RACMO and MERRA are available and some have been widely used in large number of ice sheet mass balance studies. However theses data sets exhibit the clear discrepancies in both random and systematic manner. In this study, we use our time dependent firn densification- elevation model, driven by the SMB data from MERRA-2, RACMO2.3 and ERA-Int for the period of 1982-2015 and the temperature variations from AVHRR for the same period to examine the corresponding firn thickness variations and the impacts to the mass changes over the Greenland ice sheet. The model was initialized with the1980's climate. Our results show that the relative smaller (centimeter level) differences in the firn thickness driven by the different data set occur at the early stage (1980's) of the model run. As the time progressing, the discrepancies between the SMB data sets accumulate, and the corresponding firn thickness differences quickly become larger with the value > 2m at the end of the period. Although the overall rates for the whole period driven by each of the three data sets are small ranging -0.2 - 0.2 cm a-1 (-3.0-2.7 Gt a-1), the decadal rates can vary greatly with magnitude > 3 cm a-1 and the impact to the Greenland mass change exceeds 30 Gt a-1.

  9. Trends in ice sheet mass balance, 1992 to 2017

    NASA Astrophysics Data System (ADS)

    Shepherd, A.; Ivins, E. R.; Smith, B.; Velicogna, I.; Whitehouse, P. L.; Rignot, E. J.; van den Broeke, M. R.; Briggs, K.; Hogg, A.; Krinner, G.; Joughin, I. R.; Nowicki, S.; Payne, A. J.; Scambos, T.; Schlegel, N.; Moyano, G.; Konrad, H.

    2017-12-01

    The Ice Sheet Mass Balance Inter-Comparison Exercise (IMBIE) is a community effort, jointly supported by ESA and NASA, that aims to provide a consensus estimate of ice sheet mass balance from satellite gravimetry, altimetry and mass budget assessments, on an annual basis. The project has five experiment groups, one for each of the satellite techniques and two others to analyse surface mass balance (SMB) and glacial isostatic adjustment (GIA). The basic premise for the exercise is that individual ice sheet mass balance datasets are generated by project participants using common spatial and temporal domains to allow meaningful inter-comparison, and this controlled comparison in turn supports aggregation of the individual datasets over their full period. Participation is open to the full community, and the quality and consistency of submissions is regulated through a series of data standards and documentation requirements. The second phase of IMBIE commenced in 2015, with participant data submitted in 2016 and a combined estimate due for public release in 2017. Data from 48 participant groups were submitted to one of the three satellite mass balance technique groups or to the ancillary dataset groups. The individual mass balance estimates and ancillary datasets have been compared and combined within the respective groups. Following this, estimates of ice sheet mass balance derived from the individual techniques were then compared and combined. The result is single estimates of ice sheet mass balance for Greenland, East Antarctica, West Antarctica, and the Antarctic Peninsula. The participants, methodology and results of the exercise will be presented in this paper.

  10. Surface mass balance contributions to acceleration of Antarctic ice mass loss during 2003-2013

    NASA Astrophysics Data System (ADS)

    Seo, Ki-Weon; Wilson, Clark R.; Scambos, Ted; Kim, Baek-Min; Waliser, Duane E.; Tian, Baijun; Kim, Byeong-Hoon; Eom, Jooyoung

    2015-05-01

    Recent observations from satellite gravimetry (the Gravity Recovery and Climate Experiment (GRACE) mission) suggest an acceleration of ice mass loss from the Antarctic Ice Sheet (AIS). The contribution of surface mass balance changes (due to variable precipitation) is compared with GRACE-derived mass loss acceleration by assessing the estimated contribution of snow mass from meteorological reanalysis data. We find that over much of the continent, the acceleration can be explained by precipitation anomalies. However, on the Antarctic Peninsula and other parts of West Antarctica, mass changes are not explained by precipitation and are likely associated with ice discharge rate increases. The total apparent GRACE acceleration over all of the AIS between 2003 and 2013 is -13.6 ± 7.2 Gt/yr2. Of this total, we find that the surface mass balance component is -8.2 ± 2.0 Gt/yr2. However, the GRACE estimate appears to contain errors arising from the atmospheric pressure fields used to remove air mass effects. The estimated acceleration error from this effect is about 9.8 ± 5.8 Gt/yr2. Correcting for this yields an ice discharge acceleration of -15.1 ± 6.5 Gt/yr2.

  11. Surface Mass Balance Contributions to Acceleration of Antarctic Ice Mass Loss during 2003- 2013

    NASA Astrophysics Data System (ADS)

    Seo, K. W.; Wilson, C. R.; Scambos, T. A.; Kim, B. M.; Waliser, D. E.; Tian, B.; Kim, B.; Eom, J.

    2015-12-01

    Recent observations from satellite gravimetry (the GRACE mission) suggest an acceleration of ice mass loss from the Antarctic Ice Sheet (AIS). The contribution of surface mass balance changes (due to variable precipitation) is compared with GRACE-derived mass loss acceleration by assessing the estimated contribution of snow mass from meteorological reanalysis data. We find that over much of the continent, the acceleration can be explained by precipitation anomalies. However, on the Antarctic Peninsula and other parts of West Antarctica mass changes are not explained by precipitation and are likely associated with ice discharge rate increases. The total apparent GRACE acceleration over all of the AIS between 2003 and 2013 is -13.6±7.2 GTon/yr2. Of this total, we find that the surface mass balance component is -8.2±2.0 GTon/yr2. However, the GRACE estimate appears to contain errors arising from the atmospheric pressure fields used to remove air mass effects. The estimated acceleration error from this effect is about 9.8±5.8 GTon/yr2. Correcting for this yields an ice discharge acceleration of -15.1±6.5 GTon/yr2.

  12. Ice-Shelf Tidal Flexure and Subglacial Pressure Variations

    NASA Technical Reports Server (NTRS)

    Walker, Ryan T.; Parizek, Byron R.; Alley, Richard B.; Anandakrishnan, Sridhar; Riverman, Kiya L.; Christianson, Knut

    2013-01-01

    We develop a model of an ice shelf-ice 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 ice shelf dropping at low tide can cause significant (approx 1 cm) uplift in the first few kilometers of grounded ice.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 ice-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 ice would significantly change the radar reflectivity of the grounding zone and complicate the interpretation of grounded versus floating ice based on ice-penetrating radar observations.

  13. Overview of Sea-Ice Properties, Distribution and Temporal Variations, for Application to Ice-Atmosphere Chemical Processes.

    NASA Astrophysics Data System (ADS)

    Moritz, R. E.

    2005-12-01

    The properties, distribution and temporal variation of sea-ice are reviewed for application to problems of ice-atmosphere chemical processes. Typical vertical structure of sea-ice is presented for different ice types, including young ice, first-year ice and multi-year ice, emphasizing factors relevant to surface chemistry and gas exchange. Time average annual cycles of large scale variables are presented, including ice concentration, ice extent, ice thickness and ice age. Spatial and temporal variability of these large scale quantities is considered on time scales of 1-50 years, emphasizing recent and projected changes in the Arctic pack ice. The amount and time evolution of open water and thin ice are important factors that influence ocean-ice-atmosphere chemical processes. Observations and modeling of the sea-ice thickness distribution function are presented to characterize the range of variability in open water and thin ice.

  14. Mass loss of the Greenland peripheral glaciers and ice caps from satellite altimetry

    NASA Astrophysics Data System (ADS)

    Wouters, Bert; Noël, Brice; Moholdt, Geir; Ligtenberg, Stefan; van den Broeke, Michiel

    2017-04-01

    At its rapidly warming margins, the Greenland Ice Sheet is surrounded by (semi-)detached glaciers and ice caps (GIC). Although they cover only roughly 5% of the total glaciated area in the region, they are estimated to account for 15-20% of the total sea level rise contribution of Greenland. The spatial and temporal evolution of the mass changes of the peripheral GICs, however, remains poorly constrained. In this presentation, we use satellite altimetry from ICESat and Cryosat-2 combined with a high-resolution regional climate model to derive a 14 year time series (2003-2016) of regional elevation and mass changes. The total mass loss has been relatively constant during this period, but regionally, the GICs show marked temporal variations. Whereas thinning was concentrated along the eastern margin during 2003-2009, western GICs became the prime sea level rise contributors in recent years. Mass loss in the northern region has been steadily increasing throughout the record, due to a strong atmospheric warning and a deterioration of the capacity of the firn layer to buffer the resulting melt water.

  15. Mass Balance of the Northern Antarctic Peninsula and its Ongoing Response to Ice Shelf Loss

    NASA Astrophysics Data System (ADS)

    Scambos, T. A.; Berthier, E.; Haran, T. M.; Shuman, C. A.; Cook, A. J.; Bohlander, J. A.

    2012-12-01

    An assessment of the most rapidly changing areas of the Antarctic Peninsula (north of 66°S) shows that ice mass loss for the region is dominated by areas affected by eastern-Peninsula ice shelf losses in the past 20 years. Little if any of the mass loss is compensated by increased snowfall in the northwestern or far northern areas. We combined satellite stereo-image DEM differencing and ICESat-derived along-track elevation changes to measure ice mass loss for the Antarctic Peninsula north of 66°S between 2001-2010, focusing on the ICESat-1 period of operation (2003-2009). This mapping includes all ice drainages affected by recent ice shelf loss in the northeastern Peninsula (Prince Gustav, Larsen Inlet, Larsen A, and Larsen B) as well as James Ross Island, Vega Island, Anvers Island, Brabant Island and the adjacent west-flowing glaciers. Polaris Glacier (feeding the Larsen Inlet, which collapsed in 1986) is an exception, and may have stabilized. Our method uses ASTER and SPOT-5 stereo-image DEMs to determine dh/dt for elevations below 800 m; at higher elevations ICESat along-track elevation differencing is used. To adjust along-track path offsets between its 2003-2009 campaigns, we use a recent DEM of the Peninsula to establish and correct for cross-track slope (Cook et al., 2012, doi:10.5194/essdd-5-365-2012; http://nsidc.org/data/nsidc-0516.html) . We reduce the effect of possible seasonal variations in elevation by using only integer-year repeats of the ICESat tracks for comparison. Mass losses are dominated by the major glaciers that had flowed into the Prince Gustav (Boydell, Sjorgren, Röhss), Larsen A (Edgeworth, Bombardier, Dinsmoor, Drygalski), and Larsen B (Hektoria, Jorum, and Crane) embayments. The pattern of mass loss emphasizes the significant and multi-decadal response to ice shelf loss. Areas with shelf losses occurring 30 to 100s of years ago seem to be relatively stable or losing mass only slowly (western glaciers, northernmost areas). The

  16. A reconciled estimate of ice-sheet mass balance.

    PubMed

    Shepherd, Andrew; Ivins, Erik R; A, Geruo; Barletta, Valentina R; Bentley, Mike J; Bettadpur, Srinivas; Briggs, Kate H; Bromwich, David H; Forsberg, René; Galin, Natalia; Horwath, Martin; Jacobs, Stan; Joughin, Ian; King, Matt A; Lenaerts, Jan T M; Li, Jilu; Ligtenberg, Stefan R M; Luckman, Adrian; Luthcke, Scott B; McMillan, Malcolm; Meister, Rakia; Milne, Glenn; Mouginot, Jeremie; Muir, Alan; Nicolas, Julien P; Paden, John; Payne, Antony J; Pritchard, Hamish; Rignot, Eric; Rott, Helmut; Sørensen, Louise Sandberg; Scambos, Ted A; Scheuchl, Bernd; Schrama, Ernst J O; Smith, Ben; Sundal, Aud V; van Angelen, Jan H; van de Berg, Willem J; van den Broeke, Michiel R; Vaughan, David G; Velicogna, Isabella; Wahr, John; Whitehouse, Pippa L; Wingham, Duncan J; Yi, Donghui; Young, Duncan; Zwally, H Jay

    2012-11-30

    We combined an ensemble of satellite altimetry, interferometry, and gravimetry data sets using common geographical regions, time intervals, and models of surface mass balance and glacial isostatic adjustment to estimate the mass balance of Earth's polar ice sheets. We find that there is good agreement between different satellite methods--especially in Greenland and West Antarctica--and that combining satellite data sets leads to greater certainty. Between 1992 and 2011, the ice sheets of Greenland, East Antarctica, West Antarctica, and the Antarctic Peninsula changed in mass by -142 ± 49, +14 ± 43, -65 ± 26, and -20 ± 14 gigatonnes year(-1), respectively. Since 1992, the polar ice sheets have contributed, on average, 0.59 ± 0.20 millimeter year(-1) to the rate of global sea-level rise.

  17. Variations of the earth's magnetic field and rapid climatic cooling: A possible link through changes in global ice volume

    NASA Technical Reports Server (NTRS)

    Rampino, M. R.

    1979-01-01

    A possible relationship between large scale changes in global ice volume, variations in the earth's magnetic field, and short term climatic cooling is investigated through a study of the geomagnetic and climatic records of the past 300,000 years. The calculations suggest that redistribution of the Earth's water mass can cause rotational instabilities which lead to geomagnetic excursions; these magnetic variations in turn may lead to short-term coolings through upper atmosphere effects. Such double coincidences of magnetic excursions and sudden coolings at times of ice volume changes have occurred at 13,500, 30,000, 110,000, and 135,000 YBP.

  18. Surface mass balance contributions to acceleration of Antarctic ice mass loss during 2003-2013.

    PubMed

    Seo, Ki-Weon; Wilson, Clark R; Scambos, Ted; Kim, Baek-Min; Waliser, Duane E; Tian, Baijun; Kim, Byeong-Hoon; Eom, Jooyoung

    2015-05-01

    Recent observations from satellite gravimetry (the Gravity Recovery and Climate Experiment (GRACE) mission) suggest an acceleration of ice mass loss from the Antarctic Ice Sheet (AIS). The contribution of surface mass balance changes (due to variable precipitation) is compared with GRACE-derived mass loss acceleration by assessing the estimated contribution of snow mass from meteorological reanalysis data. We find that over much of the continent, the acceleration can be explained by precipitation anomalies. However, on the Antarctic Peninsula and other parts of West Antarctica, mass changes are not explained by precipitation and are likely associated with ice discharge rate increases. The total apparent GRACE acceleration over all of the AIS between 2003 and 2013 is -13.6 ± 7.2 Gt/yr 2 . Of this total, we find that the surface mass balance component is -8.2 ± 2.0 Gt/yr 2 . However, the GRACE estimate appears to contain errors arising from the atmospheric pressure fields used to remove air mass effects. The estimated acceleration error from this effect is about 9.8 ± 5.8 Gt/yr 2 . Correcting for this yields an ice discharge acceleration of -15.1 ± 6.5 Gt/yr 2 .

  19. Monitoring southwest Greenland's ice sheet melt with ambient seismic noise.

    PubMed

    Mordret, Aurélien; Mikesell, T Dylan; Harig, Christopher; Lipovsky, Bradley P; Prieto, Germán A

    2016-05-01

    The Greenland ice sheet presently accounts for ~70% of global ice sheet mass loss. Because this mass loss is associated with sea-level rise at a rate of 0.7 mm/year, the development of improved monitoring techniques to observe ongoing changes in ice sheet mass balance is of paramount concern. Spaceborne mass balance techniques are commonly used; however, they are inadequate for many purposes because of their low spatial and/or temporal resolution. We demonstrate that small variations in seismic wave speed in Earth's crust, as measured with the correlation of seismic noise, may be used to infer seasonal ice sheet mass balance. Seasonal loading and unloading of glacial mass induces strain in the crust, and these strains then result in seismic velocity changes due to poroelastic processes. Our method provides a new and independent way of monitoring (in near real time) ice sheet mass balance, yielding new constraints on ice sheet evolution and its contribution to global sea-level changes. An increased number of seismic stations in the vicinity of ice sheets will enhance our ability to create detailed space-time records of ice mass variations.

  20. A Reconciled Estimate of Ice-Sheet Mass Balance

    NASA Technical Reports Server (NTRS)

    Shepherd, Andrew; Ivins, Erik R.; Geruo, A.; Barletta, Valentia R.; Bentley, Mike J.; Bettadpur, Srinivas; Briggs, Kate H.; Bromwich, David H.; Forsberg, Rene; Galin, Natalia; hide

    2012-01-01

    We combined an ensemble of satellite altimetry, interferometry, and gravimetry data sets using common geographical regions, time intervals, and models of surface mass balance and glacial isostatic adjustment to estimate the mass balance of Earth's polar ice sheets. We find that there is good agreement between different satellite methods-especially in Greenland and West Antarctica-and that combining satellite data sets leads to greater certainty. Between 1992 and 2011, the ice sheets of Greenland, East Antarctica, West Antarctica, and the Antarctic Peninsula changed in mass by -142 plus or minus 49, +14 plus or minus 43, -65 plus or minus 26, and -20 plus or minus 14 gigatonnes year(sup -1), respectively. Since 1992, the polar ice sheets have contributed, on average, 0.59 plus or minus 0.20 millimeter year(sup -1) to the rate of global sea-level rise.

  1. The Greenland Ice Sheet's surface mass balance in a seasonally sea ice-free Arctic

    NASA Astrophysics Data System (ADS)

    Day, J. J.; Bamber, J. L.; Valdes, P. J.

    2013-09-01

    General circulation models predict a rapid decrease in sea ice extent with concurrent increases in near-surface air temperature and precipitation in the Arctic over the 21st century. This has led to suggestions that some Arctic land ice masses may experience an increase in accumulation due to enhanced evaporation from a seasonally sea ice-free Arctic Ocean. To investigate the impact of this phenomenon on Greenland Ice Sheet climate and surface mass balance (SMB), a regional climate model, HadRM3, was used to force an insolation-temperature melt SMB model. A set of experiments designed to investigate the role of sea ice independently from sea surface temperature (SST) forcing are described. In the warmer and wetter SI + SST simulation, Greenland experiences a 23% increase in winter SMB but 65% reduced summer SMB, resulting in a net decrease in the annual value. This study shows that sea ice decline contributes to the increased winter balance, causing 25% of the increase in winter accumulation; this is largest in eastern Greenland as the result of increased evaporation in the Greenland Sea. These results indicate that the seasonal cycle of Greenland's SMB will increase dramatically as global temperatures increase, with the largest changes in temperature and precipitation occurring in winter. This demonstrates that the accurate prediction of changes in sea ice cover is important for predicting Greenland SMB and ice sheet evolution.

  2. Convergence on the Prediction of Ice Particle Mass and Projected Area in Ice Clouds

    NASA Astrophysics Data System (ADS)

    Mitchell, D. L.

    2013-12-01

    Ice particle mass- and area-dimensional power law (henceforth m-D and A-D) relationships are building-blocks for formulating microphysical processes and optical properties in cloud and climate models, and they are critical for ice cloud remote sensing algorithms, affecting the retrieval accuracy. They can be estimated by (1) directly measuring the sizes, masses and areas of individual ice particles at ground-level and (2) using aircraft probes to simultaneously measure the ice water content (IWC) and ice particle size distribution. A third indirect method is to use observations from method 1 to develop an m-A relationship representing mean conditions in ice clouds. Owing to a tighter correlation (relative to m-D data), this m-A relationship can be used to estimate m from aircraft probe measurements of A. This has the advantage of estimating m at small sizes, down to 10 μm using the 2D-Sterio probe. In this way, 2D-S measurements of maximum dimension D can be related to corresponding estimates of m to develop ice cloud type and temperature dependent m-D expressions. However, these expressions are no longer linear in log-log space, but are slowly varying curves covering most of the size range of natural ice particles. This work compares all three of the above methods and demonstrates close agreement between them. Regarding (1), 4869 ice particles and corresponding melted hemispheres were measured during a field campaign to obtain D and m. Selecting only those unrimed habits that formed between -20°C and -40°C, the mean mass values for selected size intervals are within 35% of the corresponding masses predicted by the Method 3 curve based on a similar temperature range. Moreover, the most recent m-D expression based on Method 2 differs by no more than 50% with the m-D curve from Method 3. Method 3 appears to be the most accurate over the observed ice particle size range (10-4000 μm). An m-D/A-D scheme was developed by which self-consistent m-D and A-D power laws

  3. Application of GRACE to the assessment of model-based estimates of monthly Greenland Ice Sheet mass balance (2003-2012)

    NASA Astrophysics Data System (ADS)

    Schlegel, Nicole-Jeanne; Wiese, David N.; Larour, Eric Y.; Watkins, Michael M.; Box, Jason E.; Fettweis, Xavier; van den Broeke, Michiel R.

    2016-09-01

    the models while simultaneously having more pronounced trends; thus, discrepancies are likely controlled by a combination of missing processes and errors in both the SMB products and ISSM. At the margins, we find evidence of consistent intra-annual variations in regional MB that deviate distinctively from the SMB annual cycle. Ultimately, these monthly-scale variations, likely associated with hydrology or ice-ocean interaction, contribute to steeper negative mass trends observed by GRACE_JPL. Thus, models should consider such processes at relatively high (monthly-to-seasonal) temporal resolutions to achieve accurate estimates of Greenland MB.

  4. (abstract) Variations in Polarimetric Backscatter of Saline Ice Grown Under Diurnal Thermal Cycling Condition

    NASA Technical Reports Server (NTRS)

    Nghiem, S. V.; Kwok, R.; Yueh, S. H.; Kong, J. A.; Hsu, C. C.; Ding, K. H.

    1995-01-01

    An experiment was carried out in January 1994 at the Geophysical Research Facility in the Cold Regions Research and Engineering Laboratory. To investigate effects on polarimetric scattering signatures of sea ice growth under diurnal temperature variations, an ice sheet was grown for 2.5 days for the thickness of 10 cm and a polarimetric radar operating at C-band was used to obtain backscattering data in conjunction with ice-characterization measurements. The ice sheet was grown in the late morning of January 19, 1994. The initial growth rate was slow due to high insolation and temperature. As the air temperature dropped during the night, the growth rate increased significantly. The air temperature changed drastically from about -10(deg)C to -35(deg)C between day and night. The temperature cycle was repeated during the next day and the growth rate varied in the same manner. The surface of the ice was partially covered by frost flowers and the areal coverage increased as the ice became thicker. Throughout the ice growth duration of 2.5 days, polarimetric backscatter data were collected at roughly every centimeter of ice growth. For each set of radar measurements of saline ice, a set of calibration measurements was carried out with trihedrial corner reflectors and a metallic sphere. Measured polarimetric backscattering coefficients of the ice sheet reveal a strong correlation between radar data and temperature variations. As the temperature increased (decreased), the backscatter increased (decreased) correspondingly. From the ice-characterization data, temperatures of the air, at the ice-air interface, and in the ice layer had the same variation trend. Another interesting experimental observation is that the salinity measured as a function of ice depth from a sample of 10-cm thich ice indicated that the salinity variations had a similar cycle as the temperature; i.e., the salinity profile recorded the history of the temperature variations. Characterization data of the

  5. Understanding Recent Mass Balance Changes of the Greenland Ice Sheet

    NASA Technical Reports Server (NTRS)

    vanderVeen, Cornelius

    2003-01-01

    The ultimate goal of this project is to better understand the current transfer of mass between the Greenland Ice Sheet, the world's oceans and the atmosphere, and to identify processes controlling the rate of this transfer, to be able to predict with greater confidence future contributions to global sea level rise. During the first year of this project, we focused on establishing longer-term records of change of selected outlet glaciers, reevaluation of mass input to the ice sheet and analysis of climate records derived from ice cores, and modeling meltwater production and runoff from the margins of the ice sheet.

  6. Antarctic Glacial Isostatic Adjustment and Ice Sheet Mass Balance using GRACE: A Report from the Ice-sheet Mass Balance Exercise (IMBIE)

    NASA Astrophysics Data System (ADS)

    Ivins, E. R.; Wahr, J. M.; Schrama, E. J.; Milne, G. A.; Barletta, V.; Horwath, M.; Whitehouse, P.

    2012-12-01

    In preparation for the Inter-govermental Panel on Climate Change: Assessment Report 5 (IPCC AR5), ESA and NASA have formed a committee of experts to perform a formal set of comparative experiments concerning space observations of ice sheet mass balance. This project began in August of 2011 and has now concluded with a report submitted for Science (Shepherd et al., 2012). The focus of the work conducted is to re-evaluate scientific reports on the mass balance of Greenland ice sheet (GIS) and Antarctic ice sheet (AIS). The most serious discrepancies have been reported for the AIS, amounting to as much as 0.9 mm/yr in discrepant sea level contribution. A direct method of determining the AIS is by space gravimetry. However, for this method to contribute to our understanding of sea level change, we require knowledge of present-day non-elastic vertical movements of bedrock in Antarctica. Quantifying the uncertainty and bias caused by lack of observational control on models of regional glacial isostatic adjustment (GIA), was a major focus for our experiments. This regional process is the most problematic error source for GRACE-determinations of ice mass balance in Antarctica. While GIA likely dominates some large vertical motions in Antarctica that are now observed with GPS (Thomas et al., 2011, GRL), interpretations still require models. The reported uncertainty for space gravimetric (GRACE) based sea level sourcing is roughly 0.20 to 0.35 mm/yr. The uncertainty is also part of the error budget for mass balances derived from altimetry measurements, though at a much lower level. Analysis of the GRACE time series using CSR RL04 (2003.0-2010.10) for AIS mass balance reveals a small trend of order +1 to -24 Gt/yr without a GIA correction. Three periods were selected over which to perform inter-comparisons (see Table). One class of GIA models, that relies primarily on far field sea level reconstructions (e.g. ICE-5G), provide a GIA correction that places AIS mass imbalance (

  7. Devon Ice cap's future: results from climate and ice dynamics modelling via surface mass balance modelling

    NASA Astrophysics Data System (ADS)

    Rodehacke, C. B.; Mottram, R.; Boberg, F.

    2017-12-01

    The Devon Ice Cap is an example of a relatively well monitored small ice cap in the Canadian Arctic. Close to Greenland, it shows a similar surface mass balance signal to glaciers in western Greenland. Here we various boundary conditions, ranging from ERA-Interim reanalysis data via global climate model high resolution (5km) output from the regional climate model HIRHAM5, to determine the surface mass balance of the Devon ice cap. These SMB estimates are used to drive the PISM glacier model in order to model the present day and future prospects of this small Arctic ice cap. Observational data from the Devon Ice Cap in Arctic Canada is used to evaluate the surface mass balance (SMB) data output from the HIRHAM5 model for simulations forced with the ERA-Interim climate reanalysis data and the historical emissions scenario run by the EC-Earth global climate model. The RCP8.5 scenario simulated by EC-Earth is also downscaled by HIRHAM5 and this output is used to force the PISM model to simulate the likely future evolution of the Devon Ice Cap under a warming climate. We find that the Devon Ice Cap is likely to continue its present day retreat, though in the future increased precipitation partly offsets the enhanced melt rates caused by climate change.

  8. Analysis of sea ice dynamics

    NASA Technical Reports Server (NTRS)

    Zwally, J.

    1988-01-01

    The ongoing work has established the basis for using multiyear sea ice concentrations from SMMR passive microwave for studies of largescale advection and convergence/divergence of the Arctic sea ice pack. Comparisons were made with numerical model simulations and buoy data showing qualitative agreement on daily to interannual time scales. Analysis of the 7-year SMMR data set shows significant interannual variations in the total area of multiyear ice. The scientific objective is to investigate the dynamics, mass balance, and interannual variability of the Arctic sea ice pack. The research emphasizes the direct application of sea ice parameters derived from passive microwave data (SMMR and SSMI) and collaborative studies using a sea ice dynamics model. The possible causes of observed interannual variations in the multiyear ice area are being examined. The relative effects of variations in the large scale advection and convergence/divergence within the ice pack on a regional and seasonal basis are investigated. The effects of anomolous atmospheric forcings are being examined, including the long-lived effects of synoptic events and monthly variations in the mean geostrophic winds. Estimates to be made will include the amount of new ice production within the ice pack during winter and the amount of ice exported from the pack.

  9. Antarctic Ice-Sheet Mass Balance from Satellite Altimetry 1992 to 2001

    NASA Technical Reports Server (NTRS)

    Zwally, H. Jay; Brenner, Anita C.; Cornejo, Helen; Giovinetto, Mario; Saba, Jack L.; Yi, Donghui

    2003-01-01

    A major uncertainty in understanding the causes of the current rate of sea level rise is the potential contributions from mass imbalances of the Greenland and Antarctic ice sheets. Estimates of the current mass balance of the Antarctic ice sheet are derived from surface- elevation changes obtained from 9 years of ERS - 1 & 2 radar altimeter data. Elevation time-series are created from altimeter crossovers among 90-day data periods on a 50 km grid to 81.5 S. The time series are fit with a multivariate linear/sinusoidal function to give the average rate of elevation change (dH/dt). On the major Rome-Filchner, Ross, and Amery ice shelves, the W d t are small or near zero. In contrast, the ice shelves of the Antarctic Peninsula and along the West Antarctic coast appear to be thinning significantly, with a 23 +/- 3 cm per year surface elevation decrease on the Larsen ice shelf and a 65 +/- 4 cm per year decrease on the Dotson ice shelf. On the grounded ice, significant elevation decreases are obtained over most of the drainage basins of the Pine Island and Thwaites glaciers in West Antarctica and inland of Law Dome in East Antarctica. Significant elevation increases are observed within about 200 km of the coast around much of the rest of the ice sheet. Farther inland, the changes are a mixed pattern of increases and decreases with increases of a few centimeters per year at the highest elevations of the East Antarctic plateau. The derived elevation changes are combined with estimates of the bedrock uplift from several models to provide maps of ice thickness change. The ice thickness changes enable estimates of the ice mass balances for the major drainage basins, the overall mass balance, and the current contribution of the ice sheet to global sea level change.

  10. Do Europa's Mountains Have Roots? Erosion of Topography at the Ice-Water Interface via the "Ice Pump"

    NASA Astrophysics Data System (ADS)

    Goodman, J. C.

    2016-12-01

    Are topographic features on the surface of Europa and other icy worlds isostatically compensated by variations in shell thickness (Airy isostasy)? This is only possible if variations in shell thickness can remain stable over geologic time. Here we show that melting and freezing driven by the pressure dependence of the melting point of water - the "ice pump" - can rapidly erase topography at the ice/water interface. We consider ice pumps driven by both tidal action and buoyancy-driven flow. We first show that as tidal action drives the ocean up and down along a sloping interface, ice will be melted from areas where it's thickest and deposited where the ice is thinnest. We show that this process causes the ice interface topography to relax according to a simple "diffusion" linear partial differential equation. We estimate that a 10-km-wide topographic feature would be erased by the tidal ice pump in 3000 years if Europa's tidal current amplitude is 1 cm/s; however, this timescale is inversely proportional to the cube of the tidal velocity! Next, we consider an ice pump powered by ascent of meltwater along a sloping ice-water interface. We consider layer-averaged budgets for heat, mass, and momentum, along with turbulent mixing of the meltwater layer with underlying seawater via a Richardson number dependent entrainment process, and use these to estimate the thickness and mass flux of the meltwater layer. From this we estimate the rate of melting and freezing at the interface. These two ice pump processes combine with the glacial flow of warm basal ice to rapidly flatten out any variations in the height of the ice-water interface: Europa's ice/water interface may be perfectly flat! If so, topography at Europa's surface can only be supported by variations in density of the shell or the strength of the brittle surface ice.

  11. Effect of Ice-Shell Thickness Variations on the Tidal Deformation of Enceladus

    NASA Astrophysics Data System (ADS)

    Choblet, G.; Cadek, O.; Behounkova, M.; Tobie, G.; Kozubek, T.

    2015-12-01

    Recent analysis of Enceladus's gravity and topography has suggested that the thickness of the ice shell significantly varies laterally - from 30-40 km in the south polar region to 60 km elsewhere. These variations may influence the activity of the geysers and increase the tidal heat production in regions where the ice shell is thinned. Using a model including a regional or global subsurface ocean and Maxwell viscoelasticity, we investigate the impact of these variations on the tidal deformation of the moon and its heat production. For that purpose, we use different numerical approaches - finite elements, local application of 1d spectral method, and a generalized spectral method. Results obtained with these three approaches for various models of ice-shell thickness variations are presented and compared. Implications of a reduced ice shell thickness for the south polar terrain activity are discussed.

  12. Earth Structure, Ice Mass Changes, and the Local Dynamic Geoid

    NASA Astrophysics Data System (ADS)

    Harig, C.; Simons, F. J.

    2014-12-01

    Spherical Slepian localization functions are a useful method for studying regional mass changes observed by satellite gravimetry. By projecting data onto a sparse basis set, the local field can be estimated more easily than with the full spherical harmonic basis. We have used this method previously to estimate the ice mass change in Greenland from GRACE data, and it can also be applied to other planetary problems such as global magnetic fields. Earth's static geoid, in contrast to the time-variable field, is in large part related to the internal density and rheological structure of the Earth. Past studies have used dynamic geoid kernels to relate this density structure and the internal deformation it induces to the surface geopotential at large scales. These now classical studies of the eighties and nineties were able to estimate the mantle's radial rheological profile, placing constraints on the ratio between upper and lower mantle viscosity. By combining these two methods, spherical Slepian localization and dynamic geoid kernels, we have created local dynamic geoid kernels which are sensitive only to density variations within an area of interest. With these kernels we can estimate the approximate local radial rheological structure that best explains the locally observed geoid on a regional basis. First-order differences of the regional mantle viscosity structure are accessible to this technique. In this contribution we present our latest, as yet unpublished results on the geographical and temporal pattern of ice mass changes in Antarctica over the past decade, and we introduce a new approach to extract regional information about the internal structure of the Earth from the static global gravity field. Both sets of results are linked in terms of the relevant physics, but also in being developed from the marriage of Slepian functions and geoid kernels. We make predictions on the utility of our approach to derive fully three-dimensional rheological Earth models, to

  13. On the Utilization of Ice Flow Models and Uncertainty Quantification to Interpret the Impact of Surface Radiation Budget Errors on Estimates of Greenland Ice Sheet Surface Mass Balance and Regional Estimates of Mass Balance

    NASA Astrophysics Data System (ADS)

    Schlegel, N.; Larour, E. Y.; Gardner, A. S.; Lang, C.; Miller, C. E.; van den Broeke, M. R.

    2016-12-01

    How Greenland ice flow may respond to future increases in surface runoff and to increases in the frequency of extreme melt events is unclear, as it requires detailed comprehension of Greenland surface climate and the ice sheet's sensitivity to associated uncertainties. With established uncertainty quantification tools run within the framework of Ice Sheet System Model (ISSM), we conduct decadal-scale forward modeling experiments to 1) quantify the spatial resolution needed to effectively force distinct components of the surface radiation budget, and subsequently surface mass balance (SMB), in various regions of the ice sheet and 2) determine the dynamic response of Greenland ice flow to variations in components of the net radiation budget. The Glacier Energy and Mass Balance (GEMB) software is a column surface model (1-D) that has recently been embedded as a module within ISSM. Using the ISSM-GEMB framework, we perform sensitivity analyses to determine how perturbations in various components of the surface radiation budget affect model output; these model experiments allow us predict where and on what spatial scale the ice sheet is likely to dynamically respond to changes in these parameters. Preliminary results suggest that SMB should be forced at at least a resolution of 23 km to properly capture dynamic ice response. In addition, Monte-Carlo style sampling analyses reveals that the areas with the largest uncertainty in mass flux are located near the equilibrium line altitude (ELA), upstream of major outlet glaciers in the North and West of the ice sheet. Sensitivity analysis indicates that these areas are also the most vulnerable on the ice sheet to persistent, far-field shifts in SMB, suggesting that continued warming, and upstream shift in the ELA, are likely to result in increased velocities, and consequentially SMB-induced thinning upstream of major outlet glaciers. Here, we extend our investigation to consider various components of the surface radiation

  14. Overview of Ice-Sheet Mass Balance and Dynamics from ICESat Measurements

    NASA Technical Reports Server (NTRS)

    Zwally, H. Jay

    2010-01-01

    The primary purpose of the ICESat mission was to determine the present-day mass balance of the Greenland and Antarctic ice sheets, identify changes that may be occurring in the surface-mass flux and ice dynamics, and estimate their contributions to global sea-level rise. Although ICESat's three lasers were planned to make continuous measurements for 3 to 5 years, the mission was re-planned to operate in 33-day campaigns 2 to 3 times each year following failure of the first laser after 36 days. Seventeen campaigns were conducted with the last one in the Fall of 2009. Mass balance maps derived from measured ice-sheet elevation changes show that the mass loss from Greenland has increased significantly to about 170 Gt/yr for 2003 to 2007 from a state of near balance in the 1990's. Increased losses (189 Gt/yr) from melting and dynamic thinning are over seven times larger'than increased gains (25 gt/yr) from precipitation. Parts of the West Antarctic ice sheet and the Antarctic Peninsula are losing mass at an increasing rate, but other parts of West Antarctica and the East Antarctic ice sheet are gaining mass at an increasing rate. Increased losses of 35 Gt/yr in Pine Island, Thwaites-Smith, and Marie-Bryd.Coast are more than balanced by gains in base of Peninsula and ice stream C, D, & E systems. From the 1992-2002 to 2003-2007 period, the overall mass balance for Antarctica changed from a loss of about 60 Gt/yr to near balance or slightly positive.

  15. Mass Changes of the Greenland and Antarctic Ice Sheets and Shelves and Contributions to Sea-level Rise: 1992-2002

    NASA Technical Reports Server (NTRS)

    Zwally, H. Jay; Giovinetto, Mario B.; Li, Jun; Cornejo, Helen G.; Beckley, Matthew A.; Brenner, Anita C.; Saba, Jack L.; Yi, Donghui

    2005-01-01

    Changes in ice mass are estimated from elevation changes derived from 10.5 years (Greenland) and 9 years (Antarctica) of satellite radar altimetry data from the European Remote-sensing Satellites ERS-1 and -2. For the first time, the dH/dt values are adjusted for changes in surface elevation resulting from temperature-driven variations in the rate of fun compaction. The Greenland ice sheet is thinning at the margins (-42 plus or minus 2 Gta(sup -1) below the equilibrium line altitude (ELA)) and growing inland (+53 plus or minus 2 Gt a(sup -1)above the ELA) with a small overall mass gain (+11 plus or minus 3 Gt a(sup -1); -0.03 mm a(sup -1) SLE (sea level equivalent)). The ice sheet in West Antarctica (WA) is losing mass (-47 (dot) 4 GT a(sup -1) and the ice sheet in East Antarctica (EA) shows a small mass gain (+16 plus or minus 11 Gt a(sup -1) for a combined net change of -31 plus or minus 12 Gt a(sup -1) (+0.08 mm a(sup -1) SLE)). The contribution of the three ice sheets to sea level is +0.05 plus or minus 0.03 mm a(sup -1). The Antarctic ice shelves show corresponding mass changes of -95 (dot) 11 Gt a(sup -1) in WA and +142 plus or minus 10 Gt a(sup -1) in EA. Thinning at the margins of the Greenland ice sheet and growth at higher elevations is an expected response to increasing temperatures and precipitation in a warming climate. The marked thinnings in the Pine Island and Thwaites Glacier basins of WA and the Totten Glacier basin in EA are probably ice-dynamic responses to long-term climate change and perhaps past removal of their adjacent ice shelves. The ice growth in the southern Antarctic Peninsula and parts of EA may be due to increasing precipitation during the last century.

  16. Preliminary Investigation of Ice Shape Sensitivity to Parameter Variations

    NASA Technical Reports Server (NTRS)

    Miller, Dean R.; Potapczuk, Mark G.; Langhals, Tammy J.

    2005-01-01

    A parameter sensitivity study was conducted at the NASA Glenn Research Center's Icing Research Tunnel (IRT) using a 36 in. chord (0.91 m) NACA-0012 airfoil. The objective of this preliminary work was to investigate the feasibility of using ice shape feature changes to define requirements for the simulation and measurement of SLD icing conditions. It was desired to identify the minimum change (threshold) in a parameter value, which yielded an observable change in the ice shape. Liquid Water Content (LWC), drop size distribution (MVD), and tunnel static temperature were varied about a nominal value, and the effects of these parameter changes on the resulting ice shapes were documented. The resulting differences in ice shapes were compared on the basis of qualitative and quantitative criteria (e.g., mass, ice horn thickness, ice horn angle, icing limits, and iced area). This paper will provide a description of the experimental method, present selected experimental results, and conclude with an evaluation of these results, followed by a discussion of recommendations for future research.

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

    NASA Technical Reports Server (NTRS)

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

    1987-01-01

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

  18. Radar Interferometry Studies of the Mass Balance of Polar Ice Sheets

    NASA Technical Reports Server (NTRS)

    Rignot, Eric (Editor)

    1999-01-01

    The objectives of this work are to determine the current state of mass balance of the Greenland and Antarctic Ice Sheets. Our approach combines different techniques, which include satellite synthetic-aperture radar interferometry (InSAR), radar and laser altimetry, radar ice sounding, and finite-element modeling. In Greenland, we found that 3.5 times more ice flows out of the northern part of the Greenland Ice Sheet than previously accounted for. The discrepancy between current and past estimates is explained by extensive basal melting of the glacier floating sections in the proximity of the grounding line where the glacier detaches from its bed and becomes afloat in the ocean. The inferred basal melt rates are very large, which means that the glaciers are very sensitive to changes in ocean conditions. Currently, it appears that the northern Greenland glaciers discharge more ice than is being accumulated in the deep interior, and hence are thinning. Studies of temporal changes in grounding line position using InSAR confirm the state of retreat of northern glaciers and suggest that thinning is concentrated at the lower elevations. Ongoing work along the coast of East Greenland reveals an even larger mass deficit for eastern Greenland glaciers, with thinning affecting the deep interior of the ice sheet. In Antarctica, we found that glaciers flowing into a large ice shelf system, such as the Ronne Ice Shelf in the Weddell Sea, exhibit an ice discharge in remarkable agreement with mass accumulation in the interior, and the glacier grounding line positions do not migrate with time. Glaciers flowing rapidly into the Amudsen Sea, unrestrained by a major ice shelf, are in contrast discharging more ice than required to maintain a state of mass balance and are thinning quite rapidly near the coast. The grounding line of Pine Island glacier (see diagram) retreated 5 km in 4 years, which corresponds to a glacier thinning rate of 3.5 m/yr. Mass imbalance is even more negative

  19. Surface and basal ice shelf mass balance processes of the Southern McMurdo Ice Shelf determined through radar statistical reconnaissance

    NASA Astrophysics Data System (ADS)

    Grima, C.; Koch, I.; Greenbaum, J. S.; Soderlund, K. M.; Blankenship, D. D.; Young, D. A.; Fitzsimons, S.

    2017-12-01

    The McMurdo ice shelves (northern and southern MIS), adjacent to the eponymous station and the Ross Ice Shelf, Antarctica, are known for large gradients in surface snow accumulation and snow/ice impurities. Marine ice accretion and melting are important contributors to MIS's mass balance. Due to erosive winds, the southern MIS (SMIS) shows a locally negative surface mass balance. Thus, marine ice once accreted at the ice shelf base crops out at the surface. However, the exact processes that exert primary control on SMIS mass balance have remained elusive. Radar statistical reconnaissance (RSR) is a recent technique that has been used to characterize the surface properties of the Earth's cryosphere, Mars, and Titan from the stochastic character of energy scattered by the surface. Here, we apply RSR to map the surface density and roughness of the SMIS and extend the technique to derive the basal reflectance and scattering coefficients of the ice-ocean interface. We use an airborne radar survey grid acquired over the SMIS in the 2014-2015 austral summer by the University of Texas Institute for Geophysics with the High Capability Radar Sounder (HiCARS2; 60-MHz center frequency and 15-MHz bandwidth). The RSR-derived snow density values and patterns agree with directly -measured ice shelf surface accumulation rates. We also compare the composition of SMIS ice surface samples to test the ability of RSR to discriminate ices with varying dielectric properties (e.g., marine versus meteoric ice) and hypothesize relationships between the RSR-derived basal reflectance/scattered coefficients and accretion or melting at the ice-ocean interface. This improved knowledge of air-ice and ice-ocean boundaries provides a new perspective on the processes governing SMIS surface and basal mass balance.

  20. Sea Ice Mass Reconciliation Exercise (SIMRE) for altimetry derived sea ice thickness data sets

    NASA Astrophysics Data System (ADS)

    Hendricks, S.; Haas, C.; Tsamados, M.; Kwok, R.; Kurtz, N. T.; Rinne, E. J.; Uotila, P.; Stroeve, J.

    2017-12-01

    Satellite altimetry is the primary remote sensing data source for retrieval of Arctic sea-ice thickness. Observational data sets are available from current and previous missions, namely ESA's Envisat and CryoSat as well as NASA ICESat. In addition, freeboard results have been published from the earlier ESA ERS missions and candidates for new data products are the Sentinel-3 constellation, the CNES AltiKa mission and NASA laser altimeter successor ICESat-2. With all the different aspects of sensor type and orbit configuration, all missions have unique properties. In addition, thickness retrieval algorithms have evolved over time and data centers have developed different strategies. These strategies may vary in choice of auxiliary data sets, algorithm parts and product resolution and masking. The Sea Ice Mass Reconciliation Exercise (SIMRE) is a project by the sea-ice radar altimetry community to bridge the challenges of comparing data sets across missions and algorithms. The ESA Arctic+ research program facilitates this project with the objective to collect existing data sets and to derive a reconciled estimate of Arctic sea ice mass balance. Starting with CryoSat-2 products, we compare results from different data centers (UCL, AWI, NASA JPL & NASA GSFC) at full resolution along selected orbits with independent ice thickness estimates. Three regions representative of first-year ice, multiyear ice and mixed ice conditions are used to compare the difference in thickness and thickness change between products over the seasonal cycle. We present first results and provide an outline for the further development of SIMRE activities. The methodology for comparing data sets is designed to be extendible and the project is open to contributions by interested groups. Model results of sea ice thickness will be added in a later phase of the project to extend the scope of SIMRE beyond EO products.

  1. Greenland ice sheet surface temperature, melt and mass loss: 2000-06

    USGS Publications Warehouse

    Hall, D.K.; Williams, R.S.; Luthcke, S.B.; DiGirolamo, N.E.

    2008-01-01

    A daily time series of 'clear-sky' surface temperature has been compiled of the Greenland ice sheet (GIS) using 1 km resolution moderate-resolution imaging spectroradiometer (MODIS) land-surface temperature (LST) maps from 2000 to 2006. We also used mass-concentration data from the Gravity Recovery and Climate Experiment (GRACE) to study mass change in relationship to surface melt from 2003 to 2006. The mean LST of the GIS increased during the study period by ???0.27??Ca-1. The increase was especially notable in the northern half of the ice sheet during the winter months. Melt-season length and timing were also studied in each of the six major drainage basins. Rapid (<15 days) and sustained mass loss below 2000 m elevation was triggered in 2004 and 2005 as recorded by GRACE when surface melt begins. Initiation of large-scale surface melt was followed rapidly by mass loss. This indicates that surface meltwater is flowing rapidly to the base of the ice sheet, causing acceleration of outlet glaciers, thus highlighting the metastability of parts of the GIS and the vulnerability of the ice sheet to air-temperature increases. If air temperatures continue to rise over Greenland, increased surface melt will play a large role in ice-sheet mass loss.

  2. Contribution of Deformation to Sea Ice Mass Balance: A Case Study From an N-ICE2015 Storm

    NASA Astrophysics Data System (ADS)

    Itkin, Polona; Spreen, Gunnar; Hvidegaard, Sine Munk; Skourup, Henriette; Wilkinson, Jeremy; Gerland, Sebastian; Granskog, Mats A.

    2018-01-01

    The fastest and most efficient process of gaining sea ice volume is through the mechanical redistribution of mass as a consequence of deformation events. During the ice growth season divergent motion produces leads where new ice grows thermodynamically, while convergent motion fractures the ice and either piles the resultant ice blocks into ridges or rafts one floe under the other. Here we present an exceptionally detailed airborne data set from a 9 km2 area of first year and second year ice in the Transpolar Drift north of Svalbard that allowed us to estimate the redistribution of mass from an observed deformation event. To achieve this level of detail we analyzed changes in sea ice freeboard acquired from two airborne laser scanner surveys just before and right after a deformation event brought on by a passing low-pressure system. A linear regression model based on divergence during this storm can explain 64% of freeboard variability. Over the survey region we estimated that about 1.3% of level sea ice volume was pressed together into deformed ice and the new ice formed in leads in a week after the deformation event would increase the sea ice volume by 0.5%. As the region is impacted by about 15 storms each winter, a simple linear extrapolation would result in about 7% volume increase and 20% deformed ice fraction at the end of the season.

  3. 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.

  4. Antarctic and Greenland ice sheet mass balance products from satellite gravimetry

    NASA Astrophysics Data System (ADS)

    Horwath, Martin; Groh, Andreas; Horvath, Alexander; Forsberg, René; Meister, Rakia; Barletta, Valentina R.; Shepherd, Andrew

    2017-04-01

    Because of their important role in the Earth's climate system, ESA's Climate Change Initiative (CCI) has identified both the Antarctic Ice Sheet (AIS) and the Greenland Ice Sheet (GIS) as Essential Climate Variables (ECV). Since respondents of a user survey indicated that the ice sheet mass balance is one of the most important ECV data products needed to better understand climate change, the AIS_cci and the GIS_cci project provide Gravimetric Mass Balance (GMB) products based on satellite gravimetry data. The GMB products are derived from GRACE (Gravity Recovery and Climate Experiment) monthly solutions of release ITSG-Grace2016 produced at TU Graz. GMB basin products (i.e. time series of monthly mass changes for the entire ice sheets and selected drainage basins) and GMB gridded products (e.g. mass balance estimates with a formal resolution of about 50km, covering the entire ice sheets) are generated for the period from 2002 until present. The first GMB product was released in mid 2016. Here we present an extended and updated version of the ESA CCI GMB products, which are freely available through data portals hosted by the projects (https://data1.geo.tu-dresden.de/ais_gmb, http://products.esa-icesheets-cci.org/products/downloadlist/GMB). Since the initial product release, the applied processing strategies have been improved in order to further reduce GRACE errors and to enhance the separation of signals super-imposed to the ice mass changes. While a regional integration approach is used by the AIS_cci project, the GMB products of the GIS_cci project are derived using a point mass inversion. The differences between both approaches are investigated through the example of the GIS, where an alternative GMB product was generated using the regional integration approach implemented by the AIS_cci. Finally, we present the latest mass balance estimates for both ice sheets as well as their corresponding contributions to global sea level rise.

  5. Surface mass balance of Greenland mountain glaciers and ice caps

    NASA Astrophysics Data System (ADS)

    Benson, R. J.; Box, J. E.; Bromwich, D. H.; Wahr, J. M.

    2009-12-01

    Mountain glaciers and ice caps contribute roughly half of eustatic sea-level rise. Greenland has thousands of small mountain glaciers and several ice caps > 1000 sq. km that have not been included in previous mass balance calculations. To include small glaciers and ice 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 ice sheet ablation zone, but provides information useful in downscaling melt and accumulation rates on mountain glaciers and ice 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 ice core data from various regions along the Greenland ice sheet.

  6. Accelerated West Antarctic ice mass loss continues to outpace East Antarctic gains

    NASA Astrophysics Data System (ADS)

    Harig, Christopher; Simons, Frederik J.

    2015-04-01

    While multiple data sources have confirmed that Antarctica is losing ice at an accelerating rate, different measurement techniques estimate the details of its geographically highly variable mass balance with different levels of accuracy, spatio-temporal resolution, and coverage. Some scope remains for methodological improvements using a single data type. In this study we report our progress in increasing the accuracy and spatial resolution of time-variable gravimetry from the Gravity Recovery and Climate Experiment (GRACE). We determine the geographic pattern of ice mass change in Antarctica between January 2003 and June 2014, accounting for glacio-isostatic adjustment (GIA) using the IJ05_R2 model. Expressing the unknown signal in a sparse Slepian basis constructed by optimization to prevent leakage out of the regions of interest, we use robust signal processing and statistical estimation methods. Applying those to the latest time series of monthly GRACE solutions we map Antarctica's mass loss in space and time as well as can be recovered from satellite gravity alone. Ignoring GIA model uncertainty, over the period 2003-2014, West Antarctica has been losing ice mass at a rate of - 121 ± 8 Gt /yr and has experienced large acceleration of ice mass losses along the Amundsen Sea coast of - 18 ± 5 Gt /yr2, doubling the mass loss rate in the past six years. The Antarctic Peninsula shows slightly accelerating ice mass loss, with larger accelerated losses in the southern half of the Peninsula. Ice mass gains due to snowfall in Dronning Maud Land have continued to add about half the amount of West Antarctica's loss back onto the continent over the last decade. We estimate the overall mass losses from Antarctica since January 2003 at - 92 ± 10 Gt /yr.

  7. Greenland Ice Sheet Surface Temperature, Melt, and Mass Loss: 2000-2006

    NASA Technical Reports Server (NTRS)

    Hall, Dorothy K.; Williams, Richard S., Jr.; Luthcke, Scott B.; DiGirolamo, Nocolo

    2007-01-01

    Extensive melt on the Greenland Ice Sheet has been documented by a variety of ground and satellite measurements in recent years. If the well-documented warming continues in the Arctic, melting of the Greenland Ice Sheet will likely accelerate, contributing to sea-level rise. Modeling studies indicate that an annual or summer temperature rise of 1 C on the ice sheet will increase melt by 20-50% therefore, surface temperature is one of the most important ice-sheet parameters to study for analysis of changes in the mass balance of the ice-sheet. The Greenland Ice Sheet contains enough water to produce a rise in eustatic sea level of up to 7.0 m if the ice were to melt completely. However, even small changes (centimeters) in sea level would cause important economic and societal consequences in the world's major coastal cities thus it is extremely important to monitor changes in the ice-sheet surface temperature and to ultimately quantify these changes in terms of amount of sea-level rise. We have compiled a high-resolution, daily time series of surface temperature of the Greenland Ice Sheet, using the I-km resolution, clear-sky land-surface temperature (LST) standard product from the Moderate-Resolution Imaging Spectroradiometer (MODIS), from 2000 - 2006. We also use Gravity Recovery and Climate Experiment (GRACE) data, averaged over 10-day periods, to measure change in mass of the ice sheet as it melt and snow accumulates. Surface temperature can be used to determine frequency of surface melt, timing of the start and the end of the melt season, and duration of melt. In conjunction with GRACE data, it can also be used to analyze timing of ice-sheet mass loss and gain.

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

    NASA Astrophysics Data System (ADS)

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

    2016-12-01

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

  9. Time Series of Greenland Ice-Sheet Elevations and Mass Changes from ICESat 2003-2009

    NASA Astrophysics Data System (ADS)

    Zwally, H. J.; Li, J.; Medley, B.; Robbins, J. W.; Yi, D.

    2015-12-01

    We follow the repeat-track analysis (RTA) of ICESat surface-elevation data by a second stage that adjusts the measured elevations on repeat passes to the reference track taking into account the cross-track slope (αc), in order to construct elevation time series. αc are obtained from RTA simultaneous solutions for αc, dh/dt, and h0. The height measurements on repeat tracks are initially interpolated to uniform along-track reference points (every 172 m) and times (ti) giving the h(xi,ti) used in the RTA solutions. The xi are the cross-track spacings from the reference track and i is the laser campaign index. The adjusted elevation measurements at the along-track reference points are hr(ti) = h(xi,ti) - xi tan(αc) - h0. The hr(ti) time series are averaged over 50 km cells creating H(ti) series and further averaged (weighted by cell area) to H(t) time series over drainage systems (DS), elevation bands, regions, and the entire ice sheet. Temperature-driven changes in the rate of firn compaction, CT(t), are calculated for 50 km cells with our firn-compaction model giving I(t) = H(t) - CT(t) - B(t) where B(t) is the vertical motion of the bedrock. During 2003 to 2009, the average dCT(t)/dt in the accumulation zone is -5 cm/yr, which amounts to a -75 km3/yr correction to ice volume change estimates. The I(t) are especially useful for studying the seasonal cycle of mass gains and losses and interannual variations. The H(t) for the ablation zone are fitted with a multi-variate function with a linear component describing the upward component of ice flow plus winter accumulation (fall through spring) and a portion of a sine function describing the superimposed summer melting. During fall to spring the H(t) indicate that the upward motion of the ice flow is at a rate of 1 m/yr, giving an annual mass gain of 180 Gt/yr in the ablation zone. The summer loss from surface melting in the high-melt summer of 2005 is 350 Gt/yr, giving a net surface loss of 170 Gt/yr from the

  10. Thickening and Thinning of Antarctic Ice Shelves and Tongues and Mass Balance Estimates

    NASA Technical Reports Server (NTRS)

    Zwally, H. Jay; Li, Jun; Giovinetto, Mario; Robbins, John; Saba, Jack L.; Yi, Donghui

    2011-01-01

    Previous analysis of elevation changes for 1992 to 2002 obtained from measurements by radar altimeters on ERS-l and 2 showed that the shelves in the Antarctic Peninsula (AP) and along the coast of West Antarctica (WA), including the eastern part of the Ross Ice Shelf, were mostly thinning and losing mass whereas the Ronne Ice shelf also in WA was mostly thickening. The estimated total mass loss for the floating ice shelves and ice tongues from ice draining WA and the AP was 95 Gt/a. In contrast, the floating ice shelves and ice tongues from ice draining East Antarctica (EA), including the Filchner, Fimbul, Amery, and Western Ross, were mostly thickening with a total estimated mass gain of 142 Gt/a. Data from ICESat laser altimetry for 2003-2008 gives new surface elevation changes (dH/dt) with some similar values for the earlier and latter periods, including -27.6 and -26.9 cm a-Ion the West Getz ice shelf and -42.4 and - 27.2 cm/a on the East Getz ice shelf, and some values that indicate more thinning in the latter period, including -17.9 and -36.2 cm/a on the Larsen C ice shelf, -35.5 and -76.0 cm/a on the Pine Island Glacier floating, -60.5 and -125.7 .cm/a on the Smith Glacier floating, and -34.4 and -108.9 cm/a on the Thwaites Glacier floating. Maps of measured dH/dt and estimated thickness change are produced along with mass change estimates for 2003 - 2008.

  11. Mass Balance of the West Antarctic Ice-Sheet from ICESat Measurements

    NASA Technical Reports Server (NTRS)

    Zwally, H. Jay; Li, Jun; Robins, John; Saba, Jack L.; Yi, Donghui

    2011-01-01

    Mass balance estimates for 2003-2008 are derived from ICESat laser altimetry and compared with estimates for 1992-2002 derived from ERS radar altimetry. The net mass balance of 3 drainage systems (Pine Island, Thwaites/Smith, and the coast of Marie Bryd) for 2003-2008 is a loss of 100 Gt/yr, which increased from a loss of 70 Gt/yr for the earlier period. The DS including the Bindschadler and MacAyeal ice streams draining into the Ross Ice Shelf has a mass gain of 11 Gt/yr for 2003-2008, compared to an earlier loss of 70 Gt/yr. The DS including the Whillans and Kamb ice streams has a mass gain of 12 Gt/yr, including a significant thickening on the upper part of the Kamb DS, compared to a earlier gain of 6 Gt/yr (includes interpolation for a large portion of the DS). The other two DS discharging into the Ronne Ice Shelf and the northern Ellsworth Coast have a mass gain of 39 Gt/yr, compared to a gain of 4 Gt/yr for the earlier period. Overall, the increased losses of 30 Gt/yr in the Pine Island, Thwaites/Smith, and the coast of Marie Bryd DSs are exceeded by increased gains of 59 Gt/yr in the other 4 DS. Overall, the mass loss from the West Antarctic ice sheet has decreased to 38 Gt/yr from the earlier loss of 67 Gt/yr, reducing the contribution to sea level rise to 0.11 mm/yr from 0.19 mm/yr

  12. Factors Contributing To Genetic Variation In Ice Damage Susceptibility In Shortleaf Pine

    Treesearch

    Ronald C. Schmidtling; Valerie Hipkins

    2002-01-01

    There are differences among species in susceptibility to ice damage (Williston 1974). There is also at least one report on within-species variation, where coastal Ioblolly pine was damaged more than interior seed sources in an ice storm (Jones and Wells 1969). Of ail the maladies affecting the growth and s&ival of southern pines. damage from ice storms is one of...

  13. Solar cycle and long term variations of mesospheric ice layers

    NASA Astrophysics Data System (ADS)

    Lübken, Franz-Josef; Berger, Uwe; Kiliani, Johannes; Baumgarten, Gerd; Fiedler, Jens; Gerding, Michael

    2010-05-01

    Ice layers in the summer mesosphere at middle and polar latitudes, frequently called `noctilucent clouds' (NLC) or `polar mesosphere clouds'(PMC), are considered to be sensitive indicators of long term changes in the middle atmosphere. We present a summary of long term observations from the ground and from satellites and compare with results from the LIMA model (Leibniz Institute Middle Atmosphere Model). LIMA nicely reproduces mean conditions of the summer mesopause region and also mean characteristics of ice layers. LIMA nudges to ECMWF data in the troposphere and lower stratosphere which influences the background conditions in the mesosphere and thereby the morphology of ice clouds. A strong correlation between temperatures and PMC altitudes is observed. Applied to historical measurements this give s negligible temperature trends at PMC altitudes (approximately 0.01-0.02 K/y). Trace gas concentrations are kept constant in LIMA except for water vapor which is modified by variable solar radiation. Still, long term trends in temperatures and ice layer parameters are observed, consistent with observations. As will be shown, these trends originate in the stratosphere. Solar cycle effects are expected in ice layers due to variations in background temperatures and water paper. We will present results from LIMA regarding solar cycle variations and compare with NLC observations at our lidar stations in Kühlungsborn (54°N) and ALOMAR (69°N), and also with satellite measurements.

  14. Glacier Ice Mass Fluctuations and Fault Instability in Tectonically Active Southern Alaska

    NASA Technical Reports Server (NTRS)

    SauberRosenberg, Jeanne M.; Molnia, Bruce F.

    2003-01-01

    Across southern Alaska the northwest directed subduction of the Pacific plate is accompanied by accretion of the Yakutat terrane to continental Alaska. This has led to high tectonic strain rates and dramatic topographic relief of more than 5000 meters within 15 km of the Gulf of Alaska coast. The glaciers of this area are extensive and include large glaciers undergoing wastage (glacier retreat and thinning) and surges. The large glacier ice mass changes perturb the tectonic rate of deformation at a variety of temporal and spatial scales. We estimated surface displacements and stresses associated with ice mass fluctuations and tectonic loading by examining GPS geodetic observations and numerical model predictions. Although the glacial fluctuations perturb the tectonic stress field, especially at shallow depths, the largest contribution to ongoing crustal deformation is horizontal tectonic strain due to plate convergence. Tectonic forces are thus the primary force responsible for major earthquakes. However, for geodetic sites located < 10-20 km from major ice mass fluctuations, the changes of the solid Earth due to ice loading and unloading are an important aspect of interpreting geodetic results. The ice changes associated with Bering Glacier s most recent surge cycle are large enough to cause discernible surface displacements. Additionally, ice mass fluctuations associated with the surge cycle can modify the short-term seismicity rates in a local region. For the thrust faulting environment of the study region a large decrease in ice load may cause an increase in seismic rate in a region close to failure whereas ice loading may inhibit thrust faulting.

  15. Mass Balance Changes and Ice Dynamics of Greenland and Antarctic Ice Sheets from Laser Altimetry

    NASA Astrophysics Data System (ADS)

    Babonis, G. S.; Csatho, B.; Schenk, T.

    2016-06-01

    During the past few decades the Greenland and Antarctic ice sheets have lost ice at accelerating rates, caused by increasing surface temperature. The melting of the two big ice sheets has a big impact on global sea level rise. If the ice sheets would melt down entirely, the sea level would rise more than 60 m. Even a much smaller rise would cause dramatic damage along coastal regions. In this paper we report about a major upgrade of surface elevation changes derived from laser altimetry data, acquired by NASA's Ice, Cloud and land Elevation Satellite mission (ICESat) and airborne laser campaigns, such as Airborne Topographic Mapper (ATM) and Land, Vegetation and Ice Sensor (LVIS). For detecting changes in ice sheet elevations we have developed the Surface Elevation Reconstruction And Change detection (SERAC) method. It computes elevation changes of small surface patches by keeping the surface shape constant and considering the absolute values as surface elevations. We report about important upgrades of earlier results, for example the inclusion of local ice caps and the temporal extension from 1993 to 2014 for the Greenland Ice Sheet and for a comprehensive reconstruction of ice thickness and mass changes for the Antarctic Ice Sheets.

  16. Modeled Variations of Precipitation over the Greenland Ice Sheet.

    NASA Astrophysics Data System (ADS)

    Bromwich, David H.; Robasky, Frank M.; Keen, Richard A.; Bolzan, John F.

    1993-07-01

    A parameterization of the synoptic activity at 500 hPa and a simple orographic scheme are used to model the spatial and temporal variations of precipitation over the Greenland Ice Sheet for 1963-88 from analyzed geopotential height fields produced by the National Meteorological Center (NMC). Model coefficients are fitted to observed accumulation data, primarily from the summit area of the ice sheet. All major spatial characteristics of the observed accumulation distribution are reproduced apart from the orographic accumulation maximum over the northwestern coastal slopes. The modeled time-averaged total precipitation amount over Greenland is within the range of values determined by other investigators from surface-based observations. A realistic degree of interannual variability in precipitation is also simulated.A downward trend in simulated ice sheet precipitation over the 26 years is found. This is supported by a number of lines of evidence. It matches the accumulation trends during this period from ice cores drilled in south-central Greenland. The lower tropospheric specific humidifies at two south coastal radiosonde stations also decrease over this interval. A systematic shift away from Greenland and a decrease in activity of the dominant storm track are found for relatively low precipitation periods as compared to relatively high precipitation periods. This negative precipitation trend would mean that the Greenland Ice Sheet, depending on its 1963 mass balance state, has over the 1963-88 period either decreased its negative, or increased its positive, contribution to recently observed global sea level rise.Superimposed on the declining simulated precipitation rate for the entire ice sheet is a pronounced 3-5-yr periodicity. This is prominent in the observed and modeled precipitation time series from Summit, Greenland. This cycle shows some aspects in common with the Southern Oscillation.Some deficiencies in the NMC analysts were highlighted by this work. A

  17. Abiotic versus biotic drivers of ocean pH variation under fast sea ice in McMurdo Sound, Antarctica.

    PubMed

    Matson, Paul G; Washburn, Libe; Martz, Todd R; Hofmann, Gretchen E

    2014-01-01

    Ocean acidification is expected to have a major effect on the marine carbonate system over the next century, particularly in high latitude seas. Less appreciated is natural environmental variation within these systems, particularly in terms of pH, and how this natural variation may inform laboratory experiments. In this study, we deployed sensor-equipped moorings at 20 m depths at three locations in McMurdo Sound, comprising deep (bottom depth>200 m: Hut Point Peninsula) and shallow environments (bottom depth ∼25 m: Cape Evans and New Harbor). Our sensors recorded high-frequency variation in pH (Hut Point and Cape Evans only), tide (Cape Evans and New Harbor), and water mass properties (temperature and salinity) during spring and early summer 2011. These collective observations showed that (1) pH differed spatially both in terms of mean pH (Cape Evans: 8.009±0.015; Hut Point: 8.020±0.007) and range of pH (Cape Evans: 0.090; Hut Point: 0.036), and (2) pH was not related to the mixing of two water masses, suggesting that the observed pH variation is likely not driven by this abiotic process. Given the large daily fluctuation in pH at Cape Evans, we developed a simple mechanistic model to explore the potential for biotic processes--in this case algal photosynthesis--to increase pH by fixing carbon from the water column. For this model, we incorporated published photosynthetic parameters for the three dominant algal functional groups found at Cape Evans (benthic fleshy red macroalgae, crustose coralline algae, and sea ice algal communities) to estimate oxygen produced/carbon fixed from the water column underneath fast sea ice and the resulting pH change. These results suggest that biotic processes may be a primary driver of pH variation observed under fast sea ice at Cape Evans and potentially at other shallow sites in McMurdo Sound.

  18. Abiotic versus Biotic Drivers of Ocean pH Variation under Fast Sea Ice in McMurdo Sound, Antarctica

    PubMed Central

    Matson, Paul G.; Washburn, Libe; Martz, Todd R.; Hofmann, Gretchen E.

    2014-01-01

    Ocean acidification is expected to have a major effect on the marine carbonate system over the next century, particularly in high latitude seas. Less appreciated is natural environmental variation within these systems, particularly in terms of pH, and how this natural variation may inform laboratory experiments. In this study, we deployed sensor-equipped moorings at 20 m depths at three locations in McMurdo Sound, comprising deep (bottom depth>200 m: Hut Point Peninsula) and shallow environments (bottom depth ∼25 m: Cape Evans and New Harbor). Our sensors recorded high-frequency variation in pH (Hut Point and Cape Evans only), tide (Cape Evans and New Harbor), and water mass properties (temperature and salinity) during spring and early summer 2011. These collective observations showed that (1) pH differed spatially both in terms of mean pH (Cape Evans: 8.009±0.015; Hut Point: 8.020±0.007) and range of pH (Cape Evans: 0.090; Hut Point: 0.036), and (2) pH was not related to the mixing of two water masses, suggesting that the observed pH variation is likely not driven by this abiotic process. Given the large daily fluctuation in pH at Cape Evans, we developed a simple mechanistic model to explore the potential for biotic processes – in this case algal photosynthesis – to increase pH by fixing carbon from the water column. For this model, we incorporated published photosynthetic parameters for the three dominant algal functional groups found at Cape Evans (benthic fleshy red macroalgae, crustose coralline algae, and sea ice algal communities) to estimate oxygen produced/carbon fixed from the water column underneath fast sea ice and the resulting pH change. These results suggest that biotic processes may be a primary driver of pH variation observed under fast sea ice at Cape Evans and potentially at other shallow sites in McMurdo Sound. PMID:25221950

  19. Prediction of dry ice mass for firefighting robot actuation

    NASA Astrophysics Data System (ADS)

    Ajala, M. T.; Khan, Md R.; Shafie, A. A.; Salami, MJE; Mohamad Nor, M. I.

    2017-11-01

    The limitation in the performance of electric actuated firefighting robots in high-temperature fire environment has led to research on the alternative propulsion system for the mobility of firefighting robots in such environment. Capitalizing on the limitations of these electric actuators we suggested a gas-actuated propulsion system in our earlier study. The propulsion system is made up of a pneumatic motor as the actuator (for the robot) and carbon dioxide gas (self-generated from dry ice) as the power source. To satisfy the consumption requirement (9cfm) of the motor for efficient actuation of the robot in the fire environment, the volume of carbon dioxide gas, as well as the corresponding mass of the dry ice that will produce the required volume for powering and actuation of the robot, must be determined. This article, therefore, presents the computational analysis to predict the volumetric requirement and the dry ice mass sufficient to power a carbon dioxide gas propelled autonomous firefighting robot in a high-temperature environment. The governing equation of the sublimation of dry ice to carbon dioxide is established. An operating time of 2105.53s and operating pressure ranges from 137.9kPa to 482.65kPa were achieved following the consumption rate of the motor. Thus, 8.85m3 is computed as the volume requirement of the CAFFR while the corresponding dry ice mass for the CAFFR actuation ranges from 21.67kg to 75.83kg depending on the operating pressure.

  20. Dual-sensor mapping of mass balance on Russia's northernmost ice caps

    NASA Astrophysics Data System (ADS)

    Nikolskiy, D.; Malinnikov, V.; Sharov, A.; Ukolova, M.

    2012-04-01

    Mass balance of Russia's northernmost ice caps is poorly known and scarcely mapped. Thorough information about glacier fluctuations in the outer periphery of Russian shelf seas is both lacking and highly desired since it may constitute the relevant benchmark for judging and projecting climate change impacts in the entire Arctic. The present study is focussed on geodetic measurements and medium-scale mapping of the mass balance on a dozen insular ice caps, some large and some smaller, homogeneously situated along the Eurasian boundary of Central Arctic Basin. The study region extends for approx. 2.200 km from Victoria and Arthur islands in the west across Rudolph, Eva-Liv, Ushakova, Schmidt and Komsomolets islands in the north to Bennett and Henrietta islands in the east thereby comprising the most distant and least studied ice caps in the Russian Arctic. The situation of insular ice masses close to the edge of summer minimum sea ice proved helpful in analysing spatial asymmetry of glacier accumulation signal. The overall mapping of glacier elevation changes and quantification of mass balance characteristics in the study region was performed by comparing reference elevation models of study glaciers derived from Russian topographic maps 1:200,000 (CI = 20 or 40 m) representing the glacier state as in the 1950s-1960s with modern elevation data obtained from satellite radar interferometry and lidar altimetry. In total, 14 ERS and 4 TanDEM-X high-quality SAR interferograms of 1995/96 and 2011 were acquired, processed in the standard 2-pass DINSAR manner, geocoded, calibrated, mosaicked and interpreted using reference elevation models and co-located ICESat altimetry data of 2003-2010. The DINSAR analysis revealed the existence of fast-flowing outlet glaciers at Arthur, Rudolph, Eva-Liv and Bennett islands. The calculation of separate mass-balance components is complicated in this case because of generally unknown glacier velocities and ice discharge values for the mid-20

  1. The influence of topographic feedback on a coupled mass balance and ice-flow model for Vestfonna ice-cap, Svalbard

    NASA Astrophysics Data System (ADS)

    Schäfer, Martina; Möller, Marco; Zwinger, Thomas; Moore, John

    2016-04-01

    Using a coupled simulation set-up between a by statistical climate data forced and to ice-cap resolution downscaled mass balance model and an ice-dynamic model, we study coupling effects for the Vestfonna ice cap, Nordaustlandet, Svalbard, by analysing the impacts of different imposed coupling intervals on mass-balance and sea-level rise (SLR) projections. Based on a method to estimate errors introduced by different coupling schemes, we find that neglecting the topographic feedback in the coupling leads to underestimations of 10-20% in SLR projections on century time-scales in our model compared to full coupling (i.e., exchange of properties using smallest occurring time-step). Using the same method it also is shown that parametrising mass-balance adjustment for changes in topography using lapse rates is a - in computational terms - cost-effective reasonably accurate alternative applied to an ice-cap like Vestfonna. We test the forcing imposed by different emission pathways (RCP 2.4, 4.5, 6.0 and 8.5). For most of them, over the time-period explored (2000-2100), fast-flowing outlet glaciers decrease in impacting SLR due to their deceleration and reduced mass flux as they thin and retreat from the coast, hence detaching from the ocean and thereby losing their major mass drainage mechanism, i.e., calving.

  2. Antarctic ice sheet mass loss estimates using Modified Antarctic Mapping Mission surface flow observations

    NASA Astrophysics Data System (ADS)

    Ren, Diandong; Leslie, Lance M.; Lynch, Mervyn J.

    2013-03-01

    The long residence time of ice and the relatively gentle slopes of the Antarctica Ice Sheet make basal sliding a unique positive feedback mechanism in enhancing ice discharge along preferred routes. The highly organized ice stream channels extending to the interior from the lower reach of the outlets are a manifestation of the role of basal granular material in enhancing the ice flow. In this study, constraining the model-simulated year 2000 ice flow fields with surface velocities obtained from InSAR measurements permits retrieval of the basal sliding parameters. Forward integrations of the ice model driven by atmospheric and oceanic parameters from coupled general circulation models under different emission scenarios provide a range of estimates of total ice mass loss during the 21st century. The total mass loss rate has a small intermodel and interscenario spread, rising from approximately -160 km3/yr at present to approximately -220 km3/yr by 2100. The accelerated mass loss rate of the Antarctica Ice Sheet in a warming climate is due primarily to a dynamic response in the form of an increase in ice flow speed. Ice shelves contribute to this feedback through a reduced buttressing effect due to more frequent systematic, tabular calving events. For example, by 2100 the Ross Ice Shelf is projected to shed 40 km3 during each systematic tabular calving. After the frontal section's attrition, the remaining shelf will rebound. Consequently, the submerged cross-sectional area will reduce, as will the buttressing stress. Longitudinal differential warming of ocean temperature contributes to tabular calving. Because of the prevalence of fringe ice shelves, oceanic effects likely will play a very important role in the future mass balance of the Antarctica Ice Sheet, under a possible future warming climate.

  3. Is snow-ice now a major contributor to sea ice mass balance in the western Transpolar Drift region?

    NASA Astrophysics Data System (ADS)

    Graham, R. M.; Merkouriadi, I.; Cheng, B.; Rösel, A.; Granskog, M. A.

    2017-12-01

    During the Norwegian young sea ICE (N-ICE2015) campaign, which took place in the first half of 2015 north of Svalbard, a deep winter snow pack (50 cm) on sea ice was observed, that was 50% thicker than earlier climatological studies suggested for this region. Moreover, a significant fraction of snow contributed to the total ice mass in second-year ice (SYI) (9% on average). Interestingly, very little snow (3% snow by mass) was present in first-year ice (FYI). The combination of sea ice thinning and increased precipitation north of Svalbard is expected to promote the formation of snow-ice. Here we use the 1-D snow/ice thermodynamic model HIGHTSI forced with reanalysis data, to show that for the case study of N-ICE2015, snow-ice would even form over SYI with an initial thickness of 2 m. In current conditions north of Svalbard, snow-ice is ubiquitous and contributes to the thickness growth up to 30%. This contribution is important, especially in the absence of any bottom thermodynamic growth due to the thick insulating snow cover. Growth of FYI north of Svalbard is mainly controlled by the timing of growth onset relative to snow precipitation events and cold spells. These usually short-lived conditions are largely determined by the frequency of storms entering the Arctic from the Atlantic Ocean. In our case, a later freeze onset was favorable for FYI growth due to less snow accumulation in early autumn. This limited snow-ice formation but promoted bottom thermodynamic growth. We surmise these findings are related to a regional phenomenon in the Atlantic sector of the Arctic, with frequent storm events which bring increasing amounts of precipitation in autumn and winter, and also affect the duration of cold temperatures required for ice growth in winter. We discuss the implications for the importance of snow-ice in the future Arctic, formerly believed to be non-existent in the central Arctic due to thick perennial ice.

  4. Toward Surface Mass Balance Modeling over Antarctic Peninsula with Improved Snow/Ice Physics within WRF

    NASA Astrophysics Data System (ADS)

    Villamil-Otero, G.; Zhang, J.; Yao, Y.

    2017-12-01

    The Antarctic Peninsula (AP) has long been the focus of climate change studies due to its rapid environmental changes such as significantly increased glacier melt and retreat, and ice-shelf break-up. Progress has been continuously made in the use of regional modeling to simulate surface mass changes over ice sheets. Most efforts, however, focus on the ice sheets of Greenland with considerable fewer studies in Antarctica. In this study the Weather Research and Forecasting (WRF) model, which has been applied to the Antarctic region for weather modeling, is adopted to capture the past and future surface mass balance changes over AP. In order to enhance the capabilities of WRF model simulating surface mass balance over the ice surface, we implement various ice and snow processes within the WRF and develop a new WRF suite (WRF-Ice). The WRF-Ice includes a thermodynamic ice sheet model that improves the representation of internal melting and refreezing processes and the thermodynamic effects over ice sheet. WRF-Ice also couples a thermodynamic sea ice model to improve the simulation of surface temperature and fluxes over sea ice. Lastly, complex snow processes are also taken into consideration including the implementation of a snowdrift model that takes into account the redistribution of blowing snow as well as the thermodynamic impact of drifting snow sublimation on the lower atmospheric boundary layer. Intensive testing of these ice and snow processes are performed to assess the capability of WRF-Ice in simulating the surface mass balance changes over AP.

  5. Insight into glacier climate interaction: reconstruction of the mass balance field using ice extent data

    NASA Astrophysics Data System (ADS)

    Visnjevic, Vjeran; Herman, Frédéric; Licul, Aleksandar

    2016-04-01

    With the end of the Last Glacial Maximum (LGM), about 20 000 years ago, ended the most recent long-lasting cold phase in Earth's history. We recently developed a model that describes large-scale erosion and its response to climate and dynamical changes with the application to the Alps for the LGM period. Here we will present an inverse approach we have recently developed to infer the LGM mass balance from known ice extent data, focusing on a glacier or ice cap. The ice flow model is developed using the shallow ice approximation and the developed codes are accelerated using GPUs capabilities. The mass balance field is the constrained variable defined by the balance rate β and the equilibrium line altitude (ELA), where c is the cutoff value: b = max(βṡ(S(z) - ELA), c) We show that such a mass balance can be constrained from the observed past ice extent and ice thickness. We are also investigating several different geostatistical methods to constrain spatially variable mass balance, and derive uncertainties on each of the mass balance parameters.

  6. Present-day Antarctic ice mass changes and crustal motion

    NASA Technical Reports Server (NTRS)

    James, Thomas S.; Ivins, Erik R.

    1995-01-01

    The peak vertical velocities predicted by three realistic, but contrasting, present-day scenarios of Antarctic ice sheet mass balance are found to be of the order of several mm/a. One scenario predicts local uplift rates in excess of 5 mm/a. These rates are small compared to the peak Antarctic vertical velocities of the ICE-3G glacial rebound model, which are in excess of 20 mm/a. If the Holocene Antarctic deglaciation history protrayed in ICE-3G is realistic, and if regional upper mantle viscosity is not an order of magnitude below 10(exp 21) Pa(dot)s, then a vast geographical region in West Antarctica is uplifting at a rate that could be detected by a future Global Positioning System (GPS) campaign. While present-day scenarios predict small vertical crustal velocities, their overall continent-ocean mass exchange is large enough to account for a substantial portion of the observed secular polar motion (omega m(arrow dot)) and time-varying zonal gravity field.

  7. Present-day Antarctic Ice Mass Changes and Crustal Motion

    NASA Technical Reports Server (NTRS)

    James, Thomas S.; Ivins, Erik R.

    1995-01-01

    The peak vertical velocities predicted by three realistic, but contrasting, present-day scenarios of Antarctic ice sheet mass balance are found to be of the order of several mm/a. One scenario predicts local uplift rates in excess of 5 mm/a. These rates are small compared to the peak Antarctic vertical velocities of the ICE-3G glacial rebound model, which are in excess of 20 mm/a. If the Holocene Antarctic deglaciation history portrayed in ICE-3G is realistic, and if regional upper mantle viscosity is not an order of magnitude below 10(exp 21) pa s, then a vast geographical region in West Antarctica is uplifting at a rate that could be detected by a future Global Positioning System (GPS) campaign. While present-day scenarios predict small vertical crustal velocities, their overall continent-ocean mass exchange is large enough to account for a substantial portion of the observed secular polar motion ((Omega)m(bar)) and time-varying zonal gravity field J(sub 1).

  8. Non-basal dislocations should be accounted for in simulating ice mass flow

    NASA Astrophysics Data System (ADS)

    Chauve, T.; Montagnat, M.; Piazolo, S.; Journaux, B.; Wheeler, J.; Barou, F.; Mainprice, D.; Tommasi, A.

    2017-09-01

    Prediction of ice mass flow and associated dynamics is pivotal at a time of climate change. Ice flow is dominantly accommodated by the motion of crystal defects - the dislocations. In the specific case of ice, their observation is not always accessible by means of the classical tools such as X-ray diffraction or transmission electron microscopy (TEM). Part of the dislocation population, the geometrically necessary dislocations (GNDs) can nevertheless be constrained using crystal orientation measurements via electron backscattering diffraction (EBSD) associated with appropriate analyses based on the Nye (1950) approach. The present study uses the Weighted Burgers Vectors, a reduced formulation of the Nye theory that enables the characterization of GNDs. Applied to ice, this method documents, for the first time, the presence of dislocations with non-basal [ c ] or < c + a > Burgers vectors. These [ c ] or < c + a > dislocations represent up to 35% of the GNDs observed in laboratory-deformed ice samples. Our findings offer a more complex and comprehensive picture of the key plasticity processes responsible for polycrystalline ice creep and provide better constraints on the constitutive mechanical laws implemented in ice sheet flow models used to predict the response of Earth ice masses to climate change.

  9. cm-scale variations of crystal orientation fabric in cold Alpine ice core from Colle Gnifetti

    NASA Astrophysics Data System (ADS)

    Kerch, Johanna; Weikusat, Ilka; Eisen, Olaf; Wagenbach, Dietmar; Erhardt, Tobias

    2015-04-01

    Analysis of the microstructural parameters of ice has been an important part of ice core analyses so far mainly in polar cores in order to obtain information about physical processes (e.g. deformation, recrystallisation) on the micro- and macro-scale within an ice body. More recently the influence of impurities and climatic conditions during snow accumulation on these processes has come into focus. A deeper understanding of how palaeoclimate proxies interact with physical properties of the ice matrix bears relevance for palaeoclimatic interpretations, improved geophysical measurement techniques and the furthering of ice dynamical modeling. Variations in microstructural parameters e.g. crystal orientation fabric or grain size can be observed on a scale of hundreds and tens of metres but also on a centimetre scale. The underlying processes are not necessarily the same on all scales. Especially for the short-scale variations many questions remain unanswered. We present results from a study that aims to investigate following hypotheses: 1. Variations in grain size and fabric, i.e. strong changes of the orientation of ice crystals with respect to the vertical, occur on a centimetre scale and can be observed in all depths of an ice core. 2. Palaeoclimate proxies like dust and impurities have an impact on the microstructural processes and thus are inducing the observed short-scale variations in grain size and fabric. 3. The interaction of proxies with the ice matrix leads to depth intervals that show correlating behaviour as well as ranges with anticorrelation between microstructural parameters and palaeoclimatic proxies. The respective processes need to be identified. Fabric Analyser measurements were conducted on more than 80 samples (total of 8 m) from different depth ranges of a cold Alpine ice core (72 m length) drilled in 2013 at Colle Gnifetti, Switzerland/Italy. Results were obtained by automatic image processing, providing estimates for grain size distributions

  10. Land motion due to 20th century mass balance of the Greenland Ice Sheet

    NASA Astrophysics Data System (ADS)

    Kjeldsen, K. K.; Khan, S. A.

    2017-12-01

    Quantifying the contribution from ice sheets and glaciers to past sea level change is of great value for understanding sea level projections into the 21st century. However, quantifying and understanding past changes are equally important, in particular understanding the impact in the near-field where the signal is highest. We assess the impact of 20th century mass balance of the Greenland Ice Sheet on land motion using results from Kjeldsen et al, 2015. These results suggest that the ice sheet on average lost a minimum of 75 Gt/yr, but also show that the mass balance was highly spatial- and temporal variable, and moreover that on a centennial time scale changes were driven by a decreasing surface mass balance. Based on preliminary results we discuss land motion during the 20th century due to mass balance changes and the driving components surface mass balance and ice dynamics.

  11. Infrared Observations of Hot Gas and Cold Ice Toward the Low Mass Protostar Elias 29

    NASA Technical Reports Server (NTRS)

    Boogert, A. C. A.; Tielens, A. G. G. M.; Ceccarelli, C.; Boonman, A. M. S.; vanDishoeck, E. F.; Keane, J. V.; Whittet, D. C. B.; deGraauw, T.

    2000-01-01

    We have obtained the full 1-200 micrometer spectrum of the low luminosity (36 solar luminosity Class I protostar Elias 29 in the rho Ophiuchi molecular cloud. It provides a unique opportunity to study the origin and evolution of interstellar ice and the interrelationship of interstellar ice and hot core gases around low mass protostars. We see abundant hot CO and H2O gas, as well as the absorption bands of CO, CO2, H2O and "6.85 micrometer" ices. We compare the abundances and physical conditions of the gas and ices toward Elias 29 with the conditions around several well studied luminous, high mass protostars. The high gas temperature and gas/solid ratios resemble those of relatively evolved high mass objects (e.g. GL 2591). However, none of the ice band profiles shows evidence for significant thermal processing, and in this respect Elias 29 resembles the least evolved luminous protostars, such as NGC 7538 : IRS9. Thus we conclude that the heating of the envelope of the low mass object Elias 29 is qualitatively different from that of high mass protostars. This is possibly related to a different density gradient of the envelope or shielding of the ices in a circumstellar disk. This result is important for our understanding of the evolution of interstellar ices, and their relation to cometary ices.

  12. Glacier ice mass fluctuations and fault instability in tectonically active Southern Alaska

    NASA Astrophysics Data System (ADS)

    Sauber, Jeanne M.; Molnia, Bruce F.

    2004-07-01

    Across the plate boundary zone in south central Alaska, tectonic strain rates are high in a region that includes large glaciers undergoing wastage (glacier retreat and thinning) and surges. For the coastal region between the Bering and Malaspina Glaciers, the average ice mass thickness changes between 1995 and 2000 range from 1 to 5 m/year. These ice changes caused solid Earth displacements in our study region with predicted values of -10 to 50 mm in the vertical and predicted horizontal displacements of 0-10 mm at variable orientations. Relative to stable North America, observed horizontal rates of tectonic deformation range from 10 to 40 mm/year to the north-northwest and the predicted tectonic uplift rates range from approximately 0 mm/year near the Gulf of Alaska coast to 12 mm/year further inland. The ice mass changes between 1995 and 2000 resulted in discernible changes in the Global Positioning System (GPS) measured station positions of one site (ISLE) located adjacent to the Bagley Ice Valley and at one site, DON, located south of the Bering Glacier terminus. In addition to modifying the surface displacements rates, we evaluated the influence ice changes during the Bering glacier surge cycle had on the background seismic rate. We found an increase in the number of earthquakes ( ML≥2.5) and seismic rate associated with ice thinning and a decrease in the number of earthquakes and seismic rate associated with ice thickening. These results support the hypothesis that ice mass changes can modulate the background seismic rate. During the last century, wastage of the coastal glaciers in the Icy Bay and Malaspina region indicates thinning of hundreds of meters and in areas of major retreat, maximum losses of ice thickness approaching 1 km. Between the 1899 Yakataga and Yakutat earthquakes ( Mw=8.1, 8.1) and prior to the 1979 St. Elias earthquake ( Ms=7.2), the plate interface below Icy Bay was locked and tectonic strain accumulated. We used estimated ice mass

  13. Glacier ice mass fluctuations and fault instability in tectonically active Southern Alaska

    USGS Publications Warehouse

    Sauber, J.M.; Molnia, B.F.

    2004-01-01

    Across the plate boundary zone in south central Alaska, tectonic strain rates are high in a region that includes large glaciers undergoing wastage (glacier retreat and thinning) and surges. For the coastal region between the Bering and Malaspina Glaciers, the average ice mass thickness changes between 1995 and 2000 range from 1 to 5 m/year. These ice changes caused solid Earth displacements in our study region with predicted values of -10 to 50 mm in the vertical and predicted horizontal displacements of 0-10 mm at variable orientations. Relative to stable North America, observed horizontal rates of tectonic deformation range from 10 to 40 mm/year to the north-northwest and the predicted tectonic uplift rates range from approximately 0 mm/year near the Gulf of Alaska coast to 12 mm/year further inland. The ice mass changes between 1995 and 2000 resulted in discernible changes in the Global Positioning System (GPS) measured station positions of one site (ISLE) located adjacent to the Bagley Ice Valley and at one site, DON, located south of the Bering Glacier terminus. In addition to modifying the surface displacements rates, we evaluated the influence ice changes during the Bering glacier surge cycle had on the background seismic rate. We found an increase in the number of earthquakes (ML???2.5) and seismic rate associated with ice thinning and a decrease in the number of earthquakes and seismic rate associated with ice thickening. These results support the hypothesis that ice mass changes can modulate the background seismic rate. During the last century, wastage of the coastal glaciers in the Icy Bay and Malaspina region indicates thinning of hundreds of meters and in areas of major retreat, maximum losses of ice thickness approaching 1 km. Between the 1899 Yakataga and Yakutat earthquakes (Mw=8.1, 8.1) and prior to the 1979 St. Elias earthquake (M s=7.2), the plate interface below Icy Bay was locked and tectonic strain accumulated. We used estimated ice mass

  14. Surface water mass composition changes captured by cores of Arctic land-fast sea ice

    NASA Astrophysics Data System (ADS)

    Smith, I. J.; Eicken, H.; Mahoney, A. R.; Van Hale, R.; Gough, A. J.; Fukamachi, Y.; Jones, J.

    2016-04-01

    In the Arctic, land-fast sea ice growth can be influenced by fresher water from rivers and residual summer melt. This paper examines a method to reconstruct changes in water masses using oxygen isotope measurements of sea ice cores. To determine changes in sea water isotope composition over the course of the ice growth period, the output of a sea ice thermodynamic model (driven with reanalysis data, observations of snow depth, and freeze-up dates) is used along with sea ice oxygen isotope measurements and an isotopic fractionation model. Direct measurements of sea ice growth rates are used to validate the output of the sea ice growth model. It is shown that for sea ice formed during the 2011/2012 ice growth season at Barrow, Alaska, large changes in isotopic composition of the ocean waters were captured by the sea ice isotopic composition. Salinity anomalies in the ocean were also tracked by moored instruments. These data indicate episodic advection of meteoric water, having both lower salinity and lower oxygen isotopic composition, during the winter sea ice growth season. Such advection of meteoric water during winter is surprising, as no surface meltwater and no local river discharge should be occurring at this time of year in that area. How accurately changes in water masses as indicated by oxygen isotope composition can be reconstructed using oxygen isotope analysis of sea ice cores is addressed, along with methods/strategies that could be used to further optimize the results. The method described will be useful for winter detection of meteoric water presence in Arctic fast ice regions, which is important for climate studies in a rapidly changing Arctic. Land-fast sea ice effective fractionation coefficients were derived, with a range of +1.82‰ to +2.52‰. Those derived effective fractionation coefficients will be useful for future water mass component proportion calculations. In particular, the equations given can be used to inform choices made when

  15. Insights into Spatial Sensitivities of Ice Mass Response to Environmental Change from the SeaRISE Ice Sheet Modeling Project I: Antarctica

    NASA Technical Reports Server (NTRS)

    Nowicki, Sophie; Bindschadler, Robert A.; Abe-Ouchi, Ayako; Aschwanden, Andy; Bueler, Ed; Choi, Hyengu; Fastook, Jim; Granzow, Glen; Greve, Ralf; Gutowski, Gail; hide

    2013-01-01

    Atmospheric, oceanic, and subglacial forcing scenarios from the Sea-level Response to Ice Sheet Evolution (SeaRISE) project are applied to six three-dimensional thermomechanical ice-sheet models to assess Antarctic ice 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 ice); and (iii) mass loss with enhanced ice shelf melting (with changes in West Antarctica dominating the signal due to its marine setting and extensive ice shelves; cf. minimal impact in the Terre Adelie, George V, Oates, and Victoria Land region of East Antarctica). Ice 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 ice dynamics highlight the need for improved understanding of basal conditions, grounding-zone processes, ocean-ice interactions, and the numerical representation of all three.

  16. Breaking Off of Large Ice Masses From Hanging Glaciers

    NASA Astrophysics Data System (ADS)

    Pralong, A.; Funk, M.

    In order to reduce damage to settlements or other installations (roads, railway, etc) and avoid loss of life, a forecast of the final failure time of ice masses is required. At present, the most promising approach for such a prediction is based on the regularity by which certain large ice masses accelerate prior to the instant of collapse. The lim- itation of this forecast lies in short-term irregularities and in the difficulties to obtain sufficiently accurate data. A better physical understanding of the breaking off process is required, in order to improve the forecasting method. Previous analyze has shown that a stepwise crack extension coupling with a viscous flow leads to the observed acceleration function. We propose another approach by considering a local damage evolution law (gener- alized Kachanow's law) coupled with Glen's flow law to simulate the spatial evolu- tion of damage in polycristalline ice, using a finite element computational model. The present study focuses on the transition from a diffuse to a localised damage reparti- tion occurring during the damage evolution. The influence of inhomogeneous initial conditions (inhomogeneity of the mechanical properties of ice, damage inhomogene- ity) and inhomogeneous boundary conditions on the damage repartition are especially investigated.

  17. Mass budget of the glaciers and ice caps of the Queen Elizabeth Islands, Canada, from 1991 to 2015

    NASA Astrophysics Data System (ADS)

    Millan, Romain; Mouginot, Jeremie; Rignot, Eric

    2017-02-01

    Recent studies indicate that the glaciers and ice caps in Queen Elizabeth Islands (QEI), Canada have experienced an increase in ice mass loss during the last two decades, but the contribution of ice dynamics to this loss is not well known. We present a comprehensive mapping of ice velocity using a suite of satellite data from year 1991 to 2015, combined with ice thickness data from NASA Operation IceBridge, to calculate ice discharge. We find that ice discharge increased significantly after 2011 in Prince of Wales Icefield, maintained or decreased in other sectors, whereas glacier surges have little impact on long-term trends in ice discharge. During 1991-2005, the QEI mass loss averaged 6.3 ± 1.1 Gt yr-1, 52% from ice discharge and the rest from surface mass balance (SMB). During 2005-2014, the mass loss from ice discharge averaged 3.5 ± 0.2 Gt yr-1 (10%) versus 29.6 ± 3.0 Gt yr-1 (90%) from SMB. SMB processes therefore dominate the QEI mass balance, with ice dynamics playing a significant role only in a few basins.

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

    NASA Astrophysics Data System (ADS)

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

    2013-12-01

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

  19. A 25-year Record of Antarctic Ice Sheet Elevation and Mass Change

    NASA Astrophysics Data System (ADS)

    Shepherd, A.; Muir, A. S.; Sundal, A.; McMillan, M.; Briggs, K.; Hogg, A.; Engdahl, M.; Gilbert, L.

    2017-12-01

    Since 1992, the European Remote-Sensing (ERS-1 and ERS-2), ENVISAT, and CryoSat-2 satellite radar altimeters have measured the Antarctic ice sheet surface elevation, repeatedly, at approximately monthly intervals. These data constitute the longest continuous record of ice sheet wide change. In this paper, we use these observations to determine changes in the elevation, volume and mass of the East Antarctic and West Antarctic ice sheets, and of parts of the Antarctic Peninsula ice sheet, over a 25-year period. The root mean square difference between elevation rates computed from our survey and 257,296 estimates determined from airborne laser measurements is 54 cm/yr. The longevity of the satellite altimeter data record allows to identify and chart the evolution of changes associated with meteorology and ice flow, and we estimate that 3.6 % of the continental ice sheet, and 21.7 % of West Antarctica, is in a state of dynamical imbalance. Based on this partitioning, we estimate the mass balance of the East and West Antarctic ice sheet drainage basins and the root mean square difference between these and independent estimates derived from satellite gravimetry is less than 5 Gt yr-1.

  20. Temporal and spatial variabilities of Antarctic ice mass changes inferred by GRACE in a Bayesian framework

    NASA Astrophysics Data System (ADS)

    Wang, L.; Davis, J. L.; Tamisiea, M. E.

    2017-12-01

    The Antarctic ice sheet (AIS) holds about 60% of all fresh water on the Earth, an amount equivalent to about 58 m of sea-level rise. Observation of AIS mass change is thus essential in determining and predicting its contribution to sea level. While the ice mass loss estimates for West Antarctica (WA) and the Antarctic Peninsula (AP) are in good agreement, what the mass balance over East Antarctica (EA) is, and whether or not it compensates for the mass loss is under debate. Besides the different error sources and sensitivities of different measurement types, complex spatial and temporal variabilities would be another factor complicating the accurate estimation of the AIS mass balance. Therefore, a model that allows for variabilities in both melting rate and seasonal signals would seem appropriate in the estimation of present-day AIS melting. We present a stochastic filter technique, which enables the Bayesian separation of the systematic stripe noise and mass signal in decade-length GRACE monthly gravity series, and allows the estimation of time-variable seasonal and inter-annual components in the signals. One of the primary advantages of this Bayesian method is that it yields statistically rigorous uncertainty estimates reflecting the inherent spatial resolution of the data. By applying the stochastic filter to the decade-long GRACE observations, we present the temporal variabilities of the AIS mass balance at basin scale, particularly over East Antarctica, and decipher the EA mass variations in the past decade, and their role in affecting overall AIS mass balance and sea level.

  1. Improved estimate of accelerated Antarctica ice mass loses from GRACE, Altimetry and surface mass balance from regional climate model output

    NASA Astrophysics Data System (ADS)

    Velicogna, I.; Sutterley, T. C.; A, G.; van den Broeke, M. R.; Ivins, E. R.

    2016-12-01

    We use Gravity Recovery and Climate Experiment (GRACE) monthly gravity fields to determine the regional acceleration in ice mass loss in Antarctica for 2002-2016. We find that the total mass loss is controlled by only a few regions. In Antarctica, the Amundsen Sea (AS) sector and the Antarctic Peninsula account for 65% and 18%, respectively, of the total loss (186 ± 10 Gt/yr) mainly from ice dynamics. The AS sector contributes most of the acceleration in loss (9 ± 1 Gt/yr2 ), and Queen Maud Land, East Antarctica, is the only sector with a significant mass gain due to a local increase in SMB (57 ± 5 Gt/yr). We compare GRACE regional mass balance estimates with independent estimates from ICESat-1 and Operation IceBridge laser altimetry, CryoSat-2 radar altimetry, and surface mass balance outputs from RACMO2.3. In the Amundsen Sea Embayment of West Antarctica, an area experiencing rapid retreat and mass loss to the sea, we find good agreement between GRACE and altimetry estimates. Comparison of GRACE with these independent techniques in East Antarctic shows that GIA estimates from the new regional ice deglaciation models underestimate the GIA correction in the EAIS interior, which implies larger losses of the Antarctica ice sheet by about 70 Gt/yr. Sectors where we are observing the largest losses are closest to warm circumpolar water, and with polar constriction of the westerlies enhanced by climate warming, we expect these sectors to contribute more and more to sea level as the ice shelves that protect these glaciers will melt faster in contact with more heat from the surrounding oc

  2. Calibrating a surface mass-balance model for Austfonna ice cap, Svalbard

    NASA Astrophysics Data System (ADS)

    Schuler, Thomas Vikhamar; Loe, Even; Taurisano, Andrea; Eiken, Trond; Hagen, Jon Ove; Kohler, Jack

    2007-10-01

    Austfonna (8120 km2) is by far the largest ice mass in the Svalbard archipelago. There is considerable uncertainty about its current state of balance and its possible response to climate change. Over the 2004/05 period, we collected continuous meteorological data series from the ice cap, performed mass-balance measurements using a network of stakes distributed across the ice cap and mapped the distribution of snow accumulation using ground-penetrating radar along several profile lines. These data are used to drive and test a model of the surface mass balance. The spatial accumulation pattern was derived from the snow depth profiles using regression techniques, and ablation was calculated using a temperature-index approach. Model parameters were calibrated using the available field data. Parameter calibration was complicated by the fact that different parameter combinations yield equally acceptable matches to the stake data while the resulting calculated net mass balance differs considerably. Testing model results against multiple criteria is an efficient method to cope with non-uniqueness. In doing so, a range of different data and observations was compared to several different aspects of the model results. We find a systematic underestimation of net balance for parameter combinations that predict observed ice ablation, which suggests that refreezing processes play an important role. To represent these effects in the model, a simple PMAX approach was included in its formulation. Used as a diagnostic tool, the model suggests that the surface mass balance for the period 29 April 2004 to 23 April 2005 was negative (-318 mm w.e.).

  3. Surface Mass Balance of the Greenland Ice Sheet Derived from Paleoclimate Reanalysis

    NASA Astrophysics Data System (ADS)

    Badgeley, J.; Steig, E. J.; Hakim, G. J.; Anderson, J.; Tardif, R.

    2017-12-01

    Modeling past ice-sheet behavior requires independent knowledge of past surface mass balance. Though models provide useful insight into ice-sheet response to climate forcing, if past climate is unknown, then ascertaining the rate and extent of past ice-sheet change is limited to geological and geophysical constraints. We use a novel data-assimilation framework developed under the Last Millennium Reanalysis Project (Hakim et al., 2016) to reconstruct past climate over ice sheets with the intent of creating an independent surface mass balance record for paleo ice-sheet modeling. Paleoclimate data assimilation combines the physics of climate models and the time series evidence of proxy records in an offline, ensemble-based approach. This framework allows for the assimilation of numerous proxy records and archive types while maintaining spatial consistency with known climate dynamics and physics captured by the models. In our reconstruction, we use the Community Climate System Model version 4, CMIP5 last millennium simulation (Taylor et al., 2012; Landrum et al., 2013) and a nearly complete database of ice core oxygen isotope records to reconstruct Holocene surface temperature and precipitation over the Greenland Ice Sheet on a decadal timescale. By applying a seasonality to this reconstruction (from the TraCE-21ka simulation; Liu et al., 2009), our reanalysis can be used in seasonally-based surface mass balance models. Here we discuss the methods behind our reanalysis and the performance of our reconstruction through prediction of unassimilated proxy records and comparison to paleoclimate reconstructions and reanalysis products.

  4. Snow contribution to first-year and second-year Arctic sea ice mass balance north of Svalbard

    NASA Astrophysics Data System (ADS)

    Granskog, Mats A.; Rösel, Anja; Dodd, Paul A.; Divine, Dmitry; Gerland, Sebastian; Martma, Tõnu; Leng, Melanie J.

    2017-03-01

    The salinity and water oxygen isotope composition (δ18O) of 29 first-year (FYI) and second-year (SYI) Arctic sea ice cores (total length 32.0 m) from the drifting ice pack north of Svalbard were examined to quantify the contribution of snow to sea ice mass. Five cores (total length 6.4 m) were analyzed for their structural composition, showing variable contribution of 10-30% by granular ice. In these cores, snow had been entrained in 6-28% of the total ice thickness. We found evidence of snow contribution in about three quarters of the sea ice cores, when surface granular layers had very low δ18O values. Snow contributed 7.5-9.7% to sea ice mass balance on average (including also cores with no snow) based on δ18O mass balance calculations. In SYI cores, snow fraction by mass (12.7-16.3%) was much higher than in FYI cores (3.3-4.4%), while the bulk salinity of FYI (4.9) was distinctively higher than for SYI (2.7). We conclude that oxygen isotopes and salinity profiles can give information on the age of the ice and enables distinction between FYI and SYI (or older) ice in the area north of Svalbard.Plain Language SummaryThe role of snow in sea <span class="hlt">ice</span> <span class="hlt">mass</span> balance is largely two fold. Firstly, it can slow down growth and melt due to its high insulation and high reflectance, but secondly it can actually contribute to sea <span class="hlt">ice</span> growth if the snow cover is turned into <span class="hlt">ice</span>. The latter is largely a consequence of high <span class="hlt">mass</span> of snow on top of sea <span class="hlt">ice</span> that can push the surface of the sea <span class="hlt">ice</span> below sea level and seawater can flood the <span class="hlt">ice</span>. This mixture of seawater and snow can then freeze and add to the growth of sea <span class="hlt">ice</span>. This is very typical in the Antarctic but not believed to be so important in the Arctic. In this work we show, for the first time, that snow actually contributes significantly to the growth of Arctic sea <span class="hlt">ice</span>. This is likely a consequence of the thinning of the Arctic sea <span class="hlt">ice</span>. The conditions in the Arctic, with</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C44B..01B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C44B..01B"><span>Improving Estimates of Greenland <span class="hlt">Ice</span> Sheet Surface <span class="hlt">Mass</span> Balance with Satellite Observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Briggs, K.</p> <p>2016-12-01</p> <p><span class="hlt">Mass</span> losses from the Greenland <span class="hlt">Ice</span> Sheet have been accelerating over recent years (e.g. McMillan et al., 2016; Velicogna et al., 2014). This acceleration has predominantly been linked to increasing rates of negative surface <span class="hlt">mass</span> balance, and in particular, increasing <span class="hlt">ice</span> surface melt rates (e.g. McMillan et al., 2016; Velicogna et al., 2014). At the <span class="hlt">ice</span> sheet scale, SMB is assessed using SMB model outputs, which in addition to enabling understanding of the origin of <span class="hlt">mass</span> balance signals, are required as ancillary data in <span class="hlt">mass</span> balance assessments from altimetry and the <span class="hlt">mass</span> budget method. Due to the importance of SMB for <span class="hlt">mass</span> balance over Greenland and the sensitivity of <span class="hlt">mass</span> balance assessments to SMB model outputs, high accuracy of these models is crucial. A critical limiting factor in SMB modeling is however, a lack of in-situ data that is required for model constraint and evaluation. Such data is limited in time and space due to inherent logistical and financial constraints. Remote sensing datasets, being spatially extensive and relatively densely sampled in both space and time, do not suffer such constraints. Here, we show satellite observations of Greenland SMB. McMillan, M., Leeson, A., Shepherd, A., Briggs, K., Armitage, T. W.K., Hogg, A., Kuipers Munneke, P., van den Broeke, M., Noël, B., van de Berg, W., Ligtenberg, S., Horwath, M., Groh, A. , Muir, A. and Gilbert, L. 2016. A high resolution record of Greenland <span class="hlt">Mass</span> Balance. Geophysical Research Letters. 43, doi:10.1002/2016GL069666 Velicogna, I., Sutterley, T. C. and van den Broeke, M. R. 2014. Regional acceleration in <span class="hlt">ice</span> <span class="hlt">mass</span> loss from Greenland and Antarctica using GRACE time-variable gravity data. Geophysical Research Letters. 41, 8130-8137, doi:10.1002/2014GL061052</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29546238','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29546238"><span><span class="hlt">Variations</span> in the amount of water <span class="hlt">ice</span> on Ceres' surface suggest a seasonal water cycle.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Raponi, Andrea; De Sanctis, Maria Cristina; Frigeri, Alessandro; Ammannito, Eleonora; Ciarniello, Mauro; Formisano, Michelangelo; Combe, Jean-Philippe; Magni, Gianfranco; Tosi, Federico; Carrozzo, Filippo Giacomo; Fonte, Sergio; Giardino, Marco; Joy, Steven P; Polanskey, Carol A; Rayman, Marc D; Capaccioni, Fabrizio; Capria, Maria Teresa; Longobardo, Andrea; Palomba, Ernesto; Zambon, Francesca; Raymond, Carol A; Russell, Christopher T</p> <p>2018-03-01</p> <p>The dwarf planet Ceres is known to host a considerable amount of water in its interior, and areas of water <span class="hlt">ice</span> were detected by the Dawn spacecraft on its surface. Moreover, sporadic water and hydroxyl emissions have been observed from space telescopes. We report the detection of water <span class="hlt">ice</span> in a mid-latitude crater and its unexpected <span class="hlt">variation</span> with time. The Dawn spectrometer data show a change of water <span class="hlt">ice</span> signatures over a period of 6 months, which is well modeled as ~2-km 2 increase of water <span class="hlt">ice</span>. The observed increase, coupled with Ceres' orbital parameters, points to an ongoing process that seems correlated with solar flux. The reported <span class="hlt">variation</span> on Ceres' surface indicates that this body is chemically and physically active at the present time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005JGRA..110.8103X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005JGRA..110.8103X"><span>An <span class="hlt">ice</span>-cream cone model for coronal <span class="hlt">mass</span> ejections</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xue, X. H.; Wang, C. B.; Dou, X. K.</p> <p>2005-08-01</p> <p>In this study, we use an <span class="hlt">ice</span>-cream cone model to analyze the geometrical and kinematical properties of the coronal <span class="hlt">mass</span> ejections (CMEs). Assuming that in the early phase CMEs propagate with near-constant speed and angular width, some useful properties of CMEs, namely the radial speed (v), the angular width (α), and the location at the heliosphere, can be obtained considering the geometrical shapes of a CME as an <span class="hlt">ice</span>-cream cone. This model is improved by (1) using an <span class="hlt">ice</span>-cream cone to show the near real configuration of a CME, (2) determining the radial speed via fitting the projected speeds calculated from the height-time relation in different azimuthal angles, (3) not only applying to halo CMEs but also applying to nonhalo CMEs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29540750','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29540750"><span>Recent high-resolution Antarctic <span class="hlt">ice</span> velocity maps reveal increased <span class="hlt">mass</span> loss in Wilkes Land, East Antarctica.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Shen, Qiang; Wang, Hansheng; Shum, C K; Jiang, Liming; Hsu, Hou Tse; Dong, Jinglong</p> <p>2018-03-14</p> <p>We constructed Antarctic <span class="hlt">ice</span> velocity maps from Landsat 8 images for the years 2014 and 2015 at a high spatial resolution (100 m). These maps were assembled from 10,690 scenes of displacement vectors inferred from more than 10,000 optical images acquired from December 2013 through March 2016. We estimated the <span class="hlt">mass</span> discharge of the Antarctic <span class="hlt">ice</span> sheet in 2008, 2014, and 2015 using the Landsat <span class="hlt">ice</span> velocity maps, interferometric synthetic aperture radar (InSAR)-derived <span class="hlt">ice</span> velocity maps (~2008) available from prior studies, and <span class="hlt">ice</span> thickness data. An increased <span class="hlt">mass</span> discharge (53 ± 14 Gt yr -1 ) was found in the East Indian Ocean sector since 2008 due to unexpected widespread glacial acceleration in Wilkes Land, East Antarctica, while the other five oceanic sectors did not exhibit significant changes. However, present-day increased <span class="hlt">mass</span> loss was found by previous studies predominantly in west Antarctica and the Antarctic Peninsula. The newly discovered increased <span class="hlt">mass</span> loss in Wilkes Land suggests that the ocean heat flux may already be influencing <span class="hlt">ice</span> dynamics in the marine-based sector of the East Antarctic <span class="hlt">ice</span> sheet (EAIS). The marine-based sector could be adversely impacted by ongoing warming in the Southern Ocean, and this process may be conducive to destabilization.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1810633W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1810633W"><span><span class="hlt">Ice</span> <span class="hlt">Mass</span> Changes in the Russian High Arctic from Repeat High Resolution Topography.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Willis, Michael; Zheng, Whyjay; Pritchard, Matthew; Melkonian, Andrew; Morin, Paul; Porter, Claire; Howat, Ian; Noh, Myoung-Jong; Jeong, Seongsu</p> <p>2016-04-01</p> <p>We use a combination of ASTER and cartographically derived Digital Elevation Models (DEMs) supplemented with WorldView DEMs, the ArcticDEM and ICESat lidar returns to produce a time-series of <span class="hlt">ice</span> changes occurring in the Russian High Arctic between the mid-20th century and the present. Glaciers on the western, Barents Sea coast of Novaya Zemlya are in a state of general retreat and thinning, while those on the eastern, Kara Sea coast are retreating at a slower rate. Franz Josef Land has a complicated pattern of thinning and thickening, although almost all the thinning is associated with rapid outlet glaciers feeding <span class="hlt">ice</span> shelves. Severnaya Zemlya is also thinning in a complicated manner. A very rapid surging glacier is transferring <span class="hlt">mass</span> into the ocean from the western periphery of the Vavilov <span class="hlt">Ice</span> Cap on October Revolution Island, while glaciers feeding the former Matusevich <span class="hlt">Ice</span> Shelf continue to thin at rates that are faster than those observed during the operational period of ICESat, between 2003 and 2009. Passive microwave studies indicate the total number of melt days is increasing in the Russian Arctic, although much of the melt may refreeze within the firn. It is likely that <span class="hlt">ice</span> dynamic changes will drive <span class="hlt">mass</span> loss for the immediate future. The sub-marine basins beneath several of the <span class="hlt">ice</span> caps in the region suggest the possibility that <span class="hlt">mass</span> loss rates may accelerate in the future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14.6823K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.6823K"><span>Antarctic <span class="hlt">mass</span> balance changes from GRACE</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kallenberg, B.; Tregoning, P.</p> <p>2012-04-01</p> <p>The Antarctic <span class="hlt">ice</span> sheet contains ~30 million km3 of <span class="hlt">ice</span> and constitutes a significant component of the global water balance with enough freshwater to raise global sea level by ~60 m. Altimetry measurements and climate models suggest variable behaviour across the Antarctic <span class="hlt">ice</span> sheet, with thickening occurring in a vast area of East Antarctica and substantial thinning in West Antarctica caused by increased temperature gradients in the surrounding ocean. However, the rate at which the polar <span class="hlt">ice</span> cap is melting is still poorly constrained. To calculate the <span class="hlt">mass</span> loss of an <span class="hlt">ice</span> sheet it is necessary to separate present day <span class="hlt">mass</span> balance changes from glacial isostatic adjustment (GIA), the response of the Earth's crust to <span class="hlt">mass</span> loss, wherefore it is essential to undertake sufficient geological and geomorphological sampling. As there is only a limited possibility for this in Antarctica, all models (i.e. geological, hydrological as well as atmospheric) are very poorly constrained. Therefore, space-geodetic observations play an important role in detecting changes in <span class="hlt">mass</span> and spatial <span class="hlt">variations</span> in the Earth's gravity field. The Gravity Recovery And Climate Experiment (GRACE) observed spatial <span class="hlt">variations</span> in the Earth's gravity field over the past ten years. The satellite detects <span class="hlt">mass</span> <span class="hlt">variations</span> in the Earth system including geophysical, hydrological and atmospheric shifts. GRACE itself is not able to separate the GIA from <span class="hlt">mass</span> balance changes and, due to the insufficient geological and geomorphological database, it is not possible to model the GIA effect accurately for Antarctica. However, the results from GRACE can be compared with other scientific results, coming from other geodetic observations such as satellite altimetry and GPS or by the use of geological observations. In our contribution we compare the GRACE data with recorded precipitation patterns and <span class="hlt">mass</span> anomalies over East Antarctica to separate the observed GRACE signal into its two components: GIA as a result of <span class="hlt">mass</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.5867S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.5867S"><span>Changes in <span class="hlt">ice</span> dynamics along the northern Antarctic Peninsula</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Seehaus, Thorsten; Marinsek, Sebastian; Cook, Alison; Van Wessem, Jan-Melchior; Braun, Matthias</p> <p>2017-04-01</p> <p>The climatic conditions along the Antarctic Peninsula have undergone considerable changes during the last 50 years. A period of pronounced air temperature rise, increasing ocean temperatures as well as changes in the precipitation pattern have been reported by various authors. Consequently, the glacial systems showed changes including widespread retreat, surface lowering as well as <span class="hlt">variations</span> in flow speeds. During the last decades numerous <span class="hlt">ice</span> shelves along the Antarctic Peninsula retreated, started to break-up or disintegrated completely. The loss of the buttressing effect caused tributary glaciers to accelerate with increasing <span class="hlt">ice</span> discharge along the Antarctic Peninsula. Quantification of the <span class="hlt">mass</span> changes is still subject to considerable errors although numbers derived from the different methods are converging. The aim is to study the reaction of glaciers at the northern Antarctic Peninsula to the changing climatic conditions and the readjustments of tributary glaciers to <span class="hlt">ice</span> shelf disintegration, as well as to better quantify the <span class="hlt">ice</span> <span class="hlt">mass</span> loss and its temporal changes. We analysed time series of various satellite sensors (ERS-1/2 SAR, ENVISAT ASAR, RADARSAT-1, ALOS PALSAR, TerraSAR-X/TanDEM-X, ASTER, Landsat) to detect changes in <span class="hlt">ice</span> dynamics of 74 glacier basins along the northern Antarctic Peninsula (<65°). Intensity feature tracking techniques were applied on data stacks from different SAR satellites over the last 20 years to infer temporal trends in glacier surface velocities. In combination with <span class="hlt">ice</span> thickness reconstructions and modeled climatic <span class="hlt">mass</span> balance fields regional imbalances were calculated. <span class="hlt">Variations</span> in <span class="hlt">ice</span> front position were mapped based on optical and SAR satellite data sets. Along the west coast of the northern Antarctic Peninsula an increase in flow speeds by 40% between 1992 and 2014 was observed, whereas glaciers on the east side (north of former Prince-Gustav <span class="hlt">Ice</span> Shelf) showed a strong deceleration. Nearly all former <span class="hlt">ice</span> shelf</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JGRF..119.1995M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JGRF..119.1995M"><span>Field-calibrated model of melt, refreezing, and runoff for polar <span class="hlt">ice</span> caps: Application to Devon <span class="hlt">Ice</span> Cap</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Morris, Richard M.; Mair, Douglas W. F.; Nienow, Peter W.; Bell, Christina; Burgess, David O.; Wright, Andrew P.</p> <p>2014-09-01</p> <p>Understanding the controls on the amount of surface meltwater that refreezes, rather than becoming runoff, over polar <span class="hlt">ice</span> <span class="hlt">masses</span> is necessary for modeling their surface <span class="hlt">mass</span> balance and ultimately for predicting their future contributions to global sea level change. We present a modified version of a physically based model that includes an energy balance routine and explicit calculation of near-surface meltwater refreezing capacity, to simulate the evolution of near-surface density and temperature profiles across Devon <span class="hlt">Ice</span> Cap in Arctic Canada. Uniquely, our model is initiated and calibrated using high spatial resolution measurements of snow and firn densities across almost the entire elevation range of the <span class="hlt">ice</span> cap for the summer of 2004 and subsequently validated with the same type of measurements obtained during the very different meteorological conditions of summer 2006. The model captures the spatial variability across the transect in bulk snowpack properties although it slightly underestimates the flow of meltwater into the firn of previous years. The percentage of meltwater that becomes runoff is similar in both years; however, the spatial pattern of this melt-runoff relationship is different in the 2 years. The model is found to be insensitive to <span class="hlt">variation</span> in the depth of impermeable layers within the firn but is very sensitive to <span class="hlt">variation</span> in air temperature, since the refreezing capacity of firn decreases with increasing temperature. We highlight that the sensitivity of the <span class="hlt">ice</span> cap's surface <span class="hlt">mass</span> balance to air temperature is itself dependent on air temperature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhDT........42L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhDT........42L"><span>Surface Energy and <span class="hlt">Mass</span> Balance Model for Greenland <span class="hlt">Ice</span> Sheet and Future Projections</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, Xiaojian</p> <p></p> <p>The Greenland <span class="hlt">Ice</span> Sheet contains nearly 3 million cubic kilometers of glacial <span class="hlt">ice</span>. If the entire <span class="hlt">ice</span> sheet completely melted, sea level would raise by nearly 7 meters. There is thus considerable interest in monitoring the <span class="hlt">mass</span> balance of the Greenland <span class="hlt">Ice</span> Sheet. Each year, the <span class="hlt">ice</span> sheet gains <span class="hlt">ice</span> from snowfall and loses <span class="hlt">ice</span> through iceberg calving and surface melting. In this thesis, we develop, validate and apply a physics based numerical model to estimate current and future surface <span class="hlt">mass</span> balance of the Greenland <span class="hlt">Ice</span> Sheet. The numerical model consists of a coupled surface energy balance and englacial model that is simple enough that it can be used for long time scale model runs, but unlike previous empirical parameterizations, has a physical basis. The surface energy balance model predicts <span class="hlt">ice</span> sheet surface temperature and melt production. The englacial model predicts the evolution of temperature and meltwater within the <span class="hlt">ice</span> sheet. These two models can be combined with estimates of precipitation (snowfall) to estimate the <span class="hlt">mass</span> balance over the Greenland <span class="hlt">Ice</span> Sheet. We first compare model performance with in-situ observations to demonstrate that the model works well. We next evaluate how predictions are degraded when we statistically downscale global climate data. We find that a simple, nearest neighbor interpolation scheme with a lapse rate correction is able to adequately reproduce melt patterns on the Greenland <span class="hlt">Ice</span> Sheet. These results are comparable to those obtained using empirical Positive Degree Day (PDD) methods. Having validated the model, we next drove the <span class="hlt">ice</span> sheet model using the suite of atmospheric model runs available through the CMIP5 atmospheric model inter-comparison, which in turn built upon the RCP 8.5 (business as usual) scenarios. From this exercise we predict how much surface melt production will increase in the coming century. This results in 4-10 cm sea level equivalent, depending on the CMIP5 models. Finally, we try to bound melt water</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1814608M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1814608M"><span>Present and Future Surface <span class="hlt">Mass</span> Budget of Small Arctic <span class="hlt">Ice</span> Caps in a High Resolution Regional Climate Model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mottram, Ruth; Langen, Peter; Koldtoft, Iben; Midefelt, Linnea; Hesselbjerg Christensen, Jens</p> <p>2016-04-01</p> <p>Globally, small <span class="hlt">ice</span> caps and glaciers make a substantial contribution to sea level rise; this is also true in the Arctic. Around Greenland small <span class="hlt">ice</span> caps are surprisingly important to the total <span class="hlt">mass</span> balance from the island as their marginal coastal position means they receive a large amount of precipitation and also experience high surface melt rates. Since small <span class="hlt">ice</span> caps and glaciers have had a disproportionate number of long-term monitoring and observational schemes in the Arctic, likely due to their relative accessibility, they can also be a valuable source of data. However, in climate models the surface <span class="hlt">mass</span> balance contributions are often not distinguished from the main <span class="hlt">ice</span> sheet and the presence of high relief topography is difficult to capture in coarse resolution climate models. At the same time, the diminutive size of marginal <span class="hlt">ice</span> <span class="hlt">masses</span> in comparison to the <span class="hlt">ice</span> sheet makes modelling their <span class="hlt">ice</span> dynamics difficult. Using observational data from the Devon <span class="hlt">Ice</span> Cap in Arctic Canada and the Renland <span class="hlt">Ice</span> Cap in Eastern Greenland, we assess the success of a very high resolution (~5km) regional climate model, HIRHAM5 in capturing the surface <span class="hlt">mass</span> balance (SMB) of these small <span class="hlt">ice</span> caps. The model is forced with ERA-Interim and we compare observed mean SMB and the interannual variability to assess model performance. The steep gradient in topography around Renland is challenging for climate models and additional statistical corrections are required to fit the calculated surface <span class="hlt">mass</span> balance to the high relief topography. Results from a modelling experiment at Renland <span class="hlt">Ice</span> Cap shows that this technique produces a better fit between modelled and observed surface topography. We apply this statistical relationship to modelled SMB on the Devon <span class="hlt">Ice</span> Cap and use the long time series of observations from this glacier to evaluate the model and the smoothed SMB. Measured SMB values from a number of other small <span class="hlt">ice</span> caps including Mittivakkat and A.P. Olsen <span class="hlt">ice</span> cap are also compared</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120014297','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120014297"><span>An Iterated Global Mascon Solution with Focus on Land <span class="hlt">Ice</span> <span class="hlt">Mass</span> Evolution</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Luthcke, S. B.; Sabaka, T.; Rowlands, D. D.; Lemoine, F. G.; Loomis, B. D.; Boy, J. P.</p> <p>2012-01-01</p> <p>Land <span class="hlt">ice</span> <span class="hlt">mass</span> evolution is determined from a new GRACE global mascon solution. The solution is estimated directly from the reduction of the inter-satellite K-band range rate observations taking into account the full noise covariance, and formally iterating the solution. The new solution increases signal recovery while reducing the GRACE KBRR observation residuals. The mascons are estimated with 10-day and 1-arc-degree equal area sampling, applying anisotropic constraints for enhanced temporal and spatial resolution of the recovered land <span class="hlt">ice</span> signal. The details of the solution are presented including error and resolution analysis. An Ensemble Empirical Mode Decomposition (EEMD) adaptive filter is applied to the mascon solution time series to compute timing of balance seasons and annual <span class="hlt">mass</span> balances. The details and causes of the spatial and temporal variability of the land <span class="hlt">ice</span> regions studied are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMPP23B1393S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMPP23B1393S"><span>High-resolution record of last post-glacial <span class="hlt">variations</span> of sea-<span class="hlt">ice</span> cover and river discharge in the western Laptev Sea (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>Stein, R. H.; Hörner, T.; Fahl, K.</p> <p>2014-12-01</p> <p>Here, we provide a high-resolution reconstruction of sea-<span class="hlt">ice</span> cover <span class="hlt">variations</span> in the western Laptev Sea, a crucial area in terms of sea-<span class="hlt">ice</span> production in the Arctic Ocean and a region characterized by huge river discharge. Furthermore, the shallow Laptev Sea was strongly influenced by the post-glacial sea-level rise that should also be reflected in the sedimentary records. The sea <span class="hlt">Ice</span> Proxy IP25 (Highly-branched mono-isoprenoid produced by sea-<span class="hlt">ice</span> algae; Belt et al., 2007) was measured in two sediment cores from the western Laptev Sea (PS51/154, PS51/159) that offer a high-resolution composite record over the last 18 ka. In addition, sterols are applied as indicator for marine productivity (brassicasterol, dinosterol) and input of terrigenous organic matter by river discharge into the ocean (campesterol, ß-sitosterol). The sea-<span class="hlt">ice</span> cover varies distinctly during the whole time period and shows a general increase in the Late Holocene. A maximum in IP25 concentration can be found during the Younger Dryas. This sharp increase can be observed in the whole circumarctic realm (Chukchi Sea, Bering Sea, Fram Strait and Laptev Sea). Interestingly, there is no correlation between elevated numbers of <span class="hlt">ice</span>-rafted debris (IRD) interpreted as local <span class="hlt">ice</span>-cap expansions (Taldenkova et al. 2010), and sea <span class="hlt">ice</span> cover distribution. The transgression and flooding of the shelf sea that occurred over the last 16 ka in this region, is reflected by decreasing terrigenous (riverine) input, reflected in the strong decrease in sterol (ß-sitosterol and campesterol) concentrations. ReferencesBelt, S.T., <span class="hlt">Mass</span>é, G., Rowland, S.J., Poulin, M., Michel, C., LeBlanc, B., 2007. A novel chemical fossil of palaeo sea <span class="hlt">ice</span>: IP25. Organic Geochemistry 38 (1), 16e27. Taldenkova, E., Bauch, H.A., Gottschalk, J., Nikolaev, S., Rostovtseva, Yu., Pogodina, I., Ya, Ovsepyan, Kandiano, E., 2010. History of <span class="hlt">ice</span>-rafting and water <span class="hlt">mass</span> evolution at the northern Siberian continental margin (Laptev Sea) during Late</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018RvGeo..56..142P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018RvGeo..56..142P"><span>Ocean Tide Influences on the Antarctic and Greenland <span class="hlt">Ice</span> Sheets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Padman, Laurie; Siegfried, Matthew R.; Fricker, Helen A.</p> <p>2018-03-01</p> <p>Ocean tides are the main source of high-frequency variability in the vertical and horizontal motion of <span class="hlt">ice</span> sheets near their marine margins. Floating <span class="hlt">ice</span> shelves, which occupy about three quarters of the perimeter of Antarctica and the termini of four outlet glaciers in northern Greenland, rise and fall in synchrony with the ocean tide. Lateral motion of floating and grounded portions of <span class="hlt">ice</span> sheets near their marine margins can also include a tidal component. These tide-induced signals provide insight into the processes by which the oceans can affect <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balance and dynamics. In this review, we summarize in situ and satellite-based measurements of the tidal response of <span class="hlt">ice</span> shelves and grounded <span class="hlt">ice</span>, and spatial variability of ocean tide heights and currents around the <span class="hlt">ice</span> sheets. We review sensitivity of tide heights and currents as ocean geometry responds to <span class="hlt">variations</span> in sea level, <span class="hlt">ice</span> shelf thickness, and <span class="hlt">ice</span> sheet <span class="hlt">mass</span> and extent. We then describe coupled <span class="hlt">ice</span>-ocean models and analytical glacier models that quantify the effect of ocean tides on lower-frequency <span class="hlt">ice</span> sheet <span class="hlt">mass</span> loss and motion. We suggest new observations and model developments to improve the representation of tides in coupled models that are used to predict future <span class="hlt">ice</span> sheet <span class="hlt">mass</span> loss and the associated contribution to sea level change. The most critical need is for new data to improve maps of bathymetry, <span class="hlt">ice</span> shelf draft, spatial variability of the drag coefficient at the <span class="hlt">ice</span>-ocean interface, and higher-resolution models with improved representation of tidal energy sinks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('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 <span class="hlt">Mass</span> 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 zones that contribute to material contained within 10, 15 and 20 kilometer diameter planetesimals at 1 A.V. as a function of nebular <span class="hlt">mass</span>. We find that for all reasonable nebular <span class="hlt">masses</span>, these planetesimals contain a minimum of 3% water as <span class="hlt">ice</span> by <span class="hlt">mass</span>. The fraction of <span class="hlt">ice</span> increases as the planetesimals increase in size and as the nebular <span class="hlt">mass</span> decreases, since both factors increase the feeding zones 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/2013APJAS..49..443P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013APJAS..49..443P"><span>Heat flux <span class="hlt">variations</span> over sea <span class="hlt">ice</span> observed at the coastal area of the Sejong Station, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Park, Sang-Jong; Choi, Tae-Jin; Kim, Seong-Joong</p> <p>2013-08-01</p> <p>This study presents <span class="hlt">variations</span> of sensible heat flux and latent heat flux over sea <span class="hlt">ice</span> observed in 2011 from the 10-m flux tower located at the coast of the Sejong Station on King George Island, Antarctica. A period from July to September was selected as a sea <span class="hlt">ice</span> period based on daily record of sea state and hourly photos looking at the Marian Cove in front of the Sejong Station. For the sea <span class="hlt">ice</span> period, mean sensible heat flux is about -11 Wm-2, latent heat flux is about +2 W m-2, net radiation is -12 W m-2, and residual energy is -3 W m-2 with clear diurnal <span class="hlt">variations</span>. Estimated mean values of surface exchange coefficients for momentum, heat and moisture are 5.15 × 10-3, 1.19 × 10-3, and 1.87 × 10-3, respectively. The observed exchange coefficients of heat shows clear diurnal <span class="hlt">variations</span> while those of momentum and moisture do not show diurnal <span class="hlt">variation</span>. The parameterized exchange coefficients of heat and moisture produces heat fluxes which compare well with the observed diurnal <span class="hlt">variations</span> of heat fluxes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19870027099&hterms=microwaves+water+structure&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dmicrowaves%2Bwater%2Bstructure','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19870027099&hterms=microwaves+water+structure&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dmicrowaves%2Bwater%2Bstructure"><span>Satellite microwave and in situ observations of the Weddell Sea <span class="hlt">ice</span> cover and its marginal <span class="hlt">ice</span> zone</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Comiso, J. C.; Sullivan, C. W.</p> <p>1986-01-01</p> <p>The radiative and physical characteristics of the Weddell Sea <span class="hlt">ice</span> cover and its marginal <span class="hlt">ice</span> zone are analyzed using multichannel satellite passive microwave data and ship and helicopter observations obtained during the 1983 Antarctic Marine Ecosystem Research. Winter and spring brightness temperatures are examined; spatial variability in the brightness temperatures of consolidated <span class="hlt">ice</span> in winter and spring cyclic increases and decrease in brightness temperatures of consolidated <span class="hlt">ice</span> with an amplitude of 50 K at 37 GHz and 20 K at 18 GHz are observed. The roles of <span class="hlt">variations</span> in air temperature and surface characteristics in the variability of spring brightness temperatures are investigated. <span class="hlt">Ice</span> concentrations are derived using the frequency and polarization techniques, and the data are compared with the helicopter and ship observations. Temporal changes in the <span class="hlt">ice</span> margin structure and the <span class="hlt">mass</span> balance of fresh water and of biological features of the marginal <span class="hlt">ice</span> zone are studied.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li class="active"><span>7</span></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_7 --> <div id="page_8" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="141"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.C11A0094S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.C11A0094S"><span>Estimation of Greenland's <span class="hlt">Ice</span> Sheet <span class="hlt">Mass</span> Balance Using ICESat and GRACE Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Slobbe, D.; Ditmar, P.; Lindenbergh, R.</p> <p>2007-12-01</p> <p>Data of the GRACE gravity mission and the ICESat laser altimetry mission are used to create two independent estimates of Greenland's <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balance over the full measurement period. For ICESat data, a processing strategy is developed using the elevation differences of geometrically overlapping footprints of both crossing and repeated tracks. The dataset is cleaned using quality flags defined by the GLAS science team. The cleaned dataset reveals some strong, spatially correlated signals that are shown to be related to physical phenomena. Different processing strategies are used to convert the observed temporal height differences to <span class="hlt">mass</span> changes for 6 different drainage systems, further divided into a region above and below 2000 meter elevation. The results are compared with other altimetry based <span class="hlt">mass</span> balance estimates. In general, the obtained results confirm trends discovered by others, but we also show that the choice of processing strategy strongly influences our results, especially for the areas below 2000 meter. Furthermore, GRACE based monthly <span class="hlt">variations</span> of the Earth's gravity field as processed by CNES, CSR, GFZ and DEOS are used to estimate the <span class="hlt">mass</span> balance change for North and South Greenland. It is shown that our results are comparable with recently published GRACE estimates (mascon solutions). On the other hand, the estimates based on GRACE data are only partly confirmed by the ICESat estimates. Possible explanations for the obvious differences will be discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19740004942','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19740004942"><span>Evaluation of glacier <span class="hlt">mass</span> balance by observing <span class="hlt">variations</span> in transient snowline positions. [Jostedalsbreen <span class="hlt">ice</span> cap, Norway</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Oestrem, G. (Principal Investigator)</p> <p>1973-01-01</p> <p>The author has identified the following significant results. The transient snowline on five outlet glaciers from the Jostedalsbreen <span class="hlt">ice</span>-cap in Southwestern Norway could be determined from ERTS-1 image 1336-10260, when bands MSS 5, 6, and 7 were combined in an additive color viewer. The snowline was situated at a very low altitude at the time of imagery (24 June 1973) indicating that glacier melt was behind normal schedule, a fact that has a hydrologic bearing: one could expect less melt water in the streams. The idea to use ERTS-1 imagery in snowline determinations proved realistic and relatively easy to apply in practice. The method will be useful to estimate the glaciers' <span class="hlt">mass</span> balance for large areas, provided some ground truth observations are made. Images from the end of the melt season are of course vital in this work.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.C53A0822T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.C53A0822T"><span>Modeling North American <span class="hlt">Ice</span> Sheet Response to Changes in Precession and Obliquity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tabor, C.; Poulsen, C. J.; Pollard, D.</p> <p>2012-12-01</p> <p>Milankovitch theory proposes that changes in insolation due to orbital perturbations dictate the waxing and waning of the <span class="hlt">ice</span> sheets (Hays et al., 1976). However, <span class="hlt">variations</span> in solar forcing alone are insufficient to produce the glacial oscillations observed in the climate record. Non-linear feedbacks in the Earth system likely work in concert with the orbital cycles to produce a modified signal (e.g. Berger and Loutre, 1996), but the nature of these feedbacks remain poorly understood. To gain a better understand of the <span class="hlt">ice</span> dynamics and climate feedbacks associated with changes in orbital configuration, we use a complex Earth system model consisting of the GENESIS GCM and land surface model (Pollard and Thompson, 1997), the Pennsylvania State University <span class="hlt">ice</span> sheet model (Pollard and DeConto, 2009), and the BIOME vegetation model (Kaplan et al., 2001). We began this study by investigating <span class="hlt">ice</span> sheet sensitivity to a range of commonly used <span class="hlt">ice</span> sheet model parameters, including <span class="hlt">mass</span> balance and albedo, to optimize simulations for Pleistocene orbital cycles. Our tests indicate that choice of <span class="hlt">mass</span> balance and albedo parameterizations can lead to significant differences in <span class="hlt">ice</span> sheet behavior and volume. For instance, use of an insolation-temperature <span class="hlt">mass</span> balance scheme (van den Berg, 2008) allows for a larger <span class="hlt">ice</span> sheet response to orbital changes than the commonly employed positive degree-day method. Inclusion of a large temperature dependent <span class="hlt">ice</span> albedo, representing phenomena such as melt ponds and dirty <span class="hlt">ice</span>, also enhances <span class="hlt">ice</span> sheet sensitivity. Careful tuning of <span class="hlt">mass</span> balance and albedo parameterizations can help alleviate the problem of insufficient <span class="hlt">ice</span> sheet retreat during periods of high summer insolation (Horton and Poulsen, 2007) while still accurately replicating the modern climate. Using our optimized configuration, we conducted a series of experiments with idealized transient orbits in an asynchronous coupling scheme to investigate the influence of obliquity and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC43J..06R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC43J..06R"><span>The direct mechanical influence of sea <span class="hlt">ice</span> state on <span class="hlt">ice</span> sheet <span class="hlt">mass</span> loss via iceberg mélange</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Robel, A.</p> <p>2017-12-01</p> <p>The interaction between sea <span class="hlt">ice</span> and land <span class="hlt">ice</span> has typically been considered as a large-scale exchange of moisture, heat and salinity through the ocean and atmosphere. However, recent observations from marine-terminating glaciers in Greenland indicate that the long-term decline of local sea <span class="hlt">ice</span> cover has been accompanied by an increase in nearby iceberg calving and associated <span class="hlt">ice</span> sheet <span class="hlt">mass</span> loss. Near glacier calving fronts, sea <span class="hlt">ice</span> binds icebergs together into an aggregate granular material known as iceberg mélange. Studies have hypothesized that mélange may suppress calving by exerting a mechanical buttressing force directly on the glacier terminus. Here, we show explicitly how sea <span class="hlt">ice</span> thickness and concentration play a critical role in setting the material strength of mélange. To do so, we adapt a discrete element model to simulate mélange as a cohesive granular material. In these simulations, mélange laden with thick, dense, landfast sea <span class="hlt">ice</span> can produce enough resistance to shut down calving at the terminus. When sea <span class="hlt">ice</span> thins, mélange weakens, reducing the mechanical force of mélange on the glacier terminus, and increasing the likelihood of calving. We discuss whether longer periods of sea-<span class="hlt">ice</span>-free conditions in winter may lead to a transition from currently slow calving, predominantly occurring in the summer, to rapid calving, occurring throughout the year. We also discuss the potential role of freshwater discharge in promoting sea <span class="hlt">ice</span> formation in fjords, potentially strengthening mélange.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007E%26PSL.264..391S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007E%26PSL.264..391S"><span>Regional <span class="hlt">ice-mass</span> changes and glacial-isostatic adjustment in Antarctica from GRACE</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sasgen, Ingo; Martinec, Zdeněk; Fleming, Kevin</p> <p>2007-12-01</p> <p>We infer regional <span class="hlt">mass</span> changes in Antarctica using ca. 4 years of Gravity Recovery and Climate Experiment (GRACE) level 2 data. We decompose the time series of the Stokes coefficients into their linear as well as annual and semi-annual components by a least-squares adjustment and apply a statistical reliability test to the Stokes potential-coefficients' linear temporal trends. <span class="hlt">Mass</span> changes in three regions of Antarctica that display prominent geoid-height change are determined by adjusting predictions of glacier melting at the tip of the Antarctic Peninsula and in the Amundsen Sea Sector, and of the glacial-isostatic adjustment (GIA) over the Ronne <span class="hlt">Ice</span> Shelf. We use the GFZ RL04, CNES RL01C, JPL RL04 and CSR RL04 potential-coefficient releases, and show that, although all data sets consistently reflect the prominent <span class="hlt">mass</span> changes, differences in the <span class="hlt">mass</span>-change estimates are considerably larger than the uncertainties estimated by the propagation of the GRACE errors. We then use the bootstrapping method based on the four releases and six time intervals, each with 3.5 years of data, to quantify the variability of the mean <span class="hlt">mass</span>-change estimates. We find 95% of our estimates to lie within 0.08 and 0.09 mm/a equivalent sea-level (ESL) change for the Antarctic Peninsula and within 0.18 and 0.20 mm/a ESL for the Amundsen Sea Sector. Forward modelling of the GIA over the Ronne <span class="hlt">Ice</span> Shelf region suggests that the Antarctic continent was covered by 8.4 to 9.4 m ESL of additional <span class="hlt">ice</span> during the Last-Glacial Maximum (ca. 22 to 15 ka BP). With regards to the mantle-viscosity values and the glacial history used, this value is considered as a minimum estimate. The <span class="hlt">mass</span>-change estimates derived from all GRACE releases and time intervals lie within ca. 20% (Amundsen Sea Sector), 30% (Antarctic Peninsula) and 50% (Ronne <span class="hlt">Ice</span> Shelf region) of the bootstrap-estimated mean, demonstrating the reliability of results obtained using GRACE observations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28362423','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28362423"><span><span class="hlt">Ice</span> Generation and the Heat and <span class="hlt">Mass</span> Transfer Phenomena of Introducing Water to a Cold Bath of Brine.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yun, Xiao; Quarini, Giuseppe L</p> <p>2017-03-13</p> <p>We demonstrate a method for the study of the heat and <span class="hlt">mass</span> transfer and of the freezing phenomena in a subcooled brine environment. Our experiment showed that, under the proper conditions, <span class="hlt">ice</span> can be produced when water is introduced to a bath of cold brine. To make <span class="hlt">ice</span> form, in addition to having the brine and water mix, the rate of heat transfer must bypass that of <span class="hlt">mass</span> transfer. When water is introduced in the form of tiny droplets to the brine surface, the mode of heat and <span class="hlt">mass</span> transfer is by diffusion. The buoyancy stops water from mixing with the brine underneath, but as the <span class="hlt">ice</span> grows thicker, it slows down the rate of heat transfer, making <span class="hlt">ice</span> more difficult to grow as a result. When water is introduced inside the brine in the form of a flow, a number of factors are found to influence how much <span class="hlt">ice</span> can form. Brine temperature and concentration, which are the driving forces of heat and <span class="hlt">mass</span> transfer, respectively, can affect the water-to-<span class="hlt">ice</span> conversion ratio; lower bath temperatures and brine concentrations encourage more <span class="hlt">ice</span> to form. The flow rheology, which can directly affect both the heat and <span class="hlt">mass</span> transfer coefficients, is also a key factor. In addition, the flow rheology changes the area of contact of the flow with the bulk fluid.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGeod..92..299R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGeod..92..299R"><span>Statistically optimal estimation of Greenland <span class="hlt">Ice</span> Sheet <span class="hlt">mass</span> <span class="hlt">variations</span> from GRACE monthly solutions using an improved mascon approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ran, J.; Ditmar, P.; Klees, R.; Farahani, H. H.</p> <p>2018-03-01</p> <p>We present an improved mascon approach to transform monthly spherical harmonic solutions based on GRACE satellite data into <span class="hlt">mass</span> anomaly estimates in Greenland. The GRACE-based spherical harmonic coefficients are used to synthesize gravity anomalies at satellite altitude, which are then inverted into <span class="hlt">mass</span> anomalies per mascon. The limited spectral content of the gravity anomalies is properly accounted for by applying a low-pass filter as part of the inversion procedure to make the functional model spectrally consistent with the data. The full error covariance matrices of the monthly GRACE solutions are properly propagated using the law of covariance propagation. Using numerical experiments, we demonstrate the importance of a proper data weighting and of the spectral consistency between functional model and data. The developed methodology is applied to process real GRACE level-2 data (CSR RL05). The obtained <span class="hlt">mass</span> anomaly estimates are integrated over five drainage systems, as well as over entire Greenland. We find that the statistically optimal data weighting reduces random noise by 35-69%, depending on the drainage system. The obtained <span class="hlt">mass</span> anomaly time-series are de-trended to eliminate the contribution of <span class="hlt">ice</span> discharge and are compared with de-trended surface <span class="hlt">mass</span> balance (SMB) time-series computed with the Regional Atmospheric Climate Model (RACMO 2.3). We show that when using a statistically optimal data weighting in GRACE data processing, the discrepancies between GRACE-based estimates of SMB and modelled SMB are reduced by 24-47%.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5426515','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5426515"><span>Sea-level feedback lowers projections of future Antarctic <span class="hlt">Ice</span>-Sheet <span class="hlt">mass</span> loss</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Gomez, Natalya; Pollard, David; Holland, David</p> <p>2015-01-01</p> <p>The stability of marine sectors of the Antarctic <span class="hlt">Ice</span> Sheet (AIS) in a warming climate has been identified as the largest source of uncertainty in projections of future sea-level rise. Sea-level fall near the grounding line of a retreating marine <span class="hlt">ice</span> sheet has a stabilizing influence on the <span class="hlt">ice</span> sheets, and previous studies have established the importance of this feedback on <span class="hlt">ice</span> age AIS evolution. Here we use a coupled <span class="hlt">ice</span> sheet–sea-level model to investigate the impact of the feedback mechanism on future AIS retreat over centennial and millennial timescales for a range of emission scenarios. We show that the combination of bedrock uplift and sea-surface drop associated with <span class="hlt">ice</span>-sheet retreat significantly reduces AIS <span class="hlt">mass</span> loss relative to a simulation without these effects included. Sensitivity analyses show that the stabilization tends to be greatest for lower emission scenarios and Earth models characterized by a thin elastic lithosphere and low-viscosity upper mantle, as is the case for West Antarctica. PMID:26554381</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.B21F..01H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.B21F..01H"><span>Pedogenesis on <span class="hlt">ice</span> (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hodson, A. J.</p> <p>2010-12-01</p> <p>It is well known from <span class="hlt">ice</span> cores that organic and mineral debris accumulates within glacier <span class="hlt">ice</span> following atmospheric deposition. However, the concentrations of such debris are usually greatest upon the <span class="hlt">ice</span> surface, especially at the margins of continental glaciers and <span class="hlt">ice</span> sheets, where it forms mm-scale aggregate particles called “cryoconite”. According to the literature, cryoconite covers about 2 % of the ablation areas of glaciers outside Greenland and Antarctica, equivalent to a <span class="hlt">mass</span> loading of ca. 25 g/m2. Of the great <span class="hlt">ice</span> sheets not included in this figure, Greenland is the easiest to estimate, and new observations from the NE and SW sectors indicate <span class="hlt">mass</span> loadings in the range 17 - 440 g/m2. Studies of cryoconite often report the presence of a significant biomass (usually 10^4 - 10^7 cells/g) that is capable of a wide range of biogeochemical functions. The first part of this presentation will therefore explore the contention that the formation of cryoconite represents the first stages of pedogenesis, resulting in the production of soil-type aggregates that inoculate glacial forefields following glacier retreat. Emphasis will be given to the relevant processes that result in aggregate formation, including rapid cell-mineral attachment within melting snowpacks and the slower, biological processes of cementation within thermodynamically stable habitats such as cryoconite holes. The second part of the presentation will use examples from Svalbard, Greenland and Antarctica to consider the carbon balance of the cryoconite during the longest phase of its life cycle: upon the <span class="hlt">ice</span>. It will be demonstrated how the efficacy of photosynthesis is strongly influenced by thermodynamic conditions at or near this surface. Data from the Greenland and Antarctic <span class="hlt">ice</span> sheets will show how thermal equilibration decouples <span class="hlt">variations</span> in photosynthesis from <span class="hlt">variations</span> in incident radiation over timescales > 1 d, resulting in an equitable, low-carbon economy for aggregates within</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120002589','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120002589"><span>Analysis of a Hovering Rotor 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>Narducci, Robert; Kreeger, Richard E.</p> <p>2012-01-01</p> <p>A high fidelity analysis method is proposed to evaluate the <span class="hlt">ice</span> accumulation and the ensuing rotor performance degradation for a helicopter flying through an <span class="hlt">icing</span> cloud. The process uses computational fluid dynamics (CFD) coupled to a rotorcraft comprehensive code to establish the aerodynamic environment of a trimmed rotor prior to <span class="hlt">icing</span>. Based on local aerodynamic conditions along the rotor span and accounting for the azimuthal <span class="hlt">variation</span>, an <span class="hlt">ice</span> accumulation analysis using NASA's Lewice3D code is made to establish the <span class="hlt">ice</span> geometry. Degraded rotor performance is quantified by repeating the high fidelity rotor analysis with updates which account for <span class="hlt">ice</span> shape and <span class="hlt">mass</span>. The process is applied on a full-scale UH-1H helicopter in hover using data recorded during the Helicopter <span class="hlt">Icing</span> Flight Test Program.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990071136&hterms=balance+sheet&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dbalance%2Bsheet','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990071136&hterms=balance+sheet&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dbalance%2Bsheet"><span>Large <span class="hlt">Ice</span> Discharge From 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>Rignot, Eric</p> <p>1999-01-01</p> <p>The objectives of this work are to measure the <span class="hlt">ice</span> discharge of the Greenland <span class="hlt">Ice</span> Sheet close to the grounding line and/or calving front, and compare the results with <span class="hlt">mass</span> accumulation and ablation in the interior to estimate the <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19970027961','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19970027961"><span>Seasonal <span class="hlt">Variation</span> of <span class="hlt">Mass</span> Transport Across the Tropopause</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Appenzeller, Christof; Holton, James R.; Rosenlof, Karen H.</p> <p>1996-01-01</p> <p>The annual cycle of the net <span class="hlt">mass</span> transport across the extratropical tropopause is examined. Contributions from both the global-scale meridional circulation and the <span class="hlt">mass</span> <span class="hlt">variation</span> of the lowermost stratosphere are included. For the northern hemisphere the <span class="hlt">mass</span> of the lowermost stratosphere has a distinct annual cycle, whereas for the southern hemisphere, the corresponding <span class="hlt">variation</span> is weak. The net <span class="hlt">mass</span> transport across the tropopause in the northern hemisphere has a maximum in late spring and a distinct minimum in autumn. This <span class="hlt">variation</span> and its magnitude compare well with older estimates based on representative Sr-90 mixing ratios. For the southern hemisphere the seasonal cycle of the net <span class="hlt">mass</span> transport is weaker and follows roughly the annual <span class="hlt">variation</span> of the net <span class="hlt">mass</span> flux across a nearby isentropic surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19..187K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19..187K"><span>Last Glacial-Interglacial Transition <span class="hlt">ice</span> dynamics in the Wicklow Mountains, Ireland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Knight, Lauren; Boston, Clare; Lovell, Harold; Pepin, Nick</p> <p>2017-04-01</p> <p>Understanding of the extent and dynamics of former <span class="hlt">ice</span> <span class="hlt">masses</span> in the Wicklow Mountains, Ireland, during the Last Glacial-Interglacial Transition (LGIT; 15-10 ka BP) is currently unresolved. Whilst it is acknowledged that the region hosted a local <span class="hlt">ice</span> cap within the larger British-Irish <span class="hlt">Ice</span> Sheet at the Last Glacial Maximum (LGM; 27 ka BP), there has been little consideration of <span class="hlt">ice</span> cap disintegration to a topographically constrained <span class="hlt">ice</span> <span class="hlt">mass</span> during the LGIT. This research has produced the first regional glacial geomorphological map, through remote sensing (aerial photograph and digital terrain model interrogation) and field mapping. This has allowed both the style and extent of mountain glaciation and <span class="hlt">ice</span> recession dynamics during the LGIT to be established. This geomorphological mapping has highlighted that evidence for local glaciation in the Wicklow Mountains is more extensive than previously recognised, and that small icefields and associated outlet valley glaciers existed during the LGIT following disintegration of the Wicklow <span class="hlt">Ice</span> Cap. A relative chronology based on morphostratigraphic principles is developed, which indicates complex patterns of <span class="hlt">ice</span> <span class="hlt">mass</span> oscillation characterised by periods of both sustained retreat and minor readvance. <span class="hlt">Variations</span> in the pattern of recession across the Wicklow Mountains are evident and appear to be influenced, in part, by topographic controls (e.g. slope, aspect, glacier hypsometry). In summary, this research establishes a relative chronology of glacial events in the region during the LGIT and presents constraints on <span class="hlt">ice</span> <span class="hlt">mass</span> extent, dynamics and retreat patterns, offering an insight into small <span class="hlt">ice</span> <span class="hlt">mass</span> behaviour in a warming climate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040035794','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040035794"><span>A Computational <span class="hlt">Icing</span> Effects Study for a Three-Dimensional Wing: Comparison with Experimental Data and Investigation of Spanwise <span class="hlt">Variation</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Thompson, D.; Mogili, P.; Chalasani, S.; Addy, H.; Choo, Y.</p> <p>2004-01-01</p> <p>Steady-state solutions of the Reynolds-averaged Navier-Stokes (RANS) equations were computed using the Colbalt flow solver for a constant-section, rectangular wing based on an extruded two-dimensional glaze <span class="hlt">ice</span> shape. The one equation Spalart-Allmaras turbulence model was used. The results were compared with data obtained from a recent wind tunnel test. Computed results indicate that the steady RANS solutions do not accurately capture the recirculating region downstream of the <span class="hlt">ice</span> accretion, even after a mesh refinement. The resulting predicted reattachment is farther downstream than indicated by the experimental data. Additionally, the solutions computed on a relatively coarse baseline mesh had detailed flow characteristics that were different from those computed on the refined mesh or the experimental data. Steady RANS solutions were also computed to investigate the effects of spanwise <span class="hlt">variation</span> in the <span class="hlt">ice</span> shape. The spanwise <span class="hlt">variation</span> was obtained via a bleeding function that merged the <span class="hlt">ice</span> shape with the clean wing using a sinusoidal spanwise <span class="hlt">variation</span>. For these configurations, the results predicted for the extruded shape provided conservative estimates for the performance degradation of the wing. Additionally, the spanwise <span class="hlt">variation</span> in the <span class="hlt">ice</span> shape and the resulting differences in the flow fields did not significantly change the location of the primary reattachment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.G21B0875K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.G21B0875K"><span>Exploring the effect of East Antarctic <span class="hlt">ice</span> <span class="hlt">mass</span> loss on GIA-induced horizontal bedrock motions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Konfal, S. A.; Whitehouse, P. L.; Hermans, T.; van der Wal, W.; Wilson, T. J.; Bevis, M. G.; Kendrick, E. C.; Dalziel, I.; Smalley, R., Jr.</p> <p>2017-12-01</p> <p><span class="hlt">Ice</span> history inputs used in Antarctic models of GIA include major centers of <span class="hlt">ice</span> <span class="hlt">mass</span> loss in West Antarctica. In the Transantarctic Mountains (TAM) region spanning the boundary between East and West Antarctica, horizontal crustal motions derived from GPS observations from the Antarctic Network (ANET) component of the Polar Earth Observing Network (POLENET) are towards these West Antarctic <span class="hlt">ice</span> <span class="hlt">mass</span> centers, opposite to the pattern of radial crustal motion expected in an unloading scenario. We investigate alternative <span class="hlt">ice</span> history and earth structure inputs to GIA models in an attempt to reproduce observed crustal motions in the region. The W12 <span class="hlt">ice</span> history model is altered to create scenarios including <span class="hlt">ice</span> unloading in the Wilkes Subglacial Basin based on available glaciological records. These altered <span class="hlt">ice</span> history models, along with the unmodified W12 <span class="hlt">ice</span> history model, are coupled with 60 radially varying (1D) earth model combinations, including approximations of optimal earth profiles identified in published GIA models. The resulting model-predicted motions utilizing both the modified and unmodified <span class="hlt">ice</span> history models fit ANET GPS-derived crustal motions in the northern TAM region for a suite of earth model combinations. Further south, where the influence of simulated Wilkes unloading is weakest and West Antarctic unloading is strongest, observed and predicted motions do not agree. The influence of simulated Wilkes <span class="hlt">ice</span> unloading coupled with laterally heterogeneous earth models is also investigated. The resulting model-predicted motions do not differ significantly between the original W12 and W12 with simulated Wilkes unloading <span class="hlt">ice</span> histories.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.C24A..03K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.C24A..03K"><span>Seasonal climate information preserved within West Antarctic <span class="hlt">ice</span> cores and its relation to large-scale atmospheric circulation and regional sea <span class="hlt">ice</span> <span class="hlt">variations</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Küttel, M.; Steig, E. J.; Ding, Q.; Battisti, D. S.</p> <p>2010-12-01</p> <p>Recent evidence suggests that West Antarctica has been warming since at least the 1950s. With the instrumental record being limited to the mid-20th century, indirect information from stable isotopes (δ18O and δD, hereafter collectively δ) preserved within <span class="hlt">ice</span> cores have commonly been used to place this warming into a long term context. Here, using a large number of δ records obtained during the International Trans-Antarctic Scientific Expedition (ITASE), past <span class="hlt">variations</span> in West Antarctic δ are not only investigated over time but also in space. This study therefore provides an important complement to longer records from single locations as e.g. the currently being processed West Antarctic <span class="hlt">ice</span> sheet (WAIS) Divide <span class="hlt">ice</span> core. Although snow accumulation rates at the ITASE sites in West Antarctica are variable, they are generally high enough to allow studies on sub-annual scale over the last 50-100 years. Here, we show that <span class="hlt">variations</span> in δ in this region are strongly related to the state of the large-scale atmospheric circulation as well as sea <span class="hlt">ice</span> <span class="hlt">variations</span> in the adjacent Southern Ocean, with important seasonal changes. While a strong relationship to sea <span class="hlt">ice</span> changes in the Ross and Amundsen Sea as well as to the atmospheric circulation offshore is found during austral fall (MAM) and winter (JJA), only modest correlations are found during spring (SON) and summer (DJF). Interestingly, the correlations with the atmospheric circulation in the latter two seasons have the strongest signal over the Antarctic continent, but not offshore - an important difference to MAM and JJA. These seasonal changes are in good agreement with the seasonally varying predominant circulation: meridional with more frequent storms in the Amundsen Sea during MAM and JJA and more zonal and stable during SON and DJF. The relationship to regional temperature is similarly seasonally variable with highest correlations found during MAM and JJA. Notably, the circulation pattern found to be strongest</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1917195R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1917195R"><span>A genetic algorithm approach to estimate glacier <span class="hlt">mass</span> <span class="hlt">variations</span> from GRACE data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Reimond, Stefan; Klinger, Beate; Krauss, Sandro; Mayer-Gürr, Torsten</p> <p>2017-04-01</p> <p>The application of a genetic algorithm (GA) to the inference of glacier <span class="hlt">mass</span> <span class="hlt">variations</span> with a point-<span class="hlt">mass</span> modeling method is described. GRACE K-band ranging data (available since April 2002) processed at the Graz University of Technology serve as input for this study. The reformulation of the point-<span class="hlt">mass</span> inversion method in terms of an optimization problem is motivated by two reasons: first, an improved choice of the positions of the modeled point-<span class="hlt">masses</span> (with a particular focus on the depth parameter) is expected to increase the signal-to-noise ratio. Considering these coordinates as additional unknown parameters (besides from the <span class="hlt">mass</span> change magnitudes) results in a highly non-linear optimization problem. The second reason is that the <span class="hlt">mass</span> inversion from satellite tracking data is an ill-posed problem, and hence regularization becomes necessary. The main task in this context is the determination of the regularization parameter, which is typically done by means of heuristic selection rules like, e.g., the L-curve criterion. In this study, however, the challenge of selecting a suitable balancing parameter (or even a matrix) is tackled by introducing regularization to the overall optimization problem. Based on this novel approach, estimations of <span class="hlt">ice-mass</span> changes in various alpine glacier systems (e.g. Svalbard) are presented and compared to existing results and alternative inversion methods.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014TCry....8..743G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014TCry....8..743G"><span>Empirical estimation of present-day Antarctic glacial isostatic adjustment and <span class="hlt">ice</span> <span class="hlt">mass</span> change</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gunter, B. C.; Didova, O.; Riva, R. E. M.; Ligtenberg, S. R. M.; Lenaerts, J. T. M.; King, M. A.; van den Broeke, M. R.; Urban, T.</p> <p>2014-04-01</p> <p>This study explores an approach that simultaneously estimates Antarctic <span class="hlt">mass</span> balance and glacial isostatic adjustment (GIA) through the combination of satellite gravity and altimetry data sets. The results improve upon previous efforts by incorporating a firn densification model to account for firn compaction and surface processes as well as reprocessed data sets over a slightly longer period of time. A range of different Gravity Recovery and Climate Experiment (GRACE) gravity models were evaluated and a new <span class="hlt">Ice</span>, Cloud, and Land Elevation Satellite (ICESat) surface height trend map computed using an overlapping footprint approach. When the GIA models created from the combination approach were compared to in situ GPS ground station displacements, the vertical rates estimated showed consistently better agreement than recent conventional GIA models. The new empirically derived GIA rates suggest the presence of strong uplift in the Amundsen Sea sector in West Antarctica (WA) and the Philippi/Denman sectors, as well as subsidence in large parts of East Antarctica (EA). The total GIA-related <span class="hlt">mass</span> change estimates for the entire Antarctic <span class="hlt">ice</span> sheet ranged from 53 to 103 Gt yr-1, depending on the GRACE solution used, with an estimated uncertainty of ±40 Gt yr-1. Over the time frame February 2003-October 2009, the corresponding <span class="hlt">ice</span> <span class="hlt">mass</span> change showed an average value of -100 ± 44 Gt yr-1 (EA: 5 ± 38, WA: -105 ± 22), consistent with other recent estimates in the literature, with regional <span class="hlt">mass</span> loss mostly concentrated in WA. The refined approach presented in this study shows the contribution that such data combinations can make towards improving estimates of present-day GIA and <span class="hlt">ice</span> <span class="hlt">mass</span> change, particularly with respect to determining more reliable uncertainties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17733504','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17733504"><span>Devon island <span class="hlt">ice</span> cap: core stratigraphy and paleoclimate.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Koerner, R M</p> <p>1977-04-01</p> <p>Valuable paleoclimatic information can be gained by studying the distribution of melt layers in deep <span class="hlt">ice</span> cores. A profile representing the percentage of <span class="hlt">ice</span> in melt layers in a core drilled from the Devon Island <span class="hlt">ice</span> cap plotted against both time and depth shows that the <span class="hlt">ice</span> cap has experienced a period of very warm summers since 1925, following a period of colder summers between about 1600 and 1925. The earlier period was coldest between 1680 and 1730. There is a high correlation between the melt-layer <span class="hlt">ice</span> percentage and the <span class="hlt">mass</span> balance of the <span class="hlt">ice</span> cap. The relation between them suggests that the <span class="hlt">ice</span> cap <span class="hlt">mass</span> balance was zero (accumulation equaled ablation) during the colder period but is negative in the present warmer one. There is no firm evidence of a present cooling trend in the summer conditions on the <span class="hlt">ice</span> cap. A comparison with the melt-layer <span class="hlt">ice</span> percentage in cores from the other major Canadian Arctic <span class="hlt">ice</span> caps shows that the <span class="hlt">variation</span> of summer conditions found for the Devon Island <span class="hlt">ice</span> cap is representative for all the large <span class="hlt">ice</span> caps for about 90 percent of the time. There is also a good correlation between melt-layer percentage and summer sea-<span class="hlt">ice</span> conditions in the archipelago. This suggests that the search for the northwest passage was influenced by changing climate, with the 19th-century peak of the often tragic exploration coinciding with a period of very cold summers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..44.7328C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..44.7328C"><span><span class="hlt">Mass</span> balance reassessment of glaciers draining into the Abbot and Getz <span class="hlt">Ice</span> Shelves of West Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chuter, S. J.; Martín-Español, A.; Wouters, B.; Bamber, J. L.</p> <p>2017-07-01</p> <p>We present a reassessment of input-output method <span class="hlt">ice</span> <span class="hlt">mass</span> budget estimates for the Abbot and Getz regions of West Antarctica using CryoSat-2-derived <span class="hlt">ice</span> thickness estimates. The <span class="hlt">mass</span> budget is 8 ± 6 Gt yr-1 and 5 ± 17 Gt yr-1 for the Abbot and Getz sectors, respectively, for the period 2006-2008. Over the Abbot region, our results resolve a previous discrepancy with elevation rates from altimetry, due to a previous 30% overestimation of <span class="hlt">ice</span> thickness. For the Getz sector, our results are at the more positive bound of estimates from other techniques. Grounding line velocity increases up to 20% between 2007 and 2014 alongside mean elevation rates of -0.67 ± 0.13 m yr-1 between 2010 and 2013 indicate the onset of a dynamic thinning signal. Mean snowfall trends of -0.33 m yr-1 water equivalent since 2006 indicate recent <span class="hlt">mass</span> trends are driven by both <span class="hlt">ice</span> dynamics and surface processes.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_8 --> <div id="page_9" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="161"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C23E..01R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C23E..01R"><span><span class="hlt">Variational</span> Ridging in Sea <span class="hlt">Ice</span> Models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roberts, A.; Hunke, E. C.; Lipscomb, W. H.; Maslowski, W.; Kamal, S.</p> <p>2017-12-01</p> <p>This work presents the results of a new development to make basin-scale sea <span class="hlt">ice</span> models aware of the shape, porosity and extent of individual ridges within the pack. We have derived an analytic solution for the Euler-Lagrange equation of individual ridges that accounts for non-conservative forces, and therefore the compressive strength of individual ridges. Because a region of the pack is simply a collection of paths of individual ridges, we are able to solve the Euler-Lagrange equation for a large-scale sea <span class="hlt">ice</span> field also, and therefore the compressive strength of a region of the pack that explicitly accounts for the macro-porosity of ridged debris. We make a number of assumptions that have simplified the problem, such as treating sea <span class="hlt">ice</span> as a granular material in ridges, and assuming that bending moments associated with ridging are perturbations around an isostatic state. Regardless of these simplifications, the ridge model is remarkably predictive of macro-porosity and ridge shape, and, because our equations are analytic, they do not require costly computations to solve the Euler-Lagrange equation of ridges on the large scale. The new ridge model is therefore applicable to large-scale sea <span class="hlt">ice</span> models. We present results from this theoretical development, as well as plans to apply it to the Regional Arctic System Model and a community sea <span class="hlt">ice</span> code. Most importantly, the new ridging model is particularly useful for pinpointing gaps in our observational record of sea <span class="hlt">ice</span> ridges, and points to the need for improved measurements of the evolution of porosity of deformed <span class="hlt">ice</span> in the Arctic and Antarctic. Such knowledge is not only useful for improving models, but also for improving estimates of sea <span class="hlt">ice</span> volume derived from altimetric measurements of sea <span class="hlt">ice</span> freeboard.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1918364H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1918364H"><span>Sea <span class="hlt">Ice</span> <span class="hlt">Mass</span> Balance Buoys (IMBs): First Results from a Data Processing Intercomparison Study</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hoppmann, Mario; Tiemann, Louisa; Itkin, Polona</p> <p>2017-04-01</p> <p>IMBs are autonomous instruments able to continuously monitor the growth and melt of sea <span class="hlt">ice</span> and its snow cover at a single point on an <span class="hlt">ice</span> floe. Complementing field expeditions, remote sensing observations and modelling studies, these in-situ data are crucial to assess the <span class="hlt">mass</span> balance and seasonal evolution of sea <span class="hlt">ice</span> and snow in the polar oceans. Established subtypes of IMBs combine coarse-resolution temperature profiles through air, snow, <span class="hlt">ice</span> and ocean with ultrasonic pingers to detect snow accumulation and <span class="hlt">ice</span> thermodynamic growth. Recent technological advancements enable the use of high-resolution temperature chains, which are also able to identify the surrounding medium through a „heating cycle". The temperature change during this heating cycle provides additional information on the internal properties and processes of the <span class="hlt">ice</span>. However, a unified data processing technique to reliably and accurately determine sea <span class="hlt">ice</span> thickness and snow depth from this kind of data is still missing, and an unambiguous interpretation remains a challenge. Following the need to improve techniques for remotely measuring sea <span class="hlt">ice</span> <span class="hlt">mass</span> balance, an international IMB working group has recently been established. The main goals are 1) to coordinate IMB deployments, 2) to enhance current IMB data processing and -interpretation techniques, and 3) to provide standardized IMB data products to a broader community. Here we present first results from two different data processing algorithms, applied to selected IMB datasets from the Arctic and Antarctic. Their performance with regard to sea <span class="hlt">ice</span> thickness and snow depth retrieval is evaluated, and an uncertainty is determined. Although several challenges and caveats in IMB data processing and -interpretation are found, such datasets bear great potential and yield plenty of useful information about sea <span class="hlt">ice</span> properties and processes. It is planned to include many more algorithms from contributors within the working group, and we explicitly invite</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26672555','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26672555"><span>Spatial and temporal distribution of <span class="hlt">mass</span> loss from the Greenland <span class="hlt">Ice</span> Sheet since AD 1900.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kjeldsen, Kristian K; Korsgaard, Niels J; Bjørk, Anders A; Khan, Shfaqat A; Box, Jason E; Funder, Svend; Larsen, Nicolaj K; Bamber, Jonathan L; Colgan, William; van den Broeke, Michiel; Siggaard-Andersen, Marie-Louise; Nuth, Christopher; Schomacker, Anders; Andresen, Camilla S; Willerslev, Eske; Kjær, Kurt H</p> <p>2015-12-17</p> <p>The response of the Greenland <span class="hlt">Ice</span> Sheet (GIS) to changes in temperature during the twentieth century remains contentious, largely owing to difficulties in estimating the spatial and temporal distribution of <span class="hlt">ice</span> <span class="hlt">mass</span> changes before 1992, when Greenland-wide observations first became available. The only previous estimates of change during the twentieth century are based on empirical modelling and energy balance modelling. Consequently, no observation-based estimates of the contribution from the GIS to the global-mean sea level budget before 1990 are included in the Fifth Assessment Report of the Intergovernmental Panel on Climate Change. Here we calculate spatial <span class="hlt">ice</span> <span class="hlt">mass</span> loss around the entire GIS from 1900 to the present using aerial imagery from the 1980s. This allows accurate high-resolution mapping of geomorphic features related to the maximum extent of the GIS during the Little <span class="hlt">Ice</span> Age at the end of the nineteenth century. We estimate the total <span class="hlt">ice</span> <span class="hlt">mass</span> loss and its spatial distribution for three periods: 1900-1983 (75.1 ± 29.4 gigatonnes per year), 1983-2003 (73.8 ± 40.5 gigatonnes per year), and 2003-2010 (186.4 ± 18.9 gigatonnes per year). Furthermore, using two surface <span class="hlt">mass</span> balance models we partition the <span class="hlt">mass</span> balance into a term for surface <span class="hlt">mass</span> balance (that is, total precipitation minus total sublimation minus runoff) and a dynamic term. We find that many areas currently undergoing change are identical to those that experienced considerable thinning throughout the twentieth century. We also reveal that the surface <span class="hlt">mass</span> balance term shows a considerable decrease since 2003, whereas the dynamic term is constant over the past 110 years. Overall, our observation-based findings show that during the twentieth century the GIS contributed at least 25.0 ± 9.4 millimetres of global-mean sea level rise. Our result will help to close the twentieth-century sea level budget, which remains crucial for evaluating the reliability of models used to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015Natur.528..396K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015Natur.528..396K"><span>Spatial and temporal distribution of <span class="hlt">mass</span> loss from the Greenland <span class="hlt">Ice</span> Sheet since AD 1900</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kjeldsen, Kristian K.; Korsgaard, Niels J.; Bjørk, Anders A.; Khan, Shfaqat A.; Box, Jason E.; Funder, Svend; Larsen, Nicolaj K.; Bamber, Jonathan L.; Colgan, William; van den Broeke, Michiel; Siggaard-Andersen, Marie-Louise; Nuth, Christopher; Schomacker, Anders; Andresen, Camilla S.; Willerslev, Eske; Kjær, Kurt H.</p> <p>2015-12-01</p> <p>The response of the Greenland <span class="hlt">Ice</span> Sheet (GIS) to changes in temperature during the twentieth century remains contentious, largely owing to difficulties in estimating the spatial and temporal distribution of <span class="hlt">ice</span> <span class="hlt">mass</span> changes before 1992, when Greenland-wide observations first became available. The only previous estimates of change during the twentieth century are based on empirical modelling and energy balance modelling. Consequently, no observation-based estimates of the contribution from the GIS to the global-mean sea level budget before 1990 are included in the Fifth Assessment Report of the Intergovernmental Panel on Climate Change. Here we calculate spatial <span class="hlt">ice</span> <span class="hlt">mass</span> loss around the entire GIS from 1900 to the present using aerial imagery from the 1980s. This allows accurate high-resolution mapping of geomorphic features related to the maximum extent of the GIS during the Little <span class="hlt">Ice</span> Age at the end of the nineteenth century. We estimate the total <span class="hlt">ice</span> <span class="hlt">mass</span> loss and its spatial distribution for three periods: 1900-1983 (75.1 ± 29.4 gigatonnes per year), 1983-2003 (73.8 ± 40.5 gigatonnes per year), and 2003-2010 (186.4 ± 18.9 gigatonnes per year). Furthermore, using two surface <span class="hlt">mass</span> balance models we partition the <span class="hlt">mass</span> balance into a term for surface <span class="hlt">mass</span> balance (that is, total precipitation minus total sublimation minus runoff) and a dynamic term. We find that many areas currently undergoing change are identical to those that experienced considerable thinning throughout the twentieth century. We also reveal that the surface <span class="hlt">mass</span> balance term shows a considerable decrease since 2003, whereas the dynamic term is constant over the past 110 years. Overall, our observation-based findings show that during the twentieth century the GIS contributed at least 25.0 ± 9.4 millimetres of global-mean sea level rise. Our result will help to close the twentieth-century sea level budget, which remains crucial for evaluating the reliability of models used to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EPSC...11.1010K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EPSC...11.1010K"><span>Reproducing impact ionization <span class="hlt">mass</span> spectra of E and F ring <span class="hlt">ice</span> grains at different impact speeds</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Klenner, F.; Reviol, R.; Postberg, F.</p> <p>2017-09-01</p> <p>As impact speeds of E and F ring <span class="hlt">ice</span> grains impinging onto the target of impact ionization <span class="hlt">mass</span> spectrometers in space can vary greatly, the resulting cationic or anionic <span class="hlt">mass</span> spectra can have very different appearances. The <span class="hlt">mass</span> spectra can be accurately reproduced with an analog experimental setup IR-FL-MALDI-ToF-MS (Infrared Free Liquid Matrix Assisted Laser Desorption and Ionization Time of Flight <span class="hlt">Mass</span> Spectrometry). We compare <span class="hlt">mass</span> spectra of E and F ring <span class="hlt">ice</span> grains taken by the Cosmic Dust Analyzer (CDA) onboard Cassini recorded at different impact speeds with our analog spectra and prove the capability of the analog experiment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150000279','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150000279"><span>A Range Correction for Icesat and Its Potential Impact on <span class="hlt">Ice</span>-sheet <span class="hlt">Mass</span> Balance Studies</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Borsa, A. A.; Moholdt, G.; Fricker, H. A.; Brunt, Kelly M.</p> <p>2014-01-01</p> <p>We report on a previously undocumented range error in NASA's <span class="hlt">Ice</span>, Cloud and land Elevation Satellite (ICESat) that degrades elevation precision and introduces a small but significant elevation trend over the ICESat mission period. This range error (the Gaussian-Centroid or 'G-C'offset) varies on a shot-to-shot basis and exhibits increasing scatter when laser transmit energies fall below 20 mJ. Although the G-C offset is uncorrelated over periods less than1 day, it evolves over the life of each of ICESat's three lasers in a series of ramps and jumps that give rise to spurious elevation trends of -0.92 to -1.90 cm yr(exp -1), depending on the time period considered. Using ICESat data over the Ross and Filchner-Ronne <span class="hlt">ice</span> shelves we show that (1) the G-C offset introduces significant biases in <span class="hlt">ice</span>-shelf <span class="hlt">mass</span> balance estimates, and (2) the <span class="hlt">mass</span> balance bias can vary between regions because of different temporal samplings of ICESat.We can reproduce the effect of the G-C offset over these two <span class="hlt">ice</span> shelves by fitting trends to sample-weighted mean G-C offsets for each campaign, suggesting that it may not be necessary to fully repeat earlier ICESat studies to determine the impact of the G-C offset on <span class="hlt">ice</span>-sheet <span class="hlt">mass</span> balance estimates.</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 <span class="hlt">mass</span> 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 zone and decaying rapidly downstream. Channels, likely originating from upstream subglacial channels, give rise to large melt <span class="hlt">variations</span> 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/2013JGRF..118..667S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JGRF..118..667S"><span>Decadal-scale sensitivity of Northeast Greenland <span class="hlt">ice</span> flow to errors in surface <span class="hlt">mass</span> balance using ISSM</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schlegel, N.-J.; Larour, E.; Seroussi, H.; Morlighem, M.; Box, J. E.</p> <p>2013-06-01</p> <p>The behavior of the Greenland <span class="hlt">Ice</span> Sheet, which is considered a major contributor to sea level changes, is best understood on century and longer time scales. However, on decadal time scales, its response is less predictable due to the difficulty of modeling surface climate, as well as incomplete understanding of the dynamic processes responsible for <span class="hlt">ice</span> flow. Therefore, it is imperative to understand how modeling advancements, such as increased spatial resolution or more comprehensive <span class="hlt">ice</span> flow equations, might improve projections of <span class="hlt">ice</span> sheet response to climatic trends. Here we examine how a finely resolved climate forcing influences a high-resolution <span class="hlt">ice</span> stream model that considers longitudinal stresses. We simulate <span class="hlt">ice</span> flow using a two-dimensional Shelfy-Stream Approximation implemented within the <span class="hlt">Ice</span> Sheet System Model (ISSM) and use uncertainty quantification tools embedded within the model to calculate the sensitivity of <span class="hlt">ice</span> flow within the Northeast Greenland <span class="hlt">Ice</span> Stream to errors in surface <span class="hlt">mass</span> balance (SMB) forcing. Our results suggest that the model tends to smooth <span class="hlt">ice</span> velocities even when forced with extreme errors in SMB. Indeed, errors propagate linearly through the model, resulting in discharge uncertainty of 16% or 1.9 Gt/yr. We find that <span class="hlt">mass</span> flux is most sensitive to local errors but is also affected by errors hundreds of kilometers away; thus, an accurate SMB map of the entire basin is critical for realistic simulation. Furthermore, sensitivity analyses indicate that SMB forcing needs to be provided at a resolution of at least 40 km.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C33D1227B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C33D1227B"><span>Modelling the contribution of supraglacial <span class="hlt">ice</span> cliffs to the <span class="hlt">mass</span>-balance of glaciers in the Langtang catchment, Nepalese Himalaya</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Buri, P.; Steiner, J. F.; Miles, E.; Ragettli, S.; Pellicciotti, F.</p> <p>2017-12-01</p> <p>Supraglacial cliffs are typical surface features of debris-covered glaciers worldwide, affecting surface evolution, and <span class="hlt">mass</span> balance by providing a direct <span class="hlt">ice</span>-atmosphere interface where melt rates can be very high. As a result, <span class="hlt">ice</span> cliffs act as windows of energy transfer from the atmosphere to the <span class="hlt">ice</span>, and enhance melt and <span class="hlt">mass</span> losses of otherwise insulated <span class="hlt">ice</span>. However, their contribution to glacier <span class="hlt">mass</span> balance has never been quantified at the glacier scale, and all inference has been obtained from upscaling results of point-scale models or observations at select individual cliffs. Here we use a 3D, physically-based backwasting model to estimate the volume losses associated with the melting and backwasting of supraglacial <span class="hlt">ice</span> cliffs for the entire debris-covered glacier area of the Langtang catchment. We estimate <span class="hlt">mass</span> losses for the 2014 melt season and compare them to recent values of glacier <span class="hlt">mass</span> balance determined from geodetic and numerical modelling approached. Cliff outlines and topography are derived from high-resolution stereo SPOT6-imagery from April 2014. Meteorological data to force the model are provided by automatic weather stations on- and off-glacier within the valley. The model simulates <span class="hlt">ice</span> cliff backwasting by considering the cliff-atmosphere energy-balance, reburial by debris and the effects of adjacent ponds. In the melt season of 2014, cliffs' distribution and patterns of <span class="hlt">mass</span> losses vary considerably from glacier to glacier, and we relate rates of volume loss to both glaciers' and cliffs' characteristics. Only cliffs with a northerly aspect account for substantial losses. Uncertainty in our estimates is due to the quality of the stereo DEM, uncertainties in the cliff delineation and the fact that we use a conservative approach to cliff delineation and discard very small cliffs and those for which uncertainty in topography is high. Despite these uncertainties, our work presents the first estimate of the importance of supraglacial <span class="hlt">ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.C43A0587P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.C43A0587P"><span>Heat flux <span class="hlt">variations</span> over sea-<span class="hlt">ice</span> observed at the coastal area of the Sejong Station, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Park, S.; Choi, T.; Kim, S.</p> <p>2012-12-01</p> <p>This study presents <span class="hlt">variations</span> of sensible heat flux and latent heat flux over sea-<span class="hlt">ice</span> observed in 2011 from the 10-m flux tower located at the coast of the Sejong Station on King George Island, Antarctica. A period from June to November was divided into three parts: "Freezing", "Frozen", and "Melting" periods based on daily monitoring of sea state and hourly photos looking at the Marian Cove in front of the Sejong Station. The division of periods enabled us to look into the heat flux <span class="hlt">variations</span> depending on the sea-<span class="hlt">ice</span> conditions. Over freezing sea surface during the freezing period of late June, daily mean sensible heat flux was -11.9 Wm-2 and daily mean latent heat flux was +16.3 Wm-2. Over the frozen sea-<span class="hlt">ice</span>, daily mean sensible heat flux was -10.4 Wm-2 while daily mean latent heat flux was +2.4 Wm-2. During the melting period of mid-October to early November, magnitudes of sensible heat flux increased to -14.2 Wm-2 and latent heat flux also increased to +13.5 Wm-2. In short, latent heat flux was usually upward over sea-<span class="hlt">ice</span> most of the time while sensible heat flux was downward from atmosphere to sea-<span class="hlt">ice</span>. Magnitudes of the fluxes were small but increased when freezing or melting of sea-<span class="hlt">ice</span> was occurring. Especially, latent heat flux increased five to six times compared to that of "frozen" period implying that early melting of sea-<span class="hlt">ice</span> may cause five to six times larger supply of moisture to the atmosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.8879B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.8879B"><span>Fingerprinting sea-level <span class="hlt">variations</span> in response to continental <span class="hlt">ice</span> loss: a benchmark exercise</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barletta, Valentina R.; Spada, Giorgio; Riva, Riccardo E. M.; James, Thomas S.; Simon, Karen M.; van der Wal, Wouter; Martinec, Zdenek; Klemann, Volker; Olsson, Per-Anders; Hagedoorn, Jan; Stocchi, Paolo; Vermeersen, Bert</p> <p>2013-04-01</p> <p>Understanding the response of the Earth to the waxing and waning <span class="hlt">ice</span> sheets is crucial in various contexts, ranging from the interpretation of modern satellite geodetic measurements to the projections of future sea level trends in response to climate change. All the processes accompanying Glacial Isostatic Adjustment (GIA) can be described solving the so-called Sea Level Equation (SLE), an integral equation that accounts for the interactions between the <span class="hlt">ice</span> sheets, the solid Earth, and the oceans. Modern approaches to the SLE are based on various techniques that range from purely analytical formulations to fully numerical methods. Here we present the results of a benchmark exercise of independently developed codes designed to solve the SLE. The study involves predictions of current sea level changes due to present-day <span class="hlt">ice</span> <span class="hlt">mass</span> loss. In spite of the differences in the methods employed, the comparison shows that a significant number of GIA modellers can reproduce their sea-level computations within 2% for well defined, large-scale present-day <span class="hlt">ice</span> <span class="hlt">mass</span> changes. Smaller and more detailed loads need further and dedicated benchmarking and high resolution computation. This study shows how the details of the implementation and the inputs specifications are an important, and often underappreciated, aspect. Hence this represents a step toward the assessment of reliability of sea level projections obtained with benchmarked SLE codes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRC..123..864J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123..864J"><span>Ocean-Forced <span class="hlt">Ice</span>-Shelf Thinning in a Synchronously Coupled <span class="hlt">Ice</span>-Ocean Model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jordan, James R.; Holland, Paul R.; Goldberg, Dan; Snow, Kate; Arthern, Robert; Campin, Jean-Michel; Heimbach, Patrick; Jenkins, Adrian</p> <p>2018-02-01</p> <p>The first fully synchronous, coupled <span class="hlt">ice</span> shelf-ocean model with a fixed grounding line and imposed upstream <span class="hlt">ice</span> velocity has been developed using the MITgcm (Massachusetts Institute of Technology general circulation model). Unlike previous, asynchronous, approaches to coupled modeling our approach is fully conservative of heat, salt, and <span class="hlt">mass</span>. Synchronous coupling is achieved by continuously updating the <span class="hlt">ice</span>-shelf thickness on the ocean time step. By simulating an idealized, warm-water <span class="hlt">ice</span> shelf we show how raising the pycnocline leads to a reduction in both <span class="hlt">ice</span>-shelf <span class="hlt">mass</span> and back stress, and hence buttressing. Coupled runs show the formation of a western boundary channel in the <span class="hlt">ice</span>-shelf base due to increased melting on the western boundary due to Coriolis enhanced flow. Eastern boundary <span class="hlt">ice</span> thickening is also observed. This is not the case when using a simple depth-dependent parameterized melt, as the <span class="hlt">ice</span> shelf has relatively thinner sides and a thicker central "bulge" for a given <span class="hlt">ice</span>-shelf <span class="hlt">mass</span>. <span class="hlt">Ice</span>-shelf geometry arising from the parameterized melt rate tends to underestimate backstress (and therefore buttressing) for a given <span class="hlt">ice</span>-shelf <span class="hlt">mass</span> due to a thinner <span class="hlt">ice</span> shelf at the boundaries when compared to coupled model simulations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120002070','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120002070"><span>Assessment of Antarctic <span class="hlt">Ice</span>-Sheet <span class="hlt">Mass</span> Balance Estimates: 1992 - 2009</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; Giovinetto, Mario B.</p> <p>2011-01-01</p> <p>Published <span class="hlt">mass</span> balance estimates for the Antarctic <span class="hlt">Ice</span> Sheet (AIS) lie between approximately +50 to -250 Gt/year for 1992 to 2009, which span a range equivalent to 15% of the annual <span class="hlt">mass</span> input and 0.8 mm/year Sea Level Equivalent (SLE). Two estimates from radar-altimeter measurements of elevation change by European Remote-sensing Satellites (ERS) (+28 and -31 Gt/year) lie in the upper part, whereas estimates from the Input-minus-Output Method (IOM) and the Gravity Recovery and Climate Experiment (GRACE) lie in the lower part (-40 to -246 Gt/year). We compare the various estimates, discuss the methodology used, and critically assess the results. Although recent reports of large and accelerating rates of <span class="hlt">mass</span> loss from GRACE=based studies cite agreement with IOM results, our evaluation does not support that conclusion. We find that the extrapolation used in the published IOM estimates for the 15 % of the periphery for which discharge velocities are not observed gives twice the rate of discharge per unit of associated <span class="hlt">ice</span>-sheet area than the 85% faster-moving parts. Our calculations show that the published extrapolation overestimates the <span class="hlt">ice</span> discharge by 282 Gt/yr compared to our assumption that the slower moving areas have 70% as much discharge per area as the faster moving parts. Also, published data on the time-series of discharge velocities and accumulation/precipitation do not support <span class="hlt">mass</span> output increases or input decreases with time, respectively. Our modified IOM estimate, using the 70% discharge assumption and substituting input from a field-data compilation for input from an atmospheric model over 6% of area, gives a loss of only 13 Gt/year (versus 136 Gt/year) for the period around 2000. Two ERS-based estimates, our modified IOM, and a GRACE-based estimate for observations within 1992 to 2005 lie in a narrowed range of +27 to - 40 Gt/year, which is about 3% of the annual <span class="hlt">mass</span> input and only 0.2 mm/year SLE. Our preferred estimate for 1992-2001 is - 47 Gt</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1913710C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1913710C"><span>Specific findings on <span class="hlt">ice</span> crystal microphysical properties from in-situ observation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Coutris, Pierre; Leroy, Delphine; Fontaine, Emmanuel; Schwarzenboeck, Alfons; Strapp, J. Walter</p> <p>2017-04-01</p> <p>This study focuses on microphysical properties of <span class="hlt">ice</span> particles populating high <span class="hlt">ice</span> water content areas in Mesoscale Convective Systems (MCS). These clouds have been extensively sampled during the High Altitude <span class="hlt">Ice</span> Crystal - High <span class="hlt">Ice</span> Water Content international projects (HAIC-HIWC, Dezitter et al. 2013, Strapp et al. 2015) with the objective of characterizing <span class="hlt">ice</span> particle properties such as size distribution, radar reflectivity and <span class="hlt">ice</span> water content. The in-situ data collected during these campaigns at different temperature levels and in different type of MCS (oceanic, continental) make the HAIC-HIWC data set a unique opportunity to study <span class="hlt">ice</span> particle microphysical properties. Recently, a new approach to retrieve <span class="hlt">ice</span> particle <span class="hlt">mass</span> from in-situ measurements has been developed: a forward model that relates <span class="hlt">ice</span> particles' <span class="hlt">mass</span> to Particle Size Distribution (PSD) and <span class="hlt">Ice</span> Water Content (IWC) is formulated as a linear system of equations and the retrieval process consists in solving the inverse problem with numerical optimization tools (Coutris et al. 2016). In this study, this new method is applied to HAIC-HIWC data set and main outcomes are discussed. First, the method is compared to a classical power-law based method using data from one single flight performed in Darwin area on February, 7th 2014. The observed differences in retrieved quantities such as <span class="hlt">ice</span> particle <span class="hlt">mass</span>, <span class="hlt">ice</span> water content or median <span class="hlt">mass</span> diameter, highlight the potential benefit of abandoning the power law simplistic assumption. The method is then applied to data measured at different cloud temperatures ranging from -40°C to -10°C during several flights of both Darwin 2014 and Cayenne 2015 campaigns. Specific findings about <span class="hlt">ice</span> microphysical properties such as <span class="hlt">variations</span> of effective density with particle size and the influence of cloud temperature on particle effective density are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.G13B1099B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.G13B1099B"><span>Measuring Two Decades of <span class="hlt">Ice</span> <span class="hlt">Mass</span> Loss using GRACE and SLR</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bonin, J. A.; Chambers, D. P.</p> <p>2016-12-01</p> <p>We use Satellite Laser Ranging (SLR) to extend the time series of <span class="hlt">ice</span> <span class="hlt">mass</span> change back in time to 1994. The SLR series is of far lesser spatial resolution than GRACE, so we apply a constrained inversion technique to better localize the signal. We approximate the likely errors due to SLR's measurement errors combined with the inversion errors from using a low-resolution series, then estimate the interannual <span class="hlt">mass</span> change over Greenland and Antarctica.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.6251B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.6251B"><span>Quantifying <span class="hlt">ice</span> cliff contribution to debris-covered glacier <span class="hlt">mass</span> balance from multiple sensors</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brun, Fanny; Wagnon, Patrick; Berthier, Etienne; Kraaijenbrink, Philip; Immerzeel, Walter; Shea, Joseph; Vincent, Christian</p> <p>2017-04-01</p> <p><span class="hlt">Ice</span> cliffs on debris-covered glaciers have been recognized as a hot spot for glacier melt. <span class="hlt">Ice</span> cliffs are steep (even sometimes overhanging) and fast evolving surface features, which make them challenging to monitor. We surveyed the topography of Changri Nup Glacier (Nepalese Himalayas, Everest region) in November 2015 and 2016 using multiple sensors: terrestrial photogrammetry, Unmanned Aerial Vehicle (UAV) photogrammetry, Pléiades stereo images and ASTER stereo images. We derived 3D point clouds and digital elevation models (DEMs) following a Structure-from-Motion (SfM) workflow for the first two sets of data to monitor surface elevation changes and calculate the associated volume loss. We derived only DEMs for the two last data sets. The derived DEMs had resolutions ranging from < 5 cm to 30 m. The derived point clouds and DEMs are used to quantify the <span class="hlt">ice</span> melt of the cliffs at different scales. The very high resolution SfM point clouds, together with the surface velocity field, will be used to calculate the volume losses of 14 individual cliffs, depending on their size, aspect or the presence of supra glacial lake. Then we will extend this analysis to the whole glacier to quantify the contribution of <span class="hlt">ice</span> cliff melt to the overall glacier <span class="hlt">mass</span> balance, calculated with the UAV and Pléiades DEMs. This research will provide important tools to evaluate the role of <span class="hlt">ice</span> cliffs in regional <span class="hlt">mass</span> loss.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120010516','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120010516"><span>Greenland <span class="hlt">Ice</span> Sheet <span class="hlt">Mass</span> Balance: Distribution of Increased <span class="hlt">Mass</span> Loss with Climate Warming; 2003-07 Versus 1992-2002</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; Benner, Anita C.; Beckley, Matthew; Cornejo, Helen G.; DiMarzio, John; Giovinetto, Mario B.; Neumann, Thomas A.; Robbins, John; Saba, Jack L.; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20120010516'); toggleEditAbsImage('author_20120010516_show'); toggleEditAbsImage('author_20120010516_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20120010516_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20120010516_hide"></p> <p>2011-01-01</p> <p>We derive <span class="hlt">mass</span> changes of the Greenland <span class="hlt">ice</span> sheet (GIS) for 2003-07 from ICESat laser altimetry and compare them with results for 1992-2002 from ERS radar and airborne laser altimetry. The GIS continued to grow inland and thin at the margins during 2003 07, but surface melting and accelerated flow significantly increased the marginal thinning compared with the 1990s. The net balance changed from a small loss of 7 plus or minus 3 Gt a 1(sup -1) in the 1990s to 171 plus or minus 4 Gt a (sup -1) for 2003-07, contributing 0.5 mm a(sup -1) to recent global sea-level rise. We divide the derived <span class="hlt">mass</span> changes into two components: (1) from changes in melting and <span class="hlt">ice</span> dynamics and (2) from changes in precipitation and accumulation rate. We use our firn compaction model to calculate the elevation changes driven by changes in both temperature and accumulation rate and to calculate the appropriate density to convert the accumulation-driven changes to <span class="hlt">mass</span> changes. Increased losses from melting and <span class="hlt">ice</span> dynamics (17-206 Gt a(sup-1) are over seven times larger than increased gains from precipitation (10 35 Gt a(sup-1) during a warming period of approximately 2 K (10 a)(sup -1) over the GIS. Above 2000m elevation, the rate of gain decreased from 44 to 28 Gt a(sup-1), while below 2000m the rate of loss increased from 51 to 198 Gt a(sup-1). Enhanced thinning below the equilibrium line on outlet glaciers indicates that increased melting has a significant impact on outlet glaciers, as well as accelerating <span class="hlt">ice</span> flow. Increased thinning at higher elevations appears to be induced by dynamic coupling to thinning at the margins on decadal timescales.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AHEEM..64..115S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AHEEM..64..115S"><span>SPH Modelling of Sea-<span class="hlt">ice</span> Pack Dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Staroszczyk, Ryszard</p> <p>2017-12-01</p> <p>The paper is concerned with the problem of sea-<span class="hlt">ice</span> pack motion and deformation under the action of wind and water currents. Differential equations describing the dynamics of <span class="hlt">ice</span>, with its very distinct mateFfigrial responses in converging and diverging flows, express the <span class="hlt">mass</span> and linear momentum balances on the horizontal plane (the free surface of the ocean). These equations are solved by the fully Lagrangian method of smoothed particle hydrodynamics (SPH). Assuming that the <span class="hlt">ice</span> behaviour can be approximated by a non-linearly viscous rheology, the proposed SPH model has been used to simulate the evolution of a sea-<span class="hlt">ice</span> pack driven by wind drag stresses. The results of numerical simulations illustrate the evolution of an <span class="hlt">ice</span> pack, including <span class="hlt">variations</span> in <span class="hlt">ice</span> thickness and <span class="hlt">ice</span> area fraction in space and time. The effects of different initial <span class="hlt">ice</span> pack configurations and of different conditions assumed at the coast-<span class="hlt">ice</span> interface are examined. In particular, the SPH model is applied to a pack flow driven by a vortex wind to demonstrate how well the Lagrangian formulation can capture large deformations and displacements of sea <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110006429','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110006429"><span>Changes in the <span class="hlt">Mass</span> Balance of the Greenland <span class="hlt">Ice</span> Sheet in a Warming Climate During 2003-2009</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; Luthcke, Scott</p> <p>2010-01-01</p> <p><span class="hlt">Mass</span> changes of the Greenland <span class="hlt">ice</span> sheet (GIS) derived from ICESat and GRACE data both show that the net <span class="hlt">mass</span> loss from GIS during 2003-2009 is about 175 Gt/year, which contributes 0.5mm/yr global sea-level rise. The rate of <span class="hlt">mass</span> loss has increased significantly since the 1990's when the GIS was close to <span class="hlt">mass</span> balance. Even though the GIS was close to <span class="hlt">mass</span> balance during the 1990's, it was already showing characteristics of responding to8 warmer climate, specifically thinning at the margins and thickening inland at higher elevations. During 2003-2009, increased <span class="hlt">ice</span> thinning due to increases in melting and acceleration of outlet glaciers began to strongly exceed the inland thickening from increases in accumulation. Over the entire GIS, the <span class="hlt">mass</span> loss between the two periods, from increased melting and <span class="hlt">ice</span> dynamics, increased by about 190 Gt/year while the <span class="hlt">mass</span> gain, from increased precipitation and accumulation, increased by only about 15Gt/year. These <span class="hlt">ice</span> changes occurred during a time when the temperature on GIS changed at rate of about 2K/decade. The distribution of elevation and <span class="hlt">mass</span> changes derived from ICESat have high spatial resolution showing details over outlet glaciers, by drainage systems, and by elevation. However, information on the seasonal cycle of changes from ICESat data is limited, because the ICESat lasers were only operated during two to three campaigns per year of about 35 days duration each. In contrast, the temporal resolution of GRACE data, provided by the continuous data collection, is much better showing details of the seasonal cycle and the inter-annual variability. The differing sensitivity of the ICESat altimetry and the GRACE gravity methods to motion of the underlying bedrock from glacial isostatic adjustment (GIA) is used to evaluate the GIA corrections provided by models. The two data types are also combined to make estimates of the partitioning of the <span class="hlt">mass</span> gains and losses among accumulation, melting, and <span class="hlt">ice</span> discharge from outlet</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> <span class="hlt">mass</span> balance T in snow-<span class="hlt">ice</span>-ocean, T, SLP at surface ~1 year WHOI CRREL (SeaState DRI</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_9 --> <div id="page_10" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="181"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C53C0787S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C53C0787S"><span>Development of a multi-sensor elevation time series pole-ward of 86°S in support of altimetry validation and <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balance studies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Studinger, M.; Brunt, K. M.; Casey, K.; Medley, B.; Neumann, T.; Manizade, S.; Linkswiler, M. A.</p> <p>2015-12-01</p> <p>In order to produce a cross-calibrated long-term record of <span class="hlt">ice</span>-surface elevation change for input into <span class="hlt">ice</span> sheet models and <span class="hlt">mass</span> balance studies it is necessary to "link the measurements made by airborne laser altimeters, satellite measurements of ICESat, ICESat-2, and CryoSat-2" [<span class="hlt">Ice</span>Bridge Level 1 Science Requirements, 2012] and determine the biases and the spatial <span class="hlt">variations</span> between radar altimeters and laser altimeters using different wavelengths. The convergence zones of all ICESat tracks (86°S) and all ICESat-2 and CryoSat-2 tracks (88°S) are in regions of relatively low accumulation, making them ideal for satellite altimetry calibration. In preparation for ICESat-2 validation, the <span class="hlt">Ice</span>Bridge and ICESat-2 science teams have designed <span class="hlt">Ice</span>Bridge data acquisitions around 86°S and 88°S. Several aspects need to be considered when comparing and combining elevation measurements from different radar and laser altimeters, including: a) foot print size and spatial sampling pattern; b) accuracy and precision of each data sets; c) varying signal penetration into the snow; and d) changes in geodetic reference frames over time, such as the International Terrestrial Reference Frame (ITRF). The presentation will focus on the analysis of several <span class="hlt">Ice</span>Bridge flights around 86 and 88°S with the LVIS and ATM airborne laser altimeters and will evaluate the accuracy and precision of these data sets. To properly interpret the observed elevation change (dh/dt) as <span class="hlt">mass</span> change, however, the various processes that control surface elevation fluctuations must be quantified and therefore future work will quantify the spatial variability in snow accumulation rates pole-ward of 86°S and in particular around 88°S. Our goal is to develop a cross-validated multi-sensor time series of surface elevation change pole-ward of 86°S that, in combination with measured accumulation rates, will support ICESat-2 calibration and validation and <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balance studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.3654H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.3654H"><span>Post-glacial <span class="hlt">variations</span> of sea <span class="hlt">ice</span> cover and river discharge in the western Laptev Sea (Arctic Ocean) - a high-resolution study over the last 18 ka</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hörner, Tanja; Stein, Ruediger; Fahl, Kirsten</p> <p>2015-04-01</p> <p>Here, we provide a high-resolution reconstruction of sea-<span class="hlt">ice</span> cover <span class="hlt">variations</span> in the western Laptev Sea, a crucial area in terms of sea-<span class="hlt">ice</span> production in the Arctic Ocean and a region characterized by huge river discharge. Furthermore, the shallow Laptev Sea was strongly influenced by the post-glacial sea-level rise that should also be reflected in the sedimentary records. The sea <span class="hlt">Ice</span> Proxy IP25 (Highly-branched mono-isoprenoid produced by sea-<span class="hlt">ice</span> algae; Belt et al., 2007) was measured in two sediment cores from the western Laptev Sea (PS51/154, PS51/159) that offer a high-resolution composite record over the last 18 ka. In addition, sterols are applied as indicator for marine productivity (brassicasterol, dinosterol) and input of terrigenous organic matter by river discharge into the ocean (campesterol, ß-sitosterol). The sea-<span class="hlt">ice</span> cover varies distinctly during the whole time period and shows a general increase in the Late Holocene. A maximum in IP25 concentration can be found during the Younger Dryas. This sharp increase can be observed in the whole circumarctic realm (Chukchi Sea, Bering Sea, Fram Strait and Laptev Sea). Interestingly, there is no correlation between elevated numbers of <span class="hlt">ice</span>-rafted debris (IRD) interpreted as local <span class="hlt">ice</span>-cap expansions (Taldenkova et al. 2010), and sea <span class="hlt">ice</span> cover distribution. The transgression and flooding of the shelf sea that occurred over the last 16 ka in this region, is reflected by decreasing terrigenous (riverine) input, reflected in the strong decrease in sterol (ß-sitosterol and campesterol) concentrations. References Belt, S.T., <span class="hlt">Mass</span>é, G., Rowland, S.J., Poulin, M., Michel, C., LeBlanc, B., 2007. A novel chemical fossil of palaeo sea <span class="hlt">ice</span>: IP25. Organic Geochemistry 38 (1), 16e27. Taldenkova, E., Bauch, H.A., Gottschalk, J., Nikolaev, S., Rostovtseva, Yu., Pogodina, I., Ya, Ovsepyan, Kandiano, E., 2010. History of <span class="hlt">ice</span>-rafting and water <span class="hlt">mass</span> evolution at the northern Siberian continental margin (Laptev Sea) during Late</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.2621C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.2621C"><span>Retrieval of <span class="hlt">ice</span> crystals' <span class="hlt">mass</span> from <span class="hlt">ice</span> water content and particle distribution measurements: a numerical optimization approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Coutris, Pierre; Leroy, Delphine; Fontaine, Emmanuel; Schwarzenboeck, Alfons; Strapp, J. Walter</p> <p>2016-04-01</p> <p>A new method to retrieve cloud water content from in-situ measured 2D particle images from optical array probes (OAP) is presented. With the overall objective to build a statistical model of crystals' <span class="hlt">mass</span> as a function of their size, environmental temperature and crystal microphysical history, this study presents the methodology to retrieve the <span class="hlt">mass</span> of crystals sorted by size from 2D images using a numerical optimization approach. The methodology is validated using two datasets of in-situ measurements gathered during two airborne field campaigns held in Darwin, Australia (2014), and Cayenne, France (2015), in the frame of the High Altitude <span class="hlt">Ice</span> Crystals (HAIC) / High <span class="hlt">Ice</span> Water Content (HIWC) projects. During these campaigns, a Falcon F-20 research aircraft equipped with state-of-the art microphysical instrumentation sampled numerous mesoscale convective systems (MCS) in order to study dynamical and microphysical properties and processes of high <span class="hlt">ice</span> water content areas. Experimentally, an isokinetic evaporator probe, referred to as IKP-2, provides a reference measurement of the total water content (TWC) which equals <span class="hlt">ice</span> water content, (IWC) when (supercooled) liquid water is absent. Two optical array probes, namely 2D-S and PIP, produce 2D images of individual crystals ranging from 50 μm to 12840 μm from which particle size distributions (PSD) are derived. Mathematically, the problem is formulated as an inverse problem in which the crystals' <span class="hlt">mass</span> is assumed constant over a size class and is computed for each size class from IWC and PSD data: PSD.m = IW C This problem is solved using numerical optimization technique in which an objective function is minimized. The objective function is defined as follows: 2 J(m)=∥P SD.m - IW C ∥ + λ.R (m) where the regularization parameter λ and the regularization function R(m) are tuned based on data characteristics. The method is implemented in two steps. First, the method is developed on synthetic crystal populations in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940017861','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940017861"><span>Normalized vertical <span class="hlt">ice</span> <span class="hlt">mass</span> flux profiles from vertically pointing 8-mm-wavelength Doppler radar</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Orr, Brad W.; Kropfli, Robert A.</p> <p>1993-01-01</p> <p>During the FIRE 2 (First International Satellite Cloud Climatology Project Regional Experiment) project, NOAA's Wave Propagation Laboratory (WPL) operated its 8-mm wavelength Doppler radar extensively in the vertically pointing mode. This allowed for the calculation of a number of important cirrus cloud parameters, including cloud boundary statistics, cloud particle characteristic sizes and concentrations, and <span class="hlt">ice</span> <span class="hlt">mass</span> content (imc). The flux of imc, or, alternatively, <span class="hlt">ice</span> <span class="hlt">mass</span> flux (imf), is also an important parameter of a cirrus cloud system. <span class="hlt">Ice</span> <span class="hlt">mass</span> flux is important in the vertical redistribution of water substance and thus, in part, determines the cloud evolution. It is important for the development of cloud parameterizations to be able to define the essential physical characteristics of large populations of clouds in the simplest possible way. One method would be to normalize profiles of observed cloud properties, such as those mentioned above, in ways similar to those used in the convective boundary layer. The height then scales from 0.0 at cloud base to 1.0 at cloud top, and the measured cloud parameter scales by its maximum value so that all normalized profiles have 1.0 as their maximum value. The goal is that there will be a 'universal' shape to profiles of the normalized data. This idea was applied to estimates of imf calculated from data obtained by the WPL cloud radar during FIRE II. Other quantities such as median particle diameter, concentration, and <span class="hlt">ice</span> <span class="hlt">mass</span> content can also be estimated with this radar, and we expect to also examine normalized profiles of these quantities in time for the 1993 FIRE II meeting.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.3577P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.3577P"><span>Large-Ensemble modeling of past and future <span class="hlt">variations</span> of the Antarctic <span class="hlt">Ice</span> Sheet with a coupled <span class="hlt">ice</span>-Earth-sea level model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pollard, David; DeConto, Robert; Gomez, Natalya</p> <p>2016-04-01</p> <p>To date, most modeling of the Antarctic <span class="hlt">Ice</span> Sheet's response to future warming has been calibrated using recent and modern observations. As an alternate approach, we apply a hybrid 3-D <span class="hlt">ice</span> sheet-shelf model to the last deglacial retreat of Antarctica, making use of geologic data of the last ~20,000 years to test the model against the large-scale <span class="hlt">variations</span> during this period. The <span class="hlt">ice</span> model is coupled to a global Earth-sea level model to improve modeling of the bedrock response and to capture ocean-<span class="hlt">ice</span> gravitational interactions. Following several recent <span class="hlt">ice</span>-sheet studies, we use Large Ensemble (LE) statistical methods, performing sets of 625 runs from 30,000 years to present with systematically varying model parameters. Objective scores for each run are calculated using modern data and past reconstructed grounding lines, relative sea level records, cosmogenic elevation-age data and uplift rates. The LE results are analyzed to calibrate 4 particularly uncertain model parameters that concern marginal <span class="hlt">ice</span> processes and interaction with the ocean. LE's are extended into the future with climates following RCP scenarios. An additional scoring criterion tests the model's ability to reproduce estimated sea-level high stands in the warm mid-Pliocene, for which drastic retreat mechanisms of hydrofracturing and <span class="hlt">ice</span>-cliff failure are needed in the model. The LE analysis provides future sea-level-rise envelopes with well-defined parametric uncertainty bounds. Sensitivities of future LE results to Pliocene sea-level estimates, coupling to the Earth-sea level model, and vertical profiles of Earth properties, will be presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.C23B0613H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.C23B0613H"><span>Polar <span class="hlt">Ice</span> Caps: a Canary for 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>Honsaker, W.; Lowell, T. V.; Sagredo, E.; Kelly, M. A.; Hall, B. L.</p> <p>2010-12-01</p> <p><span class="hlt">Ice</span> caps are glacier <span class="hlt">masses</span> that are highly sensitive to climate change. Because of their hypsometry they can have a binary state. When relatively slight changes in the equilibrium line altitude (ELA) either intersect or rise above the land the <span class="hlt">ice</span> can become established or disappear. Thus these upland <span class="hlt">ice</span> <span class="hlt">masses</span> have a fast response time. Here we consider a way to extract the ELA signal from independent <span class="hlt">ice</span> caps adjacent to the Greenland <span class="hlt">Ice</span> Sheet margin. It may be that these <span class="hlt">ice</span> caps are sensitive trackers of climate change that also impact the <span class="hlt">ice</span> sheet margin. One example is the Istorvet <span class="hlt">Ice</span> Cap located in Liverpool Land, East Greenland (70.881°N, 22.156°W). The <span class="hlt">ice</span> cap topography and the underlying bedrock surface dips to the north, with peak elevation of the current <span class="hlt">ice</span> ranging in elevation from 1050 to 745 m.a.s.l. On the eastern side of the <span class="hlt">ice</span> <span class="hlt">mass</span> the outlet glaciers extending down to sea level. The western margin has several small lobes in topographic depressions, with the margin reaching down to 300 m.a.s.l. Topographic highs separate the <span class="hlt">ice</span> cap into at least 5 main catchments, each having a pair of outlet lobes toward either side of the <span class="hlt">ice</span> cap. Because of the regional bedrock slope each catchment has its own elevation range. Therefore, as the ELA changes it is possible for some catchments of the <span class="hlt">ice</span> cap to experience positive <span class="hlt">mass</span> balance while others have a negative balance. Based on weather observations we estimate the present day ELA to be ~1000 m.a.s.l, meaning <span class="hlt">mass</span> balance is negative for the majority of the <span class="hlt">ice</span> cap. By tracking glacier presence/absence in these different catchments, we can reconstruct small changes in the ELA. Another example is the High <span class="hlt">Ice</span> Cap (informal name) in Milne Land (70.903°N, 25.626°W, 1080 m), East Greenland. Here at least 4 unconformities in <span class="hlt">ice</span> layers found near the southern margin of the <span class="hlt">ice</span> cap record changing intervals of accumulation and ablation. Therefore, this location may also be sensitive to slight</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70074767','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70074767"><span>Climatic impact of glacial cycle polar motion: Coupled oscillations of <span class="hlt">ice</span> sheet <span class="hlt">mass</span> and rotation pole position</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Bills, Bruce G.; James, Thomas S.; Mengel, John G.</p> <p>1999-01-01</p> <p>Precessional motion of Earth's rotation axis relative to its orbit is a well-known source of long-period climatic <span class="hlt">variation</span>. It is less well appreciated that growth and decay of polar <span class="hlt">ice</span> sheets perturb the symmetry of the global <span class="hlt">mass</span> distribution enough that the geographic location of the rotation axis will change by at least 15 km and possibly as much as 100 km during a single glacial cycle. This motion of the pole will change the seasonal and latitudinal pattern of temperatures. We present calculations, based on a diurnal average energy balance, which compare the summer and winter temperature anomalies due to a 1° decrease in obliquity with those due to a 1° motion of the rotation pole toward Hudson Bay. Both effects result in peak temperature perturbations of about 1° Celsius. The obliquity change primarily influences the amplitude of the seasonal cycle, while the polar motion primarily changes the annual mean temperatures. The polar motion induced temperature anomaly is such that it will act as a powerful negative feedback on <span class="hlt">ice</span> sheet growth. We also explore the evolution of the coupled system composed of <span class="hlt">ice</span> sheet <span class="hlt">mass</span> and pole position. Oscillatory solutions result from the conflicting constraints of rotational and thermal stability. A positive <span class="hlt">mass</span> anomaly on an otherwise featureless Earth is in rotational equilibrium only at the poles or the equator. The two polar equilibria are rotationally unstable, and the equatorial equilibrium, though rotationally stable, is thermally unstable. We find that with a plausible choice for the strength of coupling between the thermal and rotational systems, relatively modest external forcing can produce significant response at periods of 104–106 years, but it strongly attenuates polar motion at longer periods. We suggest that these coupled oscillations may contribute to the observed dominance of 100 kyr glacial cycles since the mid-Pleistocene and will tend to stabilize geographic patterns that are suitable to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22525155-distinguishing-neutrino-mass-hierarchies-using-dark-matter-annihilation-signals-icecube','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22525155-distinguishing-neutrino-mass-hierarchies-using-dark-matter-annihilation-signals-icecube"><span>Distinguishing neutrino <span class="hlt">mass</span> hierarchies using dark matter annihilation signals at <span class="hlt">Ice</span>Cube</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>Allahverdi, Rouzbeh; Knockel, Bradley; Dutta, Bhaskar</p> <p>2015-12-01</p> <p>We explore the possibility of distinguishing neutrino <span class="hlt">mass</span> hierarchies through the neutrino signal from dark matter annihilation at neutrino telescopes. We consider a simple extension of the standard model where the neutrino <span class="hlt">masses</span> and mixing angles are obtained via the type-II seesaw mechanism as an explicit example. We show that future extensions of <span class="hlt">Ice</span>Cube neutrino telescope may detect the neutrino signal from DM annihilation at the Galactic Center and inside the Sun, and differentiate between the normal and inverted <span class="hlt">mass</span> hierarchies, in this model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015E%26PSL.430..427R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015E%26PSL.430..427R"><span>Modelling the feedbacks between <span class="hlt">mass</span> balance, <span class="hlt">ice</span> flow and debris transport to predict the response to climate change of debris-covered glaciers in the Himalaya</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rowan, Ann V.; Egholm, David L.; Quincey, Duncan J.; Glasser, Neil F.</p> <p>2015-11-01</p> <p>Many Himalayan glaciers are characterised in their lower reaches by a rock debris layer. This debris insulates the glacier surface from atmospheric warming and complicates the response to climate change compared to glaciers with clean-<span class="hlt">ice</span> surfaces. Debris-covered glaciers can persist well below the altitude that would be sustainable for clean-<span class="hlt">ice</span> glaciers, resulting in much longer timescales of <span class="hlt">mass</span> loss and meltwater production. The properties and evolution of supraglacial debris present a considerable challenge to understanding future glacier change. Existing approaches to predicting <span class="hlt">variations</span> in glacier volume and meltwater production rely on numerical models that represent the processes governing glaciers with clean-<span class="hlt">ice</span> surfaces, and yield conflicting results. We developed a numerical model that couples the flow of <span class="hlt">ice</span> and debris and includes important feedbacks between debris accumulation and glacier <span class="hlt">mass</span> balance. To investigate the impact of debris transport on the response of a glacier to recent and future climate change, we applied this model to a large debris-covered Himalayan glacier-Khumbu Glacier in Nepal. Our results demonstrate that supraglacial debris prolongs the response of the glacier to warming and causes lowering of the glacier surface in situ, concealing the magnitude of <span class="hlt">mass</span> loss when compared with estimates based on glacierised area. Since the Little <span class="hlt">Ice</span> Age, Khumbu Glacier has lost 34% of its volume while its area has reduced by only 6%. We predict a decrease in glacier volume of 8-10% by AD2100, accompanied by dynamic and physical detachment of the debris-covered tongue from the active glacier within the next 150 yr. This detachment will accelerate rates of glacier decay, and similar changes are likely for other debris-covered glaciers in the Himalaya.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28361871','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28361871"><span>A tipping point in refreezing accelerates <span class="hlt">mass</span> loss of Greenland's glaciers and <span class="hlt">ice</span> caps.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Noël, B; van de Berg, W J; Lhermitte, S; Wouters, B; Machguth, H; Howat, I; Citterio, M; Moholdt, G; Lenaerts, J T M; van den Broeke, M R</p> <p>2017-03-31</p> <p>Melting of the Greenland <span class="hlt">ice</span> sheet (GrIS) and its peripheral glaciers and <span class="hlt">ice</span> caps (GICs) contributes about 43% to contemporary sea level rise. While patterns of GrIS <span class="hlt">mass</span> loss are well studied, the spatial and temporal evolution of GICs <span class="hlt">mass</span> loss and the acting processes have remained unclear. Here we use a novel, 1 km surface <span class="hlt">mass</span> balance product, evaluated against in situ and remote sensing data, to identify 1997 (±5 years) as a tipping point for GICs <span class="hlt">mass</span> balance. That year marks the onset of a rapid deterioration in the capacity of the GICs firn to refreeze meltwater. Consequently, GICs runoff increases 65% faster than meltwater production, tripling the post-1997 <span class="hlt">mass</span> loss to 36±16 Gt -1 , or ∼14% of the Greenland total. In sharp contrast, the extensive inland firn of the GrIS retains most of its refreezing capacity for now, buffering 22% of the increased meltwater production. This underlines the very different response of the GICs and GrIS to atmospheric warming.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5380968','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5380968"><span>A tipping point in refreezing accelerates <span class="hlt">mass</span> loss of Greenland's glaciers and <span class="hlt">ice</span> caps</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Noël, B.; van de Berg, W. J; Lhermitte, S.; Wouters, B.; Machguth, H.; Howat, I.; Citterio, M.; Moholdt, G.; Lenaerts, J. T. M.; van den Broeke, M. R.</p> <p>2017-01-01</p> <p>Melting of the Greenland <span class="hlt">ice</span> sheet (GrIS) and its peripheral glaciers and <span class="hlt">ice</span> caps (GICs) contributes about 43% to contemporary sea level rise. While patterns of GrIS <span class="hlt">mass</span> loss are well studied, the spatial and temporal evolution of GICs <span class="hlt">mass</span> loss and the acting processes have remained unclear. Here we use a novel, 1 km surface <span class="hlt">mass</span> balance product, evaluated against in situ and remote sensing data, to identify 1997 (±5 years) as a tipping point for GICs <span class="hlt">mass</span> balance. That year marks the onset of a rapid deterioration in the capacity of the GICs firn to refreeze meltwater. Consequently, GICs runoff increases 65% faster than meltwater production, tripling the post-1997 <span class="hlt">mass</span> loss to 36±16 Gt−1, or ∼14% of the Greenland total. In sharp contrast, the extensive inland firn of the GrIS retains most of its refreezing capacity for now, buffering 22% of the increased meltwater production. This underlines the very different response of the GICs and GrIS to atmospheric warming. PMID:28361871</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017NatCo...814730N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017NatCo...814730N"><span>A tipping point in refreezing accelerates <span class="hlt">mass</span> loss of Greenland's 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>Noël, B.; van de Berg, W. J.; Lhermitte, S.; Wouters, B.; Machguth, H.; Howat, I.; Citterio, M.; Moholdt, G.; Lenaerts, J. T. M.; van den Broeke, M. R.</p> <p>2017-03-01</p> <p>Melting of the Greenland <span class="hlt">ice</span> sheet (GrIS) and its peripheral glaciers and <span class="hlt">ice</span> caps (GICs) contributes about 43% to contemporary sea level rise. While patterns of GrIS <span class="hlt">mass</span> loss are well studied, the spatial and temporal evolution of GICs <span class="hlt">mass</span> loss and the acting processes have remained unclear. Here we use a novel, 1 km surface <span class="hlt">mass</span> balance product, evaluated against in situ and remote sensing data, to identify 1997 (+/-5 years) as a tipping point for GICs <span class="hlt">mass</span> balance. That year marks the onset of a rapid deterioration in the capacity of the GICs firn to refreeze meltwater. Consequently, GICs runoff increases 65% faster than meltwater production, tripling the post-1997 <span class="hlt">mass</span> loss to 36+/-16 Gt-1, or ~14% of the Greenland total. In sharp contrast, the extensive inland firn of the GrIS retains most of its refreezing capacity for now, buffering 22% of the increased meltwater production. This underlines the very different response of the GICs and GrIS to atmospheric warming.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20010002431&hterms=BALANCE+SHEET&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DBALANCE%2BSHEET','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20010002431&hterms=BALANCE+SHEET&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DBALANCE%2BSHEET"><span>Troughs on Martian <span class="hlt">Ice</span> Sheets: Analysis of Their Closure and <span class="hlt">Mass</span> Balance</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fountain, A.; Kargel, J.; Lewis, K.; MacAyeal, D.; Pfeffer, T.; Zwally, J.</p> <p>2000-01-01</p> <p>At the Copenhagen workshop on Martian polar processes, Ralf Greve commented that the flow regime surrounding scarps and troughs of the Martian polar <span class="hlt">ice</span> sheets cannot be modeled using traditional "plan view" <span class="hlt">ice</span>-sheet models. Such models are inadequate because they typically use reduced equations that embody certain simplifications applicable only to terrestrial <span class="hlt">ice</span> sheets where the upper <span class="hlt">ice</span> sheet surface is smooth. In response to this suggestion, we have constructed a 2-dimensional, time dependent "side view" (two spatial dimensions: one horizontal, one vertical) model of scarp closure that is designed to overcome the difficulties described by Greve. The purpose of the model is to evaluate the scales of stress <span class="hlt">variation</span> and styles of flow closure so as to estimate errors that may be encountered by "plan view" models. We show that there may be avenues whereby the complications associated with scarp closure can be overcome in "plan view" models through appropriate parameterizations of 3-dimensional effects. Following this, we apply the flow model to simulate the evolution of a typical scarp on the North Polar Cap of Mars. Our simulations investigate: (a) the role of "radiation trapping" (see our companion abstract) in creating and maintaining "spiral-like" scarps on the <span class="hlt">ice</span> sheet, (b) the consequences of different flowlaws and <span class="hlt">ice</span> compositions on scarp evolution and, in particular, scarp age, and (c) the role of dust and debris in scarp evolution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/7146760-glacioclimatological-study-perennial-ice-fuji-ice-cave-japan-part-seasonal-variation-mechanism-maintenance','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/7146760-glacioclimatological-study-perennial-ice-fuji-ice-cave-japan-part-seasonal-variation-mechanism-maintenance"><span>Glacioclimatological study of Perennial <span class="hlt">Ice</span> in the Fuji <span class="hlt">Ice</span> Cave, Japan. Part I. Seasonal <span class="hlt">variation</span> and mechanism of maintenance</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>Ohata, Tetsuo; Furukawa, Teruo; Higuchi, Keiji</p> <p>1994-08-01</p> <p>Perennial cave <span class="hlt">ice</span> in a cave located at Mt. Fuji in central Japan was studied to investigate the basic characteristics and the cause for existence of such <span class="hlt">ice</span> under warm ground-level climate considering the <span class="hlt">ice</span> cave as a thermal and hydrological system. Fuji <span class="hlt">Ice</span> Cave is a lava tube cave 150 m in length with a collapsed part at the entrance. Measurements from 1984 to 1986 showed that the surface-level change of floor <span class="hlt">ice</span> occurred due to freezing and melting at the surface and that melting at the bottom of the <span class="hlt">ice</span> was negligible. The annual amplitude of change inmore » surface level was larger near the entrance. Meterological data showed that the cold air inflow to the cave was strong in winter, but in summer the cave was maintained near 0[degrees]C with only weak inflow of warm air. The predominant wind system was from the entrance to the interior in both winter and summer, but the spatial scale of the wind system was different. Heat budget consideration of the cave showed that the largest component was the strong inflow of subzero dry air <span class="hlt">mass</span> in winter. Cooling in winter was compensated for by summer inflow of warm air, heat transport from the surrounding ground layer, and loss of sensible heat due to cooling of the cave for the observed year. Strong inflow of cold air and weak inflow of warm air, which is extremely low compared to the ground level air, seemed to be the most important condition. Thus the thermal condition of the cave is quasi-balanced at the presence condition below 0[degrees]C with <span class="hlt">ice</span>. It can be said that the interrelated result of the climatological and special structural conditions makes this cave very cold, and allows perennial <span class="hlt">ice</span> to exist in the cave. Other climatological factors such as precipitation seem to be minor factors. 17 refs., 3 figs., 3 tabs.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA112819','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA112819"><span>Breakup of Solid <span class="hlt">Ice</span> Covers Due to Rapid Water Level <span class="hlt">Variations</span>,</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1982-02-01</p> <p>Larsen, and Dr. Devinder S. Sodhi for their valuable comments and reviews of the report. He also thanks Dr. Ashton and Guenther E. Frankenstein for the...for wave periods larger than about 10 seconds. What are the minimum wave lengths that might be generated by discharge <span class="hlt">variations</span> at a hydro- electric ...Canadian Electrical Association, Research and Development, Suite 580, One Westmount Square, Montreal, Canada. 2. Ashton, G.D. (1974a) Entrainment of <span class="hlt">ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.7457N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.7457N"><span>Quantifying the <span class="hlt">mass</span> loss of peripheral Greenland glaciers and <span class="hlt">ice</span> caps (1958-2014).</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; van den Broeke, Michiel</p> <p>2016-04-01</p> <p>Since the 2000s, <span class="hlt">mass</span> loss from Greenland peripheral glaciers and <span class="hlt">ice</span> caps (GICs) has accelerated, becoming an important contributor to sea level rise. Under continued warming throughout the 21st century, GICs might yield up to 7.5 to 11 mm sea level rise, with increasing dominance of surface runoff at the expense of <span class="hlt">ice</span> discharge. However, despite multiple observation campaigns, little remains known about the contribution of GICs to total Greenland <span class="hlt">mass</span> loss. Furthermore, the relatively coarse resolutions in regional climate models, i.e. 5 km to 20 km, fail to represent the small scale patterns of surface <span class="hlt">mass</span> balance (SMB) components over these topographically complex regions including also narrow valley glaciers. Here, we present a novel approach to quantify the contribution of GICs to surface melt and runoff, based on an elevation dependent downscaling method. GICs daily SMB components at 1 km resolution are obtained by statistically downscaling the outputs of RACMO2.3 at 11 km resolution to a down-sampled version of the GIMP DEM for the period 1958-2014. This method has recently been successfully validated over the Greenland <span class="hlt">ice</span> sheet and is now applied to GICs. In this study, we first evaluate the 1 km daily downscaled GICs SMB against a newly available and comprehensive dataset of ablation stake measurements. Then, we investigate present-day trends of meltwater production and SMB for different regions and estimate GICs contribution to total Greenland <span class="hlt">mass</span> loss. These data are considered valuable for model evaluation and prediction of future sea level rise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.C21D0669C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.C21D0669C"><span>Spatial and temporal patterns of sea <span class="hlt">ice</span> <span class="hlt">variations</span> in Vilkitsky strait, Russian High Arctic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ci, T.; Cheng, X.; Hui, F.</p> <p>2013-12-01</p> <p>The Arctic Ocean has been greatly affected by climate change. Future predications show an even more drastic reduction of the <span class="hlt">ice</span> cap which will open new areas for the exploration of natural resources and maritime transportation.Shipping through the Arctic Ocean via the Northern Sea Route (NSR) could save about 40% of the sailing distance from Asia (Yokohama) to Europe (Rotterdam) compared to the traditional route via the Suez Canal. Vilkitsky strait is the narrowest and northest portion of the Northern Sea Route with heaviest traffic between the Taimyr Peninsular and the Severnaya Zemlya archipelago. The preliminary results of sea <span class="hlt">ice</span> <span class="hlt">variations</span> are presented by using moderate-resolution imaging spectro radiometer(MODIS) data with 250-m resolution in the Vilkitsky strait during 2009-2012. Temporally, the first rupture on sea <span class="hlt">ice</span> in Vilkitsky strait usually comes up in April and sea <span class="hlt">ice</span> completely break into pieces in early June. The strait would be <span class="hlt">ice</span>-free between August and late September. The frequency of <span class="hlt">ice</span> floes grows while temperature falls down in October. There are always one or two months suitable for transport. Spatially, Sea <span class="hlt">ice</span> on Laptev sea side breaks earlier than that of Kara sea side while sea <span class="hlt">ice</span> in central of strait breaks earlier than in shoreside. The phenomena are directly related with the direction of sea wind and ocean current. In summmary, study on Spatial and temporal patterns in this area is significant for the NSR. An additional research issue to be tackled is to seeking the trends of <span class="hlt">ice</span>-free duration in the context of global warming. Envisat ASAR data will also be used in this study.</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 <span class="hlt">mass</span> 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 <span class="hlt">mass</span> balance during the retreat of the Laurentide <span class="hlt">Ice</span> Sheet.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Sci...358..781M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Sci...358..781M"><span>Cordilleran <span class="hlt">Ice</span> Sheet <span class="hlt">mass</span> loss preceded climate reversals near the Pleistocene Termination</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Menounos, B.; Goehring, B. M.; Osborn, G.; Margold, M.; Ward, B.; Bond, J.; Clarke, G. K. C.; Clague, J. J.; Lakeman, T.; Koch, J.; Caffee, M. W.; Gosse, J.; Stroeven, A. P.; Seguinot, J.; Heyman, J.</p> <p>2017-11-01</p> <p>The Cordilleran <span class="hlt">Ice</span> Sheet (CIS) once covered an area comparable to that of Greenland. Previous geologic evidence and numerical models indicate that the <span class="hlt">ice</span> sheet covered much of westernmost Canada as late as 12.5 thousand years ago (ka). New data indicate that substantial areas throughout westernmost Canada were <span class="hlt">ice</span> free prior to 12.5 ka and some as early as 14.0 ka, with implications for climate dynamics and the timing of meltwater discharge to the Pacific and Arctic oceans. Early Bølling-Allerød warmth halved the <span class="hlt">mass</span> of the CIS in as little as 500 years, causing 2.5 to 3.0 meters of sea-level rise. Dozens of cirque and valley glaciers, along with the southern margin of the CIS, advanced into recently deglaciated regions during the Bølling-Allerød and Younger Dryas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C33D1236L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C33D1236L"><span>Geodetic <span class="hlt">mass</span> balance measurements on debris and clean-<span class="hlt">ice</span> tropical glaciers in Ecuador</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>La Frenierre, J.; Decker, C. R.; Jordan, E.; Wigmore, O.; Hodge, B. E.; Niederriter, C.; Michels, A.</p> <p>2017-12-01</p> <p>Glaciers are recognized as highly sensitive indicators of climate change in high altitude, low latitude environments. In the tropical Andes, various analyses of glacier surface area change have helped illuminate the manifestation of climate change in this region, however, information about actual glacier <span class="hlt">mass</span> balance behavior is much more limited given the relatively small glaciers, difficult access, poor weather, and/or limited local resources common here. Several new technologies, including aerial and terrestrial LIDAR and structure-from-motion photogrammetry using small unmanned aerial vehicles (UAVs), make <span class="hlt">mass</span> balance measurements using geodetic approaches increasingly feasible in remote mountain locations, which can both further our understanding of changing climatic conditions, and improve our ability to evaluate the downstream hydrologic impacts of <span class="hlt">ice</span> loss. At Volcán Chimborazo, Ecuador, these new technologies, combined with a unique, 5-meter resolution digital elevation model derived from 1997 aerial imagery, make possible an analysis of the magnitude and spatial patterns of <span class="hlt">mass</span> balance behavior over the past two decades. Here, we evaluate <span class="hlt">ice</span> loss between 1997 and 2017 at the tongues of two adjacent glaciers, one debris-covered and detached from its accumulation area (Reschreiter Glacier), and one debris-free and intact (Hans Meyer Glacier). Additionally, we incorporate data from 2012 and 2013 terrestrial LIDAR surveys to evaluate the behavior of the Reschreiter at a finer temporal resolution. We find that on the Hans Meyer, the mean surface deflation rate since 1997 at the present-day tongue has been nearly 3 m yr-1, while on the lower-elevation Reschreiter, the mean deflation rate has been approximately 1 m yr-1. However, the processes by which debris-covered <span class="hlt">ice</span> becomes exposed results in highly heterogeneous patterns of <span class="hlt">ice</span> loss, with some areas experiencing surface deflation rates approaching 15 m yr-1 when energy absorption is unimpeded.</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/2017EGUGA..19.4898V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.4898V"><span>Reconstruction of past equilibrium line altitude using <span class="hlt">ice</span> extent data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Visnjevic, Vjeran; Herman, Frederic; Podladchikov, Yuri</p> <p>2017-04-01</p> <p>With the end of the Last Glacial Maximum (LGM), about 20 000 years ago, ended the most recent long-lasting cold phase in Earth's history. This last glacial advance left a strong observable imprint on the landscape, such as abandoned moraines, trimlines and other glacial geomorphic features. These features provide a valuable record of past continental climate. In particular, terminal moraines reflect the extent of glaciers and <span class="hlt">ice</span>-caps, which itself reflects past temperature and precipitation conditions. Here we present an inverse approach, based on a Tikhonov regularization, we have recently developed to reconstruct the LGM <span class="hlt">mass</span> balance from observed <span class="hlt">ice</span> extent data. The <span class="hlt">ice</span> flow model is developed using the shallow <span class="hlt">ice</span> approximation and solved explicitly using Graphical Processing Units (GPU). The <span class="hlt">mass</span> balance field, b, is the constrained variable defined by the <span class="hlt">ice</span> surface S, balance rate β and the spatially variable equilibrium line altitude field (ELA): b = min (β ṡ(S(x,y)- ELA (x,y)),c). (1) where c is a maximum accumulation rate. We show that such a <span class="hlt">mass</span> balance, and thus the spatially variable ELA field, can be inferred from the observed past <span class="hlt">ice</span> extent and <span class="hlt">ice</span> thickness at high resolution and very efficiently. The GPU implementation allows us solve one 1024x1024 grid points forward model run under 0.5s, which significantly reduces the time needed for our inverse method to converge. We start with synthetic test to demonstrate the method. We then apply the method to LGM <span class="hlt">ice</span> extents of South Island of New Zealand, the Patagonian Andes, where we can see a clear influence of Westerlies on the ELA, and the European Alps. These examples show that the method is capable of constraining spatial <span class="hlt">variations</span> in <span class="hlt">mass</span> balance at the scale of a mountain range, and provide us with information on past continental climate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C51E..07C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C51E..07C"><span>Investigation of Controls on <span class="hlt">Ice</span> Dynamics in Northeast Greenland from <span class="hlt">Ice</span>-Thickness Change Record Using <span class="hlt">Ice</span> Sheet System Model (ISSM)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Csatho, B. M.; Larour, E. Y.; Schenk, A. F.; Schlegel, N.; Duncan, K.</p> <p>2015-12-01</p> <p>We present a new, complete <span class="hlt">ice</span> thickness change reconstruction of the NE sector of the Greenland <span class="hlt">Ice</span> Sheet for 1978-2014, partitioned into changes due to surface processes and <span class="hlt">ice</span> dynamics. Elevation changes are computed from all available stereoscopic DEMs, and laser altimetry data (ICESat, ATM, LVIS). Surface <span class="hlt">Mass</span> Balance and firn-compaction estimates are from RACMO2.3. Originating nearly at the divide of the Greenland <span class="hlt">Ice</span> Sheet (GrIS), the dynamically active North East <span class="hlt">Ice</span> Stream (NEGIS) is capable of rapidly transmitting <span class="hlt">ice</span>-marginal forcing far inland. Thus, NEGIS provides a possible mechanism for a rapid drawdown of <span class="hlt">ice</span> from the <span class="hlt">ice</span> sheet interior as marginal warming, thinning and retreat continues. Our altimetry record shows accelerating dynamic thinning of Zachariæ Isstrom, initially limited to the deepest part of the fjord near the calving front (1978-2000) and then extending at least 75 km inland. At the same time, changes over the Nioghalvfjerdsfjorden (N79) Glacier are negligible. We also detect localized large dynamic changes at higher elevations on the <span class="hlt">ice</span> sheet. These thickness changes, often occurring at the onset of fast flow, could indicate rapid <span class="hlt">variations</span> of basal lubrication due to rerouting of subglacial drainage. We investigate the possible causes of the observed spatiotemporal pattern of <span class="hlt">ice</span> sheet elevation changes using the <span class="hlt">Ice</span> Sheet System Model (ISSM). This work build on our previous studies examining the sensitivity of <span class="hlt">ice</span> flow within the Northeast Greenland <span class="hlt">Ice</span> Stream (NEGIS) to key fields, including <span class="hlt">ice</span> viscosity, basal drag. We assimilate the new altimetry record into ISSM to improve the reconstruction of basal friction and <span class="hlt">ice</span> viscosity. Finally, airborne geophysical (gravity, magnetic) and <span class="hlt">ice</span>-penetrating radar data is examined to identify the potential geologic controls on the <span class="hlt">ice</span> thickness change pattern. Our study provides the first comprehensive reconstruction of <span class="hlt">ice</span> thickness changes for the entire NEGIS drainage basin during</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C51B0979M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C51B0979M"><span>Using a Vertically Integrated Model to Determine the Effects of Seasonal Forcing on the Basal Topography of <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>MacMackin, C. T.; Wells, A.</p> <p>2017-12-01</p> <p>While relatively small in <span class="hlt">mass</span>, <span class="hlt">ice</span> shelves play an important role in buttressing <span class="hlt">ice</span> sheets, slowing their flow into the ocean. As such, an understanding of <span class="hlt">ice</span> shelf stability is needed for predictions of future sea level rise. Networks of channels have been observed underneath Antarctic <span class="hlt">ice</span> shelves and are thought to affect their stability. While the origins of channels running parallel to <span class="hlt">ice</span> flow are thought to be well understood, transverse channels have also been observed and the mechanism for their formation is less clear. It has been suggested that seasonal <span class="hlt">variations</span> in <span class="hlt">ice</span> and ocean properties could be a source and we run nonlinear, vertically integrated 1-D simulations of a coupled <span class="hlt">ice</span> shelf and plume to test this hypothesis. We also examine how these <span class="hlt">variations</span> might alter the shape of internal radar reflectors within the <span class="hlt">ice</span>, suggesting a new technique to model their distribution using a vertically integrated model of <span class="hlt">ice</span> flow. We examine a range of sources for seasonal forcing which might lead to channel formation, finding that variability in subglacial discharge results in small <span class="hlt">variations</span> of <span class="hlt">ice</span> thickness. Additional mechanisms would be required to expand these into large transverse channels.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3950934','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3950934"><span>IR-MALDESI <span class="hlt">MASS</span> SPECTROMETRY IMAGING OF BIOLOGICAL TISSUE SECTIONS USING <span class="hlt">ICE</span> AS A MATRIX</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Robichaud, Guillaume; Barry, Jeremy A.; Muddiman, David C.</p> <p>2014-01-01</p> <p>Infrared Matrix-Assisted Laser Desorption Electrospray Ionization (IR-MALDESI) <span class="hlt">Mass</span> Spectrometry imaging of biological tissue sections using a layer of deposited <span class="hlt">ice</span> as an energy absorbing matrix was investigated. Dynamics of plume ablation were first explored using a nanosecond exposure shadowgraphy system designed to simultaneously collect pictures of the plume with a camera and collect the FT-ICR <span class="hlt">mass</span> spectrum corresponding to that same ablation event. Ablation of fresh tissue analyzed with and without using <span class="hlt">ice</span> as a matrix were both compared using this technique. Effect of spot-to-spot distance, number of laser shots per pixel and tissue condition (matrix) on ion abundance was also investigated for 50 µm thick tissue sections. Finally, the statistical method called design of experiments was used to compare source parameters and determine the optimal conditions for IR-MALDESI of tissue sections using deposited <span class="hlt">ice</span> as a matrix. With a better understanding of the fundamentals of ablation dynamics and a systematic approach to explore the experimental space, it was possible to improve ion abundance by nearly one order of magnitude. PMID:24385399</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.C11D0699A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.C11D0699A"><span>Programme for Monitoring of the Greenland <span class="hlt">Ice</span> Sheet - <span class="hlt">Ice</span> Surface Velocities</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Andersen, S. B.; Ahlstrom, A. P.; Boncori, J. M.; Dall, J.</p> <p>2011-12-01</p> <p>In 2007, the Danish Ministry of Climate and Energy launched the Programme for Monitoring of the Greenland <span class="hlt">Ice</span> Sheet (PROMICE) as an ongoing effort to assess changes in the <span class="hlt">mass</span> budget of the Greenland <span class="hlt">Ice</span> Sheet. Iceberg calving from the outlet glaciers of the Greenland <span class="hlt">Ice</span> Sheet, often termed the <span class="hlt">ice</span>-dynamic <span class="hlt">mass</span> loss, is responsible for an important part of the <span class="hlt">mass</span> loss during the last decade. To quantify this part of the <span class="hlt">mass</span> loss, we combine airborne surveys yielding <span class="hlt">ice</span>-sheet thickness along the entire margin, with surface velocities derived from satellite synthetic-aperture radar (SAR). In order to derive <span class="hlt">ice</span> sheet surface velocities from SAR a processing chain has been developed for GEUS by DTU Space based on a commercial software package distributed by GAMMA Remote Sensing. The processor, named SUSIE (Scripts and Utilities for SAR <span class="hlt">Ice</span>-motion Estimation), can use both differential SAR interferometry and offset-tracking techniques to measure the horizontal velocity components, providing also an estimate of the corresponding measurement error. So far surface velocities have been derived for a number of sites including Nioghalvfjerdsfjord Glacier, the Kangerlussuaq region, the Nuuk region, Helheim Glacier and Daugaard-Jensen Glacier using data from ERS-1/ERS-2, ENVISAT ASAR and ALOS Palsar. Here we will present these first results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3917821','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3917821"><span><span class="hlt">Ice</span> hockey lung – a case of <span class="hlt">mass</span> nitrogen dioxide poisoning in the Czech Republic</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Brat, Kristian; Merta, Zdenek; Plutinsky, Marek; Skrickova, Jana; Ing, Miroslav Stanek</p> <p>2013-01-01</p> <p>Nitrogen dioxide (NO2) is a toxic gas, a product of combustion in malfunctioning <span class="hlt">ice</span>-resurfacing machines. NO2 poisoning is rare but potentially lethal. The authors report a case of <span class="hlt">mass</span> NO2 poisoning involving 15 amateur <span class="hlt">ice</span> hockey players in the Czech Republic. All players were treated in the Department of Respiratory Diseases at Brno University Hospital in November 2010 – three as inpatients because they developed pneumonitis. All patients were followed-up until November 2011. Complete recovery in all but one patient was achieved by December 2010. None of the 15 patients developed asthma-like disease or chronic cough. Corticosteroids appeared to be useful in treatment. Electric-powered <span class="hlt">ice</span>-resurfacing machines are preferable in indoor <span class="hlt">ice</span> skating arenas. PMID:24032121</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 <span class="hlt">variation</span> 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 <span class="hlt">variation</span> 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/2017EGUGA..1912332S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1912332S"><span>Geodetic glacier <span class="hlt">mass</span> balancing on <span class="hlt">ice</span> caps - inseparably connected to firn modelling?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Saß, Björn L.; Sauter, Tobias; Seehaus, Thorsten; Braun, Matthias H.</p> <p>2017-04-01</p> <p>Observed melting of glaciers and <span class="hlt">ice</span> caps in the polar regions contribute to the ongoing global sea level rise (SLR). A rising sea level and its consequences are one of the major challenges for coastal societies in the next decades to centuries. Gaining knowledge about the main drivers of SLR and bringing it together is one recent key-challenge for environmental science. The high arctic Svalbard archipelago faced a strong climatic change in the last decades, associated with a change in the cryosphere. Vestfonna, a major Arctic <span class="hlt">ice</span> cap in the north east of Svalbard, harbors land and marine terminating glaciers, which expose a variability of behavior. We use high resolution remote sensing data from space-borne radar (TanDEM-X, TerraSAR-X, Sentinel-1a), acquired between 2009 and 2015, to estimate glacier velocity and high accurate surface elevation changes. For DEM registration we use space-borne laser altimetry (ICESat) and an existing in-situ data archive (IPY Kinnvika). In order to separate individual glacier basin changes for a detailed <span class="hlt">mass</span> balance study and for further SLR contribution estimates, we use glacier outlines from the Global Land <span class="hlt">Ice</span> Measurements from Space (GLIMS) project. Remaining challenges of space-borne observations are the reduction of measurement uncertainties, in the case of Synthetic Aperture Radar most notably signal penetration into the glacier surface. Furthermore, in order to convert volume to <span class="hlt">mass</span> change one has to use the density of the changed <span class="hlt">mass</span> (conversion factor) and one has to account for the <span class="hlt">mass</span> conservation processes in the firn package (firn compaction). Both, the conversion factor and the firn compaction are not (yet) measurable for extensive <span class="hlt">ice</span> bodies. They have to be modelled by coupling point measurements and regional gridded climate data. Results indicate a slight interior thickening contrasted with wide spread thinning in the ablation zone of the marine terminating outlets. While one glacier system draining to the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018QSRv..189....1M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018QSRv..189....1M"><span>Reconciling records of <span class="hlt">ice</span> streaming and <span class="hlt">ice</span> margin retreat to produce a palaeogeographic reconstruction of the deglaciation of the Laurentide <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Margold, Martin; Stokes, Chris R.; Clark, Chris D.</p> <p>2018-06-01</p> <p>This paper reconstructs the deglaciation of the Laurentide <span class="hlt">Ice</span> Sheet (LIS; including the Innuitian <span class="hlt">Ice</span> Sheet) from the Last Glacial Maximum (LGM), with a particular focus on the spatial and temporal <span class="hlt">variations</span> in <span class="hlt">ice</span> streaming and the associated changes in flow patterns and <span class="hlt">ice</span> divides. We build on a recent inventory of Laurentide <span class="hlt">ice</span> streams and use an existing <span class="hlt">ice</span> margin chronology to produce the first detailed transient reconstruction of the <span class="hlt">ice</span> stream drainage network in the LIS, which we depict in a series of palaeogeographic maps. Results show that the drainage network at the LGM was similar to modern-day Antarctica. The majority of the <span class="hlt">ice</span> streams were marine terminating and topographically-controlled and many of these continued to function late into the deglaciation, until the <span class="hlt">ice</span> sheet lost its marine margin. <span class="hlt">Ice</span> streams with a terrestrial <span class="hlt">ice</span> margin in the west and south were more transient and <span class="hlt">ice</span> flow directions changed with the build-up, peak-phase and collapse of the Cordilleran-Laurentide <span class="hlt">ice</span> saddle. The south-eastern marine margin in Atlantic Canada started to retreat relatively early and some of the <span class="hlt">ice</span> streams in this region switched off at or shortly after the LGM. In contrast, the <span class="hlt">ice</span> streams draining towards the north-western and north-eastern marine margins in the Beaufort Sea and in Baffin Bay appear to have remained stable throughout most of the Late Glacial, and some of them continued to function until after the Younger Dryas (YD). The YD influenced the dynamics of the deglaciation, but there remains uncertainty about the response of the <span class="hlt">ice</span> sheet in several sectors. We tentatively ascribe the switching-on of some major <span class="hlt">ice</span> streams during this period (e.g. M'Clintock Channel <span class="hlt">Ice</span> Stream at the north-west margin), but for other large <span class="hlt">ice</span> streams whose timing partially overlaps with the YD, the drivers are less clear and <span class="hlt">ice</span>-dynamical processes, rather than effects of climate and surface <span class="hlt">mass</span> balance are viewed as more likely drivers. Retreat</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22253455-novel-two-step-laser-ablation-ionization-mass-spectrometry-laims-actor-spectator-ice-layers-probing-chemical-composition-sub-ice-beneath-sub-ice-layer','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22253455-novel-two-step-laser-ablation-ionization-mass-spectrometry-laims-actor-spectator-ice-layers-probing-chemical-composition-sub-ice-beneath-sub-ice-layer"><span>Novel two-step laser ablation and ionization <span class="hlt">mass</span> spectrometry (2S-LAIMS) of actor-spectator <span class="hlt">ice</span> layers: Probing chemical composition of D{sub 2}O <span class="hlt">ice</span> beneath a H{sub 2}O <span class="hlt">ice</span> layer</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, Rui, E-mail: ryang73@ustc.edu; Gudipati, Murthy S., E-mail: gudipati@jpl.nasa.gov</p> <p>2014-03-14</p> <p>In this work, we report for the first time successful analysis of organic aromatic analytes imbedded in D{sub 2}O <span class="hlt">ices</span> by novel infrared (IR) laser ablation of a layered non-absorbing D{sub 2}O <span class="hlt">ice</span> (spectator) containing the analytes and an ablation-active IR-absorbing H{sub 2}O <span class="hlt">ice</span> layer (actor) without the analyte. With these studies we have opened up a new method for the in situ analysis of solids containing analytes when covered with an IR laser-absorbing layer that can be resonantly ablated. This soft ejection method takes advantage of the tenability of two-step infrared laser ablation and ultraviolet laser ionization <span class="hlt">mass</span> spectrometry,more » previously demonstrated in this lab to study chemical reactions of polycyclic aromatic hydrocarbons (PAHs) in cryogenic <span class="hlt">ices</span>. The IR laser pulse tuned to resonantly excite only the upper H{sub 2}O <span class="hlt">ice</span> layer (actor) generates a shockwave upon impact. This shockwave penetrates the lower analyte-containing D{sub 2}O <span class="hlt">ice</span> layer (spectator, a non-absorbing <span class="hlt">ice</span> that cannot be ablated directly with the wavelength of the IR laser employed) and is reflected back, ejecting the contents of the D{sub 2}O layer into the vacuum where they are intersected by a UV laser for ionization and detection by a time-of-flight <span class="hlt">mass</span> spectrometer. Thus, energy is transmitted from the laser-absorbing actor layer into the non-absorbing spectator layer resulting its ablation. We found that isotope cross-contamination between layers was negligible. We also did not see any evidence for thermal or collisional chemistry of PAH molecules with H{sub 2}O molecules in the shockwave. We call this “shockwave mediated surface resonance enhanced subsurface ablation” technique as “two-step laser ablation and ionization <span class="hlt">mass</span> spectrometry of actor-spectator <span class="hlt">ice</span> layers.” This method has its roots in the well-established MALDI (matrix assisted laser desorption and ionization) method. Our method offers more flexibility to optimize both the processes</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018TCry...12.1273R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018TCry...12.1273R"><span>Changing pattern of <span class="hlt">ice</span> flow and <span class="hlt">mass</span> balance for glaciers discharging into the Larsen A and B embayments, Antarctic Peninsula, 2011 to 2016</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rott, Helmut; Abdel Jaber, Wael; Wuite, Jan; Scheiblauer, Stefan; Floricioiu, Dana; Melchior van Wessem, Jan; Nagler, Thomas; Miranda, Nuno; van den Broeke, Michiel R.</p> <p>2018-04-01</p> <p>We analysed volume change and <span class="hlt">mass</span> balance of outlet glaciers on the northern Antarctic Peninsula over the periods 2011 to 2013 and 2013 to 2016, using high-resolution topographic data from the bistatic interferometric radar satellite mission TanDEM-X. Complementary to the geodetic method that applies DEM differencing, we computed the net <span class="hlt">mass</span> balance of the main outlet glaciers using the <span class="hlt">mass</span> budget method, accounting for the difference between the surface <span class="hlt">mass</span> balance (SMB) and the discharge of <span class="hlt">ice</span> into an ocean or <span class="hlt">ice</span> shelf. The SMB values are based on output of the regional climate model RACMO version 2.3p2. To study glacier flow and retrieve <span class="hlt">ice</span> discharge we generated time series of <span class="hlt">ice</span> velocity from data from different satellite radar sensors, with radar images of the satellites TerraSAR-X and TanDEM-X as the main source. The study area comprises tributaries to the Larsen A, Larsen Inlet and Prince Gustav Channel embayments (region A), the glaciers calving into the Larsen B embayment (region B) and the glaciers draining into the remnant part of the Larsen B <span class="hlt">ice</span> shelf in Scar Inlet (region C). The glaciers of region A, where the buttressing <span class="hlt">ice</span> shelf disintegrated in 1995, and of region B (<span class="hlt">ice</span> shelf break-up in 2002) show continuing losses in <span class="hlt">ice</span> <span class="hlt">mass</span>, with significant reduction of losses after 2013. The <span class="hlt">mass</span> balance numbers for the grounded glacier area of region A are -3.98 ± 0.33 Gt a-1 from 2011 to 2013 and -2.38 ± 0.18 Gt a-1 from 2013 to 2016. The corresponding numbers for region B are -5.75 ± 0.45 and -2.32 ± 0.25 Gt a-1. The <span class="hlt">mass</span> balance in region C during the two periods was slightly negative, at -0.54 ± 0.38 Gt a-1 and -0.58 ± 0.25 Gt a-1. The main share in the overall <span class="hlt">mass</span> losses of the region was contributed by two glaciers: Drygalski Glacier contributing 61 % to the <span class="hlt">mass</span> deficit of region A, and Hektoria and Green glaciers accounting for 67 % to the <span class="hlt">mass</span> deficit of region B. Hektoria and Green glaciers accelerated significantly in 2010</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 <span class="hlt">masses</span> 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 <span class="hlt">masses</span> 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://adsabs.harvard.edu/abs/2015AGUFM.C31A..03A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C31A..03A"><span>Interactions Between <span class="hlt">Ice</span> Thickness, Bottom <span class="hlt">Ice</span> Algae, and Transmitted Spectral Irradiance in the Chukchi Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Arntsen, A. E.; Perovich, D. K.; Polashenski, C.; Stwertka, C.</p> <p>2015-12-01</p> <p>The amount of light that penetrates the Arctic sea <span class="hlt">ice</span> cover impacts sea-<span class="hlt">ice</span> <span class="hlt">mass</span> balance as well as ecological processes in the upper ocean. The seasonally evolving macro and micro spatial variability of transmitted spectral irradiance observed in the Chukchi Sea from May 18 to June 17, 2014 can be primarily attributed to <span class="hlt">variations</span> in snow depth, <span class="hlt">ice</span> thickness, and bottom <span class="hlt">ice</span> algae concentrations. This study characterizes the interactions among these dominant variables using observed optical properties at each sampling site. We employ a normalized difference index to compute estimates of Chlorophyll a concentrations and analyze the increased attenuation of incident irradiance due to absorption by biomass. On a kilometer spatial scale, the presence of bottom <span class="hlt">ice</span> algae reduced the maximum transmitted irradiance by about 1.5 orders of magnitude when comparing floes of similar snow and <span class="hlt">ice</span> thicknesses. On a meter spatial scale, the combined effects of disparities in the depth and distribution of the overlying snow cover along with algae concentrations caused maximum transmittances to vary between 0.0577 and 0.282 at a single site. Temporal variability was also observed as the average integrated transmitted photosynthetically active radiation increased by one order of magnitude to 3.4% for the last eight measurement days compared to the first nine. Results provide insight on how interrelated physical and ecological parameters of sea <span class="hlt">ice</span> in varying time and space may impact new trends in Arctic sea <span class="hlt">ice</span> extent and the progression of melt.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19860013335','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19860013335"><span>Periodic <span class="hlt">variations</span> in the signal-to-noise ratios of signals received from the <span class="hlt">ICE</span> spacecraft</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nadeau, T.</p> <p>1986-01-01</p> <p>Data from the <span class="hlt">ICE</span> probe to comet Giacobini-Zinner are analyzed to determine the effects of spacecraft rotation upon the signal to noise ratio (SNR) for the two channels of data. In addition, long-term <span class="hlt">variations</span> from sources other than rotations are considered. Results include a pronounced SNR <span class="hlt">variation</span> over a period of three seconds (one rotation) and a lesser effect over a two minute period (possibly due to the receiving antenna conscan).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1817400S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1817400S"><span>Comparison of <span class="hlt">ice</span> particle size <span class="hlt">variations</span> across Ganymede and Callisto</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stephan, Katrin; Hoffmann, Harald; Hibbitts, Karl; Wagner, Roland; Jaumann, Ralf</p> <p>2016-04-01</p> <p>Ratios of band depths of different H2O <span class="hlt">ice</span> absorptions as measured by the Near Infrared Spectrometer NIMS onboard the Galileo spacecraft [1] have been found to be semi-quantitative indicator of changes in the particle size of <span class="hlt">ice</span> across the surfaces of the Jovian satellite Ganymede [2]. This method is now applied to Ganymede's neighboring satellite Callisto. On Ganymede, sizes reach from 1 μm near the poles to 1 mm near the equator [2]. Smallest particles occur at latitudes higher than ±30° where the closed magnetic field lines of Ganymede's magnetic field change into open ones and Ganymede's polar caps become apparent. Thus, the formation of these polar caps has often been attributed to brightening effects due to plasma bombardment of the surface [3,4]. Callisto, which does not exhibit an intrinsic magnetic field, however, also shows the same trend as observed on Ganymede with slightly larger particle sizes on Callisto than on Ganymede at low and mid latitude but similar particle sizes in the polar regions. Similar trends in the particle size <span class="hlt">variations</span> on Callisto and on Ganymede imply that these <span class="hlt">variations</span> are caused by similar surface processes. Our measurements rather point to a continuous decreasing of <span class="hlt">ice</span> particle sizes toward the poles on both satellites related to changes of the surface temperatures [5]. Maximum temperatures during the day reach 150 K and 165 K near the equator of Ganymede and Callisto [6, 7], respectively and sublimation of <span class="hlt">ice</span> particles and crystal growth [8] is expected to be the dominant surface process in these regions. In contrast, polar temperatures do not exceed 80 ± 5 K [5]. Larger particles in the equatorial region of Callisto than on Ganymede could be explained due to the slight higher maximum temperature but also a longer Callistoan day (Callisto: ~ 17 Earth days; Ganymede: ~ 7 Earth days). References: [1] Carlson et al.. (1999) Science 274, 385-388, 1996; [2] Stephan et al., 2009, EPSC, Abstract #EPSC2009-633; [3] Johnson</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUFM.U44A..01A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUFM.U44A..01A"><span>Recent Changes in Arctic Glaciers, <span class="hlt">Ice</span> Caps, and the Greenland <span class="hlt">Ice</span> Sheet: Cold Facts About Warm <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>Abdalati, W.</p> <p>2005-12-01</p> <p>One of the major manifestations of Arctic change can be observed in the state of balance of Arctic glaciers and <span class="hlt">ice</span> caps and the Greenland <span class="hlt">ice</span> sheet. These <span class="hlt">ice</span> <span class="hlt">masses</span> are estimated to contain nearly 3 million cubic kilometers of <span class="hlt">ice</span>, which is more than six times greater than all the water stored in the Earth's lakes, rivers, and snow combined and is the equivalent of over 7 meters of sea level. Most of these <span class="hlt">ice</span> <span class="hlt">masses</span> have been shrinking in recent in years, but their <span class="hlt">mass</span> balance is highly variable on a wide range of spatial and temporal scales. On the Greenland <span class="hlt">ice</span> sheet most of the coastal regions have thinned substantially as melt has increased and some of its outlet glaciers have accelerated. Near the equilibrium line in West Greenland, we have seen evidence of summer acceleration that is linked to surface meltwater production, suggesting a relatively rapid response mechanism of the <span class="hlt">ice</span> sheet change to a warming climate. At the same time, however, the vast interior regions of the Greenland <span class="hlt">ice</span> sheet have shown little change or slight growth, as accumulation in these areas may have increased. Throughout much of the rest of the Arctic, many glaciers and <span class="hlt">ice</span> caps have been shrinking in the past few decades, and in Canada and Alaska, the rate of <span class="hlt">ice</span> loss seems to have accelerated during the late 1990s. These recent observations offer only a snapshot in time of the long-term behavior, but they are providing crucial information about the current state of <span class="hlt">ice</span> <span class="hlt">mass</span> balance and the mechanisms that control it in one of the most climatically sensitive regions on Earth. As we continue to learn more through a combination of remote sensing observations, in situ measurements and improved modeling capabilities, it is important that we coordinate and integrate these approaches effectively in order to predict future changes and their impact on sea level, freshwater discharge, and ocean circulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA238039','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA238039"><span>Aircraft <span class="hlt">Icing</span> Handbook. Volume 1</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1991-03-01</p> <p>Maryland - . . . Kohiman Aviation, Lawrence , Kansas Ohio State University, Columbus, Ohio .I --- t-r 1-- - -t I.Q,,- t ../e . Pratt and Whitney...lower; about six percent at -22 ’F (-30 *C). 1.2.3 <span class="hlt">Variations</span> with Season The summer or warm season months create large warm air <span class="hlt">masses</span> which can...on Aircraft Surfaces," NASA TM 87184, May 1986. 2-54 Hausman , R.J. and Turnock, S.R., "Investigation of Surface Water Behavior During Glaze <span class="hlt">Ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017TCry...11.1913F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017TCry...11.1913F"><span>From cyclic <span class="hlt">ice</span> streaming to Heinrich-like events: the grow-and-surge instability in the Parallel <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>Feldmann, Johannes; Levermann, Anders</p> <p>2017-08-01</p> <p>Here we report on a cyclic, physical <span class="hlt">ice</span>-discharge instability in the Parallel <span class="hlt">Ice</span> Sheet Model, simulating the flow of a three-dimensional, inherently buttressed <span class="hlt">ice</span>-sheet-shelf system which periodically surges on a millennial timescale. The thermomechanically coupled model on 1 km horizontal resolution includes an enthalpy-based formulation of the thermodynamics, a nonlinear stress-balance-based sliding law and a very simple subglacial hydrology. The simulated unforced surging is characterized by rapid <span class="hlt">ice</span> streaming through a bed trough, resulting in abrupt discharge of <span class="hlt">ice</span> across the grounding line which is eventually calved into the ocean. We visualize the central feedbacks that dominate the subsequent phases of <span class="hlt">ice</span> buildup, surge and stabilization which emerge from the interaction between <span class="hlt">ice</span> dynamics, thermodynamics and the subglacial till layer. Results from the <span class="hlt">variation</span> of surface <span class="hlt">mass</span> balance and basal roughness suggest that <span class="hlt">ice</span> sheets of medium thickness may be more susceptible to surging than relatively thin or thick ones for which the surge feedback loop is damped. We also investigate the influence of different basal sliding laws (ranging from purely plastic to nonlinear to linear) on possible surging. The presented mechanisms underlying our simulations of self-maintained, periodic <span class="hlt">ice</span> growth and destabilization may play a role in large-scale <span class="hlt">ice</span>-sheet surging, such as the surging of the Laurentide <span class="hlt">Ice</span> Sheet, which is associated with Heinrich events, and <span class="hlt">ice</span>-stream shutdown and reactivation, such as observed in the Siple Coast region of West Antarctica.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C51B0713H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C51B0713H"><span>Probability based hydrologic catchments 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>Hudson, B. D.</p> <p>2015-12-01</p> <p>Greenland <span class="hlt">Ice</span> Sheet melt water impacts <span class="hlt">ice</span> sheet flow dynamics, fjord and coastal circulation, and sediment and biogeochemical fluxes. Melt water exiting the <span class="hlt">ice</span> sheet also is a key term in its <span class="hlt">mass</span> balance. Because of this, knowledge of the area of the <span class="hlt">ice</span> sheet that contributes melt water to a given outlet (its hydrologic catchment) is important to many <span class="hlt">ice</span> sheet studies and is especially critical to methods using river runoff to assess <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balance. Yet uncertainty in delineating <span class="hlt">ice</span> sheet hydrologic catchments is a problem that is rarely acknowledged. <span class="hlt">Ice</span> sheet catchments are delineated as a function of both basal and surface topography. While surface topography is well known, basal topography is less certain because it is dependent on radar surveys. Here, I a present a Monte Carlo based approach to delineating <span class="hlt">ice</span> sheet catchments that quantifies the impact of uncertain basal topography. In this scheme, over many iterations I randomly vary the <span class="hlt">ice</span> sheet bed elevation within published error bounds (using Morlighem et al., 2014 bed and bed error datasets). For each iteration of <span class="hlt">ice</span> sheet bed elevation, I calculate the hydraulic potentiometric surface and route water over its path of 'steepest' descent to delineate the catchment. I then use all realizations of the catchment to arrive at a probability map of all major melt water outlets in Greenland. I often find that catchment size is uncertain, with small, random perturbations in basal topography leading to large <span class="hlt">variations</span> in catchments size. While some catchments are well defined, others can double or halve in size within published basal topography error bars. While some uncertainty will likely always remain, this work points to locations where studies of <span class="hlt">ice</span> sheet hydrology would be the most successful, allows reinterpretation of past results, and points to where future radar surveys would be most advantageous.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21633379','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21633379"><span>Geographic <span class="hlt">variation</span> in left ventricular <span class="hlt">mass</span> and <span class="hlt">mass</span> index: a systematic review.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Poppe, K K; Bachmann, M Edgerton; Triggs, C M; Doughty, R N; Whalley, G A</p> <p>2012-07-01</p> <p>Left ventricular (LV) hypertrophy, defined as an abnormal increase in LV <span class="hlt">mass</span> (LVM), is an important prognostic indicator and therapeutic target. LVM is often divided by body surface area to derive indexed <span class="hlt">mass</span>; however, this does not correctly identify pathological LV hypertrophy in all people, especially when body composition is altered, or in different ethnic groups. We evaluated published ranges of echocardiographic LVM in healthy adult populations from different countries, excluding control groups, and compared them with the American Society of Echocardiography reference ranges. A total of 33 studies met the inclusion criteria. In men and women, there was wide <span class="hlt">variation</span> in the ranges of LVM with a tendency for the upper limit to increase geographically westward; this <span class="hlt">variation</span> remained for indexed <span class="hlt">mass</span>. Several ranges fell outside the upper reference limits: in men, 13 of the <span class="hlt">mass</span> ranges and 16 of indexed <span class="hlt">mass</span>; and in women, 8 <span class="hlt">mass</span> and 16 indexed <span class="hlt">mass</span>. This review has shown that current guidelines may need revision as some published series suggest that greater LV <span class="hlt">mass</span> should be considered normal. This may be explained by ethnic differences and supports the need for widely applicable and ethnically diverse reference ranges to be established.</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/2010EGUGA..12.6638C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12.6638C"><span>Periodical climate <span class="hlt">variations</span> and their impact on Earth rotation for the last 800Kyr</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chapanov, Yavor; Gambis, Daniel</p> <p>2010-05-01</p> <p>The Earth rotation <span class="hlt">variations</span> are highly affected by climatic <span class="hlt">variations</span> associated with the glacial cycles in the late Pleistocene. The processes of glaciation, followed by <span class="hlt">ice</span> melting, are connected with significant changes of the mean sea level. These processes redistribute great amount of water <span class="hlt">masses</span> between oceans and <span class="hlt">ice</span> sheets, which lead to changes of the axial moment of inertia and corresponding <span class="hlt">variations</span> of the Universal Time UT1 and Length of Day LOD, according to the law of angular momentum conservation. The climatic <span class="hlt">variations</span> for the last 800Kyr are analyzed by means of time series of temperature changes, determined by deuterium data from Antarctica <span class="hlt">ice</span> core. Reconstructed glacial sea level <span class="hlt">variations</span> for the last 380Kyr, determined by the sediments from the Red sea, are used, too. Common periodicities of the temperature and mean sea level <span class="hlt">variations</span> are determined. Time series of the long-periodical UT1 and LOD oscillations for the last 380Kyr and 800Kyr are reconstructed by means of empirical hydrological model of global water redistribution between the ocean and <span class="hlt">ice</span> sheets during the last glacial events.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910063773&hterms=1087&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3D%2526%25231087','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910063773&hterms=1087&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3D%2526%25231087"><span>Antarctic Sea <span class="hlt">ice</span> <span class="hlt">variations</span> and seasonal air temperature relationships</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Weatherly, John W.; Walsh, John E.; Zwally, H. J.</p> <p>1991-01-01</p> <p>Data through 1987 are used to determine the regional and seasonal dependencies of recent trends of Antarctic temperature and sea <span class="hlt">ice</span>. Lead-lag relationships involving regional sea <span class="hlt">ice</span> and air temperature are systematically evaluated, with an eye toward the <span class="hlt">ice</span>-temperature feedbacks that may influence climatic change. Over the 1958-1087 period the temperature trends are positive in all seasons. For the 15 years (l973-l987) for which <span class="hlt">ice</span> data are available, the trends are predominantly positive only in winter and summer, and are most strongly positive over the Antarctic Peninsula. The spatially aggregated trend of temperature for this latter period is small but positive, while the corresponding trend of <span class="hlt">ice</span> coverage is small but negative. Lag correlations between seasonal anomalies of the two variables are generally stronger with <span class="hlt">ice</span> lagging the summer temperatures and with <span class="hlt">ice</span> leading the winter temperatures. The implication is that summer temperatures predispose the near-surface waters to above-or below-normal <span class="hlt">ice</span> coverage in the following fall and winter.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70026900','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70026900"><span>Reconciling different observations of the CO2 <span class="hlt">ice</span> <span class="hlt">mass</span> loading of the Martian north polar cap</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Haberle, R.M.; Mattingly, B.; Titus, T.N.</p> <p>2004-01-01</p> <p>The GRS measurements of the peak <span class="hlt">mass</span> loading of the north polar CO2 <span class="hlt">ice</span> cap on Mars are about 60% lower than those calculated from MGS TES radiation data and those inferred from the MOLA cap thicknesses. However, the GRS data provide the most accurate measurement of the <span class="hlt">mass</span> loading. We show that the TES and MOLA data can be reconciled with the GRS data if (1) subsurface heat conduction and atmospheric heat transport are included in the TES <span class="hlt">mass</span> budget calculations, and (2) the density of the polar deposits is ???600 kg m-3. The latter is much less than that expected for slab <span class="hlt">ice</span> (???1600 kg m-3) and suggests that processes unique to the north polar region are responsible for the low cap density. Copyright 2004 by the American Geophysical Union.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6760381-iceberg-severity-off-eastern-north-america-its-relationship-sea-ice-variability-climate-change','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6760381-iceberg-severity-off-eastern-north-america-its-relationship-sea-ice-variability-climate-change"><span>Iceberg severity off eastern North America: Its relationship to sea <span class="hlt">ice</span> variability and climate change</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>Marko, J.R.; Fissel, D.B.; Wadhams, P.</p> <p>1994-09-01</p> <p>Iceberg trajectory, deterioration (<span class="hlt">mass</span> loss), and sea <span class="hlt">ice</span> data are reviewed to identify the sources of observed interannual and seasonal <span class="hlt">variations</span> in the numbers of icebergs passing south of 48[degrees]N off eastern North America. The results show the dominant role of sea <span class="hlt">ice</span> in the observed <span class="hlt">variations</span>. Important mechanisms involved include both seasonal modulation of the southerly iceberg flow by <span class="hlt">ice</span> cover control of probabilities for entrapment and decay in shallow water, and the suppression of iceberg melt/deterioration rates by high concentrations of sea <span class="hlt">ice</span>. The Labrador spring <span class="hlt">ice</span> extent, shown to be the critical parameter in interannual iceberg numbermore » variability, was found to be either determined by or closely correlated with midwinter Davis Strait <span class="hlt">ice</span> extents. Agreement obtained between observed year-to-year and seasonal number <span class="hlt">variations</span> with computations based upon a simple iceberg dissipation model suggests that downstream iceberg numbers are relatively insensitive to iceberg production rates and to fluctuations in southerly iceberg fluxes in areas north of Baffin Island. Past <span class="hlt">variations</span> in the Davis Strait <span class="hlt">ice</span> index and annual <span class="hlt">ice</span> extents are studied to identify trends and relationships between regional and larger-scale global climate parameters. It was found that, on decadal timescales in the post-1960 period of reasonable data quality, regional climate parameters have varied, roughly, out of phase with corresponding global and hemispheric changes. These observations are compared with expectations in terms of model results to evaluate current GCM-based capabilities for simulating recent regional behavior. 64 refs., 11 figs., 3 tabs.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.P21B2093A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.P21B2093A"><span>Local Time <span class="hlt">Variation</span> of Water <span class="hlt">Ice</span> Clouds on Mars as Observed by TES During Aerobraking.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>AlJanaahi, A. A.; AlShamsi, M. R.; Smith, M. D.; Altunaiji, E. S.; Edwards, C. S.</p> <p>2016-12-01</p> <p>The large elliptical orbit during Mars Global Surveyor aerobraking enabled sampling the martian atmosphere over many local times. The Thermal Emission Spectrometer (TES) aerobraking spectra were taken between Mars Year 23, Ls=180° and Mars Year 24, Ls=30°. These early data from before the main "mapping" part of the mission have been mostly overlooked, and relatively little analysis has been done with them. These datasets have not been used before to study local time <span class="hlt">variation</span>. Radiative transfer modeling is used to fit the spectra to retrieve surface and atmospheric temperature, and dust and water <span class="hlt">ice</span> optical depths. Retrievals show significant and systematic <span class="hlt">variation</span> in water <span class="hlt">ice</span> cloud optical depth as a function of local time. Cloud optical depth is higher in the early morning (before 9:00) and in the evening (after 17:00) for all seasons observed (Ls=180°-30°). Clouds form consistently in the Tyrrhena region and in the area around Tharsis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMPP13A2057L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMPP13A2057L"><span>Sea <span class="hlt">ice</span> <span class="hlt">variations</span> in the central Okhotsk Sea during the last two glacial-interglacial cycles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lo, L.; Cabedo-Sanz, P.; Lattaud, J.; Belt, S. T.; Schouten, S.; Huang, J. J.; Timmermann, A.; Zeeden, C.; Wei, K. Y.; Shen, C. C.; Hodell, D. A.; Elderfield, H.</p> <p>2016-12-01</p> <p>Sea <span class="hlt">ice</span> system as one of the critical and sensitive climate components in the Earth's climate system has experienced dramatically declination for the past few decades. Little knowledge, however, about the sea <span class="hlt">ice</span> <span class="hlt">variations</span> in the past orbital timescales has been obtained by paleoclimatic studies due to the lack of reliable sea <span class="hlt">ice</span> proxy and age model constrain in the high productivity subpolar to polar regions. Here we present continuous 180,000 years subarctic northwestern Pacific sea <span class="hlt">ice</span> and surface temperature (SST) records in the center Okhotsk Sea, the southernmost of seasonal sea <span class="hlt">ice</span> fomration region in the Northern Hemisphere by using by using novel organic and non-destructive geochemical proxies from Site MD01-2414 (53oN, 149oE, water depth 1123 m). High resolution X-ray fluoresces scanning biogenic/terrestrial (Ba/Ti) elemental ratio represent clear glacial-interglacial cycles. Organic geochemical proxies (IP25 and TEX86) derived sea <span class="hlt">ice</span> and SST changes in the same time resolution reveal the seasonality in the center Okhotsk Sea. Sea <span class="hlt">ice</span> shows strong 23-kyr precession cycle control with modulation of 100-kyr eccentricity cycle during the peak interglacial periods (Marine Isotope Stage 5e and Holocene). On the other hand, SST represent global background climate change of 100-kyr cycle with very strong obliquity changes. According to the timeseries analyses, we argue that the sea <span class="hlt">ice</span> minimum in the center of Okhotsk Sea has mainly been controlled by the local autumn insolation. SST represent annual insolation increasing due to local summer insolation and the obliquity pacing. This study firstly demonstrated clear seasonality in the same site. Further study of the relationship between sea <span class="hlt">ice</span> and seawater thermal hisotries on the orbital timescale in the subarctic Pacific is crucial in the understanding of past major climate event, e.g. Middle Pleistocene Transition and Middle Brunhes Event.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C23A1194T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C23A1194T"><span>The Sensitivity of the Greenland <span class="hlt">Ice</span> Sheet to Glacial-Interglacial Oceanic Forcing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tabone, I.; Blasco Navarro, J.; Robinson, A.; Alvarez-Solas, J.; Montoya, M.</p> <p>2017-12-01</p> <p>Up to now, the scientific community has mainly focused on the sensitivity of the Greenland <span class="hlt">Ice</span> Sheet (GrIS) to atmospheric <span class="hlt">variations</span>. However, several studies suggest that the enhanced <span class="hlt">ice</span> <span class="hlt">mass</span> loss experienced by the GrIS in the past decades is directly connected to the increasing North Atlantic temperatures. Melting of GrIS outlet glaciers triggers grounding-line retreat increasing <span class="hlt">ice</span> discharge into the ocean. This new evidence leads to consider the ocean as a relevant driver to be taken into account when modeling the evolution of the GrIS. The <span class="hlt">ice</span>-ocean interaction is a primary factor controling not only the likely future retreat of GrIS outlet glaciers, or the huge <span class="hlt">ice</span> loss in past warming climates, but also, and more strongly, the past GrIS glacial expansion. The latter assumption is supported by reconstructions which propose the GrIS to be fully marine-based during glacials, and thus more exposed to the influence of the ocean. Here, for the first time, we investigate the response of the GrIS to past oceanic changes using a three-dimensional hybrid <span class="hlt">ice-sheet/ice</span>-shelf model, which combines the Shallow <span class="hlt">Ice</span> Approximation (SIA) for slow grounded <span class="hlt">ice</span> sheets and the Shallow Shelf Approximation (SSA) in <span class="hlt">ice</span> shelves and <span class="hlt">ice</span> streams. The model accounts for a time-dependent parametrisation of the marine basal melting rate, which is used to reproduce past oceanic <span class="hlt">variations</span>. In this work simulations of the last two glacial cycles are performed. Our results show that the GrIS is very sensitive to the ocean-triggered submarine melting (freezing). Mild oceanic temperature <span class="hlt">variations</span> lead to a rapid retreat (expansion) of the GrIS margins, which, inducing a dynamic adjustment of the grounded <span class="hlt">ice</span> sheet, drive the evolution of the whole <span class="hlt">ice</span> sheet. Our results strongly suggest the need to consider the ocean as an active forcing in paleo <span class="hlt">ice</span> sheet models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014ACP....14.1205J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014ACP....14.1205J"><span>On the relationship between Arctic <span class="hlt">ice</span> clouds and polluted air <span class="hlt">masses</span> over the North Slope of Alaska in April 2008</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jouan, C.; Pelon, J.; Girard, E.; Ancellet, G.; Blanchet, J. P.; Delanoë, J.</p> <p>2014-02-01</p> <p>Recently, two types of <span class="hlt">ice</span> clouds (TICs) properties have been characterized using the Indirect and Semi-Direct Aerosol Campaign (ISDAC) airborne measurements (Alaska, April 2008). TIC-2B were characterized by fewer (< 10 L-1) and larger (> 110 μm) <span class="hlt">ice</span> crystals, and a larger <span class="hlt">ice</span> supersaturation (> 15%) compared to TIC-1/2A. It has been hypothesized that emissions of SO2 may reduce the <span class="hlt">ice</span> nucleating properties of <span class="hlt">ice</span> nuclei (IN) through acidification, resulting in a smaller concentration of larger <span class="hlt">ice</span> crystals and leading to precipitation (e.g., cloud regime TIC-2B). Here, the origin of air <span class="hlt">masses</span> forming the ISDAC TIC-1/2A (1 April 2008) and TIC-2B (15 April 2008) is investigated using trajectory tools and satellite data. Results show that the synoptic conditions favor air <span class="hlt">masses</span> transport from three potential SO2 emission sources into Alaska: eastern China and Siberia where anthropogenic and biomass burning emissions, respectively, are produced, and the volcanic region of the Kamchatka/Aleutians. Weather conditions allow the accumulation of pollutants from eastern China and Siberia over Alaska, most probably with the contribution of acidic volcanic aerosol during the TIC-2B period. Observation Monitoring Instrument (OMI) satellite observations reveal that SO2 concentrations in air <span class="hlt">masses</span> forming the TIC-2B were larger than in air <span class="hlt">masses</span> forming the TIC-1/2A. Airborne measurements show high acidity near the TIC-2B flight where humidity was low. These results support the hypothesis that acidic coating on IN could be at the origin of the formation of TIC-2B.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.G42A..02J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.G42A..02J"><span>Towards Estimate of Present Day <span class="hlt">Ice</span> Melting in Polar Regions From Altimetry, Gravity, Ocean Bottom Pressure and GPS Observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jiang, Y.; Wu, X.; van den Broeke, M. R.; Munneke, P. K.; Simonsen, S. B.; van der Wal, W.; Vermeersen, B. L.</p> <p>2013-12-01</p> <p>The <span class="hlt">ice</span> sheet in Polar Regions stores the largest freshwater bodies on Earth, sufficient to elevate global sea level by more than 65 meters if melted. The earth may have entered an intensive <span class="hlt">ice</span>-melting episode, possibly due to anthropogenic global warming rather than natural orbit <span class="hlt">variations</span>. Determining present-day <span class="hlt">ice</span> <span class="hlt">mass</span> balance, however, is complicated by the fact that most observations contain both present day <span class="hlt">ice</span> melting signal and residual signals from past glacier melting. Despite decades of progress in geodynamic modeling and new observations, significant uncertainties remain in both. The key to separate present-day <span class="hlt">ice</span> <span class="hlt">mass</span> change and signals from past melting is to include data of different physical characteristics. We conducted a new global kinematic inversion scheme to estimate both present-day <span class="hlt">ice</span> melting and past glacier signatures simultaneously and assess their contribution to current and future global mean sea level change. Our approach is designed to invert and separate present-day melting signal in the spherical harmonic domain using a globally distributed interdisciplinary data with distinct physical information. Interesting results with unprecedented precisions have been achieved so far. We will present our results of the estimated present-day <span class="hlt">ice</span> <span class="hlt">mass</span> balance trend in both Greenland and Antarctica <span class="hlt">ice</span> sheet as well as other regions where significant <span class="hlt">mass</span> change occurs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.G31C0924M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.G31C0924M"><span>Temporal variability of the Antarctic <span class="hlt">Ice</span> sheet observed from space-based geodesy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Memin, A.; King, M. A.; Boy, J. P.; Remy, F.</p> <p>2017-12-01</p> <p>Quantifying the Antarctic <span class="hlt">Ice</span> Sheet (AIS) <span class="hlt">mass</span> balance still remains challenging as several processes compete to differing degrees at the basin scale with regional <span class="hlt">variations</span>, leading to multiple <span class="hlt">mass</span> redistribution patterns. For instance, analysis of linear trends in surface-height <span class="hlt">variations</span> from 1992-2003 and 2002-2006 shows that the AIS is subject to decimetric scale variability over periods of a few years. Every year, snowfalls in Antarctica represent the equivalent of 6 mm of the mean sea level. Therefore, any fluctuation in precipitation can lead to changes in sea level. Besides, over the last decade, several major glaciers have been thinning at an accelerating rate. Understanding the processes that interact on the <span class="hlt">ice</span> sheet is therefore important to precisely determine the response of the <span class="hlt">ice</span> sheet to a rapid changing climate and estimate its contribution to sea level changes. We estimate seasonal and interannual changes of the AIS between January 2003 and October 2010 and to the end of 2016 from a combined analysis of surface-elevation and surface-<span class="hlt">mass</span> changes derived from Envisat data and GRACE solutions, and from GRACE solutions only, respectively. While we obtain a good correlation for the interannual signal between the two techniques, important differences (in amplitude, phase, and spatial pattern) are obtained for the seasonal signal. We investigate these discrepancies by comparing the crustal motion observed by GPS and those predicted using monthly surface <span class="hlt">mass</span> balance derived from the regional atmospheric climate model RACMO.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUFM.C41A..02R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUFM.C41A..02R"><span>Leakage of the Greenland <span class="hlt">Ice</span> Sheet through accelerated <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>Rignot, E.</p> <p>2005-12-01</p> <p>A map of coastal velocities of the Greenland <span class="hlt">ice</span> sheet was produced from Radarsat-1 acquired during the background mission of 2000 and combined with radio echo sounding data to estimate the <span class="hlt">ice</span> discharge from the <span class="hlt">ice</span> sheet. On individual glaciers, <span class="hlt">ice</span> discharge was compared with snow input from the interior and melt above the flux gate to determine the glacier <span class="hlt">mass</span> balance. Time series of velocities on several glaciers at different latitudes reveal seasonal fluctuations of only 7-8 percent so that winter velocities are only 2 percent less than the yearly mean. The results show the northern Greenland glaciers to be close to balance yet losing <span class="hlt">mass</span>. No change in <span class="hlt">ice</span> flow is detected on Petermann, 79north and Zachariae Isstrom in 2000-2004. East Greenland glaciers are in balance and flowing steadily north of Kangerdlussuaq, but Kangerdlussuaq, Helheim and all the southeastern glaciers are thinning dramatically. All these glaciers accelerated, Kangerdlussuaq in 2000, Helheim prior to 2004, and southeast Greenland glaciers accelerated 10 to 50 percent in 2000-2004. Glacier acceleration is generally brutal, probably once the glacier reached a threshold, and sustained. In the northwest, most glaciers are largely out of balance. Jakobshavn accelerated significantly in 2002, and glaciers in its immediate vicinity accelerated more than 50 percent in 2000-2004. Less is known about southwest Greenland glaciers due to a lack of <span class="hlt">ice</span> thickness data but the glaciers have accelerated there as well and are likely to be strongly out of balance despite thickening of the interior. Overall, I estimate the <span class="hlt">mass</span> balance of the Greenland <span class="hlt">ice</span> sheet to be about -80 +/-10 cubic km of <span class="hlt">ice</span> per year in 2000 and -110 +/-15 cubic km of <span class="hlt">ice</span> per year in 2004, i.e. more negative than based on partial altimetry surveys of the outlet glaciers. As climate continues to warm, more glaciers will accelerate, and the <span class="hlt">mass</span> balance will become increasingly negative, regardless of the evolution of the <span class="hlt">ice</span> sheet</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.1579W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.1579W"><span>Early 21st-Century <span class="hlt">Mass</span> loss of the North-Atlantic Glaciers and <span class="hlt">Ice</span> Caps (Arne Richter Award for Outstanding Young Scientists Lecture)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wouters, Bert; Ligtenberg, Stefan; Moholdt, Geir; Gardner, Alex S.; Noel, Brice; Kuipers Munneke, Peter; van den Broeke, Michiel; Bamber, Jonathan L.</p> <p>2016-04-01</p> <p>Historically, <span class="hlt">ice</span> loss from mountain glaciers and <span class="hlt">ice</span> caps has been one of the largest contributors to sea level rise over the last century. Of particular interest are the glaciers and <span class="hlt">ice</span> caps in the North-Atlantic region of the Arctic. Despite the cold climate in this area, considerable melting and runoff occurs in summer. A small increase in temperature will have an immediate effect on these processes, so that a large change in the Arctic <span class="hlt">ice</span> volume can be expected in response to the anticipated climate change in the coming century. Unfortunately, direct observations of glaciers are sparse and are biased toward glaciers systems in accessible, mostly maritime, climate conditions. Remote sensing is therefore essential to monitor the state of the the North-Atlantic glaciers and <span class="hlt">ice</span> caps. In this presentation, we will discuss the progress that has been made in estimating the <span class="hlt">ice</span> <span class="hlt">mass</span> balance of these regions, with a particular focus on measurements made by ESA's Cryosat-2 radar altimeter mission (2010-present). Compared to earlier altimeter mission, Cryosat-2 provides unprecedented coverage of the cryosphere, with a resolution down to 1 km or better and sampling at monthly intervals. Combining the Cryosat-2 measurements with the laser altimetry data from ICESat (2003-2009) gives us a 12 yr time series of glacial <span class="hlt">mass</span> loss in the North Atlantic. We find excellent agreement between the altimetry measurements and independent observations by the GRACE mission, which directly 'weighs' the <span class="hlt">ice</span> caps, albeit at a much lower resolution. <span class="hlt">Mass</span> loss in the region has increased from 120 Gigatonnes per year in 2003-2009 to roughly 140 Gt/yr in 2010-2014, with an important contribution from Greenland's peripheral glaciers and <span class="hlt">ice</span> caps. Importantly, the <span class="hlt">mass</span> loss is not stationary, but shows large regional interannual variability, with <span class="hlt">mass</span> loss shifting between eastern and western regions from year to year. Comparison with regional climate models shows that these shifts can be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.9833A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.9833A"><span>Phase relations of natural 65 year SST <span class="hlt">variations</span>, ocean sea level <span class="hlt">variations</span> over 260 years, and Arctic sea-<span class="hlt">ice</span> retreat of the satellite era - issues of cause and effect.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Asten, Michael</p> <p>2017-04-01</p> <p>We study sea level <span class="hlt">variations</span> over the past 300yr in order to quantify what fraction of <span class="hlt">variations</span> may be considered cyclic, and what phase relations exist with respect to those cycles. The 64yr cycle detected by Chambers et al (2012) is found in the 1960-2000 data set which Hamlington et al (2013) interpreted as an expression of the PDO; we show that fitting a 64yr cycle is a better fit, accounting for 92% of variance. In a 300yr GMSL tide guage record Jeverejeva et al (2008) identified a 60-65yr cycle superimposed on an upward trend from 1800CE. Using break-points and removal of centennial trends identified by Kemp et al (2015), we produce a detrended GMSL record for 1700-2000CE which emphasizes the 60-65yr oscillations. A least-square fit using a 64yr period cosine yields an amplitude 12mm and origin at year 1958.6, which accounts for 30% of the variance. A plot of the cosine against the entire length of the 300yr detrended GMSL record shows a clear phase lock for the interval 1740 to 2000CE, denoting either a very consistent timing of an internally generated natural <span class="hlt">variation</span>, or adding to evidence for an external forcing of astronomical origin (Scafetta 2012, 2013). Barcikowska et al (2016) have identified a 65yr cyclic <span class="hlt">variation</span> in sea surface temperature in the first multidecadal component of Multi- Channel Singular Spectrum Analysis (MSSA) on the Hadley SST data set (RC60). A plot of RC60 versus our fitted cosine shows the phase shift to be 16 yr, close to a 90 degree phase lag of GMSL relative to RC60. This is the relation to be expected for a simple low-pass or integrating filter, which suggests that cyclic natural <span class="hlt">variations</span> in sea-surface temperature drive similar <span class="hlt">variations</span> in GMSL. We compare the extent of Arctic sea-<span class="hlt">ice</span> using the time interval of 1979- 2016 (window of satellite imagery). The decrease in summer <span class="hlt">ice</span> cover has been subject of many predictions as to when summer <span class="hlt">ice</span> will reach zero. The plot of measured <span class="hlt">ice</span> area can be fitted with many</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1988ClDy....3...93C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1988ClDy....3...93C"><span>Late Pleistocene <span class="hlt">variations</span> in Antarctic sea <span class="hlt">ice</span> II: effect of interhemispheric deep-ocean heat exchange</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Crowley, Thomas J.; Parkinson, Claire L.</p> <p>1988-10-01</p> <p><span class="hlt">Variations</span> in production rates of warm North Atlantic Deep Water (NADW) have been proposed as a mechanism for linking climate fluctuations in the northern and southern hemispheres during the Pleistocene. We have tested this hypothesis by examining the sensitivity of a thermodynamic/dynamic model for Antarctic sea <span class="hlt">ice</span> to changes in vertical ocean heat flux and comparing the simulations with modified CLIMAP sea-<span class="hlt">ice</span> maps for 18 000 B.P. Results suggest that changes in NADW production rates, and the consequent changes in the vertical ocean heat flux in the Antarctic, can only account for about 20% 30% of the overall variance in Antarctic sea-<span class="hlt">ice</span> extent. This conclusion has been validated against an independent geological data set involving a time series of sea-surface temperatures from the subantarctic. The latter comparison suggests that, although the overall influence of NADW is relatively minor, the linkage may be much more significant at the 41 000-year obliquity period. Despite some limitations in the models and geological data, we conclude that NADW <span class="hlt">variations</span> may have played only a modest role in causing late Pleistocene climate change in the high latitudes of the southern hemisphere. Our conclusion is consistent with calculations by Manabe and Broccoli (1985) suggesting that atmospheric CO2 changes may be more important for linking the two hemispheres.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1712799K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1712799K"><span>Characterization of signatures from organic compounds in CDA <span class="hlt">mass</span> spectra of <span class="hlt">ice</span> particles in Saturn's E-ring</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Khawaja, Nozair; Postberg, Frank; Reviol, Rene; Srama, Ralf</p> <p>2015-04-01</p> <p>The major source of <span class="hlt">ice</span> particles in Saturn's E-ring is Enceladus - a geological active moon of Saturn. Enceladus is emanating <span class="hlt">ice</span> particles from its fractured south polar terrain (SPT), the so-called "Tiger Stripes". The source of Enceladus activity and many of the <span class="hlt">ice</span> particles is a subsurface ocean. The Cosmic Dust Analyzer (CDA) onboard the Cassini spacecraft is sampling these icy particles and producing TOF <span class="hlt">mass</span> spectra of cations of impinging particles [1]. Three compositional types of <span class="hlt">ice</span> particles have been identified from CDA-<span class="hlt">mass</span> spectra: (i) pure water <span class="hlt">ice</span> (Type-1) (ii) organic rich (Type-2) (iii) salt rich (Type-3) [2][3]. These organic rich (Type-2) spectra are particularly abundant in the icy jets of Enceladus as we found out during the Cassini's Enceladus flybys (E17 and E18) in 2012 [4]. We present a compositional analysis of the CDA spectra of these organic rich icy grains sampled in the E ring. We have characterized hundreds of Type-2 spectra of impinging <span class="hlt">ice</span> particles. These were recorded at different impact velocities causing different molecular fragmentation patterns observed in the <span class="hlt">mass</span> spectra. We defined 3 typical impact speed intervals: (i) 4-7 km/s (ii) 8-11 km/s and (iii) 12-16km/s. Organic features best observed at slow (4-7 km/s) or at intermediate (8-11 km/s) impact velocity ranges. Several classes of organic rich spectra are identified. Classifying Type-2 spectra are according to their characteristic <span class="hlt">mass</span> lines of possible organic species. We try to infer the composition of each class of organic rich spectra is inferred by using an experimental setup (IR-FL-MALDI) to simulate the CDA spectra of different compositional types. In the laboratory we have used infrared laser to disperse a micro-beam of a water solution [5]. The laser energy is adjusted to simulate different impact velocities of <span class="hlt">ice</span> particles on the CDA. Four families of organic compounds including alcohols, fatty acids, amines and aromatic, with varying number of carbon</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.C54A..03L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.C54A..03L"><span>Inferring unknow boundary conditions of the Greenland <span class="hlt">Ice</span> Sheet by assimilating ICESat-1 and <span class="hlt">Ice</span>Bridge altimetry intothe <span class="hlt">Ice</span> Sheet System Model.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Larour, E. Y.; Khazendar, A.; Seroussi, H. L.; Schlegel, N.; Csatho, B. M.; Schenk, A. F.; Rignot, E. J.; Morlighem, M.</p> <p>2014-12-01</p> <p>Altimetry signals from missions such as ICESat-1, CryoSat, EnviSat, as well as altimeters onboard Operation <span class="hlt">Ice</span>Bridge provide vital insights into processes such as surface <span class="hlt">mass</span> balance, <span class="hlt">mass</span> transport and <span class="hlt">ice</span>-flow dynamics. Historically however, <span class="hlt">ice</span>-flow models have been focused on assimilating surface velocities from satellite-based radar observations, to infer properties such as basal friction or the position of the bedrock. Here, we leverage a new methodology based on automatic differentation of the <span class="hlt">Ice</span> Sheet System Model to assimilate surface altimetry data into a reconstruction of the past decade of <span class="hlt">ice</span> flow on the North Greenland area. We infer corrections to boundary conditions such as basal friction and surface <span class="hlt">mass</span> balance, as well as corrections to the <span class="hlt">ice</span> hardness, to best-match the observed altimetry record. We compare these corrections between glaciers such as Petermann Glacier, 79 North and Zacchariae Isstrom. The altimetry signals exhibit very different patterns between East and West, which translate into very different signatures for the inverted boundary conditions. This study gives us greater insights into what differentiates different basins, both in terms of <span class="hlt">mass</span> transport and <span class="hlt">ice</span>-flow dynamics, and what could bethe controlling mechanisms behind the very different evolutions of these basins.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C23C0797N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C23C0797N"><span>A downscaled 1 km dataset of daily Greenland <span class="hlt">ice</span> sheet surface <span class="hlt">mass</span> balance components (1958-2014)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Noel, B.; Van De Berg, W. J.; Fettweis, X.; Machguth, H.; Howat, I. M.; van den Broeke, M. R.</p> <p>2015-12-01</p> <p>The current spatial resolution in regional climate models (RCMs), typically around 5 to 20 km, remains too coarse to accurately reproduce the spatial variability in surface <span class="hlt">mass</span> balance (SMB) components over the narrow ablation zones, marginal outlet glaciers and neighbouring <span class="hlt">ice</span> caps of the Greenland <span class="hlt">ice</span> sheet (GrIS). In these topographically rough terrains, the SMB components are highly dependent on local <span class="hlt">variations</span> in topography. However, the relatively low-resolution elevation and <span class="hlt">ice</span> mask prescribed in RCMs contribute to significantly underestimate melt and runoff in these regions due to unresolved valley glaciers and fjords. Therefore, near-km resolution topography is essential to better capture SMB variability in these spatially restricted regions. We present a 1 km resolution dataset of daily GrIS SMB covering the period 1958-2014, which is statistically downscaled from data of the polar regional climate model RACMO2.3 at 11 km, using an elevation dependence. The dataset includes all individual SMB components projected on the elevation and <span class="hlt">ice</span> mask from the GIMP DEM, down-sampled to 1 km. Daily runoff and sublimation are interpolated to the 1 km topography using a local regression to elevation valid for each day specifically; daily precipitation is bi-linearly downscaled without elevation corrections. The daily SMB dataset is then reconstructed by summing downscaled precipitation, sublimation and runoff. High-resolution elevation and <span class="hlt">ice</span> mask allow for properly resolving the narrow ablation zones and valley glaciers at the GrIS margins, leading to significant increase in runoff estimate. In these regions, and especially over narrow glaciers tongues, the downscaled products improve on the original RACMO2.3 outputs by better representing local SMB patterns through a gradual ablation increase towards the GrIS margins. We discuss the impact of downscaling on the SMB components in a case study for a spatially restricted region, where large elevation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998LPICo.953...40T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998LPICo.953...40T"><span>Terrestrial <span class="hlt">Ice</span> Sheets: Studies of Climate History, Internal Structure, Surface, and Bedrock</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thorsteinsson, Th.; Kipfstuhl, J.; Nixdorf, U.; Oerter, H.; Miller, H.; Fritsche, D.; Jung-Rothenhaeusler, F.; Mayer, C.; Schwager, M.; Wilhelms, F.; Steinhage, D.; Goektas, F.</p> <p>1998-01-01</p> <p>Recently drilled deep <span class="hlt">ice</span> cores from Central Greenland (GRIP and GISP2) provide the most detailed results available on climatic <span class="hlt">variation</span> in the northern hemisphere during the last 100,000 years, a period that includes the Holocene (0-11.5 ka) and most of the Wisconsin glacial period. Summer-winter <span class="hlt">variation</span> in various physical and chemical properties of polar <span class="hlt">ice</span> allows dating of <span class="hlt">ice</span> cores by annual layer counting. Several such methods are currently being employed on an <span class="hlt">ice</span> core drilled by the new North Greenland <span class="hlt">Ice</span> Core Project (NGRIP), which is aimed at extending the Greenland <span class="hlt">ice</span> palaeoclimatic record through the last interglacial, the Eemian. Two examples will be presented: (1) visual and photographic studies of seasonal <span class="hlt">variation</span> in stratigraphic layering, crystal size, air bubble and clathrate concentration, and (2) studies of electric stratigraphy, using the method of dielectric profiling (DEP). This method records the AC conductivity of <span class="hlt">ice</span> cores, which is negatively correlated with the concentration of airborne dust in the <span class="hlt">ice</span> but positively correlated with volcanic and marine aerosols. Comprehensive surface traverse programs, which include shallow coring and <span class="hlt">ice</span> velocity measurements, have recently been carried out by the Alfred Wegener Institute in previously little-investigated regions of Greenland and Antarctica. Serving partly as reconnaissance prior to deep drilling projects, such studies also help to reduce considerable uncertainties in the <span class="hlt">mass</span> balance of the two large polar <span class="hlt">ice</span> sheets and thus in their estimated response to climate change. Main results of a recent traverse in North Greenland include the following: (1) A new map of the accumulation distribution on the <span class="hlt">ice</span> sheet indicates a large low-accumulation region in Northeast-Greenland; (2) North Greenland records show significantly greater climatic variability during the last 500 yr than corresponding records from the southern part of the <span class="hlt">ice</span> sheet; and (3) data on <span class="hlt">variation</span> in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.T33I..04V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.T33I..04V"><span>GIA Modeling with 3D Rheology and Recent <span class="hlt">Ice</span> Thickness Changes in Polar Regions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Van Der Wal, W.; Wu, P. P.</p> <p>2012-12-01</p> <p>Models for Glacial Isostatic Adjustment (GIA) mainly focus on the response of the solid Earth to <span class="hlt">ice</span> thickness changes on the scale of thousands of years. However, some of the fastest vertical movement in former glaciated regions is due to changes in <span class="hlt">ice</span> thickness that occurred within the last 1,000 years. Similar studies for the polar regions are limited, possibly due to a lack of knowledge on past <span class="hlt">ice</span> sheet thicknesses there. Still, predictions of uplift rate and <span class="hlt">mass</span> change due to recent <span class="hlt">ice</span> thickness changes need to improve in order to provide accurate estimates of current <span class="hlt">mass</span> loss. In order to obtain a measurable response to <span class="hlt">variations</span> in <span class="hlt">ice</span> thickness in the last 1,000 years, viscosity in the lithosphere or top of the upper mantle needs to be lower than the mantle viscosity values in conventional GIA models. In the absence of reliable models for recent <span class="hlt">ice</span> thickness changes we aim to bracket the predicted uplift rates and gravity rates for such changes by assuming simplified past <span class="hlt">ice</span> growth and melt patterns. Instead of adding a low-viscous layer in the mantle a priori, creep parameters are based on information from experimental constraints, seismology and heatflow measurements. Thus the model includes viscosity varying in space and time. The simulations are performed on a finite element model of a spherical, self-gravitating, incompressible Earth using the commercial software Abaqus. 3D composite rheology is implemented based on temperature fields from heatflow measurements or seismic velocity anomalies. The lithospheric thickness does not need to be specified as the effective elastic thickness is determined by the local effective viscosity. <span class="hlt">ICE</span>-5G is used as <span class="hlt">ice</span> loading history while <span class="hlt">ice</span> changes during and around the Little <span class="hlt">Ice</span> Age in Greenland are assumed to take place near the coast. A 3D composite rheology has been shown to match historic sea levels well, but uplift rates are somewhat underestimated. With the GIA models that best match uplift rates in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140006602','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140006602"><span>Dynamic Inland Propagation of Thinning Due to <span class="hlt">Ice</span> Loss at the Margins 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>Wang, Wei Li; Li, Jun J.; Zwally, H. Jay</p> <p>2012-01-01</p> <p><span class="hlt">Mass</span>-balance analysis of the Greenland <span class="hlt">ice</span> sheet based on surface elevation changes observed by the European Remote-sensing Satellite (ERS) (1992-2002) and <span class="hlt">Ice</span>, Cloud and land Elevation Satellite (ICESat) (2003-07) indicates that the strongly increased <span class="hlt">mass</span> loss at lower elevations (<2000 m) of the <span class="hlt">ice</span> sheet, as observed during 2003-07, appears to induce interior <span class="hlt">ice</span> thinning at higher elevations. In this paper, we perform a perturbation experiment with a three-dimensional anisotropic <span class="hlt">ice</span>-flow model (AIF model) to investigate this upstream propagation. Observed thinning rates in the regions below 2000m elevation are used as perturbation inputs. The model runs with perturbation for 10 years show that the extensive <span class="hlt">mass</span> loss at the <span class="hlt">ice</span>-sheet margins does in fact cause interior thinning on short timescales (i.e. decadal). The modeled pattern of thinning over the <span class="hlt">ice</span> sheet agrees with the observations, which implies that the strong <span class="hlt">mass</span> loss since the early 2000s at low elevations has had a dynamic impact on the entire <span class="hlt">ice</span> sheet. The modeling results also suggest that even if the large <span class="hlt">mass</span> loss at the margins stopped, the interior <span class="hlt">ice</span> sheet would continue thinning for 300 years and would take thousands of years for full dynamic recovery.</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/2013ACPD...13.4331J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013ACPD...13.4331J"><span>On the relationship between Arctic <span class="hlt">ice</span> clouds and polluted air <span class="hlt">masses</span> over the north slope of Alaska in April 2008</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jouan, C.; Pelon, J.; Girard, E.; Ancellet, G.; Blanchet, J. P.; Delanoë, J.</p> <p>2013-02-01</p> <p>Recently, two Types of <span class="hlt">Ice</span> Clouds (TICs) properties have been characterized using ISDAC airborne measurements (Alaska, April 2008). TIC-2B were characterized by fewer (<10 L-1) and larger (>110 μm) <span class="hlt">ice</span> crystals, a larger <span class="hlt">ice</span> supersaturation (>15%) and a fewer <span class="hlt">ice</span> nuclei (IN) concentration (<2 order of magnitude) when compared to TIC-1/2A. It has been hypothesized that emissions of SO2 may reduce the <span class="hlt">ice</span> nucleating properties of IN through acidification, resulting to a smaller concentration of larger <span class="hlt">ice</span> crystals and leading to precipitation (e.g. cloud regime TIC-2B) because of the reduced competition for the same available moisture. Here, the origin of air <span class="hlt">masses</span> forming the ISDAC TIC-1/2A (1 April 2008) and TIC-2B (15 April 2008) is investigated using trajectory tools and satellite data. Results show that the synoptic conditions favor air <span class="hlt">masses</span> transport from the three potentials SO2 emission areas to Alaska: eastern China and Siberia where anthropogenic and biomass burning emission respectively are produced and the volcanic region from the Kamchatka/Aleutians. Weather conditions allow the accumulation of pollutants from eastern China/Siberia over Alaska, most probably with the contribution of acid volcanic aerosol during the TIC-2B period. OMI observations reveal that SO2 concentrations in air <span class="hlt">masses</span> forming the TIC-2B were larger than in air <span class="hlt">masses</span> forming the TIC-1/2A. Airborne measurements show high acidity near the TIC-2B flight where humidity was low. These results strongly support the hypothesis that acidic coating on IN are at the origin of the formation of TIC-2B.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018TCry...12.1699R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018TCry...12.1699R"><span>Tidal bending of <span class="hlt">ice</span> shelves as a mechanism for large-scale temporal <span class="hlt">variations</span> in <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>Rosier, Sebastian H. R.; Hilmar Gudmundsson, G.</p> <p>2018-05-01</p> <p>GPS measurements reveal strong modulation of horizontal <span class="hlt">ice</span> shelf and <span class="hlt">ice</span> stream flow at a variety of tidal frequencies, most notably a fortnightly (Msf) frequency not present in the vertical tides themselves. Current theories largely fail to explain the strength and prevalence of this signal over floating <span class="hlt">ice</span> shelves. We show how well-known non-linear aspects of <span class="hlt">ice</span> rheology can give rise to widespread, long-periodic tidal modulation in <span class="hlt">ice</span> shelf flow, generated within <span class="hlt">ice</span> shelves themselves through tidal flexure acting at diurnal and semidiurnal frequencies. Using full-Stokes viscoelastic modelling, we show that inclusion of tidal bending within the model accounts for much of the observed tidal modulation of <span class="hlt">ice</span> shelf flow. Furthermore, our model shows that, in the absence of vertical tidal forcing, the mean flow of the <span class="hlt">ice</span> shelf is reduced by almost 30 % for the geometry that we consider.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014SolED...6...91N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014SolED...6...91N"><span><span class="hlt">Variations</span> of soil profile characteristics due to varying time spans since <span class="hlt">ice</span> retreat in the inner Nordfjord, western Norway</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Navas, A.; Laute, K.; Beylich, A. A.; Gaspar, L.</p> <p>2014-01-01</p> <p>In the Erdalen and Bødalen drainage basins located in the inner Nordfjord in western Norway the soils have been formed after deglaciation. The climate in the uppermost valley areas is sub-arctic oceanic and the lithology consists of Precambrian granitic orthogneisses on which Leptosols and Regosols are the most common soils. The Little <span class="hlt">Ice</span> Age glacier advance affected parts of the valleys with the maximum glacier extent around AD 1750. In this study five sites on moraine and colluvium materials were selected to examine the main soil properties to assess if soil profile characteristics and pattern of fallout radionuclides (FRNs) and environmental radionuclides (ERNs) are affected by different stages of <span class="hlt">ice</span> retreat. The Leptosols on the moraines are shallow, poorly developed and vegetated with moss and small birches. The two selected profiles show different radionuclide activities and grain size distribution. The sampled soils on the colluviums outside the LIA glacier limit became <span class="hlt">ice</span>-free during the Preboral. The Regosols present better-developed profiles, thicker organic horizons and are fully covered by grasses. Activity of 137Cs and 210Pbex concentrate at the topsoil and decrease sharply with depth. The grain size distribution of these soils also reflects the difference in geomorphic processes that have affected the colluvium sites. Significant lower <span class="hlt">mass</span> activities of FRNs are found in soils on the moraines than on colluviums. <span class="hlt">Variations</span> of ERNs activities in the valleys are related to characteristics soil mineralogical composition. These results indicate differences in soil development that are consistent with the age of <span class="hlt">ice</span> retreat. In addition, the pattern distribution of 137Cs and 210Pbex activities differs in the soils related to the LIA glacier limits in the drainage basins.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014SolE....5..485N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014SolE....5..485N"><span><span class="hlt">Variations</span> of soil profile characteristics due to varying time spans since <span class="hlt">ice</span> retreat in the inner Nordfjord, western Norway</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Navas, A.; Laute, K.; Beylich, A. A.; Gaspar, L.</p> <p>2014-06-01</p> <p>In the Erdalen and Bødalen drainage basins located in the inner Nordfjord in western Norway the soils were formed after deglaciation. The climate in the uppermost valley areas is sub-arctic oceanic, and the lithology consists of Precambrian granitic orthogneisses on which Leptosols and Regosols are the most common soils. The Little <span class="hlt">Ice</span> Age glacier advance affected parts of the valleys with the maximum glacier extent around AD 1750. In this study five sites on moraine and colluvium materials were selected to examine main soil properties, grain size distribution, soil organic carbon and pH to assess if soil profile characteristics and patterns of fallout radionuclides (FRNs) and environmental radionuclides (ERNs) are affected by different stages of <span class="hlt">ice</span> retreat. The Leptosols on the moraines are shallow, poorly developed and vegetated with moss and small birches. The two selected profiles show different radionuclide activities and grain size distribution. The sampled soils on the colluviums outside the LIA glacier limit became <span class="hlt">ice</span>-free during the Preboral. The Regosols present better-developed profiles, thicker organic horizons and are fully covered by grasses. Activity of 137Cs and 210Pbex concentrate at the topsoil and decrease sharply with depth. The grain size distribution of these soils also reflects the difference in geomorphic processes that have affected the colluvium sites. Significantly lower <span class="hlt">mass</span> activities of FRNs were found in soils on the moraines than on colluviums. <span class="hlt">Variations</span> of ERN activities in the valleys were related to characteristics of soil mineralogical composition. These results indicate differences in soil development that are consistent with the age of <span class="hlt">ice</span> retreat. In addition, the pattern distribution of 137Cs and 210Pbex activities differs in the soils related to the LIA glacier limits in the drainage basins.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.C44A..02B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.C44A..02B"><span>connecting the dots between Greenland <span class="hlt">ice</span> sheet surface melting and <span class="hlt">ice</span> flow dynamics (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Box, J. E.; Colgan, W. T.; Fettweis, X.; Phillips, T. P.; Stober, M.</p> <p>2013-12-01</p> <p>This presentation is of a 'unified theory' in glaciology that first identifies surface albedo as a key factor explaining total <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balance and then surveys a mechanistic self-reinforcing interaction between melt water and <span class="hlt">ice</span> flow dynamics. The theory is applied in a near-real time total Greenland <span class="hlt">mass</span> balance retrieval based on surface albedo, a powerful integrator of the competing effects of accumulation and ablation. New snowfall reduces sunlight absorption and increases meltwater retention. Melting amplifies absorbed sunlight through thermal metamorphism and bare <span class="hlt">ice</span> expansion in space and time. By ';following the melt'; we reveal mechanisms linking existing science into a unified theory. Increasing meltwater softens the <span class="hlt">ice</span> sheet in three ways: 1.) sensible heating given the water temperature exceeds that of the <span class="hlt">ice</span> sheet interior; 2.) Some infiltrating water refreezes, transferring latent heat to the <span class="hlt">ice</span>; 3.) Friction from water turbulence heats the <span class="hlt">ice</span>. It has been shown that for a point on the <span class="hlt">ice</span> sheet, basal lubrication increases <span class="hlt">ice</span> flow speed to a time when an efficient sub-glacial drainage network develops that reduces this effect. Yet, with an increasing melt duration the point where the <span class="hlt">ice</span> sheet glides on a wet bed increases inland to a larger area. This effect draws down the <span class="hlt">ice</span> surface elevation, contributing to the ';elevation feedback'. In a perpetual warming scenario, the elevation feedback ultimately leads to <span class="hlt">ice</span> sheet loss reversible only through much slower <span class="hlt">ice</span> sheet growth in an <span class="hlt">ice</span> age environment. As the inland <span class="hlt">ice</span> sheet accelerates, the horizontal extension pulls cracks and crevasses open, trapping more sunlight, amplifying the effect of melt accelerated <span class="hlt">ice</span>. As the bare <span class="hlt">ice</span> area increases, the direct sun-exposed crevassed and infiltration area increases further allowing the <span class="hlt">ice</span> warming process to occur more broadly. Considering hydrofracture [a.k.a. hydrofracking]; surface meltwater fills cracks, attacking the <span class="hlt">ice</span> integrity</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011TCry....5..791K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011TCry....5..791K"><span>Deriving <span class="hlt">mass</span> balance and calving <span class="hlt">variations</span> from reanalysis data and sparse observations, Glaciar San Rafael, northern Patagonia, 1950-2005</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Koppes, M.; Conway, H.; Rasmussen, L. A.; Chernos, M.</p> <p>2011-09-01</p> <p><span class="hlt">Mass</span> balance <span class="hlt">variations</span> of Glaciar San Rafael, the northernmost tidewater glacier in the Southern Hemisphere, are reconstructed over the period 1950-2005 using NCEP-NCAR reanalysis climate data together with sparse, local historical observations of air temperature, precipitation, accumulation, ablation, thinning, calving, and glacier retreat. The combined observations over the past 50 yr indicate that Glaciar San Rafael has thinned and retreated since 1959, with a total <span class="hlt">mass</span> loss of ~22 km3 of <span class="hlt">ice</span> eq. Over that period, except for a short period of cooling from 1998-2003, the climate has become progressively warmer and drier, which has resulted primarily in pervasive thinning of the glacier surface and a decrease in calving rates, with only minor acceleration in retreat of the terminus. A comparison of calving fluxes derived from the <span class="hlt">mass</span> balance <span class="hlt">variations</span> and from theoretical calving and sliding laws suggests that calving rates are inversely correlated with retreat rates, and that terminus geometry is more important than balance fluxes to the terminus in driving calving dynamics. For Glaciar San Rafael, regional climate warming has not yet resulted in the significant changes in glacier length seen in other calving glaciers in the region, emphasizing the complex dynamics between climate inputs, topographic constraints and glacier response in calving glacier systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011TCD.....5.1123K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011TCD.....5.1123K"><span>Deriving <span class="hlt">mass</span> balance and calving <span class="hlt">variations</span> from reanalysis data and sparse observations, Glaciar San Rafael, northern Patagonia, 1950-2005</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Koppes, M.; Conway, H.; Rasmussen, L. A.; Chernos, M.</p> <p>2011-04-01</p> <p><span class="hlt">Mass</span> balance <span class="hlt">variations</span> of Glaciar San Rafael, the most equatorial tidewater glacier in the North Patagonian Icefield, are reconstructed over the period 1950-2005 using NCEP-NCAR reanalysis climate data together with sparse, local historical observations of air temperature, precipitation, accumulation, ablation, thinning, calving, and glacier retreat. The combined observations over the past 50 yr indicate that Glaciar San Rafael has thinned and retreated since 1959, with a total <span class="hlt">mass</span> loss of ~22 km3 of <span class="hlt">ice</span> equivalent. Over that period, except for a short period of cooling from 1998-2003, the climate has become progressively warmer and drier, which has resulted primarily in pervasive thinning of the glacier surface and a decrease in calving rates, with only minor acceleration in retreat of the terminus. A comparison of calving fluxes derived from the <span class="hlt">mass</span> balance <span class="hlt">variations</span> and from theoretical calving and sliding laws suggest that calving rates are inversely correlated with retreat rates, and that terminus geometry is more important than changes in balance fluxes to the terminus in driving calving dynamics. For Glaciar San Rafael, regional climate warming has not yet resulted in the significant changes in glacier length seen in other calving glaciers in the region, emphasizing the complex dynamics between climate inputs, topographic constraints and glacier response in calving glacier systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C53C0799H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C53C0799H"><span>Validation of Modelled <span class="hlt">Ice</span> Dynamics of the Greenland <span class="hlt">Ice</span> Sheet using Historical Forcing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hoffman, M. J.; Price, S. F.; Howat, I. M.; Bonin, J. A.; Chambers, D. P.; Tezaur, I.; Kennedy, J. H.; Lenaerts, J.; Lipscomb, W. H.; Neumann, T.; Nowicki, S.; Perego, M.; Saba, J. L.; Salinger, A.; Guerber, J. R.</p> <p>2015-12-01</p> <p>Although <span class="hlt">ice</span> sheet models are used for sea level rise projections, the degree to which these models have been validated by observations is fairly limited, due in part to the limited duration of the satellite observation era and the long adjustment time scales of <span class="hlt">ice</span> sheets. Here we describe a validation framework for the Greenland <span class="hlt">Ice</span> Sheet applied to the Community <span class="hlt">Ice</span> Sheet Model by forcing the model annually with flux anomalies at the major outlet glaciers (Enderlin et al., 2014, observed from Landsat/ASTER/Operation <span class="hlt">Ice</span>Bridge) and surface <span class="hlt">mass</span> balance (van Angelen et al., 2013, calculated from RACMO2) for the period 1991-2012. The <span class="hlt">ice</span> sheet model output is compared to <span class="hlt">ice</span> surface elevation observations from ICESat and <span class="hlt">ice</span> sheet <span class="hlt">mass</span> change observations from GRACE. Early results show promise for assessing the performance of different model configurations. Additionally, we explore the effect of <span class="hlt">ice</span> sheet model resolution on validation skill.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..4411463S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..4411463S"><span>Algae Drive Enhanced Darkening of Bare <span class="hlt">Ice</span> 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>Stibal, Marek; Box, Jason E.; Cameron, Karen A.; Langen, Peter L.; Yallop, Marian L.; Mottram, Ruth H.; Khan, Alia L.; Molotch, Noah P.; Chrismas, Nathan A. M.; Calı Quaglia, Filippo; Remias, Daniel; Smeets, C. J. P. Paul; van den Broeke, Michiel R.; Ryan, Jonathan C.; Hubbard, Alun; Tranter, Martyn; van As, Dirk; Ahlstrøm, Andreas P.</p> <p>2017-11-01</p> <p>Surface ablation of the Greenland <span class="hlt">ice</span> sheet is amplified by surface darkening caused by light-absorbing impurities such as mineral dust, black carbon, and pigmented microbial cells. We present the first quantitative assessment of the microbial contribution to the <span class="hlt">ice</span> sheet surface darkening, based on field measurements of surface reflectance and concentrations of light-absorbing impurities, including pigmented algae, during the 2014 melt season in the southwestern part of the <span class="hlt">ice</span> sheet. The impact of algae on bare <span class="hlt">ice</span> darkening in the study area was greater than that of nonalgal impurities and yielded a net albedo reduction of 0.038 ± 0.0035 for each algal population doubling. We argue that algal growth is a crucial control of bare <span class="hlt">ice</span> darkening, and incorporating the algal darkening effect will improve <span class="hlt">mass</span> balance and sea level projections of the Greenland <span class="hlt">ice</span> sheet and <span class="hlt">ice</span> <span class="hlt">masses</span> elsewhere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1917148O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1917148O"><span>Water <span class="hlt">ice</span> cloud property retrievals at Mars with OMEGA:Spatial distribution and column <span class="hlt">mass</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Olsen, Kevin S.; Madeleine, Jean-Baptiste; Szantai, Andre; Audouard, Joachim; Geminale, Anna; Altieri, Francesca; Bellucci, Giancarlo; Montabone, Luca; Wolff, Michael J.; Forget, Francois</p> <p>2017-04-01</p> <p>Spectral images of Mars recorded by OMEGA (Observatoire pour la Minéralogie, l'Eau, les Glaces et l'Activité) on Mars Express can be used to deduce the mean effective radius (r_eff) and optical depth (τ_i) of water <span class="hlt">ice</span> particles in clouds. Using new data sets for a priori surface temperature, vertical profiles of atmospheric temperature, dust opacity, and multi-spectral surface albedo, we have analyzed over 40 OMEGA image cubes over the Tharsis, Arabia, and Syrtis Major quadrangles, and mapped the spatial distribution of r_eff, τ_i, and water <span class="hlt">ice</span> column <span class="hlt">mass</span>. We also explored the parameter space of r_eff and τ_i, which are inversely proportional, and the <span class="hlt">ice</span> cloud index (ICI), which is the ratio of the reflectance at 3.4 and 3.52 μm, and indicates the thickness of water <span class="hlt">ice</span> clouds. We found that the ICI, trivial to calculate for OMEGA image cubes, can be a proxy for column <span class="hlt">mass</span>, which is very expensive to compute, requiring accurate retrievals of surface albedo, r_eff, and τ_i. Observing the spatial distribution, we find that within each cloud system, r_eff varies about a mean of 2.1 μm, that τi is closely related to r_eff, and that the values allowed for τ_i, given r_eff, are related to the ICI. We also observe areas where our retrieval detects very thin clouds made of very large particles (mean of 12.5 μm), which are still under investigation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMGC31A1017F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMGC31A1017F"><span>Sea-level responses to sediment transport over the last <span class="hlt">ice</span> age cycle</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ferrier, K.; Mitrovica, J. X.</p> <p>2013-12-01</p> <p>Sea-level changes over the last <span class="hlt">ice</span> age cycle were instrumental in steering Earth's topographic evolution. These sea-level <span class="hlt">variations</span> were driven by changes in surface <span class="hlt">mass</span> loads, including not only <span class="hlt">ice</span> and ocean <span class="hlt">mass</span> <span class="hlt">variations</span> but also the transfer of rock from eroding mountains to sedimentary deposits. Here we use an extended numerical model of <span class="hlt">ice</span> age sea level (Dalca et al., 2013) to explore how sediment erosion and deposition affected global sea-level <span class="hlt">variations</span> over the last <span class="hlt">ice</span> age cycle. The model takes histories of <span class="hlt">ice</span> and sediment loads as inputs, and it computes gravitationally self-consistent sea level responses by accounting for the deformational, gravitational, and rotational perturbations in the Earth's viscoelastic form. In these model simulations, we use published estimates of erosion rates, sedimentation rates, and <span class="hlt">ice</span> sheet <span class="hlt">variations</span> to constrain sediment and <span class="hlt">ice</span> loading since the Last Interglacial. We explore sea-level responses to several erosional and depositional scenarios, and in each we quantify the relative contributions of crustal deformation and gravitational perturbation to the computed sea-level change. We also present a case study to illustrate the effects that sediment transfer can have on sea level at the regional scale. In particular, we focus on the region surrounding the Indus River, where fluvial sediment fluxes are among the highest on Earth. Preliminary model results suggest that sediment fluxes from Asia to the ocean are large enough to produce a significant response in sea level along the northeastern coast of the Arabian Sea. Moreover, they suggest that modeled sea-level histories are sensitive to the timing and spatial distribution of sediment erosion and deposition. For instance, sediment deposition along the continental shelf - which may have been the primary site of Indus River sediment deposition during the Holocene - produces a different sea-level response than sediment deposition on the deep-sea Indus Fan, where</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 <span class="hlt">mass</span> 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 <span class="hlt">mass</span> 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 zones, 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('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5489271','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5489271"><span>Decreasing cloud cover drives the recent <span class="hlt">mass</span> loss on the Greenland <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Hofer, Stefan; Tedstone, Andrew J.; Fettweis, Xavier; Bamber, Jonathan L.</p> <p>2017-01-01</p> <p>The Greenland <span class="hlt">Ice</span> Sheet (GrIS) has been losing <span class="hlt">mass</span> at an accelerating rate since the mid-1990s. This has been due to both increased <span class="hlt">ice</span> discharge into the ocean and melting at the surface, with the latter being the dominant contribution. This change in state has been attributed to rising temperatures and a decrease in surface albedo. We show, using satellite data and climate model output, that the abrupt reduction in surface <span class="hlt">mass</span> balance since about 1995 can be attributed largely to a coincident trend of decreasing summer cloud cover enhancing the melt-albedo feedback. Satellite observations show that, from 1995 to 2009, summer cloud cover decreased by 0.9 ± 0.3% per year. Model output indicates that the GrIS summer melt increases by 27 ± 13 gigatons (Gt) per percent reduction in summer cloud cover, principally because of the impact of increased shortwave radiation over the low albedo ablation zone. The observed reduction in cloud cover is strongly correlated with a state shift in the North Atlantic Oscillation promoting anticyclonic conditions in summer and suggests that the enhanced surface <span class="hlt">mass</span> loss from the GrIS is driven by synoptic-scale changes in Arctic-wide atmospheric circulation. PMID:28782014</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28782014','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28782014"><span>Decreasing cloud cover drives the recent <span class="hlt">mass</span> loss on the Greenland <span class="hlt">Ice</span> Sheet.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hofer, Stefan; Tedstone, Andrew J; Fettweis, Xavier; Bamber, Jonathan L</p> <p>2017-06-01</p> <p>The Greenland <span class="hlt">Ice</span> Sheet (GrIS) has been losing <span class="hlt">mass</span> at an accelerating rate since the mid-1990s. This has been due to both increased <span class="hlt">ice</span> discharge into the ocean and melting at the surface, with the latter being the dominant contribution. This change in state has been attributed to rising temperatures and a decrease in surface albedo. We show, using satellite data and climate model output, that the abrupt reduction in surface <span class="hlt">mass</span> balance since about 1995 can be attributed largely to a coincident trend of decreasing summer cloud cover enhancing the melt-albedo feedback. Satellite observations show that, from 1995 to 2009, summer cloud cover decreased by 0.9 ± 0.3% per year. Model output indicates that the GrIS summer melt increases by 27 ± 13 gigatons (Gt) per percent reduction in summer cloud cover, principally because of the impact of increased shortwave radiation over the low albedo ablation zone. The observed reduction in cloud cover is strongly correlated with a state shift in the North Atlantic Oscillation promoting anticyclonic conditions in summer and suggests that the enhanced surface <span class="hlt">mass</span> loss from the GrIS is driven by synoptic-scale changes in Arctic-wide atmospheric circulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900040276&hterms=heat+exchange&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dheat%2Bexchange','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900040276&hterms=heat+exchange&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dheat%2Bexchange"><span>Late Pleistocene <span class="hlt">variations</span> in Antarctica sea <span class="hlt">ice</span>. I - Effect of orbital isolation changes. II - Effect of interhemispheric deep-ocean heat exchange</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Crowley, Thomas J.; Parkinson, Claire L.</p> <p>1988-01-01</p> <p>A dynamic-thermodynamic sea-<span class="hlt">ice</span> model is presently used to ascertain the effects of orbitally-induced insolation changes on Antarctic sea-<span class="hlt">ice</span> cover; the results thus obtained are compared with modified CLIMAP reconstructions of sea-<span class="hlt">ice</span> 18,000 years ago. The minor influence exerted by insolation on Pleistocene sea-<span class="hlt">ice</span> distributions is attributable to a number of factors. In the second part of this investigation, <span class="hlt">variations</span> in the production of warm North Atlantic Deep Water are proposed as a mechanism constituting the linkage between climate fluctuations in the Northern and Southern hemispheres during the Pleistocene; this hypothesis is tested by examining the sensitivity of the dynamic-thermodynamic model for Antarctic sea-<span class="hlt">ice</span> changes in vertical ocean heat flux, and comparing the simulations with modified CLIMAP sea-<span class="hlt">ice</span> maps for 18,000 years ago.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A13E2121S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A13E2121S"><span>Impacts of a Stochastic <span class="hlt">Ice</span> <span class="hlt">Mass</span>-Size Relationship on Squall Line Ensemble Simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stanford, M.; Varble, A.; Morrison, H.; Grabowski, W.; McFarquhar, G. M.; Wu, W.</p> <p>2017-12-01</p> <p>Cloud and precipitation structure, evolution, and cloud radiative forcing of simulated mesoscale convective systems (MCSs) are significantly impacted by <span class="hlt">ice</span> microphysics parameterizations. Most microphysics schemes assume power law relationships with constant parameters for <span class="hlt">ice</span> particle <span class="hlt">mass</span>, area, and terminal fallspeed relationships as a function of size, despite observations showing that these relationships vary in both time and space. To account for such natural variability, a stochastic representation of <span class="hlt">ice</span> microphysical parameters was developed using the Predicted Particle Properties (P3) microphysics scheme in the Weather Research and Forecasting model, guided by in situ aircraft measurements from a number of field campaigns. Here, the stochastic framework is applied to the "a" and "b" parameters of the unrimed <span class="hlt">ice</span> <span class="hlt">mass</span>-size (m-D) relationship (m=aDb) with co-varying "a" and "b" values constrained by observational distributions tested over a range of spatiotemporal autocorrelation scales. Diagnostically altering a-b pairs in three-dimensional (3D) simulations of the 20 May 2011 Midlatitude Continental Convective Clouds Experiment (MC3E) squall line suggests that these parameters impact many important characteristics of the simulated squall line, including reflectivity structure (particularly in the anvil region), surface rain rates, surface and top of atmosphere radiative fluxes, buoyancy and latent cooling distributions, and system propagation speed. The stochastic a-b P3 scheme is tested using two frameworks: (1) a large ensemble of two-dimensional idealized squall line simulations and (2) a smaller ensemble of 3D simulations of the 20 May 2011 squall line, for which simulations are evaluated using observed radar reflectivity and radial velocity at multiple wavelengths, surface meteorology, and surface and satellite measured longwave and shortwave radiative fluxes. Ensemble spreads are characterized and compared against initial condition ensemble spreads</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/1001106','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/1001106"><span><span class="hlt">Variation</span> in body <span class="hlt">mass</span> of wild canvasback and redhead ducklings</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Austin, Jane E.; Serie, Jerome R.</p> <p>1994-01-01</p> <p>We assessed <span class="hlt">variation</span> in body <span class="hlt">mass</span> of ducklings in single- and mixed-species broods of wild Canvasbacks (Aythya valisineria) and Redheads (Aythya americana) 20-50 days old. Body <span class="hlt">mass</span> of canvasback ducklings was not affected by year and season (early vs. late hatch date) despite changes in water conditions. Mean body <span class="hlt">mass</span> of male and female Canvasbacks did not differ in Class IIA but did differ in older age classes. Within-brood differences in body <span class="hlt">mass</span> tended to be higher in Class IIA ducklings (6-7% of mean body <span class="hlt">mass</span> for Canvasbacks, 9-11% in Redheads) and generally declined to 4-6% in Class IIC and older ducklings. Some within-brood differences were as high as 20-30% of mean body <span class="hlt">mass</span>. Tests to assess sources of within-brood <span class="hlt">variation</span> (age, sex, and season) in body <span class="hlt">mass</span> for Canvasbacks were inconclusive. <span class="hlt">Variation</span> within broods was generally less than that among broods for both Canvasbacks and Redheads. The lack of differences in duckling body <span class="hlt">mass</span> between single- and mixed-species broods for any age class, sex, or species suggests that <span class="hlt">mass</span> was not affected by interspecific brood parasitism.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.4521L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.4521L"><span>Long-term <span class="hlt">mass</span> <span class="hlt">variations</span> from SLR, VLBI and GPS data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Luceri, Vincenza; Sciarretta, Cecilia; Bianco, Giuseppe</p> <p>2013-04-01</p> <p>The second-degree geopotential coefficients reflect the behaviour of the Earth's inertia tensor of order 2 which describes the main <span class="hlt">mass</span> <span class="hlt">variations</span> of our planet impacting polar motion and length of day (EOP). SLR, VLBI and GPS allow the estimation of those <span class="hlt">variations</span>, either directly in the case of SLR through its dynamics, and indirectly, for all the three geodetic techniques, by deriving excitation functions from the EOP estimations. The geodetic estimates include the influence of the Earth's atmosphere and oceans, both from their <span class="hlt">mass</span> and motion components, which can be modelled using the atmospheric and oceanic angular momenta <span class="hlt">variations</span>. The different C21, S21 and C20 geodetic time series are compared in order to evaluate their coherence and their response to the <span class="hlt">mass</span> <span class="hlt">variations</span> after the removal of the motion terms. Moreover, the residual signal contents of the geodetic values, deprived by the atmospheric and oceanic <span class="hlt">mass</span> and motion components, will be investigated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017TCry...11.1501B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017TCry...11.1501B"><span>Winter <span class="hlt">mass</span> balance of Drangajökull <span class="hlt">ice</span> cap (NW Iceland) derived from satellite sub-meter stereo images</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Belart, Joaquín M. C.; Berthier, Etienne; Magnússon, Eyjólfur; Anderson, Leif S.; Pálsson, Finnur; Thorsteinsson, Thorsteinn; Howat, Ian M.; Aðalgeirsdóttir, Guðfinna; Jóhannesson, Tómas; Jarosch, Alexander H.</p> <p>2017-06-01</p> <p>Sub-meter resolution, stereoscopic satellite images allow for the generation of accurate and high-resolution digital elevation models (DEMs) over glaciers and <span class="hlt">ice</span> caps. Here, repeated stereo images of Drangajökull <span class="hlt">ice</span> cap (NW Iceland) from Pléiades and WorldView2 (WV2) are combined with in situ estimates of snow density and densification of firn and fresh snow to provide the first estimates of the glacier-wide geodetic winter <span class="hlt">mass</span> balance obtained from satellite imagery. Statistics in snow- and <span class="hlt">ice</span>-free areas reveal similar vertical relative accuracy (< 0.5 m) with and without ground control points (GCPs), demonstrating the capability for measuring seasonal snow accumulation. The calculated winter (14 October 2014 to 22 May 2015) <span class="hlt">mass</span> balance of Drangajökull was 3.33 ± 0.23 m w.e. (meter water equivalent), with ∼ 60 % of the accumulation occurring by February, which is in good agreement with nearby ground observations. On average, the repeated DEMs yield 22 % less elevation change than the length of eight winter snow cores due to (1) the time difference between in situ and satellite observations, (2) firn densification and (3) elevation changes due to <span class="hlt">ice</span> dynamics. The contributions of these three factors were of similar magnitude. This study demonstrates that seasonal geodetic <span class="hlt">mass</span> balance can, in many areas, be estimated from sub-meter resolution satellite stereo images.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017TCry...11.2655S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017TCry...11.2655S"><span>GPS-derived estimates of surface <span class="hlt">mass</span> balance and ocean-induced basal melt for Pine Island Glacier <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>Shean, David E.; Christianson, Knut; Larson, Kristine M.; Ligtenberg, Stefan R. M.; Joughin, Ian R.; Smith, Ben E.; Stevens, C. Max; Bushuk, Mitchell; Holland, David M.</p> <p>2017-11-01</p> <p>In the last 2 decades, Pine Island Glacier (PIG) experienced marked speedup, thinning, and grounding-line retreat, likely due to marine <span class="hlt">ice</span>-sheet instability and <span class="hlt">ice</span>-shelf basal melt. To better understand these processes, we combined 2008-2010 and 2012-2014 GPS records with dynamic firn model output to constrain local surface and basal <span class="hlt">mass</span> balance for PIG. We used GPS interferometric reflectometry to precisely measure absolute surface elevation (zsurf) and Lagrangian surface elevation change (Dzsurf/ Dt). Observed surface elevation relative to a firn layer tracer for the initial surface (zsurf - zsurf0') is consistent with model estimates of surface <span class="hlt">mass</span> balance (SMB, primarily snow accumulation). A relatively abrupt ˜ 0.2-0.3 m surface elevation decrease, likely due to surface melt and increased compaction rates, is observed during a period of warm atmospheric temperatures from December 2012 to January 2013. Observed Dzsurf/ Dt trends (-1 to -4 m yr-1) for the PIG shelf sites are all highly linear. Corresponding basal melt rate estimates range from ˜ 10 to 40 m yr-1, in good agreement with those derived from <span class="hlt">ice</span>-bottom acoustic ranging, phase-sensitive <span class="hlt">ice</span>-penetrating radar, and high-resolution stereo digital elevation model (DEM) records. The GPS and DEM records document higher melt rates within and near features associated with longitudinal extension (i.e., transverse surface depressions, rifts). Basal melt rates for the 2012-2014 period show limited temporal variability despite large changes in ocean temperature recorded by moorings in Pine Island Bay. Our results demonstrate the value of long-term GPS records for <span class="hlt">ice</span>-shelf <span class="hlt">mass</span> balance studies, with implications for the sensitivity of <span class="hlt">ice</span>-ocean interaction at PIG.</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://hdl.handle.net/2060/19720021734','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19720021734"><span>Microwave emission characteristics of 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>Edgerton, A. T.; Poe, G.</p> <p>1972-01-01</p> <p>A general classification is presented for sea <span class="hlt">ice</span> brightness temperatures with categories of high and low emission, corresponding to young and weathered sea <span class="hlt">ice</span>, respectively. A sea <span class="hlt">ice</span> emission model was developed which allows <span class="hlt">variations</span> of <span class="hlt">ice</span> salinity and temperature in directions perpendicular to the <span class="hlt">ice</span> surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170009395','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170009395"><span>Remote Sensing of Crystal Shapes in <span class="hlt">Ice</span> Clouds</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>van Diedenhoven, Bastiaan</p> <p>2017-01-01</p> <p><span class="hlt">Ice</span> crystals in clouds exist in a virtually limitless <span class="hlt">variation</span> of geometries. The most basic shapes of <span class="hlt">ice</span> crystals are columnar or plate-like hexagonal prisms with aspect ratios determined by relative humidity and temperature. However, crystals in <span class="hlt">ice</span> clouds generally display more complex structures owing to aggregation, riming and growth histories through varying temperature and humidity regimes. Crystal shape is relevant for cloud evolution as it affects microphysical properties such as fall speeds and aggregation efficiency. Furthermore, the scattering properties of <span class="hlt">ice</span> crystals are affected by their general shape, as well as by microscopic features such as surface roughness, impurities and internal structure. To improve the representation of <span class="hlt">ice</span> clouds in climate models, increased understanding of the global <span class="hlt">variation</span> of crystal shape and how it relates to, e.g., location, cloud temperature and atmospheric state is crucial. Here, the remote sensing of <span class="hlt">ice</span> crystal macroscale and microscale structure from airborne and space-based lidar depolarization observations and multi-directional measurements of total and polarized reflectances is reviewed. In addition, a brief overview is given of in situ and laboratory observations of <span class="hlt">ice</span> crystal shape as well as the optical properties of <span class="hlt">ice</span> crystals that serve as foundations for the remote sensing approaches. Lidar depolarization is generally found to increase with increasing cloud height and to vary with latitude. Although this <span class="hlt">variation</span> is generally linked to the <span class="hlt">variation</span> of <span class="hlt">ice</span> crystal shape, the interpretation of the depolarization remains largely qualitative and more research is needed before quantitative conclusions about <span class="hlt">ice</span> shape can be deduced. The angular <span class="hlt">variation</span> of total and polarized reflectances of <span class="hlt">ice</span> clouds has been analyzed by numerous studies in order to infer information about <span class="hlt">ice</span> crystal shapes from them. From these studies it is apparent that pristine crystals with smooth surfaces are generally</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011JGRD..116.0P03L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011JGRD..116.0P03L"><span>Latitudinal and interhemispheric <span class="hlt">variation</span> of stratospheric effects on mesospheric <span class="hlt">ice</span> layer trends</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lübken, F.-J.; Berger, U.</p> <p>2011-02-01</p> <p>Latitudinal and interhemispheric differences of model results on trends in mesospheric <span class="hlt">ice</span> layers and background conditions are analyzed. The model nudges to European Centre for Medium-Range Weather Forecasts data below ˜45 km. Greenhouse gas concentrations in the mesosphere are kept constant. Temperature trends in the mesosphere mainly come from shrinking of the stratosphere and from dynamical effects. Water vapor increases at noctilucent cloud (NLC) heights and decreases above due to increased freeze drying caused by temperature trends. There is no tendency for <span class="hlt">ice</span> clouds in the Northern Hemisphere for extending farther southward with time. Trends of NLC albedo are similar to satellite measurements, but only if a time period longer than observations is considered. <span class="hlt">Ice</span> cloud trends get smaller if albedo thresholds relevant to satellite instruments are applied, in particular at high polar latitudes. This implies that weak and moderate NLC is favored when background conditions improve for NLC formation, whereas strong NLC benefits less. Trends of <span class="hlt">ice</span> cloud parameters are generally smaller in the Southern Hemisphere (SH) compared to the Northern Hemisphere (NH), consistent with observations. Trends in background conditions have counteracting effects on NLC: temperature trends would suggest stronger <span class="hlt">ice</span> increase in the SH, and water vapor trends would suggest a weaker increase. Larger trends in NLC brightness or occurrence rates are not necessarily associated with larger (more negative) temperature trends. They can also be caused by larger trends of water vapor caused by larger freeze drying, which in turn can be caused by generally lower temperatures and/or more background water. Trends of NLC brightness and occurrence rates decrease with decreasing latitude in both hemispheres. The latitudinal <span class="hlt">variation</span> of these trends is primarily determined by induced water vapor trends. Trends in NLC altitudes are generally small. Stratospheric temperature trends vary</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14.1177S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.1177S"><span>Glacier <span class="hlt">mass</span> balance in high-arctic areas with anomalous gravity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sharov, A.; Rieser, D.; Nikolskiy, D.</p> <p>2012-04-01</p> <p>All known glaciological models describing the evolution of Arctic land- and sea-<span class="hlt">ice</span> <span class="hlt">masses</span> in changing climate treat the Earth's gravity as horizontally constant, but it isn't. In the High Arctic, the strength of the gravitational field varies considerably across even short distances under the influence of a density gradient, and the magnitude of free air gravity anomalies attains 100 mGal and more. On long-term base, instantaneous deviations of gravity can have a noticeable effect on the regime and <span class="hlt">mass</span> budget of glaciological objects. At best, the gravity-induced component of <span class="hlt">ice</span> <span class="hlt">mass</span> <span class="hlt">variations</span> can be determined on topographically smooth, open and steady surfaces, like those of arctic planes, regular <span class="hlt">ice</span> caps and landfast sea <span class="hlt">ice</span>. The present research is devoted to studying gravity-driven impacts on glacier <span class="hlt">mass</span> balance in the outer periphery of four Eurasian shelf seas with a very cold, dry climate and rather episodic character of winter precipitation. As main study objects we had chosen a dozen Russia's northernmost insular <span class="hlt">ice</span> caps, tens to hundreds of square kilometres in extent, situated in a close vicinity of strong gravity anomalies and surrounded with extensive fields of fast and/or drift <span class="hlt">ice</span> for most of the year. The supposition about gravitational forcing on glacioclimatic settings in the study region is based on the results of quantitative comparison and joint interpretation of existing glacier change maps and available data on the Arctic gravity field and solid precipitation. The overall mapping of medium-term (from decadal to half-centennial) changes in glacier volumes and quantification of <span class="hlt">mass</span> balance characteristics in the study region was performed by comparing reference elevation models of study glaciers derived from Russian topographic maps 1:200,000 (CI = 20 or 40 m) representing the glacier state as in the 1950s-1980s with modern elevation data obtained from satellite radar interferometry and lidar altimetry. Free-air gravity anomalies were</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C51C0998K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C51C0998K"><span><span class="hlt">Variations</span> in West Antarctic <span class="hlt">Ice</span> Front and Passive Microwave Brightness Temperature for 8 Years Duration in 2000s</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kim, J.; Yu, J.; Wang, L.; Liu, H.</p> <p>2017-12-01</p> <p>Changes in Antarctic <span class="hlt">ice</span> sheet are caused by various reasons such as changes in Holocene climate, precipitation, and ocean temperature. Such issues of changes in <span class="hlt">ice</span> sheet has been mainly focused on the Antarctic peninsula, and it is known that <span class="hlt">ice</span> retreat of the area is caused by changes in atmospheric and ocean temperatures. For the case of West Antarctica, <span class="hlt">ice</span> front change research is relatively rarely conducted except the Pine island glacier area. This study has monitored <span class="hlt">ice</span> front changes of West Antarctica and compared the patterns with the changes in brightness temperature based on remote sensing techniques. We used 2000 Radarsat-1 and 2008 Rasarsat-2 SAR data to delineate coastlines of whole West Antarctica based on the locally thresholding adaptive algorithm. The delineated coast lines are analyzed to figure out <span class="hlt">ice</span> front change patterns between the duration. The <span class="hlt">variations</span> in brightness temperature for the same duration are calculated based on Defense Meteorological Satellite Program (DMSP)'s Special Sensor Microwave/Images-Special Sensor Microwave Imager/Sounder (SSM/I-SSMIS) passive microwave data. The results show <span class="hlt">ice</span> front of West Antarctica shows advancing trend except the pine island glacier area. The brightness temperature had decreasing trend during the study period. It infers that changes in <span class="hlt">ice</span> front and brightness temperature of West Antarctica have considerable relationships. It is expected that a long term monitoring of the relationship would contribute understanding <span class="hlt">ice</span> dynamics of West Antarctica significantly.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRF..122..167M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRF..122..167M"><span>Tidally induced <span class="hlt">variations</span> in vertical and horizontal motion on Rutford <span class="hlt">Ice</span> Stream, West Antarctica, inferred from remotely sensed observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Minchew, B. M.; Simons, M.; Riel, B.; Milillo, P.</p> <p>2017-01-01</p> <p>To better understand the influence of stress changes over floating <span class="hlt">ice</span> shelves on grounded <span class="hlt">ice</span> streams, we develop a Bayesian method for inferring time-dependent 3-D surface velocity fields from synthetic aperture radar (SAR) and optical remote sensing data. Our specific goal is to observe ocean tide-induced variability in vertical <span class="hlt">ice</span> shelf position and horizontal <span class="hlt">ice</span> stream flow. Thus, we consider the special case where observed surface displacement at a given location can be defined by a 3-D secular velocity vector, a family of 3-D sinusoidal functions, and a correction to the digital elevation model used to process the SAR data. Using nearly 9 months of SAR data collected from multiple satellite viewing geometries with the COSMO-SkyMed 4-satellite constellation, we infer the spatiotemporal response of Rutford <span class="hlt">Ice</span> Stream, West Antarctica, to ocean tidal forcing. Consistent with expected tidal uplift, inferred vertical motion over the <span class="hlt">ice</span> shelf is dominated by semidiurnal and diurnal tidal constituents. Horizontal <span class="hlt">ice</span> flow variability, on the other hand, occurs primarily at the fortnightly spring-neap tidal period (Msf). We propose that periodic grounding of the <span class="hlt">ice</span> shelf is the primary mechanism for translating vertical tidal motion into horizontal flow variability, causing <span class="hlt">ice</span> flow to accelerate first and most strongly over the <span class="hlt">ice</span> shelf. Flow <span class="hlt">variations</span> then propagate through the grounded <span class="hlt">ice</span> stream at a mean rate of ˜29 km/d and decay quasi-linearly with distance over ˜85 km upstream of the grounding zone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=dielectrics&pg=3&id=EJ196723','ERIC'); return false;" href="https://eric.ed.gov/?q=dielectrics&pg=3&id=EJ196723"><span>Experiments in <span class="hlt">Ice</span> Physics.</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Martin, P. F.; And Others</p> <p>1978-01-01</p> <p>Describes experiments in <span class="hlt">ice</span> physics that demonstrate the behavior and properties of <span class="hlt">ice</span>. Show that <span class="hlt">ice</span> behaves as an ionic conductor in which charge is transferred by the movement of protons, its electrical conductivity is highly temperature-dependent, and its dielectric properties show dramatic <span class="hlt">variation</span> in the kilohertz range. (Author/GA)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70074654','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70074654"><span>Seismicity within a propagating <span class="hlt">ice</span> shelf rift: the relationship between icequake locations and <span class="hlt">ice</span> shelf structure</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Heeszel, David S.; Fricker, Helen A.; Bassis, Jeremy N.; O'Neel, Shad; Walter, Fabian</p> <p>2014-01-01</p> <p>Iceberg calving is a dominant <span class="hlt">mass</span> loss mechanism for Antarctic <span class="hlt">ice</span> shelves, second only to basal melting. An important known process involved in calving is the initiation and propagation of through-penetrating fractures called rifts; however, the mechanisms controlling rift propagation remain poorly understood. To investigate the mechanics of <span class="hlt">ice</span>-shelf rifting, we analyzed seismicity associated with a propagating rift tip on the Amery <span class="hlt">Ice</span> Shelf, using data collected during the Austral summers of 2004-2007. We investigated seismicity associated with fracture propagation using a suite of passive seismological techniques including icequake locations, back projection, and moment tensor inversion. We confirm previous results that show that seismicity is characterized by periods of relative quiescence punctuated by swarms of intense seismicity of one to three hours. However, even during periods of quiescence, we find significant seismic deformation around the rift tip. Moment tensors, calculated for a subset of the largest icequakes (MW > -2.0) located near the rift tip, show steeply dipping fault planes, horizontal or shallowly plunging stress orientations, and often have a significant volumetric component. They also reveal that much of the observed seismicity is limited to the upper 50 m of the <span class="hlt">ice</span> shelf. This suggests a complex system of deformation that involves the propagating rift, the region behind the rift tip, and a system of rift-transverse crevasses. Small-scale <span class="hlt">variations</span> in the mechanical structure of the <span class="hlt">ice</span> shelf, especially rift-transverse crevasses and accreted marine <span class="hlt">ice</span>, play an important role in modulating the rate and location of seismicity associated with propagating <span class="hlt">ice</span> shelf rifts.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.8479X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.8479X"><span><span class="hlt">Ice</span> particle <span class="hlt">mass</span>-dimensional parameter retrieval and uncertainty analysis using an Optimal Estimation framework applied to in situ data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xu, Zhuocan; Mace, Jay; Avalone, Linnea; Wang, Zhien</p> <p>2015-04-01</p> <p>The extreme variability of <span class="hlt">ice</span> particle habits in precipitating clouds affects our understanding of these cloud systems in every aspect (i.e. radiation transfer, dynamics, precipitation rate, etc) and largely contributes to the uncertainties in the model representation of related processes. <span class="hlt">Ice</span> particle <span class="hlt">mass</span>-dimensional power law relationships, M=a*(D ^ b), are commonly assumed in models and retrieval algorithms, while very little knowledge exists regarding the uncertainties of these M-D parameters in real-world situations. In this study, we apply Optimal Estimation (OE) methodology to infer <span class="hlt">ice</span> particle <span class="hlt">mass</span>-dimensional relationship from <span class="hlt">ice</span> particle size distributions and bulk water contents independently measured on board the University of Wyoming King Air during the Colorado Airborne Multi-Phase Cloud Study (CAMPS). We also utilize W-band radar reflectivity obtained on the same platform (King Air) offering a further constraint to this ill-posed problem (Heymsfield et al. 2010). In addition to the values of retrieved M-D parameters, the associated uncertainties are conveniently acquired in the OE framework, within the limitations of assumed Gaussian statistics. We find, given the constraints provided by the bulk water measurement and in situ radar reflectivity, that the relative uncertainty of <span class="hlt">mass</span>-dimensional power law prefactor (a) is approximately 80% and the relative uncertainty of exponent (b) is 10-15%. With this level of uncertainty, the forward model uncertainty in radar reflectivity would be on the order of 4 dB or a factor of approximately 2.5 in <span class="hlt">ice</span> water content. The implications of this finding are that inferences of bulk water from either remote or in situ measurements of particle spectra cannot be more certain than this when the <span class="hlt">mass</span>-dimensional relationships are not known a priori which is almost never the case.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3597251','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3597251"><span>Seasonal sea <span class="hlt">ice</span> cover as principal driver of spatial and temporal <span class="hlt">variation</span> in depth extension and annual production of kelp in Greenland</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Krause-Jensen, Dorte; Marbà, Núria; Olesen, Birgit; Sejr, Mikael K; Christensen, Peter Bondo; Rodrigues, João; Renaud, Paul E; Balsby, Thorsten JS; Rysgaard, Søren</p> <p>2012-01-01</p> <p>We studied the depth distribution and production of kelp along the Greenland coast spanning Arctic to sub-Arctic conditions from 78 °N to 64 °N. This covers a wide range of sea <span class="hlt">ice</span> conditions and water temperatures, with those presently realized in the south likely to move northwards in a warmer future. Kelp forests occurred along the entire latitudinal range, and their depth extension and production increased southwards presumably in response to longer annual <span class="hlt">ice</span>-free periods and higher water temperature. The depth limit of 10% kelp cover was 9–14 m at the northernmost sites (77–78 °N) with only 94–133 <span class="hlt">ice</span>-free days per year, but extended to depths of 21–33 m further south (73 °N–64 °N) where >160 days per year were <span class="hlt">ice</span>-free, and annual production of Saccharina longicruris and S. latissima, measured as the size of the annual blade, ranged up to sevenfold among sites. The duration of the open-water period, which integrates light and temperature conditions on an annual basis, was the best predictor (relative to summer water temperature) of kelp production along the latitude gradient, explaining up to 92% of the <span class="hlt">variation</span> in depth extension and 80% of the <span class="hlt">variation</span> in kelp production. In a decadal time series from a high Arctic site (74 °N), inter-annual <span class="hlt">variation</span> in sea <span class="hlt">ice</span> cover also explained a major part (up to 47%) of the <span class="hlt">variation</span> in kelp production. Both spatial and temporal data sets thereby support the prediction that northern kelps will play a larger role in the coastal marine ecosystem in a warmer future as the length of the open-water period increases. As kelps increase carbon-flow and habitat diversity, an expansion of kelp forests may exert cascading effects on the coastal Arctic ecosystem. PMID:28741817</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28741817','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28741817"><span>Seasonal sea <span class="hlt">ice</span> cover as principal driver of spatial and temporal <span class="hlt">variation</span> in depth extension and annual production of kelp in Greenland.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Krause-Jensen, Dorte; Marbà, Núria; Olesen, Birgit; Sejr, Mikael K; Christensen, Peter Bondo; Rodrigues, João; Renaud, Paul E; Balsby, Thorsten J S; Rysgaard, Søren</p> <p>2012-10-01</p> <p>We studied the depth distribution and production of kelp along the Greenland coast spanning Arctic to sub-Arctic conditions from 78 ºN to 64 ºN. This covers a wide range of sea <span class="hlt">ice</span> conditions and water temperatures, with those presently realized in the south likely to move northwards in a warmer future. Kelp forests occurred along the entire latitudinal range, and their depth extension and production increased southwards presumably in response to longer annual <span class="hlt">ice</span>-free periods and higher water temperature. The depth limit of 10% kelp cover was 9-14 m at the northernmost sites (77-78 ºN) with only 94-133 <span class="hlt">ice</span>-free days per year, but extended to depths of 21-33 m further south (73 ºN-64 ºN) where >160 days per year were <span class="hlt">ice</span>-free, and annual production of Saccharina longicruris and S. latissima, measured as the size of the annual blade, ranged up to sevenfold among sites. The duration of the open-water period, which integrates light and temperature conditions on an annual basis, was the best predictor (relative to summer water temperature) of kelp production along the latitude gradient, explaining up to 92% of the <span class="hlt">variation</span> in depth extension and 80% of the <span class="hlt">variation</span> in kelp production. In a decadal time series from a high Arctic site (74 ºN), inter-annual <span class="hlt">variation</span> in sea <span class="hlt">ice</span> cover also explained a major part (up to 47%) of the <span class="hlt">variation</span> in kelp production. Both spatial and temporal data sets thereby support the prediction that northern kelps will play a larger role in the coastal marine ecosystem in a warmer future as the length of the open-water period increases. As kelps increase carbon-flow and habitat diversity, an expansion of kelp forests may exert cascading effects on the coastal Arctic ecosystem. © 2012 Blackwell Publishing Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016TCry...10..811D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016TCry...10..811D"><span>Constraining variable density of <span class="hlt">ice</span> shelves using wide-angle radar measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Drews, Reinhard; Brown, Joel; Matsuoka, Kenichi; Witrant, Emmanuel; Philippe, Morgane; Hubbard, Bryn; Pattyn, Frank</p> <p>2016-04-01</p> <p>The thickness of <span class="hlt">ice</span> shelves, a basic parameter for <span class="hlt">mass</span> balance estimates, is typically inferred using hydrostatic equilibrium, for which knowledge of the depth-averaged density is essential. The densification from snow to <span class="hlt">ice</span> depends on a number of local factors (e.g., temperature and surface <span class="hlt">mass</span> balance) causing spatial and temporal <span class="hlt">variations</span> in density-depth profiles. However, direct measurements of firn density are sparse, requiring substantial logistical effort. Here, we infer density from radio-wave propagation speed using ground-based wide-angle radar data sets (10 MHz) collected at five sites on Roi Baudouin <span class="hlt">Ice</span> Shelf (RBIS), Dronning Maud Land, Antarctica. We reconstruct depth to internal reflectors, local <span class="hlt">ice</span> thickness, and firn-air content using a novel algorithm that includes traveltime inversion and ray tracing with a prescribed shape of the depth-density relationship. For the particular case of an <span class="hlt">ice</span>-shelf channel, where <span class="hlt">ice</span> thickness and surface slope change substantially over a few kilometers, the radar data suggest that firn inside the channel is about 5 % denser than outside the channel. Although this density difference is at the detection limit of the radar, it is consistent with a similar density anomaly reconstructed from optical televiewing, which reveals that the firn inside the channel is 4.7 % denser than that outside the channel. Hydrostatic <span class="hlt">ice</span> thickness calculations used for determining basal melt rates should account for the denser firn in <span class="hlt">ice</span>-shelf channels. The radar method presented here is robust and can easily be adapted to different radar frequencies and data-acquisition geometries.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.C31E0470D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.C31E0470D"><span>The <span class="hlt">variation</span> of polar firn subject to percolation - characterizing processes and glacier <span class="hlt">mass</span> budget uncertainty using high-resolution instruments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Demuth, M. N.; Marshall, H.; Morris, E. M.; Burgess, D. O.; Gray, L.</p> <p>2009-12-01</p> <p>As the Earth's glaciers and <span class="hlt">ice</span> sheets are subjected to the effects of recent and predicted warming, the distribution of their glaciological facies zones will alter. Percolation and wet snow facies zones will, in general, move upwards; encroaching upon, for some glacier configurations, regions of dry snow facies. Meltwater percolation and internal accumulation processes that characterize these highly variable facies may confound reliable estimates of surface <span class="hlt">mass</span> budgets based on traditional point measurements alone. If the extents of these zones are indeed increasing, as has been documented through recent analysis of QuickScat data for the <span class="hlt">ice</span> caps of the Canadian Arctic, then the certainty of glacier <span class="hlt">mass</span> budget estimates using traditional techniques may be degraded to an as yet un-quantified degree. Indeed, the application of remote sensing, in particular that utilizing repeat altimetry to retrieve surface <span class="hlt">mass</span> budget estimates, is also subject to the complexity of glacier facies from the standpoint of their near-surface stratigraphy, density <span class="hlt">variations</span> and rates of compaction. We first review the problem of measuring glacier <span class="hlt">mass</span> budgets in the context of nested scales of variability, where auto-correlation structure varies with the scale of observation. We then consider specifically firn subject to percolation and describe the application of high-resolution instruments to characterize variability at the field-scale. The data collected include measurements of micro-topography, snow hardness, and snow density and texture; retrieved using airborne scanning lidar, a snow micro-penetrometer, neutron probe and ground-penetrating radars. The analysis suggests corresponding scales of correlation as it concerns the influence of antecedent conditions (surface roughness and hardness, and stratigraphic variability) and post-depositional processes (percolation and refreezing of surface melt water).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP51B1063A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP51B1063A"><span>Reconstructing Holocene Summer Sea-<span class="hlt">Ice</span> Conditions in the Central and Western Arctic Ocean: Morphological <span class="hlt">Variations</span> and Stable Isotope Composition of Neogloboquadrina pachyderma</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Asahi, H.; Nam, S. I.; Stein, R. H.; Mackensen, A.; Son, Y. J.</p> <p>2017-12-01</p> <p>The usability of planktic foraminiferal census data in Arctic paleoceanography is limited by the predominance of Neogloboquadrina pachyderma (sinistral). Though a potential usability of their morphological <span class="hlt">variation</span> has been suggested by recent studies, its application is restricted to the central part of the Arctic Ocean. Here we present their regional distribution, using 80 surface sediment samples from the central and the western Arctic Ocean. Among seven morphological <span class="hlt">variations</span> encountered, distinct presence of "large-sized" N. pachyderma morphotypes at the summer sea-<span class="hlt">ice</span> edge in the western Arctic demonstrates its strong potential as sea-<span class="hlt">ice</span> distribution indicator. Based on their regional patterns, we further developed planktic foraminifer (PF)-based transfer functions (TFs) to reconstruct summer surface-water temperature, salinity and sea-<span class="hlt">ice</span> concentration in the western and central Arctic. The comparison of sea-<span class="hlt">ice</span> reconstructions by PF-based TF to other pre-existed approaches showed their recognizable advantages/disadvantages: the PF-based approach in the nearby/within heavily <span class="hlt">ice</span>-covered region, the dinocyst-based approach in the extensively seasonal <span class="hlt">ice</span> retreat region, and the IP25-based approach with overall reflection over a wide range of sea-<span class="hlt">ice</span> coverage, which is likely attributed to their (a) taphonomical information-loss, (b) different seasonal production patterns or combination of both. The application of these TFs on a sediment core from Northwind Ridge suggests general warming, freshening, and sea-<span class="hlt">ice</span> reduction after 6.0 ka. This generally agrees with PF stable isotope records and sea-<span class="hlt">ice</span> reconstructions from dinocyst-based TF at proximal locations, indicating that the sea-<span class="hlt">ice</span> behavior at the Northwind Ridge is notably different from the IP25-based sea-<span class="hlt">ice</span> reconstructions reported from elsewhere in the Arctic Ocean. Lack of regional coverage of PF-based reconstructions hampers further discussion whether the observed inconsistency is simply</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70012715','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70012715"><span>Time-dependence of sea-<span class="hlt">ice</span> concentration and multiyear <span class="hlt">ice</span> fraction in the Arctic Basin</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Gloersen, P.; Zwally, H.J.; Chang, A.T.C.; Hall, D.K.; Campbell, W.J.; Ramseier, R.O.</p> <p>1978-01-01</p> <p>The time <span class="hlt">variation</span> of the sea-<span class="hlt">ice</span> concentration and multiyear <span class="hlt">ice</span> fraction within the pack <span class="hlt">ice</span> in the Arctic Basin is examined, using microwave images of sea <span class="hlt">ice</span> recently acquired by the Nimbus-5 spacecraft and the NASA CV-990 airborne laboratory. The images used for these studies were constructed from data acquired from the Electrically Scanned Microwave Radiometer (ESMR) which records radiation from earth and its atmosphere at a wavelength of 1.55 cm. Data are analyzed for four seasons during 1973-1975 to illustrate some basic differences in the properties of the sea <span class="hlt">ice</span> during those times. Spacecraft data are compared with corresponding NASA CV-990 airborne laboratory data obtained over wide areas in the Arctic Basin during the Main Arctic <span class="hlt">Ice</span> Dynamics Joint Experiment (1975) to illustrate the applicability of passive-microwave remote sensing for monitoring the time dependence of sea-<span class="hlt">ice</span> concentration (divergence). These observations indicate significant <span class="hlt">variations</span> in the sea-<span class="hlt">ice</span> concentration in the spring, late fall and early winter. In addition, deep in the interior of the Arctic polar sea-<span class="hlt">ice</span> pack, heretofore unobserved large areas, several hundred kilometers in extent, of sea-<span class="hlt">ice</span> concentrations as low as 50% are indicated. ?? 1978 D. Reidel Publishing Company.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMED34A..05S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMED34A..05S"><span>Incorporating Geodetic Data in Introductory Geoscience Classrooms through UNAVCO's GETSI "<span class="hlt">Ice</span> <span class="hlt">Mass</span> and Sea Level Changes" Module</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stearns, L. A.; Walker, B.; Pratt-Sitaula, B.</p> <p>2015-12-01</p> <p>GETSI (Geodesy Tools for Societal Issues) is an NSF-funded partnership program between UNAVCO, Indiana University, Mt. San Antonio College, and the Science Education Resource Center (SERC). We present results from classroom testing and assessment of the GETSI <span class="hlt">Ice</span> <span class="hlt">Mass</span> and Sea Level Changes module that utilizes geodetic data to teach about <span class="hlt">ice</span> sheet <span class="hlt">mass</span> loss in introductory undergraduate courses. The module explores the interactions between global sea level rise, Greenland <span class="hlt">ice</span> <span class="hlt">mass</span> loss, and the response of the solid Earth. It brings together topics typically addressed in introductory Earth science courses (isostatic rebound, geologic measurements, and climate change) in a way that highlights the interconnectivity of the Earth system and the interpretation of geodetic data. The module was tested 3 times at 3 different institution types (R1 institution, comprehensive university, and community college), and formative and summative assessment data were obtained. We will provide an overview of the instructional materials, describe our teaching methods, and discuss how formative and summative assessment data assisted in revisions of the teaching materials and changes in our pedagogy during subsequent implementation of the module. We will also provide strategies for faculty who wish to incorporate the module into their curricula. Instructional materials, faculty and student resources, and implementation tips are freely available on the GETSI website.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70015528','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70015528"><span><span class="hlt">Mass</span> balance and sliding velocity of the Puget lobe of the cordilleran <span class="hlt">ice</span> sheet during the last glaciation</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Booth, D.B.</p> <p>1986-01-01</p> <p>An estimate of the sliding velocity and basal meltwater discharge of the Puget lobe of the Cordilleran <span class="hlt">ice</span> sheet can be calculated from its reconstructed extent, altitude, and <span class="hlt">mass</span> balance. Lobe dimensions and surface altitudes are inferred from <span class="hlt">ice</span> limits and flow-direction indicators. Net annual <span class="hlt">mass</span> balance and total ablation are calculated from relations empirically derived from modern maritime glaciers. An equilibrium-line altitude between 1200 and 1250 m is calculated for the maximum glacial advance (ca. 15,000 yr B.P.) during the Vashon Stade of the Fraser Glaciation. This estimate is in accord with geologic data and is insensitive to plausible variability in the parameters used in the reconstruction. Resultant sliding velocities are as much as 650 m/a at the equilibrium line, decreasing both up- and downglacier. Such velocities for an <span class="hlt">ice</span> sheet of this size are consistent with nonsurging behavior. Average meltwater discharge increases monotonically downglacier to 3000 m3/sec at the terminus and is of a comparable magnitude to <span class="hlt">ice</span> discharge over much of the glacier's ablation area. Palcoclimatic inferences derived from this reconstruction are consistent with previous, independently derived studies of late Pleistocene temperature and precipitation in the Pacific Northwest. ?? 1986.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AtmRe.107...42B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AtmRe.107...42B"><span>Aerosol size distribution at Nansen <span class="hlt">Ice</span> Sheet Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Belosi, F.; Contini, D.; Donateo, A.; Santachiara, G.; Prodi, F.</p> <p>2012-04-01</p> <p>During austral summer 2006, in the framework of the XXII Italian Antarctic expedition of PNRA (Italian National Program for Research in Antarctica), aerosol particle number size distribution measurements were performed in the 10-500 range nm over the Nansen <span class="hlt">Ice</span> Sheet glacier (NIS, 74°30' S, 163°27' E; 85 m a.s.l), a permanently <span class="hlt">iced</span> branch of the Ross Sea. Observed total particle number concentrations varied between 169 and 1385 cm- 3. A monomodal number size distribution, peaking at about 70 nm with no <span class="hlt">variation</span> during the day, was observed for continental air <span class="hlt">mass</span>, high wind speed and low relative humidity. Trimodal number size distributions were also observed, in agreement with measurements performed at Aboa station, which is located on the opposite side of the Antarctic continent to the NIS. In this case new particle formation, with subsequent particle growth up to about 30 nm, was observed even if not associated with maritime air <span class="hlt">masses</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRD..122.3396H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRD..122.3396H"><span>Examining impacts of <span class="hlt">mass</span>-diameter (m-D) and area-diameter (A-D) relationships of <span class="hlt">ice</span> particles on retrievals of effective radius and <span class="hlt">ice</span> water content from radar and lidar measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ham, Seung-Hee; Kato, Seiji; Rose, Fred G.</p> <p>2017-03-01</p> <p><span class="hlt">Mass</span>-diameter (m-D) and projected area-diameter (A-D) relations are often used to describe the shape of nonspherical <span class="hlt">ice</span> particles. This study analytically investigates how retrieved effective radius (reff) and <span class="hlt">ice</span> water content (IWC) from radar and lidar measurements depend on the assumption of m-D [m(D) = a Db] and A-D [A(D) = γ Dδ] relationships. We assume that unattenuated reflectivity factor (Z) and visible extinction coefficient (kext) by cloud particles are available from the radar and lidar measurements, respectively. A sensitivity test shows that reff increases with increasing a, decreasing b, decreasing γ, and increasing δ. It also shows that a 10% <span class="hlt">variation</span> of a, b, γ, and δ induces more than a 100% change of reff. In addition, we consider both gamma and lognormal particle size distributions (PSDs) and examine the sensitivity of reff to the assumption of PSD. It is shown that reff increases by up to 10% with increasing dispersion (μ) of the gamma PSD by 2, when large <span class="hlt">ice</span> particles are predominant. Moreover, reff decreases by up to 20% with increasing the width parameter (ω) of the lognormal PSD by 0.1. We also derive an analytic conversion equation between two effective radii when different particle shapes and PSD assumptions are used. When applying the conversion equation to nine types of m-D and A-D relationships, reff easily changes up to 30%. The proposed reff conversion method can be used to eliminate the inconsistency of assumptions that made in a cloud retrieval algorithm and a forward radiative transfer model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ISPAr41B7..585X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ISPAr41B7..585X"><span>Extraction of <span class="hlt">Ice</span> Sheet Layers from Two Intersected Radar Echograms Near Neem <span class="hlt">Ice</span> Core in Greenland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xiong, S.; Muller, J.-P.</p> <p>2016-06-01</p> <p>Accumulation of snow and <span class="hlt">ice</span> over time result in <span class="hlt">ice</span> sheet layers. These can be remotely sensed where there is a contrast in electromagnetic properties, which reflect <span class="hlt">variations</span> of the <span class="hlt">ice</span> density, acidity and fabric orientation. Internal <span class="hlt">ice</span> layers are assumed to be isochronous, deep beneath the <span class="hlt">ice</span> surface, and parallel to the direction of <span class="hlt">ice</span> flow. The distribution of internal layers is related to <span class="hlt">ice</span> sheet dynamics, such as the basal melt rate, basal elevation <span class="hlt">variation</span> and changes in <span class="hlt">ice</span> flow mode, which are important parameters to model the <span class="hlt">ice</span> sheet. Radar echo sounder is an effective instrument used to study the sedimentology of the Earth and planets. <span class="hlt">Ice</span> Penetrating Radar (IPR) is specific kind of radar echo sounder, which extends studies of <span class="hlt">ice</span> sheets from surface to subsurface to deep internal <span class="hlt">ice</span> sheets depending on the frequency utilised. In this study, we examine a study site where folded <span class="hlt">ice</span> occurs in the internal <span class="hlt">ice</span> sheet south of the North Greenland Eemian <span class="hlt">ice</span> drilling (NEEM) station, where two intersected radar echograms acquired by the Multi-channel Coherent Radar Depth Sounder (MCoRDS) employed in the NASA's Operation <span class="hlt">Ice</span>Bridge (OIB) mission imaged this folded <span class="hlt">ice</span>. We propose a slice processing flow based on a Radon Transform to trace and extract these two sets of curved <span class="hlt">ice</span> sheet layers, which can then be viewed in 3-D, demonstrating the 3-D structure of the <span class="hlt">ice</span> folds.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_14 --> <div id="page_15" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="281"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PNAS..113.3453L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PNAS..113.3453L"><span>Antarctic <span class="hlt">ice</span> sheet sensitivity to atmospheric CO2 <span class="hlt">variations</span> in the early to mid-Miocene</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Levy, Richard; Harwood, David; Florindo, Fabio; Sangiorgi, Francesca; Tripati, Robert; von Eynatten, Hilmar; Gasson, Edward; Kuhn, Gerhard; Tripati, Aradhna; DeConto, Robert; Fielding, Christopher; Field, Brad; Golledge, Nicholas; McKay, Robert; Naish, Timothy; Olney, Matthew; Pollard, David; Schouten, Stefan; Talarico, Franco; Warny, Sophie; Willmott, Veronica; Acton, Gary; Panter, Kurt; Paulsen, Timothy; Taviani, Marco; SMS Science Team; Acton, Gary; Askin, Rosemary; Atkins, Clifford; Bassett, Kari; Beu, Alan; Blackstone, Brian; Browne, Gregory; Ceregato, Alessandro; Cody, Rosemary; Cornamusini, Gianluca; Corrado, Sveva; DeConto, Robert; Del Carlo, Paola; Di Vincenzo, Gianfranco; Dunbar, Gavin; Falk, Candice; Field, Brad; Fielding, Christopher; Florindo, Fabio; Frank, Tracy; Giorgetti, Giovanna; Grelle, Thomas; Gui, Zi; Handwerger, David; Hannah, Michael; Harwood, David M.; Hauptvogel, Dan; Hayden, Travis; Henrys, Stuart; Hoffmann, Stefan; Iacoviello, Francesco; Ishman, Scott; Jarrard, Richard; Johnson, Katherine; Jovane, Luigi; Judge, Shelley; Kominz, Michelle; Konfirst, Matthew; Krissek, Lawrence; Kuhn, Gerhard; Lacy, Laura; Levy, Richard; Maffioli, Paola; Magens, Diana; Marcano, Maria C.; Millan, Cristina; Mohr, Barbara; Montone, Paola; Mukasa, Samuel; Naish, Timothy; Niessen, Frank; Ohneiser, Christian; Olney, Mathew; Panter, Kurt; Passchier, Sandra; Patterson, Molly; Paulsen, Timothy; Pekar, Stephen; Pierdominici, Simona; Pollard, David; Raine, Ian; Reed, Joshua; Reichelt, Lucia; Riesselman, Christina; Rocchi, Sergio; Sagnotti, Leonardo; Sandroni, Sonia; Sangiorgi, Francesca; Schmitt, Douglas; Speece, Marvin; Storey, Bryan; Strada, Eleonora; Talarico, Franco; Taviani, Marco; Tuzzi, Eva; Verosub, Kenneth; von Eynatten, Hilmar; Warny, Sophie; Wilson, Gary; Wilson, Terry; Wonik, Thomas; Zattin, Massimiliano</p> <p>2016-03-01</p> <p>Geological records from the Antarctic margin offer direct evidence of environmental variability at high southern latitudes and provide insight regarding <span class="hlt">ice</span> sheet sensitivity to past climate change. The early to mid-Miocene (23-14 Mya) is a compelling interval to study as global temperatures and atmospheric CO2 concentrations were similar to those projected for coming centuries. Importantly, this time interval includes the Miocene Climatic Optimum, a period of global warmth during which average surface temperatures were 3-4 °C higher than today. Miocene sediments in the ANDRILL-2A drill core from the Western Ross Sea, Antarctica, indicate that the Antarctic <span class="hlt">ice</span> sheet (AIS) was highly variable through this key time interval. A multiproxy dataset derived from the core identifies four distinct environmental motifs based on changes in sedimentary facies, fossil assemblages, geochemistry, and paleotemperature. Four major disconformities in the drill core coincide with regional seismic discontinuities and reflect transient expansion of grounded <span class="hlt">ice</span> across the Ross Sea. They correlate with major positive shifts in benthic oxygen isotope records and generally coincide with intervals when atmospheric CO2 concentrations were at or below preindustrial levels (˜280 ppm). Five intervals reflect <span class="hlt">ice</span> sheet minima and air temperatures warm enough for substantial <span class="hlt">ice</span> <span class="hlt">mass</span> loss during episodes of high (˜500 ppm) atmospheric CO2. These new drill core data and associated <span class="hlt">ice</span> sheet modeling experiments indicate that polar climate and the AIS were highly sensitive to relatively small changes in atmospheric CO2 during the early to mid-Miocene.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4822588','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4822588"><span>Antarctic <span class="hlt">ice</span> sheet sensitivity to atmospheric CO2 <span class="hlt">variations</span> in the early to mid-Miocene</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Levy, Richard; Harwood, David; Florindo, Fabio; Sangiorgi, Francesca; Tripati, Robert; von Eynatten, Hilmar; Tripati, Aradhna; DeConto, Robert; Fielding, Christopher; Field, Brad; Golledge, Nicholas; McKay, Robert; Naish, Timothy; Olney, Matthew; Pollard, David; Schouten, Stefan; Talarico, Franco; Warny, Sophie; Willmott, Veronica; Acton, Gary; Panter, Kurt; Paulsen, Timothy; Taviani, Marco</p> <p>2016-01-01</p> <p>Geological records from the Antarctic margin offer direct evidence of environmental variability at high southern latitudes and provide insight regarding <span class="hlt">ice</span> sheet sensitivity to past climate change. The early to mid-Miocene (23–14 Mya) is a compelling interval to study as global temperatures and atmospheric CO2 concentrations were similar to those projected for coming centuries. Importantly, this time interval includes the Miocene Climatic Optimum, a period of global warmth during which average surface temperatures were 3–4 °C higher than today. Miocene sediments in the ANDRILL-2A drill core from the Western Ross Sea, Antarctica, indicate that the Antarctic <span class="hlt">ice</span> sheet (AIS) was highly variable through this key time interval. A multiproxy dataset derived from the core identifies four distinct environmental motifs based on changes in sedimentary facies, fossil assemblages, geochemistry, and paleotemperature. Four major disconformities in the drill core coincide with regional seismic discontinuities and reflect transient expansion of grounded <span class="hlt">ice</span> across the Ross Sea. They correlate with major positive shifts in benthic oxygen isotope records and generally coincide with intervals when atmospheric CO2 concentrations were at or below preindustrial levels (∼280 ppm). Five intervals reflect <span class="hlt">ice</span> sheet minima and air temperatures warm enough for substantial <span class="hlt">ice</span> <span class="hlt">mass</span> loss during episodes of high (∼500 ppm) atmospheric CO2. These new drill core data and associated <span class="hlt">ice</span> sheet modeling experiments indicate that polar climate and the AIS were highly sensitive to relatively small changes in atmospheric CO2 during the early to mid-Miocene. PMID:26903644</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26903644','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26903644"><span>Antarctic <span class="hlt">ice</span> sheet sensitivity to atmospheric CO2 <span class="hlt">variations</span> in the early to mid-Miocene.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Levy, Richard; Harwood, David; Florindo, Fabio; Sangiorgi, Francesca; Tripati, Robert; von Eynatten, Hilmar; Gasson, Edward; Kuhn, Gerhard; Tripati, Aradhna; DeConto, Robert; Fielding, Christopher; Field, Brad; Golledge, Nicholas; McKay, Robert; Naish, Timothy; Olney, Matthew; Pollard, David; Schouten, Stefan; Talarico, Franco; Warny, Sophie; Willmott, Veronica; Acton, Gary; Panter, Kurt; Paulsen, Timothy; Taviani, Marco</p> <p>2016-03-29</p> <p>Geological records from the Antarctic margin offer direct evidence of environmental variability at high southern latitudes and provide insight regarding <span class="hlt">ice</span> sheet sensitivity to past climate change. The early to mid-Miocene (23-14 Mya) is a compelling interval to study as global temperatures and atmospheric CO2 concentrations were similar to those projected for coming centuries. Importantly, this time interval includes the Miocene Climatic Optimum, a period of global warmth during which average surface temperatures were 3-4 °C higher than today. Miocene sediments in the ANDRILL-2A drill core from the Western Ross Sea, Antarctica, indicate that the Antarctic <span class="hlt">ice</span> sheet (AIS) was highly variable through this key time interval. A multiproxy dataset derived from the core identifies four distinct environmental motifs based on changes in sedimentary facies, fossil assemblages, geochemistry, and paleotemperature. Four major disconformities in the drill core coincide with regional seismic discontinuities and reflect transient expansion of grounded <span class="hlt">ice</span> across the Ross Sea. They correlate with major positive shifts in benthic oxygen isotope records and generally coincide with intervals when atmospheric CO2 concentrations were at or below preindustrial levels (∼280 ppm). Five intervals reflect <span class="hlt">ice</span> sheet minima and air temperatures warm enough for substantial <span class="hlt">ice</span> <span class="hlt">mass</span> loss during episodes of high (∼500 ppm) atmospheric CO2 These new drill core data and associated <span class="hlt">ice</span> sheet modeling experiments indicate that polar climate and the AIS were highly sensitive to relatively small changes in atmospheric CO2 during the early to mid-Miocene.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015E%26PSL.422..150M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015E%26PSL.422..150M"><span>Interannual <span class="hlt">variation</span> of the Antarctic <span class="hlt">Ice</span> Sheet from a combined analysis of satellite gravimetry and altimetry data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mémin, A.; Flament, T.; Alizier, B.; Watson, C.; Rémy, F.</p> <p>2015-07-01</p> <p>Assessment of the long term <span class="hlt">mass</span> balance of the Antarctic <span class="hlt">Ice</span> Sheet, and thus the determination of its contribution to sea level rise, requires an understanding of interannual variability and associated causal mechanisms. We performed a combined analysis of surface-<span class="hlt">mass</span> and elevation changes using data from the GRACE and Envisat satellite missions, respectively. Using empirical orthogonal functions and singular value decompositions of each data set, we find a quasi 4.7-yr periodic signal between 08/2002 and 10/2010 that accounts for ∼ 15- 30% of the time variability of the filtered and detrended surface-<span class="hlt">mass</span> and elevation data. Computation of the density of this variable <span class="hlt">mass</span> load corresponds to snow or uncompacted firn. Changes reach maximum amplitude within the first 100 km from the coast where it contributes up to 30-35% of the annual rate of accumulation. Extending the analysis to 09/2014 using surface-<span class="hlt">mass</span> changes only, we have found anomalies with a periodicity of about 4-6 yrs that circle the AIS in about 9-10 yrs. These properties connect the observed anomalies to the Antarctic Circumpolar Wave (ACW) which is known to affect several key climate variables, including precipitation. It suggests that variability in the surface-<span class="hlt">mass</span> balance of the Antarctic <span class="hlt">Ice</span> Sheet may also be modulated by the ACW.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRF..122.2324S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRF..122.2324S"><span>Assimilating the <span class="hlt">ICE</span>-6G_C Reconstruction of the Latest Quaternary <span class="hlt">Ice</span> Age Cycle Into Numerical Simulations of the Laurentide and Fennoscandian <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>Stuhne, G. R.; Peltier, W. R.</p> <p>2017-12-01</p> <p>We analyze the effects of nudging 100 kyr numerical simulations of the Laurentide and Fennoscandian <span class="hlt">ice</span> sheets toward the glacial isostatic adjustment-based (GIA-based) <span class="hlt">ICE</span>-6G_C reconstruction of the most recent <span class="hlt">ice</span> age cycle. Starting with the <span class="hlt">ice</span> physics approximations of the PISM <span class="hlt">ice</span> sheet model and the SeaRISE simulation protocols, we incorporate nudging at characteristic time scales, τf, through anomalous <span class="hlt">mass</span> balance terms in the <span class="hlt">ice</span> <span class="hlt">mass</span> conservation equation. As should be expected, these <span class="hlt">mass</span> balances exhibit physically unrealistic details arising from pure GIA-based reconstruction geometry when nudging is very strong (τf=20 years for North America), while weakly nudged (τf=1,000 years) solutions deviate from <span class="hlt">ICE</span>-6G_C sufficiently to degrade its observational fit quality. For reasonable intermediate time scales (τf=100 years and 200 years), we perturbatively analyze nudged <span class="hlt">ice</span> dynamics as a superposition of "leading-order smoothing" that diffuses <span class="hlt">ICE</span>-6G_C in a physically and observationally consistent manner and "higher-order" deviations arising, for instance, from biases in the time dependence of surface climate boundary conditions. Based upon the relative deviations between respective nudged simulations in which these biases follow surface temperature from <span class="hlt">ice</span> cores and eustatic sea level from marine sediment cores, we compute "<span class="hlt">ice</span> core climate adjustments" that suggest how local paleoclimate observations may be applied to the systematic refinement of <span class="hlt">ICE</span>-6G_C. Our results are consistent with a growing body of evidence suggesting that the geographical origins of Meltwater Pulse 1B (MWP1b) may lie primarily in North America as opposed to Antarctica (as reconstructed in <span class="hlt">ICE</span>-6G_C).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19890018779','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19890018779"><span><span class="hlt">Ice</span> sheet radar altimetry</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zwally, J.</p> <p>1988-01-01</p> <p>The surface topography of the Greenland and Antarctic <span class="hlt">ice</span> sheets between 72 degrees north and south was mapped using radar altimetry data from the U.S. Navy GEOSAT. The glaciological objectives of this activity were to study the dynamics of the <span class="hlt">ice</span> flow, changes in the position of floating <span class="hlt">ice</span>-shelf fronts, and ultimately to measure temporal changes in <span class="hlt">ice</span> surface elevation indicative of <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balance.</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 <span class="hlt">mass</span> 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('http://adsabs.harvard.edu/abs/2015AGUFM.C21A0728W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C21A0728W"><span>Spatio-temporal <span class="hlt">Variation</span> in Glacier <span class="hlt">Ice</span> as Habitat for Harbor Seals in an Alaskan Tidewater Glacier Fjord</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Womble, J. N.; McNabb, R. W.; Gens, R.; Prakash, A.</p> <p>2015-12-01</p> <p>Some of the largest aggregations of harbor seals (Phoca vitulina richardii) in Alaska occur in tidewater glacier fjords where seals rest upon icebergs that are calved from tidewater glaciers into the marine environment. The distribution, amount, and size of floating <span class="hlt">ice</span> in fjords are likely important factors influencing the spatial distribution and abundance of harbor seals; however, fine-scale characteristics of <span class="hlt">ice</span> habitat that are used by seals have not been quantified using automated methods. We quantified the seasonal changes in <span class="hlt">ice</span> habitat for harbor seals in Johns Hopkins Inlet, a tidewater glacier fjord in Glacier Bay National Park, Alaska, using aerial photography, object-based image analysis, and spatial models. Aerial photographic surveys (n = 53) were conducted of seals and <span class="hlt">ice</span> during the whelping (June) and molting (August) seasons from 2007-2014. Surveys were flown along a grid of 12 transects and high-resolution digital photos were taken directly under the plane using a vertically aimed camera. Seal abundance and spatial distribution was consistently higher during June (range: 1,672-4,340) than August (range: 1,075-2,582) and corresponded to the spatial distribution and amount of <span class="hlt">ice</span>. Preliminary analyses from 2007 suggest that the average percent of icebergs (<span class="hlt">ice</span> ≥ than 1.6m2) and brash <span class="hlt">ice</span> (<span class="hlt">ice</span> < 1.6m2) per scene were greater in June (icebergs: 1.8% ± 1.6%; brash <span class="hlt">ice</span>: 43.8% ± 38.9%) than August (icebergs: 0.2% ± 0.7%; brash <span class="hlt">ice</span>; 15.8% ± 26.4%). Iceberg angularity (an index of iceberg shape) was also greater in June (1.7 ± 0.9) than August (0.9 ± 0.9). Potential factors that may influence the spatio-temporal <span class="hlt">variation</span> in <span class="hlt">ice</span> habitat for harbor seals in tidewater glacier fjords include frontal ablation rates of glaciers, fjord circulation, and local winds. Harbor seals exhibit high seasonal fidelity to tidewater glacier fjords, thus understanding the relationships between glacier dynamics and harbor seal distribution will be critical for</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ACP....18.5307W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ACP....18.5307W"><span>Concentration and variability of <span class="hlt">ice</span> nuclei in the subtropical maritime boundary layer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Welti, André; Müller, Konrad; Fleming, Zoë L.; Stratmann, Frank</p> <p>2018-04-01</p> <p>Measurements of the concentration and variability of <span class="hlt">ice</span> nucleating particles in the subtropical maritime boundary layer are reported. Filter samples collected in Cabo Verde over the period 2009-2013 are analyzed with a drop freezing experiment with sensitivity to detect the few rare <span class="hlt">ice</span> nuclei active at low supercooling. The data set is augmented with continuous flow diffusion chamber measurements at temperatures below -24 °C from a 2-month field campaign in Cabo Verde in 2016. The data set is used to address the following questions: what are typical concentrations of <span class="hlt">ice</span> nucleating particles active at a certain temperature? What affects their concentration and where are their sources? Concentration of <span class="hlt">ice</span> nucleating particles is found to increase exponentially by 7 orders of magnitude from -5 to -38 °C. Sample-to-sample <span class="hlt">variation</span> in the steepness of the increase indicates that particles of different origin, with different <span class="hlt">ice</span> nucleation properties (size, composition), contribute to the <span class="hlt">ice</span> nuclei concentration at different temperatures. The concentration of <span class="hlt">ice</span> nuclei active at a specific temperature varies over a range of up to 4 orders of magnitude. The frequency with which a certain <span class="hlt">ice</span> nuclei concentration is measured within this range is found to follow a lognormal distribution, which can be explained by random dilution during transport. To investigate the geographic origin of <span class="hlt">ice</span> nuclei, source attribution of air <span class="hlt">masses</span> from dispersion modeling is used to classify the data into seven typical conditions. While no source could be attributed to the <span class="hlt">ice</span> nuclei active at temperatures higher than -12 °C, concentrations at lower temperatures tend to be elevated in air <span class="hlt">masses</span> originating from the Sahara.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17731883','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17731883"><span><span class="hlt">Ice</span> core evidence for extensive melting of the greenland <span class="hlt">ice</span> sheet in the last interglacial.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Koerner, R M</p> <p>1989-05-26</p> <p>Evidence from <span class="hlt">ice</span> at the bottom of <span class="hlt">ice</span> cores from the Canadian Arctic Islands and Camp Century and Dye-3 in Greenland suggests that the Greenland <span class="hlt">ice</span> sheet melted extensively or completely during the last interglacial period more than 100 ka (thousand years ago), in contrast to earlier interpretations. The presence of dirt particles in the basal <span class="hlt">ice</span> has previously been thought to indicate that the base of the <span class="hlt">ice</span> sheets had melted and that the evidence for the time of original growth of these <span class="hlt">ice</span> <span class="hlt">masses</span> had been destroyed. However, the particles most likely blew onto the <span class="hlt">ice</span> when the dimensions of the <span class="hlt">ice</span> caps and <span class="hlt">ice</span> sheets were much smaller. <span class="hlt">Ice</span> texture, gas content, and other evidence also suggest that the basal <span class="hlt">ice</span> at each drill site is superimposed <span class="hlt">ice</span>, a type of <span class="hlt">ice</span> typical of the early growth stages of an <span class="hlt">ice</span> cap or <span class="hlt">ice</span> sheet. If the present-day <span class="hlt">ice</span> <span class="hlt">masses</span> began their growth during the last interglacial, the <span class="hlt">ice</span> sheet from the earlier (Illinoian) glacial period must have competely or largely melted during the early part of the same interglacial period. If such melting did occur, the 6-meter higher-than-present sea level during the Sangamon cannot be attributed to disintegration of the West Antarctic <span class="hlt">ice</span> sheet, as has been suggested.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C23C0798L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C23C0798L"><span>How much can Greenland melt? An upper bound on <span class="hlt">mass</span> loss from the Greenland <span class="hlt">Ice</span> Sheet through surface melting</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, X.; Bassis, J. N.</p> <p>2015-12-01</p> <p>With observations showing accelerated <span class="hlt">mass</span> loss from the Greenland <span class="hlt">Ice</span> Sheet due to surface melt, the Greenland <span class="hlt">Ice</span> Sheet is becoming one of the most significant contributors to sea level rise. The contribution of the Greenland <span class="hlt">Ice</span> Sheet o sea level rise is likely to accelerate in the coming decade and centuries as atmospheric temperatures continue to rise, potentially triggering ever larger surface melt rates. However, at present considerable uncertainty remains in projecting the contribution to sea level of the Greenland <span class="hlt">Ice</span> Sheet both due to uncertainty in atmospheric forcing and the <span class="hlt">ice</span> sheet response to climate forcing. Here we seek an upper bound on the contribution of surface melt from the Greenland to sea level rise in the coming century using a surface energy balance model coupled to an englacial model. We use IPCC Representative Concentration Pathways (RCP8.5, RCP6, RCP4.5, RCP2.6) climate scenarios from an ensemble of global climate models in our simulations to project the maximum rate of <span class="hlt">ice</span> volume loss and related sea-level rise associated with surface melting. To estimate the upper bound, we assume the Greenland <span class="hlt">Ice</span> Sheet is perpetually covered in thick clouds, which maximize longwave radiation to the <span class="hlt">ice</span> sheet. We further assume that deposition of black carbon darkens the <span class="hlt">ice</span> substantially turning it nearly black, substantially reducing its albedo. Although assuming that all melt water not stored in the snow/firn is instantaneously transported off the <span class="hlt">ice</span> sheet increases <span class="hlt">mass</span> loss in the short term, refreezing of retained water warms the <span class="hlt">ice</span> and may lead to more melt in the long term. Hence we examine both assumptions and use the scenario that leads to the most surface melt by 2100. Preliminary models results suggest that under the most aggressive climate forcing, surface melt from the Greenland <span class="hlt">Ice</span> Sheet contributes ~1 m to sea level by the year 2100. This is a significant contribution and ignores dynamic effects. We also examined a lower bound</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.C41D..06B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.C41D..06B"><span>Mounting evidence for intense ocean interaction with the Pine Island Glacier <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>Bindschadler, R.; Holland, D.; Vaughan, D.; Vornberger, P.</p> <p>2008-12-01</p> <p>The spatial signature of thinning and acceleration of the Pine Island Glacier has led to the inference that these changes originate at the seaward end of the glacier, possibly within or under the <span class="hlt">ice</span> shelf (Payne et al., 2004; Shepherd et al., 2004). We present new analyses resulting from both new and archived satellite imagery of the <span class="hlt">ice</span> shelf that supports this inference and provides new insights into strong seasonal and intra- annual characters of ocean-<span class="hlt">ice</span> shelf interaction. Strong longitudinal <span class="hlt">variations</span> in both thickness and surface elevation measured by British Antarctic Survey airborne radars (Vaughan et al., 2006) have wavelengths that correspond roughly to the annual motion of the <span class="hlt">ice</span> shelf. These could be caused by seasonal <span class="hlt">variations</span> in flow speed, but such <span class="hlt">variations</span> of flow speed have never been reported and are not seen in the most recent continuous GPS observations of the <span class="hlt">ice</span> shelf. We suggest that these strong <span class="hlt">variations</span> in <span class="hlt">ice</span> thickness, as large as 200 meters in an average thickness of 600 meters, are caused by seasonal <span class="hlt">variations</span> in the properties of the water circulating underneath the <span class="hlt">ice</span> shelf. One likely explanation is that the dominant water <span class="hlt">mass</span> reaching the deepest parts of the <span class="hlt">ice</span> shelf alternates between cold High Salinity Shelf Water in the winter and warm Circumpolar Deep Water in the summer. Evidence for recent strengthening of the sub- shelf circulation is the sudden occurrence of three persistent polynyas immediately adjacent to the <span class="hlt">ice</span> front. These are located in precisely the locations expected from modeled sub-shelf circulation (Payne et al., 2007). This mode was never observed in any satellite imagery prior to the 1999-2000 austral summer (data of 7 summers since 1973 were available), but has occurred in 7 of the 9 summers since and persists throughout the summer. Payne, A.J., A. Vieli, A.P. Shepherd, D.J. Wingham and E. Rignot, 2004. Recent dramatic thinning of largest West Antarctic <span class="hlt">ice</span> stream triggered by oceans, Geophysical</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160010510','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160010510"><span>The Effect of CO2 <span class="hlt">Ice</span> Cap Sublimation on Mars Atmosphere</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Batterson, Courtney</p> <p>2016-01-01</p> <p>Sublimation of the polar CO2 <span class="hlt">ice</span> caps on Mars is an ongoing phenomenon that may be contributing to secular climate change on Mars. The transfer of CO2 between the surface and atmosphere via sublimation and deposition may alter atmospheric <span class="hlt">mass</span> such that net atmospheric <span class="hlt">mass</span> is increasing despite seasonal <span class="hlt">variations</span> in CO2 transfer. My study builds on previous studies by Kahre and Haberle that analyze and compare data from the Phoenix and Viking Landers 1 and 2 to determine whether secular climate change is happening on Mars. In this project, I use two years worth of temperature, pressure, and elevation data from the MSL Curiosity rover to create a program that allows for successful comparison of Curiosity pressure data to Viking Lander pressure data so a conclusion can be drawn regarding whether CO2 <span class="hlt">ice</span> cap sublimation is causing a net increase in atmospheric <span class="hlt">mass</span> and is thus contributing to secular climate change on Mars.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C51C0997M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C51C0997M"><span>Glacial Boundary Features Delineated Using Enhanced-resolution Passive-microwave Data to Determine Melt Season <span class="hlt">Variation</span> of the Vatnajokull <span class="hlt">Ice</span> Cap, Iceland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marzillier, D. M.; Ramage, J. M.</p> <p>2017-12-01</p> <p>Temperate glaciers such as those seen in Iceland experience high annual <span class="hlt">mass</span> flux, thereby responding to small scale changes in Earth's climate. Decadal changes in the glacial margins of Iceland's <span class="hlt">ice</span> caps are observable in the Landsat record, however twice daily AMSR-E Calibrated Enhanced-Resolution Passive Microwave Daily EASE-Grid 2.0 Brightness Temperature (CETB) Earth System Data Record (ESDR) allow for observation on a daily temporal scale and a 3.125 km spatial scale, which can in turn be connected to patterns seen over longer periods of time. Passive microwave data allow for careful observation of melt onset and duration in Iceland's glacial regions by recording changes in emissivity of the <span class="hlt">ice</span> surface, known as brightness temperature (TB), which is sensitive to fluctuations in the liquid water content of snow and <span class="hlt">ice</span> seen during melting in glaciated regions. Enhanced resolution of this data set allows for a determination of a threshold that defines the melting season. The XPGR snowmelt algorithm originally presented by Abdalati and Steffen (1995) is used as a comparison with the diurnal amplitude <span class="hlt">variation</span> (DAV) values on Iceland's Vatnajokull <span class="hlt">ice</span> cap located at 64.4N, -16.8W. Ground-based air temperature data in this region, digital elevation models (DEMs), and river discharge dominated by glacial runoff are used to confirm the glacial response to changes in global climate. Results show that Iceland glaciers have a bimodal distribution of brightness temperature delineating when the snow/<span class="hlt">ice</span> is melting and refreezing. Ground based temperatures have increased on a decadal trend. Clear glacial boundaries are visible on the passive microwave delineating strong features, and we are working to understand their variability and contribution to glacier evolution. The passive microwave data set allows connections to be made between observations seen on a daily scale and the long term glacier changes observed by the Landsat satellite record that integrates the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1175859','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/1175859"><span>Methods and apparatus for rotor blade <span class="hlt">ice</span> detection</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>LeMieux, David Lawrence</p> <p>2006-08-08</p> <p>A method for detecting <span class="hlt">ice</span> on a wind turbine having a rotor and one or more rotor blades each having blade roots includes monitoring meteorological conditions relating to <span class="hlt">icing</span> conditions and monitoring one or more physical characteristics of the wind turbine in operation that vary in accordance with at least one of the <span class="hlt">mass</span> of the one or more rotor blades or a <span class="hlt">mass</span> imbalance between the rotor blades. The method also includes using the one or more monitored physical characteristics to determine whether a blade <span class="hlt">mass</span> anomaly exists, determining whether the monitored meteorological conditions are consistent with blade <span class="hlt">icing</span>; and signaling an <span class="hlt">icing</span>-related blade <span class="hlt">mass</span> anomaly when a blade <span class="hlt">mass</span> anomaly is determined to exist and the monitored meteorological conditions are determined to be consistent with <span class="hlt">icing</span>.</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> <span class="hlt">Mass</span> 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 zone 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 <span class="hlt">mass</span> 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 zone (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 zone; at the surface, the estimated FSM was larger but more localized to the lower reaches of glacial ablation zones. 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/2016AGUFM.B31G0545V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.B31G0545V"><span>Monitoring stress-related <span class="hlt">mass</span> <span class="hlt">variations</span> in Amazon trees using accelerometers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>van Emmerik, T. H. M.; Steele-Dunne, S. C.; Gentine, P.; Hut, R.; Guerin, M. F.; Leus, G.; Oliveira, R. S.; Van De Giesen, N.</p> <p>2016-12-01</p> <p>Containing half of the world's rainforests, the Amazon plays a key role in the global water and carbon budget. However, the Amazon remains poorly understood, but appears to be vulnerable to increasing moisture stress, and future droughts have the potential to considerably change the global water and carbon budget. Field measurements will allow further investigations of the effects of moisture stress and droughts on tree dynamics, and its impact on the water and carbon budget. This study focuses on studying the diurnal <span class="hlt">mass</span> <span class="hlt">variations</span> of seven Amazonian tree species. The <span class="hlt">mass</span> of trees is influenced by physiological processes within the tree (e.g. transpiration and root water uptake), as well as external loads (e.g. intercepted precipitation). Depending on the physiological traits of an individual tree, moisture stress and drought affect processes such as photosynthesis, assimilation, transpiration, and root water uptake. In turn, these have their influence on diurnal <span class="hlt">mass</span> <span class="hlt">variations</span> of a tree. Our study uses measured three-dimensional displacement and acceleration of trees, to detect and quantify their diurnal (bio)<span class="hlt">mass</span> <span class="hlt">variations</span>. Nineteen accelerometers and dendrometers were installed on seven different tree species in the Amazon rainforest, covering an area of 250 x 250 m. The selected species span a wide range in wood density (0.5 - 1.1), diameter (15 - 40 cm) and height (25 - 60 m). Acceleration was measured with a frequency of 10 Hz, from August 2015 to June 2016, covering both the wet and dry season. On-site additional measurements of net radiation, wind speed at three heights, temperature, and precipitation as available every 15 minutes. Dendrometers measured <span class="hlt">variation</span> in xylem and bark thickness every 5 minutes. The MUltiple SIgnal Classification (MUSIC) algorithm was applied to the acceleration time series to estimate the frequency spectrum of each tree. A correction was necessary to account for the dominant effect of wind. The resulting spectra reveal</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..11.6008T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..11.6008T"><span>Influences of Ocean Thermohaline Stratification on Arctic 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>Toole, J. M.; Timmermans, M.-L.; Perovich, D. K.; Krishfield, R. A.; Proshutinsky, A.; Richter-Menge, J. A.</p> <p>2009-04-01</p> <p>The Arctic Ocean's surface mixed layer constitutes the dynamical and thermodynamical link between the sea <span class="hlt">ice</span> and the underlying waters. Wind stress, acting directly on the surface mixed layer or via wind-forced <span class="hlt">ice</span> motion, produce surface currents that can in turn drive deep ocean flow. Mixed layer temperature is intimately related to basal sea <span class="hlt">ice</span> growth and melting. Heat fluxes into or out of the surface mixed layer can occur at both its upper and lower interfaces: the former via air-sea exchange at leads and conduction through the <span class="hlt">ice</span>, the latter via turbulent mixing and entrainment at the layer base. <span class="hlt">Variations</span> in Arctic Ocean mixed layer properties are documented based on more than 16,000 temperature and salinity profiles acquired by <span class="hlt">Ice</span>-Tethered Profilers since summer 2004 and analyzed in conjunction with sea <span class="hlt">ice</span> observations from <span class="hlt">Ice</span> <span class="hlt">Mass</span> Balance Buoys and atmospheric heat flux estimates. Guidance interpreting the observations is provided by a one-dimensional ocean mixed layer model. The study focuses attention on the very strong density stratification about the mixed layer base in the Arctic that, in regions of sea <span class="hlt">ice</span> melting, is increasing with time. The intense stratification greatly impedes mixed layer deepening by vertical convection and shear mixing, and thus limits the flux of deep ocean heat to the surface that could influence sea <span class="hlt">ice</span> growth/decay. Consistent with previous work, this study demonstrates that the Arctic sea <span class="hlt">ice</span> is most sensitive to changes in ocean mixed layer heat resulting from fluxes across its upper (air-sea and/or <span class="hlt">ice</span>-water) interface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12368852','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12368852"><span>Switch of flow direction in an Antarctic <span class="hlt">ice</span> stream.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Conway, H; Catania, G; Raymond, C F; Gades, A M; Scambos, T A; Engelhardt, H</p> <p>2002-10-03</p> <p>Fast-flowing <span class="hlt">ice</span> streams transport <span class="hlt">ice</span> from the interior of West Antarctica to the ocean, and fluctuations in their activity control the <span class="hlt">mass</span> balance of the <span class="hlt">ice</span> sheet. The <span class="hlt">mass</span> balance of the Ross Sea sector of the West Antarctic <span class="hlt">ice</span> sheet is now positive--that is, it is growing--mainly because one of the <span class="hlt">ice</span> streams (<span class="hlt">ice</span> stream C) slowed down about 150 years ago. Here we present evidence from both surface measurements and remote sensing that demonstrates the highly dynamic nature of the Ross drainage system. We show that the flow in an area that once discharged into <span class="hlt">ice</span> stream C has changed direction, now draining into the Whillans <span class="hlt">ice</span> stream (formerly <span class="hlt">ice</span> stream B). This switch in flow direction is a result of continuing thinning of the Whillans <span class="hlt">ice</span> stream and recent thickening of <span class="hlt">ice</span> stream C. Further abrupt reorganization of the activity and configuration of the <span class="hlt">ice</span> streams over short timescales is to be expected in the future as the surface topography of the <span class="hlt">ice</span> sheet responds to the combined effects of internal dynamics and long-term climate change. We suggest that caution is needed when using observations of short-term <span class="hlt">mass</span> changes to draw conclusions about the large-scale <span class="hlt">mass</span> balance of the <span class="hlt">ice</span> sheet.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C14B..04B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C14B..04B"><span>Understanding <span class="hlt">Ice</span> Shelf Basal Melting Using Convergent ICEPOD Data Sets: ROSETTA-<span class="hlt">Ice</span> Study of 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>Bell, R. E.; Frearson, N.; Tinto, K. J.; Das, I.; Fricker, H. A.; Siddoway, C. S.; Padman, L.</p> <p>2017-12-01</p> <p>The future stability of the <span class="hlt">ice</span> shelves surrounding Antarctica will be susceptible to increases in both surface and basal melt as the atmosphere and ocean warm. The ROSETTA-<span class="hlt">Ice</span> program is targeted at using the ICEPOD airborne technology to produce new constraints on Ross <span class="hlt">Ice</span> Shelf, the underlying ocean, bathymetry, and geologic setting, using radar sounding, gravimetry and laser altimetry. This convergent approach to studying the <span class="hlt">ice</span>-shelf and basal processes enables us to develop an understanding of the fundamental controls on <span class="hlt">ice</span>-shelf evolution. This work leverages the stratigraphy of the <span class="hlt">ice</span> shelf, which is detected as individual reflectors by the shallow-<span class="hlt">ice</span> radar and is often associated with surface scour, form close to the grounding line or pinning points on the <span class="hlt">ice</span> shelf. Surface accumulation on the <span class="hlt">ice</span> shelf buries these reflectors as the <span class="hlt">ice</span> flows towards the calving front. This distinctive stratigraphy can be traced across the <span class="hlt">ice</span> shelf for the major East Antarctic outlet glaciers and West Antarctic <span class="hlt">ice</span> streams. Changes in the <span class="hlt">ice</span> thickness below these reflectors are a result of strain and basal melting and freezing. Correcting the estimated thickness changes for strain using RIGGS strain measurements, we can develop decadal-resolution flowline distributions of basal melt. Close to East Antarctica elevated melt-rates (>1 m/yr) are found 60-100 km from the calving front. On the West Antarctic side high melt rates primarily develop within 10 km of the calving front. The East Antarctic side of Ross <span class="hlt">Ice</span> Shelf is dominated by melt driven by saline water <span class="hlt">masses</span> that develop in Ross Sea polynyas, while the melting on the West Antarctic side next to Hayes Bank is associated with modified Continental Deep Water transported along the continental shelf. The two sides of Ross <span class="hlt">Ice</span> Shelf experience differing basal melt in part due to the duality in the underlying geologic structure: the East Antarctic side consists of relatively dense crust, with low amplitude</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_15 --> <div id="page_16" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="301"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22042434','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22042434"><span>Anchor <span class="hlt">ice</span> and benthic disturbance in shallow Antarctic waters: interspecific <span class="hlt">variation</span> in initiation and propagation of <span class="hlt">ice</span> crystals.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Denny, Mark; Dorgan, Kelly M; Evangelista, Dennis; Hettinger, Annaliese; Leichter, James; Ruder, Warren C; Tuval, Idan</p> <p>2011-10-01</p> <p>Sea <span class="hlt">ice</span> typically forms at the ocean's surface, but given a source of supercooled water, an unusual form of <span class="hlt">ice</span>--anchor <span class="hlt">ice</span>--can grow on objects in the water column or at the seafloor. For several decades, ecologists have considered anchor <span class="hlt">ice</span> to be an important agent of disturbance in the shallow-water benthic communities of McMurdo Sound, Antarctica, and potentially elsewhere in polar seas. Divers have documented anchor <span class="hlt">ice</span> in the McMurdo communities, and its presence coincides with reduced abundance of the sponge Homaxinella balfourensis, which provides habitat for a diverse assemblage of benthic organisms. However, the mechanism of this disturbance has not been explored. Here we show interspecific differences in anchor-<span class="hlt">ice</span> formation and propagation characteristics for Antarctic benthic organisms. The sponges H. balfourensis and Suberites caminatus show increased incidence of formation and accelerated spread of <span class="hlt">ice</span> crystals compared to urchins and sea stars. Anchor <span class="hlt">ice</span> also forms readily on sediments, from which it can grow and adhere to organisms. Our results are consistent with, and provide a potential first step toward, an explanation for disturbance patterns observed in shallow polar benthic communities. Interspecific differences in <span class="hlt">ice</span> formation raise questions about how surface tissue characteristics such as surface area, rugosity, and mucus coating affect <span class="hlt">ice</span> formation on invertebrates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19970014011','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19970014011"><span>Spatial and Temporal <span class="hlt">Variations</span> of Surface Characteristics on the Greenland <span class="hlt">Ice</span> Sheet as Derived from Passive Microwave Observations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Anderson, Mark; Rowe, Clinton; Kuivinen, Karl; Mote, Thomas</p> <p>1996-01-01</p> <p>The primary goals of this research were to identify and begin to comprehend the spatial and temporal <span class="hlt">variations</span> in surface characteristics of the Greenland <span class="hlt">ice</span> sheet using passive microwave observations, physically-based models of the snowpack and field observations of snowpack and firn properties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015NatGe...8..534U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015NatGe...8..534U"><span>Laurentide <span class="hlt">ice</span>-sheet instability during the last deglaciation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ullman, David J.; Carlson, Anders E.; Anslow, Faron S.; Legrande, Allegra N.; Licciardi, Joseph M.</p> <p>2015-07-01</p> <p>Changes in the amount of summer incoming solar radiation (insolation) reaching the Northern Hemisphere are the underlying pacemaker of glacial cycles. However, not all rises in boreal summer insolation over the past 800,000 years resulted in deglaciation to present-day <span class="hlt">ice</span> volumes, suggesting that there may be a climatic threshold for the disappearance of land-based <span class="hlt">ice</span>. Here we assess the surface <span class="hlt">mass</span> balance stability of the Laurentide <span class="hlt">ice</span> sheet--the largest glacial <span class="hlt">ice</span> <span class="hlt">mass</span> in the Northern Hemisphere--during the last deglaciation (24,000 to 9,000 years ago). We run a surface energy balance model with climate data from simulations with a fully coupled atmosphere-ocean general circulation model for key time slices during the last deglaciation. We find that the surface <span class="hlt">mass</span> balance of the Laurentide <span class="hlt">ice</span> sheet was positive throughout much of the deglaciation, and suggest that dynamic discharge was mainly responsible for <span class="hlt">mass</span> loss during this time. Total surface <span class="hlt">mass</span> balance became negative only in the early Holocene, indicating the transition to a new state where <span class="hlt">ice</span> loss occurred primarily by surface ablation. We conclude that the Laurentide <span class="hlt">ice</span> sheet remained a viable <span class="hlt">ice</span> sheet before the Holocene and began to fully deglaciate only once summer temperatures and radiative forcing over the <span class="hlt">ice</span> sheet increased by 6-7 °C and 16-20 W m-2, respectively, relative to full glacial conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19890004057','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19890004057"><span>Analytical <span class="hlt">ice</span> shape predictions for flight in natural <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>Berkowitz, Brian M.; Riley, James T.</p> <p>1988-01-01</p> <p>LEWICE is an analytical <span class="hlt">ice</span> prediction code that has been evaluated against <span class="hlt">icing</span> tunnel data, but on a more limited basis against flight data. <span class="hlt">Ice</span> shapes predicted by LEWICE is compared with experimental <span class="hlt">ice</span> shapes accreted on the NASA Lewis <span class="hlt">Icing</span> Research Aircraft. The flight data selected for comparison includes liquid water content recorded using a hot wire device and droplet distribution data from a laser spectrometer; the <span class="hlt">ice</span> shape is recorded using stereo photography. The main findings are as follows: (1) An equivalent sand grain roughness correlation different from that used for LEWICE tunnel comparisons must be employed to obtain satisfactory results for flight; (2) Using this correlation and making no other changes in the code, the comparisons to <span class="hlt">ice</span> shapes accreted in flight are in general as good as the comparisons to <span class="hlt">ice</span> shapes accreted in the tunnel (as in the case of tunnel <span class="hlt">ice</span> shapes, agreement is least reliable for large glaze <span class="hlt">ice</span> shapes at high angles of attack); (3) In some cases comparisons can be somewhat improved by utilizing the code so as to take account of the <span class="hlt">variation</span> of parameters such as liquid water content, which may vary significantly in flight.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950049157&hterms=solar+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dsolar%2Benergy','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950049157&hterms=solar+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dsolar%2Benergy"><span>The effect of sea <span class="hlt">ice</span> on the solar energy budget in the astmosphere-sea <span class="hlt">ice</span>-ocean system: A model study</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jin, Z.; Stamnes, Knut; Weeks, W. F.; Tsay, Si-Chee</p> <p>1994-01-01</p> <p>A coupled one-dimensional multilayer and multistream radiative transfer model has been developed and applied to the study of radiative interactions in the atmosphere, sea <span class="hlt">ice</span>, and ocean system. The consistent solution of the radiative transfer equation in this coupled system automatically takes into account the refraction and reflection at the air-<span class="hlt">ice</span> interface and allows flexibility in choice of stream numbers. The solar radiation spectrum (0.25 micron-4.0 micron) is divided into 24 spectral bands to account adequately for gaseous absorption in the atmosphere. The effects of <span class="hlt">ice</span> property changes, including salinity and density <span class="hlt">variations</span>, as well as of melt ponds and snow cover <span class="hlt">variations</span> over the <span class="hlt">ice</span> on the solar energy distribution in the entire system have been studied quantitatively. The results show that for bare <span class="hlt">ice</span> it is the scattering, determined by air bubbles and brine pockets, in just a few centimeters of the top layer of <span class="hlt">ice</span> that plays the most important role in the solar energy absorption and partitioning in the entire system. <span class="hlt">Ice</span> thickness is important to the energy distribution only when the <span class="hlt">ice</span> is thin, while the absorption in the atmosphere is not sensitive to <span class="hlt">ice</span> thickness exceeds about 70 cm. The presence of clouds moderates all the sensitivities of the absorptive amounts in each layer to the <span class="hlt">variations</span> in the <span class="hlt">ice</span> properties and <span class="hlt">ice</span> thickness. Comparisons with observational spectral albedo values for two simple <span class="hlt">ice</span> types are also presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C32B..01T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C32B..01T"><span>Some Results on Sea <span class="hlt">Ice</span> Rheology for the Seasonal <span class="hlt">Ice</span> Zone, Obtained from the Deformation Field of Sea <span class="hlt">Ice</span> Drift Pattern</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Toyota, T.; Kimura, N.</p> <p>2017-12-01</p> <p>Sea <span class="hlt">ice</span> rheology which relates sea <span class="hlt">ice</span> stress to the large-scale deformation of the <span class="hlt">ice</span> cover has been a big issue to numerical sea <span class="hlt">ice</span> modelling. At present the treatment of internal stress within sea <span class="hlt">ice</span> area is based mostly on the rheology formulated by Hibler (1979), where the whole sea <span class="hlt">ice</span> 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 <span class="hlt">ice</span> area and horizontal resolution of the model. However, this formulation was initially developed to reproduce the seasonal <span class="hlt">variation</span> of the perennial <span class="hlt">ice</span> in the Arctic Ocean. As for its applicability to the seasonal <span class="hlt">ice</span> zones (SIZ), where various types of sea <span class="hlt">ice</span> are present, it still needs validation from observational data. In this study, the validity of this rheology was examined for the Sea of Okhotsk <span class="hlt">ice</span>, typical of the SIZ, based on the AMSR-derived <span class="hlt">ice</span> 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. <span class="hlt">Ice</span> 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 <span class="hlt">variation</span> 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 <span class="hlt">ice</span> areas. Since this result corresponds with the yield criterion by Tresca and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/14685228','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/14685228"><span>Recent <span class="hlt">ice</span> ages on Mars.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Head, James W; Mustard, John F; Kreslavsky, Mikhail A; Milliken, Ralph E; Marchant, David R</p> <p>2003-12-18</p> <p>A key pacemaker of <span class="hlt">ice</span> ages on the Earth is climatic forcing due to <span class="hlt">variations</span> in planetary orbital parameters. Recent Mars exploration has revealed dusty, water-<span class="hlt">ice</span>-rich mantling deposits that are layered, metres thick and latitude dependent, occurring in both hemispheres from mid-latitudes to the poles. Here we show evidence that these deposits formed during a geologically recent <span class="hlt">ice</span> age that occurred from about 2.1 to 0.4 Myr ago. The deposits were emplaced symmetrically down to latitudes of approximately 30 degrees--equivalent to Saudi Arabia and the southern United States on the Earth--in response to the changing stability of water <span class="hlt">ice</span> and dust during <span class="hlt">variations</span> in obliquity (the angle between Mars' pole of rotation and the ecliptic plane) reaching 30-35 degrees. Mars is at present in an 'interglacial' period, and the <span class="hlt">ice</span>-rich deposits are undergoing reworking, degradation and retreat in response to the current instability of near-surface <span class="hlt">ice</span>. Unlike the Earth, martian <span class="hlt">ice</span> ages are characterized by warmer polar climates and enhanced equatorward transport of atmospheric water and dust to produce widespread smooth deposits down to mid-latitudes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003Natur.426..797H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003Natur.426..797H"><span>Recent <span class="hlt">ice</span> ages on Mars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Head, James W.; Mustard, John F.; Kreslavsky, Mikhail A.; Milliken, Ralph E.; Marchant, David R.</p> <p>2003-12-01</p> <p>A key pacemaker of <span class="hlt">ice</span> ages on the Earth is climatic forcing due to <span class="hlt">variations</span> in planetary orbital parameters. Recent Mars exploration has revealed dusty, water-<span class="hlt">ice</span>-rich mantling deposits that are layered, metres thick and latitude dependent, occurring in both hemispheres from mid-latitudes to the poles. Here we show evidence that these deposits formed during a geologically recent <span class="hlt">ice</span> age that occurred from about 2.1 to 0.4 Myr ago. The deposits were emplaced symmetrically down to latitudes of ~30°-equivalent to Saudi Arabia and the southern United States on the Earth-in response to the changing stability of water <span class="hlt">ice</span> and dust during <span class="hlt">variations</span> in obliquity (the angle between Mars' pole of rotation and the ecliptic plane) reaching 30-35°. Mars is at present in an `interglacial' period, and the <span class="hlt">ice</span>-rich deposits are undergoing reworking, degradation and retreat in response to the current instability of near-surface <span class="hlt">ice</span>. Unlike the Earth, martian <span class="hlt">ice</span> ages are characterized by warmer polar climates and enhanced equatorward transport of atmospheric water and dust to produce widespread smooth deposits down to mid-latitudes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015TCD.....9.5647D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015TCD.....9.5647D"><span>Anomalously-dense firn in an <span class="hlt">ice</span>-shelf channel revealed by wide-angle radar</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Drews, R.; Brown, J.; Matsuoka, K.; Witrant, E.; Philippe, M.; Hubbard, B.; Pattyn, F.</p> <p>2015-10-01</p> <p>The thickness of <span class="hlt">ice</span> shelves, a basic parameter for <span class="hlt">mass</span> balance estimates, is typically inferred using hydrostatic equilibrium for which knowledge of the depth-averaged density is essential. The densification from snow to <span class="hlt">ice</span> depends on a number of local factors (e.g. temperature and surface <span class="hlt">mass</span> balance) causing spatial and temporal <span class="hlt">variations</span> in density-depth profiles. However, direct measurements of firn density are sparse, requiring substantial logistical effort. Here, we infer density from radio-wave propagation speed using ground-based wide-angle radar datasets (10 MHz) collected at five sites on Roi Baudouin <span class="hlt">Ice</span> Shelf (RBIS), Dronning Maud Land, Antarctica. Using a novel algorithm including traveltime inversion and raytracing with a prescribed shape of the depth-density relationship, we show that the depth to internal reflectors, the local <span class="hlt">ice</span> thickness and depth-averaged densities can reliably be reconstructed. For the particular case of an <span class="hlt">ice</span>-shelf channel, where <span class="hlt">ice</span> thickness and surface slope change substantially over a few kilometers, the radar data suggests that firn inside the channel is about 5 % denser than outside the channel. Although this density difference is at the detection limit of the radar, it is consistent with a similar density anomaly reconstructed from optical televiewing, which reveals 10 % denser firn inside compared to outside the channel. The denser firn in the <span class="hlt">ice</span>-shelf channel should be accounted for when using the hydrostatic <span class="hlt">ice</span> thickness for determining basal melt rates. The radar method presented here is robust and can easily be adapted to different radar frequencies and data-acquisition geometries.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170007301','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170007301"><span>Evaluation of Alternative Altitude Scaling Methods for Thermal <span class="hlt">Ice</span> Protection System in NASA <span class="hlt">Icing</span> Research Tunnel</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lee, Sam; Addy, Harold; Broeren, Andy P.; Orchard, David M.</p> <p>2017-01-01</p> <p>A test was conducted at NASA <span class="hlt">Icing</span> Research Tunnel to evaluate altitude scaling methods for thermal <span class="hlt">ice</span> protection system. Two scaling methods based on Weber number were compared against a method based on the Reynolds number. The results generally agreed with the previous set of tests conducted in NRCC Altitude <span class="hlt">Icing</span> Wind Tunnel. The Weber number based scaling methods resulted in smaller runback <span class="hlt">ice</span> <span class="hlt">mass</span> than the Reynolds number based scaling method. The <span class="hlt">ice</span> accretions from the Weber number based scaling method also formed farther upstream. However there were large differences in the accreted <span class="hlt">ice</span> <span class="hlt">mass</span> between the two Weber number based scaling methods. The difference became greater when the speed was increased. This indicated that there may be some Reynolds number effects that isnt fully accounted for and warrants further study.</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 <span class="hlt">mass</span> 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/2010AGUFM.C11A0533C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.C11A0533C"><span>From Outlet Glacier Changes to <span class="hlt">Ice</span> Sheet <span class="hlt">Mass</span> Balance - Evolution of Greenland <span class="hlt">Ice</span> Sheet from Laser Altimetry Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Csatho, B. M.; Schenk, A.; Nagarajan, S.; Babonis, G. S.</p> <p>2010-12-01</p> <p>Investigations of <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balance and the changing dynamics of outlet glaciers have been hampered by the lack of comprehensive data. In recent years, this situation has been remedied. Satellite laser altimetry data from the <span class="hlt">Ice</span> Cloud and land Elevation Satellite mission (ICESat), combined with airborne laser altimetry, provide accurate measurements of surface elevation changes, and surface velocities derived from various satellite platforms yield crucial information on changing glacier dynamics. Taken together, a rich and diverse data set is emerging that allows for characterizing the spatial and temporal evolution of <span class="hlt">ice</span> sheets and outlet glaciers. In particular, it enables quantitative studies of outlet glaciers undergoing rapid and complex changes. Although airborne and laser altimetry have been providing precise measurements of <span class="hlt">ice</span> sheet topography since the early 1990s, determining detailed and accurate spatial and temporal distribution of surface changes remains a challenging problem. We have developed a new, comprehensive method, called Surface Elevation Reconstruction And Change detection (SERAC), which estimates surface changes by a simultaneous reconstruction of surface topography from fused multisensor data. The mathematical model is based on the assumption that for a small surface area, only the absolute elevation changes over time but not the shape of the surface patch. Therefore, laser points of all time epochs contribute to the shape parameters; points of each time period determine the absolute elevation of the surface patch at that period. This method provides high-resolution surface topography, precise changes and a rigorous error estimate of the quantities. By using SERAC we combined ICESat and ATM laser altimetry data to determine the evolution of surface change rates of the whole Greenland <span class="hlt">Ice</span> Sheet between 2003 and 2009 on a high-resolution grid. Our reconstruction, consistent with GRACE results, shows <span class="hlt">ice</span> sheet thinning propagating</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11689941','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11689941"><span>Thinning of the <span class="hlt">ice</span> sheet in northwest Greenland over the past forty years.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Paterson, W S; Reeh, N</p> <p>2001-11-01</p> <p>Thermal expansion of the oceans, as well as melting of glaciers, <span class="hlt">ice</span> sheets and <span class="hlt">ice</span> caps have been the main contributors to global sea level rise over the past century. The greatest uncertainty in predicting future sea level changes lies with our estimates of the <span class="hlt">mass</span> balance of the <span class="hlt">ice</span> sheets in Greenland and Antarctica. Satellite measurements have been used to determine changes in these <span class="hlt">ice</span> sheets on short timescales, demonstrating that surface-elevation changes on timescales of decades or less result mainly from <span class="hlt">variations</span> in snow accumulation. Here we present direct measurements of the changes in surface elevation between 1954 and 1995 on a traverse across the north Greenland <span class="hlt">ice</span> sheet. Measurements over a time interval of this length should reflect changes in <span class="hlt">ice</span> flow-the important quantity for predicting changes in sea level-relatively unperturbed by short-term fluctuations in snow accumulation. We find only small changes in the eastern part of the transect, except for some thickening of the north <span class="hlt">ice</span> stream. On the west side, however, the thinning rates of the <span class="hlt">ice</span> sheet are significantly higher and thinning extends to higher elevations than had been anticipated from previous studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRF..121.2494C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRF..121.2494C"><span>Controls on the early Holocene collapse of the Bothnian Sea <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>Clason, Caroline C.; Greenwood, Sarah L.; Selmes, Nick; Lea, James M.; Jamieson, Stewart S. R.; Nick, Faezeh M.; Holmlund, Per</p> <p>2016-12-01</p> <p>New high-resolution multibeam data in the Gulf of Bothnia reveal for the first time the subglacial environment of a Bothnian Sea <span class="hlt">Ice</span> Stream. The geomorphological record suggests that increased meltwater production may have been important in driving rapid retreat of Bothnian Sea <span class="hlt">Ice</span> during deglaciation. Here we apply a well-established, one-dimensional flow line model to simulate <span class="hlt">ice</span> flow through the Gulf of Bothnia and investigate controls on retreat of the <span class="hlt">ice</span> stream during the post-Younger Dryas deglaciation of the Fennoscandian <span class="hlt">Ice</span> Sheet. The relative influence of atmospheric and marine forcings are investigated, with the modeled <span class="hlt">ice</span> stream exhibiting much greater sensitivity to surface melting, implemented through surface <span class="hlt">mass</span> balance and hydrofracture-induced calving, than to submarine melting or relative sea level change. Such sensitivity is supported by the presence of extensive meltwater features in the geomorphological record. The modeled <span class="hlt">ice</span> stream does not demonstrate significant sensitivity to changes in prescribed <span class="hlt">ice</span> stream width or overall bed slope, but local <span class="hlt">variations</span> in basal topography and <span class="hlt">ice</span> stream width result in nonlinear retreat of the grounding line, notably demonstrating points of short-lived retreat slowdown on reverse bed slopes. Retreat of the <span class="hlt">ice</span> stream was most likely governed by increased <span class="hlt">ice</span> surface meltwater production, with the modeled retreat rate less sensitive to marine forcings despite the marine setting.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.C41D..02R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.C41D..02R"><span><span class="hlt">Ice</span>-shelf melting around Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rignot, E.; Jacobs, S.</p> <p>2008-12-01</p> <p>The traditional view on the <span class="hlt">mass</span> balance of Antarctic <span class="hlt">ice</span> shelves is that they loose <span class="hlt">mass</span> principally from iceberg calving with bottom melting a much lower contributing factor. Because <span class="hlt">ice</span> shelves are now known to play a fundamental role in <span class="hlt">ice</span> sheet evolution, it is important to re-evaluate their wastage processes from a circumpolar perspective using a combination of remote sensing techniques. We present area average rates deduced from grounding line discharge, snow accumulation, firn depth correction and <span class="hlt">ice</span> shelf topography. We find that <span class="hlt">ice</span> shelf melting accounts for roughly half of <span class="hlt">ice</span>-shelf ablation, with a total melt water production of 1027 Gt/yr. The attrition fraction due to in-situ melting varies from 9 to 90 percent around Antarctica. High melt producers include the Ronne, Ross, Getz, Totten, Amery, George VI, Pine Island, Abbot, Dotson/Crosson, Shackleton, Thwaites and Moscow University <span class="hlt">Ice</span> Shelves. Low producers include the Larsen C, Princess Astrid and Ragnhild coast, Fimbul, Brunt and Filchner. Correlation between melt water production and grounding line discharge is low (R2 = 0.65). Correlation with thermal ocean forcing from the ocean are highest in the northern parts of West Antarctica where regressions yield R2 of 0.93-0.97. Melt rates in the Amundsen Sea exhibit a quadratic sensitivity to thermal ocean forcing. We conclude that <span class="hlt">ice</span> shelf melting plays a dominant role in <span class="hlt">ice</span> shelf <span class="hlt">mass</span> balance, with a potential to change rapidly in response to altered ocean heat transport onto the Antarctic continental shelf.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006PhDT........43D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006PhDT........43D"><span>Numerical simulations of <span class="hlt">icing</span> in turbomachinery</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Das, Kaushik</p> <p></p> <p>Safety concerns over aircraft <span class="hlt">icing</span> and the high experimental cost of testing have spurred global interest in numerical simulations of the <span class="hlt">ice</span> accretion process. Extensive experimental and computational studies have been carried out to understand the <span class="hlt">icing</span> on external surfaces. No parallel initiatives were reported for <span class="hlt">icing</span> on engine components. However, the supercooled water droplets in moist atmosphere that are ingested into the engine can impinge on the component surfaces and freeze to form <span class="hlt">ice</span> deposits. <span class="hlt">Ice</span> accretion could block the engine passage causing reduced airflow. It raises safety and performance concerns such as mechanical damage from <span class="hlt">ice</span> shedding as well as slow acceleration leading to compressor stall. The current research aims at developing a computational methodology for prediction of <span class="hlt">icing</span> phenomena on turbofan compression system. Numerical simulation of <span class="hlt">ice</span> accretion in aircraft engines is highly challenging because of the complex 3-D unsteady turbomachinery flow and the effects of rotation on droplet trajectories. The aim of the present research focuses on (i) Developing a computational methodology for <span class="hlt">ice</span> accretion in rotating turbomachinery components; (ii) Investigate the effect of inter-phase heat exchange; (iii) Characterize droplet impingement pattern and <span class="hlt">ice</span> accretion at different operating conditions. The simulations of droplet trajectories are based on a Eulerian-Lagrangian approach for the continuous and discrete phases. The governing equations are solved in the rotating blade frame of reference. The flow field is computed by solving the 3-D solution of the compressible Reynolds Averaged Navier Stokes (RANS) equations. One-way interaction models simulate the effects of aerodynamic forces and the energy exchange between the flow and the droplets. The methodology is implemented in the cool, TURBODROP and applied to the flow field and droplet trajectories in NASA Roto-67r and NASA-GE E3 booster rotor. The results highlight the <span class="hlt">variation</span></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 <span class="hlt">variations</span>, 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> <span class="hlt">masses</span>. 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 <span class="hlt">variations</span>, 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 <span class="hlt">variations</span> in the <span class="hlt">ice</span>-sheet ablation zone caused by dust loading may represent an extremely important ablation mechanism. Using our parameterization of "dirty" snow in the ablation zone 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://www.osti.gov/pages/biblio/1352361-present-day-future-antarctic-ice-sheet-climate-surface-mass-balance-community-earth-system-model','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1352361-present-day-future-antarctic-ice-sheet-climate-surface-mass-balance-community-earth-system-model"><span>Present-day and future Antarctic <span class="hlt">ice</span> sheet climate and surface <span class="hlt">mass</span> balance in the Community Earth System Model</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Lenaerts, Jan T. M.; Vizcaino, Miren; Fyke, Jeremy Garmeson; ...</p> <p>2016-02-01</p> <p>Here, we present climate and surface <span class="hlt">mass</span> balance (SMB) of the Antarctic <span class="hlt">ice</span> sheet (AIS) as simulated by the global, coupled ocean–atmosphere–land Community Earth System Model (CESM) with a horizontal resolution of ~1° in the past, present and future (1850–2100). CESM correctly simulates present-day Antarctic sea <span class="hlt">ice</span> extent, large-scale atmospheric circulation and near-surface climate, but fails to simulate the recent expansion of Antarctic sea <span class="hlt">ice</span>. The present-day Antarctic <span class="hlt">ice</span> sheet SMB equals 2280 ± 131Gtyear –1, which concurs with existing independent estimates of AIS SMB. When forced by two CMIP5 climate change scenarios (high mitigation scenario RCP2.6 and high-emission scenariomore » RCP8.5), CESM projects an increase of Antarctic <span class="hlt">ice</span> sheet SMB of about 70 Gtyear –1 per degree warming. This increase is driven by enhanced snowfall, which is partially counteracted by more surface melt and runoff along the <span class="hlt">ice</span> sheet’s edges. This intensifying hydrological cycle is predominantly driven by atmospheric warming, which increases (1) the moisture-carrying capacity of the atmosphere, (2) oceanic source region evaporation, and (3) summer AIS cloud liquid water content.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110005552','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110005552"><span>ICESat Observations of Seasonal and Interannual <span class="hlt">Variations</span> of Sea-<span class="hlt">Ice</span> Freeboard and Estimated Thickness in the Weddell Sea, Antarctica (2003-2009)</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Yi, Donghui; Robbins, John W.</p> <p>2010-01-01</p> <p>Sea-<span class="hlt">ice</span> freeboard heights for 17 ICESat campaign periods from 2003 to 2009 are derived from ICESat data. Freeboard is combined with snow depth from Advanced Microwave Scanning Radiometer for Earth Observing System (AMSR-E) data and nominal densities of snow, water and sea <span class="hlt">ice</span>, to estimate sea-<span class="hlt">ice</span> thickness. Sea-<span class="hlt">ice</span> freeboard and thickness distributions show clear seasonal <span class="hlt">variations</span> that reflect the yearly cycle of growth and decay of the Weddell Sea (Antarctica) pack <span class="hlt">ice</span>. During October-November, sea <span class="hlt">ice</span> grows to its seasonal maximum both in area and thickness; the mean freeboards are 0.33-0.41 m and the mean thicknesses are 2.10-2.59 m. During February-March, thinner sea <span class="hlt">ice</span> melts away and the sea-<span class="hlt">ice</span> pack is mainly distributed in the west Weddell Sea; the mean freeboards are 0.35-0.46 m and the mean thicknesses are 1.48-1.94 m. During May-June, the mean freeboards and thicknesses are 0.26-0.29 m and 1.32-1.37 m, respectively. The 6 year trends in sea-<span class="hlt">ice</span> extent and volume are (0.023+/-0.051) x 10(exp 6)sq km/a (0.45%/a) and (0.007+/-1.0.092) x 10(exp 3)cu km/a (0.08%/a); however, the large standard deviations indicate that these positive trends are not statistically significant.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUSM.C24A..01S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUSM.C24A..01S"><span>Sea <span class="hlt">Ice</span> Formation Rate and Temporal <span class="hlt">Variation</span> of Temperature and Salinity at the Vicinity of Wilkins <span class="hlt">Ice</span> Shelf from Data Collected by Southern Elephant Seals in 2008</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Santini, M. F.; Souza, R.; Wainer, I.; Muelbert, M.; Hindell, M.</p> <p>2013-05-01</p> <p>The use of marine mammals as autonomous platforms for collecting oceanographic data has revolutionized the understanding of physical properties of low or non-sampled regions of the polar oceans. The use of these animals became possible due to advancements in the development of electronic devices, sensors and batteries carried by them. Oceanographic data collected by two southern elephant seals (Mirounga leonina) during the Fall of 2008 were used to infer the sea-<span class="hlt">ice</span> formation rate in the region adjacent to the Wilkins <span class="hlt">Ice</span> Shelf, west of the Antarctic Peninsula at that period. The sea-<span class="hlt">ice</span> formation rate was estimated from the salt balance equation for the upper (100 m) ocean at a daily frequency for the period between 13 February and 20 June 2008. The oceanographic data collected by the animals were also used to present the temporal <span class="hlt">variation</span> of the water temperature and salinity from surface to 300 m depth in the study area. Sea <span class="hlt">ice</span> formation rate ranged between 0,087 m/day in early April and 0,008 m/day in late June. Temperature and salinity ranged from -1.84°C to 1.60°C and 32.85 to 34.85, respectively, for the upper 300 m of the water column in the analyzed period. The sea-<span class="hlt">ice</span> formation rate estimations do not consider water advection, only temporal changes of the vertical profile of salinity. This may cause underestimates of the real sea-<span class="hlt">ice</span> formation rate. The intense reduction of sea <span class="hlt">ice</span> rate formation from April to June 2008 may be related to the intrusion of the Circumpolar Depth Water (CDW) into the study region. As a consequence of that we believe that this process can be partly responsible for the disintegration of the Wilkins <span class="hlt">Ice</span> Shelf during the winter of 2008. The data presented here are considered a new frontier in physical and biological oceanography, providing a new approach for monitoring sea <span class="hlt">ice</span> changes and oceanographic conditions in polar oceans. This is especially valid for regions covered by sea <span class="hlt">ice</span> where traditional instruments deployed by</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://ntrs.nasa.gov/search.jsp?R=20150021521&hterms=sea&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dsea','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20150021521&hterms=sea&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dsea"><span>An Assessment of Southern Ocean Water <span class="hlt">Masses</span> and Sea <span class="hlt">Ice</span> During 1988-2007 in a Suite of Interannual CORE-II Simulations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Downes, Stephanie M.; Farneti, Riccardo; Uotila, Petteri; Griffies, Stephen M.; Marsland, Simon J.; Bailey, David; Behrens, Erik; Bentsen, Mats; Bi, Daohua; Biastoch, Arne; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20150021521'); toggleEditAbsImage('author_20150021521_show'); toggleEditAbsImage('author_20150021521_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20150021521_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20150021521_hide"></p> <p>2015-01-01</p> <p>We characterise the representation of the Southern Ocean water <span class="hlt">mass</span> structure and sea <span class="hlt">ice</span> within a suite of 15 global ocean-<span class="hlt">ice</span> models run with the Coordinated Ocean-<span class="hlt">ice</span> Reference Experiment Phase II (CORE-II) protocol. The main focus is the representation of the present (1988-2007) mode and intermediate waters, thus framing an analysis of winter and summer mixed layer depths; temperature, salinity, and potential vorticity structure; and temporal variability of sea <span class="hlt">ice</span> distributions. We also consider the interannual variability over the same 20 year period. Comparisons are made between models as well as to observation-based analyses where available. The CORE-II models exhibit several biases relative to Southern Ocean observations, including an underestimation of the model mean mixed layer depths of mode and intermediate water <span class="hlt">masses</span> in March (associated with greater ocean surface heat gain), and an overestimation in September (associated with greater high latitude ocean heat loss and a more northward winter sea-<span class="hlt">ice</span> extent). In addition, the models have cold and fresh/warm and salty water column biases centred near 50 deg S. Over the 1988-2007 period, the CORE-II models consistently simulate spatially variable trends in sea-<span class="hlt">ice</span> concentration, surface freshwater fluxes, mixed layer depths, and 200-700 m ocean heat content. In particular, sea-<span class="hlt">ice</span> coverage around most of the Antarctic continental shelf is reduced, leading to a cooling and freshening of the near surface waters. The shoaling of the mixed layer is associated with increased surface buoyancy gain, except in the Pacific where sea <span class="hlt">ice</span> is also influential. The models are in disagreement, despite the common CORE-II atmospheric state, in their spatial pattern of the 20-year trends in the mixed layer depth and sea-<span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70043697','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70043697"><span>Annual accumulation over the Greenland <span class="hlt">ice</span> sheet interpolated from historical and newly compiled observation data</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Shen, Dayong; Liu, Yuling; Huang, Shengli</p> <p>2012-01-01</p> <p>The estimation of <span class="hlt">ice</span>/snow accumulation is of great significance in quantifying the <span class="hlt">mass</span> balance of <span class="hlt">ice</span> sheets and <span class="hlt">variation</span> in water resources. Improving the accuracy and reducing uncertainty has been a challenge for the estimation of annual accumulation over the Greenland <span class="hlt">ice</span> sheet. In this study, we kriged and analyzed the spatial pattern of accumulation based on an observation data series including 315 points used in a recent research, plus 101 <span class="hlt">ice</span> cores and snow pits and newly compiled 23 coastal weather station data. The estimated annual accumulation over the Greenland <span class="hlt">ice</span> sheet is 31.2 g cm−2 yr−1, with a standard error of 0.9 g cm−2 yr−1. The main differences between the improved map developed in this study and the recently published accumulation maps are in the coastal areas, especially southeast and southwest regions. The analysis of accumulations versus elevation reveals the distribution patterns of accumulation over the Greenland <span class="hlt">ice</span> sheet.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C11B0906W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C11B0906W"><span>Gaussian Process Model for Antarctic Surface <span class="hlt">Mass</span> Balance and <span class="hlt">Ice</span> Core Site Selection</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>White, P. A.; Reese, S.; Christensen, W. F.; Rupper, S.</p> <p>2017-12-01</p> <p>Surface <span class="hlt">mass</span> balance (SMB) is an important factor in the estimation of sea level change, and data are collected to estimate models for prediction of SMB on the Antarctic <span class="hlt">ice</span> sheet. Using Favier et al.'s (2013) quality-controlled aggregate data set of SMB field measurements, a fully Bayesian spatial model is posed to estimate Antarctic SMB and propose new field measurement locations. Utilizing Nearest-Neighbor Gaussian process (NNGP) models, SMB is estimated over the Antarctic <span class="hlt">ice</span> sheet. An Antarctic SMB map is rendered using this model and is compared with previous estimates. A prediction uncertainty map is created to identify regions of high SMB uncertainty. The model estimates net SMB to be 2173 Gton yr-1 with 95% credible interval (2021,2331) Gton yr-1. On average, these results suggest lower Antarctic SMB and higher uncertainty than previously purported [Vaughan et al. (1999); Van de Berg et al. (2006); Arthern, Winebrenner and Vaughan (2006); Bromwich et al. (2004); Lenaerts et al. (2012)], even though this model utilizes significantly more observations than previous models. Using the Gaussian process' uncertainty and model parameters, we propose 15 new measurement locations for field study utilizing a maximin space-filling, error-minimizing design; these potential measurements are identied to minimize future estimation uncertainty. Using currently accepted Antarctic <span class="hlt">mass</span> balance estimates and our SMB estimate, we estimate net <span class="hlt">mass</span> loss [Shepherd et al. (2012); Jacob et al. (2012)]. Furthermore, we discuss modeling details for both space-time data and combining field measurement data with output from mathematical models using the NNGP framework.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.C43A0585U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.C43A0585U"><span>Changes and <span class="hlt">variations</span> in the turning angle of Arctic 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>Ukita, J.; Honda, M.; Ishizuka, S.</p> <p>2012-12-01</p> <p>The motion of sea <span class="hlt">ice</span> is under influences of forcing from winds and currents and of sea <span class="hlt">ice</span> properties. In facing rapidly changing Arctic climate we are interested in whether we observe and quantify changes in sea <span class="hlt">ice</span> conditions reflected in its velocity field. Theoretical consideration on the freedrift model predicts a change in the sea <span class="hlt">ice</span> turning angle with respect to the direction of forcing wind in association with thinning sea <span class="hlt">ice</span> thickness. Possible changes in atmospheric and ocean boundary layer conditions may be reflected in the sea <span class="hlt">ice</span> turning angle through modification of both atmospheric and oceanic Ekman spirals. With these in mind this study examines statistical properties of the turning angle of the Arctic sea <span class="hlt">ice</span> and compares them with atmospheric/<span class="hlt">ice</span>/ocean conditions for the period of 1979-2010 on the basis of IABP buoy data. Preliminary results indicate that over this period the turning angle has varying trends depending on different seasons. We found weakly significant (>90% level) changes in the turning angle from August to October with the maximum trend in October. The direction of trends is counter-clockwise with respect to the geostrophic wind direction, which is consistent with the thinning of sea <span class="hlt">ice</span>. The interannual variability of the turning angle for this peak season of the reduced sea <span class="hlt">ice</span> cover is not the same as that of the Arctic SIE. However, in recent years the turning angle appears to covary with the surface air temperature, providing supporting evidence for the relationship between the angle and sea <span class="hlt">ice</span> thickness. In the presentation we will provide results on the relationships between the turning angle and atmospheric and oceanic variables and further discuss their implications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990064090&hterms=Parkinsons&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3DParkinsons','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990064090&hterms=Parkinsons&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3DParkinsons"><span>Variability of Arctic Sea <span class="hlt">Ice</span> as Viewed from Space</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>1998-01-01</p> <p>Over the past 20 years, satellite passive-microwave radiometry has provided a marvelous means for obtaining information about the variability of the Arctic sea <span class="hlt">ice</span> cover and particularly about sea <span class="hlt">ice</span> concentrations (% areal coverages) and from them <span class="hlt">ice</span> extents and the lengths of the sea <span class="hlt">ice</span> season. This ability derives from the sharp contrast between the microwave emissions of sea <span class="hlt">ice</span> versus liquid water and allows routine monitoring of the vast Arctic sea <span class="hlt">ice</span> cover, which typically varies in extent from a minimum of about 8,000,000 sq km in September to a maximum of about 15,000,000 sq km in March, the latter value being over 1.5 times the area of either the United States or Canada. The vast Arctic <span class="hlt">ice</span> cover has many impacts, including hindering heat, <span class="hlt">mass</span>, and y momentum exchanges between the oceans and the atmosphere, reducing the amount of solar radiation absorbed at the Earth's surface, affecting freshwater transports and ocean circulation, and serving as a vital surface for many species of polar animals. These direct impacts also lead to indirect impacts, including effects on local and perhaps global atmospheric temperatures, effects that are being examined in general circulation modeling studies, where preliminary results indicate that changes on the order of a few percent sea <span class="hlt">ice</span> concentration can lead to temperature changes of 1 K or greater even in local areas outside of the sea <span class="hlt">ice</span> region. Satellite passive-microwave data for November 1978 through December 1996 reveal marked regional and interannual variabilities in both the <span class="hlt">ice</span> extents and the lengths of the sea <span class="hlt">ice</span> season, as well as some statistically significant trends. For the north polar <span class="hlt">ice</span> cover as a whole, maximum <span class="hlt">ice</span> extents varied over a range of 14,700,000 - 15,900,000 km(2), while individual regions showed much greater percentage <span class="hlt">variations</span>, e.g., with the Greenland Sea experiencing a range of 740,000 - 1,1110,000 km(2) in its yearly maximum <span class="hlt">ice</span> coverage. Although <span class="hlt">variations</span> from year to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DPS....4921418S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DPS....4921418S"><span>Water <span class="hlt">ice</span> and sub-micron <span class="hlt">ice</span> particles on Tethys and Mimas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Scipioni, Francesca; Nordheim, Tom; Clark, Roger Nelson; D'Aversa, Emiliano; Cruikshank, Dale P.; Tosi, Federico; Schenk, Paul M.; Combe, Jean-Philippe; Dalle Ore, Cristina M.</p> <p>2017-10-01</p> <p>IntroductionWe present our ongoing work, mapping the <span class="hlt">variation</span> of the main water <span class="hlt">ice</span> absorption bands, and the distribution of the sub-micron particles, across Mimas and Tethys’ surfaces using Cassini-VIMS cubes acquired in the IR range (0.8-5.1 μm). We present our results in the form of maps of <span class="hlt">variation</span> of selected spectral indicators (depth of absorption bands, reflectance peak height, spectral slopes).Data analysisVIMS acquires hyperspectral data in the 0.3-5.1 μm spectral range. We selected VIMS cubes of Tethys and Mimas in the IR range (0.8-5.1 μm). For all pixels in the selected cubes, we measured the band depths for water-<span class="hlt">ice</span> absorptions at 1.25, 1.5 and 2.02 μm and the height of the 3.6 μm reflection peak. Moreover, we considered the spectral indictors for particles smaller than 1 µm [1]: (i) the 2 µm absorption band is asymmetric and (ii) it has the minimum shifted to longer λ (iii) the band depth ratio 1.5/2.0 µm decreases; (iv) the reflection peak at 2.6 µm decreases; (v) the Fresnel reflection peak is suppressed; (vi) the 5 µm reflectance is decreased relative to the 3.6 µm peak. To characterize the global <span class="hlt">variation</span> of water-<span class="hlt">ice</span> band depths, and of sub-micron particles spectral indicators, across Mimas and Tethys, we sampled the two satellites’ surfacees with a 1°x1° fixed-resolution grid and then averaged the band depths and peak values inside each square cell.3. ResultsFor both moons we find that large geologic features, such as the Odysseus and Herschel impact basins, do not correlate with water ice’s abundance <span class="hlt">variation</span>. For Tethys, we found a quite uniform surface on both hemispheres. The only deviation from this pattern shows up on the trailing hemisphere, where we notice two north-oriented, dark areas around 225° and 315°. For Mimas, the leading and trailing hemispheres appear to be quite similar in water <span class="hlt">ice</span> abundance, the trailing portion having water <span class="hlt">ice</span> absorption bands lightly more suppressed than the leading side</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4455714','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4455714"><span>Regional variability in sea <span class="hlt">ice</span> melt in a changing 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>Perovich, Donald K.; Richter-Menge, Jacqueline A.</p> <p>2015-01-01</p> <p>In recent years, the Arctic sea <span class="hlt">ice</span> cover has undergone a precipitous decline in summer extent. The sea <span class="hlt">ice</span> <span class="hlt">mass</span> balance integrates heat and provides insight on atmospheric and oceanic forcing. The amount of surface melt and bottom melt that occurs during the summer melt season was measured at 41 sites over the time period 1957 to 2014. There are large regional and temporal <span class="hlt">variations</span> in both surface and bottom melting. Combined surface and bottom melt ranged from 16 to 294 cm, with a mean of 101 cm. The mean <span class="hlt">ice</span> equivalent surface melt was 48 cm and the mean bottom melt was 53 cm. On average, surface melting decreases moving northward from the Beaufort Sea towards the North Pole; however interannual differences in atmospheric forcing can overwhelm the influence of latitude. Substantial increases in bottom melting are a major contributor to <span class="hlt">ice</span> losses in the Beaufort Sea, due to decreases in <span class="hlt">ice</span> concentration. In the central Arctic, surface and bottom melting demonstrate interannual variability, but show no strong temporal trends from 2000 to 2014. This suggests that under current conditions, summer melting in the central Arctic is not large enough to completely remove the sea <span class="hlt">ice</span> cover. PMID:26032323</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26032323','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26032323"><span>Regional variability in sea <span class="hlt">ice</span> melt in a changing Arctic.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Perovich, Donald K; Richter-Menge, Jacqueline A</p> <p>2015-07-13</p> <p>In recent years, the Arctic sea <span class="hlt">ice</span> cover has undergone a precipitous decline in summer extent. The sea <span class="hlt">ice</span> <span class="hlt">mass</span> balance integrates heat and provides insight on atmospheric and oceanic forcing. The amount of surface melt and bottom melt that occurs during the summer melt season was measured at 41 sites over the time period 1957 to 2014. There are large regional and temporal <span class="hlt">variations</span> in both surface and bottom melting. Combined surface and bottom melt ranged from 16 to 294 cm, with a mean of 101 cm. The mean <span class="hlt">ice</span> equivalent surface melt was 48 cm and the mean bottom melt was 53 cm. On average, surface melting decreases moving northward from the Beaufort Sea towards the North Pole; however interannual differences in atmospheric forcing can overwhelm the influence of latitude. Substantial increases in bottom melting are a major contributor to <span class="hlt">ice</span> losses in the Beaufort Sea, due to decreases in <span class="hlt">ice</span> concentration. In the central Arctic, surface and bottom melting demonstrate interannual variability, but show no strong temporal trends from 2000 to 2014. This suggests that under current conditions, summer melting in the central Arctic is not large enough to completely remove the sea <span class="hlt">ice</span> cover. © 2015 The Author(s) Published by the Royal Society. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20130009418','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130009418"><span>Airborne Tomographic Swath <span class="hlt">Ice</span> Sounding Processing System</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wu, Xiaoqing; Rodriquez, Ernesto; Freeman, Anthony; Jezek, Ken</p> <p>2013-01-01</p> <p>Glaciers and <span class="hlt">ice</span> sheets modulate global sea level by storing water deposited as snow on the surface, and discharging water back into the ocean through melting. Their physical state can be characterized in terms of their <span class="hlt">mass</span> balance and dynamics. To estimate the current <span class="hlt">ice</span> <span class="hlt">mass</span> balance, and to predict future changes in the motion of the Greenland and Antarctic <span class="hlt">ice</span> sheets, it is necessary to know the <span class="hlt">ice</span> sheet thickness and the physical conditions of the <span class="hlt">ice</span> sheet surface and bed. This information is required at fine resolution and over extensive portions of the <span class="hlt">ice</span> sheets. A tomographic algorithm has been developed to take raw data collected by a multiple-channel synthetic aperture sounding radar system over a polar <span class="hlt">ice</span> sheet and convert those data into two-dimensional (2D) <span class="hlt">ice</span> thickness measurements. Prior to this work, conventional processing techniques only provided one-dimensional <span class="hlt">ice</span> thickness measurements along profiles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS22A..07H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS22A..07H"><span>Improved regional sea-level estimates from <span class="hlt">Ice</span> Sheets, Glaciers and land water storage using GRACE time series and other data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>He, Z.; Velicogna, I.; Hsu, C. W.; Rignot, E. J.; Mouginot, J.; Scheuchl, B.; Fettweis, X.; van den Broeke, M. R.</p> <p>2017-12-01</p> <p>Changes in <span class="hlt">ice</span> sheets, glaciers and <span class="hlt">ice</span> caps (GIC) and land water <span class="hlt">mass</span> cause regional sea level <span class="hlt">variations</span> that differ significantly from a uniform re-distribution of <span class="hlt">mass</span> over the ocean, with a decrease in sea level compared to the global mean sea level contribution (GMSL) near the sources of <span class="hlt">mass</span> added to the ocean and an increase up to 30% larger than the GMSL in the far field. The corresponding sea level fingerprints (SLF) are difficult to separate from ocean dynamics on short time and spatial scales but as <span class="hlt">ice</span> melt continues, the SLF signal will become increasingly dominant in the pattern of regional sea level rise. It has been anticipated that it will be another few decades before the land <span class="hlt">ice</span> SLF could be identified in the pattern of regional sea level rise. Here, we combine 40 years of observations of <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balance for Antarctica (1975-present) and Greenland (1978-present), along with surface <span class="hlt">mass</span> balance reconstructions of glacier and <span class="hlt">ice</span> caps <span class="hlt">mass</span> balance (GIC) from 1970s to present to determine the contribution to the SLF from melting land <span class="hlt">ice</span> (MAR and RACMO). We compare the results with observations from GRACE for the time period 2002 to present for evaluation of our approach. Land hydrology is constrained by GRACE data for the period 2002-present and by the GLDAS-NOAH land hydrology model for the longer time period. Over the long time period, we find that the contribution from land <span class="hlt">ice</span> dominates. We quantify the contribution to the total SLF from Greenland and Antarctica in various parts of the world over the past 40 years. More important, we compare the cumulative signal from SLF with tide gauge records around the world, corrected for earth dynamics, to determine whether the land <span class="hlt">ice</span> SLF can be detected in that record. Early results will be reported at the meeting. This work was performed at UC Irvine and at Caltech's Jet Propulsion Laboratory under a contract with NASA's Cryospheric Science Program.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C44A..07D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C44A..07D"><span>Bayesian prediction of future <span class="hlt">ice</span> sheet volume using local approximation Markov chain Monte Carlo methods</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Davis, A. D.; Heimbach, P.; Marzouk, Y.</p> <p>2017-12-01</p> <p>We develop a Bayesian inverse modeling framework for predicting future <span class="hlt">ice</span> sheet volume with associated formal uncertainty estimates. Marine <span class="hlt">ice</span> sheets are drained by fast-flowing <span class="hlt">ice</span> streams, which we simulate using a flowline model. Flowline models depend on geometric parameters (e.g., basal topography), parameterized physical processes (e.g., calving laws and basal sliding), and climate parameters (e.g., surface <span class="hlt">mass</span> balance), most of which are unknown or uncertain. Given observations of <span class="hlt">ice</span> surface velocity and thickness, we define a Bayesian posterior distribution over static parameters, such as basal topography. We also define a parameterized distribution over variable parameters, such as future surface <span class="hlt">mass</span> balance, which we assume are not informed by the data. Hyperparameters are used to represent climate change scenarios, and sampling their distributions mimics internal <span class="hlt">variation</span>. For example, a warming climate corresponds to increasing mean surface <span class="hlt">mass</span> balance but an individual sample may have periods of increasing or decreasing surface <span class="hlt">mass</span> balance. We characterize the predictive distribution of <span class="hlt">ice</span> volume by evaluating the flowline model given samples from the posterior distribution and the distribution over variable parameters. Finally, we determine the effect of climate change on future <span class="hlt">ice</span> sheet volume by investigating how changing the hyperparameters affects the predictive distribution. We use state-of-the-art Bayesian computation to address computational feasibility. Characterizing the posterior distribution (using Markov chain Monte Carlo), sampling the full range of variable parameters and evaluating the predictive model is prohibitively expensive. Furthermore, the required resolution of the inferred basal topography may be very high, which is often challenging for sampling methods. Instead, we leverage regularity in the predictive distribution to build a computationally cheaper surrogate over the low dimensional quantity of interest (future <span class="hlt">ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70029576','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70029576"><span>Effects of maternal characteristics and climatic <span class="hlt">variation</span> on birth <span class="hlt">masses</span> of Alaskan caribou</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Adams, Layne G.</p> <p>2005-01-01</p> <p>Understanding factors that influence birth <span class="hlt">mass</span> of mammals provides insights to nutritional trade-offs made by females to optimize their reproduction, growth, and survival. I evaluated <span class="hlt">variation</span> in birth <span class="hlt">mass</span> of caribou (Rangifer tarandus) in central Alaska relative to maternal characteristics (age, body <span class="hlt">mass</span>, cohort, and nutritional condition as influenced by winter severity) during 11 years with substantial <span class="hlt">variation</span> in winter snowfall. Snowfall during gestation was the predominant factor explaining <span class="hlt">variation</span> in birth <span class="hlt">masses</span>, influencing birth <span class="hlt">mass</span> inversely and through interactions with maternal age and lactation status. Maternal age effects were noted for females ≤ 5 years old, declining in magnitude with each successive age class. Birth <span class="hlt">mass</span> as a proportion of autumn maternal <span class="hlt">mass</span> was inversely related to winter snowfall, even though there was no decrease in <span class="hlt">masses</span> of adult females in late winter associated with severe winters. I found no evidence of a hypothesized intergenerational effect of lower birth <span class="hlt">masses</span> for offspring of females born after severe winters. Caribou produce relatively small offspring but provide exceptional lactation support for those that survive. Conservative maternal investment before parturition may represent an optimal reproductive strategy given that caribou experience stochastic <span class="hlt">variation</span> in winter severity during gestation, uncertainty of environmental conditions surrounding the birth season, and intense predation on neonates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015ApJ...807...29Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015ApJ...807...29Y"><span>Systematic <span class="hlt">Variations</span> in CO2/H2O <span class="hlt">Ice</span> Abundance Ratios in Nearby Galaxies Found with AKARI Near-infrared Spectroscopy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yamagishi, M.; Kaneda, H.; Ishihara, D.; Oyabu, S.; Onaka, T.; Shimonishi, T.; Suzuki, T.</p> <p>2015-07-01</p> <p>We report CO2/H2O <span class="hlt">ice</span> abundance ratios in seven nearby star-forming galaxies based on the AKARI near-infrared (2.5-5.0 μm) spectra. The CO2/H2O <span class="hlt">ice</span> abundance ratios show clear <span class="hlt">variations</span> between 0.05 and 0.2 with the averaged value of 0.14 ± 0.01. The previous study on M82 revealed that the CO2/H2O <span class="hlt">ice</span> abundance ratios strongly correlate with the intensity ratios of the hydrogen recombination Brα line to the polycyclic aromatic hydrocarbon (PAH) 3.3 μm feature. In the present study, however, we find no correlation for the seven galaxies as a whole due to systematic differences in the relation between CO2/H2O <span class="hlt">ice</span> abundance and Brα/PAH 3.3 μm intensity ratios from galaxy to galaxy. This result suggests that there is another parameter that determines the CO2/H2O <span class="hlt">ice</span> abundance ratios in a galaxy in addition to the Brα/PAH 3.3 μm ratios. We find that the CO2/H2O <span class="hlt">ice</span> abundance ratios positively correlate with the specific star formation rates of the galaxies. From these results, we conclude that CO2/H2O <span class="hlt">ice</span> abundance ratios tend to be high in young star-forming galaxies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1989QuRes..31..119P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1989QuRes..31..119P"><span>Modeling the growth and decay of the Antarctic Peninsula <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Payne, A. J.; Sugden, D. E.; Clapperton, C. M.</p> <p>1989-03-01</p> <p>A model of the growth and decay of the Antarctic Peninsula <span class="hlt">Ice</span> Sheet during the last glacial/interglacial cycle is used to identify the main controls on <span class="hlt">ice</span> sheet behavior. Using as input glaciological assumptions derived by W. F. Budd and I. N. Smith (1982, Annals of Glaciology3, 42-49), bedrock topography, isostatic compensation, and <span class="hlt">mass</span> balance relationships, the model is driven by sea-level change over the last 40,000 yr in association with assumed changes in the rate of melting beneath <span class="hlt">ice</span> shelves. An <span class="hlt">ice</span> sheet dome over 3.5 km thick grows on the offshore shelf and straits west of the Antarctic Peninsula and reaches a maximum at 18,000 yr B.P. Collapse begins at 14,000 yr B.P. but becomes rapid and continuous after 10,000 yr B.P. The present stable <span class="hlt">ice</span> cover is achieved at 6500 yr B.P. <span class="hlt">Ice</span> growth and decay are characterized by thresholds which separate periods of steady state from periods of rapid transition; the thresholds usually relate to topography. Tests show that <span class="hlt">ice</span> sheet behavior is most sensitive to sea-level change, basal marine melting, and accumulation and is less sensitive to isostasy, spatial <span class="hlt">variation</span> in accumulation, calving rates, and <span class="hlt">ice</span> flow parameterization. Tests of the model against field evidence show good agreement in places, as well as discrepancies which require further work.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.2064S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.2064S"><span>Using the glacial geomorphology of palaeo-<span class="hlt">ice</span> streams to understand mechanisms of <span class="hlt">ice</span> sheet collapse</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stokes, Chris R.; Margold, Martin; Clark, Chris; Tarasov, Lev</p> <p>2017-04-01</p> <p>Processes which bring about <span class="hlt">ice</span> sheet deglaciation are critical to our understanding of glacial-interglacial cycles and <span class="hlt">ice</span> sheet sensitivity to climate change. The precise mechanisms of deglaciation are also relevant to our understanding of modern-day <span class="hlt">ice</span> sheet stability and concerns over global sea level rise. <span class="hlt">Mass</span> loss from <span class="hlt">ice</span> sheets can be broadly partitioned between melting and a 'dynamic' component whereby rapidly-flowing <span class="hlt">ice</span> streams/outlet glaciers transfer <span class="hlt">ice</span> from the interior to the oceans. Surface and basal melting (e.g. of <span class="hlt">ice</span> shelves) are closely linked to atmospheric and oceanic conditions, but the mechanisms that drive dynamic changes in <span class="hlt">ice</span> stream discharge are more complex, which generates much larger uncertainties about their future contribution to <span class="hlt">ice</span> sheet <span class="hlt">mass</span> loss and sea level rise. A major problem is that observations of modern-day <span class="hlt">ice</span> streams typically span just 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 during deglaciation. A key question is whether <span class="hlt">ice</span> streams might increase and sustain rates of <span class="hlt">mass</span> loss over centuries or millennia, beyond those expected for a given ocean-climate forcing. To address this issue, numerous workers have sought to understand <span class="hlt">ice</span> stream dynamics over longer time-scales using their glacial geomorphology in the palaeo-record. Indeed, our understanding of their geomorphology has grown rapidly in the last three decades, from almost complete ignorance to a detailed knowledge of their geomorphological products. Building on this body of work, this paper uses the glacial geomorphology of 117 <span class="hlt">ice</span> streams in the North American Laurentide <span class="hlt">Ice</span> Sheet to reconstruct their activity during its deglaciation ( 22,000 to 7,000 years ago). <span class="hlt">Ice</span> stream activity was characterised by high variability in both time and space, with <span class="hlt">ice</span> streams switching on and off in different locations. During deglaciation, we find that their overall number decreased, they occupied a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1258751-developing-bounding-ice-particle-mass-area-dimension-expressions-use-atmospheric-models-remote-sensing','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1258751-developing-bounding-ice-particle-mass-area-dimension-expressions-use-atmospheric-models-remote-sensing"><span>Developing and bounding <span class="hlt">ice</span> particle <span class="hlt">mass</span>- and area-dimension expressions for use in atmospheric models and remote sensing</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Erfani, Ehsan; Mitchell, David L.</p> <p>2016-04-07</p> <p>Here, <span class="hlt">ice</span> particle <span class="hlt">mass</span>- and projected area-dimension ( m- D and A- D) power laws are commonly used in the treatment of <span class="hlt">ice</span> cloud microphysical and optical properties and the remote sensing of <span class="hlt">ice</span> cloud properties. Although there has long been evidence that a single m- D or A- D power law is often not valid over all <span class="hlt">ice</span> particle sizes, few studies have addressed this fact. This study develops self-consistent m- D and A- D expressions that are not power laws but can easily be reduced to power laws for the <span class="hlt">ice</span> particle size (maximum dimension or D) rangemore » of interest, and they are valid over a much larger D range than power laws. This was done by combining ground measurements of individual <span class="hlt">ice</span> particle m and D formed at temperature T < –20 °C during a cloud seeding field campaign with 2-D stereo (2D-S) and cloud particle imager (CPI) probe measurements of D and A, and estimates of m, in synoptic and anvil <span class="hlt">ice</span> clouds at similar temperatures. The resulting m- D and A- D expressions are functions of temperature and cloud type (synoptic vs. anvil), and are in good agreement with m- D power laws developed from recent field studies considering the same temperature range (–60 °C < T < –20 °C).« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140007380','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140007380"><span>Microwave Properties of <span class="hlt">Ice</span>-Phase Hydrometeors for Radar and Radiometers: Sensitivity to Model Assumptions</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Johnson, Benjamin T.; Petty, Grant W.; Skofronick-Jackson, Gail</p> <p>2012-01-01</p> <p>A simplied framework is presented for assessing the qualitative sensitivities of computed microwave properties, satellite brightness temperatures, and radar reflectivities to assumptions concerning the physical properties of <span class="hlt">ice</span>-phase hydrometeors. Properties considered included the shape parameter of a gamma size distribution andthe melted-equivalent <span class="hlt">mass</span> median diameter D0, the particle density, dielectric mixing formula, and the choice of complex index of refraction for <span class="hlt">ice</span>. We examine these properties at selected radiometer frequencies of 18.7, 36.5, 89.0, and 150.0 GHz; and radar frequencies at 2.8, 13.4, 35.6, and 94.0 GHz consistent with existing and planned remote sensing instruments. Passive and active microwave observables of <span class="hlt">ice</span> particles arefound to be extremely sensitive to the melted-equivalent <span class="hlt">mass</span> median diameter D0 ofthe size distribution. Similar large sensitivities are found for <span class="hlt">variations</span> in the <span class="hlt">ice</span> vol-ume fraction whenever the geometric <span class="hlt">mass</span> median diameter exceeds approximately 1/8th of the wavelength. At 94 GHz the two-way path integrated attenuation is potentially large for dense compact particles. The distribution parameter mu has a relatively weak effect on any observable: less than 1-2 K in brightness temperature and up to 2.7 dB difference in the effective radar reflectivity. Reversal of the roles of <span class="hlt">ice</span> and air in the MaxwellGarnett dielectric mixing formula leads to a signicant change in both microwave brightness temperature (10 K) and radar reflectivity (2 dB). The choice of Warren (1984) or Warren and Brandt (2008) for the complex index of refraction of <span class="hlt">ice</span> can produce a 3%-4% change in the brightness temperature depression.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AIPC.1547..659M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AIPC.1547..659M"><span>Simulation of air-droplet mixed phase flow in <span class="hlt">icing</span> wind-tunnel</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mengyao, Leng; Shinan, Chang; Menglong, Wu; Yunhang, Li</p> <p>2013-07-01</p> <p><span class="hlt">Icing</span> wind-tunnel is the main ground facility for the research of aircraft <span class="hlt">icing</span>, which is different from normal wind-tunnel for its refrigeration system and spraying system. In stable section of <span class="hlt">icing</span> wind-tunnel, the original parameters of droplets and air are different, for example, to keep the nozzles from freezing, the droplets are heated while the temperature of air is low. It means that complex <span class="hlt">mass</span> and heat transfer as well as dynamic interactive force would happen between droplets and air, and the parameters of droplet will acutely change along the passageway. Therefore, the prediction of droplet-air mixed phase flow is necessary in the evaluation of <span class="hlt">icing</span> researching wind-tunnel. In this paper, a simplified droplet-air mixed phase flow model based on Lagrangian method was built. The <span class="hlt">variation</span> of temperature, diameter and velocity of droplet, as well as the air flow field, during the flow process were obtained under different condition. With calculating three-dimensional air flow field by FLUENT, the droplet could be traced and the droplet distribution could also be achieved. Furthermore, the patterns about how initial parameters affect the parameters in test section were achieved. The numerical simulation solving the flow and heat and <span class="hlt">mass</span> transfer characteristics in the mixing process is valuable for the optimization of experimental parameters design and equipment adjustment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.4347K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.4347K"><span>Temperature <span class="hlt">variations</span> in Greenland from 10 to 110 kyr b2k derived from the NGRIP <span class="hlt">ice</span> core</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kindler, Philippe; Leuenberger, Markus; Landais, Amaelle; Guillevic, Myriam</p> <p>2013-04-01</p> <p>During the last <span class="hlt">ice</span> age dramatic temperature <span class="hlt">variations</span> of up to 16 °C took place in Greenland which are now known as Dansgaard-Oeschger-events (DO-events). They most probably originate from the North Atlantic oceanic and atmospheric circulation system and are characterised by an abrupt warming within decades followed by a gradual cooling over hundreds to thousands of years. We have determined local temperature <span class="hlt">variations</span> for DO-event 1 to 25 in Greenland based on δ15N measurements from the NorthGRIP <span class="hlt">ice</span> core, corresponding to the period from 10 to 110 kyr b2k. The record is a composite of measurements from two laboratories, Laboratoire des Sciences du Climat et de l'Environnement, Paris (DO 18 to 25) and the Climate and Environmental Physics Division of the Physics Institute of the University of Bern (DO 1 to 17) with new measurements from the beginning of the Holocene to DO 8. Temperature <span class="hlt">variations</span> were reconstructed by reproducing the measured 15N/14N ratio of air enclosed in <span class="hlt">ice</span> bubbles by the firn densification and heat diffusion model from Schwander. The reconstruction show temperature amplitudes for the DO-events ranging from 5 to 16 °C, thereby the corresponding rates of change can exceed 0.5 °C/decade. In order get an agreement between measured δ15N, Δdepth and Δage values with their modelled analogues, a lower accumulation rate than the one associated with the used ss09sea06bm1 time scale had to be assumed. We had to reduce the accumulation rate time dependently by 0 to nearly 40% with a mean reduction over the whole time period of 16%. With these adjustments both the Δdepth and the Δage values agree between model and measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C11C0775W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C11C0775W"><span>Seismic Excitation of the Ross <span class="hlt">Ice</span> Shelf by Whillans <span class="hlt">Ice</span> Stream Stick-Slip Events</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wiens, D.; Pratt, M. J.; Aster, R. C.; Nyblade, A.; Bromirski, P. D.; Stephen, R. A.; Gerstoft, P.; Diez, A.; Cai, C.; Anthony, R. E.; Shore, P.</p> <p>2015-12-01</p> <p>Rapid <span class="hlt">variations</span> in the flow rate of upstream glaciers and <span class="hlt">ice</span> streams may cause significant deformation of <span class="hlt">ice</span> shelves. The Whillans <span class="hlt">Ice</span> Stream (WIS) represents an extreme example of rapid <span class="hlt">variations</span> in velocity, with motions near the grounding line consisting almost entirely of once or twice-daily stick-slip events with a displacement of up to 0.7 m (Winberry et al, 2014). Here we report observations of compressional waves from the WIS slip events propagating hundreds of kilometers across the Ross <span class="hlt">Ice</span> Shelf (RIS) detected by broadband seismographs deployed on the <span class="hlt">ice</span> shelf. The WIS slip events consist of rapid basal slip concentrated at three high friction regions (often termed sticky-spots or asperities) within a period of about 25 minutes (Pratt et al, 2014). Compressional displacement pulses from the second and third sticky spots are detected across the entire RIS up to about 600 km away from the source. The largest pulse results from the third sticky spot, located along the northwestern grounding line of the WIS. Propagation velocities across the <span class="hlt">ice</span> shelf are significantly slower than the P wave velocity in <span class="hlt">ice</span>, as the long period displacement pulse is also sensitive to velocities of the water and sediments beneath the <span class="hlt">ice</span> shelf. Particle motions are, to the limit of resolution, entirely within the horizontal plane and roughly radial with respect to the WIS sticky-spots, but show significant complexity, presumably due to differences in <span class="hlt">ice</span> velocity, thickness, and the thickness of water and sediment beneath. Study of this phenomenon should lead to greater understanding of how the <span class="hlt">ice</span> shelf responds to sudden forcing around the periphery.</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://hdl.handle.net/2060/19910013870','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910013870"><span>Advanced <span class="hlt">ice</span> protection systems test in the NASA Lewis <span class="hlt">icing</span> research tunnel</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bond, Thomas H.; Shin, Jaiwon; Mesander, Geert A.</p> <p>1991-01-01</p> <p>Tests of eight different deicing systems based on <span class="hlt">variations</span> of three different technologies were conducted in the NASA Lewis Research Center <span class="hlt">Icing</span> Research Tunnel (IRT) in June and July 1990. The systems used pneumatic, eddy current repulsive, and electro-expulsive means to shed <span class="hlt">ice</span>. The tests were conducted on a 1.83 m span, 0.53 m chord NACA 0012 airfoil operated at a 4 degree angle of attack. The models were tested at two temperatures: a glaze condition at minus 3.9 C and a rime condition at minus 17.2 C. The systems were tested through a range of <span class="hlt">icing</span> spray times and cycling rates. Characterization of the deicers was accomplished by monitoring power consumption, <span class="hlt">ice</span> shed particle size, and residual <span class="hlt">ice</span>. High speed video motion analysis was performed to quantify <span class="hlt">ice</span> particle size.</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' zone, 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 zone 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 <span class="hlt">mass</span> flux that satisfies the contact conditions. When no sliding is allowed at the bed, however, we find a range of <span class="hlt">mass</span> 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/2014EGUGA..16.5811B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.5811B"><span>On the capability of Swarm for surface <span class="hlt">mass</span> <span class="hlt">variation</span> monitoring: Quantitative assessment based on orbit information from CHAMP, GRACE and GOCE</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Baur, Oliver; Weigelt, Matthias; Zehentner, Norbert; Mayer-Gürr, Torsten; Jäggi, Adrian</p> <p>2014-05-01</p> <p>In the last decade, temporal <span class="hlt">variations</span> of the gravity field from GRACE observations have become one of the most ubiquitous and valuable sources of information for geophysical and environmental studies. In the context of global climate change, <span class="hlt">mass</span> balance of the Arctic and Antarctic <span class="hlt">ice</span> sheets gained particular attention. Because GRACE has outlived its predicted lifetime by several years already, it is very likely that a gap between GRACE and its successor GRACE follow-on (supposed to be launched in 2017, at the earliest) occurs. The Swarm mission - launched on November 22, 2013 - is the most promising candidate to bridge this potential gap, i.e., to directly acquire large-scale <span class="hlt">mass</span> <span class="hlt">variation</span> information on the Earth's surface in case of a gap between the present GRACE and the upcoming GRACE follow-on projects. Although the magnetometry mission Swarm has not been designed for gravity field purposes, its three satellites have the characteristics for such an endeavor: (i) low, near-circular and near-polar orbits, (ii) precise positioning with high-quality GNSS receivers, (iii) on-board accelerometers to measure the influence of non-gravitational forces. Hence, from an orbit analysis point of view the Swarm satellites are comparable to the CHAMP, GRACE and GOCE spacecraft. Indeed and as data analysis from CHAMP has been shown, the detection of annual signals and trends from orbit analysis is possible for long-wavelength features of the gravity field, although the accuracy associated with the inter-satellite GRACE measurements cannot be reached. We assess the capability of the (non-dedicated) mission Swarm for <span class="hlt">mass</span> <span class="hlt">variation</span> detection in a real-case environment (opposed to simulation studies). For this purpose, we "approximate" the Swarm scenario by the GRACE+CHAMP and GRACE+GOCE constellations. In a first step, kinematic orbits of the individual satellites are derived from GNSS observations. From these orbits, we compute monthly combined GRACE+CHAMP and GRACE</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.9455M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.9455M"><span>Submesoscale Sea <span class="hlt">Ice</span>-Ocean Interactions in Marginal <span class="hlt">Ice</span> Zones</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Manucharyan, Georgy E.; Thompson, Andrew F.</p> <p>2017-12-01</p> <p>Signatures of ocean eddies, fronts, and filaments are commonly observed within marginal <span class="hlt">ice</span> zones (MIZs) from satellite images of sea <span class="hlt">ice</span> concentration, and in situ observations via <span class="hlt">ice</span>-tethered profilers or underice gliders. However, localized and intermittent sea <span class="hlt">ice</span> heating and advection by ocean eddies are currently not accounted for in climate models and may contribute to their biases and errors in sea <span class="hlt">ice</span> forecasts. Here, we explore mechanical sea <span class="hlt">ice</span> 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 <span class="hlt">ice</span> and advect it over warmer surface ocean waters where it can effectively melt. The horizontal eddy diffusivity of sea <span class="hlt">ice</span> <span class="hlt">mass</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> can contribute to the seasonal evolution of MIZs. With the continuing global warming and sea <span class="hlt">ice</span> thickness reduction in the Arctic Ocean, submesoscale sea <span class="hlt">ice</span>-ocean processes are expected to become increasingly prominent.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003AGUFM.P32B..02H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003AGUFM.P32B..02H"><span>Geological Evidence for Recent <span class="hlt">Ice</span> Ages on Mars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Head, J. W.; Mustard, J. F.; Kreslavsky, M. A.; Milliken, R. E.; Marchant, D. R.</p> <p>2003-12-01</p> <p>A primary cause of <span class="hlt">ice</span> ages on Earth is orbital forcing from <span class="hlt">variations</span> in orbital parameters of the planet. On Mars such <span class="hlt">variations</span> are known to be much more extreme. Recent exploration of Mars has revealed abundant water <span class="hlt">ice</span> in the near-surface at high latitudes in both hemispheres. We outline evidence that these near-surface, water-<span class="hlt">ice</span> rich mantling deposits represent a mixture of <span class="hlt">ice</span> and dust that is layered, meters thick, and latitude dependent. These units were formed during a geologically recent major martian <span class="hlt">ice</span> age, and were emplaced in response to the changing stability of water <span class="hlt">ice</span> and dust on the surface during <span class="hlt">variations</span> in orbital parameters. Evidence for these units include a smoothing of topography at subkilometer baselines from about 30o north and south latitudes to the poles, a distinctive dissected texture in MOC images in the +/-30o-60o latitude band, latitude-dependent sets of topographic characteristics and morphologic features (e.g., polygons, 'basketball' terrain texture, gullies, viscous flow features), and hydrogen concentrations consistent with the presence of abundant <span class="hlt">ice</span> at shallow depths above 60o latitude. The most equatorward extent of these <span class="hlt">ice</span>-rich deposits was emplaced down to latitudes equivalent to Saudi Arabia and the southern United States on Earth during the last major martian <span class="hlt">ice</span> age, probably about 0.4-2.1 million years ago. Mars is currently in an inter-<span class="hlt">ice</span> age period and the <span class="hlt">ice</span>-rich deposits are presently undergoing reworking, degradation and retreat in response to the current stability relations of near-surface <span class="hlt">ice</span>. Unlike Earth, martian <span class="hlt">ice</span> ages are characterized by warmer climates in the polar regions and the enhanced role of atmospheric water <span class="hlt">ice</span> and dust transport and deposition to produce widespread and relatively evenly distributed smooth deposits at mid-latitudes during obliquity maxima.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20050071088&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=20050071088&hterms=sauber&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsauber"><span>Southern Alaska Glaciers: Spatial and Temporal <span class="hlt">Variations</span> in <span class="hlt">Ice</span> Volume</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sauber, J.; Molnia, B. F.; Lutchke, S.; Rowlands, D.; Harding, D.; Carabajal, C.; Hurtado, J. M.; Spade, G.</p> <p>2004-01-01</p> <p>Although temperate mountain glaciers comprise less than 1% of the glacier-covered area on Earth, they are important because they appear to be melting rapidly under present climatic conditions and, therefore, make significant contributions to rising sea level. In this study, we use ICESat observations made in the last 1.5 years of southern Alaska glaciers to estimate <span class="hlt">ice</span> elevation profiles, <span class="hlt">ice</span> surface slopes and roughness, and bi-annual and/or annual <span class="hlt">ice</span> elevation changes. We report initial results from the near coastal region between Yakutat Bay and Cape Suckling that includes the Malaspina and Bering Glaciers. We show and interpret <span class="hlt">ice</span> elevations changes across the lower reaches of the Bagley <span class="hlt">Ice</span> Valley for the period between October 2003 and May 2004. In addition, we use off-nadir pointing observations to reference tracks over the Bering and Malaspina Glaciers in order to estimate annual <span class="hlt">ice</span> elevation change. Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) and Shuttle Radar Topography Mission (SRTM) derived DEMs are used to estimate across track regional slopes between ICESat data acquisitions. Although the distribution and quantity of ICESat elevation profiles with multiple, exact repeat data is currently limited in Alaska, individual ICESat data tracks, provide an accurate reference surface for comparison to other elevation data (e.g. ASTER and SRTM X- and C-band derived DEMs). Specifically we report the elevation change over the Malaspina Glacier's piedmont lobe between a DEM derived from SRTM C-band data acquired in Feb. 2000 and ICESat Laser #2b data from Feb.-March 2004. We also report use of ICESat elevation data to enhance ASTER derived absolute DEMs. Mountain glaciers generally have rougher surfaces and steeper regional slopes than the <span class="hlt">ice</span> sheets for which the ICESat design was optimized. Therefore, rather than averaging ICESat observations over large regions or relying on crossovers, we are working with well-located ICESat</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1346837','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1346837"><span>A New Discrete Element Sea-<span class="hlt">Ice</span> Model for Earth System Modeling</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>Turner, Adrian Keith</p> <p></p> <p>Sea <span class="hlt">ice</span> forms a frozen crust of sea water oating in high-latitude oceans. It is a critical component of the Earth system because its formation helps to drive the global thermohaline circulation, and its seasonal waxing and waning in the high north and Southern Ocean signi cantly affects planetary albedo. Usually 4{6% of Earth's marine surface is covered by sea <span class="hlt">ice</span> at any one time, which limits the exchange of heat, momentum, and <span class="hlt">mass</span> between the atmosphere and ocean in the polar realms. Snow accumulates on sea <span class="hlt">ice</span> and inhibits its vertical growth, increases its albedo, and contributes to pooledmore » water in melt ponds that darken the Arctic <span class="hlt">ice</span> surface in the spring. <span class="hlt">Ice</span> extent and volume are subject to strong seasonal, inter-annual and hemispheric <span class="hlt">variations</span>, and climatic trends, which Earth System Models (ESMs) are challenged to simulate accurately (Stroeve et al., 2012; Stocker et al., 2013). This is because there are strong coupled feedbacks across the atmosphere-<span class="hlt">ice</span>-ocean boundary layers, including the <span class="hlt">ice</span>-albedo feedback, whereby a reduced <span class="hlt">ice</span> cover leads to increased upper ocean heating, further enhancing sea-<span class="hlt">ice</span> melt and reducing incident solar radiation re ected back into the atmosphere (Perovich et al., 2008). A reduction in perennial Arctic sea-<span class="hlt">ice</span> during the satellite era has been implicated in mid-latitude weather changes, including over North America (Overland et al., 2015). Meanwhile, most ESMs have been unable to simulate observed inter-annual variability and trends in Antarctic sea-<span class="hlt">ice</span> extent during the same period (Gagne et al., 2014).« less</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 <span class="hlt">variations</span> 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-<span class="hlt">mass</span> 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 zone in warm climate simulations. When combined with recently suggested mechanisms for retreat into subglacial basins due to <span class="hlt">ice</span> shelf hydrofracture and <span class="hlt">ice</span> cliff failure, we are able to simulate large-scale variability of the 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://adsabs.harvard.edu/abs/2017Chaos..27g3101K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Chaos..27g3101K"><span>Fire, <span class="hlt">ice</span>, water, and dirt: A simple climate model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kroll, John</p> <p>2017-07-01</p> <p>A simple paleoclimate model was developed as a modeling exercise. The model is a lumped parameter system consisting of an ocean (water), land (dirt), glacier, and sea <span class="hlt">ice</span> (<span class="hlt">ice</span>) and driven by the sun (fire). In comparison with other such models, its uniqueness lies in its relative simplicity yet yielding good results. For nominal values of parameters, the system is very sensitive to small changes in the parameters, yielding equilibrium, steady oscillations, and catastrophes such as freezing or boiling oceans. However, stable solutions can be found, especially naturally oscillating solutions. For nominally realistic conditions, natural periods of order 100kyrs are obtained, and chaos ensues if the Milankovitch orbital forcing is applied. An analysis of a truncated system shows that the naturally oscillating solution is a limit cycle with the characteristics of a relaxation oscillation in the two major dependent variables, the ocean temperature and the glacier <span class="hlt">ice</span> extent. The key to getting oscillations is having the effective emissivity decreasing with temperature and, at the same time, the effective ocean albedo decreases with increasing glacier extent. Results of the original model compare favorably to the proxy data for <span class="hlt">ice</span> <span class="hlt">mass</span> <span class="hlt">variation</span>, but not for temperature <span class="hlt">variation</span>. However, modifications to the effective emissivity and albedo can be made to yield much more realistic results. The primary conclusion is that the opinion of Saltzman [Clim. Dyn. 5, 67-78 (1990)] is plausible that the external Milankovitch orbital forcing is not sufficient to explain the dominant 100kyr period in the data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28764399','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28764399"><span>Fire, <span class="hlt">ice</span>, water, and dirt: A simple climate model.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kroll, John</p> <p>2017-07-01</p> <p>A simple paleoclimate model was developed as a modeling exercise. The model is a lumped parameter system consisting of an ocean (water), land (dirt), glacier, and sea <span class="hlt">ice</span> (<span class="hlt">ice</span>) and driven by the sun (fire). In comparison with other such models, its uniqueness lies in its relative simplicity yet yielding good results. For nominal values of parameters, the system is very sensitive to small changes in the parameters, yielding equilibrium, steady oscillations, and catastrophes such as freezing or boiling oceans. However, stable solutions can be found, especially naturally oscillating solutions. For nominally realistic conditions, natural periods of order 100kyrs are obtained, and chaos ensues if the Milankovitch orbital forcing is applied. An analysis of a truncated system shows that the naturally oscillating solution is a limit cycle with the characteristics of a relaxation oscillation in the two major dependent variables, the ocean temperature and the glacier <span class="hlt">ice</span> extent. The key to getting oscillations is having the effective emissivity decreasing with temperature and, at the same time, the effective ocean albedo decreases with increasing glacier extent. Results of the original model compare favorably to the proxy data for <span class="hlt">ice</span> <span class="hlt">mass</span> <span class="hlt">variation</span>, but not for temperature <span class="hlt">variation</span>. However, modifications to the effective emissivity and albedo can be made to yield much more realistic results. The primary conclusion is that the opinion of Saltzman [Clim. Dyn. 5, 67-78 (1990)] is plausible that the external Milankovitch orbital forcing is not sufficient to explain the dominant 100kyr period in the data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.G21A0871Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.G21A0871Z"><span>Rapid <span class="hlt">Ice</span> Loss at Vatnajokull,Iceland Since Late 1990s Constrained by Synthetic Aperture Radar Interferometry</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>2012-12-01</p> <p>Synthetic aperture radar interferometry time series is applied over Vatnajokull, Iceland by using 15 years ERS data. <span class="hlt">Ice</span> loss at Vatnajokull accelerates since late 1990s especially after 21th century. Clear uplift signal due to <span class="hlt">ice</span> <span class="hlt">mass</span> loss is detected. The rebound signal is generally linear and increases a little bit after 2000. The relative annual velocity (GPS station 7485 as reference) is about 12 mm/yr at the <span class="hlt">ice</span> cap edge, which matches the previous studies using GPS. The standard deviation compared to 11 GPS stations in this area is about 2 mm/yr. A relative-value modeling method ignoring the effect of viscous flow is chosen assuming elastic half space earth. The final <span class="hlt">ice</span> loss estimation - 83 cm/yr - matches the climatology model with ground observations. Small Baseline Subsets is applied for time series analysis. Orbit error coupling with long wavelength phase trend due to horizontal plate motion is removed based on a second polynomial model. For simplicity, we do not consider atmospheric delay in this area because of no complex topography and small-scale turbulence is eliminated well after long-term average when calculating the annual mean velocity. Some unwrapping error still exits because of low coherence. Other uncertainties can be the basic assumption of <span class="hlt">ice</span> loss pattern and spatial <span class="hlt">variation</span> of the elastic parameters. It is the first time we apply InSAR time series for <span class="hlt">ice</span> <span class="hlt">mass</span> balance study and provide detailed error and uncertainty analysis. The successful of this application proves InSAR as an option for <span class="hlt">mass</span> balance study and it is also important for validation of different <span class="hlt">ice</span> loss estimation techniques.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.7451H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.7451H"><span>Organic components in hair-<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>Hofmann, Diana; Steffen, Bernhard; Disko, Ulrich; Wagner, Gerhard; Mätzler, Christian</p> <p>2013-04-01</p> <p>Hair-<span class="hlt">ice</span> is a rather unknown phenomenon. In contrast to generally known frost needles, originating from atmospheric water and expanding e.g. from plant surfaces in all directions, hair <span class="hlt">ice</span> grows from the basis of wet, rotten hardwood. The hair-like, flexible, linear structures may reach up to 10 cm in length without any ramifications. Hair-<span class="hlt">ice</span> appears to be related to the biological activity of a fungus mycelium within the wood. Hair-<span class="hlt">ice</span> can attract winter-active Collemboles (snow flea, Isotoma nivalis). At the onset of hair-<span class="hlt">ice</span> melt a very thin fibre becomes apparent, which carries brownish pearl-like water drops. Therefore, it is supposed that organic substances are inherent, which could possibly act as freezing catalyst as well as recrystallization inhibitor. The aim of this work was the chemical characterization of organic substances contained in hair-<span class="hlt">ice</span>. First analyses of melted hair-<span class="hlt">ice</span> show a total organic carbon (TOC) value of 235 mg/l in contrast to 11 mg/l total nitrogen. Most of inherent nitrogen (70 %) exists thereby as ammonium. Screened by different (<span class="hlt">mass</span> spectrometric) methods, no evidence could be found for the initially expected organic substances like proteins, lipids, small volatile substances or carboxylic acids. By coupling of Ultra Performance Liquid Chromatography with a triple quadrupol <span class="hlt">mass</span> spectrometer (UPLC-MS) a non-resolved chromatogram from a melted hair-<span class="hlt">ice</span> sample was received. Averaged spectra from different regions are similar among themselves with a broad peak spreading over the <span class="hlt">mass</span> range 100-650 Da with favored intense, odd-numbered peaks. Such spectra are similar to dissolved organic matter (DOM), known e.g. from terrestrial and marine waters, soil extracts or aerosols. In the next step, samples were desalted and concentrated by solid phase extraction (SPE) and subsequently analyzed by flow injection analysis (FIA) in a Fourier Transform Ion Cyclotron Resonance <span class="hlt">Mass</span> Spectrometer (FTICR-MS), equipped with an ESI source and a 7 T</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Natur.541...72B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Natur.541...72B"><span>Centennial-scale Holocene climate <span class="hlt">variations</span> amplified by Antarctic <span class="hlt">Ice</span> Sheet discharge</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bakker, Pepijn; Clark, Peter U.; Golledge, Nicholas R.; Schmittner, Andreas; Weber, Michael E.</p> <p>2017-01-01</p> <p>Proxy-based indicators of past climate change show that current global climate models systematically underestimate Holocene-epoch climate variability on centennial to multi-millennial timescales, with the mismatch increasing for longer periods. Proposed explanations for the discrepancy include ocean-atmosphere coupling that is too weak in models, insufficient energy cascades from smaller to larger spatial and temporal scales, or that global climate models do not consider slow climate feedbacks related to the carbon cycle or interactions between <span class="hlt">ice</span> sheets and climate. Such interactions, however, are known to have strongly affected centennial- to orbital-scale climate variability during past glaciations, and are likely to be important in future climate change. Here we show that fluctuations in Antarctic <span class="hlt">Ice</span> Sheet discharge caused by relatively small changes in subsurface ocean temperature can amplify multi-centennial climate variability regionally and globally, suggesting that a dynamic Antarctic <span class="hlt">Ice</span> Sheet may have driven climate fluctuations during the Holocene. We analysed high-temporal-resolution records of iceberg-rafted debris derived from the Antarctic <span class="hlt">Ice</span> Sheet, and performed both high-spatial-resolution <span class="hlt">ice</span>-sheet modelling of the Antarctic <span class="hlt">Ice</span> Sheet and multi-millennial global climate model simulations. <span class="hlt">Ice</span>-sheet responses to decadal-scale ocean forcing appear to be less important, possibly indicating that the future response of the Antarctic <span class="hlt">Ice</span> Sheet will be governed more by long-term anthropogenic warming combined with multi-centennial natural variability than by annual or decadal climate oscillations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19870060021&hterms=marginal&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dmarginal','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19870060021&hterms=marginal&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dmarginal"><span>Multisensor comparison of <span class="hlt">ice</span> concentration estimates in the marginal <span class="hlt">ice</span> zone</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Burns, B. A.; Cavalieri, D. J.; Gloersen, P.; Keller, M. R.; Campbell, W. J.</p> <p>1987-01-01</p> <p>Aircraft remote sensing data collected during the 1984 summer Marginal <span class="hlt">Ice</span> Zone Experiment in the Fram Strait are used to compare <span class="hlt">ice</span> 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 <span class="hlt">ice</span> surface conditions, imaging geometry, and choice of algorithm parameters affect estimates made by each sensor.Active and passive microwave sensor estimates of <span class="hlt">ice</span> 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 <span class="hlt">variations</span> in <span class="hlt">ice</span> surface signatures in the scene.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C23C..03S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C23C..03S"><span>Surface water hydrology and 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>Smith, L. C.; Yang, K.; Pitcher, L. H.; Overstreet, B. T.; Chu, V. W.; Rennermalm, A. K.; Cooper, M. G.; Gleason, C. J.; Ryan, J.; Hubbard, A.; Tedesco, M.; Behar, A.</p> <p>2016-12-01</p> <p><span class="hlt">Mass</span> loss from the Greenland <span class="hlt">Ice</span> Sheet now exceeds 260 Gt/year, raising global sea level by >0.7 mm annually. Approximately two-thirds of this total <span class="hlt">mass</span> loss is now driven by negative <span class="hlt">ice</span> sheet surface <span class="hlt">mass</span> balance (SMB), attributed mainly to production and runoff of meltwater from the <span class="hlt">ice</span> sheet surface. This new dominance of runoff as a driver of GrIS total <span class="hlt">mass</span> loss will likely persist owing to anticipated further increases in surface melting, reduced meltwater storage in firn, and the waning importance of dynamical <span class="hlt">mass</span> losses (<span class="hlt">ice</span> calving) as the <span class="hlt">ice</span> sheets retreat from their marine-terminating margins. It also creates the need and opportunity for integrative research pairing traditional surface water hydrology approaches with glaciology. As one example, we present a way to measure supraglacial "runoff" (i.e. specific discharge) at the supraglacial catchment scale ( 101-102 km2), using in situ measurements of supraglacial river discharge and high-resolution satellite/drone mapping of upstream catchment area. This approach, which is standard in terrestrial hydrology but novel for <span class="hlt">ice</span> sheet science, enables independent verification and improvement of modeled SMB runoff estimates used to project sea level rise. Furthermore, because current SMB models do not consider the role of fluvial watershed processes operating on the <span class="hlt">ice</span> surface, inclusion of even a simple surface routing model materially improves simulations of runoff delivered to moulins, the critical pathways for meltwater entry into the <span class="hlt">ice</span> sheet. Incorporating principles of surface water hydrology and fluvial geomorphology and into glaciological models will thus aid estimates of Greenland meltwater runoff to the global ocean as well as connections to subglacial hydrology and <span class="hlt">ice</span> sheet dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3623855','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3623855"><span>Patterns of Cross-Continental <span class="hlt">Variation</span> in Tree Seed <span class="hlt">Mass</span> in the Canadian Boreal Forest</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Liu, Jushan; Bai, Yuguang; Lamb, Eric G.; Simpson, Dale; Liu, Guofang; Wei, Yongsheng; Wang, Deli; McKenney, Daniel W.; Papadopol, Pia</p> <p>2013-01-01</p> <p>Seed <span class="hlt">mass</span> is an adaptive trait affecting species distribution, population dynamics and community structure. In widely distributed species, <span class="hlt">variation</span> in seed <span class="hlt">mass</span> may reflect both genetic adaptation to local environments and adaptive phenotypic plasticity. Acknowledging the difficulty in separating these two aspects, we examined the causal relationships determining seed <span class="hlt">mass</span> <span class="hlt">variation</span> to better understand adaptability and/or plasticity of selected tree species to spatial/climatic <span class="hlt">variation</span>. A total of 504, 481 and 454 seed collections of black spruce (Picea mariana (Mill.) B.S.P.), white spruce (Picea glauca (Moench) Voss) and jack pine (Pinus banksiana Lamb) across the Canadian Boreal Forest, respectively, were selected. Correlation analyses were used to determine how seed <span class="hlt">mass</span> vary with latitude, longitude, and altitude. Structural Equation Modeling was used to examine how geographic and climatic variables influence seed <span class="hlt">mass</span>. Climatic factors explained a large portion of the <span class="hlt">variation</span> in seed <span class="hlt">mass</span> (34, 14 and 29%, for black spruce, white spruce and jack pine, respectively), indicating species-specific adaptation to long term climate conditions. Higher annual mean temperature and winter precipitation caused greater seed <span class="hlt">mass</span> in black spruce, but annual precipitation was the controlling factor for white spruce. The combination of factors such as growing season temperature and evapotranspiration, temperature seasonality and annual precipitation together determined seed <span class="hlt">mass</span> of jack pine. Overall, sites with higher winter temperatures were correlated with larger seeds. Thus, long-term climatic conditions, at least in part, determined spatial <span class="hlt">variation</span> in seed <span class="hlt">mass</span>. Black spruce and Jack pine, species with relatively more specific habitat requirements and less plasticity, had more <span class="hlt">variation</span> in seed <span class="hlt">mass</span> explained by climate than did the more plastic species white spruce. As traits such as seed <span class="hlt">mass</span> are related to seedling growth and survival, they potentially</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ApJ...839...82N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ApJ...839...82N"><span>Development of a Full <span class="hlt">Ice</span>-cream Cone Model for Halo Coronal <span class="hlt">Mass</span> Ejections</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Na, Hyeonock; Moon, Y.-J.; Lee, Harim</p> <p>2017-04-01</p> <p>It is essential to determine three-dimensional parameters (e.g., radial speed, angular width, and source location) of coronal <span class="hlt">mass</span> ejections (CMEs) for the space weather forecast. In this study, we investigate which cone type represents a halo CME morphology using 29 CMEs (12 Solar and Heliospheric Observatory (SOHO)/Large Angle and Spectrometric Coronagraph (LASCO) halo CMEs and 17 Solar Terrestrial Relations Observatory (STEREO)/Sun-Earth Connection Coronal and Heliospheric Investigation COR2 halo CMEs) from 2010 December to 2011 June. These CMEs are identified as halo CMEs by one spacecraft (SOHO or one of STEREO A and B) and limb ones by the other spacecraft (One of STEREO A and B or SOHO). From cone shape parameters of these CMEs, such as their front curvature, we find that the CME observational structures are much closer to a full <span class="hlt">ice</span>-cream cone type than a shallow <span class="hlt">ice</span>-cream cone type. Thus, we develop a full <span class="hlt">ice</span>-cream cone model based on a new methodology that the full <span class="hlt">ice</span>-cream cone consists of many flat cones with different heights and angular widths to estimate the three-dimensional parameters of the halo CMEs. This model is constructed by carrying out the following steps: (1) construct a cone for a given height and angular width, (2) project the cone onto the sky plane, (3) select points comprising the outer boundary, and (4) minimize the difference between the estimated projection speeds with the observed ones. By applying this model to 12 SOHO/LASCO halo CMEs, we find that 3D parameters from our method are similar to those from other stereoscopic methods (I.e., a triangulation method and a Graduated Cylindrical Shell model).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C21E1165W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C21E1165W"><span>A Detailed Geophysical Investigation of the Grounding of Henry <span class="hlt">Ice</span> Rise, with Implications for Holocene <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>Wearing, M.; Kingslake, J.</p> <p>2017-12-01</p> <p>It is generally assumed that since the Last Glacial Maximum the West Antarctic <span class="hlt">Ice</span> Sheet (WAIS) has experienced monotonic retreat of the grounding line (GL). However, recent studies have cast doubt on this assumption, suggesting that the retreat of the WAIS grounding line may have been followed by a significant advance during the Holocene in the Weddell and Ross Sea sectors. Constraining this evolution is important as reconstructions of past <span class="hlt">ice</span>-sheet extent are used to spin-up predictive <span class="hlt">ice</span>-sheet models and correct <span class="hlt">mass</span>-balance observations for glacial isostatic adjustment. Here we examine in detail the formation of the Henry <span class="hlt">Ice</span> Rise (HIR), which <span class="hlt">ice</span>-sheet model simulations suggest played a key role in Holocene <span class="hlt">ice-mass</span> changes in the Weddell Sea sector. Observations from a high-resolution ground-based, <span class="hlt">ice</span>-penetrating radar survey are best explained if the <span class="hlt">ice</span> rise formed when the Ronne <span class="hlt">Ice</span> Shelf grounded on a submarine high, underwent a period of <span class="hlt">ice</span>-rumple flow, before the GL migrated outwards to form the present-day <span class="hlt">ice</span> rise. We constrain the relative chronology of this evolution by comparing the alignment and intersection of isochronal internal layers, relic crevasses, surface features and investigating the dynamic processes leading to their complex structure. We also draw analogies between HIR and the neighbouring Doake <span class="hlt">Ice</span> Rumples. The date of formation is estimated using vertical velocities derived with a phase-sensitive radio-echo sounder (pRES). <span class="hlt">Ice</span>-sheet models suggest that the formation of the HIR and other <span class="hlt">ice</span> rises may have halted and reversed large-scale GL retreat. Hence the small-scale dynamics of these crucial regions could have wide-reaching consequences for future <span class="hlt">ice</span>-sheet <span class="hlt">mass</span> changes and constraining their formation and evolution further would be beneficial. One stringent test of our geophysics-based conclusions would be to drill to the bed of HIR to sample the <span class="hlt">ice</span> for isotopic analysis and the bed for radiocarbon analysis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28811530','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28811530"><span>Evidence for <span class="hlt">ice</span>-ocean albedo feedback in the Arctic Ocean shifting to a seasonal <span class="hlt">ice</span> zone.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kashiwase, Haruhiko; Ohshima, Kay I; Nihashi, Sohey; Eicken, Hajo</p> <p>2017-08-15</p> <p><span class="hlt">Ice</span>-albedo feedback due to the albedo contrast between water and <span class="hlt">ice</span> is a major factor in seasonal sea <span class="hlt">ice</span> retreat, and has received increasing attention with the Arctic Ocean shifting to a seasonal <span class="hlt">ice</span> 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 <span class="hlt">variations</span> in Arctic sea <span class="hlt">ice</span> retreat. Analyses of satellite data (1979-2014) and a simplified <span class="hlt">ice</span>-upper ocean coupled model reveal that divergent <span class="hlt">ice</span> motion in the early melt season triggers large-scale feedback which subsequently amplifies summer sea <span class="hlt">ice</span> anomalies. The magnitude of divergence controlling the feedback has doubled since 2000 due to a more mobile <span class="hlt">ice</span> cover, which can partly explain the recent drastic <span class="hlt">ice</span> reduction in the Arctic Ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=61546&keyword=high+AND+mountain+AND+ecosystems&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=61546&keyword=high+AND+mountain+AND+ecosystems&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>ION COMPOSITION ELUCIDATION (<span class="hlt">ICE</span>)</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><br><br>Ion Composition Elucidation (<span class="hlt">ICE</span>) utilizes selected ion recording with a double focusing <span class="hlt">mass</span> spectrometer to simultaneously determine exact <span class="hlt">masses</span> and relative isotopic abundances from <span class="hlt">mass</span> peak profiles. These can be determined more accurately and at higher sensitivity ...</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_18 --> <div id="page_19" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="361"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.osti.gov/sciencecinema/biblio/987230','SCIGOVIMAGE-SCICINEMA'); return false;" href="http://www.osti.gov/sciencecinema/biblio/987230"><span>The Role of Snow and <span class="hlt">Ice</span> in the Climate System</span></a></p> <p><a target="_blank" href="http://www.osti.gov/sciencecinema/">ScienceCinema</a></p> <p>Barry, Roger G.</p> <p>2017-12-09</p> <p>Global snow and <span class="hlt">ice</span> cover (the 'cryosphere') plays a major role in global climate and hydrology through a range of complex interactions and feedbacks, the best known of which is the <span class="hlt">ice</span> - albedo feedback. Snow and <span class="hlt">ice</span> cover undergo marked seasonal and long term changes in extent and thickness. The perennial elements - the major <span class="hlt">ice</span> sheets and permafrost - play a role in present-day regional and local climate and hydrology, but the large seasonal <span class="hlt">variations</span> in snow cover and sea <span class="hlt">ice</span> are of importance on continental to hemispheric scales. The characteristics of these <span class="hlt">variations</span>, especially in the Northern Hemisphere, and evidence for recent trends in snow and <span class="hlt">ice</span> extent are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C31D..06T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C31D..06T"><span>Submesoscale sea <span class="hlt">ice</span>-ocean interactions in marginal <span class="hlt">ice</span> zones</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thompson, A. F.; Manucharyan, G.</p> <p>2017-12-01</p> <p>Signatures of ocean eddies, fronts and filaments are commonly observed within the marginal <span class="hlt">ice</span> zones (MIZ) from satellite images of sea <span class="hlt">ice</span> concentration, in situ observations via <span class="hlt">ice</span>-tethered profilers or under-<span class="hlt">ice</span> gliders. Localized and intermittent sea <span class="hlt">ice</span> heating and advection by ocean eddies are currently not accounted for in climate models and may contribute to their biases and errors in sea <span class="hlt">ice</span> forecasts. Here, we explore mechanical sea <span class="hlt">ice</span> 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 <span class="hlt">ice</span> and advect it over warmer surface ocean waters where it can effectively melt. The horizontal eddy diffusivity of sea <span class="hlt">ice</span> <span class="hlt">mass</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> can potentially contribute to the seasonal evolution of MIZs. With continuing global warming and sea <span class="hlt">ice</span> thickness reduction in the Arctic Ocean, as well as the large expanse of thin sea <span class="hlt">ice</span> in the Southern Ocean, submesoscale sea <span class="hlt">ice</span>-ocean processes are expected to play a significant role in the climate system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1995EOSTr..76..265C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1995EOSTr..76..265C"><span><span class="hlt">Ice</span> sheets play important role in climate change</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clark, Peter U.; MacAyeal, Douglas R.; Andrews, John T.; Bartlein, Patrick J.</p> <p></p> <p><span class="hlt">Ice</span> sheets once were viewed as passive elements in the climate system enslaved to orbitally generated <span class="hlt">variations</span> in solar radiation. Today, modeling results and new geologic records suggest that <span class="hlt">ice</span> sheets actively participated in late-Pleistocene climate change, amplifying or driving significant variability at millennial as well as orbital timescales. Although large changes in global <span class="hlt">ice</span> volume were ultimately caused by orbital <span class="hlt">variations</span> (the Milankovitch hypothesis), once in existence, the former <span class="hlt">ice</span> sheets behaved dynamically and strongly influenced regional and perhaps even global climate by altering atmospheric and oceanic circulation and temperature.Experiments with General Circulation Models (GCMs) yielded the first inklings of <span class="hlt">ice</span> sheets' climatic significance. Manabe and Broccoli [1985], for example, found that the topographic and albedo effects of <span class="hlt">ice</span> sheets alone explain much of the Northern Hemisphere cooling identified in paleoclimatic records of the last glacial maximum (˜21 ka).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMSH51B2010N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMSH51B2010N"><span>Comparison of Asymmetric and <span class="hlt">Ice</span>-cream Cone Models for Halo Coronal <span class="hlt">Mass</span> Ejections</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Na, H.; Moon, Y.</p> <p>2011-12-01</p> <p>Halo coronal <span class="hlt">mass</span> ejections (HCMEs) are major cause of the geomagnetic storms. To minimize the projection effect by coronagraph observation, several cone models have been suggested: an <span class="hlt">ice</span>-cream cone model, an asymmetric cone model etc. These models allow us to determine the three dimensional parameters of HCMEs such as radial speed, angular width, and the angle between sky plane and central axis of the cone. In this study, we compare these parameters obtained from different models using 48 well-observed HCMEs from 2001 to 2002. And we obtain the root mean square error (RMS error) between measured projection speeds and calculated projection speeds for both cone models. As a result, we find that the radial speeds obtained from the models are well correlated with each other (R = 0.86), and the correlation coefficient of angular width is 0.6. The correlation coefficient of the angle between sky plane and central axis of the cone is 0.31, which is much smaller than expected. The reason may be due to the fact that the source locations of the asymmetric cone model are distributed near the center, while those of the <span class="hlt">ice</span>-cream cone model are located in a wide range. The average RMS error of the asymmetric cone model (85.6km/s) is slightly smaller than that of the <span class="hlt">ice</span>-cream cone model (87.8km/s).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C13C0833S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C13C0833S"><span>Using ATM laser altimetry to constrain surface <span class="hlt">mass</span> balance estimates and supraglacial hydrology 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>Studinger, M.; Medley, B.; Manizade, S.; Linkswiler, M. A.</p> <p>2016-12-01</p> <p>Repeat airborne laser altimetry measurements can provide large-scale field observations to better quantify spatial and temporal variability of surface processes contributing to seasonal elevation change and therefore surface <span class="hlt">mass</span> balance. As part of NASA's Operation <span class="hlt">Ice</span>Bridge the Airborne Topographic Mapper (ATM) laser altimeter measured the surface elevation of the Greenland <span class="hlt">Ice</span> Sheet during spring (March - May) and fall (September - October) of 2015. Comparison of the two surveys reveals a general trend of thinning for outlet glaciers and for the <span class="hlt">ice</span> sheet in a manner related to elevation and latitude. In contrast, some thickening is observed on the west (but not on the east) side of the <span class="hlt">ice</span> divide above 2200 m elevation in the southern half, below latitude 69°N.The observed magnitude and spatial patterns of the summer melt signal can be utilized as input into <span class="hlt">ice</span> sheet models and for validating reanalysis of regional climate models such as RACMO and MAR. We use seasonal anomalies in MERRA-2 climate fields (temperature, precipitation) to understand the observed spatial signal in seasonal change. Aside from surface elevation change, runoff from meltwater pooling in supraglacial lakes and meltwater channels accounts for at least half of the total <span class="hlt">mass</span> loss. The ability of the ATM laser altimeters to image glacial hydrological features in 3-D and determine the depth of supraglacial lakes could be used for process studies and for quantifying melt processes over large scales. The 1-meter footprint diameter of ATM laser on the surface, together with a high shot density, allows for the production of large-scale, high-resolution, geodetic quality DEMs (50 x 50 cm) suitable for fine-scale glacial hydrology research and as input to hydrological models quantifying runoff.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRC..123.1406T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123.1406T"><span>An Examination of the Sea <span class="hlt">Ice</span> Rheology for Seasonal <span class="hlt">Ice</span> Zones Based on <span class="hlt">Ice</span> Drift and Thickness Observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Toyota, Takenobu; Kimura, Noriaki</p> <p>2018-02-01</p> <p>The validity of the sea <span class="hlt">ice</span> rheological model formulated by Hibler (1979), which is widely used in present numerical sea <span class="hlt">ice</span> models, is examined for the Sea of Okhotsk as an example of the seasonal <span class="hlt">ice</span> zone (SIZ), based on satellite-derived sea <span class="hlt">ice</span> velocity, concentration and thickness. Our focus was the formulation of the yield curve, the shape of which can be estimated from <span class="hlt">ice</span> drift pattern based on the energy equation of deformation, while the strength of the <span class="hlt">ice</span> cover that determines its magnitude was evaluated using <span class="hlt">ice</span> concentration and thickness data. <span class="hlt">Ice</span> 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 <span class="hlt">ice</span> thickness was obtained with a spatial resolution of 100 m from a regression of the PALSAR backscatter coefficients with <span class="hlt">ice</span> thickness. To assess scale dependence, the <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> velocities reduce the deformation magnitude by half due to the large <span class="hlt">variation</span> of the deformation field in the SIZ.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1255085-reactivation-kamb-ice-stream-tributaries-triggers-century-scale-reorganization-siple-coast-ice-flow-west-antarctica','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1255085-reactivation-kamb-ice-stream-tributaries-triggers-century-scale-reorganization-siple-coast-ice-flow-west-antarctica"><span>Reactivation of Kamb <span class="hlt">Ice</span> Stream tributaries triggers century-scale reorganization of Siple Coast <span class="hlt">ice</span> flow in West Antarctica</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Bougamont, M.; Christoffersen, P.; Price, S. F.; ...</p> <p>2015-10-21</p> <p>Ongoing, centennial-scale flow variability within the Ross <span class="hlt">ice</span> streams of West Antarctica suggests that the present-day positive <span class="hlt">mass</span> balance in this region may reverse in the future. Here we use a three-dimensional <span class="hlt">ice</span> sheet model to simulate <span class="hlt">ice</span> flow in this region over 250 years. The flow responds to changing basal properties, as a subglacial till layer interacts with water transported in an active subglacial hydrological system. We show that a persistent weak bed beneath the tributaries of the dormant Kamb <span class="hlt">Ice</span> Stream is a source of internal <span class="hlt">ice</span> flow instability, which reorganizes all <span class="hlt">ice</span> streams in this region, leadingmore » to a reduced (positive) <span class="hlt">mass</span> balance within decades and a net loss of <span class="hlt">ice</span> within two centuries. This hitherto unaccounted for flow variability could raise sea level by 5 mm this century. Furthermore, better constraints on future sea level change from this region will require improved estimates of geothermal heat flux and subglacial water transport.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29016475','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29016475"><span>Relationship between Physiological Off-<span class="hlt">Ice</span> Testing, On-<span class="hlt">Ice</span> Skating, and Game Performance in Division I Women's <span class="hlt">Ice</span> Hockey Players.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Boland, Michelle; Miele, Emily M; Delude, Katie</p> <p>2017-10-07</p> <p>The purpose was to identify off-<span class="hlt">ice</span> testing variables that correlate to skating and game performance in Division I collegiate women <span class="hlt">ice</span> hockey players. Twenty female, forward and defensive players (19.95 ± 1.35 yr) were assessed for weight, height, percent fat <span class="hlt">mass</span> (%FAT), bone mineral density, predicted one repetition maximum (RM) absolute and relative (REL%) bench press (BP) and hex bar deadlift (HDL), lower body explosive power, anaerobic power, countermovement vertical jump (CMJ), maximum inspiratory pressure (MIP), and on-<span class="hlt">ice</span> repeated skate sprint (RSS) performance. The on-<span class="hlt">ice</span> RSS test included 6 timed 85.6 m sprints with participants wearing full hockey equipment; fastest time (FT), average time (AT) and fatigue index (FI) for the first length skate (FLS; 10 m) and total length skate (TLS; 85.6 m) were used for analysis. Game performance was evaluated with game statistics: goals, assists, points, plus-minus, and shots on goal (SOG). Correlation coefficients were used to determine relationships. Percent fat <span class="hlt">mass</span> was positively correlated (p < 0.05) with FLS-FI and TLS-AT; TLS-FT was negatively correlated with REL%HDL; BP-RM was negatively correlated with FLS-FT and FLS-AT; MIP positively correlated with assists, points, and SOG; FLS-AT negatively correlated with assists. Game performance in women <span class="hlt">ice</span> hockey players may be enhanced by greater MIP, repeat acceleration ability, and mode-specific training. Faster skating times were associated with lower %FAT. Skating performance in women <span class="hlt">ice</span> hockey players may be enhanced by improving body composition, anaerobic power, and both lower and upper body strength in off-<span class="hlt">ice</span> training.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24037377','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24037377"><span>Calving fluxes and basal melt rates of Antarctic <span class="hlt">ice</span> shelves.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Depoorter, M A; Bamber, J L; Griggs, J A; Lenaerts, J T M; Ligtenberg, S R M; van den Broeke, M R; Moholdt, G</p> <p>2013-10-03</p> <p>Iceberg calving has been assumed to be the dominant cause of <span class="hlt">mass</span> loss for the Antarctic <span class="hlt">ice</span> sheet, with previous estimates of the calving flux exceeding 2,000 gigatonnes per year. More recently, the importance of melting by the ocean has been demonstrated close to the grounding line and near the calving front. So far, however, no study has reliably quantified the calving flux and the basal <span class="hlt">mass</span> balance (the balance between accretion and ablation at the <span class="hlt">ice</span>-shelf base) for the whole of Antarctica. The distribution of fresh water in the Southern Ocean and its partitioning between the liquid and solid phases is therefore poorly constrained. Here we estimate the <span class="hlt">mass</span> balance components for all <span class="hlt">ice</span> shelves in Antarctica, using satellite measurements of calving flux and grounding-line flux, modelled <span class="hlt">ice</span>-shelf snow accumulation rates and a regional scaling that accounts for unsurveyed areas. We obtain a total calving flux of 1,321 ± 144 gigatonnes per year and a total basal <span class="hlt">mass</span> balance of -1,454 ± 174 gigatonnes per year. This means that about half of the <span class="hlt">ice</span>-sheet surface <span class="hlt">mass</span> gain is lost through oceanic erosion before reaching the <span class="hlt">ice</span> front, and the calving flux is about 34 per cent less than previous estimates derived from iceberg tracking. In addition, the fraction of <span class="hlt">mass</span> loss due to basal processes varies from about 10 to 90 per cent between <span class="hlt">ice</span> shelves. We find a significant positive correlation between basal <span class="hlt">mass</span> loss and surface elevation change for <span class="hlt">ice</span> shelves experiencing surface lowering and enhanced discharge. We suggest that basal <span class="hlt">mass</span> loss is a valuable metric for predicting future <span class="hlt">ice</span>-shelf vulnerability to oceanic forcing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1915674M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1915674M"><span>The future of the Devon <span class="hlt">Ice</span> cap: results from climate and <span class="hlt">ice</span> dynamics modelling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mottram, Ruth; Rodehacke, Christian; Boberg, Fredrik</p> <p>2017-04-01</p> <p>The Devon <span class="hlt">Ice</span> Cap is an example of a relatively well monitored small <span class="hlt">ice</span> cap in the Canadian Arctic. Close to Greenland, it shows a similar surface <span class="hlt">mass</span> balance signal to glaciers in western Greenland. Here we use high resolution (5km) simulations from HIRHAM5 to drive the PISM glacier model in order to model the present day and future prospects of this small Arctic <span class="hlt">ice</span> cap. Observational data from the Devon <span class="hlt">Ice</span> Cap in Arctic Canada is used to evaluate the surface <span class="hlt">mass</span> balance (SMB) data output from the HIRHAM5 model for simulations forced with the ERA-Interim climate reanalysis data and the historical emissions scenario run by the EC-Earth global climate model. The RCP8.5 scenario simulated by EC-Earth is also downscaled by HIRHAM5 and this output is used to force the PISM model to simulate the likely future evolution of the Devon <span class="hlt">Ice</span> Cap under a warming climate. We find that the Devon <span class="hlt">Ice</span> Cap is likely to continue its present day retreat, though in the future increased precipitation partly offsets the enhanced melt rates caused by climate change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16782607','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16782607"><span><span class="hlt">Ice</span>-sheet contributions to future sea-level change.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gregory, J M; Huybrechts, P</p> <p>2006-07-15</p> <p>Accurate simulation of <span class="hlt">ice</span>-sheet surface <span class="hlt">mass</span> balance requires higher spatial resolution than is afforded by typical atmosphere-ocean general circulation models (AOGCMs), owing, in particular, to the need to resolve the narrow and steep margins where the majority of precipitation and ablation occurs. We have developed a method for calculating <span class="hlt">mass</span>-balance changes by combining <span class="hlt">ice</span>-sheet average time-series from AOGCM projections for future centuries, both with information from high-resolution climate models run for short periods and with a 20km <span class="hlt">ice</span>-sheet <span class="hlt">mass</span>-balance model. Antarctica contributes negatively to sea level on account of increased accumulation, while Greenland contributes positively because ablation increases more rapidly. The uncertainty in the results is about 20% for Antarctica and 35% for Greenland. Changes in <span class="hlt">ice</span>-sheet topography and dynamics are not included, but we discuss their possible effects. For an annual- and area-average warming exceeding 4.5+/-0.9K in Greenland and 3.1+/-0.8K in the global average, the net surface <span class="hlt">mass</span> balance of the Greenland <span class="hlt">ice</span> sheet becomes negative, in which case it is likely that the <span class="hlt">ice</span> sheet would eventually be eliminated, raising global-average sea level by 7m.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C41E0713C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C41E0713C"><span>Evaluation of a 12-km Satellite-Era Reanalysis of Surface <span class="hlt">Mass</span> Balance for 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>Cullather, R. I.; Nowicki, S.; Zhao, B.; Max, S.</p> <p>2016-12-01</p> <p>The recent contribution to sea level change from the Greenland <span class="hlt">Ice</span> Sheet is thought to be strongly driven by surface processes including melt and runoff. Global reanalyses are potential means of reconstructing the historical time series of <span class="hlt">ice</span> sheet surface <span class="hlt">mass</span> balance (SMB), but lack spatial resolution needed to resolve ablation areas along the periphery of the <span class="hlt">ice</span> sheet. In this work, the Modern-Era Retrospective analysis for Research and Applications, version 2 (MERRA-2) is used to examine the spatial and temporal variability of surface melt over the Greenland <span class="hlt">Ice</span> Sheet. MERRA-2 is produced for the period 1980 to the present at a grid spacing of ½° latitude by ⅝° longitude, and includes snow hydrology processes including compaction, meltwater percolation and refreezing, runoff, and a prognostic surface albedo. The configuration of the MERRA-2 system allows for the background model - the Goddard Earth Observing System model, version 5 (GEOS-5) - to be carried in phase space through analyzed states via the computation of analysis increments, a capability referred to as "replay". Here, a MERRA-2 replay integration is conducted in which atmospheric forcing fields are interpolated and adjusted to sub- atmospheric grid-scale resolution. These adjustments include lapse-rate effects on temperature, humidity, precipitation, and other atmospheric variables that are known to have a strong elevation dependency over <span class="hlt">ice</span> sheets. The surface coupling is performed such that <span class="hlt">mass</span> and energy are conserved. The atmospheric forcing influences the surface representation, which operates on land surface tiles with an approximate 12-km spacing. This produces a high-resolution, downscaled SMB which is interactively coupled to the reanalysis model. We compare the downscaled SMB product with other reanalyses, regional climate model values, and a second MERRA-2 replay in which the background model has been replaced with a 12-km, non-hydrostatic version of GEOS-5. The assessment</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AcAau.146...15S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AcAau.146...15S"><span>Effect of <span class="hlt">mass</span> <span class="hlt">variation</span> on dynamics of tethered system in orbital maneuvering</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sun, Liang; Zhao, Guowei; Huang, Hai</p> <p>2018-05-01</p> <p>In orbital maneuvering, the <span class="hlt">mass</span> <span class="hlt">variation</span> due to fuel consumption has an obvious impact on the dynamics of tethered system, which cannot be neglected. The contributions of the work are mainly shown in two aspects: 1) the improvement of the model; 2) the analysis of dynamics characteristics. As the <span class="hlt">mass</span> is variable, and the derivative of the <span class="hlt">mass</span> is directly considered in the traditional Lagrange equation, the expression of generalized force is complicated. To solve this problem, the coagulated derivative is adopted in the paper; besides, the attitude dynamics equations derived in this paper take into account the effect of <span class="hlt">mass</span> <span class="hlt">variation</span> and the drift of orbital trajectory at the same time. The bifurcation phenomenon, the pendular motion angular frequency, and amplitudes of tether vibration revealed in this paper can provide a reference for the parameters and controller design in practical engineering. In the article, a dumbbell model is adopted to analyze the dynamics of tethered system, in which the <span class="hlt">mass</span> <span class="hlt">variation</span> of base satellite is fully considered. Considering the practical application, the case of orbital transfer under a transversal thrust is mainly studied. Besides, compared with the analytical solutions of librational angles, the effects of <span class="hlt">mass</span> <span class="hlt">variation</span> on stability and librational characteristic are studied. Finally, in order to make an analysis of the effect on vibrational characteristic, a lumped model is introduced, which reveals a strong coupling of librational and vibrational characteristics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1993JGR....9813045B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1993JGR....9813045B"><span>Hemispheric atmospheric <span class="hlt">variations</span> and oceanographic impacts associated with katabatic surges across 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>Bromwich, David H.; Carrasco, Jorge F.; Liu, Zhong; Tzeng, Ren-Yow</p> <p>1993-07-01</p> <p>Numerical simulations and surface-based observations show that katabatic winds persistently converge toward and blow across the Siple Coast part of West Antarctica onto the Ross <span class="hlt">Ice</span> Shelf. About 14% of the time during winter (April to August 1988), thermal infrared satellite images reveal the horizontal propagation of this negatively buoyant katabatic airstream for about 1000 km across the <span class="hlt">ice</span> shelf to its northwestern edge, a trajectory that nearly parallels the Transantarctic Mountains. This takes place when the pressure field supports such airflow, and is caused by synoptic scale cyclones that decay near and/or over Marie Byrd Land. The northwestward propagation of the katabatic winds is accompanied by other changes in the hemispheric long wave pattern. An upper level ridge develops over Wilkes Land, resulting in an enhancement of the split jet in the Pacific Ocean. Then, more frequent and/or intensified synoptic scale cyclones are steered toward Marie Byrd Land where they become nearly stationary to the northeast of the climatological location. The resulting isobaric configuration accelerates the katabatic winds crossing Siple Coast and supports their horizontal propagation across the Ross <span class="hlt">Ice</span> Shelf. An immediate impact of this katabatic airflow, that crosses from the <span class="hlt">ice</span> shelf to the Ross Sea, is expansion of the persistent polynya that is present just to the east of Ross Island. This polynya is a conspicuous feature on passive microwave images of Antarctic sea <span class="hlt">ice</span> and plays a central role in the salt budget of water <span class="hlt">masses</span> over the Ross Sea continental shelf. The impact of this katabatic airflow upon mesoscale cyclogenesis over the South Pacific Ocean is also discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20000074257&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=20000074257&hterms=Antarctic+icebergs&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DAntarctic%2Bicebergs"><span>Glacier and <span class="hlt">Ice</span> Shelves Studies Using Satellite SAR Interferometry</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rignot, Eric</p> <p>1999-01-01</p> <p>Satellite radar interferometry is a powerful technique to measure the surface velocity and topography of glacier <span class="hlt">ice</span>. On <span class="hlt">ice</span> shelves, a quadruple difference technique separates tidal motion from the steady creep flow deformation of <span class="hlt">ice</span>. The results provide a wealth of information about glacier grounding lines , <span class="hlt">mass</span> fluxes, stability, elastic properties of <span class="hlt">ice</span>, and tidal regime. The grounding line, which is where the glacier detaches from its bed and becomes afloat, is detected with a precision of a few tens of meters. Combining this information with satellite radar altimetry makes it possible to measure glacier discharge into the ocean and state of <span class="hlt">mass</span> balance with greater precision than ever before, and in turn provide a significant revision of past estimates of <span class="hlt">mass</span> balance of the Greenland and Antarctic <span class="hlt">Ice</span> Sheets. Analysis of creep rates on floating <span class="hlt">ice</span> permits an estimation of basal melting at the <span class="hlt">ice</span> shelf underside. The results reveal that the action of ocean water in sub-<span class="hlt">ice</span>-shelf cavities has been largely underestimated by oceanographic models and is the dominant mode of <span class="hlt">mass</span> release to the ocean from an <span class="hlt">ice</span> shelf. Precise mapping of grounding line positions also permits the detection of grounding line migration, which is a fine indicator of glacier change, independent of our knowledge of snow accumulation and <span class="hlt">ice</span> melting. This technique has been successfully used to detect the rapid retreat of Pine Island Glacier, the largest <span class="hlt">ice</span> stream in West Antarctica. Finally, tidal motion of <span class="hlt">ice</span> shelves measured interferometrically provides a modern, synoptic view of the physical processes which govern the formation of tabular icebergs in the Antarctic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.C51A0254Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.C51A0254Y"><span>Modelling the Climate - Greenland <span class="hlt">Ice</span> Sheet Interaction in the Coupled <span class="hlt">Ice</span>-sheet/Climate Model EC-EARTH - PISM</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, S.; Madsen, M. S.; Rodehacke, C. B.; Svendsen, S. H.; Adalgeirsdottir, G.</p> <p>2014-12-01</p> <p>Recent observations show that the Greenland <span class="hlt">ice</span> sheet (GrIS) has been losing <span class="hlt">mass</span> with an increasing speed during the past decades. Predicting the GrIS changes and their climate consequences relies on the understanding of the interaction of the GrIS with the climate system on both global and local scales, and requires climate model systems with an explicit and physically consistent <span class="hlt">ice</span> sheet module. A fully coupled global climate model with a dynamical <span class="hlt">ice</span> sheet model for the GrIS has recently been developed. The model system, EC-EARTH - PISM, consists of the EC-EARTH, an atmosphere, ocean and sea <span class="hlt">ice</span> model system, and the Parallel <span class="hlt">Ice</span> Sheet Model (PISM). The coupling of PISM includes a modified surface physical parameterization in EC-EARTH adapted to the land <span class="hlt">ice</span> surface over glaciated regions in Greenland. The PISM <span class="hlt">ice</span> sheet model is forced with the surface <span class="hlt">mass</span> balance (SMB) directly computed inside the EC-EARTH atmospheric module and accounting for the precipitation, the surface evaporation, and the melting of snow and <span class="hlt">ice</span> over land <span class="hlt">ice</span>. PISM returns the simulated basal melt, <span class="hlt">ice</span> discharge and <span class="hlt">ice</span> cover (extent and thickness) as boundary conditions to EC-EARTH. This coupled system is <span class="hlt">mass</span> and energy conserving without being constrained by any anomaly correction or flux adjustment, and hence is suitable for investigation of <span class="hlt">ice</span> sheet - climate feedbacks. Three multi-century experiments for warm climate scenarios under (1) the RCP85 climate forcing, (2) an abrupt 4xCO2 and (3) an idealized 1% per year CO2 increase are performed using the coupled model system. The experiments are compared with their counterparts of the standard CMIP5 simulations (without the interactive <span class="hlt">ice</span> sheet) to evaluate the performance of the coupled system and to quantify the GrIS feedbacks. In particular, the evolution of the Greenland <span class="hlt">ice</span> sheet under the warm climate and its impacts on the climate system are investigated. Freshwater fluxes from the Greenland <span class="hlt">ice</span> sheet melt to the Arctic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018TCry...12..811N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018TCry...12..811N"><span>Modelling the climate and surface <span class="hlt">mass</span> balance of polar <span class="hlt">ice</span> sheets using RACMO2 - Part 1: Greenland (1958-2016)</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; Melchior van Wessem, J.; van Meijgaard, Erik; van As, Dirk; Lenaerts, Jan T. M.; Lhermitte, Stef; Kuipers Munneke, Peter; Smeets, C. J. P. Paul; van Ulft, Lambertus H.; van de Wal, Roderik S. W.; van den Broeke, Michiel R.</p> <p>2018-03-01</p> <p>We evaluate modelled Greenland <span class="hlt">ice</span> sheet (GrIS) near-surface climate, surface energy balance (SEB) and surface <span class="hlt">mass</span> balance (SMB) from the updated regional climate model RACMO2 (1958-2016). The new model version, referred to as RACMO2.3p2, incorporates updated glacier outlines, topography and <span class="hlt">ice</span> albedo fields. Parameters in the cloud scheme governing the conversion of cloud condensate into precipitation have been tuned to correct inland snowfall underestimation: snow properties are modified to reduce drifting snow and melt production in the <span class="hlt">ice</span> sheet percolation zone. The <span class="hlt">ice</span> albedo prescribed in the updated model is lower at the <span class="hlt">ice</span> sheet margins, increasing <span class="hlt">ice</span> melt locally. RACMO2.3p2 shows good agreement compared to in situ meteorological data and point SEB/SMB measurements, and better resolves the spatial patterns and temporal variability of SMB compared with the previous model version, notably in the north-east, south-east and along the K-transect in south-western Greenland. This new model version provides updated, high-resolution gridded fields of the GrIS present-day climate and SMB, and will be used for projections of the GrIS climate and SMB in response to a future climate scenario in a forthcoming study.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1813991B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1813991B"><span>Evolution of a Greenland <span class="hlt">Ice</span> sheet Including Shelves and Regional Sea Level <span class="hlt">Variations</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bradley, Sarah; Reerink, Thomas; van de Wal, Roderik S. W.; Helsen, Michiel; Goelzer, Heiko</p> <p>2016-04-01</p> <p>Observational evidence, including offshore moraines and marine sediment cores infer that at the Last Glacial maximum (LGM) the Greenland <span class="hlt">ice</span> sheet (GIS) grounded out across the Davis Strait into Baffin Bay, with fast flowing <span class="hlt">ice</span> streams extending out to the continental shelf break along the NW margin. These observations lead to a number of questions as to weather the GIS and Laurentide <span class="hlt">ice</span> sheet (LIS) coalesced during glacial maximums, and if so, did a significant <span class="hlt">ice</span> shelf develop across Baffin Bay and how would such a configuration impact on the relative contribution of these <span class="hlt">ice</span> sheets to eustatic sea level (ESL). Most previous paleo <span class="hlt">ice</span> sheet modelling simulations of the GIS recreated an <span class="hlt">ice</span> sheet that either did not extend out onto the continental shelf or utilised a simplified marine <span class="hlt">ice</span> parameterisation to recreate an extended GIS, and therefore did not fully include <span class="hlt">ice</span> shelf dynamics. In this study we simulate the evolution of the GIS from 220 kyr BP to present day using IMAU-<span class="hlt">ice</span>; a 3D thermodynamical <span class="hlt">ice</span> sheet model which fully accounts for grounded and floating <span class="hlt">ice</span>, calculates grounding line migration and <span class="hlt">ice</span> shelf dynamics. As there are few observational estimates of the long-term (yrs) sub marine basal melting rates (mbm) for the GIS, we developed a mbm parameterization within IMAU-<span class="hlt">ice</span> controlled primarily by changes in paleo water depth. We also investigate the influence of the LIS on the GIS evolution by including relative sea level forcing's derived from a Glacial Isostatic Adjustment model. We will present results of how changes in the mbm directly impacts on the <span class="hlt">ice</span> sheet dynamics, timing and spatial extent of the GIS at the glacial maximums, but also on the rate of retreat and spatial extent at the Last interglacial (LIG) minimum. Results indicate that with the inclusion of <span class="hlt">ice</span> shelf dynamics, a larger GIS is generated which is grounded out into Davis strait, up to a water depth of -750 m, but significantly reduces the GIS contribution to Last</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMPP43C2299B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMPP43C2299B"><span>Evolution of a Greenland <span class="hlt">Ice</span> sheet Including Shelves and Regional Sea Level <span class="hlt">Variations</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bradley, S.; Reerink, T.; Vandewal, R.; Helsen, M.</p> <p>2015-12-01</p> <p>Observational evidence, including offshore moraines and marine sediment cores infer that at the Last Glacial maximum (LGM) the Greenland <span class="hlt">ice</span> sheet (GIS) grounded out across the Davis Strait into Baffin Bay, with fast flowing <span class="hlt">ice</span> streams extending out to the continental shelf break along the NW margin. These observations lead to a number of questions as to weather the GIS and Laurentide <span class="hlt">ice</span> sheet (LIS) coalesced during glacial maximums, and if so, did a significant <span class="hlt">ice</span> shelf develop across Baffin Bay and how would such a configuration impact on the relative contribution of these <span class="hlt">ice</span> sheets to eustatic sea level (ESL). Most previous paleo <span class="hlt">ice</span> sheet modelling simulations of the GIS recreated an <span class="hlt">ice</span> sheet that either did not extend out onto the continental shelf or utilised a simplified marine <span class="hlt">ice</span> parameterisation to recreate an extended GIS, and therefore did not fully include <span class="hlt">ice</span> shelf dynamics. In this study we simulate the evolution of the GIS from 220 kyr BP to present day using IMAU-<span class="hlt">ice</span>; a 3D thermodynamical <span class="hlt">ice</span> sheet model which fully accounts for grounded and floating <span class="hlt">ice</span>, calculates grounding line migration and <span class="hlt">ice</span> shelf dynamics. There is few observational estimates of long-term (yrs) sub marine basal melting rates (mbm) for the GIS. Therefore we investigate a range of relationships to constrain the spatial and temporal parameterisation of mbm within IMAU-<span class="hlt">ice</span> related to changes in paleo water depth, driven by changes in relative sea level and ocean temperature. We will present results of how changes in the mbm directly impacts on the <span class="hlt">ice</span> sheet dynamics, timing and spatial extent of the GIS at the glacial maximums, but also on the rate of retreat and spatial extent at the Last interglacial (LIG) minimum. Initial results indicate that with the inclusion of <span class="hlt">ice</span> shelf dynamics, a larger GIS is generated which is grounded out into Davis strait, up to a water depth of -750 m, but the total contribution to LIG ESL is reduced by up to 0.6 m.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22663702-development-full-ice-cream-cone-model-halo-coronal-mass-ejections','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22663702-development-full-ice-cream-cone-model-halo-coronal-mass-ejections"><span>Development of a Full <span class="hlt">Ice</span>-cream Cone Model for Halo Coronal <span class="hlt">Mass</span> Ejections</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>Na, Hyeonock; Moon, Y.-J.; Lee, Harim, E-mail: nho0512@khu.ac.kr, E-mail: moonyj@khu.ac.kr</p> <p></p> <p>It is essential to determine three-dimensional parameters (e.g., radial speed, angular width, and source location) of coronal <span class="hlt">mass</span> ejections (CMEs) for the space weather forecast. In this study, we investigate which cone type represents a halo CME morphology using 29 CMEs (12 Solar and Heliospheric Observatory (SOHO) /Large Angle and Spectrometric Coronagraph (LASCO) halo CMEs and 17 Solar Terrestrial Relations Observatory ( STEREO )/Sun–Earth Connection Coronal and Heliospheric Investigation COR2 halo CMEs) from 2010 December to 2011 June. These CMEs are identified as halo CMEs by one spacecraft ( SOHO or one of STEREO A and B ) and limbmore » ones by the other spacecraft (One of STEREO A and B or SOHO ). From cone shape parameters of these CMEs, such as their front curvature, we find that the CME observational structures are much closer to a full <span class="hlt">ice</span>-cream cone type than a shallow <span class="hlt">ice</span>-cream cone type. Thus, we develop a full <span class="hlt">ice</span>-cream cone model based on a new methodology that the full <span class="hlt">ice</span>-cream cone consists of many flat cones with different heights and angular widths to estimate the three-dimensional parameters of the halo CMEs. This model is constructed by carrying out the following steps: (1) construct a cone for a given height and angular width, (2) project the cone onto the sky plane, (3) select points comprising the outer boundary, and (4) minimize the difference between the estimated projection speeds with the observed ones. By applying this model to 12 SOHO /LASCO halo CMEs, we find that 3D parameters from our method are similar to those from other stereoscopic methods (i.e., a triangulation method and a Graduated Cylindrical Shell model).« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_19 --> <div id="page_20" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="381"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19790056630&hterms=interplay&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dinterplay','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19790056630&hterms=interplay&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dinterplay"><span>Evolution of Martian polar landscapes - Interplay of long-term <span class="hlt">variations</span> in perennial <span class="hlt">ice</span> cover and dust storm intensity</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cutts, J. A.; Blasius, K. R.; Roberts, W. J.</p> <p>1979-01-01</p> <p>The discovery of a new type of Martian polar terrain, called undulating plain, is reported and the evolution of the plains and other areas of the Martian polar region is discussed in terms of the trapping of dust by the perennial <span class="hlt">ice</span> cover. High-resolution Viking Orbiter 2 observations of the north polar terrain reveal perennially <span class="hlt">ice</span>-covered surfaces with low relief, wavelike, regularly spaced, parallel ridges and troughs (undulating plains) occupying areas of the polar terrain previously thought to be flat, and associated with troughs of considerable local relief which exhibit at least partial annual melting. It is proposed that the wavelike topography of the undulating plains originates from long-term periodic <span class="hlt">variations</span> in cyclical dust precipitation at the margin of a growing or receding perennial polar cap in response to changes in insolation. The troughs are proposed to originate from areas of steep slope in the undulating terrain which have lost their perennial <span class="hlt">ice</span> cover and have become incapable of trapping dust. The polar landscape thus appears to record the migrations, expansions and contractions of the Martian polar cap.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/10903197','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/10903197"><span><span class="hlt">Mass</span> Balance of the Greenland <span class="hlt">Ice</span> Sheet at High Elevations.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Thomas; Akins; Csatho; Fahnestock; Gogineni; Kim; Sonntag</p> <p>2000-07-21</p> <p>Comparison of <span class="hlt">ice</span> discharge from higher elevation areas of the entire Greenland <span class="hlt">Ice</span> Sheet with total snow accumulation gives estimates of <span class="hlt">ice</span> thickening rates over the past few decades. On average, the region has been in balance, but with thickening of 21 centimeters per year in the southwest and thinning of 30 centimeters per year in the southeast. The north of the <span class="hlt">ice</span> sheet shows less variability, with average thickening of 2 centimeters per year in the northeast and thinning of about 5 centimeters per year in the northwest. These results agree well with those from repeated altimeter surveys, except in the extreme south, where we find substantially higher rates of both thickening and thinning.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19879587','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19879587"><span>Ultra-trace determination of Persistent Organic Pollutants in Arctic <span class="hlt">ice</span> using stir bar sorptive extraction and gas chromatography coupled to <span class="hlt">mass</span> spectrometry.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lacorte, S; Quintana, J; Tauler, R; Ventura, F; Tovar-Sánchez, A; Duarte, C M</p> <p>2009-12-04</p> <p>This study presents the optimization and application of an analytical method based on the use of stir bar sorptive extraction (SBSE) gas chromatography coupled to <span class="hlt">mass</span> spectrometry (GC-MS) for the ultra-trace analysis of POPs (Persistent Organic Pollutants) in Arctic <span class="hlt">ice</span>. In a first step, the <span class="hlt">mass</span>-spectrometry conditions were optimized to quantify 48 compounds (polycyclic aromatic hydrocarbons, brominated diphenyl ethers, chlorinated biphenyls, and organochlorinated pesticides) at the low pg/L level. In a second step, the performance of this analytical method was evaluated to determine POPs in Arctic cores collected during an oceanographic campaign. Using a calibration range from 1 to 1800 pg/L and by adjusting acquisition parameters, limits of detection at the 0.1-99 and 102-891 pg/L for organohalogenated compounds and polycyclic aromatic hydrocarbons, respectively, were obtained by extracting 200 mL of unfiltered <span class="hlt">ice</span> water. alpha-hexachlorocyclohexane, DDTs, chlorinated biphenyl congeners 28, 101 and 118 and brominated diphenyl ethers congeners 47 and 99 were detected in <span class="hlt">ice</span> cores at levels between 0.5 to 258 pg/L. We emphasise the advantages and disadvantages of in situ SBSE in comparison with traditional extraction techniques used to analyze POPs in <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28753208','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28753208"><span><span class="hlt">Ice</span> nucleation active bacteria in precipitation are genetically diverse and nucleate <span class="hlt">ice</span> by employing different mechanisms.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Failor, K C; Schmale, D G; Vinatzer, B A; Monteil, C L</p> <p>2017-12-01</p> <p>A growing body of circumstantial evidence suggests that <span class="hlt">ice</span> nucleation active (<span class="hlt">Ice</span> + ) bacteria contribute to the initiation of precipitation by heterologous freezing of super-cooled water in clouds. However, little is known about the concentration of <span class="hlt">Ice</span> + bacteria in precipitation, their genetic and phenotypic diversity, and their relationship to air <span class="hlt">mass</span> trajectories and precipitation chemistry. In this study, 23 precipitation events were collected over 15 months in Virginia, USA. Air <span class="hlt">mass</span> trajectories and water chemistry were determined and 33 134 isolates were screened for <span class="hlt">ice</span> nucleation activity (INA) at -8 °C. Of 1144 isolates that tested positive during initial screening, 593 had confirmed INA at -8 °C in repeated tests. Concentrations of <span class="hlt">Ice</span> + strains in precipitation were found to range from 0 to 13 219 colony forming units per liter, with a mean of 384±147. Most <span class="hlt">Ice</span> + bacteria were identified as members of known and unknown <span class="hlt">Ice</span> + species in the Pseudomonadaceae, Enterobacteriaceae and Xanthomonadaceae families, which nucleate <span class="hlt">ice</span> employing the well-characterized membrane-bound INA protein. Two <span class="hlt">Ice</span> + strains, however, were identified as Lysinibacillus, a Gram-positive genus not previously known to include <span class="hlt">Ice</span> + bacteria. INA of the Lysinibacillus strains is due to a nanometer-sized molecule that is heat resistant, lysozyme and proteinase resistant, and secreted. <span class="hlt">Ice</span> + bacteria and the INA mechanisms they employ are thus more diverse than expected. We discuss to what extent the concentration of culturable <span class="hlt">Ice</span> + bacteria in precipitation and the identification of a new heat-resistant biological INA mechanism support a role for <span class="hlt">Ice</span> + bacteria in the initiation of precipitation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C14A..01C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C14A..01C"><span>Local processes and regional patterns - Interpreting a multi-decadal altimetry record of Greenland <span class="hlt">Ice</span> Sheet changes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Csatho, B. M.; Schenk, A. F.; Babonis, G. S.; van den Broeke, M. R.; Kuipers Munneke, P.; van der Veen, C. J.; Khan, S. A.; Porter, D. F.</p> <p>2016-12-01</p> <p>This study presents a new, comprehensive reconstruction of Greenland <span class="hlt">Ice</span> Sheet elevation changes, generated using the Surface Elevation And Change detection (SERAC) approach. 35-year long elevation-change time series (1980-2015) were obtained at more than 150,000 locations from observations acquired by NASA's airborne and spaceborne laser altimeters (ATM, LVIS, ICESat), PROMICE laser altimetry data (2007-2011) and a DEM covering the <span class="hlt">ice</span> sheet margin derived from stereo aerial photographs (1970s-80s). After removing the effect of Glacial Isostatic Adjustment (GIA) and the elastic crustal response to changes in <span class="hlt">ice</span> loading, the time series were partitioned into changes due to surface processes and <span class="hlt">ice</span> dynamics and then converted into <span class="hlt">mass</span> change histories. Using gridded products, we examined <span class="hlt">ice</span> sheet elevation, and <span class="hlt">mass</span> change patterns, and compared them with other estimates at different scales from individual outlet glaciers through large drainage basins, on to the entire <span class="hlt">ice</span> sheet. Both the SERAC time series and the grids derived from these time series revealed significant spatial and temporal <span class="hlt">variations</span> of dynamic <span class="hlt">mass</span> loss and widespread intermittent thinning, indicating the complexity of <span class="hlt">ice</span> sheet response to climate forcing. To investigate the regional and local controls of <span class="hlt">ice</span> dynamics, we examined thickness change time series near outlet glacier grounding lines. Changes on most outlet glaciers were consistent with one or more episodes of dynamic thinning that propagates upstream from the glacier terminus. The spatial pattern of the onset, duration, and termination of these dynamic thinning events suggest a regional control, such as warming ocean and air temperatures. However, the intricate spatiotemporal pattern of dynamic thickness change suggests that, regardless of the forcing responsible for initial glacier acceleration and thinning, the response of individual glaciers is modulated by local conditions. We use statistical methods, such as principal</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1913308B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1913308B"><span>Longwave radiative effects of Saharan dust during the <span class="hlt">ICE-D</span> campaign</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brooke, Jennifer; Havemann, Stephan; Ryder, Claire; O'Sullivan, Debbie</p> <p>2017-04-01</p> <p>The Havemann-Taylor Fast Radiative Transfer Code (HT-FRTC) is a fast radiative transfer model based on Principal Components. Scattering has been incorporated into HT-FRTC which allows simulations of aerosol as well as clear-sky atmospheres. This work evaluates the scattering scheme in HT-FRTC and investigates dust-affected brightness temperatures using in-situ observations from <span class="hlt">Ice</span> in Clouds Experiment - Dust (<span class="hlt">ICE-D</span>) campaign. The <span class="hlt">ICE-D</span> campaign occurred during August 2015 and was based from Cape Verde. The <span class="hlt">ICE-D</span> campaign is a multidisciplinary project which achieved measurements of in-situ mineral dust properties of the dust advected from the Sahara, and on the aerosol-cloud interactions using the FAAM BAe-146 research aircraft. <span class="hlt">ICE-D</span> encountered a range of low (0.3), intermediate (0.8) and high (1.3) aerosol optical depths, AODs, and therefore provides a range of atmospheric dust loadings in the assessment of dust scattering in HT-FRTC. Spectral radiances in the thermal infrared window region (800 - 1200 cm-1) are sensitive to the presence of mineral dust; mineral dust acts to reduce the upwelling infrared radiation caused by the absorption and re-emission of radiation by the dust layer. ARIES (Airborne Research Interferometer Evaluation System) is a nadir-facing interferometer, measuring infrared radiances between 550 and 3000 cm-1. The ARIES spectral radiances are converted to brightness temperatures by inversion of the Planck function. The mineral dust size distribution is important for radiative transfer applications as it provides a measure of aerosol scattering. The longwave spectral mineral dust optical properties including the <span class="hlt">mass</span> extinction coefficients, single scattering albedos and the asymmetry parameter have been derived from the mean <span class="hlt">ICE-D</span> size distribution. HT-FRTC scattering simulations are initialised with vertical <span class="hlt">mass</span> fractions which can be derived from extinction profiles from the lidar along with the specific extinction coefficient, kext (m2</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=PIA03729&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=PIA03729&hterms=Antarctic+icebergs&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DAntarctic%2Bicebergs"><span>Amery <span class="hlt">Ice</span> Shelf's 'Loose Tooth' Gets Looser</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>2002-01-01</p> <p><p/>The Amery <span class="hlt">Ice</span> Shelf is an important dynamic system responsible for draining about 16% of the grounded East Antarctic <span class="hlt">ice</span> sheet through only 2% of its coastline. Most of the <span class="hlt">mass</span> input to the system occurs from the Lambert and several other glaciers. <span class="hlt">Mass</span> loss from the system occurs through basal melting and iceberg calving. These images from the Multi-angle Imaging SpectroRadiometer (MISR) portray the <span class="hlt">ice</span> shelf front on October 6, 2001 (top) and September 29, 2002 (bottom), and illustrate changes that took place over the year elapsed between the two views.<p/>Two longitudinal rifts, oriented roughly parallel to the direction of <span class="hlt">ice</span> flow and measuring about 25 and 15 kilometers in length, are apparent near the seaward edge of the <span class="hlt">ice</span> shelf. Between them, a transverse fracture extends eastward from the base of the western rift. This rift system is colloquially named the Amery 'loose tooth.' Over the course of the one-year interval between these two MISR images, the <span class="hlt">ice</span> front has advanced approximately 1.6 - 1.7 kilometers, and the transverse fracture and a three-way fissure at the juncture of the rifts have widened. When the transverse fracture eventually reaches the eastern rift, a large iceberg (25 kilometers x 25 kilometers) will be released.<p/>These false-color multi-angle composites combine red-band data from MISR's 60o forward, nadir, and 60o aftward viewing cameras, displayed as red, green and blue, respectively. Different colors represent angular reflectance <span class="hlt">variations</span>. Since generally smooth surfaces predominantly forward-scatter sunlight, these appear in shades of blue. Rough surfaces tend to backward-scatter sunlight, and these appear in shades of red or orange. Low clouds appear bright purple, since they exhibit both forward and backward-scattering. Using this technique, textural <span class="hlt">variations</span> among <span class="hlt">ice</span> types are revealed, and clouds can be easily distinguished from <span class="hlt">ice</span>. Illumination conditions on the two dates are nearly identical.<p/>Understanding the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20170003112&hterms=core&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dcore','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20170003112&hterms=core&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dcore"><span>Holocene Accumulation and <span class="hlt">Ice</span> Flow near the West Antarctic <span class="hlt">Ice</span> Sheet Divide <span class="hlt">Ice</span> Core Site</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Koutnik, Michelle R.; Fudge, T.J.; Conway, Howard; Waddington, Edwin D.; Neumann, Thomas A.; Cuffey, Kurt M.; Buizert, Christo; Taylor, Kendrick C.</p> <p>2016-01-01</p> <p>The West Antarctic <span class="hlt">Ice</span> Sheet Divide Core (WDC) provided a high-resolution climate record from near the Ross-Amundsen Divide in Central West Antarctica. In addition, radar-detected internal layers in the vicinity of the WDC site have been dated directly from the <span class="hlt">ice</span> core to provide spatial <span class="hlt">variations</span> in the age structure of the region. Using these two data sets together, we first infer a high-resolution Holocene accumulation-rate history from 9.2 thousand years of the <span class="hlt">ice</span>-core timescale and then confirm that this climate history is consistent with internal layers upstream of the core site. Even though the WDC was drilled only 24 kilometers from the modern <span class="hlt">ice</span> divide, advection of <span class="hlt">ice</span> from upstream must be taken into account. We evaluate histories of accumulation rate by using a flowband model to generate internal layers that we compare to observed layers. Results show that the centennially averaged accumulation rate was over 20 percent lower than modern at 9.2 thousand years before present (B.P.), increased by 40 percent from 9.2 to 2.3 thousand years B.P., and decreased by at least 10 percent over the past 2 thousand years B.P. to the modern values; these Holocene accumulation-rate changes in Central West Antarctica are larger than changes inferred from East Antarctic <span class="hlt">ice</span>-core records. Despite significant changes in accumulation rate, throughout the Holocene the regional accumulation pattern has likely remained similar to today, and the <span class="hlt">ice</span>-divide position has likely remained on average within 5 kilometers of its modern position. Continent-scale <span class="hlt">ice</span>-sheet models used for reconstructions of West Antarctic <span class="hlt">ice</span> volume should incorporate this accumulation history.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.7865I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.7865I"><span>On Land <span class="hlt">Ice</span> <span class="hlt">Mass</span> Change in Southernmost South America, Antarctic Peninsula and Coastal Antarctica consistent with GRACE, GPS and Reconstructed <span class="hlt">Ice</span> History for Past 1000 years.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ivins, Erik; Wiese, David; Watkins, Michael; Yuan, Dah-Ning; Landerer, Felix; Simms, Alex; Boening, Carmen</p> <p>2014-05-01</p> <p>The improved spatial coverage provided by high-quality Global Positioning System observing systems on exposed bedrock has allowed these space geodetic experiments to play an increasingly important role in constraining both glacial isostatic adjustment (GIA) processes and viscoelastic responses to present-day glacial <span class="hlt">mass</span> changes (PGMC). Improved constraints on models of <span class="hlt">ice</span> <span class="hlt">mass</span> change in the Southern Hemisphere at present-day, during the Little <span class="hlt">Ice</span> Age, and during the Late Holocene are invaluable for reconciling climate and sea-level variability on a global scale during the present solar radiation forcing and Milankovic orbital configuration. Studies by Jacobs et al. (1992), Whitehouse et al. (2012), King et al. (2012), Boening et al (2012), and others, support the contention that GRACE observations of both GIA and PGMC in the Southern Hemisphere are dominated by the geography and climate of coastal environments. This makes the proper masking of those environments for GRACE-determinations of secular <span class="hlt">mass</span> balance especially sensitive, and downscaling, rescaling, and use of correlation mascon methods a non-trivial part of the analysis. Here we employ two analysis methods to determine the <span class="hlt">mass</span> balances of the Antarctic Peninsula and Patagonia and incorporate GPS observations of ongoing uplift for GIA correction into both. Using data that roughly span 2002-2013, we determine -25 ± 5 Gt/yr for the uncorrected Antarctic Peninsula (AP) and -12 Gt/yr for southern Patagonia and the Cordillera Darwin (PCD). With corrections for GIA these are increased to -34 ± 8 Gt/yr for AP and -22 ± 6 Gt/yr for PCD.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.6421B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.6421B"><span>Summary of the SeaRISE Project's Experiments on Modeled <span class="hlt">Ice</span>-Sheet Contributions to Future Sea Level: Linearities and Non-linearities</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bindschadler, Robert</p> <p>2013-04-01</p> <p>The SeaRISE (Sea-level Response to <span class="hlt">Ice</span> Sheet Evolution) project achieved <span class="hlt">ice</span>-sheet model ensemble responses to a variety of prescribed changes to surface <span class="hlt">mass</span> balance, basal sliding and ocean boundary melting. Greenland <span class="hlt">ice</span> sheet models are more sensitive than Antarctic <span class="hlt">ice</span> sheet models to likely atmospheric changes in surface <span class="hlt">mass</span> balance, while Antarctic models are most sensitive to basal melting of its <span class="hlt">ice</span> shelves. An experiment approximating the IPCC's RCP8.5 scenario produces first century contributions to sea level of 22.3 and 7.3 cm from Greenland and Antarctica, respectively, with a range among models of 62 and 17 cm, respectively. By 200 years, these projections increase to 53.2 and 23.4 cm, respectively, with ranges of 79 and 57 cm. The considerable range among models was not only in the magnitude of <span class="hlt">ice</span> lost, but also in the spatial pattern of response to identical forcing. Despite this <span class="hlt">variation</span>, the response of any single model to a large range in the forcing intensity was remarkably linear in most cases. Additionally, the results of sensitivity experiments to single types of forcing (i.e., only one of the surface <span class="hlt">mass</span> balance, or basal sliding, or ocean boundary melting) could be summed to accurately predict any model's result for an experiment when multiple forcings were applied simultaneously. This suggests a limited amount of feedback through the <span class="hlt">ice</span> sheet's internal dynamics between these types of forcing over the time scale of a few centuries (SeaRISE experiments lasted 500 years).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018EPJWC.16804010P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018EPJWC.16804010P"><span>Searches for magnetic monopoles with <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>Pollmann, Anna</p> <p>2018-01-01</p> <p>Particles that carry a magnetic monopole charge are proposed by various theories which go beyond the Standard Model of particle physics. The expected <span class="hlt">mass</span> of magnetic monopoles varies depending on the theory describing its origin, generally the monopole <span class="hlt">mass</span> far exceeds those which can be created at accelerators. Magnetic monopoles gain kinetic energy in large scale galactic magnetic fields and, depending on their <span class="hlt">mass</span>, can obtain relativistic velocities. <span class="hlt">Ice</span>Cube is a high energy neutrino detector using the clear <span class="hlt">ice</span> at the South Pole as a detection medium. As monopoles pass through this <span class="hlt">ice</span> they produce optical light by a variety of mechanisms. With increasing velocity, they produce light by catalysis of baryon decay, luminescence in the <span class="hlt">ice</span> associated with electronic excitations, indirect and direct Cherenkov light from the monopole track, and Cherenkov light from cascades induced by pair creation and photonuclear reactions. By searching for this light, current best limits for the monopole flux over a broad range of velocities was achieved using the <span class="hlt">Ice</span>Cube detector. A review of these magnetic monopole searches is presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22259152','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22259152"><span>Arctic <span class="hlt">ice</span> cover, <span class="hlt">ice</span> thickness and tipping points.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wadhams, Peter</p> <p>2012-02-01</p> <p>We summarize the latest results on the rapid changes that are occurring to Arctic sea <span class="hlt">ice</span> thickness and extent, the reasons for them, and the methods being used to monitor the changing <span class="hlt">ice</span> thickness. Arctic sea <span class="hlt">ice</span> extent had been shrinking at a relatively modest rate of 3-4% per decade (annually averaged) but after 1996 this speeded up to 10% per decade and in summer 2007 there was a massive collapse of <span class="hlt">ice</span> extent to a new record minimum of only 4.1 million km(2). Thickness has been falling at a more rapid rate (43% in the 25 years from the early 1970s to late 1990s) with a specially rapid loss of <span class="hlt">mass</span> from pressure ridges. The summer 2007 event may have arisen from an interaction between the long-term retreat and more rapid thinning rates. We review thickness monitoring techniques that show the greatest promise on different spatial and temporal scales, and for different purposes. We show results from some recent work from submarines, and speculate that the trends towards retreat and thinning will inevitably lead to an eventual loss of all <span class="hlt">ice</span> in summer, which can be described as a 'tipping point' in that the former situation, of an Arctic covered with mainly multi-year <span class="hlt">ice</span>, cannot be retrieved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=Remote+AND+sensing&id=EJ1016786','ERIC'); return false;" href="https://eric.ed.gov/?q=Remote+AND+sensing&id=EJ1016786"><span>Reading the <span class="hlt">Ice</span>: Using Remote Sensing to Analyze Radar Data</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Gillette, Brandon; Leinmiller-Renick, Kelsey; Foga, Steve</p> <p>2013-01-01</p> <p>Understanding the behavior of <span class="hlt">ice</span> sheets (thick, continent-size <span class="hlt">ice</span> <span class="hlt">masses</span>) and glaciers (smaller, flowing <span class="hlt">masses</span> of <span class="hlt">ice</span>) is increasingly important as our climate changes, particularly in the Polar Regions. This article describes two lessons, based on the 5E (engage, explore, explain, elaborate, and evaluate) model, that help students practice…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20010066068','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20010066068"><span>Determining Greenland <span class="hlt">Ice</span> Sheet Accumulation Rates from Radar Remote Sensing</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.</p> <p>2001-01-01</p> <p>An important component of NASA's Program for Arctic Regional Climate Assessment (PARCA) is a <span class="hlt">mass</span> balance investigation of the Greenland <span class="hlt">Ice</span> Sheet. The <span class="hlt">mass</span> balance is calculated by taking the difference between the snow accumulation and the <span class="hlt">ice</span> discharge of the <span class="hlt">ice</span> sheet. Uncertainties in this calculation include the snow accumulation rate, which has traditionally been determined by interpolating data from <span class="hlt">ice</span> core samples taken throughout the <span class="hlt">ice</span> sheet. The sparse data associated with <span class="hlt">ice</span> cores, coupled with the high spatial and temporal resolution provided by remote sensing, have motivated scientists to investigate relationships between accumulation rate and microwave observations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70012549','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70012549"><span><span class="hlt">Ice</span> sheet topography by satellite altimetry</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Brooks, R.L.; Campbell, W.J.; Ramseier, R.O.; Stanley, H.R.; Zwally, H.J.</p> <p>1978-01-01</p> <p>The surface elevation of the southern Greenland <span class="hlt">ice</span> sheet and surface features of the <span class="hlt">ice</span> flow are obtained from the radar altimeter on the GEOS 3 satellite. The achieved accuracy in surface elevation is ???2 m. As changes in surface elevation are indicative of changes in <span class="hlt">ice</span> volume, the <span class="hlt">mass</span> balance of the present <span class="hlt">ice</span> sheets could be determined by repetitive mapping of the surface elevation and the surface could be monitored to detect surging or significant changes in <span class="hlt">ice</span> flow. ?? 1978 Nature Publishing Group.</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><span class="hlt">Mass</span> 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 zones 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> Zone Observing Network 2 Polar Airborne Measurements and Arctic Regional Climate Model</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012Icar..220.1112S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012Icar..220.1112S"><span>History and anatomy of subsurface <span class="hlt">ice</span> on Mars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schorghofer, Norbert; Forget, Francois</p> <p>2012-08-01</p> <p><span class="hlt">Ice</span> buried beneath a thin layer of soil has been revealed by neutron spectroscopy and explored by the Phoenix Mars Lander. It has also been exposed by recent impacts. This subsurface <span class="hlt">ice</span> is thought to lose and gain volume in response to orbital <span class="hlt">variations</span> (Milankovitch cycles). We use a powerful numerical model to follow the growth and retreat of near-surface <span class="hlt">ice</span> as a result of regolith-atmosphere exchange continuously over millions of years. If a thick layer of almost pure <span class="hlt">ice</span> has been deposited recently, it has not yet reached equilibrium with the atmospheric water vapor and may still remain as far equatorward as 43°N, where <span class="hlt">ice</span> has been revealed by recent impacts. A potentially observable consequence is present-day humidity output from the still retreating <span class="hlt">ice</span>. We also demonstrate that in a sublimation environment, subsurface pore <span class="hlt">ice</span> can accumulate in two ways. The first mode, widely known, is the progressive filling of pores by <span class="hlt">ice</span> over a range of depths. The second mode occurs on top of an already impermeable <span class="hlt">ice</span> layer; subsequent <span class="hlt">ice</span> accumulates in the form of pasted on horizontal layers such that beneath the <span class="hlt">ice</span> table, the pores are completely full with <span class="hlt">ice</span>. Most or all of the pore <span class="hlt">ice</span> on Mars today may be of the second type. At the Phoenix landing site, where such a layer is also expected to exist above an underlying <span class="hlt">ice</span> sheet, it may be extremely thin, due to exceptionally small <span class="hlt">variations</span> in <span class="hlt">ice</span> stability over time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930049208&hterms=earth+day&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dearth%2Bday','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930049208&hterms=earth+day&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dearth%2Bday"><span>Present-day secular <span class="hlt">variations</span> in the zonal harmonics of earth's geopotential</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mitrovica, J. X.; Peltier, W. R.</p> <p>1993-01-01</p> <p>The mathematical formulation required for predicting secular <span class="hlt">variation</span> in the geopotential is developed for the case of a spherically symmetric, self-gravitating, viscoelastic earth model and an arbitrary surface load which can include a gravitational self-consistent ocean loading component. The theory is specifically applied to predict the present-day secular <span class="hlt">variation</span> in the zonal harmonics of the geopotenial arising from the surface <span class="hlt">mass</span> loading associated with the late Pleistocene glacial cycles. A procedure is outlined in which predictions of the present-day geopotential signal due to the late Pleistocene glacial cycles may be used to derive bounds on the net present-day <span class="hlt">mass</span> flux from the Antarctic and Greenland <span class="hlt">ice</span> sheets to the local oceans.</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 <span class="hlt">mass</span> 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 <span class="hlt">variations</span> 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 zone 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://adsabs.harvard.edu/abs/2016EGUGA..18..575B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18..575B"><span>Investigating <span class="hlt">ice</span> cliff evolution and contribution to glacier <span class="hlt">mass</span>-balance using a physically-based dynamic model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Buri, Pascal; Miles, Evan; Ragettli, Silvan; Brun, Fanny; Steiner, Jakob; Pellicciotti, Francesca</p> <p>2016-04-01</p> <p>Supraglacial cliffs are a surface feature typical of debris-covered glaciers, affecting surface evolution, glacier downwasting and <span class="hlt">mass</span> balance by providing a direct <span class="hlt">ice</span>-atmosphere interface. As a result, melt rates can be very high and <span class="hlt">ice</span> cliffs may account for a significant portion of the total glacier <span class="hlt">mass</span> loss. However, their contribution to glacier <span class="hlt">mass</span> balance has rarely been quantified through physically-based models. Most cliff energy balance models are point scale models which calculate energy fluxes at individual cliff locations. Results from the only grid based model to date accurately reflect energy fluxes and cliff melt, but modelled backwasting patterns are in some cases unrealistic, as the distribution of melt rates would lead to progressive shallowing and disappearance of cliffs. Based on a unique multitemporal dataset of cliff topography and backwasting obtained from high-resolution terrestrial and aerial Structure-from-Motion analysis on Lirung Glacier in Nepal, it is apparent that cliffs exhibit a range of behaviours but most do not rapidly disappear. The patterns of evolution cannot be explained satisfactorily by atmospheric melt alone, and are moderated by the presence of supraglacial ponds at the base of cliffs and by cliff reburial with debris. Here, we document the distinct patterns of evolution including disappearance, growth and stability. We then use these observations to improve the grid-based energy balance model, implementing periodic updates of the cliff geometry resulting from modelled melt perpendicular to the <span class="hlt">ice</span> surface. Based on a slope threshold, pixels can be reburied by debris or become debris-free. The effect of ponds are taken into account through enhanced melt rates in horizontal direction on pixels selected based on an algorithm considering distance to the water surface, slope and lake level. We use the dynamic model to first study the evolution of selected cliffs for which accurate, high resolution DEMs are available</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_20 --> <div id="page_21" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="401"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19970040868&hterms=feather&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dfeather','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19970040868&hterms=feather&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dfeather"><span>Implementation of Combined Feather and Surface-Normal <span class="hlt">Ice</span> Growth Models in LEWICE/X</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Velazquez, M. T.; Hansman, R. J., Jr.</p> <p>1995-01-01</p> <p>Experimental observations have shown that discrete rime <span class="hlt">ice</span> growths called feathers, which grow in approximately the direction of water droplet impingement, play an important role in the growth of <span class="hlt">ice</span> on accreting surfaces for some thermodynamic conditions. An improved physical model of <span class="hlt">ice</span> accretion has been implemented in the LEWICE 2D panel-based <span class="hlt">ice</span> accretion code maintained by the NASA Lewis Research Center. The LEWICE/X model of <span class="hlt">ice</span> accretion explicitly simulates regions of feather growth within the framework of the LEWICE model. Water droplets impinging on an accreting surface are withheld from the normal LEWICE <span class="hlt">mass</span>/energy balance and handled in a separate routine; <span class="hlt">ice</span> growth resulting from these droplets is performed with enhanced convective heat transfer approximately along droplet impingement directions. An independent underlying <span class="hlt">ice</span> shape is grown along surface normals using the unmodified LEWICE method. The resulting dual-surface <span class="hlt">ice</span> shape models roughness-induced feather growth observed in <span class="hlt">icing</span> wind tunnel tests. Experiments indicate that the exact direction of feather growth is dependent on external conditions. Data is presented to support a linear <span class="hlt">variation</span> of growth direction with temperature and cloud water content. Test runs of LEWICE/X indicate that the sizes of surface regions containing feathers are influenced by initial roughness element height. This suggests that a previous argument that feather region size is determined by boundary layer transition may be incorrect. Simulation results for two typical test cases give improved shape agreement over unmodified LEWICE.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012ApJ...756L..24G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012ApJ...756L..24G"><span>In-situ Probing of Radiation-induced Processing of Organics in Astrophysical <span class="hlt">Ice</span> Analogs—Novel Laser Desorption Laser Ionization Time-of-flight <span class="hlt">Mass</span> Spectroscopic Studies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gudipati, Murthy S.; Yang, Rui</p> <p>2012-09-01</p> <p>Understanding the evolution of organic molecules in <span class="hlt">ice</span> grains in the interstellar medium (ISM) under cosmic rays, stellar radiation, and local electrons and ions is critical to our understanding of the connection between ISM and solar systems. Our study is aimed at reaching this goal of looking directly into radiation-induced processing in these <span class="hlt">ice</span> grains. We developed a two-color laser-desorption laser-ionization time-of-flight <span class="hlt">mass</span> spectroscopic method (2C-MALDI-TOF), similar to matrix-assisted laser desorption and ionization time-of-flight (MALDI-TOF) <span class="hlt">mass</span> spectroscopy. Results presented here with polycyclic aromatic hydrocarbon (PAH) probe molecules embedded in water-<span class="hlt">ice</span> at 5 K show for the first time that hydrogenation and oxygenation are the primary chemical reactions that occur in astrophysical <span class="hlt">ice</span> analogs when subjected to Lyα radiation. We found that hydrogenation can occur over several unsaturated bonds and the product distribution corresponds to their stabilities. Multiple hydrogenation efficiency is found to be higher at higher temperatures (100 K) compared to 5 K—close to the interstellar <span class="hlt">ice</span> temperatures. Hydroxylation is shown to have similar efficiencies at 5 K or 100 K, indicating that addition of O atoms or OH radicals to pre-ionized PAHs is a barrierless process. These studies—the first glimpses into interstellar <span class="hlt">ice</span> chemistry through analog studies—show that once accreted onto <span class="hlt">ice</span> grains PAHs lose their PAH spectroscopic signatures through radiation chemistry, which could be one of the reason for the lack of PAH detection in interstellar <span class="hlt">ice</span> grains, particularly the outer regions of cold, dense clouds or the upper molecular layers of protoplanetary disks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.P34A..05S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.P34A..05S"><span>Breaking <span class="hlt">Ice</span>: Fracture Processes in Floating <span class="hlt">Ice</span> on Earth and Elsewhere</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Scambos, T. A.</p> <p>2016-12-01</p> <p>Rapid, intense fracturing events in the <span class="hlt">ice</span> shelves of the Antarctic Peninsula reveal a set of processes that were not fully appreciated prior to the series of <span class="hlt">ice</span> shelf break-ups observed in the late 1990s and early 2000s. A series of studies have uncovered a fascinating array of relationships between climate, ocean, and <span class="hlt">ice</span>: intense widespread hydrofracture; repetitive hydrofracture induced by <span class="hlt">ice</span> plate bending; the ability for sub-surface flooded firn to support hydrofracture; potential triggering by long-period wave action; accelerated fracturing by trapped tsunamic waves; iceberg disintegration, and a remarkable <span class="hlt">ice</span> rebound process from lake drainage that resembles runaway nuclear fission. The events and subsequent studies have shown that rapid regional warming in <span class="hlt">ice</span> shelf areas leads to catastrophic changes in a previously stable <span class="hlt">ice</span> <span class="hlt">mass</span>. More typical fracturing of thick <span class="hlt">ice</span> plates is a natural consequence of <span class="hlt">ice</span> flow in a complex geographic setting, i.e., it is induced by shear and divergence of spreading plate flow around obstacles. While these are not a result of climate or ocean change, weather and ocean processes may impact the exact timing of final separation of an iceberg from a shelf. Taking these terrestrial perspectives to other <span class="hlt">ice</span>-covered ocean worlds, cautiously, provides an observational framework for interpreting features on Europa and Enceladus.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150008371','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150008371"><span>Effects of Extreme Obliquity <span class="hlt">Variations</span> on the Habitability of Exoplanets</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Armstrong, J. C.; Barnes, R.; Domagal-Goldman, S.; Breiner, J.; Quinn, T. R.; Meadows, V. S.</p> <p>2014-01-01</p> <p>We explore the impact of obliquity <span class="hlt">variations</span> on planetary habitability in hypothetical systems with high mutual inclination. We show that large-amplitude, high-frequency obliquity oscillations on Earth-like exoplanets can suppress the <span class="hlt">ice</span>-albedo feedback, increasing the outer edge of the habitable zone. We restricted our exploration to hypothetical systems consisting of a solar-<span class="hlt">mass</span> star, an Earth-<span class="hlt">mass</span> planet at 1 AU, and 1 or 2 larger planets. We verified that these systems are stable for 108 years with N-body simulations and calculated the obliquity <span class="hlt">variations</span> induced by the orbital evolution of the Earth-<span class="hlt">mass</span> planet and a torque from the host star. We ran a simplified energy balance model on the terrestrial planet to assess surface temperature and <span class="hlt">ice</span> coverage on the planet's surface, and we calculated differences in the outer edge of the habitable zone for planets with rapid obliquity <span class="hlt">variations</span>. For each hypothetical system, we calculated the outer edge of habitability for two conditions: (1) the full evolution of the planetary spin and orbit and (2) the eccentricity and obliquity fixed at their average values. We recovered previous results that higher values of fixed obliquity and eccentricity expand the habitable zone, but we also found that obliquity oscillations further expand habitable orbits in all cases. Terrestrial planets near the outer edge of the habitable zone may be more likely to support life in systems that induce rapid obliquity oscillations as opposed to fixed-spin planets. Such planets may be the easiest to directly characterize with space-borne telescopes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24611714','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24611714"><span>Effects of extreme obliquity <span class="hlt">variations</span> on the habitability of exoplanets.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Armstrong, J C; Barnes, R; Domagal-Goldman, S; Breiner, J; Quinn, T R; Meadows, V S</p> <p>2014-04-01</p> <p>We explore the impact of obliquity <span class="hlt">variations</span> on planetary habitability in hypothetical systems with high mutual inclination. We show that large-amplitude, high-frequency obliquity oscillations on Earth-like exoplanets can suppress the <span class="hlt">ice</span>-albedo feedback, increasing the outer edge of the habitable zone. We restricted our exploration to hypothetical systems consisting of a solar-<span class="hlt">mass</span> star, an Earth-<span class="hlt">mass</span> planet at 1 AU, and 1 or 2 larger planets. We verified that these systems are stable for 10(8) years with N-body simulations and calculated the obliquity <span class="hlt">variations</span> induced by the orbital evolution of the Earth-<span class="hlt">mass</span> planet and a torque from the host star. We ran a simplified energy balance model on the terrestrial planet to assess surface temperature and <span class="hlt">ice</span> coverage on the planet's surface, and we calculated differences in the outer edge of the habitable zone for planets with rapid obliquity <span class="hlt">variations</span>. For each hypothetical system, we calculated the outer edge of habitability for two conditions: (1) the full evolution of the planetary spin and orbit and (2) the eccentricity and obliquity fixed at their average values. We recovered previous results that higher values of fixed obliquity and eccentricity expand the habitable zone, but we also found that obliquity oscillations further expand habitable orbits in all cases. Terrestrial planets near the outer edge of the habitable zone may be more likely to support life in systems that induce rapid obliquity oscillations as opposed to fixed-spin planets. Such planets may be the easiest to directly characterize with space-borne telescopes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.7677A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.7677A"><span>Melting beneath Greenland outlet glaciers and <span class="hlt">ice</span> streams</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alexander, David; Perrette, Mahé; Beckmann, Johanna</p> <p>2015-04-01</p> <p>Basal melting of fast-flowing Greenland outlet glaciers and <span class="hlt">ice</span> streams due to frictional heating at the <span class="hlt">ice</span>-bed interface contributes significantly to total glacier <span class="hlt">mass</span> balance and subglacial meltwater flux, yet modelling this basal melt process in Greenland has received minimal research attention. A one-dimensional dynamic <span class="hlt">ice</span>-flow model is calibrated to the present day longitudinal profiles of 10 major Greenland outlet glaciers and <span class="hlt">ice</span> streams (including the Jakobshavn Isbrae, Petermann Glacier and Helheim Glacier) and is validated against published <span class="hlt">ice</span> flow and surface elevation measurements. Along each longitudinal profile, basal melt is calculated as a function of <span class="hlt">ice</span> flow velocity and basal shear stress. The basal shear stress is dependent on the effective pressure (difference between <span class="hlt">ice</span> overburden pressure and water pressure), basal roughness and a sliding parametrization. Model output indicates that where outlet glaciers and <span class="hlt">ice</span> streams terminate into the ocean with either a small floating <span class="hlt">ice</span> tongue or no floating tongue whatsoever, the proportion of basal melt to total melt (surface, basal and submarine melt) is 5-10% (e.g. Jakobshavn Isbrae; Daugaard-Jensen Glacier). This proportion is, however, negligible where larger <span class="hlt">ice</span> tongues lose <span class="hlt">mass</span> mostly by submarine melt (~1%; e.g. Nioghalvfjerdsfjorden Glacier). Modelled basal melt is highest immediately upvalley of the grounding line, with contributions typically up to 20-40% of the total melt for slippery beds and up to 30-70% for resistant beds. Additionally, modelled grounding line and calving front migration inland for all outlet glaciers and <span class="hlt">ice</span> streams of hundreds of metres to several kilometres occurs. Including basal melt due to frictional heating in outlet glacier and <span class="hlt">ice</span> stream models is important for more accurately modelling <span class="hlt">mass</span> balance and subglacial meltwater flux, and therefore, more accurately modelling outlet glacier and <span class="hlt">ice</span> stream dynamics and responses to future climate change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20070016601&hterms=time+zone&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dtime%2Bzone','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20070016601&hterms=time+zone&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dtime%2Bzone"><span><span class="hlt">Variations</span> in the Sea <span class="hlt">Ice</span> Edge and the Marginal <span class="hlt">Ice</span> Zone on Different Spatial Scales as Observed from Different Satellite Sensor</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Markus, Thorsten; Henrichs, John</p> <p>2006-01-01</p> <p>The Marginal sea <span class="hlt">Ice</span> Zone (MIZ) and the sea <span class="hlt">ice</span> edge are the most dynamic areas of the sea <span class="hlt">ice</span> cover. Knowledge of the sea <span class="hlt">ice</span> edge location is vital for routing shipping in the polar regions. The <span class="hlt">ice</span> 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 <span class="hlt">ice</span> edge because of induced atmospheric baroclinicity, and the <span class="hlt">ice</span> edge is also the location of both vertical and horizontal ocean currents driven by thermal and salinity gradients. Finally, sea <span class="hlt">ice</span> is both a driver and indicator of climate change and monitoring the position of the <span class="hlt">ice</span> 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 <span class="hlt">ice</span> edge. These sensors, though, have different spatial resolutions, different limitations, and different repeat frequencies. Satellite passive microwave sensors can monitor the <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> on the basis of surface</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C21B0683C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C21B0683C"><span>Patterns of variability in steady- and non steady-state Ross <span class="hlt">Ice</span> Shelf flow</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Campbell, A. J.; Hulbe, C. L.; Scambos, T. A.; Klinger, M. J.; Lee, C. K.</p> <p>2016-12-01</p> <p><span class="hlt">Ice</span> shelves are gateways through which climate change can be transmitted from the ocean or atmosphere to a grounded <span class="hlt">ice</span> sheet. It is thus important to separate patterns of <span class="hlt">ice</span> shelf change driven internally (from the <span class="hlt">ice</span> sheet) and patterns driven externally (by the ocean or atmosphere) so that modern observations can be viewed in an appropriate context. Here, we focus on the Ross <span class="hlt">Ice</span> Shelf (RIS), a major component of the West Antarctic <span class="hlt">Ice</span> Sheet system and a feature known to experience variable <span class="hlt">ice</span> flux from tributary <span class="hlt">ice</span> streams and glaciers, for example, <span class="hlt">ice</span> stream stagnation and glacier surges. We perturb a model of the Ross <span class="hlt">Ice</span> Shelf with periodic influx <span class="hlt">variations</span>, <span class="hlt">ice</span> rise and <span class="hlt">ice</span> plain grounding events, and iceberg calving in order to generate transients in the <span class="hlt">ice</span> shelf flow and thickness. Characteristic patterns associated with those perturbations are identified using empirical orthogonal functions (EOFs). The leading EOFs reveal shelf-wide pattern of response to local perturbations that can be interpreted in terms of coupled <span class="hlt">mass</span> and momentum balance. For example, speed changes on Byrd Glacier cause both thinning and thickening in a broad region that extends to Roosevelt Island. We calculate decay times at various locations for various perturbations and find that mutli-decadal to century time scales are typical. Unique identification of responses to particular forcings may thus be difficlult to achieve and flow divergence cannot be assumed to be constant when interpreting observed changes in <span class="hlt">ice</span> thickness. In reality, perturbations to the <span class="hlt">ice</span> shelf do not occur individually, rather the <span class="hlt">ice</span> shelf contains a history of boundary perturbations. To explore the degree individual perturbations are seperable from their ensemble, EOFs from individual events are combined in pairs and compared against experiments with the same periodic perturbations pairs. Residuals between these EOFs reveal the degree interaction between between disctinct perturbations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/7061','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/7061"><span>Columbia Glacier stake location, <span class="hlt">mass</span> balance, glacier surface altitude, and <span class="hlt">ice</span> radar data, 1978 measurement year</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Mayo, L.R.; Trabant, D.C.; March, Rod; Haeberli, Wilfried</p> <p>1979-01-01</p> <p>A 1 year data-collection program on Columbia Glacier, Alaska has produced a data set consisting of near-surface <span class="hlt">ice</span> kinematics, <span class="hlt">mass</span> balance, and altitude change at 57 points and 34 <span class="hlt">ice</span> radar soundings. These data presented in two tables, are part of the basic data required for glacier dynamic analysis, computer models, and predictions of the number and size of icebergs which Columbia Glacier will calve into shipping lanes of eastern Prince William Sound. A metric, sea-level coordinate system was developed for use in surveying throughout the basin. Its use is explained and monument coordinates listed. A series of seven integrated programs for calculators were used in both the field and office to reduce the surveying data. These programs are thoroughly documented and explained in the report. (Kosco-USGS)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930063818&hterms=balance+sheet&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dbalance%2Bsheet','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930063818&hterms=balance+sheet&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dbalance%2Bsheet"><span>A combined surface/volume scattering retracking algorithm for <span class="hlt">ice</span> sheet satellite altimetry</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Davis, Curt H.</p> <p>1992-01-01</p> <p>An algorithm that is based upon a combined surface-volume scattering model is developed. It can be used to retrack individual altimeter waveforms over <span class="hlt">ice</span> sheets. An iterative least-squares procedure is used to fit the combined model to the return waveforms. The retracking algorithm comprises two distinct sections. The first generates initial model parameter estimates from a filtered altimeter waveform. The second uses the initial estimates, the theoretical model, and the waveform data to generate corrected parameter estimates. This retracking algorithm can be used to assess the accuracy of elevations produced from current retracking algorithms when subsurface volume scattering is present. This is extremely important so that repeated altimeter elevation measurements can be used to accurately detect changes in the <span class="hlt">mass</span> balance of the <span class="hlt">ice</span> sheets. By analyzing the distribution of the model parameters over large portions of the <span class="hlt">ice</span> sheet, regional and seasonal <span class="hlt">variations</span> in the near-surface properties of the snowpack can be quantified.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1990JGR....9513411C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1990JGR....9513411C"><span>Arctic multiyear <span class="hlt">ice</span> classification and summer <span class="hlt">ice</span> cover using passive microwave satellite data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Comiso, J. C.</p> <p>1990-08-01</p> <p>The ability to classify and monitor Arctic multiyear sea <span class="hlt">ice</span> cover using multispectral passive microwave data is studied. Sea <span class="hlt">ice</span> concentration maps during several summer minima have been analyzed to obtain estimates of <span class="hlt">ice</span> surviving the summer. The results are compared with multiyear <span class="hlt">ice</span> concentrations derived from data the following winter, using an algorithm that assumes a certain emissivity for multiyear <span class="hlt">ice</span>. The multiyear <span class="hlt">ice</span> cover inferred from the winter data is approximately 25 to 40% less than the summer <span class="hlt">ice</span> cover minimum, suggesting that even during winter when the emissivity of sea <span class="hlt">ice</span> is most stable, passive microwave data may account for only a fraction of the total multiyear <span class="hlt">ice</span> cover. The difference of about 2×106 km2 is considerably more than estimates of advection through Fram Strait during the intervening period. It appears that as in the Antarctic, some multiyear <span class="hlt">ice</span> floes in the Arctic, especially those near the summer marginal <span class="hlt">ice</span> zone, have first-year <span class="hlt">ice</span> or intermediate signatures in the subsequent winter. A likely mechanism for this is the intrusion of seawater into the snow-<span class="hlt">ice</span> interface, which often occurs near the marginal <span class="hlt">ice</span> zone or in areas where snow load is heavy. Spatial <span class="hlt">variations</span> in melt and melt ponding effects also contribute to the complexity of the microwave emissivity of multiyear <span class="hlt">ice</span>. Hence the multiyear <span class="hlt">ice</span> data should be studied in conjunction with the previous summer <span class="hlt">ice</span> data to obtain a more complete characterization of the state of the Arctic <span class="hlt">ice</span> cover. The total extent and actual areas of the summertime Arctic pack <span class="hlt">ice</span> were estimated to be 8.4×106 km2 and 6.2×106 km2, respectively, and exhibit small interannual variability during the years 1979 through 1985, suggesting a relatively stable <span class="hlt">ice</span> cover.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C43B0750J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C43B0750J"><span>Landfast Sea <span class="hlt">Ice</span> Breakouts: Stabilizing <span class="hlt">Ice</span> Features, Oceanic and Atmospheric Forcing at Barrow, Alaska</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jones, J.; Eicken, H.; Mahoney, A. R.; MV, R.; Kambhamettu, C.; Fukamachi, Y.; Ohshima, K. I.; George, C.</p> <p>2016-12-01</p> <p>Landfast sea <span class="hlt">ice</span> is an important seasonal feature along most Arctic coastlines, such as that of the Chukchi Sea near Barrow, Alaska. Its stability throughout the <span class="hlt">ice</span> season is determined by many factors but grounded pressure ridges are the primary stabilizing component. Landfast <span class="hlt">ice</span> breakouts occur when these grounded ridges fail or unground, and previously stationary <span class="hlt">ice</span> detaches from the coast and drifts away. Using ground-based radar imagery from a coastal <span class="hlt">ice</span> and ocean observatory at Barrow, we have developed a method to estimate the extent of grounded ridges by tracking <span class="hlt">ice</span> motion and deformation over the course of winter and have derived <span class="hlt">ice</span> keel depth and potential for grounding from cumulative convergent <span class="hlt">ice</span> motion. Estimates of landfast <span class="hlt">ice</span> grounding strength have been compared to the atmospheric and oceanic stresses acting on the landfast <span class="hlt">ice</span> before and during breakout events to determine prevailing causes for the failure of stabilizing features. Applying this approach to two case studies in 2008 and 2010, we conclude that a combination of atmospheric and oceanic stresses may have caused the breakouts analyzed in this study, with the latter as the dominant force. Preconditioning (as weakening) of grounded ridges by sea level <span class="hlt">variations</span> may facilitate failure of the <span class="hlt">ice</span> sheet leading to breakout events.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016CSR...126...50J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016CSR...126...50J"><span>Landfast sea <span class="hlt">ice</span> breakouts: Stabilizing <span class="hlt">ice</span> features, oceanic and atmospheric forcing at Barrow, Alaska</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jones, Joshua; Eicken, Hajo; Mahoney, Andrew; MV, Rohith; Kambhamettu, Chandra; Fukamachi, Yasushi; Ohshima, Kay I.; George, J. Craig</p> <p>2016-09-01</p> <p>Landfast sea <span class="hlt">ice</span> is an important seasonal feature along most Arctic coastlines, such as that of the Chukchi Sea near Barrow, Alaska. Its stability throughout the <span class="hlt">ice</span> season is determined by many factors but grounded pressure ridges are the primary stabilizing component. Landfast <span class="hlt">ice</span> breakouts occur when these grounded ridges fail or unground, and previously stationary <span class="hlt">ice</span> detaches from the coast and drifts away. Using ground-based radar imagery from a coastal <span class="hlt">ice</span> and ocean observatory at Barrow, we have developed a method to estimate the extent of grounded ridges by tracking <span class="hlt">ice</span> motion and deformation over the course of winter and have derived <span class="hlt">ice</span> keel depth and potential for grounding from cumulative convergent <span class="hlt">ice</span> motion. Estimates of landfast <span class="hlt">ice</span> grounding strength have been compared to the atmospheric and oceanic stresses acting on the landfast <span class="hlt">ice</span> before and during breakout events to determine prevailing causes for the failure of stabilizing features. Applying this approach to two case studies in 2008 and 2010, we conclude that a combination of atmospheric and oceanic stresses may have caused the breakouts analyzed in this study, with the latter as the dominant force. Preconditioning (as weakening) of grounded ridges by sea level <span class="hlt">variations</span> may facilitate failure of the <span class="hlt">ice</span> sheet leading to breakout events.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19884496','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19884496"><span>The future of <span class="hlt">ice</span> sheets and sea <span class="hlt">ice</span>: between reversible retreat and unstoppable loss.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Notz, Dirk</p> <p>2009-12-08</p> <p>We discuss the existence of cryospheric "tipping points" in the Earth's climate system. Such critical thresholds have been suggested to exist for the disappearance of Arctic sea <span class="hlt">ice</span> and the retreat of <span class="hlt">ice</span> sheets: Once these <span class="hlt">ice</span> <span class="hlt">masses</span> have shrunk below an anticipated critical extent, the <span class="hlt">ice</span>-albedo feedback might lead to the irreversible and unstoppable loss of the remaining <span class="hlt">ice</span>. We here give an overview of our current understanding of such threshold behavior. By using conceptual arguments, we review the recent findings that such a tipping point probably does not exist for the loss of Arctic summer sea <span class="hlt">ice</span>. Hence, in a cooler climate, sea <span class="hlt">ice</span> could recover rapidly from the loss it has experienced in recent years. In addition, we discuss why this recent rapid retreat of Arctic summer sea <span class="hlt">ice</span> might largely be a consequence of a slow shift in <span class="hlt">ice</span>-thickness distribution, which will lead to strongly increased year-to-year variability of the Arctic summer sea-<span class="hlt">ice</span> extent. This variability will render seasonal forecasts of the Arctic summer sea-<span class="hlt">ice</span> extent increasingly difficult. We also discuss why, in contrast to Arctic summer sea <span class="hlt">ice</span>, a tipping point is more likely to exist for the loss of the Greenland <span class="hlt">ice</span> sheet and the West Antarctic <span class="hlt">ice</span> sheet.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45.4086A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45.4086A"><span>Variable Basal Melt Rates of Antarctic Peninsula <span class="hlt">Ice</span> Shelves, 1994-2016</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Adusumilli, Susheel; Fricker, Helen Amanda; Siegfried, Matthew R.; Padman, Laurie; Paolo, Fernando S.; Ligtenberg, Stefan R. M.</p> <p>2018-05-01</p> <p>We have constructed 23-year (1994-2016) time series of Antarctic Peninsula (AP) <span class="hlt">ice</span>-shelf height change using data from four satellite radar altimeters (ERS-1, ERS-2, Envisat, and CryoSat-2). Combining these time series with output from atmospheric and firn models, we partitioned the total height-change signal into contributions from varying surface <span class="hlt">mass</span> balance, firn state, <span class="hlt">ice</span> dynamics, and basal <span class="hlt">mass</span> balance. On the Bellingshausen coast of the AP, <span class="hlt">ice</span> shelves lost 84 ± 34 Gt a-1 to basal melting, compared to contributions of 50 ± 7 Gt a-1 from surface <span class="hlt">mass</span> balance and <span class="hlt">ice</span> dynamics. Net basal melting on the Weddell coast was 51 ± 71 Gt a-1. Recent changes in <span class="hlt">ice</span>-shelf height include increases over major AP <span class="hlt">ice</span> shelves driven by changes in firn state. Basal melt rates near Bawden <span class="hlt">Ice</span> Rise, a major pinning point of Larsen C <span class="hlt">Ice</span> Shelf, showed large increases, potentially leading to substantial loss of buttressing if sustained.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('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 <span class="hlt">mass</span> and dynamic changes of Larsen B’s southern neighbour Larsen C, the fourth largest <span class="hlt">ice</span> shelf in Antarctica, may herald a similar instability. Here, using a validated <span class="hlt">ice</span>-shelf model run in diagnostic mode, constrained by satellite and in situ geophysical data, we identify the nature of this potential instability. We demonstrate that the present-day spatial distribution and orientation of the principal stresses within Larsen C <span class="hlt">ice</span> shelf are akin to those within pre-collapse Larsen B. When Larsen B’s stabilizing frontal portion was lost in 1995, the unstable remaining shelf accelerated, crumbled and ultimately collapsed. We hypothesize that Larsen C <span class="hlt">ice</span> shelf may suffer a similar fate if it were not stabilized by warm and mechanically soft marine <span class="hlt">ice</span>, entrained within narrow suture zones. PMID:24751641</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14.3773S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.3773S"><span>A better GRACE solution for improving the regional Greenland <span class="hlt">mass</span> balance</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schrama, E.; Xu, Z.</p> <p>2012-04-01</p> <p>In most GRACE based researches, a variety of smoothing methods is employed to remove alternating bands of positive and negative stripes stretching in the north-south direction. Many studies have suggested to smooth the GRACE maps, on which <span class="hlt">mass</span> <span class="hlt">variations</span> are represented as equivalent water height (EWH). Such maps are capable of exposing the redistribution of earth surface <span class="hlt">mass</span> over time. In Greenland the shrinking of the <span class="hlt">ice</span> cap becomes significant in the last decade. Our present study confirms that the dominating melting trends are in the east and southeast coastal zones, however, the smoothed signals along the coastline in these areas do not represent the original but averaged measurements from GRACE satellites which means the signal strength indicating that negative <span class="hlt">mass</span> <span class="hlt">variations</span> are mixed with some positive signals that are very close to this area. An exact identification of the topographic edge is not possible and visually the EWH maps appear to be blurred. To improve this, we firstly used spherical harmonic coefficients of GRACE level-2 data from CSR-RL04 and produced a smoothed EWH map. Empirical Orthogonal Functions(EOF)/Principal Component Analysis(PCA) have been introduced as well, in order to extract the melting information associated with the recent warming climate. Next, the Greenland area is redefined by 16 basins and the corresponding melting zones are quantified respectively. Least Squares methods are invoked to interpolate the <span class="hlt">mass</span> distribution function on each basin. In this way we are able to estimate more accurately regional <span class="hlt">ice</span> melting rate and we sharpen the EWH map. After comparing our results with a hydrological model the combination SMB - D is established which contains the surface <span class="hlt">mass</span> balance (SMB) and <span class="hlt">ice</span>-discharge (D). A general agreement can be reached and it turns out this method is capable to enhance our understanding of the shrinking global cryosphere</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMGC21G..03W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMGC21G..03W"><span>Dust Records in <span class="hlt">Ice</span> Cores from the Tibetan Plateau</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, N.; Yao, T.; Thompson, L. G.</p> <p>2014-12-01</p> <p>Dust plays an important role in the Earth system, and it usually displays largely spatial and temporal <span class="hlt">variations</span>. It is necessary for us to reconstruct the past <span class="hlt">variations</span> of dust in different regions to better understand the interactions between dust and environments. <span class="hlt">Ice</span> core records can reveal the history of dust <span class="hlt">variations</span>. In this paper, we used the Guliya, Dunde, Malan and Dasuopu <span class="hlt">ice</span> cores from the Tibetan Plateau to study the spatial distribution, the seasonal <span class="hlt">variations</span> and the secular trends of dust. It was found that the mean dust concentration was higher by one or two order of magnitudes in the Guliya and Dunde <span class="hlt">ice</span> cores from the northern Tibetan Plateau than in the Dasuopu <span class="hlt">ice</span> core from the southern Tibetan Plateau. During the year, the highest dust concentration occurs in the springtime in the northern Tibetan Plateau while in the non-monsoon season in the southern Tibetan Plateau. Over the last millennium, the Dasuopu <span class="hlt">ice</span> core record shows that the 1270s~1380s and 1870s~1990s were the two epochs with high dust concentration. However, the Malan <span class="hlt">ice</span> core from the northern Tibetan Plateau indicates that high dust concentration occurred in the 1130s~1550s and 1770s~1940s. Interestingly, climatic and environmental records of the <span class="hlt">ice</span> cores from the Tibetan Plateau reflected that the correlation between dust concentration and air temperature was strongly positive in the southern Plateau while negative in the northern Plateau over the last millennium. This implies that climatic and environmental changes existed considerable differences in the different parts of the Plateau. Moreover, four Asian megadroughts occurred in 1638~1641, 1756~1758, 1790~1796 and 1876~1878, which caused more than tens millions people died, were revealed clearly by dust record in the Dasuopu <span class="hlt">ice</span> core.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.P53E2187S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.P53E2187S"><span>Geomorphological Evidence for Pervasive Ground <span class="hlt">Ice</span> on Ceres from Dawn Observations of Craters and Flows.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schmidt, B. E.; Chilton, H.; Hughson, K.; Scully, J. E. C.; Russell, C. T.; Sizemore, H. G.; Nathues, A.; Platz, T.; Bland, M. T.; Schenk, P.; Hiesinger, H.; Jaumann, R.; Byrne, S.; Schorghofer, N.; Ammannito, E.; Marchi, S.; O'Brien, D. P.; Sykes, M. V.; Le Corre, L.; Capria, M. T.; Reddy, V.; Raymond, C. A.; Mest, S. C.; Feldman, W. C.</p> <p>2015-12-01</p> <p>Five decades of observations of Ceres' albedo, surface composition, shape and density suggest that Ceres is comprised of both silicates and tens of percent of <span class="hlt">ice</span>. Historical suggestions of surficial hydrated silicates and evidence for water emission, coupled with its bulk density of ~2100 kg/m3 and Dawn observations of young craters containing high albedo spots support this conclusion. We report geomorphological evidence from survey data demonstrating that evaporative and fluid-flow processes within silicate-<span class="hlt">ice</span> mixtures are prevalent on Ceres, and indicate that its surface materials contain significant water <span class="hlt">ice</span>. Here we highlight three classes of features that possess strong evidence for ground <span class="hlt">ice</span>. First, ubiquitous scalloped and "breached" craters are characterized by <span class="hlt">mass</span> wasting and by the recession of crater walls in asymmetric patterns; these appear analogous to scalloped terrain on Mars and protalus lobes formed by <span class="hlt">mass</span> wasting in terrestrial glaciated regions. The degradation of crater walls appears to be responsible for the nearly complete removal of some craters, particularly at low latitudes. Second, several high latitude, high elevation craters feature lobed flows that emanate from cirque-shaped head walls and bear strikingly similar morphology to terrestrial rock glaciers. These similarities include lobate toes and indications of furrows and ridges consistent with <span class="hlt">ice</span>-cored or <span class="hlt">ice</span>-cemented material. Other lobed flows persist at the base of crater walls and <span class="hlt">mass</span> wasting features. Many flow features evidently terminate at ramparts. Third, there are frequent irregular domes, peaks and mounds within crater floors that depart from traditional crater central peaks or peak complexes. In some cases the irregular domes show evidence for high albedo or activity, and thus given other evidence for <span class="hlt">ice</span>, these could be due to local melt and extrusion via hydrologic gradients, forming domes similar to pingos. The global distribution of these classes of features</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018CliPa..14..455T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018CliPa..14..455T"><span>The sensitivity of the Greenland <span class="hlt">Ice</span> Sheet to glacial-interglacial oceanic forcing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tabone, Ilaria; Blasco, Javier; Robinson, Alexander; Alvarez-Solas, Jorge; Montoya, Marisa</p> <p>2018-04-01</p> <p>Observations suggest that during the last decades the Greenland <span class="hlt">Ice</span> Sheet (GrIS) has experienced a gradually accelerating <span class="hlt">mass</span> loss, in part due to the observed speed-up of several of Greenland's marine-terminating glaciers. Recent studies directly attribute this to warming North Atlantic temperatures, which have triggered melting of the outlet glaciers of the GrIS, grounding-line retreat and enhanced <span class="hlt">ice</span> discharge into the ocean, contributing to an acceleration of sea-level rise. Reconstructions suggest that the influence of the ocean has been of primary importance in the past as well. This was the case not only in interglacial periods, when warmer climates led to a rapid retreat of the GrIS to land above sea level, but also in glacial periods, when the GrIS expanded as far as the continental shelf break and was thus more directly exposed to oceanic changes. However, the GrIS response to palaeo-oceanic <span class="hlt">variations</span> has yet to be investigated in detail from a mechanistic modelling perspective. In this work, the evolution of the GrIS over the past two glacial cycles is studied using a three-dimensional hybrid <span class="hlt">ice</span>-sheet-shelf model. We assess the effect of the <span class="hlt">variation</span> of oceanic temperatures on the GrIS evolution on glacial-interglacial timescales through changes in submarine melting. The results show a very high sensitivity of the GrIS to changing oceanic conditions. Oceanic forcing is found to be a primary driver of GrIS expansion in glacial times and of retreat in interglacial periods. If switched off, palaeo-atmospheric <span class="hlt">variations</span> alone are not able to yield a reliable glacial configuration of the GrIS. This work therefore suggests that considering the ocean as an active forcing should become standard practice in palaeo-<span class="hlt">ice</span>-sheet modelling.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_21 --> <div id="page_22" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="421"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2791593','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2791593"><span>The future of <span class="hlt">ice</span> sheets and sea <span class="hlt">ice</span>: Between reversible retreat and unstoppable loss</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Notz, Dirk</p> <p>2009-01-01</p> <p>We discuss the existence of cryospheric “tipping points” in the Earth's climate system. Such critical thresholds have been suggested to exist for the disappearance of Arctic sea <span class="hlt">ice</span> and the retreat of <span class="hlt">ice</span> sheets: Once these <span class="hlt">ice</span> <span class="hlt">masses</span> have shrunk below an anticipated critical extent, the ice–albedo feedback might lead to the irreversible and unstoppable loss of the remaining <span class="hlt">ice</span>. We here give an overview of our current understanding of such threshold behavior. By using conceptual arguments, we review the recent findings that such a tipping point probably does not exist for the loss of Arctic summer sea <span class="hlt">ice</span>. Hence, in a cooler climate, sea <span class="hlt">ice</span> could recover rapidly from the loss it has experienced in recent years. In addition, we discuss why this recent rapid retreat of Arctic summer sea <span class="hlt">ice</span> might largely be a consequence of a slow shift in <span class="hlt">ice</span>-thickness distribution, which will lead to strongly increased year-to-year variability of the Arctic summer sea-<span class="hlt">ice</span> extent. This variability will render seasonal forecasts of the Arctic summer sea-<span class="hlt">ice</span> extent increasingly difficult. We also discuss why, in contrast to Arctic summer sea <span class="hlt">ice</span>, a tipping point is more likely to exist for the loss of the Greenland <span class="hlt">ice</span> sheet and the West Antarctic <span class="hlt">ice</span> sheet. PMID:19884496</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C33A0766L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C33A0766L"><span>Stick-slip Cycles and Tidal Modulation of <span class="hlt">Ice</span> Stream Flow</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lipovsky, B.; Dunham, E. M.</p> <p>2016-12-01</p> <p>The reactivation of a single dormant Antarctic <span class="hlt">ice</span> stream would double the continent's <span class="hlt">mass</span> imbalance. Despite importance of understanding the likelihood of such an event, direct observation of the basal processes that lead to the activation and stagnation of streaming <span class="hlt">ice</span> are minimal. As the only <span class="hlt">ice</span> stream undergoing stagnation, the Whillans <span class="hlt">Ice</span> Plain (WIP) occupies a central role in our understanding of these subglacial processes. Complicating matters is the observation, from GPS records, that the WIP experiences most of its motion during episodes of rapid sliding. These sliding events are tidally modulated and separated by 12 hour periods of quiescence. We conduct numerical simulations of <span class="hlt">ice</span> stream stick-slip cycles. Our simulations include rate- and state-dependent frictional sliding, tidal forcing, inertia, upstream loading in a cross-stream, thickness-averaged formulation. Our principal finding is that <span class="hlt">ice</span> stream motion may respond to ocean tidal forcing with one of two end member behaviors. In one limit, tidally modulated slip events have rupture velocities that approach the shear wave speed and slip events have a duration that scales with the <span class="hlt">ice</span> stream width divided by the shear wave speed. In the other limit, tidal modulation results in <span class="hlt">ice</span> stream sliding velocities with lower amplitude <span class="hlt">variation</span> but at much longer timescales, i.e. semi-diurnal and longer. This latter behavior more closely mimics the behavior of several active <span class="hlt">ice</span> streams (Bindschadler, Rutford). We find that WIP slip events exist between these two end member behaviors: rupture velocities are far below the inertial limit yet sliding occurs only episodically. The continuum of sliding behaviors is governed by a critical <span class="hlt">ice</span> stream width over which slip event nucleate. When the critical width is much longer than the <span class="hlt">ice</span> stream width, slip events are unable to nucleate. The critical width depends on the subglacial effective pressure, <span class="hlt">ice</span> thickness, and frictional and elastic constitutive</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.C23E0542F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.C23E0542F"><span>Validation and Interpretation of a New Sea <span class="hlt">Ice</span> Globice 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>2011-12-01</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 <span class="hlt">mass</span> 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://www.osti.gov/biblio/22522230-systematic-variations-co-sub-sub-ice-abundance-ratios-nearby-galaxies-found-akari-near-infrared-spectroscopy','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22522230-systematic-variations-co-sub-sub-ice-abundance-ratios-nearby-galaxies-found-akari-near-infrared-spectroscopy"><span>SYSTEMATIC <span class="hlt">VARIATIONS</span> IN CO{sub 2}/H{sub 2}O <span class="hlt">ICE</span> ABUNDANCE RATIOS IN NEARBY GALAXIES FOUND WITH AKARI NEAR-INFRARED SPECTROSCOPY</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>Yamagishi, M.; Kaneda, H.; Ishihara, D.</p> <p>2015-07-01</p> <p>We report CO{sub 2}/H{sub 2}O <span class="hlt">ice</span> abundance ratios in seven nearby star-forming galaxies based on the AKARI near-infrared (2.5–5.0 μm) spectra. The CO{sub 2}/H{sub 2}O <span class="hlt">ice</span> abundance ratios show clear <span class="hlt">variations</span> between 0.05 and 0.2 with the averaged value of 0.14 ± 0.01. The previous study on M82 revealed that the CO{sub 2}/H{sub 2}O <span class="hlt">ice</span> abundance ratios strongly correlate with the intensity ratios of the hydrogen recombination Brα line to the polycyclic aromatic hydrocarbon (PAH) 3.3 μm feature. In the present study, however, we find no correlation for the seven galaxies as a whole due to systematic differences in themore » relation between CO{sub 2}/H{sub 2}O <span class="hlt">ice</span> abundance and Brα/PAH 3.3 μm intensity ratios from galaxy to galaxy. This result suggests that there is another parameter that determines the CO{sub 2}/H{sub 2}O <span class="hlt">ice</span> abundance ratios in a galaxy in addition to the Brα/PAH 3.3 μm ratios. We find that the CO{sub 2}/H{sub 2}O <span class="hlt">ice</span> abundance ratios positively correlate with the specific star formation rates of the galaxies. From these results, we conclude that CO{sub 2}/H{sub 2}O <span class="hlt">ice</span> abundance ratios tend to be high in young star-forming galaxies.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007JGRD..11210208Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007JGRD..11210208Y"><span>Intra-annual <span class="hlt">variations</span> in atmospheric dust and tritium in the North Pacific region detected from an <span class="hlt">ice</span> core from Mount Wrangell, Alaska</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yasunari, Teppei J.; Shiraiwa, Takayuki; Kanamori, Syosaku; Fujii, Yoshiyuki; Igarashi, Makoto; Yamazaki, Koji; Benson, Carl S.; Hondoh, Takeo</p> <p>2007-05-01</p> <p>The North Pacific is subject to various seasonal climate phenomena and material circulations. Therefore intra-annual <span class="hlt">ice</span> core data are necessary for an assessment of the climate <span class="hlt">variations</span>. To assess past <span class="hlt">variations</span>, a 50-m <span class="hlt">ice</span> core was drilled at the summit of Mount Wrangell Volcano, Alaska. The dust number, tritium concentrations, and stable hydrogen isotope were analyzed. The period covered was from 1992 to 2002. We found that the concentrations of both fine dust (0.52-1.00 μm), an indicator of long-range transport, and coarse dust (1.00-8.00 μm) increased together every spring. Moreover, their concentrations increased drastically after 2000, corresponding to the recent increase in Asian dust outbreaks in spring. Additionally, an increase in the spring of 2001 corresponded to the largest dust storm recorded in east Asia since 1979. Therefore our findings imply that Asian dust strongly polluted Mount Wrangell every spring. The stratospheric tracer, tritium, had late spring maxima almost every year, and we found this useful for <span class="hlt">ice</span> core dating to identify late spring in the North Pacific region. We also found that a high positive annual correlation existed between the calculated tritium and fine dust fluxes from late spring to summer. We propose that an annual relationship between the stratosphere-troposphere exchange and Asian dust storm are most closely connected in late spring because their activities are weak in summer. The Mount Wrangell <span class="hlt">ice</span> core is important and useful for assessing the dust and tritium circulation in the distant past around the North Pacific with probable intra-annual timescale information.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ApJ...834..115T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ApJ...834..115T"><span>Multi-epoch Detections of Water <span class="hlt">Ice</span> Absorption in Edge-on Disks around Herbig Ae Stars: PDS 144N and PDS 453</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Terada, Hiroshi; Tokunaga, Alan T.</p> <p>2017-01-01</p> <p>We report the multi-epoch detections of water <span class="hlt">ice</span> in 2.8-4.2 μ {{m}} spectra of two Herbig Ae stars, PDS 144N (A2 IVe) and PDS 453 (F2 Ve), which have an edge-on circumstellar disk. The detected water <span class="hlt">ice</span> absorption is found to originate from their protoplanetary disks. The spectra show a relatively shallow absorption of water <span class="hlt">ice</span> of around 3.1 μ {{m}} for both objects. The optical depths of the water <span class="hlt">ice</span> absorption are ˜0.1 and ˜0.2 for PDS 144N and PDS 453, respectively. Compared to the water <span class="hlt">ice</span> previously detected in low-<span class="hlt">mass</span> young stellar objects with an edge-on disk with a similar inclination angle, these optical depths are significantly lower. It suggests that stronger UV radiation from the central stars effectively decreases the water <span class="hlt">ice</span> abundance around the Herbig Ae stars through photodesorption. The water <span class="hlt">ice</span> absorption in PDS 453 shows a possible <span class="hlt">variation</span> of the feature among the six observing epochs. This <span class="hlt">variation</span> could be due to a change of absorption materials passing through our line of sight to the central star. The overall profile of the water <span class="hlt">ice</span> absorption in PDS 453 is quite similar to the absorption previously reported in the edge-on disk object d216-0939, and this unique profile may be seen only at a high inclination angle in the range of 76°-80°.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990008060&hterms=3G&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3D3G','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990008060&hterms=3G&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3D3G"><span>Global Geodetic Signatures of the Antarctic <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>James, Thomas S.; Ivins, Erik R.</p> <p>1997-01-01</p> <p>Four scenarios of present day Antarctic <span class="hlt">ice</span> sheet <span class="hlt">mass</span> change are developed from comprehensive reviews of the available glaciological and oceanographic evidence. The gridded scenarios predict widely varying contributions to secular sea level change xi ranging from -1.1 to 0.45 mm/yr, and predict polar motion m and time-varying low-degree gravitational coefficients J(sub l) that differ significantly from earlier estimates. A reasonably linear relationship between the rate of sea level change from Antarctica xi(sub A) and the predicted Antarctic J(sub l) is found for the four scenarios. This linearity permits a series of forward models to be constructed that incorporate the effects of <span class="hlt">ice</span> <span class="hlt">mass</span> changes in Antarctica, Greenland, and distributed smaller glaciers, as well as postglacial rebound (assuming the <span class="hlt">ICE</span>-3G deglaciation history), with the goal of obtaining optimum reconciliation between observed constraints on J(sub l) and sea level rise xi. Numerous viable combinations of lower mantle viscosity and hydrologic sources are found that safely "observed" in the range of 1 to 2-2.5 mm/yr and observed J(sub l) for degrees 2, 3, and 4. In contrast, rates of global sea level rise above 2.5 mm/yr are inconsistent with available J(sub l) observations. The successful composite models feature a pair of lower mantle viscosity solutions arising from the sensitivity of J(sub l) to glacial rebound. The paired values are well separated at xi = 1 mm/yr, but move closer together as xi is increased, and, in fact, merge around xi = 2 - 2.5 mm/yr, revealing an intimate relation between xi and preferred lower mantle viscosity. This general pattern is quite robust and persists for different J(sub l) solutions, for <span class="hlt">variations</span> in source assumptions, and for different styles of lower mantle viscosity stratification. Tighter J(sub l) constraints for l greater than 2 may allow some viscosity stratification schemes and source assumptions to be excluded in the future. For a given total</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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>Cloud <span class="hlt">ice</span> plays important roles in Earth's energy budget and cloud-precipitation processes. Knowledge of global cloud <span class="hlt">ice</span> and its properties is critical for understanding and quantifying its roles in Earth's atmospheric system. It remains a great challenge to measure these variables accurately from space. Submillimeter (submm) wave remote sensing has capability of penetrating clouds and measuring <span class="hlt">ice</span> <span class="hlt">mass</span> and microphysical properties. In particular, the 883-GHz frequency is a highest spectral window in microwave frequencies that can be used to fill a sensitivity gap between thermal infrared (IR) and mm-wave sensors in current spaceborne cloud <span class="hlt">ice</span> observations. <span class="hlt">Ice</span>Cube is a cubesat spaceflight demonstration of 883-GHz radiometer technology. Its primary objective is to raise the technology readiness level (TRL) of 883-GHz cloud radiometer for future Earth science missions. By flying a commercial receiver on a 3U cubesat, <span class="hlt">Ice</span>Cube is able to achieve fast-track maturation of space technology, by completing its development, integration and testing in 2.5 years. <span class="hlt">Ice</span>Cube was successfully delivered to ISS in April 2017 and jettisoned from the International Space Station (ISS) in May 2017. The <span class="hlt">Ice</span>Cube cloud-<span class="hlt">ice</span> radiometer (ICIR) has been acquiring data since the jettison on a daytime-only operation. <span class="hlt">Ice</span>Cube adopted a simple design without payload mechanism. It makes maximum utilization of solar power by spinning the spacecraft continuously about the Sun vector at a rate of 1.2° per second. As a result, the ICIR is operated under the limited resources (8.6 W without heater) and largely-varying (18°C-28°C) thermal environments. The spinning cubesat also allows ICIR to have periodical views between the Earth (atmosphere and clouds) and cold space (calibration), from which the first 883-GHz cloud map is obtained. The 883-GHz cloud radiance, sensitive to <span class="hlt">ice</span> particle scattering, is proportional to cloud <span class="hlt">ice</span> amount above 10 km. The ICIR cloud map acquired during June 20-July 2</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910044114&hterms=marginal&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dmarginal','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910044114&hterms=marginal&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dmarginal"><span>Ku band airborne radar altimeter observations of marginal sea <span class="hlt">ice</span> during the 1984 Marginal <span class="hlt">Ice</span> Zone Experiment</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>1991-01-01</p> <p>Pulse-limited, airborne radar data taken in June and July 1984 with a 13.8-GHz altimeter over the Fram Strait marginal <span class="hlt">ice</span> zone are analyzed with the aid of large-format aerial photography, airborne synthetic aperture radar data, and surface observations. <span class="hlt">Variations</span> in the radar return pulse waveforms are quantified and correlated with <span class="hlt">ice</span> properties recorded during the Marginal <span class="hlt">Ice</span> Zone Experiment. Results indicate that the wide-beam altimeter is a flexible instrument, capable of identifying the <span class="hlt">ice</span> edge with a high degree of accuracy, calculating the <span class="hlt">ice</span> concentration, and discriminating a number of different <span class="hlt">ice</span> classes. This suggests that microwave radar altimeters have a sensitivity to sea <span class="hlt">ice</span> 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 <span class="hlt">ice</span> geophysics puzzle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20000038175&hterms=balance+sheet&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dbalance%2Bsheet','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20000038175&hterms=balance+sheet&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dbalance%2Bsheet"><span>Snowmelt on the Greenland <span class="hlt">Ice</span> Sheet as Derived From Passive Microwave Satellite Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Abdalati, Waleed; Steffen, Konrad</p> <p>1997-01-01</p> <p>The melt extent of the snow on the Greenland <span class="hlt">ice</span> sheet is of considerable importance to the <span class="hlt">ice</span> sheet's <span class="hlt">mass</span> and energy balance, as well as Arctic and global climates. By comparing passive microwave satellite data to field observations, <span class="hlt">variations</span> in melt extent have been detected by establishing melt thresholds in the cross-polarized gradient ratio (XPGR). The XPGR, defined as the normalized difference between the 19-GHz horizontal channel and the 37-GHz vertical channel of the Special Sensor Microwave/Imager (SSM/I), exploits the different effects of snow wetness on different frequencies and polarizations and establishes a distinct melt signal. Using this XPGR melt signal, seasonal and interannual <span class="hlt">variations</span> in snowmelt extent of the <span class="hlt">ice</span> sheet are studied. The melt is found to be most extensive on the western side of the <span class="hlt">ice</span> sheet and peaks in late July. Moreover, there is a notable increasing trend in melt area between the years 1979 and 1991 of 4.4% per year, which came to an abrupt halt in 1992 after the eruption of Mt. Pinatubo. A similar trend is observed in the temperatures at six coastal stations. The relationship between the warming trend and increasing melt trend between 1979 and 1991 suggests that a 1 C temperature rise corresponds to an increase in melt area of 73000 sq km, which in general exceeds one standard deviation of the natural melt area variability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20130014062','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130014062"><span>The <span class="hlt">Ice</span>, Cloud, and land Elevation Satellite (ICESat) Summary Mission Timeline and Performance Relative to Pre-Launch Mission Success Criteria</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Webb, Charles E.; Zwally H. Jay; Abdalati, Waleed</p> <p>2012-01-01</p> <p>The <span class="hlt">Ice</span>, Cloud and land Elevation Satellite (ICESat) mission was conceived, primarily, to quantify the spatial and temporal <span class="hlt">variations</span> in the topography of the Greenland and Antarctic <span class="hlt">ice</span> sheets. It carried on board the Geoscience Laser Altimeter System (GLAS), which measured the round-trip travel time of a laser pulse emitted from the satellite to the surface of the Earth and back. Each range derived from these measurements was combined with precise, concurrent orbit and pointing information to determine the location of the laser spot centroid on the Earth. By developing a time series of precise topographic maps for each <span class="hlt">ice</span> sheet, changes in their surface elevations can be used to infer their <span class="hlt">mass</span> balances.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28973875','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28973875"><span>Katabatic winds diminish precipitation contribution to the Antarctic <span class="hlt">ice</span> <span class="hlt">mass</span> balance.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Grazioli, Jacopo; Madeleine, Jean-Baptiste; Gallée, Hubert; Forbes, Richard M; Genthon, Christophe; Krinner, Gerhard; Berne, Alexis</p> <p>2017-10-10</p> <p>Snowfall in Antarctica is a key term of the <span class="hlt">ice</span> sheet <span class="hlt">mass</span> budget that influences the sea level at global scale. Over the continental margins, persistent katabatic winds blow all year long and supply the lower troposphere with unsaturated air. We show that this dry air leads to significant low-level sublimation of snowfall. We found using unprecedented data collected over 1 year on the coast of Adélie Land and simulations from different atmospheric models that low-level sublimation accounts for a 17% reduction of total snowfall over the continent and up to 35% on the margins of East Antarctica, significantly affecting satellite-based estimations close to the ground. Our findings suggest that, as climate warming progresses, this process will be enhanced and will limit expected precipitation increases at the ground level.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19760011494','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19760011494"><span>Skylab floating <span class="hlt">ice</span> experiment</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Campbell, W. J. (Principal Investigator); Ramseier, R. O.; Weaver, R. J.; Weeks, W. F.</p> <p>1975-01-01</p> <p>The author has identified the following significant results. Coupling of the aircraft data with the ground truth observations proved to be highly successful with interesting results being obtained with IR and SLAR passive microwave techniques, and standard photography. Of particular interest were the results of the PMIS system which operated at 10.69 GHz with both vertical and horizontal polarizations. This was the first time that dual polarized images were obtained from floating <span class="hlt">ice</span>. In both sea and lake <span class="hlt">ice</span>, it was possible to distinguish a wide variety of thin <span class="hlt">ice</span> types because of their large differences in brightness temperatures. It was found that the higher brightness temperature was invariably obtained in the vertically polarized mode, and as the age of the <span class="hlt">ice</span> increases the brightness temperature increases in both polarizations. Associated with this change in age, the difference in temperature was observed as the different polarizations decreased. It appears that the horizontally polarized data is the most sensitive to <span class="hlt">variations</span> in <span class="hlt">ice</span> type for both fresh water and sea <span class="hlt">ice</span>. The study also showed the great amount of information on <span class="hlt">ice</span> surface roughness and deformation patterns that can be obtained from X-band SLAR observations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050123573','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050123573"><span>Coupled Gravity and Elevation Measurement of <span class="hlt">Ice</span> Sheet <span class="hlt">Mass</span> Change</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jezek, K. C.; Baumgartner, F.</p> <p>2005-01-01</p> <p>During June 2003, we measured surface gravity at six locations about a glaciological measurement site located on the South-central Greenland <span class="hlt">Ice</span>. We operated a GPS unit for 90 minutes at each site -the unit was operated simultaneously with a base station unit in Sondrestrom Fjord so as to enable differential, post-processing of the data. We installed an aluminum, accumulation-rate-pole at each site. The base section of the pole also served as the mount for the GPS antenna. Two gravimeters were used simultaneously at each site. Measurements were repeated at each site with at time lapse of at least 50 minutes. We measured snow physical properties in two shallow pits The same measurement sites were occupied in 1981 and all were part of a hexagonal network of geodetic and glaciological measurements established by The Ohio State University in 1980. Additional gravity observations were acquired at three of the sites in 1993 and 1995. Gravity data were collected in conjunction with Doppler satellite measurements of position and elevation in 1981 and global positioning system measurements subsequently. The use of satellite navigation techniques permitted reoccupation of the same sites in each year to within a few 10 s of meters or better. After detrending the gravity data, making adjustments for tides and removing the residual effects of local spatial gradients in gravity, we observe an average secular decrease in gravity of about 0.01 milligal/year, but with tenths of milligal <span class="hlt">variations</span> about the mean trend. The trend is consistent with a nearly linear increase in surface elevation of between 7 to 10 c d y r (depending on location) as measured by repeated airborne laser altimeter, surface Doppler satellite and GPS elevation measurements. Differences between the residual gravity anomalies after free air correction may be attributable to local <span class="hlt">mass</span> changes. This project is a collaboration between the Byrd Polar Research Center of the Ohio State University and the Arctic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013Sci...341..266R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013Sci...341..266R"><span><span class="hlt">Ice</span>-Shelf Melting Around Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rignot, E.; Jacobs, S.; Mouginot, J.; Scheuchl, B.</p> <p>2013-07-01</p> <p>We compare the volume flux divergence of Antarctic <span class="hlt">ice</span> shelves in 2007 and 2008 with 1979 to 2010 surface accumulation and 2003 to 2008 thinning to determine their rates of melting and <span class="hlt">mass</span> balance. Basal melt of 1325 ± 235 gigatons per year (Gt/year) exceeds a calving flux of 1089 ± 139 Gt/year, making <span class="hlt">ice</span>-shelf melting the largest ablation process in Antarctica. The giant cold-cavity Ross, Filchner, and Ronne <span class="hlt">ice</span> shelves covering two-thirds of the total <span class="hlt">ice</span>-shelf area account for only 15% of net melting. Half of the meltwater comes from 10 small, warm-cavity Southeast Pacific <span class="hlt">ice</span> shelves occupying 8% of the area. A similar high melt/area ratio is found for six East Antarctic <span class="hlt">ice</span> shelves, implying undocumented strong ocean thermal forcing on their deep grounding lines.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17834534','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17834534"><span>The little <span class="hlt">ice</span> age as recorded in the stratigraphy of the tropical quelccaya <span class="hlt">ice</span> cap.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Thompson, L G; Mosley-Thompson, E; Dansgaard, W; Grootes, P M</p> <p>1986-10-17</p> <p>The analyses of two <span class="hlt">ice</span> cores from a southern tropical <span class="hlt">ice</span> cap provide a record of climatic conditions over 1000 years for a region where other proxy records are nearly absent. Annual <span class="hlt">variations</span> in visible dust layers, oxygen isotopes, microparticle concentrations, conductivity, and identification of the historical (A.D. 1600) Huaynaputina ash permit accurate dating and time-scale verification. The fact that the Little <span class="hlt">Ice</span> Age (about A.D. 1500 to 1900) stands out as a significant climatic event in the oxygen isotope and electrical conductivity records confirms the worldwide character of this event.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19880011759','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19880011759"><span>An experimental and theoretical study of the <span class="hlt">ice</span> accretion process during artificial and natural <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>Kirby, Mark S.; Hansman, R. John</p> <p>1988-01-01</p> <p>Real-time measurements of <span class="hlt">ice</span> growth during artificial and natural <span class="hlt">icing</span> conditions were conducted using an ultrasonic pulse-echo technique. This technique allows <span class="hlt">ice</span> thickness to be measured with an accuracy of + or - 0.5 mm; in addition, the ultrasonic signal characteristics may be used to detect the presence of liquid on the <span class="hlt">ice</span> surface and hence discern wet and dry <span class="hlt">ice</span> growth behavior. <span class="hlt">Ice</span> growth was measured on the stagnation line of a cylinder exposed to artificial <span class="hlt">icing</span> conditions in the NASA Lewis <span class="hlt">Icing</span> Research Tunnel (IRT), and similarly for a cylinder exposed in flight to natural <span class="hlt">icing</span> conditions. <span class="hlt">Ice</span> thickness was observed to increase approximately linearly with exposure time during the initial <span class="hlt">icing</span> period. The <span class="hlt">ice</span> accretion rate was found to vary with cloud temperature during wet <span class="hlt">ice</span> growth, and liquid runback from the stagnation region was inferred. A steady-state energy balance model for the <span class="hlt">icing</span> surface was used to compare heat transfer characteristics for IRT and natural <span class="hlt">icing</span> conditions. Ultrasonic measurements of wet and dry <span class="hlt">ice</span> growth observed in the IRT and in flight were compared with <span class="hlt">icing</span> regimes predicted by a series of heat transfer coefficients. The heat transfer magnitude was generally inferred to be higher for the IRT than for the natural <span class="hlt">icing</span> conditions encountered in flight. An apparent <span class="hlt">variation</span> in the heat transfer magnitude was also observed for flights conducted through different natural <span class="hlt">icing</span>-cloud formations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016OcSci..12..507M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016OcSci..12..507M"><span>Turbulent heat transfer as a control of platelet <span class="hlt">ice</span> growth in supercooled under-<span class="hlt">ice</span> ocean boundary layers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McPhee, Miles G.; Stevens, Craig L.; Smith, Inga J.; Robinson, Natalie J.</p> <p>2016-04-01</p> <p>Late winter measurements of turbulent quantities in tidally modulated flow under land-fast sea <span class="hlt">ice</span> near the Erebus Glacier Tongue, McMurdo Sound, Antarctica, identified processes that influence growth at the interface of an <span class="hlt">ice</span> surface in contact with supercooled seawater. The data show that turbulent heat exchange at the ocean-<span class="hlt">ice</span> boundary is characterized by the product of friction velocity and (negative) water temperature departure from freezing, analogous to similar results for moderate melting rates in seawater above freezing. Platelet <span class="hlt">ice</span> growth appears to increase the hydraulic roughness (drag) of fast <span class="hlt">ice</span> compared with undeformed fast <span class="hlt">ice</span> without platelets. Platelet growth in supercooled water under thick <span class="hlt">ice</span> appears to be rate-limited by turbulent heat transfer and that this is a significant factor to be considered in <span class="hlt">mass</span> transfer at the underside of <span class="hlt">ice</span> shelves and sea <span class="hlt">ice</span> in the vicinity of <span class="hlt">ice</span> shelves.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22426697','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22426697"><span>Contribution of myostatin gene polymorphisms to normal <span class="hlt">variation</span> in lean <span class="hlt">mass</span>, fat <span class="hlt">mass</span> and peak BMD in Chinese male offspring.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yue, Hua; He, Jin-wei; Zhang, Hao; Wang, Chun; Hu, Wei-wei; Gu, Jie-mei; Ke, Yao-hua; Fu, Wen-zhen; Hu, Yun-qiu; Li, Miao; Liu, Yu-juan; Wu, Song-hua; Zhang, Zhen-lin</p> <p>2012-05-01</p> <p>Myostatin gene is a member of the transforming growth factor-β (TGF-β) family that negatively regulates skeletal muscle growth. Genetic polymorphisms in Myostatin were found to be associated with the peak bone mineral density (BMD) in Chinese women. The purpose of this study was to investigate whether myostatin played a role in the normal <span class="hlt">variation</span> in peak BMD, lean <span class="hlt">mass</span> (LM), and fat <span class="hlt">mass</span> (FM) of Chinese men. Four hundred male-offspring nuclear families of Chinese Han ethnic group were recruited. Anthropometric measurements, including the peak BMD, body LM and FM were measured using dual-energy X-ray absorptiometry (DXA). The single nucleotide polymorphisms (SNPs) studied were tag-SNPs selected by sequencing. Both rs2293284 and +2278GA were genotyped using TaqMan assay, and rs3791783 was genotyped with PCR-restriction fragment length polymorphism (RFLP) analysis. The associations of the SNPs with anthropometric <span class="hlt">variations</span> were analyzed using the quantitative transmission disequilibrium test (QTDT). Using QTDT to detect within-family associations, neither single SNP nor haplotype was found to be associated with peak BMD at any bone site. However, rs3791783 was found to be significantly associated with fat <span class="hlt">mass</span> of the trunk (P<0.001). Moreover, for within-family associations, haplotypes AGG, AAA, and TGG were found to be significantly associated with the trunk fat <span class="hlt">mass</span> (all P<0.001). Our results suggest that genetic <span class="hlt">variation</span> within myostatin may play a role in regulating the <span class="hlt">variation</span> in fat <span class="hlt">mass</span> in Chinese males. Additionally, the myostatin gene may be a candidate that determines body fat <span class="hlt">mass</span> in Chinese men.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22538614','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22538614"><span>Antarctic <span class="hlt">ice</span>-sheet loss driven by basal melting of <span class="hlt">ice</span> shelves.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pritchard, H D; Ligtenberg, S R M; Fricker, H A; Vaughan, D G; van den Broeke, M R; Padman, L</p> <p>2012-04-25</p> <p>Accurate prediction of global sea-level rise requires that we understand the cause of recent, widespread and intensifying glacier acceleration along Antarctic <span class="hlt">ice</span>-sheet coastal margins. Atmospheric and oceanic forcing have the potential to reduce the thickness and extent of floating <span class="hlt">ice</span> shelves, potentially limiting their ability to buttress the flow of grounded tributary glaciers. Indeed, recent <span class="hlt">ice</span>-shelf collapse led to retreat and acceleration of several glaciers on the Antarctic Peninsula. But the extent and magnitude of <span class="hlt">ice</span>-shelf thickness change, the underlying causes of such change, and its link to glacier flow rate are so poorly understood that its future impact on the <span class="hlt">ice</span> sheets cannot yet be predicted. Here we use satellite laser altimetry and modelling of the surface firn layer to reveal the circum-Antarctic pattern of <span class="hlt">ice</span>-shelf thinning through increased basal melt. We deduce that this increased melt is the primary control of Antarctic <span class="hlt">ice</span>-sheet loss, through a reduction in buttressing of the adjacent <span class="hlt">ice</span> sheet leading to accelerated glacier flow. The highest thinning rates occur where warm water at depth can access thick <span class="hlt">ice</span> shelves via submarine troughs crossing the continental shelf. Wind forcing could explain the dominant patterns of both basal melting and the surface melting and collapse of Antarctic <span class="hlt">ice</span> shelves, through ocean upwelling in the Amundsen and Bellingshausen seas, and atmospheric warming on the Antarctic Peninsula. This implies that climate forcing through changing winds influences Antarctic <span class="hlt">ice</span>-sheet <span class="hlt">mass</span> balance, and hence global sea level, on annual to decadal timescales.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_22 --> <div id="page_23" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="441"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JPhCS.718e2033R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JPhCS.718e2033R"><span>Cosmic ray spectrum and composition from three years of <span class="hlt">Ice</span>Top and <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>Rawlins, K.; <author pre="for ">IceCube Collaboration</p> <p>2016-05-01</p> <p><span class="hlt">Ice</span>Top is the surface component of the <span class="hlt">Ice</span>Cube Observatory, composed of frozen water tanks at the top of <span class="hlt">Ice</span>Cube’s strings. Data from this detector can be analyzed in different ways with the goal of measuring cosmic ray spectrum and composition. The shower size S125 from <span class="hlt">Ice</span>Top alone can be used as a proxy for primary energy, and unfolded into an all-particle spectrum. In addition, S125 from the surface can be combined with high-energy muon energy loss information from the deep <span class="hlt">Ice</span>Cube detector for those air showers which pass through both. Using these coincident events in a complementary analysis, both the spectrum and <span class="hlt">mass</span> composition of primary cosmic rays can be extracted in parallel using a neural network. Both of these analyses have been performed on three years of <span class="hlt">Ice</span>Top and <span class="hlt">Ice</span>Cube data. Both all-particle spectra as well as individual spectra for elemental groups are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040035786&hterms=ships+location&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dships%2Blocation','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040035786&hterms=ships+location&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dships%2Blocation"><span>Studies of the Antarctic Sea <span class="hlt">Ice</span> Edges and <span class="hlt">Ice</span> Extents from Satellite and Ship Observations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Worby, Anthony P.; Comiso, Josefino C.</p> <p>2003-01-01</p> <p>Passive-microwave derived <span class="hlt">ice</span> edge locations in Antarctica are assessed against other satellite data as well as in situ observations of <span class="hlt">ice</span> edge location made between 1989 and 2000. The passive microwave data generally agree with satellite and ship data but the <span class="hlt">ice</span> concentration at the observed <span class="hlt">ice</span> edge varies greatly with averages of 14% for the TEAM algorithm and 19% for the Bootstrap algorithm. The comparisons of passive microwave with the field data show that in the <span class="hlt">ice</span> growth season (March - October) the agreement is extremely good, with r(sup 2) values of 0.9967 and 0.9797 for the Bootstrap and TEAM algorithms respectively. In the melt season however (November - February) the passive microwave <span class="hlt">ice</span> edge is typically 1-2 degrees south of the observations due to the low concentration and saturated nature of the <span class="hlt">ice</span>. Sensitivity studies show that these results can have significant impact on trend and <span class="hlt">mass</span> balance studies of the sea <span class="hlt">ice</span> cover in the Southern Ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4371949','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4371949"><span>Ocean-driven thinning enhances iceberg calving and retreat of Antarctic <span class="hlt">ice</span> shelves</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Liu, Yan; Moore, John C.; Cheng, Xiao; Gladstone, Rupert M.; Bassis, Jeremy N.; Liu, Hongxing; Wen, Jiahong; Hui, Fengming</p> <p>2015-01-01</p> <p>Iceberg calving from all Antarctic <span class="hlt">ice</span> shelves has never been directly measured, despite playing a crucial role in <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balance. Rapid changes to iceberg calving naturally arise from the sporadic detachment of large tabular bergs but can also be triggered by climate forcing. Here we provide a direct empirical estimate of <span class="hlt">mass</span> loss due to iceberg calving and melting from Antarctic <span class="hlt">ice</span> shelves. We find that between 2005 and 2011, the total <span class="hlt">mass</span> loss due to iceberg calving of 755 ± 24 gigatonnes per year (Gt/y) is only half the total loss due to basal melt of 1516 ± 106 Gt/y. However, we observe widespread retreat of <span class="hlt">ice</span> shelves that are currently thinning. Net <span class="hlt">mass</span> loss due to iceberg calving for these <span class="hlt">ice</span> shelves (302 ± 27 Gt/y) is comparable in magnitude to net <span class="hlt">mass</span> loss due to basal melt (312 ± 14 Gt/y). Moreover, we find that iceberg calving from these decaying <span class="hlt">ice</span> shelves is dominated by frequent calving events, which are distinct from the less frequent detachment of isolated tabular icebergs associated with <span class="hlt">ice</span> shelves in neutral or positive <span class="hlt">mass</span> balance regimes. Our results suggest that thinning associated with ocean-driven increased basal melt can trigger increased iceberg calving, implying that iceberg calving may play an overlooked role in the demise of shrinking <span class="hlt">ice</span> shelves, and is more sensitive to ocean forcing than expected from steady state calving estimates. PMID:25733856</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1914046W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1914046W"><span>Bayesian inference of <span class="hlt">ice</span> thickness from 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>Werder, Mauro A.; Huss, Matthias</p> <p>2017-04-01</p> <p>Knowledge about <span class="hlt">ice</span> thickness and volume is indispensable for studying <span class="hlt">ice</span> dynamics, future sea-level rise due to glacier melt or their contribution to regional hydrology. Accurate measurements of glacier thickness require on-site work, usually employing radar techniques. However, these field measurements are time consuming, expensive and sometime downright impossible. Conversely, measurements of the <span class="hlt">ice</span> surface, namely elevation and flow velocity, are becoming available world-wide through remote sensing. The model of Farinotti et al. (2009) calculates <span class="hlt">ice</span> thicknesses based on a <span class="hlt">mass</span> conservation approach paired with shallow <span class="hlt">ice</span> physics using estimates of the surface <span class="hlt">mass</span> balance. The presented work applies a Bayesian inference approach to estimate the parameters of a modified version of this forward model by fitting it to both measurements of surface flow speed and of <span class="hlt">ice</span> thickness. The inverse model outputs <span class="hlt">ice</span> thickness as well the distribution of the error. We fit the model to ten test glaciers and <span class="hlt">ice</span> caps and quantify the improvements of thickness estimates through the usage of surface <span class="hlt">ice</span> flow measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70031148','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70031148"><span>Life-history and ecological correlates of geographic <span class="hlt">variation</span> in egg and clutch <span class="hlt">mass</span> among passerine species</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Martin, T.E.; Bassar, R.D.; Bassar, S.K.; Fontaine, J.J.; Lloyd, P.; Mathewson, Heather A.; Niklison, Alina M.; Chalfoun, A.</p> <p>2006-01-01</p> <p>Broad geographic patterns in egg and clutch <span class="hlt">mass</span> are poorly described, and potential causes of <span class="hlt">variation</span> remain largely unexamined. We describe interspecific <span class="hlt">variation</span> in avian egg and clutch <span class="hlt">mass</span> within and among diverse geographic regions and explore hypotheses related to allometry, clutch size, nest predation, adult mortality, and parental care as correlates and possible explanations of <span class="hlt">variation</span>. We studied 74 species of Passeriformes at four latitudes on three continents: the north temperate United States, tropical Venezuela, subtropical Argentina, and south temperate South Africa. Egg and clutch <span class="hlt">mass</span> increased with adult body <span class="hlt">mass</span> in all locations, but differed among locations for the same body <span class="hlt">mass</span>, demonstrating that egg and clutch <span class="hlt">mass</span> have evolved to some extent independent of body <span class="hlt">mass</span> among regions. A major portion of egg <span class="hlt">mass</span> <span class="hlt">variation</span> was explained by an inverse relationship with clutch size within and among regions, as predicted by life-history theory. However, clutch size did not explain all geographic differences in egg <span class="hlt">mass</span>; eggs were smallest in South Africa despite small clutch sizes. These small eggs might be explained by high nest predation rates in South Africa; life-history theory predicts reduced reproductive effort under high risk of offspring mortality. This prediction was supported for clutch <span class="hlt">mass</span>, which was inversely related to nest predation but not for egg <span class="hlt">mass</span>. Nevertheless, clutch <span class="hlt">mass</span> <span class="hlt">variation</span> was not fully explained by nest predation, possibly reflecting interacting effects of adult mortality. Tests of the possible effects of nest predation on egg <span class="hlt">mass</span> were compromised by limited power and by counterposing direct and indirect effects. Finally, components of parental investment, defined as effort per offspring, might be expected to positively coevolve. Indeed, egg <span class="hlt">mass</span>, but not clutch <span class="hlt">mass</span>, was greater in species that shared incubation by males and females compared with species in which only females incubate eggs. However, egg and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PrOce.136..151D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PrOce.136..151D"><span>Effects of recent decreases in arctic sea <span class="hlt">ice</span> on an <span class="hlt">ice</span>-associated marine bird</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Divoky, George J.; Lukacs, Paul M.; Druckenmiller, Matthew L.</p> <p>2015-08-01</p> <p>Recent major reductions in summer arctic sea <span class="hlt">ice</span> extent could be expected to be affecting the distributions and life histories of arctic marine biota adapted to living adjacent to sea <span class="hlt">ice</span>. Of major concern are the effects of <span class="hlt">ice</span> reductions, and associated increasing SST, on the most abundant forage fish in the Arctic, Arctic cod (Boreogadus saida), the primary prey for the region's upper trophic level marine predators. The black guillemot (Cepphus grylle mandtii) is an <span class="hlt">ice</span>-obligate diving seabird specializing in feeding on Arctic cod and has been studied annually since 1975 at a breeding colony in the western Beaufort Sea. The data set is one of the few allowing assessment of the response of an upper trophic marine predator to recent decadal changes in the region's cryosphere. Analysis of oceanographic conditions north of the colony from 1975 to 2012 for the annual period when parents provision young (mid-July to early September), found no major regime shifts in <span class="hlt">ice</span> extent or SST until the late 1990s with major decreases in <span class="hlt">ice</span> and increases in SST in the first decade of the 21st Century. We examined decadal <span class="hlt">variation</span> in late summer oceanographic conditions, nestling diet and success, and overwinter adult survival, comparing a historical period (1975-1984) with a recent (2003-2012) one. In the historical period sea <span class="hlt">ice</span> retreated an average of 1.8 km per day from 15 July to 1 September to an average distance of 95.8 km from the colony, while in the recent period <span class="hlt">ice</span> retreat averaged 9.8 km per day to an average distance of 506.9 km for the same time period. SST adjacent to the island increased an average of 2.9 °C between the two periods. While Arctic cod comprised over 95% of the prey provided to nestlings in the historical period, in the recent period 80% of the years had seasonal decreases, with Arctic cod decreasing to <5% of the nestling diet, and nearshore demersals, primarily sculpin (Cottidae), comprising the majority of the diet. A five-fold increase in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19980151107','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19980151107"><span>West-Antarctic <span class="hlt">Ice</span> Streams: Analog to <span class="hlt">Ice</span> Flow in Channels on Mars</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lucchitta, B. K.</p> <p>1997-01-01</p> <p>Sounding of the sea floor in front of the Ross <span class="hlt">Ice</span> Shelf in Antarctica recently revealed large persistent patterns of longitudinal megaflutes and drumlinoid forms, which are interpreted to have formed at the base of <span class="hlt">ice</span> streams during the list glacial advance. The flutes bear remarkable resemblance to longitudinal grooves and highly elongated streamlined islands found on the floors of some large martian channels, called outflow channels. ln addition, other similarities exist between Antarctic <span class="hlt">ice</span> streams and outflow channels. <span class="hlt">Ice</span> streams are 30 to 80 km wide and hundreds of kilometers long, as are the martian channels. <span class="hlt">Ice</span> stream beds are below sea level. Floors of many martian outflow channels lie below martian datum, which may have been close to or below past martian sea levels. The Antarctic <span class="hlt">ice</span> stream bed gradient is flat and locally may go uphill, and surface slopes are exceptionally low. So are gradients of martian channels. The depth to the bed in <span class="hlt">ice</span> streams is 1 to 1.5 km. At bankful stage, the depth of the fluid in outflow channels would have been 1 to 2 km. These similarities suggest that the martian outflow channels, whose origin is commonly attributed to gigantic catastrophic floods, were locally filled by <span class="hlt">ice</span> that left a conspicuous morphologic imprint. Unlike the West-Antarctic-<span class="hlt">ice</span> streams, which discharge <span class="hlt">ice</span> from an <span class="hlt">ice</span> sheet, <span class="hlt">ice</span> in the martian channels came from water erupting from the ground. In the cold martian environment, this water, if of moderate volume, would eventually freeze. Thus it may have formed <span class="hlt">icings</span> on springs, <span class="hlt">ice</span> dams and jams on constrictions in the channel path, or frozen pools. Given sufficient thickness and downhill surface gradient, these <span class="hlt">ice</span> <span class="hlt">masses</span> would have moved; and given the right conditions, they could have moved like Antarctic <span class="hlt">ice</span> streams.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/20020695-arctic-sea-ice-variability-context-recent-atmospheric-circulation-trends','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/20020695-arctic-sea-ice-variability-context-recent-atmospheric-circulation-trends"><span>Arctic sea <span class="hlt">ice</span> variability in the context of recent atmospheric circulation trends</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Deser, C.; Walsh, J.E.; Timlin, M.S.</p> <p></p> <p>Sea <span class="hlt">ice</span> is a sensitive component of the climate system, influenced by conditions in both the atmosphere and ocean. <span class="hlt">Variations</span> in sea <span class="hlt">ice</span> may in turn modulate climate by altering the surface albedo; the exchange of heat, moisture, and momentum between the atmosphere and ocean; and the upper ocean stratification in areas of deep water formation. The surface albedo effect is considered to be one of the dominant factors in the poleward amplification of global warming due to increased greenhouse gas concentrations simulated in many climate models. Forty years (1958--97) of reanalysis products and corresponding sea <span class="hlt">ice</span> concentration data aremore » used to document Arctic sea <span class="hlt">ice</span> variability and its association with surface air temperature (SAT) and sea level pressure (SLP) throughout the Northern Hemisphere extratropics. The dominant mode of winter (January-March) sea <span class="hlt">ice</span> variability exhibits out-of-phase fluctuations between the western and eastern North Atlantic, together with a weaker dipole in the North Pacific. The time series of this mode has a high winter-to-winter autocorrelation (0.69) and is dominated by decadal-scale <span class="hlt">variations</span> and a longer-term trend of diminishing <span class="hlt">ice</span> cover east of Greenland and increasing <span class="hlt">ice</span> cover west of Greenland. Associated with the dominant pattern of winter sea <span class="hlt">ice</span> variability are large-scale changes in SAT and SLP that closely resemble the North Atlantic oscillation. The associated SAT and surface sensible and latent heat flux anomalies are largest over the portions of the marginal sea <span class="hlt">ice</span> zone in which the trends of <span class="hlt">ice</span> coverage have been greatest, although the well-documented warming of the northern continental regions is also apparent. the temporal and spatial relationships between the SLP and <span class="hlt">ice</span> anomaly fields are consistent with the notion that atmospheric circulation anomalies force the sea <span class="hlt">ice</span> <span class="hlt">variations</span>. However, there appears to be a local response of the atmospheric circulation to the changing sea <span class="hlt">ice</span> <span class="hlt">variations</span>. However</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.C41A0440W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.C41A0440W"><span>Cosmogenic 10Be Depth Profile in top 560 m of West Antarctic <span class="hlt">Ice</span> Sheet Divide <span class="hlt">Ice</span> Core</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Welten, K. C.; Woodruff, T. E.; Caffee, M. W.; Edwards, R.; McConnell, J. R.; Bisiaux, M. M.; Nishiizumi, K.</p> <p>2009-12-01</p> <p>Concentrations of cosmogenic 10Be in polar <span class="hlt">ice</span> samples are a function of <span class="hlt">variations</span> in solar activity, geomagnetic field strength, atmospheric mixing and annual snow accumulation rates. The 10Be depth profile in <span class="hlt">ice</span> cores also provides independent chronological markers to tie Antarctic to Greenland <span class="hlt">ice</span> cores and to tie Holocene <span class="hlt">ice</span> cores to the 14C dendrochronology record. We measured 10Be concentrations in 187 samples from depths of 0-560 m of the main WAIS Divide core, WDC06A. The <span class="hlt">ice</span> samples are typically 1-2 kg and represent 2-4 m of <span class="hlt">ice</span>, equivalent to an average temporal resolution of ~12 years, based on the preliminary age-depth scale proposed for the WDC core, (McConnell et al., in prep). Be, Al and Cl were separated using ion exchange chromatography techniques and the 10Be concentrations were measured by accelerator <span class="hlt">mass</span> spectrometry (AMS) at PRIME lab. The 10Be concentrations range from 8.1 to 19.1 x 10^3 at/g, yielding an average of (13.1±2.1) x 10^3 at/g. Adopting an average snow accumulation rate of 20.9 cm weq/yr, as derived from the age-depth scale, this value corresponds to an average 10Be flux of (2.7±0.5) x 10^5 atoms/yr/cm2. This flux is similar to that of the Holocene part of the Siple Dome (Nishiizumi and Finkel, 2007) and Dome Fuji (Horiuchi et al. 2008) <span class="hlt">ice</span> cores, but ~30% lower than the value of 4.0 x 10^5 atoms/yr/cm2 for GISP2 (Finkel and Nishiizumi, 1997). The periods of low solar activity, known as Oort, Wolf, Spörer, Maunder and Dalton minima, show ~20% higher 10Be concentrations/fluxes than the periods of average solar activity in the last millennium. The maximum 10Be fluxes during some of these periods of low solar activity are up to ~50% higher than average 10Be fluxes, as seen in other polar <span class="hlt">ice</span> cores, which makes these peaks suitable as chronologic markers. We will compare the 10Be record in the WAIS Divide <span class="hlt">ice</span> core with that in other Antarctic as well as Greenland <span class="hlt">ice</span> cores and with the 14C treering record. Acknowledgment. This</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1986QuRes..26....3D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1986QuRes..26....3D"><span>Global <span class="hlt">ice</span>-sheet system interlocked by sea level</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Denton, George H.; Hughes, Terence J.; Karlén, Wibjörn</p> <p>1986-07-01</p> <p>Denton and Hughes (1983, Quaternary Research20, 125-144) postulated that sea level linked a global <span class="hlt">ice</span>-sheet system with both terrestrial and grounded marine components during late Quaternary <span class="hlt">ice</span> ages. Summer temperature changes near Northern Hemisphere melting margins initiated sea-level fluctuations that controlled marine components in both polar hemispheres. It was further proposed that <span class="hlt">variations</span> of this <span class="hlt">ice</span>-sheet system amplified and transmitted Milankovitch summer half-year insolation changes between 45 and 75°N into global climatic changes. New tests of this hypothesis implicate sea level as a major control of the areal extent of grounded portions of the Antarctic <span class="hlt">Ice</span> Sheet, thus fitting the concept of a globally interlocked <span class="hlt">ice</span>-sheet system. But recent atmospheric modeling results ( Manabe and Broccoli, 1985, Journal of Geophysical Research90, 2167-2190) suggest that factors other than areal changes of the grounded Antarctic <span class="hlt">Ice</span> Sheet strongly influenced Southern Hemisphere climate and terminated the last <span class="hlt">ice</span> age simultaneously in both polar hemispheres. Atmospheric carbon dioxide linked to high-latitude oceans is the most likely candidate ( Shackleton and Pisias, 1985, Atmospheric carbon dioxide, orbital forcing, and climate. In "The Carbon Cycle and Atmospheric CO 2: Natural <span class="hlt">Variations</span> Archean to Present" (E. T. Sundquest and W. S. Broecker, Eds.), pp. 303-318. Geophysical Monograph 32, American Geophysical Union, Washington, D.C.), but another potential influence was high-frequency climatic oscillations (2500 yr). It is postulated that <span class="hlt">variations</span> in atmospheric carbon dioxide acted through an Antarctic <span class="hlt">ice</span> shelf linked to the grounded <span class="hlt">ice</span> sheet to produce and terminate Southern Hemisphere <span class="hlt">ice</span>-age climate. It is further postulated that Milankovitch summer insolation combined with a warm high-frequency oscillation caused marked recession of Northern Hemisphere <span class="hlt">ice</span>-sheet melting margins and the North Atlantic polar front about 14,000 14C yr B.P. This</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170003145','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170003145"><span>Antarctic Sea-<span class="hlt">Ice</span> Freeboard and Estimated Thickness from NASA's ICESat and <span class="hlt">Ice</span>Bridge Observations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Yi, Donghui; Kurtz, Nathan; Harbeck, Jeremy; Manizade, Serdar; Hofton, Michelle; Cornejo, Helen G.; Zwally, H. Jay; Robbins, John</p> <p>2016-01-01</p> <p>ICESat completed 18 observational campaigns during its lifetime from 2003 to 2009. Data from all of the 18 campaign periods are used in this study. Most of the operational periods were between 34 and 38 days long. Because of laser failure and orbit transition from 8-day to 91-day orbit, there were four periods lasting 57, 16, 23, and 12 days. <span class="hlt">Ice</span>Bridge data from 2009, 2010, and 2011 are used in this study. Since 2009, there are 19 Airborne Topographic Mapper (ATM) campaigns, and eight Land, Vegetation, and <span class="hlt">Ice</span> Sensor (LVIS) campaigns over the Antarctic sea <span class="hlt">ice</span>. Freeboard heights are derived from ICESat, ATM and LVIS elevation and waveform data. With nominal densities of snow, water, and sea <span class="hlt">ice</span>, combined with snow depth data from AMSR-E/AMSR2 passive microwave observation over the southern ocean, sea-<span class="hlt">ice</span> thickness is derived from the freeboard. Combined with AMSR-E/AMSR2 <span class="hlt">ice</span> concentration, sea-<span class="hlt">ice</span> area and volume are also calculated. During the 2003-2009 period, sea-<span class="hlt">ice</span> freeboard and thickness distributions show clear seasonal <span class="hlt">variations</span> that reflect the yearly cycle of the growth and decay of the Antarctic pack <span class="hlt">ice</span>. We found no significant trend of thickness or area for the Antarctic sea <span class="hlt">ice</span> during the ICESat period. <span class="hlt">Ice</span>Bridge sea <span class="hlt">ice</span> freeboard and thickness data from 2009 to 2011 over the Weddell Sea and Amundsen and Bellingshausen Seas are compared with the ICESat results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007JGRC..11211013D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007JGRC..11211013D"><span>Influence of sea <span class="hlt">ice</span> cover and icebergs on circulation and water <span class="hlt">mass</span> formation in a numerical circulation model of the Ross Sea, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dinniman, Michael S.; Klinck, John M.; Smith, Walker O.</p> <p>2007-11-01</p> <p>Satellite imagery shows that there was substantial variability in the sea <span class="hlt">ice</span> extent in the Ross Sea during 2001-2003. Much of this variability is thought to be due to several large icebergs that moved through the area during that period. The effects of these changes in sea <span class="hlt">ice</span> on circulation and water <span class="hlt">mass</span> distributions are investigated with a numerical general circulation model. It would be difficult to simulate the highly variable sea <span class="hlt">ice</span> from 2001 to 2003 with a dynamic sea <span class="hlt">ice</span> model since much of the variability was due to the floating icebergs. Here, sea <span class="hlt">ice</span> concentration is specified from satellite observations. To examine the effects of changes in sea <span class="hlt">ice</span> due to iceberg C-19, simulations were performed using either climatological <span class="hlt">ice</span> concentrations or the observed <span class="hlt">ice</span> for that period. The heat balance around the Ross Sea Polynya (RSP) shows that the dominant term in the surface heat budget is the net exchange with the atmosphere, but advection of oceanic warm water is also important. The area average annual basal melt rate beneath the Ross <span class="hlt">Ice</span> Shelf is reduced by 12% in the observed sea <span class="hlt">ice</span> simulation. The observed sea <span class="hlt">ice</span> simulation also creates more High-Salinity Shelf Water. Another simulation was performed with observed sea <span class="hlt">ice</span> and a fixed iceberg representing B-15A. There is reduced advection of warm surface water during summer from the RSP into McMurdo Sound due to B-15A, but a much stronger reduction is due to the late opening of the RSP in early 2003 because of C-19.</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><span class="hlt">Mass</span> 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 zones 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://www.dtic.mil/docs/citations/AD1013710','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1013710"><span><span class="hlt">Mass</span> 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>2015-09-30</p> <p>1) Determination of the net growth and melt of multiyear (MY) sea <span class="hlt">ice</span> during its transit through the southern Beaufort Sea 2) Identification of...which we refer to as the FGIV dataset. Analysis of melt processes from <span class="hlt">ice</span> core and IMB data (Eicken) Through stratigraphic analysis of sea <span class="hlt">ice</span>...samples that are brought back to shore were melted and used to determine profiles of salinity and stable isotope ratios. These data allow us to identify</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.G11A0909M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.G11A0909M"><span>Using aerogravity and seismic data to model the bathymetry and upper crustal structure beneath the Pine Island Glacier <span class="hlt">ice</span> shelf, West Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Muto, A.; Peters, L. E.; Anandakrishnan, S.; Alley, R. B.; Riverman, K. L.</p> <p>2013-12-01</p> <p>Recent estimates indicate that <span class="hlt">ice</span> shelves along the Amundsen Sea coast in West Antarctica are losing substantial <span class="hlt">mass</span> through sub-<span class="hlt">ice</span>-shelf melting and contributing to the accelerating <span class="hlt">mass</span> loss of the grounded <span class="hlt">ice</span> buttressed by them. For Pine Island Glacier (PIG), relatively warm Circumpolar Deep Water has been identified as the key driver of the sub-<span class="hlt">ice</span>-shelf melting although poor constraints on PIG sub-<span class="hlt">ice</span> shelf have restricted thorough understanding of these <span class="hlt">ice</span>-ocean interactions. Aerogravity data from NASA's Operation <span class="hlt">Ice</span>Bridge (OIB) have been useful in identifying large-scale (on the order of ten kilometers) features but the results have relatively large uncertainties due to the inherent non-uniqueness of the gravity inversion. Seismic methods offer the most direct means of providing water thickness and upper crustal geological constraints, but availability of such data sets over the PIG <span class="hlt">ice</span> shelf has been limited due to logistical constraints. Here we present a comparative analysis of the bathymetry and upper crustal structure beneath the <span class="hlt">ice</span> shelf of PIG through joint inversion of OIB aerogravity data and in situ active-source seismic measurements collected in the 2012-13 austral summer. Preliminary results indicate improved resolution of the ocean cavity, particularly in the interior and sides of the PIG <span class="hlt">ice</span> shelf, and sedimentary drape across the region. Seismically derived <span class="hlt">variations</span> in <span class="hlt">ice</span> and ocean water densities are also applied to the gravity inversion to produce a more robust model of PIG sub-<span class="hlt">ice</span> shelf structure, as opposed to commonly used single <span class="hlt">ice</span> and water densities across the entire study region. Misfits between the seismically-constrained gravity inversion and that estimated previously from aerogravity alone provide insights on the sensitivity of gravity measurements to model perturbations and highlight the limitations of employing gravity data to model <span class="hlt">ice</span> shelf environments when no other sub-<span class="hlt">ice</span> constraints are available.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GMD....11.1257N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GMD....11.1257N"><span>Intercomparison of Antarctic <span class="hlt">ice</span>-shelf, ocean, and sea-<span class="hlt">ice</span> interactions simulated by MetROMS-iceshelf and FESOM 1.4</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Naughten, Kaitlin A.; Meissner, Katrin J.; Galton-Fenzi, Benjamin K.; England, Matthew H.; Timmermann, Ralph; Hellmer, Hartmut H.; Hattermann, Tore; Debernard, Jens B.</p> <p>2018-04-01</p> <p>An increasing number of Southern Ocean models now include Antarctic <span class="hlt">ice</span>-shelf cavities, and simulate thermodynamics at the <span class="hlt">ice</span>-shelf/ocean interface. This adds another level of complexity to Southern Ocean simulations, as <span class="hlt">ice</span> shelves interact directly with the ocean and indirectly with sea <span class="hlt">ice</span>. Here, we present the first model intercomparison and evaluation of present-day ocean/sea-<span class="hlt">ice/ice</span>-shelf interactions, as simulated by two models: a circumpolar Antarctic configuration of MetROMS (ROMS: Regional Ocean Modelling System coupled to CICE: Community <span class="hlt">Ice</span> CodE) and the global model FESOM (Finite Element Sea-<span class="hlt">ice</span> Ocean Model), where the latter is run at two different levels of horizontal resolution. From a circumpolar Antarctic perspective, we compare and evaluate simulated <span class="hlt">ice</span>-shelf basal melting and sub-<span class="hlt">ice</span>-shelf circulation, as well as sea-<span class="hlt">ice</span> properties and Southern Ocean water <span class="hlt">mass</span> characteristics as they influence the sub-<span class="hlt">ice</span>-shelf processes. Despite their differing numerical methods, the two models produce broadly similar results and share similar biases in many cases. Both models reproduce many key features of observations but struggle to reproduce others, such as the high melt rates observed in the small warm-cavity <span class="hlt">ice</span> shelves of the Amundsen and Bellingshausen seas. Several differences in model design show a particular influence on the simulations. For example, FESOM's greater topographic smoothing can alter the geometry of some <span class="hlt">ice</span>-shelf cavities enough to affect their melt rates; this improves at higher resolution, since less smoothing is required. In the interior Southern Ocean, the vertical coordinate system affects the degree of water <span class="hlt">mass</span> erosion due to spurious diapycnal mixing, with MetROMS' terrain-following coordinate leading to more erosion than FESOM's z coordinate. Finally, increased horizontal resolution in FESOM leads to higher basal melt rates for small <span class="hlt">ice</span> shelves, through a combination of stronger circulation and small-scale intrusions of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008epsc.conf..238K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008epsc.conf..238K"><span>Peculiarities of the Bound Water and Water <span class="hlt">Ice</span> Seasonal <span class="hlt">Variations</span> in the Martian Surface Layer of the Regolith.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kuzmin, R. O.; Zabalueva, E. V.; Evdokimova, N. A.; Christensen, P. H.; Mitrofanov, I. G.; Litvak, M. L.</p> <p>2008-09-01</p> <p>Introduction: The processes of the hydration/ dehydration of salt minerals within the Martian soil and the condensation/sublimation of water <span class="hlt">ice</span> (and frost) in the surficial soil layer and on the polar cap surface play great significance in the modern water cycle on Mars and directly affect the redistribution of the water phases and forms in the system "atmosphere/regolith/polar caps" [1, 2, 3, 4, 5]. The processes are reversible in time and their intensity is strongly dependent on such time-variable climatic parameters as atmospheric and surface temperature, atmospheric water vapour content and specific features of atmospheric seasonal circulation [6, 7, 8, 9, 10]. In the work we report the study results of the seasonal <span class="hlt">variations</span> of the chemically bound water (BW) spectral signature (based on the TES and OMEGA data), estimation and mapping of the winterand spring-time water <span class="hlt">ice</span> increase within the Martian surface soil (based on the TES and HEND data). Analysis and results: Regional and global mapping of the BW spectral index distribution as function of the seasons was conducted by using of the 6.1 μm emission pick from the TES dataset and the 1.91 μm absorption band from reflectance spectra of the OMEGA data. The study of the seasonal redistribution of the water <span class="hlt">ice</span> (and frost) within the thin surficial soil layer was conducted based on the TES thermal inertia (TI) data and the HEND neutrons flux mapping data. Bound water mapping: The mapping of the TES 6.1 μm BW index distributions was conducted at the time steps from 30° to 60° of Ls [11]. The mapping results show remarkable changes of the BW index values from one season to other one at notable latitudinal dependence of the index (Fig.1). At that, the higher BW index values are disposed mostly within the peripheral zone near the edge of the perennial and seasonal polar caps (cooler, wetter areas), while the lower BW index values are observed at low latitudes (warmer, drier areas). Between the Nspring (Ls=0</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008epsc.conf..259K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008epsc.conf..259K"><span>Peculiarities of the Bound Water and Water <span class="hlt">Ice</span> Seasonal <span class="hlt">Variations</span> in the Martian Surface Layer of the Regolith.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kuzmin, R. O.; Zabalueva, E. V.; Evdokimova, N. A.; Christensen, P. H.; Mitrofanov, I. G.; Litvak, M. L.</p> <p>2008-09-01</p> <p>Introduction: The processes of the hydration/ dehydration of salt minerals within the Martian soil and the condensation/sublimation of water <span class="hlt">ice</span> (and frost) in the surficial soil layer and on the polar cap surface play great significance in the modern water cycle on Mars and directly affect the redistribution of the water phases and forms in the system "atmosphere/regolith/polar caps" [1, 2, 3, 4, 5]. The processes are reversible in time and their intensity is strongly dependent on such time-variable climatic parameters as atmospheric and surface temperature, atmospheric water vapour content and specific features of atmospheric seasonal circulation [6, 7, 8, 9, 10]. In the work we report the study results of the seasonal <span class="hlt">variations</span> of the chemically bound water (BW) spectral signature (based on the TES and OMEGA data), estimation and mapping of the winterand spring-time water <span class="hlt">ice</span> increase within the Martian surface soil (based on the TES and HEND data). Analysis and results: Regional and global mapping of the BW spectral index distribution as function of the seasons was conducted by using of the 6.1 μm emission pick from the TES dataset and the 1.91 μm absorption band from reflectance spectra of the OMEGA data. The study of the seasonal redistribution of the water <span class="hlt">ice</span> (and frost) within the thin surficial soil layer was conducted based on the TES thermal inertia (TI) data and the HEND neutrons flux mapping data. Bound water mapping: The mapping of the TES 6.1 μm BW index distributions was conducted at the time steps from 30° to 60° of Ls [11]. The mapping results show remarkable changes of the BW index values from one season to other one at notable latitudinal dependence of the index (Fig.1). At that, the higher BW index values are disposed mostly within the peripheral zone near the edge of the perennial and seasonal polar caps (cooler, wetter areas), while the lower BW index values are observed at low latitudes (warmer, drier areas). Between the Nspring (Ls=0</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/14749827','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/14749827"><span>Enhanced <span class="hlt">ice</span> sheet growth in Eurasia owing to adjacent <span class="hlt">ice</span>-dammed lakes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Krinner, G; Mangerud, J; Jakobsson, M; Crucifix, M; Ritz, C; Svendsen, J I</p> <p>2004-01-29</p> <p>Large proglacial lakes cool regional summer climate because of their large heat capacity, and have been shown to modify precipitation through mesoscale atmospheric feedbacks, as in the case of Lake Agassiz. Several large <span class="hlt">ice</span>-dammed lakes, with a combined area twice that of the Caspian Sea, were formed in northern Eurasia about 90,000 years ago, during the last glacial period when an <span class="hlt">ice</span> sheet centred over the Barents and Kara seas blocked the large northbound Russian rivers. Here we present high-resolution simulations with an atmospheric general circulation model that explicitly simulates the surface <span class="hlt">mass</span> balance of the <span class="hlt">ice</span> sheet. We show that the main influence of the Eurasian proglacial lakes was a significant reduction of <span class="hlt">ice</span> sheet melting at the southern margin of the Barents-Kara <span class="hlt">ice</span> sheet through strong regional summer cooling over large parts of Russia. In our simulations, the summer melt reduction clearly outweighs lake-induced decreases in moisture and hence snowfall, such as has been reported earlier for Lake Agassiz. We conclude that the summer cooling mechanism from proglacial lakes accelerated <span class="hlt">ice</span> sheet growth and delayed <span class="hlt">ice</span> sheet decay in Eurasia and probably also in North America.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014GeoRL..41.2411S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014GeoRL..41.2411S"><span>Predicting September sea <span class="hlt">ice</span>: Ensemble skill of the SEARCH Sea <span class="hlt">Ice</span> Outlook 2008-2013</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stroeve, Julienne; Hamilton, Lawrence C.; Bitz, Cecilia M.; Blanchard-Wrigglesworth, Edward</p> <p>2014-04-01</p> <p>Since 2008, the Study of Environmental Arctic Change Sea <span class="hlt">Ice</span> Outlook has solicited predictions of September sea-<span class="hlt">ice</span> extent from the Arctic research community. Individuals and teams employ a variety of modeling, statistical, and heuristic approaches to make these predictions. Viewed as monthly ensembles each with one or two dozen individual predictions, they display a bimodal pattern of success. In years when observed <span class="hlt">ice</span> extent is near its trend, the median predictions tend to be accurate. In years when the observed extent is anomalous, the median and most individual predictions are less accurate. Statistical analysis suggests that year-to-year variability, rather than methods, dominate the <span class="hlt">variation</span> in ensemble prediction success. Furthermore, ensemble predictions do not improve as the season evolves. We consider the role of initial <span class="hlt">ice</span>, atmosphere and ocean conditions, and summer storms and weather in contributing to the challenge of sea-<span class="hlt">ice</span> prediction.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_23 --> <div id="page_24" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="461"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/655432-heavy-metals-antarctic-ice-from-law-dome-initial-results','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/655432-heavy-metals-antarctic-ice-from-law-dome-initial-results"><span>Heavy metals in Antarctic <span class="hlt">ice</span> from Law Dome: Initial results</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>Hong, S.; Boutron, C.F.; Edwards, R.</p> <p>1998-08-01</p> <p>Pb, Cd, Cu, and Zn have been measured using ultraclean procedures in eight sections taken from two well-dated <span class="hlt">ice</span> cores from Law Dome, an independent small size <span class="hlt">ice</span> cap with high accumulation rate situated in the coastal area of East Antarctica. Seven sections were dated from the 1830s to 1940s and one was dated from three millennia ago. The data show that there are strong seasonal <span class="hlt">variations</span> in the concentrations of Pb and Cd, with values {approximately} two- to four-fold higher in winter than in spring-summer. Evaluation of the contributions from the different sources suggests that contribution from sea saltmore » spray is relatively important, especially for Cd. Contribution from marine biogenic emissions could also be very significant. The importance of marine contributions is consistent with strong intrusions of marine air <span class="hlt">masses</span> at this coastal site, especially during wintertime.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3995117','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3995117"><span>Effects of Extreme Obliquity <span class="hlt">Variations</span> on the Habitability of Exoplanets</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Barnes, R.; Domagal-Goldman, S.; Breiner, J.; Quinn, T.R.; Meadows, V.S.</p> <p>2014-01-01</p> <p>Abstract We explore the impact of obliquity <span class="hlt">variations</span> on planetary habitability in hypothetical systems with high mutual inclination. We show that large-amplitude, high-frequency obliquity oscillations on Earth-like exoplanets can suppress the <span class="hlt">ice</span>-albedo feedback, increasing the outer edge of the habitable zone. We restricted our exploration to hypothetical systems consisting of a solar-<span class="hlt">mass</span> star, an Earth-<span class="hlt">mass</span> planet at 1 AU, and 1 or 2 larger planets. We verified that these systems are stable for 108 years with N-body simulations and calculated the obliquity <span class="hlt">variations</span> induced by the orbital evolution of the Earth-<span class="hlt">mass</span> planet and a torque from the host star. We ran a simplified energy balance model on the terrestrial planet to assess surface temperature and <span class="hlt">ice</span> coverage on the planet's surface, and we calculated differences in the outer edge of the habitable zone for planets with rapid obliquity <span class="hlt">variations</span>. For each hypothetical system, we calculated the outer edge of habitability for two conditions: (1) the full evolution of the planetary spin and orbit and (2) the eccentricity and obliquity fixed at their average values. We recovered previous results that higher values of fixed obliquity and eccentricity expand the habitable zone, but we also found that obliquity oscillations further expand habitable orbits in all cases. Terrestrial planets near the outer edge of the habitable zone may be more likely to support life in systems that induce rapid obliquity oscillations as opposed to fixed-spin planets. Such planets may be the easiest to directly characterize with space-borne telescopes. Key Words: Exoplanets—Habitable zone—Energy balance models. Astrobiology 14, 277–291. PMID:24611714</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.G13B1098S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.G13B1098S"><span>An integrated approach for estimating global glacio isostatic adjustment, land <span class="hlt">ice</span>, hydrology and ocean <span class="hlt">mass</span> trends within a complete coupled Earth system framework</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schumacher, M.; Bamber, J. L.; Martin, A.</p> <p>2016-12-01</p> <p>Future sea level rise (SLR) is one of the most serious consequences of climate change. Therefore, understanding the drivers of past sea level change is crucial for improving predictions. SLR integrates many Earth system components including oceans, land <span class="hlt">ice</span>, terrestrial water storage, as well as solid Earth effects. Traditionally, each component have been tackled separately, which has often lead to inconsistencies between discipline-specific estimates of each part of the sea level budget. To address these issues, the European Research Council has funded a five year project aimed at producing a physically-based, data-driven solution for the complete coupled land-ocean-solid Earth system that is consistent with the full suite of observations, prior knowledge and fundamental geophysical constraints. The project is called "Global<span class="hlt">Mass</span>" and based at University of Bristol. Observed <span class="hlt">mass</span> movement from the GRACE mission plus vertical land motion from a global network of permanent GPS stations will be utilized in a data-driven approach to estimate glacial isostatic adjustment (GIA) without introducing any assumptions about the Earth structure or <span class="hlt">ice</span> loading history. A Bayesian Hierarchical Model (BHM) will be used as the framework to combine the satellite and in-situ observations alongside prior information that incorporates the physics of the coupled system such as conservation of <span class="hlt">mass</span> and characteristic length scales of different processes in both space and time. The BHM is used to implement a simultaneous solution at a global scale. It will produce a consistent partitioning of the integrated SLR signal into its steric (thermal) and barystatic (<span class="hlt">mass</span>) component for the satellite era. The latter component is induced by hydrological <span class="hlt">mass</span> trends and melting of land <span class="hlt">ice</span>. The BHM was developed and tested on Antarctica, where it has been used to separate surface, <span class="hlt">ice</span> dynamic and GIA signals simultaneously. We illustrate the approach and concepts with examples from this test case</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSHE21A..03O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSHE21A..03O"><span>Quantifying the Evolution of Melt Ponds in the Marginal <span class="hlt">Ice</span> Zone Using High Resolution Optical Imagery and Neural Networks</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ortiz, M.; Pinales, J. C.; Graber, H. C.; Wilkinson, J.; Lund, B.</p> <p>2016-02-01</p> <p>Melt ponds on sea <span class="hlt">ice</span> play a significant and complex role on the thermodynamics in the Marginal <span class="hlt">Ice</span> Zone (MIZ). Ponding reduces the sea <span class="hlt">ice</span>'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 <span class="hlt">ice</span>, 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 <span class="hlt">Ice</span> Zone Program, including <span class="hlt">ice</span> <span class="hlt">mass</span>-balance buoys, arctic weather stations and wave buoys. The goal of the study is to capture the spatial <span class="hlt">variation</span> 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 <span class="hlt">variation</span> information of the imagery. We will compare the evolution of the melt ponds against several different array sites on the sea <span class="hlt">ice</span> to explore if there are spatial differences among the separated platforms in the MIZ.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.9551L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.9551L"><span>HAIC/HIWC field campaign - investigating <span class="hlt">ice</span> microphysics in high <span class="hlt">ice</span> water content regions of mesoscale convective systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Leroy, Delphine; Fontaine, Emmanuel; Schwarzenboeck, Alfons; Strapp, J. Walter; Lilie, Lyle; Dezitter, Fabien; Grandin, Alice</p> <p>2015-04-01</p> <p>Despite existing research programs focusing on tropical convection, high <span class="hlt">ice</span> water content (IWC) regions in Mesoscale Convective Systems (MCS) - potentially encountered by commercial aircraft and related to reported in-service events - remain poorly documented either because investigation of such high IWC regions was not of highest priority or because utilized instrumentation was not capable of providing accurate cloud microphysical measurements. To gather quantitative data in high IWC regions, a multi-year international HAIC/HIWC (High Altitude <span class="hlt">Ice</span> Crystals / High <span class="hlt">Ice</span> Water Content) field project has been designed including a first field campaign conducted out of Darwin (Australia) in 2014. The French Falcon 20 research aircraft had been equipped among others with a state-of-the-art in situ microphysics package including the IKP (isokinetic evaporator probe which provides a reference measurement of IWC and TWC), the CDP (cloud droplet spectrometer probe measuring particles in the range 2-50 µm), the 2D-S (2D-Stereo, 10-1280 µm) and PIP (precipitation imaging probe, 100-6400 µm) optical array probes. Microphysical data collection has been performed mainly at -40°C and -30°C levels, whereas little data could be sampled at -50°C and at -15C/-10°C. The study presented here focuses on <span class="hlt">ice</span> crystal size properties, thereby analyzing in detail the 2D image data from 2D-S and PIP optical array imaging probes. 2D images recorded with 2D-S and PIP were processed in order to extract a large variety of geometrical parameters, such as maximum diameter (Dmax), 2D surface equivalent diameter (Deq), and the corresponding number particle size distribution (PSD). Using the PSD information from both probes, a composite size distribution was then built, with sizes ranging from few tens of µm to roughly 10 mm. Finally, <span class="hlt">mass</span>-size relationships for <span class="hlt">ice</span> crystals in tropical convection were established in terms of power laws in order to compute median <span class="hlt">mass</span> diameters MMDmax and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19820036704&hterms=Parkinsons+circulation&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DParkinsons%2Bcirculation','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19820036704&hterms=Parkinsons+circulation&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DParkinsons%2Bcirculation"><span>Large-scale <span class="hlt">variations</span> in observed Antarctic Sea <span class="hlt">ice</span> extent and associated atmospheric circulation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cavalieri, D. J.; Parkinson, C. L.</p> <p>1981-01-01</p> <p>The 1974 Antarctic large scale sea <span class="hlt">ice</span> extent is studied from data from Nimbus 2 and 5 and temperature and sea level pressure fields from the Australian Meteorological Data Set. Electrically Scanning Microwave Radiometer data were three-day averaged and compared with 1000 mbar atmospheric pressure and sea level pressure data, also in three-day averages. Each three-day period was subjected to a Fourier analysis and included the mean latitude of the <span class="hlt">ice</span> extent and the phases and percent variances in terms of the first six Fourier harmonics. Centers of low pressure were found to be generally east of regions which displayed rapid <span class="hlt">ice</span> growth, and winds acted to extend the <span class="hlt">ice</span> equatorward. An atmospheric response was also noted as caused by the changing <span class="hlt">ice</span> cover.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ApJ...841...28P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ApJ...841...28P"><span>Further Constraints on <span class="hlt">Variations</span> in the Initial <span class="hlt">Mass</span> Function from Low-<span class="hlt">mass</span> X-ray Binary Populations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Peacock, Mark B.; Zepf, Stephen E.; Kundu, Arunav; Maccarone, Thomas J.; Lehmer, Bret D.; Maraston, Claudia; Gonzalez, Anthony H.; Eufrasio, Rafael T.; Coulter, David A.</p> <p>2017-05-01</p> <p>We present constraints on <span class="hlt">variations</span> in the initial <span class="hlt">mass</span> function (IMF) of nine local early-type galaxies based on their low-<span class="hlt">mass</span> X-ray binary (LMXB) populations. Comprised of accreting black holes and neutron stars, these LMXBs can be used to constrain the important high-<span class="hlt">mass</span> end of the IMF. We consider LMXB populations beyond the cores of the galaxies (>0.2R e; covering 75%-90% of their stellar light) and find no evidence for systematic <span class="hlt">variations</span> of the IMF with velocity dispersion (σ). We reject IMFs which become increasingly bottom-heavy with σ, up to steep power laws (exponent, α > 2.8) in massive galaxies (σ > 300 {km} {{{s}}}-1), for galactocentric radii >1/4 R e. Previously proposed IMFs that become increasingly bottom-heavy with σ are consistent with these data if only the number of low-<span class="hlt">mass</span> stars (<0.5 M ⊙) varies. We note that our results are consistent with some recent work which proposes that extreme IMFs are only present in the central regions of these galaxies. We also consider IMFs that become increasingly top-heavy with σ, resulting in significantly more LMXBs. Such a model is consistent with these observations, but additional data are required to significantly distinguish between this and an invariant IMF. For six of these galaxies, we directly compare with published “IMF mismatch” parameters from the Atlas3D survey, α dyn. We find good agreement with the LMXB population if galaxies with higher α dyn have more top-heavy IMFs—although we caution that our sample is quite small. Future LMXB observations can provide further insights into the origin of α dyn <span class="hlt">variations</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5642703','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5642703"><span>Katabatic winds diminish precipitation contribution to the Antarctic <span class="hlt">ice</span> <span class="hlt">mass</span> balance</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Grazioli, Jacopo; Madeleine, Jean-Baptiste; Gallée, Hubert; Forbes, Richard M.; Genthon, Christophe; Krinner, Gerhard; Berne, Alexis</p> <p>2017-01-01</p> <p>Snowfall in Antarctica is a key term of the <span class="hlt">ice</span> sheet <span class="hlt">mass</span> budget that influences the sea level at global scale. Over the continental margins, persistent katabatic winds blow all year long and supply the lower troposphere with unsaturated air. We show that this dry air leads to significant low-level sublimation of snowfall. We found using unprecedented data collected over 1 year on the coast of Adélie Land and simulations from different atmospheric models that low-level sublimation accounts for a 17% reduction of total snowfall over the continent and up to 35% on the margins of East Antarctica, significantly affecting satellite-based estimations close to the ground. Our findings suggest that, as climate warming progresses, this process will be enhanced and will limit expected precipitation increases at the ground level. PMID:28973875</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMPP52A..04A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMPP52A..04A"><span>How and when to terminate the Pleistocene <span class="hlt">ice</span> ages?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Abe-Ouchi, A.; Saito, F.; Kawamura, K.; Takahashi, K.; Raymo, M. E.; Okuno, J.; Blatter, H.</p> <p>2015-12-01</p> <p>Climate change with wax and wane of large Northern Hemisphere <span class="hlt">ice</span> sheet occurred in the past 800 thousand years characterized by 100 thousand year cycle with a large amplitude of sawtooth pattern, following a transition from a period of 40 thousand years cycle with small amplitude of <span class="hlt">ice</span> sheet change at about 1 million years ago. Although the importance of insolation as the ultimate driver is now appreciated, the mechanism what determines timing and strength of terminations are far from clearly understood. Here we show, using comprehensive climate and <span class="hlt">ice</span>-sheet models, that insolation and internal feedbacks between the climate, the <span class="hlt">ice</span> sheets and the lithosphere-asthenosphere system explain the 100,000-year periodicity. The responses of equilibrium states of <span class="hlt">ice</span> sheets to summer insolation show hysteresis, with the shape and position of the hysteresis loop playing a key part in determining the periodicities of glacial cycles. The hysteresis loop of the North American <span class="hlt">ice</span> sheet is such that after inception of the <span class="hlt">ice</span> sheet, its <span class="hlt">mass</span> balance remains mostly positive through several precession cycles, whose amplitudes decrease towards an eccentricity minimum. The larger the <span class="hlt">ice</span> sheet grows and extends towards lower latitudes, the smaller is the insolation required to make the <span class="hlt">mass</span> balance negative. Therefore, once a large <span class="hlt">ice</span> sheet is established, a moderate increase in insolation is sufficient to trigger a negative <span class="hlt">mass</span> balance, leading to an almost complete retreat of the <span class="hlt">ice</span> sheet within several thousand years. We discuss further the mechanism which determine the timing of <span class="hlt">ice</span> age terminations by examining the role of astronomical forcing and change of atmospheric carbon dioxide contents through sensitivity experiments and comparison of several <span class="hlt">ice</span> age cycles with different settings of astronomical forcings.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..4411878S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..4411878S"><span>The Response of <span class="hlt">Ice</span> Sheets to Climate Variability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Snow, K.; Goldberg, D. N.; Holland, P. R.; Jordan, J. R.; Arthern, R. J.; Jenkins, A.</p> <p>2017-12-01</p> <p>West Antarctic <span class="hlt">Ice</span> Sheet loss is a significant contributor to sea level rise. While the <span class="hlt">ice</span> loss is thought to be triggered by fluctuations in oceanic heat at the <span class="hlt">ice</span> shelf bases, <span class="hlt">ice</span> sheet response to ocean variability remains poorly understood. Using a synchronously coupled <span class="hlt">ice</span>-ocean model permitting grounding line migration, this study evaluates the response of an <span class="hlt">ice</span> sheet to periodic <span class="hlt">variations</span> in ocean forcing. Resulting oscillations in grounded <span class="hlt">ice</span> volume amplitude is shown to grow as a nonlinear function of ocean forcing period. This implies that slower oscillations in climatic forcing are disproportionately important to <span class="hlt">ice</span> sheets. The <span class="hlt">ice</span> shelf residence time offers a critical time scale, above which the <span class="hlt">ice</span> response amplitude is a linear function of ocean forcing period and below which it is quadratic. These results highlight the sensitivity of West Antarctic <span class="hlt">ice</span> streams to perturbations in heat fluxes occurring at decadal time scales.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009QSRv...28.3101G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009QSRv...28.3101G"><span>Reconstructing the last Irish <span class="hlt">Ice</span> Sheet 2: a geomorphologically-driven model of <span class="hlt">ice</span> sheet growth, retreat and dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Greenwood, Sarah L.; Clark, Chris D.</p> <p>2009-12-01</p> <p>The <span class="hlt">ice</span> sheet that once covered Ireland has a long history of investigation. Much prior work focussed on localised evidence-based reconstructions and <span class="hlt">ice</span>-marginal dynamics and chronologies, with less attention paid to an <span class="hlt">ice</span> sheet wide view of the first order properties of the <span class="hlt">ice</span> sheet: centres of <span class="hlt">mass</span>, <span class="hlt">ice</span> divide structure, <span class="hlt">ice</span> flow geometry and behaviour and changes thereof. In this paper we focus on the latter aspect and use our new, countrywide glacial geomorphological mapping of the Irish landscape (>39 000 landforms), and our analysis of the palaeo-glaciological significance of observed landform assemblages (article Part 1), to build an <span class="hlt">ice</span> sheet reconstruction yielding these fundamental <span class="hlt">ice</span> sheet properties. We present a seven stage model of <span class="hlt">ice</span> sheet evolution, from initiation to demise, in the form of palaeo-geographic maps. An early incursion of <span class="hlt">ice</span> from Scotland likely coalesced with local <span class="hlt">ice</span> caps and spread in a south-westerly direction 200 km across Ireland. A semi-independent Irish <span class="hlt">Ice</span> Sheet was then established during <span class="hlt">ice</span> sheet growth, with a branching <span class="hlt">ice</span> divide structure whose main axis migrated up to 140 km from the west coast towards the east. <span class="hlt">Ice</span> stream systems converging on Donegal Bay in the west and funnelling through the North Channel and Irish Sea Basin in the east emerge as major flow components of the maximum stages of glaciation. <span class="hlt">Ice</span> cover is reconstructed as extending to the continental shelf break. The Irish <span class="hlt">Ice</span> Sheet became autonomous (i.e. separate from the British <span class="hlt">Ice</span> Sheet) during deglaciation and fragmented into multiple <span class="hlt">ice</span> <span class="hlt">masses</span>, each decaying towards the west. Final sites of demise were likely over the mountains of Donegal, Leitrim and Connemara. Patterns of growth and decay of the <span class="hlt">ice</span> sheet are shown to be radically different: asynchronous and asymmetric in both spatial and temporal domains. We implicate collapse of the <span class="hlt">ice</span> stream system in the North Channel - Irish Sea Basin in driving such asymmetry, since rapid</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990064613&hterms=Parkinsons&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DParkinsons','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990064613&hterms=Parkinsons&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DParkinsons"><span>Variability of Arctic Sea <span class="hlt">Ice</span> as Determined from Satellite Observations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parkinson, Claire L.</p> <p>1999-01-01</p> <p>The compiled, quality-controlled satellite multichannel passive-microwave record of polar sea <span class="hlt">ice</span> now spans over 18 years, from November 1978 through December 1996, and is revealing considerable information about the Arctic sea <span class="hlt">ice</span> cover and its variability. The information includes data on <span class="hlt">ice</span> concentrations (percent areal coverages of <span class="hlt">ice</span>), <span class="hlt">ice</span> extents, <span class="hlt">ice</span> melt, <span class="hlt">ice</span> velocities, the seasonal cycle of the <span class="hlt">ice</span>, the interannual variability of the <span class="hlt">ice</span>, the frequency of <span class="hlt">ice</span> coverage, and the length of the sea <span class="hlt">ice</span> season. The data reveal marked regional and interannual variabilities, as well as some statistically significant trends. For the north polar <span class="hlt">ice</span> cover as a whole, maximum <span class="hlt">ice</span> extents varied over a range of 14,700,000 - 15,900,000 sq km, while individual regions experienced much greater percent <span class="hlt">variations</span>, for instance, with the Greenland Sea having a range of 740,000 - 1,110,000 sq km in its yearly maximum <span class="hlt">ice</span> coverage. In spite of the large <span class="hlt">variations</span> from year to year and region to region, overall the Arctic <span class="hlt">ice</span> extents showed a statistically significant, 2.80% / decade negative trend over the 18.2-year period. <span class="hlt">Ice</span> season lengths, which vary from only a few weeks near the <span class="hlt">ice</span> margins to the full year in the large region of perennial <span class="hlt">ice</span> coverage, also experienced interannual variability, along with spatially coherent overall trends. Linear least squares trends show the sea <span class="hlt">ice</span> season to have lengthened in much of the Bering Sea, Baffin Bay, the Davis Strait, and the Labrador Sea, but to have shortened over a much larger area, including the Sea of Okhotsk, the Greenland Sea, the Barents Sea, and the southeastern Arctic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19295607','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19295607"><span>Obliquity-paced Pliocene West Antarctic <span class="hlt">ice</span> sheet oscillations.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Naish, T; Powell, R; Levy, R; Wilson, G; Scherer, R; Talarico, F; Krissek, L; Niessen, F; Pompilio, M; Wilson, T; Carter, L; DeConto, R; Huybers, P; McKay, R; Pollard, D; Ross, J; Winter, D; Barrett, P; Browne, G; Cody, R; Cowan, E; Crampton, J; Dunbar, G; Dunbar, N; Florindo, F; Gebhardt, C; Graham, I; Hannah, M; Hansaraj, D; Harwood, D; Helling, D; Henrys, S; Hinnov, L; Kuhn, G; Kyle, P; Läufer, A; Maffioli, P; Magens, D; Mandernack, K; McIntosh, W; Millan, C; Morin, R; Ohneiser, C; Paulsen, T; Persico, D; Raine, I; Reed, J; Riesselman, C; Sagnotti, L; Schmitt, D; Sjunneskog, C; Strong, P; Taviani, M; Vogel, S; Wilch, T; Williams, T</p> <p>2009-03-19</p> <p>Thirty years after oxygen isotope records from microfossils deposited in ocean sediments confirmed the hypothesis that <span class="hlt">variations</span> in the Earth's orbital geometry control the <span class="hlt">ice</span> ages, fundamental questions remain over the response of the Antarctic <span class="hlt">ice</span> sheets to orbital cycles. Furthermore, an understanding of the behaviour of the marine-based West Antarctic <span class="hlt">ice</span> sheet (WAIS) during the 'warmer-than-present' early-Pliocene epoch ( approximately 5-3 Myr ago) is needed to better constrain the possible range of <span class="hlt">ice</span>-sheet behaviour in the context of future global warming. Here we present a marine glacial record from the upper 600 m of the AND-1B sediment core recovered from beneath the northwest part of the Ross <span class="hlt">ice</span> shelf by the ANDRILL programme and demonstrate well-dated, approximately 40-kyr cyclic <span class="hlt">variations</span> in <span class="hlt">ice</span>-sheet extent linked to cycles in insolation influenced by changes in the Earth's axial tilt (obliquity) during the Pliocene. Our data provide direct evidence for orbitally induced oscillations in the WAIS, which periodically collapsed, resulting in a switch from grounded <span class="hlt">ice</span>, or <span class="hlt">ice</span> shelves, to open waters in the Ross embayment when planetary temperatures were up to approximately 3 degrees C warmer than today and atmospheric CO(2) concentration was as high as approximately 400 p.p.m.v. (refs 5, 6). The evidence is consistent with a new <span class="hlt">ice-sheet/ice</span>-shelf model that simulates fluctuations in Antarctic <span class="hlt">ice</span> volume of up to +7 m in equivalent sea level associated with the loss of the WAIS and up to +3 m in equivalent sea level from the East Antarctic <span class="hlt">ice</span> sheet, in response to ocean-induced melting paced by obliquity. During interglacial times, diatomaceous sediments indicate high surface-water productivity, minimal summer sea <span class="hlt">ice</span> and air temperatures above freezing, suggesting an additional influence of surface melt under conditions of elevated CO(2).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.P31A2077L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.P31A2077L"><span>Insights Into <span class="hlt">Ice</span>-Ocean Interactions on Earth and Europa</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lawrence, J.; Schmidt, B. E.; Winslow, L.; Doran, P. T.; Kim, S.; Walker, C. C.; Buffo, J.; Skidmore, M. L.; Soderlund, K. M.; Blankenship, D. D.; Bramall, N. E.; Johnson, A.; Rack, F. R.; Stone, W.; Kimball, P.; Clark, E.</p> <p>2016-12-01</p> <p>Europa and Earth appear to be drastically different worlds, yet below their icy crusts the two likely share similar oceanic conditions including temperatures, pressures (relatively), and salinity. Earth's <span class="hlt">ice</span> shelves provide an important analog for the physiochemical, and potentially microbial, characteristics of icy worlds. NASA's ASTEP program funded Sub-<span class="hlt">Ice</span> Marine and PLanetary-analog Ecosystems (SIMPLE) to help address the fundamental processes occurring at <span class="hlt">ice</span> ocean interfaces, the extent and limitations of life in sub-<span class="hlt">ice</span> environments, and how environmental properties and biological communities interact. The relationships between currents, temperature, and salinity with physical processes such as melt, freeze, and marine <span class="hlt">ice</span> accretion at the basal surfaces of <span class="hlt">ice</span> shelves influence habitability yet are poorly understood even on Earth. Resultant processes such as the inclusion of ocean-derived material in <span class="hlt">ice</span> shelves and the transport of biotics from the interface towards the surface via ablation, convection, and diapirism also have important astrobiological implications for Europa.Here, we present results from CTD and imaging data gathered at multiple locations beneath the McMurdo <span class="hlt">Ice</span> Shelf (MIS) to highlight how the <span class="hlt">ice</span> and ocean interact in a Europan analog environment. Over the course of three years, the SIMPLE team observed heterogeneity in the water column and basal <span class="hlt">ice</span> beneath the MIS. During the recent 2015 field season we deployed ARTEMIS, an AUV capable of characterizing the interface over multiple kilometer missions, and conducted daily CTD casts to 480 m (bottom depth 529 m) in November adjacent to the terminus of the MIS to capture temporal <span class="hlt">variation</span> in the water column. These casts show the presence of transient water <span class="hlt">masses</span> related to the tidal period, each containing a single or double temperature minimum (down to -1.97 °C from -1.93 °C) between 60 to 150 m depth. Further comparisons between years and sampling locations demonstrate the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70027302','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70027302"><span>DEM, tide and velocity over sulzberger <span class="hlt">ice</span> shelf, West Antarctica</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Baek, S.; Shum, C.K.; Lee, H.; Yi, Y.; Kwoun, Oh-Ig; Lu, Z.; Braun, Andreas</p> <p>2005-01-01</p> <p>Arctic and Antarctic <span class="hlt">ice</span> sheets preserve more than 77% of the global fresh water and could raise global sea level by several meters if completely melted. Ocean tides near and under <span class="hlt">ice</span> shelves shifts the grounding line position significantly and are one of current limitations to study glacier dynamics and <span class="hlt">mass</span> balance. The Sulzberger <span class="hlt">ice</span> shelf is an area of <span class="hlt">ice</span> <span class="hlt">mass</span> flux change in West Antarctica and has not yet been well studied. In this study, we use repeat-pass synthetic aperture radar (SAR) interferometry data from the ERS-1 and ERS-2 tandem missions for generation of a high-resolution (60-m) Digital Elevation Model (DEM) including tidal deformation detection and <span class="hlt">ice</span> stream velocity of the Sulzberger <span class="hlt">Ice</span> Shelf. Other satellite data such as laser altimeter measurements with fine foot-prints (70-m) from NASA's ICESat are used for validation and analyses. The resulting DEM has an accuracy of-0.57??5.88 m and is demonstrated to be useful for grounding line detection and <span class="hlt">ice</span> <span class="hlt">mass</span> balance studies. The deformation observed by InSAR is found to be primarily due to ocean tides and atmospheric pressure. The 2-D <span class="hlt">ice</span> stream velocities computed agree qualitatively with previous methods on part of the <span class="hlt">Ice</span> Shelf from passive microwave remote-sensing data (i.e., LANDSAT). ?? 2005 IEEE.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28518108','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28518108"><span>Identification of Plant <span class="hlt">Ice</span>-binding Proteins Through Assessment of <span class="hlt">Ice</span>-recrystallization Inhibition and Isolation Using <span class="hlt">Ice</span>-affinity Purification.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bredow, Melissa; Tomalty, Heather E; Walker, Virginia K</p> <p>2017-05-05</p> <p><span class="hlt">Ice</span>-binding proteins (IBPs) belong to a family of stress-induced proteins that are synthesized by certain organisms exposed to subzero temperatures. In plants, freeze damage occurs when extracellular <span class="hlt">ice</span> crystals grow, resulting in the rupture of plasma membranes and possible cell death. Adsorption of IBPs to <span class="hlt">ice</span> crystals restricts further growth by a process known as <span class="hlt">ice</span>-recrystallization inhibition (IRI), thereby reducing cellular damage. IBPs also demonstrate the ability to depress the freezing point of a solution below the equilibrium melting point, a property known as thermal hysteresis (TH) activity. These protective properties have raised interest in the identification of novel IBPs due to their potential use in industrial, medical and agricultural applications. This paper describes the identification of plant IBPs through 1) the induction and extraction of IBPs in plant tissue, 2) the screening of extracts for IRI activity, and 3) the isolation and purification of IBPs. Following the induction of IBPs by low temperature exposure, extracts are tested for IRI activity using a 'splat assay', which allows the observation of <span class="hlt">ice</span> crystal growth using a standard light microscope. This assay requires a low protein concentration and generates results that are quickly obtained and easily interpreted, providing an initial screen for <span class="hlt">ice</span> binding activity. IBPs can then be isolated from contaminating proteins by utilizing the property of IBPs to adsorb to <span class="hlt">ice</span>, through a technique called '<span class="hlt">ice</span>-affinity purification'. Using cell lysates collected from plant extracts, an <span class="hlt">ice</span> hemisphere can be slowly grown on a brass probe. This incorporates IBPs into the crystalline structure of the polycrystalline <span class="hlt">ice</span>. Requiring no a priori biochemical or structural knowledge of the IBP, this method allows for recovery of active protein. <span class="hlt">Ice</span>-purified protein fractions can be used for downstream applications including the identification of peptide sequences by <span class="hlt">mass</span> spectrometry and the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70028080','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70028080"><span>Satellite-derived, melt-season surface temperature of the Greenland <span class="hlt">Ice</span> Sheet (2000-2005) and its relationship to <span class="hlt">mass</span> balance</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hall, D.K.; Williams, R.S.; Casey, K.A.; DiGirolamo, N.E.; Wan, Z.</p> <p>2006-01-01</p> <p>Mean, clear-sky surface temperature of the Greenland <span class="hlt">Ice</span> Sheet was measured for each melt season from 2000 to 2005 using Moderate-Resolution Imaging Spectroradiometer (MODIS)–derived land-surface temperature (LST) data-product maps. During the period of most-active melt, the mean, clear-sky surface temperature of the <span class="hlt">ice</span> sheet was highest in 2002 (−8.29 ± 5.29°C) and 2005 (−8.29 ± 5.43°C), compared to a 6-year mean of −9.04 ± 5.59°C, in agreement with recent work by other investigators showing unusually extensive melt in 2002 and 2005. Surface-temperature variability shows a correspondence with the dry-snow facies of the <span class="hlt">ice</span> sheet; a reduction in area of the dry-snow facies would indicate a more-negative <span class="hlt">mass</span> balance. Surface-temperature variability generally increased during the study period and is most pronounced in the 2005 melt season; this is consistent with surface instability caused by air-temperature fluctuations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014TCry....8.2409L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014TCry....8.2409L"><span><span class="hlt">Ice</span> and AIS: ship speed data and sea <span class="hlt">ice</span> forecasts in the Baltic Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Löptien, U.; Axell, L.</p> <p>2014-12-01</p> <p>The Baltic Sea is a seasonally <span class="hlt">ice</span>-covered marginal sea located in a densely populated area in northern Europe. Severe sea <span class="hlt">ice</span> conditions have the potential to hinder the intense ship traffic considerably. Thus, sea <span class="hlt">ice</span> fore- and nowcasts are regularly provided by the national weather services. Typically, the forecast comprises several <span class="hlt">ice</span> properties that are distributed as prognostic variables, but their actual usefulness is difficult to measure, and the ship captains must determine their relative importance and relevance for optimal ship speed and safety ad hoc. The present study provides a more objective approach by comparing the ship speeds, obtained by the automatic identification system (AIS), with the respective forecasted <span class="hlt">ice</span> conditions. We find that, despite an unavoidable random component, this information is useful to constrain and rate fore- and nowcasts. More precisely, 62-67% of ship speed <span class="hlt">variations</span> can be explained by the forecasted <span class="hlt">ice</span> properties when fitting a mixed-effect model. This statistical fit is based on a test region in the Bothnian Sea during the severe winter 2011 and employs 15 to 25 min averages of ship speed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014TCD.....8.3811L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014TCD.....8.3811L"><span><span class="hlt">Ice</span> and AIS: ship speed data and sea <span class="hlt">ice</span> forecasts in the Baltic Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Löptien, U.; Axell, L.</p> <p>2014-07-01</p> <p>The Baltic Sea is a seasonally <span class="hlt">ice</span> covered marginal sea located in a densely populated area in northern Europe. Severe sea <span class="hlt">ice</span> conditions have the potential to hinder the intense ship traffic considerably. Thus, sea <span class="hlt">ice</span> fore- and nowcasts are regularly provided by the national weather services. Typically, several <span class="hlt">ice</span> properties are allocated, but their actual usefulness is difficult to measure and the ship captains must determine their relative importance and relevance for optimal ship speed and safety ad hoc. The present study provides a more objective approach by comparing the ship speeds, obtained by the Automatic Identification System (AIS), with the respective forecasted <span class="hlt">ice</span> conditions. We find that, despite an unavoidable random component, this information is useful to constrain and rate fore- and nowcasts. More precisely, 62-67% of ship speed <span class="hlt">variations</span> can be explained by the forecasted <span class="hlt">ice</span> properties when fitting a mixed effect model. This statistical fit is based on a test region in the Bothnian Bay during the severe winter 2011 and employes 15 to 25 min averages of ship speed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011MsT.........18M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011MsT.........18M"><span>Quantification of Changes for the Milne <span class="hlt">Ice</span> Shelf, Nunavut, Canada, 1950 -- 2009</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mortimer, Colleen Adel</p> <p></p> <p>This study presents a comprehensive overview of the current state of the Milne <span class="hlt">Ice</span> Shelf and how it has changed over the last 59 years. The 205 +/-1 km2 <span class="hlt">ice</span> shelf experienced a 28% (82 +/-0.8 km 2) reduction in area between 1950 -- 2009, and a 20% (2.5 +/-0.9km 3 water equivalent (w.e.)) reduction in volume between 1981 -- 2008/2009, suggesting a long-term state of negative <span class="hlt">mass</span> balance. Comparison of mean annual specific <span class="hlt">mass</span> balances (up to -0.34 m w.e. yr-1) with surface <span class="hlt">mass</span> balance measurements for the nearby Ward Hunt <span class="hlt">Ice</span> Shelf suggest that basal melt is a key contributor to total <span class="hlt">ice</span> shelf thinning. The development and expansion of new and existing surface cracks, as well as <span class="hlt">ice</span>-marginal and epishelf lake development, indicate significant <span class="hlt">ice</span> shelf weakening. Over the next few decades it is likely that the Milne <span class="hlt">Ice</span> Shelf will continue to deteriorate.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_24 --> <div id="page_25" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="481"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC43H1150W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC43H1150W"><span>Geoengineering 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>Wolovick, M.</p> <p>2017-12-01</p> <p><span class="hlt">Mass</span> loss from Greenland and Antarctica is highly sensitive to the presence of warm ocean water that drives melting at the grounding line. Rapid melting near the grounding line causes <span class="hlt">ice</span> shelf thinning, loss of buttressing, flow acceleration, grounding line retreat, and ultimately <span class="hlt">mass</span> loss and sea-level rise. If the grounding line enters a section of overdeepened bed the <span class="hlt">ice</span> sheet may even enter a runaway collapse via the marine <span class="hlt">ice</span> sheet instability. The warm water that triggers this process resides offshore at depth and accesses the grounding line through deep troughs in the continental shelf. In Greenland, warm water transport is further constricted through narrow fjords. Here, I propose blocking warm water transport through these choke points with an artificial sill. Using a simple width- and depth-averaged model of <span class="hlt">ice</span> stream flow coupled to a buoyant-plume model of ocean melting, I find that grounding line retreat and sea level rise can be delayed or reversed for hundreds of years if warm water is prevented from accessing the grounding line at depth. Blocking of warm water from the sub-<span class="hlt">ice</span> cavity causes <span class="hlt">ice</span> shelf thickening, increased buttressing, and grounding line readvance. The increase in buttressing is greatly magnified if the thickened <span class="hlt">ice</span> shelf regrounds on a bathymetric high or on the artificial sill itself. In some experiments for Thwaites Glacier the grounding line is able to recover from a severely retreated state over 100 km behind its present-day position. Such a dramatic recovery demonstrates that it is possible, at least in principle, to stop and reverse an ongoing marine <span class="hlt">ice</span> sheet collapse. If the <span class="hlt">ice</span> shelf regrounds on the artificial sill itself, erosion of the sill beneath the grounded <span class="hlt">ice</span> could reduce the effectiveness of the intervention. However, experiments including sill erosion suggest that even a very weak sill (1 kPa) could delay a collapse for centuries. The scale of the artificial sills in Greenlandic fjords is comparable to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AcMSn..31....1Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AcMSn..31....1Z"><span>Modeling ocean wave propagation under sea <span class="hlt">ice</span> covers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhao, Xin; Shen, Hayley H.; Cheng, Sukun</p> <p>2015-02-01</p> <p>Operational ocean wave models need to work globally, yet current ocean wave models can only treat <span class="hlt">ice</span>-covered regions crudely. The purpose of this paper is to provide a brief overview of <span class="hlt">ice</span> effects on wave propagation and different research methodology used in studying these effects. Based on its proximity to land or sea, sea <span class="hlt">ice</span> can be classified as: landfast <span class="hlt">ice</span> zone, shear zone, and the marginal <span class="hlt">ice</span> zone. All <span class="hlt">ice</span> covers attenuate wave energy. Only long swells can penetrate deep into an <span class="hlt">ice</span> cover. Being closest to open water, wave propagation in the marginal <span class="hlt">ice</span> zone is the most complex to model. The physical appearance of sea <span class="hlt">ice</span> in the marginal <span class="hlt">ice</span> zone varies. Grease <span class="hlt">ice</span>, pancake <span class="hlt">ice</span>, brash <span class="hlt">ice</span>, floe aggregates, and continuous <span class="hlt">ice</span> sheet may be found in this zone at different times and locations. These types of <span class="hlt">ice</span> are formed under different thermal-mechanical forcing. There are three classic models that describe wave propagation through an idealized <span class="hlt">ice</span> cover: <span class="hlt">mass</span> loading, thin elastic plate, and viscous layer models. From physical arguments we may conjecture that <span class="hlt">mass</span> loading model is suitable for disjoint aggregates of <span class="hlt">ice</span> floes much smaller than the wavelength, thin elastic plate model is suitable for a continuous <span class="hlt">ice</span> sheet, and the viscous layer model is suitable for grease <span class="hlt">ice</span>. For different sea <span class="hlt">ice</span> types we may need different wave <span class="hlt">ice</span> interaction models. A recently proposed viscoelastic model is able to synthesize all three classic models into one. Under suitable limiting conditions it converges to the three previous models. The complete theoretical framework for evaluating wave propagation through various <span class="hlt">ice</span> covers need to be implemented in the operational ocean wave models. In this review, we introduce the sea <span class="hlt">ice</span> types, previous wave <span class="hlt">ice</span> interaction models, wave attenuation mechanisms, the methods to calculate wave reflection and transmission between different <span class="hlt">ice</span> covers, and the effect of <span class="hlt">ice</span> floe breaking on shaping the sea <span class="hlt">ice</span> morphology</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26PSL.481..316M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26PSL.481..316M"><span>Precipitation regime influence on oxygen triple-isotope distributions in Antarctic precipitation and <span class="hlt">ice</span> cores</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Miller, Martin F.</p> <p>2018-01-01</p> <p>The relative abundance of 17O in meteoric precipitation is usually reported in terms of the 17O-excess parameter. <span class="hlt">Variations</span> of 17O-excess in Antarctic precipitation and <span class="hlt">ice</span> cores have hitherto been attributed to normalised relative humidity changes at the moisture source region, or to the influence of a temperature-dependent supersaturation-controlled kinetic isotope effect during in-cloud <span class="hlt">ice</span> formation below -20 °C. Neither mechanism, however, satisfactorily explains the large range of 17O-excess values reported from measurements. A different approach, based on the regression characteristics of 103 ln (1 +δ17 O) versus 103 ln (1 +δ18 O), is applied here to previously published isotopic data sets. The analysis indicates that clear-sky precipitation ('diamond dust'), which occurs widely in inland Antarctica, is characterised by an unusual relative abundance of 17O, distinct from that associated with cloud-derived, synoptic snowfall. Furthermore, this distinction appears to be largely preserved in the <span class="hlt">ice</span> core record. The respective <span class="hlt">mass</span> contributions to snowfall accumulation - on both temporal and spatial scales - provides the basis of a simple, first-order explanation for the observed oxygen triple-isotope ratio <span class="hlt">variations</span> in Antarctic precipitation, surface snow and <span class="hlt">ice</span> cores. Using this approach, it is shown that precipitation during the last major deglaciation, both in western Antarctica at the West Antarctic <span class="hlt">Ice</span> Sheet (WAIS) Divide and at Vostok on the eastern Antarctic plateau, consisted essentially of diamond dust only, despite a large temperature differential (and thus different water vapour supersaturation conditions) at the two locations. In contrast, synoptic snowfall events dominate the accumulation record throughout the Holocene at both sites.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFMPP33B1558D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFMPP33B1558D"><span>Large <span class="hlt">Variations</span> in <span class="hlt">Ice</span> Volume During the Middle Eocene "Doubthouse"</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dawber, C. F.; Tripati, A. K.</p> <p>2008-12-01</p> <p>The onset of glacial conditions in the Cenozoic is widely held to have begun ~34 million years ago, coincident with the Eocene-Oligocene boundary1. Warm and high pCO2 'greenhouse' intervals such as the Eocene are generally thought to be <span class="hlt">ice</span>-free2. Yet the sequence stratigraphic record supports the occurrence of high-frequency sea-level change of tens of meters in the Middle and Late Eocene3, and large calcite and seawater δ18O excursions (~0.5-1.0 permil) have been reported in foraminifera from open ocean sediments4. As a result, the Middle Eocene is often considered the intermediary "doubthouse". The extent of continental <span class="hlt">ice</span> during the 'doubthouse' is controversial, with estimates of glacioeustatic sea level fall ranging from 30 to 125m2,3,5. We present a new δ18Osw reconstruction for Ocean Drilling Project (ODP) Site 1209 in the tropical Pacific Ocean. It is the first continuous high-resolution record for an open-ocean site that is not directly influenced by changes in the carbonate compensation depth, which enables us to circumvent many of the limitations of existing records. Our record shows increases of 0.8 ± 0.2 (1 s.e) permil and 1.1 ± 0.2 permil at ~44-45 and ~42-41 Ma respectively, which suggests glacioeustatic sea level <span class="hlt">variations</span> of ~90 m during the Middle Eocene. Modelling studies have shown that fully glaciating Antarctica during the Eocene should drive a change in seawater (δ18Osw) of 0.45 permil, and lower sea level by ~55 m6. Our results therefore support significant <span class="hlt">ice</span> storage in both the Northern and Southern Hemisphere during the Middle Eocene 'doubthouse'. 1.Miller, Kenneth G. et al., 1990, Eocene-Oligocene sea-level changes in the New Jersey coastal plain linked to the deep-sea record. Geological Society of America Bulletin 102, 331-339 2.Pagani, M. et al., 2005, Marked decline in atmospheric carbon dioxide concentrations during the Paleogene. Science 309 (5734), 600-603. 3.Browning, J., Miller, K., and Pak, D., 1996, Global implications</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> <span class="hlt">mass</span> 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> zone, was observed during two <span class="hlt">ice</span> stations with melt rates of up to 20 cm per 24 hours. To reinforce the local measurements around the ship and to confirm their significance on a larger scale, we compare them to airborne thickness measurements and classified SAR-satellite scenes. The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRF..122.2269K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRF..122.2269K"><span>Can Seismic Observations of Bed Conditions on <span class="hlt">Ice</span> Streams Help Constrain Parameters in <span class="hlt">Ice</span> Flow Models?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kyrke-Smith, Teresa M.; Gudmundsson, G. Hilmar; Farrell, Patrick E.</p> <p>2017-11-01</p> <p>We investigate correlations between seismically derived estimates of basal acoustic impedance and basal slipperiness values obtained from a surface-to-bed inversion using a Stokes <span class="hlt">ice</span> flow model. Using high-resolution measurements along several seismic profiles on Pine Island Glacier (PIG), we find no significant correlation at kilometer scale between acoustic impedance and either retrieved basal slipperiness or basal drag. However, there is a stronger correlation when comparing average values along the individual profiles. We hypothesize that the correlation appears at the length scales over which basal <span class="hlt">variations</span> are important to large-scale <span class="hlt">ice</span> sheet flow. Although the seismic technique is sensitive to the material properties of the bed, at present there is no clear way of incorporating high-resolution seismic measurements of bed properties on <span class="hlt">ice</span> streams into <span class="hlt">ice</span> flow models. We conclude that more theoretical work needs to be done before constraints on mechanical conditions at the <span class="hlt">ice</span>-bed interface from acoustic impedance measurements can be of direct use to <span class="hlt">ice</span> sheet models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20170002775&hterms=inversion&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dinversion','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20170002775&hterms=inversion&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dinversion"><span>Spatial and Temporal Antarctic <span class="hlt">Ice</span> Sheet <span class="hlt">Mass</span> Trends, Glacio-Isostatic Adjustment, and Surface Processes from a Joint Inversion of Satellite Altimeter, Gravity, and GPS Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Martin-Espanol, Alba; Zammit-Mangion, Andrew; Clarke, Peter J.; Flament, Thomas; Helm, Veit; King, Matt A.; Luthcke, Scott B.; Petrie, Elizabeth; Remy, Frederique; Schon, Nana; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20170002775'); toggleEditAbsImage('author_20170002775_show'); toggleEditAbsImage('author_20170002775_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20170002775_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20170002775_hide"></p> <p>2016-01-01</p> <p>We present spatiotemporal <span class="hlt">mass</span> balance trends for the Antarctic <span class="hlt">Ice</span> Sheet from a statistical inversion of satellite altimetry, gravimetry, and elastic-corrected GPS data for the period 2003-2013. Our method simultaneously determines annual trends in <span class="hlt">ice</span> dynamics, surface <span class="hlt">mass</span> balance anomalies, and a time-invariant solution for glacio-isostatic adjustment while remaining largely independent of forward models. We establish that over the period 2003-2013, Antarctica has been losing <span class="hlt">mass</span> at a rateof -84 +/- 22 Gt per yr, with a sustained negative mean trend of dynamic imbalance of -111 +/- 13 Gt per yr. West Antarctica is the largest contributor with -112 +/- 10 Gt per yr, mainly triggered by high thinning rates of glaciers draining into the Amundsen Sea Embayment. The Antarctic Peninsula has experienced a dramatic increase in <span class="hlt">mass</span> loss in the last decade, with a mean rate of -28 +/- 7 Gt per yr and significantly higher values for the most recent years following the destabilization of the Southern Antarctic Peninsula around 2010. The total <span class="hlt">mass</span> loss is partly compensated by a significant <span class="hlt">mass</span> gain of 56 +/- 18 Gt per yr in East Antarctica due to a positive trend of surface <span class="hlt">mass</span> balance anomalies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C44A..03Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C44A..03Y"><span>Greenland <span class="hlt">ice</span> sheet beyond 2100: Simulating its evolution and influence using the coupled climate-<span class="hlt">ice</span> sheet model EC-Earth - PISM</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, S.; Christensen, J. H.; Madsen, M. S.; Ringgaard, I. M.; Petersen, R. A.; Langen, P. P.</p> <p>2017-12-01</p> <p>Greenland <span class="hlt">ice</span> sheet (GrIS) is observed undergoing a rapid change in the recent decades, with an increasing area of surface melting and ablation and a speeding <span class="hlt">mass</span> loss. Predicting the GrIS changes and their climate consequences relies on the understanding of the interaction of the GrIS with the climate system on both global and local scales, and requires climate model systems incorporating with an explicit and physically consistent <span class="hlt">ice</span> sheet module. In this work we study the GrIS evolution and its interaction with the climate system using a fully coupled global climate model with a dynamical <span class="hlt">ice</span> sheet model for the GrIS. The coupled model system, EC-EARTH - PISM, consisting of the atmosphere-ocean-sea <span class="hlt">ice</span> model system EC-EARTH, and the Parallel <span class="hlt">Ice</span> Sheet Model (PISM), has been employed for a 1400-year simulation forced by CMIP5 historical forcing from 1850 to 2005 and continued along an extended RCP8.5 scenario with the forcing peaking at 2200 and stabilized hereafter. The simulation reveals that, following the anthropogenic forcing increase, the global mean surface temperature rapidly rises about 10 °C in the 21st and 22nd century. After the forcing stops increasing after 2200, the temperature change slows down and eventually stabilizes at about 12.5 °C above the preindustrial level. In response to the climate warming, the GrIS starts losing <span class="hlt">mass</span> slowly in the 21st century, but the <span class="hlt">ice</span> retreat accelerates substantially after 2100 and <span class="hlt">ice</span> <span class="hlt">mass</span> loss continues hereafter at a constant rate of approximately 0.5 m sea level rise equivalence per 100 years, even as the warming rate gradually levels off. Ultimately the volume and extent of GrIS reduce to less than half of its preindustrial value. To understand the interaction of GrIS with the climate system, the characteristics of atmospheric and oceanic circulation in the warm climate are analyzed. The circulation patterns associated with the negative surface <span class="hlt">mass</span> balance that leads to GrIS retreat are investigated</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5687855','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5687855"><span>Should coastal planners have concern over where land <span class="hlt">ice</span> is melting?</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Larour, Eric; Ivins, Erik R.; Adhikari, Surendra</p> <p>2017-01-01</p> <p>There is a general consensus among Earth scientists that melting of land <span class="hlt">ice</span> greatly contributes to sea-level rise (SLR) and that future warming will exacerbate the risks posed to human civilization. As land <span class="hlt">ice</span> is lost to the oceans, both the Earth’s gravitational and rotational potentials are perturbed, resulting in strong spatial patterns in SLR, termed sea-level fingerprints. We lack robust forecasting models for future <span class="hlt">ice</span> changes, which diminishes our ability to use these fingerprints to accurately predict local sea-level (LSL) changes. We exploit an advanced mathematical property of adjoint systems and determine the exact gradient of sea-level fingerprints with respect to local <span class="hlt">variations</span> in the <span class="hlt">ice</span> thickness of all of the world’s <span class="hlt">ice</span> drainage systems. By exhaustively mapping these fingerprint gradients, we form a new diagnosis tool, henceforth referred to as gradient fingerprint mapping (GFM), that readily allows for improved assessments of future coastal inundation or emergence. We demonstrate that for Antarctica and Greenland, changes in the predictions of inundation at major port cities depend on the location of the drainage system. For example, in London, GFM shows LSL that is significantly affected by changes on the western part of the Greenland <span class="hlt">Ice</span> Sheet (GrIS), whereas in New York, LSL change predictions are greatly sensitive to changes in the northeastern portions of the GrIS. We apply GFM to 293 major port cities to allow coastal planners to readily calculate LSL change as more reliable predictions of cryospheric <span class="hlt">mass</span> changes become available. PMID:29152565</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.5738V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.5738V"><span>The Tweeting <span class="hlt">Ice</span> Shelf: geophysics and outreach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Van Liefferinge, Brice; Berger, Sophie; Drews, Reinhard; Pattyn, Frank</p> <p>2015-04-01</p> <p>Over the last decade the Antarctic and Greenland <span class="hlt">ice</span> sheets have contributed about one third of the annual sea level rise (Hanna et al., 2013). However, it remains difficult to reconcile global <span class="hlt">mass</span> balance estimates obtained from different satellite-based methods. A typical approach is to balance the <span class="hlt">mass</span> input from atmospheric modelling with the outgoing <span class="hlt">mass</span> flux at the <span class="hlt">ice</span>-sheet boundary (Shepherd et al., 2012). The flux calculations at the boundary rely on satellite-derived surface velocities, which are currently only available as snapshots in time, and which need ground truth for validation. Here, we report on continuous, year-round measurements that aim at improving the input-output method in several aspects and carefully map the flow speed allowing for detecting seasonal variability. For this purpose, we set up in December 2014 three stand-alone single-frequency GPSes on the Roi Baudouin <span class="hlt">ice</span> shelf (East Antarctica). The GPSes are installed across a surface depression (typical for large <span class="hlt">ice</span>-shelf channels), where subglacial melting is expected. This setup allows us to investigate how these channels behave, i.e., if they become wider, whether or not they enhance the <span class="hlt">ice</span> flow, and, in combination with an installed phase-sensitive radar, what amount of melting occurs below the channels in contact with the ocean. The GPS data are transmitted on a daily basis. <span class="hlt">Ice</span>-shelf velocity is derived from the raw hourly location following the methods described in den Ouden et al. (2010), Dunse et al. (2012), and Ahlstrøm et al. (2013). However, a reference station has not been used for the correction. Basic processing involves outliers removal, smoothing, time-series analysis and comparison with tidal models. The project comes alongside an outreach event: on a weekly basis, the <span class="hlt">ice</span> shelf 'tweets' its position, motion and relays other information with respect to the project. The GPS systems can be followed on Twitter via @Tweetin<span class="hlt">Ice</span>Shelf as well as the Tweeting <span class="hlt">Ice</span> Shelf</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002AGUFM.U72A0009M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002AGUFM.U72A0009M"><span>Recent Trends in the Arctic Navigable <span class="hlt">Ice</span> Season and Links to Atmospheric Circulation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Maslanik, J.; Drobot, S.</p> <p>2002-12-01</p> <p>One of the potential effects of Arctic climate warming is an increase in the navigable <span class="hlt">ice</span> season, perhaps resulting in development of the Arctic as a major shipping route. The distance from western North American ports to Europe through the Northwest Passage (NWP) or the Northern Sea Route (NSR) is typically 20 to 60 percent shorter than travel through the Panama Canal, while travel between Europe and the Far East may be reduced by as much as three weeks compared to transport through the Suez Canal. An increase in the navigable <span class="hlt">ice</span> season would also improve commercial opportunities within the Arctic region, such as mineral and oil exploration and tourism, which could potentially expand the economic base of Arctic residents and companies, but which would also have negative environmental impacts. Utilizing daily passive-microwave derived sea <span class="hlt">ice</span> concentrations, trends and variability in the Arctic navigable <span class="hlt">ice</span> season are examined from 1979 through 2001. Trend analyses suggest large increases in the length of the navigable <span class="hlt">ice</span> season in the Kara and Barents seas, the Sea of Okhotsk, and the Beaufort Sea, with decreases in the length of the navigable <span class="hlt">ice</span> season in the Bering Sea. Interannual <span class="hlt">variations</span> in the navigable <span class="hlt">ice</span> season largely are governed by fluctuations in low-frequency atmospheric circulation, although the specific annular modes affecting the length of the navigable <span class="hlt">ice</span> season vary by region. In the Beaufort and East Siberian seas, <span class="hlt">variations</span> in the North Atlantic Oscillation/Arctic Oscillation control the navigable <span class="hlt">ice</span> season, while <span class="hlt">variations</span> in the East Pacific anomaly play an important role in controlling the navigable <span class="hlt">ice</span> season in the Kara and Barents seas. In Hudson Bay, the Canadian Arctic Archipelago, and Baffin Bay, interannual <span class="hlt">variations</span> in the navigable <span class="hlt">ice</span> season are strongly related to the Pacific Decadal Oscillation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012JGRC..117.9031G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012JGRC..117.9031G"><span>Modeling the basal melting and marine <span class="hlt">ice</span> accretion of the Amery <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>Galton-Fenzi, B. K.; Hunter, J. R.; Coleman, R.; Marsland, S. J.; Warner, R. C.</p> <p>2012-09-01</p> <p>The basal <span class="hlt">mass</span> balance of the Amery <span class="hlt">Ice</span> Shelf (AIS) in East Antarctica is investigated using a numerical ocean model. The main improvements of this model over previous studies are the inclusion of frazil formation and dynamics, tides and the use of the latest estimate of the sub-<span class="hlt">ice</span>-shelf cavity geometry. The model produces a net basal melt rate of 45.6 Gt year-1 (0.74 m <span class="hlt">ice</span> year-1) which is in good agreement with reviewed observations. The melting at the base of the <span class="hlt">ice</span> shelf is primarily due to interaction with High Salinity Shelf Water created from the surface sea-<span class="hlt">ice</span> formation in winter. The temperature difference between the coldest waters created in the open ocean and the in situ freezing point of ocean water in contact with the deepest part of the AIS drives a melt rate that can exceed 30 m of <span class="hlt">ice</span> year-1. The inclusion of frazil dynamics is shown to be important for both melting and marine <span class="hlt">ice</span> accretion (refreezing). Frazil initially forms in the supercooled water layer adjacent to the base of the <span class="hlt">ice</span> shelf. The net accretion of marine <span class="hlt">ice</span> is 5.3 Gt year-1, comprised of 3.7 Gt year-1 of frazil accretion and 1.6 Gt year-1 of direct basal refreezing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018NewA...62...26K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018NewA...62...26K"><span>Effects of <span class="hlt">mass</span> <span class="hlt">variation</span> on structures of differentially rotating polytropic stars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kumar, Sunil; Saini, Seema; Singh, Kamal Krishan</p> <p>2018-07-01</p> <p>A method is proposed for determining equilibrium structures and various physical parameters of differentially rotating polytropic models of stars, taking into account the effect of <span class="hlt">mass</span> <span class="hlt">variation</span> inside the star and on its equipotential surfaces. The law of differential rotation has been assumed to be the form of ω2(s) =b1 +b2s2 +b3s4 . The proposed method utilizes the averaging approach of Kippenhahn and Thomas and concepts of Roche-equipotential to incorporate the effects of differential rotation on the equilibrium structures of polytropic stellar models. Mathematical expressions of determining the equipotential surfaces, volume, surface area and other physical parameters are also obtained under the effects of <span class="hlt">mass</span> <span class="hlt">variation</span> inside the stars. Some significant conclusions are also drawn.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C13F1017M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C13F1017M"><span>Atmospheric river impacts on Greenland <span class="hlt">Ice</span> Sheet surface melt and <span class="hlt">mass</span> balance</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mattingly, K.; Mote, T. L.</p> <p>2017-12-01</p> <p><span class="hlt">Mass</span> loss from the Greenland <span class="hlt">Ice</span> Sheet (GrIS) has accelerated during the early part of the 21st Century. Several episodes of widespread GrIS melt in recent years have coincided with intense poleward moisture transport by atmospheric rivers (ARs), suggesting that variability in the frequency and intensity of these events may be an important driver of the surface <span class="hlt">mass</span> balance (SMB) of the GrIS. ARs may contribute to GrIS surface melt through the greenhouse effect of water vapor, the radiative effects of clouds, condensational latent heating within poleward-advected air <span class="hlt">masses</span>, and the energy provided by liquid precipitation. However, ARs may also provide significant positive contributions to GrIS SMB through enhanced snow accumulation. Prior research on the role of ARs in Arctic climate has consisted of case studies of ARs associated with major GrIS melt events or examined the effects of poleward moisture flux on Arctic sea <span class="hlt">ice</span>. In this study, a long-term (1979-2016) record of intense moisture transport events affecting Greenland is compiled using a conventional AR identification algorithm as well as a self-organizing map (SOM) classification applied to integrated water vapor transport (IVT) data from several atmospheric reanalysis datasets. An analysis of AR effects on GrIS melt and SMB is then performed with GrIS surface melt data from passive microwave satellite observations and the Modèle Atmosphérique Régional (MAR) regional climate model. Results show that meltwater production is above normal during and after AR impact days throughout the GrIS during all seasons, with surface melt enhanced most by strong (> 85th percentile IVT) and extreme (> 95th percentile IVT) ARs. This relationship holds at the seasonal scale, as the total amount of water vapor transported to the GrIS by ARs is significantly greater during above-normal melt seasons. ARs exert a more complex influence on SMB. Normal (< 85th percentile IVT) ARs generally do not have a substantial impact on</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23274717','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23274717"><span><span class="hlt">Mass</span> carbon monoxide poisoning at an <span class="hlt">ice</span>-hockey game: initial approach and long-term follow-up.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mortelmans, Luc J M; Populaire, Jacques; Desruelles, Didier; Sabbe, Marc B</p> <p>2013-12-01</p> <p>A <span class="hlt">mass</span> carbon monoxide (CO) intoxication during an <span class="hlt">ice</span>-hockey game is described. Two hundred and thirty-five patients were seen in different hospitals, 88 of them the same night at the nearby emergency department. To evaluate long-term implications and to identify relevant indicators, a follow-up study was organized 1 year after the incident. Apart from the file data from the emergency departments, a 1-year follow-up mailing was sent to all patients. One hundred and ninety-one patients returned their questionnaire (86%). The mean age of the patients was 28 years, with 61% men. The mean carboxyhaemoglobin (COHb) was 9.9%. COHb levels were significantly higher for individuals on the <span class="hlt">ice</span> (referee, players and maintenance personnel). There was a significant relationship with the initial presence of dizziness, fatigue and the COHb level. Headache, abdominal pain, nausea and vomiting were not significantly related to the COHb levels. The relationship between symptoms and CO level, however, should be interpreted with caution as there was a wide range between exposure and blood tests. 5.2% of patients had residual complaints, all including headache, with a significant higher incidence with high COHb levels. Only two patients had an abnormal neurological control (one slightly disturbed electroencephalography and one persistent encephalopathic complaint). Work incapacity was also significantly related to COHb levels. CO <span class="hlt">mass</span> poisonings remain a risk in indoor sporting events. Although it causes an acute <span class="hlt">mass</span> casualty incident, it is limited in time and delayed problems are scarce. Symptomatology is a poor tool for triage. The best prevention is the use of nonmineral energy sources such as for example electricity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910004108','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910004108"><span>A review of <span class="hlt">ice</span> accretion data from a model rotor <span class="hlt">icing</span> test and comparison with theory</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Britton, Randall K.; Bond, Thomas H.</p> <p>1991-01-01</p> <p>An experiment was conducted by the Helicopter <span class="hlt">Icing</span> Consortium (HIC) in the NASA Lewis <span class="hlt">Icing</span> Research Tunnel (IRT) in which a 1/6 scale fuselage model of a UH-60A Black Hawk helicopter with a generic rotor was subjected to a wide range of <span class="hlt">icing</span> conditions. The HIC consists of members from NASA, Bell Helicopter, Boeing Helicopter, McDonnell Douglas Helicopters, Sikorsky Aircraft, and Texas A&M University. Data was taken in the form of rotor torque, internal force balance measurements, blade strain gage loading, and two dimensional <span class="hlt">ice</span> shape tracings. A review of the <span class="hlt">ice</span> shape data is performed with special attention given to repeatability and correctness of trends in terms of radial <span class="hlt">variation</span>, rotational speed, <span class="hlt">icing</span> time, temperature, liquid water content, and volumetric median droplet size. Moreover, an indepth comparison between the experimental data and the analysis of NASA's <span class="hlt">ice</span> accretion code LEWICE is given. Finally, conclusions are drawn as to the quality of the <span class="hlt">ice</span> accretion data and the predictability of the data base as a whole. Recommendations are also given for improving data taking technique as well as potential future work.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19830034350&hterms=drainage+blocked&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Ddrainage%2Bblocked','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19830034350&hterms=drainage+blocked&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Ddrainage%2Bblocked"><span><span class="hlt">Ice</span> sculpture in the Martian outflow channels</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lucchitta, B. K.</p> <p>1982-01-01</p> <p>Viking Orbiter and terrestrial satellite images are examined at similar resolution to compare features of the Martian outflow channels with features produced by the movement of <span class="hlt">ice</span> on earth, and many resemblances are found. These include the anastomoses, sinuosities, and U-shaped cross profiles of valleys; hanging valleys; linear scour marks on valley walls; grooves and ridges on valley floors; and the streamlining of bedrock highs. Attention is given to the question whether <span class="hlt">ice</span> could have moved in the Martian environment. It is envisaged that springs or small catastrophic outbursts discharged fluids from structural outlets or chaotic terrains. These fluids built <span class="hlt">icings</span> that may have grown into substantial <span class="hlt">masses</span> and eventually flowed like glaciers down preexisting valleys. An alternative is that the fluids formed rivers or floods that in turn formed <span class="hlt">ice</span> jams and consolidated into icy <span class="hlt">masses</span> in places where obstacles blocked their flow.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20080018456&hterms=Secret&qs=N%3D0%26Ntk%3DTitle%26Ntx%3Dmode%2Bmatchall%26Ntt%3DThe%2BSecret','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20080018456&hterms=Secret&qs=N%3D0%26Ntk%3DTitle%26Ntx%3Dmode%2Bmatchall%26Ntt%3DThe%2BSecret"><span>The Secret of the Svalbard Sea <span class="hlt">Ice</span> Barrier</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nghiem, Son V.; Van Woert, Michael L.; Neumann, Gregory</p> <p>2004-01-01</p> <p>An elongated sea <span class="hlt">ice</span> feature called the Svalbard sea <span class="hlt">ice</span> barrier rapidly formed over an area in the Barents Sea to the east of Svalbard posing navigation hazards. The secret of its formation lies in the bottom bathymetry that governs the distribution of cold Arctic waters <span class="hlt">masses</span>, which impacts sea <span class="hlt">ice</span> growth on the water surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/990526-global-simulations-ice-nucleation-ice-supersaturation-improved-cloud-scheme-community-atmosphere-model','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/990526-global-simulations-ice-nucleation-ice-supersaturation-improved-cloud-scheme-community-atmosphere-model"><span>Global Simulations of <span class="hlt">Ice</span> nucleation and <span class="hlt">Ice</span> Supersaturation with an Improved Cloud Scheme in the Community Atmosphere Model</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Gettelman, A.; Liu, Xiaohong; Ghan, Steven J.</p> <p>2010-09-28</p> <p>A process-based treatment of <span class="hlt">ice</span> supersaturation and <span class="hlt">ice</span>-nucleation is implemented in the National Center for Atmospheric Research (NCAR) Community Atmosphere Model (CAM). The new scheme is designed to allow (1) supersaturation with respect to <span class="hlt">ice</span>, (2) <span class="hlt">ice</span> nucleation by aerosol particles and (3) <span class="hlt">ice</span> cloud cover consistent with <span class="hlt">ice</span> microphysics. The scheme is implemented with a 4-class 2 moment microphysics code and is used to evaluate <span class="hlt">ice</span> cloud nucleation mechanisms and supersaturation in CAM. The new model is able to reproduce field observations of <span class="hlt">ice</span> <span class="hlt">mass</span> and mixed phase cloud occurrence better than previous versions of the model. Simulations indicatemore » heterogeneous freezing and contact nucleation on dust are both potentially important over remote areas of the Arctic. Cloud forcing and hence climate is sensitive to different formulations of the <span class="hlt">ice</span> microphysics. Arctic radiative fluxes are sensitive to the parameterization of <span class="hlt">ice</span> clouds. These results indicate that <span class="hlt">ice</span> clouds are potentially an important part of understanding cloud forcing and potential cloud feedbacks, particularly in the Arctic.« less</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 <span class="hlt">mass</span> imbalance. Accurate knowledge of <span class="hlt">ice</span> shelf thickness is essential for input-output method <span class="hlt">mass</span> 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 zone 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 zone. 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> </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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