Sample records for ice sheet snow

  1. 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.

  2. Snow Grain Size Retrieval over the Polar Ice Sheets with the Ice, Cloud, and land Elevation Satellite (ICESat) Observations

    PubMed Central

    Yang, Yuekui; Marshak, Alexander; Han, Mei; Palm, Stephen P.; Harding, David J.

    2018-01-01

    Snow grain size is an important parameter for cryosphere studies. As a proof of concept, this paper presents an approach to retrieve this parameter over Greenland, East and West Antarctica ice sheets from surface reflectances observed with the Geoscience Laser Altimeter System (GLAS) onboard the Ice, Cloud, and land Elevation Satellite (ICESat) at 1064 nm. Spaceborne lidar observations overcome many of the disadvantages in passive remote sensing, including difficulties in cloud screening and low sun angle limitations; hence tend to provide more accurate and stable retrievals. Results from the GLAS L2A campaign, which began on 25 September and lasted until 19 November, 2003, show that the mode of the grain size distribution over Greenland is the largest (~300 μm) among the three, West Antarctica is the second (~220 μm) and East Antarctica is the smallest (~190 μm). Snow grain sizes are larger over the coastal regions compared to inland the ice sheets. These results are consistent with previous studies. Applying the broadband snow surface albedo parameterization scheme developed by Garder and Sharp (2010) to the retrieved snow grain size, ice sheet surface albedo is also derived. In the future, more accurate retrievals can be achieved with multiple wavelengths lidar observations. PMID:29636591

  3. Snow Grain Size Retrieval over the Polar Ice Sheets with the Ice, Cloud and Land Elevation Satellite (ICESat) Observations

    NASA Technical Reports Server (NTRS)

    Yang, Yuekui; Marshak, Alexander; Han, Mei; Palm, Stephen P.; Harding, David J.

    2016-01-01

    Snow grain size is an important parameter for cryosphere studies. As a proof of concept, this paper presents an approach to retrieve this parameter over Greenland, East and West Antarctica ice sheets from surface reflectances observed with the Geoscience Laser Altimeter System (GLAS) onboard the Ice, Cloud, and land Elevation Satellite (ICESat) at 1064 nanometers. Spaceborne lidar observations overcome many of the disadvantages in passive remote sensing, including difficulties in cloud screening and low sun angle limitations; hence tend to provide more accurate and stable retrievals. Results from the GLAS L2A campaign, which began on 25 September and lasted until 19 November, 2003, show that the mode of the grain size distribution over Greenland is the largest (approximately 300 microns) among the three, West Antarctica is the second (220 microns) and East Antarctica is the smallest (190 microns). Snow grain sizes are larger over the coastal regions compared to inland the ice sheets. These results are consistent with previous studies. Applying the broadband snow surface albedo parameterization scheme developed by Garder and Sharp (2010) to the retrieved snow grain size, ice sheet surface albedo is also derived. In the future, more accurate retrievals can be achieved with multiple wavelengths lidar observations.

  4. Radar backscattering from snow facies of the Greenland ice sheet: Results from the AIRSAR 1991 campaign

    NASA Technical Reports Server (NTRS)

    Rignot, Eric; Jezek, K.; Vanzyl, J. J.; Drinkwater, Mark R.; Lou, Y. L.

    1993-01-01

    In June 1991, the NASA/JPL airborne SAR (AIRSAR) acquired C- (lambda = 5.6cm), L- (lambda = 24cm), and P- (lambda = 68m) band polarimetric SAR data over the Greenland ice sheet. These data are processed using version 3.55 of the AIRSAR processor which provides radiometrically and polarimetrically calibrated images. The internal calibration of the AIRSAR data is cross-checked using the radar response from corner reflectors deployed prior to flight in one of the scenes. In addition, a quantitative assessment of the noise power level at various frequencies and polarizations is made in all the scenes. Synoptic SAR data corresponding to a swath width of about 12 by 50 km in length (compared to the standard 12 x 12 km size of high-resolution scenes) are also processed and calibrated to study transitions in radar backscatter as a function of snow facies at selected frequencies and polarizations. The snow facies on the Greenland ice sheet are traditionally categorized based on differences in melting regime during the summer months. The interior of Greenland corresponds to the dry snow zone where terrain elevation is the highest and no snow melt occurs. The lowest elevation boundary of the dry snow zone is known traditionally as the dry snow line. Beneath it is the percolation zone where melting occurs in the summer and water percolates through the snow freezing at depth to form massive ice lenses and ice pipes. At the downslope margin of this zone is the wet snow line. Below it, the wet snow zone corresponds to the lowest elevations where snow remains at the end of the summer. Ablation produces enough meltwater to create areas of snow saturated with water, together with ponds and lakes. The lowest altitude zone of ablation sees enough summer melt to remove all traces of seasonal snow accumulation, such that the surface comprises bare glacier ice.

  5. Ultra-Wideband Radiometry Remote Sensing of Polar Ice Sheet Temperature Profile, Sea Ice and Terrestrial Snow Thickness: Forward Modeling and Data Analysis

    NASA Astrophysics Data System (ADS)

    Tsang, L.; Tan, S.; Sanamzadeh, M.; Johnson, J. T.; Jezek, K. C.; Durand, M. T.

    2017-12-01

    The recent development of an ultra-wideband software defined radiometer (UWBRAD) operating over the unprotected spectrum of 0.5 2.0 GHz using radio-frequency interference suppression techniques offers new methodologies for remote sensing of the polar ice sheets, sea ice, and terrestrial snow. The instrument was initially designed for remote sensing of the intragalcial temperature profile of the ice sheet, where a frequency dependent penetration depth yields a frequency dependent brightness temperature (Tb) spectrum that can be linked back to the temperature profile of the ice sheet. The instrument was tested during a short flight over Northwest Greenland in September, 2016. Measurements were successfully made over the different snow facies characteristic of Greenland including the ablation, wet snow and percolation facies, and ended just west of Camp Century during the approach to the dry snow zone. Wide-band emission spectra collected during the flight have been processed and analyzed. Results show that the spectra are highly sensitive to the facies type with scattering from ice lenses being the dominant reason for low Tbs in the percolation zone. Inversion of Tb to physical temperature at depth was conducted on the measurements near Camp Century, achieving a -1.7K ten-meter error compared to borehole measurements. However, there is a relatively large uncertainty in the lower part possibly due to the large scattering near the surface. Wideband radiometry may also be applicable to sea ice and terrestrial snow thickness retrieval. Modeling studies suggest that the UWBRAD spectra reduce ambiguities inherent in other sea ice thickness retrievals by utilizing coherent wave interferences that appear in the Tb spectrum. When applied to a lossless medium such as terrestrial snow, this coherent oscillation turns out to be the single key signature that can be used to link back to snow thickness. In this paper, we report our forward modeling findings in support of instrument

  6. Unusual radar echoes from the Greenland ice sheet

    NASA Technical Reports Server (NTRS)

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

    1993-01-01

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

  7. [Psycrophilic organisms in snow and ice].

    PubMed

    Kohshima, S

    2000-12-01

    Psychrophilic and psycrotrophic organisms are important in global ecology as a large proportion of our planet is cold. Two-third of sea-water covering more than 70% of Earth is cold deep sea water with temperature around 2 degrees C, and more than 90% of freshwater is in polar ice-sheets and mountain glaciers. Though biological activity in snow and ice had been believed to be extremely limited, various specialized biotic communities were recently discovered at glaciers of various part of the world. The glacier is relatively simple and closed ecosystem with special biotic community containing various psychrophilic and psycrotrophic organisms. Since psychrophilic organisms was discovered in the deep ice-core recovered from the antarctic ice-sheet and a lake beneath it, snow and ice environments in Mars and Europa are attracting a great deal of scientific attention as possible extraterrestrial habitats of life. This paper briefly reviews the results of the studies on ecology of psychrophilic organisms living in snow and ice environments and their physiological and biochemical adaptation to low temperature.

  8. Snow and ice in a changing hydrological world.

    USGS Publications Warehouse

    Meier, M.F.

    1983-01-01

    Snow cover on land (especially in the Northern Hemisphere) and sea ice (especially in the Southern Hemisphere) vary seasonally, and this seasonal change has an important affect on the world climate because snow and sea ice reflect solar radiation efficiently and affect other heat flow processes between atmosphere and land or ocean. Glaciers, including ice sheets, store most of the fresh water on Earth, but change dimensions relatively slowly. There is no clear evidence that the glacier ice volume currently is declining, but more needs to be known about mountain glacier and ice sheet mass balances. -from Author

  9. 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.

  10. Recent increase in snow-melt area in the Greenland Ice sheet as an indicator of the effect of reduced surface albedo by snow impurities

    NASA Astrophysics Data System (ADS)

    Rikiishi, K.

    2008-12-01

    Recent rapid decline of cryosphere including mountain glaciers, sea ice, and seasonal snow cover tends to be associated with global warming. However, positive feedback is likely to operate between the cryosphere and air temperature, and then it may not be so simple to decide the cause-and-effect relation between them. The theory of heat budget for snow surface tells us that sensible heat transfer from the air to the snow by atmospheric warming by 1°C is about 10 W/m2, which is comparable with heat supply introduced by reduction of the snow surface albedo by only 0.02. Since snow impurities such as black carbon and soil- origin dusts have been accumulated every year on the snow surface in snow-melting season, it is very important to examine whether the snow-melting on the ice sheets, mountain glaciers, and sea ice is caused by global warming or by accumulated snow impurities originated from atmospheric pollutants. In this paper we analyze the dataset of snow-melt area in the Greenland ice sheet for the years 1979 - 2007 (available from the National Snow and Ice Data Center), which is reduced empirically from the satellite micro-wave observations by SMMR and SMM/I. It has been found that, seasonally, the snow-melt area extends most significantly from the second half of June to the first half of July when the sun is highest and sunshine duration is longest, while it doesn't extend any more from the second half of July to the first half of August when the air temperature is highest. This fact may imply that sensible heat required for snow-melting comes from the solar radiation rather than from the atmosphere. As for the interannual variation of snow-melt area, on the other hand, we have found that the growth rate of snow-melt area gradually increases from July, to August, and to the first half of September as the impurities come out to and accumulated at the snow surface. However, the growth rate is almost zero in June and the second half of September when fresh snow

  11. Remote Sensing of Terrestrial Snow and Ice for Global Change Studies

    NASA Technical Reports Server (NTRS)

    Kelly, Richard; Hall, Dorothy K.

    2007-01-01

    Snow and ice play a significant role in the Earth's water cycle and are sensitive and informative indicators climate change. Significant changes in terrestrial snow and ice water storage are forecast, and while evidence of large-scale changes is emerging, in situ measurements alone are insufficient to help us understand and explain these changes. Imaging remote sensing systems are capable of successfully observing snow and ice in the cryosphere. This chapter examines how those remote sensing sensors, that now have more than 35 years of observation records, are capable of providing information about snow cover, snow water equivalent, snow melt, ice sheet temperature and ice sheet albedo. While significant progress has been made, especially in the last five years, a better understanding is required of the records of satellite observations of these cryospheric variables.

  12. Continuous Estimates of Surface Density and Annual Snow Accumulation with Multi-Channel Snow/Firn Penetrating Radar in the Percolation Zone, Western Greenland Ice Sheet

    NASA Astrophysics Data System (ADS)

    Meehan, T.; Marshall, H. P.; Bradford, J.; Hawley, R. L.; Osterberg, E. C.; McCarthy, F.; Lewis, G.; Graeter, K.

    2017-12-01

    A priority of ice sheet surface mass balance (SMB) prediction is ascertaining the surface density and annual snow accumulation. These forcing data can be supplied into firn compaction models and used to tune Regional Climate Models (RCM). RCMs do not accurately capture subtle changes in the snow accumulation gradient. Additionally, leading RCMs disagree among each other and with accumulation studies in regions of the Greenland Ice Sheet (GrIS) over large distances and temporal scales. RCMs tend to yield inconsistencies over GrIS because of sparse and outdated validation data in the reanalysis pool. Greenland Traverse for Accumulation and Climate Studies (GreenTrACS) implemented multi-channel 500 MHz Radar in multi-offset configuration throughout two traverse campaigns totaling greater than 3500 km along the western percolation zone of GrIS. The multi-channel radar has the capability of continuously estimating snow depth, average density, and annual snow accumulation, expressed at 95% confidence (+-) 0.15 m, (+-) 17 kgm-3, (+-) 0.04 m w.e. respectively, by examination of the primary reflection return from the previous year's summer surface.

  13. Snow Accumulation Variability Over the West Antarctic Ice Sheet Since 1900: A Comparison of Ice Core Records With ERA-20C Reanalysis

    NASA Astrophysics Data System (ADS)

    Wang, Yetang; Thomas, Elizabeth R.; Hou, Shugui; Huai, Baojuan; Wu, Shuangye; Sun, Weijun; Qi, Shanzhong; Ding, Minghu; Zhang, Yulun

    2017-11-01

    This study uses a set of 37 firn core records over the West Antarctic Ice Sheet (WAIS) to test the performance of the twentieth century from the European Centre for Medium-Range Weather Forecasts (ERA-20C) reanalysis for snow accumulation and quantify temporal variability in snow accumulation since 1900. The firn cores are allocated to four geographical areas demarcated by drainage divides (i.e., Antarctic Peninsula (AP), western WAIS, central WAIS, and eastern WAIS) to calculate stacked records of regional snow accumulation. Our results show that the interannual variability in ERA-20C precipitation minus evaporation (P - E) agrees well with the corresponding ice core snow accumulation composites in each of the four geographical regions, suggesting its skill for simulating snow accumulation changes before the modern satellite era (pre-1979). Snow accumulation experiences significantly positive trends for the AP and eastern WAIS, a negative trend for the western WAIS, and no significant trend for the central WAIS from 1900 to 2010. The contrasting trends are associated with changes in the large-scale moisture transport driven by a deepening of the low-pressure systems and anomalies of sea ice in the Amundsen Sea Low region.

  14. Determining Greenland Ice Sheet Accumulation Rates from Radar Remote Sensing

    NASA Technical Reports Server (NTRS)

    Jezek, Kenneth C.

    2001-01-01

    An important component of NASA's Program for Arctic Regional Climate Assessment (PARCA) is a mass balance investigation of the Greenland Ice Sheet. The mass balance is calculated by taking the difference between the snow accumulation and the ice discharge of the ice sheet. Uncertainties in this calculation include the snow accumulation rate, which has traditionally been determined by interpolating data from ice core samples taken throughout the ice sheet. The sparse data associated with ice 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.

  15. The Role of Snow and Ice in the Climate System

    ScienceCinema

    Barry, Roger G.

    2017-12-09

    Global snow and ice 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 ice - albedo feedback. Snow and ice cover undergo marked seasonal and long term changes in extent and thickness. The perennial elements - the major ice sheets and permafrost - play a role in present-day regional and local climate and hydrology, but the large seasonal variations in snow cover and sea ice are of importance on continental to hemispheric scales. The characteristics of these variations, especially in the Northern Hemisphere, and evidence for recent trends in snow and ice extent are discussed.

  16. Radiative transfer model of snow for bare ice regions

    NASA Astrophysics Data System (ADS)

    Tanikawa, T.; Aoki, T.; Niwano, M.; Hosaka, M.; Shimada, R.; Hori, M.; Yamaguchi, S.

    2016-12-01

    Modeling a radiative transfer (RT) for coupled atmosphere-snow-bare ice systems is of fundamental importance for remote sensing applications to monitor snow and bare ice regions in the Greenland ice sheet and for accurate climate change predictions by regional and global climate models. Recently, the RT model for atmosphere-snow system was implemented for our regional and global climate models. However, the bare ice region where recently it has been expanded on the Greenland ice sheet due to the global warming, has not been implemented for these models, implying that this region leads miscalculations in these climate models. Thus, the RT model of snow for bare ice regions is needed for accurate climate change predictions. We developed the RT model for coupled atmosphere-snow-bare ice systems, and conducted a sensitivity analysis of the RT model to know the effect of snow, bare ice and geometry parameters on the spectral radiant quantities. The RT model considers snow and bare-ice inherent optical properties (IOPs), including snow grain size, air bubble size and its concentration and bare ice thickness. The conventional light scattering theory, Mie theory, was used for IOP calculations. Monte Carlo method was used for the multiple scattering. The sensitivity analyses showed that spectral albedo for the bare ice increased with increasing the concentration of the air bubble in the bare ice for visible wavelengths because the air bubble is scatterer with no absorption. For near infrared wavelengths, spectral albedo has no dependence on the air bubble due to the strong light absorption by ice. When increasing solar zenith angle, the spectral albedo were increased for all wavelengths. This is the similar trend with spectral snow albedo. Cloud cover influenced the bare ice spectral albedo by covering direct radiation into diffuse radiation. The purely diffuse radiation has an effective solar zenith angle near 50°. Converting direct into diffuse radiation reduces the

  17. 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.

  18. Studies of ice sheet hydrology using SAR

    NASA Technical Reports Server (NTRS)

    Bindschadler, R. A.; Vornberger, P. L.

    1989-01-01

    Analysis of SAR data of the Greenland ice sheet in summer and winter suggest the use of SAR to monitor the temporal hydrology of ice sheets. Comparisons of each SAR data set with summer Landsat TM imagery show an areal-positive correlation with summer SAR data and a negative correlation with winter SAR data. It is proposed that the summer SAR data are most sensitive to the variable concentrations of free water in the surface snow and that the winter SAR data indicate variations in snow grain size.

  19. Albedo Drop on the Greenland Ice Sheet: Relative Impacts of Wet and Dry Snow Processes

    NASA Astrophysics Data System (ADS)

    Chen, J.; Polashenski, C.

    2014-12-01

    The energy balance of the Greenland Ice Sheet (GIS) is strongly impacted by changes in snow albedo. MODIS (Moderate Resolution Imaging Spectroradiometer) observations indicate that the GIS albedo has dropped since the early part of this century. We analyze data from the MODIS products MOD10A1 for broadband snow albedo and MOD09A1 for surface spectral reflectance since 2001 to better explain the physical mechanisms driving these changes. The MODIS products are filtered, and the data is masked using microwave-derived surface melt maps to isolate albedo changes due to dry snow processes from those driven by melt impacts. Results show that the majority of recent changes in the GIS albedo - even at high elevations - are driven by snow wetting rather than dry snow processes such as grain metamorphosis and aerosol impurity deposition. The spectral signature of the smaller changes occurring within dry snow areas suggests that grain metamorphosis dominates the albedo decline in these regions.

  20. National Snow and Ice Data Center |

    Science.gov Websites

    Temperature Glaciers Ice Sheets Permafrost Sea Ice Soil Moisture Snow ...search for more Scientific Data Web pages Data Sets Drought on the range Drought on the range Using satellite soil moisture data as a tool for drought monitoring. Read more ... SMAP Soil Moisture Active Passive Data (SMAP) NASA SMAP data

  1. Ice sheet climate modeling: past achievements, ongoing challenges, and future endeavors

    NASA Astrophysics Data System (ADS)

    Lenaerts, J.

    2017-12-01

    Fluctuations in surface mass balance (SMB) mask out a substantial portion of contemporary Greenland and Antarctic ice sheet mass loss. That implies that we need accurate, consistent, and long-term SMB time series to isolate the mass loss signal. This in turn requires understanding of the processes driving SMB, and how they interplay. The primary controls on present-day ice sheet SMB are snowfall, which is regulated by large-scale atmospheric variability, and surface meltwater production at the ice sheet's edges, which is a complex result of atmosphere-surface interactions. Additionally, wind-driven snow redistribution and sublimation are large SMB contributors on the downslope areas of the ice sheets. Climate models provide an integrated framework to simulate all these individual ice sheet components. Recent developments in RACMO2, a regional climate model bound by atmospheric reanalyses, have focused on enhancing horizontal resolution, including blowing snow, snow albedo, and meltwater processes. Including these physics not only enhanced our understanding of the ice sheet climate system, but also enabled to obtain increasingly accurate estimates of ice sheet SMB. However, regional models are not suitable to capture the mutual interactions between ice sheet and the remainder of the global climate system in transient climates. To take that next step, global climate models are essential. In this talk, I will highlight our present work on improving ice sheet climate in the Community Earth System Model (CESM). In particular, we focus on an improved representation of polar firn, ice sheet clouds, and precipitation. For this exercise, we extensively use field observations, remote sensing data, as well as RACMO2. Next, I will highlight how CESM is used to enhance our understanding of ice sheet SMB, its drivers, and past and present changes.

  2. Use of Unmanned Aircraft Systems in Observations of Glaciers, Ice Sheets, Sea Ice and Snow Fields

    NASA Astrophysics Data System (ADS)

    Herzfeld Mayer, M. U.

    2015-12-01

    Unmanned Aircraft Systems (UAS) are being used increasingly in observations of the Earth, especially as such UAS become smaller, lighter and hence less expensive. In this paper, we present examples of observations of snow fields, glaciers and ice sheets and of sea ice in the Arctic that have been collected from UAS. We further examine possibilities for instrument miniaturization, using smaller UAS and smaller sensors for collecting data. The quality and type of data is compared to that of satellite observations, observations from manned aircraft and to measurements made during field experiments on the ground. For example, a small UAS can be sent out to observe a sudden event, such as a natural catastrophe, and provide high-resolution imagery, but a satellite has the advantage of providing the same type of data over much of the Earth's surface and for several years, but the data is generally of lower resolution. Data collected on the ground typically have the best control and quality, but the survey area is usually small. Here we compare micro-topographic measurements made on snow fields the Colorado Rocky Mountains with airborne and satellite data.

  3. The microbiome of glaciers and ice sheets.

    PubMed

    Anesio, Alexandre M; Lutz, Stefanie; Chrismas, Nathan A M; Benning, Liane G

    2017-01-01

    Glaciers and ice sheets, like other biomes, occupy a significant area of the planet and harbour biological communities with distinct interactions and feedbacks with their physical and chemical environment. In the case of the glacial biome, the biological processes are dominated almost exclusively by microbial communities. Habitats on glaciers and ice sheets with enough liquid water to sustain microbial activity include snow, surface ice, cryoconite holes, englacial systems and the interface between ice and overridden rock/soil. There is a remarkable similarity between the different specific glacial habitats across glaciers and ice sheets worldwide, particularly regarding their main primary producers and ecosystem engineers. At the surface, cyanobacteria dominate the carbon production in aquatic/sediment systems such as cryoconite holes, while eukaryotic Zygnematales and Chlamydomonadales dominate ice surfaces and snow dynamics, respectively. Microbially driven chemolithotrophic processes associated with sulphur and iron cycle and C transformations in subglacial ecosystems provide the basis for chemical transformations at the rock interface under the ice that underpin an important mechanism for the delivery of nutrients to downstream ecosystems. In this review, we focus on the main ecosystem engineers of glaciers and ice sheets and how they interact with their chemical and physical environment. We then discuss the implications of this microbial activity on the icy microbiome to the biogeochemistry of downstream ecosystems.

  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. Potential Climatic Effects on the Greenland Ice Sheet

    NASA Technical Reports Server (NTRS)

    Bindschadler, R. A.

    1984-01-01

    The Greenland Ice Sheet covers an area of 1,720,000 sq. km and contains approximately 2,600,000 cu km of ice. Most of the ice sheet receives an excess of snow accumulation over the amount of ice lost to wind, meltwater run-off or other ablative processes. The majority of mass loss occurs at the margin of the ice sheet as either surface melt, which flows into the sea or calving of icebergs from the tongues of outlet glaciers. Many estimates of these processes were published. An average of five published estimates is summarized. If these estimates are correct, then the Greenland Ice Sheet is in approximate equilibrium and contributes 490 cu km/a of fresh water to the North Atlantic and Arctic Oceans. Climate effects, ice sheet flow, and application of remote sensing to tracking of the ice sheet are discussed.

  6. Ice sheets and nitrogen.

    PubMed

    Wolff, Eric W

    2013-07-05

    Snow and ice play their most important role in the nitrogen cycle as a barrier to land-atmosphere and ocean-atmosphere exchanges that would otherwise occur. The inventory of nitrogen compounds in the polar ice sheets is approximately 260 Tg N, dominated by nitrate in the much larger Antarctic ice sheet. Ice cores help to inform us about the natural variability of the nitrogen cycle at global and regional scale, and about the extent of disturbance in recent decades. Nitrous oxide concentrations have risen about 20 per cent in the last 200 years and are now almost certainly higher than at any time in the last 800 000 years. Nitrate concentrations recorded in Greenland ice rose by a factor of 2-3, particularly between the 1950s and 1980s, reflecting a major change in NOx emissions reaching the background atmosphere. Increases in ice cores drilled at lower latitudes can be used to validate or constrain regional emission inventories. Background ammonium concentrations in Greenland ice show no significant recent trend, although the record is very noisy, being dominated by spikes of input from biomass burning events. Neither nitrate nor ammonium shows significant recent trends in Antarctica, although their natural variations are of biogeochemical and atmospheric chemical interest. Finally, it has been found that photolysis of nitrate in the snowpack leads to significant re-emissions of NOx that can strongly impact the regional atmosphere in snow-covered areas.

  7. Ice sheets and nitrogen

    PubMed Central

    Wolff, Eric W.

    2013-01-01

    Snow and ice play their most important role in the nitrogen cycle as a barrier to land–atmosphere and ocean–atmosphere exchanges that would otherwise occur. The inventory of nitrogen compounds in the polar ice sheets is approximately 260 Tg N, dominated by nitrate in the much larger Antarctic ice sheet. Ice cores help to inform us about the natural variability of the nitrogen cycle at global and regional scale, and about the extent of disturbance in recent decades. Nitrous oxide concentrations have risen about 20 per cent in the last 200 years and are now almost certainly higher than at any time in the last 800 000 years. Nitrate concentrations recorded in Greenland ice rose by a factor of 2–3, particularly between the 1950s and 1980s, reflecting a major change in NOx emissions reaching the background atmosphere. Increases in ice cores drilled at lower latitudes can be used to validate or constrain regional emission inventories. Background ammonium concentrations in Greenland ice show no significant recent trend, although the record is very noisy, being dominated by spikes of input from biomass burning events. Neither nitrate nor ammonium shows significant recent trends in Antarctica, although their natural variations are of biogeochemical and atmospheric chemical interest. Finally, it has been found that photolysis of nitrate in the snowpack leads to significant re-emissions of NOx that can strongly impact the regional atmosphere in snow-covered areas. PMID:23713125

  8. Clouds enhance Greenland ice sheet meltwater runoff

    PubMed Central

    Van Tricht, K.; Lhermitte, S.; Lenaerts, J. T. M.; Gorodetskaya, I. V.; L'Ecuyer, T. S.; Noël, B.; van den Broeke, M. R.; Turner, D. D.; van Lipzig, N. P. M.

    2016-01-01

    The Greenland ice sheet has become one of the main contributors to global sea level rise, predominantly through increased meltwater runoff. The main drivers of Greenland ice sheet runoff, however, remain poorly understood. Here we show that clouds enhance meltwater runoff by about one-third relative to clear skies, using a unique combination of active satellite observations, climate model data and snow model simulations. This impact results from a cloud radiative effect of 29.5 (±5.2) W m−2. Contrary to conventional wisdom, however, the Greenland ice sheet responds to this energy through a new pathway by which clouds reduce meltwater refreezing as opposed to increasing surface melt directly, thereby accelerating bare-ice exposure and enhancing meltwater runoff. The high sensitivity of the Greenland ice sheet to both ice-only and liquid-bearing clouds highlights the need for accurate cloud representations in climate models, to better predict future contributions of the Greenland ice sheet to global sea level rise. PMID:26756470

  9. Clouds enhance Greenland ice sheet meltwater runoff.

    PubMed

    Van Tricht, K; Lhermitte, S; Lenaerts, J T M; Gorodetskaya, I V; L'Ecuyer, T S; Noël, B; van den Broeke, M R; Turner, D D; van Lipzig, N P M

    2016-01-12

    The Greenland ice sheet has become one of the main contributors to global sea level rise, predominantly through increased meltwater runoff. The main drivers of Greenland ice sheet runoff, however, remain poorly understood. Here we show that clouds enhance meltwater runoff by about one-third relative to clear skies, using a unique combination of active satellite observations, climate model data and snow model simulations. This impact results from a cloud radiative effect of 29.5 (±5.2) W m(-2). Contrary to conventional wisdom, however, the Greenland ice sheet responds to this energy through a new pathway by which clouds reduce meltwater refreezing as opposed to increasing surface melt directly, thereby accelerating bare-ice exposure and enhancing meltwater runoff. The high sensitivity of the Greenland ice sheet to both ice-only and liquid-bearing clouds highlights the need for accurate cloud representations in climate models, to better predict future contributions of the Greenland ice sheet to global sea level rise.

  10. Monitoring Antarctic ice sheet surface melting with TIMESAT algorithm

    NASA Astrophysics Data System (ADS)

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

    2011-12-01

    Antarctic ice sheet contributes significantly to the global heat budget by controlling the exchange of heat, moisture, and momentum at the surface-atmosphere interface, which directly influence the global atmospheric circulation and climate change. Ice sheet melting will cause snow humidity increase, which will accelerate the disintegration and movement of ice sheet. As a result, detecting Antarctic ice sheet melting is essential for global climate change research. In the past decades, various methods have been proposed for extracting snowmelt information from multi-channel satellite passive microwave data. Some methods are based on brightness temperature values or a composite index of them, and others are based on edge detection. TIMESAT (Time-series of Satellite sensor data) is an algorithm for extracting seasonality information from time-series of satellite sensor data. With TIMESAT long-time series brightness temperature (SSM/I 19H) is simulated by Double Logistic function. Snow is classified to wet and dry snow with generalized Gaussian model. The results were compared with those from a wavelet algorithm. On this basis, Antarctic automatic weather station data were used for ground verification. It shows that this algorithm is effective in ice sheet melting detection. The spatial distribution of melting areas(Fig.1) shows that, the majority of melting areas are located on the edge of Antarctic ice shelf region. It is affected by land cover type, surface elevation and geographic location (latitude). In addition, the Antarctic ice sheet melting varies with seasons. It is particularly acute in summer, peaking at December and January, staying low in March. In summary, from 1988 to 2008, Ross Ice Shelf and Ronnie Ice Shelf have the greatest interannual variability in amount of melting, which largely determines the overall interannual variability in Antarctica. Other regions, especially Larsen Ice Shelf and Wilkins Ice Shelf, which is in the Antarctic Peninsula

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

    NASA Astrophysics Data System (ADS)

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

    2015-12-01

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

  12. Investigating the Impact of Aerosol Deposition on Snow Melt over the Greenland Ice Sheet Using a New Kernel

    NASA Astrophysics Data System (ADS)

    Li, Y.; Flanner, M.

    2017-12-01

    Accelerating surface melt on the Greenland Ice Sheet (GrIS) has led to a doubling of Greenland's contribution to global sea level rise during recent decades. The darkening effect due to black carbon (BC), dust, and other light absorbing impurities (LAI) enhances snow melt by boosting its absorption of solar energy. It is therefore important for coupled aerosol-climate and ice sheet models to include snow darkening effects from LAI, and yet most do not. In this study, we develop an aerosol deposition—snow melt kernel based on the Community Earth System Model (CESM) to investigate changes in melt flux due to variations in the amount and timing of aerosol deposition on the GrIS. The Community Land Model (CLM) component of CESM is driven with a large range of aerosol deposition fluxes to determine non-linear relationships between melt perturbation and deposition amount occurring in different months and location (thereby capturing variations in base state associated with elevation and latitude). The kernel product will include climatological-mean effects and standard deviations associated with interannual variability. Finally, the kernel will allow aerosol deposition fluxes from any global or regional aerosol model to be translated into surface melt perturbations of the GrIS, thus extending the utility of state-of-the-art aerosol models.

  13. Accumulation Rates in the Dry Snow Zone of the Greenland Ice Sheet Inferred from L-band InSAR Data

    NASA Astrophysics Data System (ADS)

    Chen, A. C.; Zebker, H. A.

    2012-12-01

    The Greenland ice sheet contains about 2.9 million km3 of ice and would raise global sea levels by about 7.1 m if it melted completely. Two unusually large iceberg calving events at Petermann Glacier in the past several years, along with the unusually large extent of ice sheet melt this summer point to the relevance of understanding the mass balance of the Greenland ice sheet. In this study, we use data from the PALSAR instrument aboard the ALOS satellite to form L-band (23-centimeter carrier wavelength) InSAR images of the dry snow zone of the Greenland ice sheet. We form geocoded differential interferograms, using the ice sheet elevation model produced by Howat et.al. [1]. By applying phase and radiometric calibration, we can examine interferograms formed between any pair of transmit and receive polarization channels. In co-polarized interferograms, the InSAR correlation ranges from about 0.35 at the summit (38.7 deg W, 73.0 deg N) where accumulation is about 20 cm w.e./yr to about 0.70 at the north-eastern part of the dry snow zone (35.1 deg W, 77.1 deg N), where accumulation is about 11.7 cm w.e./yr. Cross-polarized interferograms show similar geographic variation with overall lower correlation. We compare our InSAR data with in-situ measurements published by Bales et.al. [2]. We examine the applicability of dense-medium radiative transfer electromagnetic scattering models for estimating accumulation rates from L-band InSAR data. The large number and broad coverage of ALOS scenes acquired between 2007 and 2009 with good InSAR coherence at 46-day repeat times and 21.5 degree incidence angles gives us the opportunity to examine the empirical relationship between in-situ accumulation rate observations and the polarimetric InSAR correlation and radar brightness at this particular imaging geometry. This helps us quantify the accuracy of accumulation rates estimated from InSAR data. In some regions, 46-day interferograms acquired in the winters of several consecutive

  14. The Preservation and Recycling of Snow Pack Nitrate at the West Antarctic Ice Sheet (WAIS) Divide Ice Core Site from the Present Day to the Last Glacial Period.

    NASA Astrophysics Data System (ADS)

    Robinson, J. W.; Buffen, A.; Hastings, M. G.; Schauer, A. J.; Moore, L.; Isaacs, A.; Geng, L.; Savarino, J. P.; Alexander, B.

    2017-12-01

    We use observations of the nitrogen isotopic composition of nitrate (δ15N(NO3-)) from snow and ice collected at the West Antarctic ice sheet (WAIS) divide ice core site to quantify the preservation and recycling of snow nitrate. Ice-core samples cover a continuous section from 36 to 52 thousand years ago and discrete samples from the Holocene, the last glacial maximum (LGM), and the glacial-Holocene transition. Higher δ15N of nitrate is consistently associated with lower temperatures with δ15N(NO3-) varying from 26 to 45 ‰ during the last glacial period and from 1 to 45 ‰ between the Holocene and glacial periods, respectively. We attribute the higher δ15N in colder periods to lower snow accumulation rates which lead to greater loss of snow nitrate via photolysis before burial beneath the snow photic zone. Modeling of nitrate preservation in snow pack was performed for modern and LGM conditions. The model is used in conjunction with observations to estimate the fraction of snow nitrate that is photolyzed, re-oxidized, and re-deposited over WAIS divide versus the fraction of primary nitrate that is deposited via long range transport. We used these estimates of fractional loss of snow nitrate in different time periods to determine the variation in the deposition flux of primary nitrate at WAIS divide with climate. Our findings have implications for the climate sensitivity of the oxidizing capacity of the polar atmosphere and the interpretation of ice-core records of nitrate in terms of past atmospheric composition.

  15. Refreezing on the Greenland ice sheet: a model comparison

    NASA Astrophysics Data System (ADS)

    Steger, Christian; Reijmer, Carleen; van den Broeke, Michiel; Ligtenberg, Stefan; Kuipers Munneke, Peter; Noël, Brice

    2016-04-01

    Mass loss of the Greenland ice sheet (GrIS) is an important contributor to global sea level rise. Besides calving, surface melt is the dominant source of mass loss. However, only part of the surface melt leaves the ice sheet as runoff whereas the other part percolates into the snow cover and refreezes. Due to this process, part of the meltwater is (intermediately) stored. Refreezing thus impacts the surface mass balance of the ice sheet but it also affects the vertical structure of the snow cover due to transport of mass and energy. Due to the sparse availability of in situ data and the demand of future projections, it is inevitable to use numerical models to simulate refreezing and related processes. Currently, the magnitude of refrozen mass is neither well constrained nor well validated. In this study, we model the snow and firn layer, and compare refreezing on the GrIS as modelled with two different numerical models. Both models are forced with meteorological data from the regional climate model RACMO 2 that has been shown to simulate realistic conditions for Greenland. One model is the UU/IMAU firn densification model (FDM) that can be used both in an on- and offline mode with RACMO 2. The other model is SNOWPACK; a model originally designed to simulate seasonal snow cover in alpine conditions. In contrast to FDM, SNOWPACK accounts for snow metamorphism and microstructure and contains a more physically based snow densification scheme. A first comparison of the models indicates that both seem to be able to capture the general spatial and temporal pattern of refreezing. Spatially, refreezing occurs mostly in the ablation zone and decreases in the accumulation zone towards the interior of the ice sheet. Below the equilibrium line altitude (ELA) where refreezing occurs in seasonal snow cover on bare ice, the storage effect is only intermediate. Temporal patterns on a seasonal range indicate two peaks in refreezing; one at the beginning of the melt season where

  16. Radar Detection of Layering in Ice: Experiments on a Constructed Layered Ice Sheet

    NASA Astrophysics Data System (ADS)

    Carter, L. M.; Koenig, L.; Courville, Z.; Ghent, R. R.; Koutnik, M. R.

    2016-12-01

    The polar caps and glaciers of both Earth and Mars display internal layering that preserves a record of past climate. These layers are apparent both in optical datasets (high resolution images, core samples) and in ground penetrating radar (GPR) data. On Mars, the SHARAD (Shallow Radar) radar on the Mars Reconnaissance Orbiter shows fine layering that changes spatially and with depth across the polar caps. This internal layering has been attributed to changes in fractional dust contamination due to obliquity-induced climate variations, but there are other processes that can lead to internal layers visible in radar data. In particular, terrestrial sounding of ice sheets compared with core samples have revealed that ice density and composition differences account for the majority of the radar reflectors. The large cold rooms and ice laboratory facility at the U.S. Army Cold Regions Research and Engineering Laboratory (CRREL) provide us a unique opportunity to construct experimental ice sheets in a controlled setting and measure them with radar. In a CRREL laboratory, we constructed a layered ice sheet that is 3-m deep with a various snow and ice layers with known dust concentrations (using JSC Mars-1 basaltic simulant) and density differences. These ice sheets were profiled using a commercial GPR, at frequencies of 200, 400 and 900 MHz, to determine how the radar profile changes due to systematic and known changes in snow and ice layers, including layers with sub-wavelength spacing. We will report results from these experiments and implications for interpreting radar-detected layering in ice on Earth and Mars.

  17. Determining Greenland Ice Sheet Accumulation Rates from Radar Remote Sensing

    NASA Technical Reports Server (NTRS)

    Jezek, Kenneth C.

    2002-01-01

    An important component of NASA's Program for Arctic Regional Climate Assessment (PARCA) is a mass balance investigation of the Greenland Ice Sheet. The mass balance is calculated by taking the difference between the areally Integrated snow accumulation and the net ice discharge of the ice sheet. Uncertainties in this calculation Include the snow accumulation rate, which has traditionally been determined by interpolating data from ice core samples taken from isolated spots across the ice sheet. The sparse data associated with ice cores juxtaposed against the high spatial and temporal resolution provided by remote sensing , has motivated scientists to investigate relationships between accumulation rate and microwave observations as an option for obtaining spatially contiguous estimates. The objective of this PARCA continuation proposal was to complete an estimate of surface accumulation rate on the Greenland Ice Sheet derived from C-band radar backscatter data compiled in the ERS-1 SAR mosaic of data acquired during, September-November, 1992. An empirical equation, based on elevation and latitude, is used to determine the mean annual temperature. We examine the influence of accumulation rate, and mean annual temperature on C-band radar backscatter using a forward model, which incorporates snow metamorphosis and radar backscatter components. Our model is run over a range of accumulation and temperature conditions. Based on the model results, we generate a look-up table, which uniquely maps the measured radar backscatter, and mean annual temperature to accumulation rate. Our results compare favorably with in situ accumulation rate measurements falling within our study area.

  18. Airborne radar surveys of snow depth over Antarctic sea ice during Operation IceBridge

    NASA Astrophysics Data System (ADS)

    Panzer, B.; Gomez-Garcia, D.; Leuschen, C.; Paden, J. D.; Gogineni, P. S.

    2012-12-01

    Over the last decade, multiple satellite-based laser and radar altimeters, optimized for polar observations, have been launched with one of the major objectives being the determination of global sea ice thickness and distribution [5, 6]. Estimation of sea-ice thickness from these altimeters relies on freeboard measurements and the presence of snow cover on sea ice affects this estimate. Current means of estimating the snow depth rely on daily precipitation products and/or data from passive microwave sensors [2, 7]. Even a small uncertainty in the snow depth leads to a large uncertainty in the sea-ice thickness estimate. To improve the accuracy of the sea-ice thickness estimates and provide validation for measurements from satellite-based sensors, the Center for Remote Sensing of Ice Sheets deploys the Snow Radar as a part of NASA Operation IceBridge. The Snow Radar is an ultra-wideband, frequency-modulated, continuous-wave radar capable of resolving snow depth on sea ice from 5 cm to more than 2 meters from long-range, airborne platforms [4]. This paper will discuss the algorithm used to directly extract snow depth estimates exclusively using the Snow Radar data set by tracking both the air-snow and snow-ice interfaces. Prior work in this regard used data from a laser altimeter for tracking the air-snow interface or worked under the assumption that the return from the snow-ice interface was greater than that from the air-snow interface due to a larger dielectric contrast, which is not true for thick or higher loss snow cover [1, 3]. This paper will also present snow depth estimates from Snow Radar data during the NASA Operation IceBridge 2010-2011 Antarctic campaigns. In 2010, three sea ice flights were flown, two in the Weddell Sea and one in the Amundsen and Bellingshausen Seas. All three flight lines were repeated in 2011, allowing an annual comparison of snow depth. In 2011, a repeat pass of an earlier flight in the Weddell Sea was flown, allowing for a

  19. Antarctic Sea Ice Thickness and Snow-to-Ice Conversion from Atmospheric Reanalysis and Passive Microwave Snow Depth

    NASA Technical Reports Server (NTRS)

    Markus, Thorsten; Maksym, Ted

    2007-01-01

    Passive microwave snow depth, ice concentration, and ice motion estimates are combined with snowfall from the European Centre for Medium Range Weather Forecasting (ECMWF) reanalysis (ERA-40) from 1979-200 1 to estimate the prevalence of snow-to-ice conversion (snow-ice formation) on level sea ice in the Antarctic for April-October. Snow ice is ubiquitous in all regions throughout the growth season. Calculated snow- ice thicknesses fall within the range of estimates from ice core analysis for most regions. However, uncertainties in both this analysis and in situ data limit the usefulness of snow depth and snow-ice production to evaluate the accuracy of ERA-40 snowfall. The East Antarctic is an exception, where calculated snow-ice production exceeds observed ice thickness over wide areas, suggesting that ERA-40 precipitation is too high there. Snow-ice thickness variability is strongly controlled not just by snow accumulation rates, but also by ice divergence. Surprisingly, snow-ice production is largely independent of snow depth, indicating that the latter may be a poor indicator of total snow accumulation. Using the presence of snow-ice formation as a proxy indicator for near-zero freeboard, we examine the possibility of estimating level ice thickness from satellite snow depths. A best estimate for the mean level ice thickness in September is 53 cm, comparing well with 51 cm from ship-based observations. The error is estimated to be 10-20 cm, which is similar to the observed interannual and regional variability. Nevertheless, this is comparable to expected errors for ice thickness determined by satellite altimeters. Improvement in satellite snow depth retrievals would benefit both of these methods.

  20. Snow depth evolution on sea ice from Snow Buoy measurement

    NASA Astrophysics Data System (ADS)

    Nicolaus, M.; Arndt, S.; Hendricks, S.; Hoppmann, M.; Katlein, C.; König-Langlo, G.; Nicolaus, A.; Rossmann, H. L.; Schiller, M.; Schwegmann, S.; Langevin, D.

    2016-12-01

    Snow cover is an Essential Climate Variable. On sea ice, snow dominates the energy and momentum exchanges across the atmosphere-ice-ocean interfaces, and actively contributes to sea ice mass balance. Yet, snow depth on sea ice is one of the least known and most difficult to observe parameters of the Arctic and Antarctic; mainly due to its exceptionally high spatial and temporal variability. In this study; we present a unique time series dataset of snow depth and air temperature evolution on Arctic and Antarctic sea ice recorded by autonomous instruments. Snow Buoys record snow depth with four independent ultrasonic sensors, increasing the reliability of the measurements and allowing for additional analyses. Auxiliary measurements include surface and air temperature, barometric pressure and GPS position. 39 deployments of such Snow Buoys were achieved over the last three years either on drifting pack ice, on landfast sea ice or on an ice shelf. Here we highlight results from two pairs of Snow Buoys installed on drifting pack ice in the Weddell Sea. The data reveals large regional differences in the annual cycle of snow depth. Almost no reduction in snow depth (snow melt) was observed in the inner and southern part of the Weddell Sea, allowing a net snow accumulation of 0.2 to 0.9 m per year. In contrast, summer snow melt close to the ice edge resulted in a decrease of about 0.5 m during the summer 2015/16. Another array of eight Snow Buoys was installed on central Arctic sea ice in September 2015. Their air temperature record revealed exceptionally high air temperatures in the subsequent winter, even exceeding the melting point but with almost no impact on snow depth at that time. Future applications of Snow Buoys on Arctic and Antarctic sea ice will allow additional inter-annual studies of snow depth and snow processes, e.g. to support the development of snow depth data products from airborne and satellite data or though assimilation in numerical models.

  1. Thinning of the ice sheet in northwest Greenland over the past forty years.

    PubMed

    Paterson, W S; Reeh, N

    2001-11-01

    Thermal expansion of the oceans, as well as melting of glaciers, ice sheets and ice 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 mass balance of the ice sheets in Greenland and Antarctica. Satellite measurements have been used to determine changes in these ice sheets on short timescales, demonstrating that surface-elevation changes on timescales of decades or less result mainly from variations 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 ice sheet. Measurements over a time interval of this length should reflect changes in ice 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 ice stream. On the west side, however, the thinning rates of the ice sheet are significantly higher and thinning extends to higher elevations than had been anticipated from previous studies.

  2. Modelling the Climate - Greenland Ice Sheet Interaction in the Coupled Ice-sheet/Climate Model EC-EARTH - PISM

    NASA Astrophysics Data System (ADS)

    Yang, S.; Madsen, M. S.; Rodehacke, C. B.; Svendsen, S. H.; Adalgeirsdottir, G.

    2014-12-01

    Recent observations show that the Greenland ice sheet (GrIS) has been losing mass 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 ice sheet module. A fully coupled global climate model with a dynamical ice 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 ice model system, and the Parallel Ice Sheet Model (PISM). The coupling of PISM includes a modified surface physical parameterization in EC-EARTH adapted to the land ice surface over glaciated regions in Greenland. The PISM ice sheet model is forced with the surface mass balance (SMB) directly computed inside the EC-EARTH atmospheric module and accounting for the precipitation, the surface evaporation, and the melting of snow and ice over land ice. PISM returns the simulated basal melt, ice discharge and ice cover (extent and thickness) as boundary conditions to EC-EARTH. This coupled system is mass and energy conserving without being constrained by any anomaly correction or flux adjustment, and hence is suitable for investigation of ice 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 ice sheet) to evaluate the performance of the coupled system and to quantify the GrIS feedbacks. In particular, the evolution of the Greenland ice sheet under the warm climate and its impacts on the climate system are investigated. Freshwater fluxes from the Greenland ice sheet melt to the Arctic

  3. Radar measurements of melt zones on the Greenland Ice Sheet

    NASA Technical Reports Server (NTRS)

    Jezek, Kenneth C.; Gogineni, Prasad; Shanableh, M.

    1994-01-01

    Surface-based microwave radar measurements were performed at a location on the western flank of the Greenland Ice Sheet. Here, firn metamorphasis is dominated by seasonal melt, which leads to marked contrasts in the vertical structure of winter and summer firn. This snow regime is also one of the brightest radar targets on Earth with an average backscatter coefficient of 0 dB at 5.3 GHz and an incidence angle of 25 deg. By combining detailed observations of firn physical properties with ranging radar measurements we find that the glaciological mechanism associated with this strong electromagnetic response is summer ice lens formation within the previous winter's snow pack. This observation has important implications for monitoring and understanding changes in ice sheet volume using spaceborne microwave sensors.

  4. Annual accumulation over the Greenland ice sheet interpolated from historical and newly compiled observation data

    USGS Publications Warehouse

    Shen, Dayong; Liu, Yuling; Huang, Shengli

    2012-01-01

    The estimation of ice/snow accumulation is of great significance in quantifying the mass balance of ice sheets and variation in water resources. Improving the accuracy and reducing uncertainty has been a challenge for the estimation of annual accumulation over the Greenland ice 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 ice cores and snow pits and newly compiled 23 coastal weather station data. The estimated annual accumulation over the Greenland ice 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 ice sheet.

  5. MODIS Snow and Sea Ice Products

    NASA Technical Reports Server (NTRS)

    Hall, Dorothy K.; Riggs, George A.; Salomonson, Vincent V.

    2004-01-01

    In this chapter, we describe the suite of Earth Observing System (EOS) Moderate-Resolution Imaging Spectroradiometer (MODIS) Terra and Aqua snow and sea ice products. Global, daily products, developed at Goddard Space Flight Center, are archived and distributed through the National Snow and Ice Data Center at various resolutions and on different grids useful for different communities Snow products include binary snow cover, snow albedo, and in the near future, fraction of snow in a 5OO-m pixel. Sea ice products include ice extent determined with two different algorithms, and sea ice surface temperature. The algorithms used to develop these products are described. Both the snow and sea ice products, available since February 24,2000, are useful for modelers. Validation of the products is also discussed.

  6. Extensive Liquid Meltwater Storage in Firn Within the Greenland Ice Sheet

    NASA Technical Reports Server (NTRS)

    Forster, Richard R.; Box, Jason E.; vandenBroeke, Michael R.; Miege, Clement; Burgess, Evan W.; vanAngelen, Jan H.; Lenaerts, Jan T. M.; Koenig, Lora S.; Paden, John; Lewis, Cameron; hide

    2013-01-01

    The accelerating loss of mass from the Greenland ice sheet is a major contribution to current sea level rise. Increased melt water runoff is responsible for half of Greenlands mass loss increase. Surface melt has been increasing in extent and intensity, setting a record for surface area melt and runoff in 2012. The mechanisms and timescales involved in allowing surface melt water to reach the ocean where it can contribute to sea level rise are poorly understood. The potential capacity to store this water in liquid or frozen form in the firn (multi-year snow layer) is significant, and could delay its sea-level contribution. Here we describe direct observation of water within a perennial firn aquifer persisting throughout the winter in the southern ice sheet,where snow accumulation and melt rates are high. This represents a previously unknown storagemode for water within the ice sheet. Ice cores, groundairborne radar and a regional climatemodel are used to estimate aquifer area (70 plue or minus 10 x 10(exp 3) square kilometers ) and water table depth (5-50 m). The perennial firn aquifer represents a new glacier facies to be considered 29 in future ice sheet mass 30 and energy budget calculations.

  7. Extraction of Ice Sheet Layers from Two Intersected Radar Echograms Near Neem Ice Core in Greenland

    NASA Astrophysics Data System (ADS)

    Xiong, S.; Muller, J.-P.

    2016-06-01

    Accumulation of snow and ice over time result in ice sheet layers. These can be remotely sensed where there is a contrast in electromagnetic properties, which reflect variations of the ice density, acidity and fabric orientation. Internal ice layers are assumed to be isochronous, deep beneath the ice surface, and parallel to the direction of ice flow. The distribution of internal layers is related to ice sheet dynamics, such as the basal melt rate, basal elevation variation and changes in ice flow mode, which are important parameters to model the ice sheet. Radar echo sounder is an effective instrument used to study the sedimentology of the Earth and planets. Ice Penetrating Radar (IPR) is specific kind of radar echo sounder, which extends studies of ice sheets from surface to subsurface to deep internal ice sheets depending on the frequency utilised. In this study, we examine a study site where folded ice occurs in the internal ice sheet south of the North Greenland Eemian ice drilling (NEEM) station, where two intersected radar echograms acquired by the Multi-channel Coherent Radar Depth Sounder (MCoRDS) employed in the NASA's Operation IceBridge (OIB) mission imaged this folded ice. We propose a slice processing flow based on a Radon Transform to trace and extract these two sets of curved ice sheet layers, which can then be viewed in 3-D, demonstrating the 3-D structure of the ice folds.

  8. MODIS Snow and Ice Production

    NASA Technical Reports Server (NTRS)

    Hall, Dorthoy K.; Hoser, Paul (Technical Monitor)

    2002-01-01

    Daily, global snow cover maps, and sea ice cover and sea ice surface temperature (IST) maps are derived from NASA's Moderate Resolution Imaging Spectroradiometer (MODIS), are available at no cost through the National Snow and Ice Data Center (NSIDC). Included on this CD-ROM are samples of the MODIS snow and ice products. In addition, an animation, done by the Scientific Visualization studio at Goddard Space Flight Center, is also included.

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

    PubMed

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

    2016-02-18

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

  10. NHM-SMAP: spatially and temporally high-resolution nonhydrostatic atmospheric model coupled with detailed snow process model for Greenland Ice Sheet

    NASA Astrophysics Data System (ADS)

    Niwano, Masashi; Aoki, Teruo; Hashimoto, Akihiro; Matoba, Sumito; Yamaguchi, Satoru; Tanikawa, Tomonori; Fujita, Koji; Tsushima, Akane; Iizuka, Yoshinori; Shimada, Rigen; Hori, Masahiro

    2018-02-01

    To improve surface mass balance (SMB) estimates for the Greenland Ice Sheet (GrIS), we developed a 5 km resolution regional climate model combining the Japan Meteorological Agency Non-Hydrostatic atmospheric Model and the Snow Metamorphism and Albedo Process model (NHM-SMAP) with an output interval of 1 h, forced by the Japanese 55-year reanalysis (JRA-55). We used in situ data to evaluate NHM-SMAP in the GrIS during the 2011-2014 mass balance years. We investigated two options for the lower boundary conditions of the atmosphere: an offline configuration using snow, firn, and ice albedo, surface temperature data from JRA-55, and an online configuration using values from SMAP. The online configuration improved model performance in simulating 2 m air temperature, suggesting that the surface analysis provided by JRA-55 is inadequate for the GrIS and that SMAP results can better simulate physical conditions of snow/firn/ice. It also reproduced the measured features of the GrIS climate, diurnal variations, and even a strong mesoscale wind event. In particular, it successfully reproduced the temporal evolution of the GrIS surface melt area extent as well as the record melt event around 12 July 2012, at which time the simulated melt area extent reached 92.4 %. Sensitivity tests showed that the choice of calculation schemes for vertical water movement in snow and firn has an effect as great as 200 Gt year-1 in the GrIS-wide accumulated SMB estimates; a scheme based on the Richards equation provided the best performance.

  11. Mass Balance of the Greenland Ice Sheet at High Elevations.

    PubMed

    Thomas; Akins; Csatho; Fahnestock; Gogineni; Kim; Sonntag

    2000-07-21

    Comparison of ice discharge from higher elevation areas of the entire Greenland Ice Sheet with total snow accumulation gives estimates of ice 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 ice 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.

  12. Microwave signatures of snow, ice and soil at several wavelengths

    NASA Technical Reports Server (NTRS)

    Gloersen, P.; Schmugge, T. J.; Chang, T. C.

    1974-01-01

    Analyses of data obtained from aircraft-borne radiometers have shown that the microwave signatures of various parts of the terrain depend on both the volume scattering cross-section and the dielectric loss in the medium. In soil, it has been found that experimental data fit a model in which the scattering cross section is negligible compared to the dielectric loss. On the other hand, the volume scattering cross-section in snow and continental ice was found, from analyzing data obtained with aircraft- and spacecraft-borne radiometers, to be more important than the dielectric loss or surface reflectivity in determining the observed microwave emissivity. A model which assumes Mie scattering of ice particles of various sizes was found to be the dominant volume scattering mechanism in these media. Both spectral variation in the microwave signatures of snow and ice fields, as well as the variation in the emissivity of continental ice sheets such as those covering Greenland and Antarctica appear to be consistent with this model.

  13. Remote sensing of snow and ice

    NASA Technical Reports Server (NTRS)

    Rango, A.

    1979-01-01

    This paper reviews remote sensing of snow and ice, techniques for improved monitoring, and incorporation of the new data into forecasting and management systems. The snowcover interpretation of visible and infrared data from satellites, automated digital methods, radiative transfer modeling to calculate the solar reflectance of snow, and models using snowcover input data and elevation zones for calculating snowmelt are discussed. The use of visible and near infrared techniques for inferring snow properties, microwave monitoring of snowpack characteristics, use of Landsat images for collecting glacier data, monitoring of river ice with visible imagery from NOAA satellites, use of sequential imagery for tracking ice flow movement, and microwave studies of sea ice are described. Applications of snow and ice research to commercial use are examined, and it is concluded that a major problem to be solved is characterization of snow and ice in nature, since assigning of the correct properties to a real system to be modeled has been difficult.

  14. Ice sheet margins and ice shelves

    NASA Technical Reports Server (NTRS)

    Thomas, R. H.

    1984-01-01

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

  15. Leakage of the Greenland Ice Sheet through accelerated ice flow

    NASA Astrophysics Data System (ADS)

    Rignot, E.

    2005-12-01

    A map of coastal velocities of the Greenland ice sheet was produced from Radarsat-1 acquired during the background mission of 2000 and combined with radio echo sounding data to estimate the ice discharge from the ice sheet. On individual glaciers, ice discharge was compared with snow input from the interior and melt above the flux gate to determine the glacier mass 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 mass. No change in ice 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 ice 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 mass balance of the Greenland ice sheet to be about -80 +/-10 cubic km of ice per year in 2000 and -110 +/-15 cubic km of ice 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 mass balance will become increasingly negative, regardless of the evolution of the ice sheet

  16. Climate change and forest fires synergistically drive widespread melt events of the Greenland Ice Sheet.

    PubMed

    Keegan, Kaitlin M; Albert, Mary R; McConnell, Joseph R; Baker, Ian

    2014-06-03

    In July 2012, over 97% of the Greenland Ice Sheet experienced surface melt, the first widespread melt during the era of satellite remote sensing. Analysis of six Greenland shallow firn cores from the dry snow region confirms that the most recent prior widespread melt occurred in 1889. A firn core from the center of the ice sheet demonstrated that exceptionally warm temperatures combined with black carbon sediments from Northern Hemisphere forest fires reduced albedo below a critical threshold in the dry snow region, and caused the melting events in both 1889 and 2012. We use these data to project the frequency of widespread melt into the year 2100. Since Arctic temperatures and the frequency of forest fires are both expected to rise with climate change, our results suggest that widespread melt events on the Greenland Ice Sheet may begin to occur almost annually by the end of century. These events are likely to alter the surface mass balance of the ice sheet, leaving the surface susceptible to further melting.

  17. Spatiotemporal variability in surface energy balance across tundra, snow and ice in Greenland.

    PubMed

    Lund, Magnus; Stiegler, Christian; Abermann, Jakob; Citterio, Michele; Hansen, Birger U; van As, Dirk

    2017-02-01

    The surface energy balance (SEB) is essential for understanding the coupled cryosphere-atmosphere system in the Arctic. In this study, we investigate the spatiotemporal variability in SEB across tundra, snow and ice. During the snow-free period, the main energy sink for ice sites is surface melt. For tundra, energy is used for sensible and latent heat flux and soil heat flux leading to permafrost thaw. Longer snow-free period increases melting of the Greenland Ice Sheet and glaciers and may promote tundra permafrost thaw. During winter, clouds have a warming effect across surface types whereas during summer clouds have a cooling effect over tundra and a warming effect over ice, reflecting the spatial variation in albedo. The complex interactions between factors affecting SEB across surface types remain a challenge for understanding current and future conditions. Extended monitoring activities coupled with modelling efforts are essential for assessing the impact of warming in the Arctic.

  18. 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.

  19. 14 CFR 139.313 - Snow and ice control.

    Code of Federal Regulations, 2014 CFR

    2014-01-01

    ... 14 Aeronautics and Space 3 2014-01-01 2014-01-01 false Snow and ice control. 139.313 Section 139... AIRPORTS Operations § 139.313 Snow and ice control. (a) As determined by the Administrator, each... carry out a snow and ice control plan in a manner authorized by the Administrator. (b) The snow and ice...

  20. 14 CFR 139.313 - Snow and ice control.

    Code of Federal Regulations, 2010 CFR

    2010-01-01

    ... 14 Aeronautics and Space 3 2010-01-01 2010-01-01 false Snow and ice control. 139.313 Section 139... AIRPORTS Operations § 139.313 Snow and ice control. (a) As determined by the Administrator, each... carry out a snow and ice control plan in a manner authorized by the Administrator. (b) The snow and ice...

  1. 14 CFR 139.313 - Snow and ice control.

    Code of Federal Regulations, 2011 CFR

    2011-01-01

    ... 14 Aeronautics and Space 3 2011-01-01 2011-01-01 false Snow and ice control. 139.313 Section 139... AIRPORTS Operations § 139.313 Snow and ice control. (a) As determined by the Administrator, each... carry out a snow and ice control plan in a manner authorized by the Administrator. (b) The snow and ice...

  2. 14 CFR 139.313 - Snow and ice control.

    Code of Federal Regulations, 2013 CFR

    2013-01-01

    ... 14 Aeronautics and Space 3 2013-01-01 2013-01-01 false Snow and ice control. 139.313 Section 139... AIRPORTS Operations § 139.313 Snow and ice control. (a) As determined by the Administrator, each... carry out a snow and ice control plan in a manner authorized by the Administrator. (b) The snow and ice...

  3. 14 CFR 139.313 - Snow and ice control.

    Code of Federal Regulations, 2012 CFR

    2012-01-01

    ... 14 Aeronautics and Space 3 2012-01-01 2012-01-01 false Snow and ice control. 139.313 Section 139... AIRPORTS Operations § 139.313 Snow and ice control. (a) As determined by the Administrator, each... carry out a snow and ice control plan in a manner authorized by the Administrator. (b) The snow and ice...

  4. Validation of Airborne FMCW Radar Measurements of Snow Thickness Over Sea Ice in Antarctica

    NASA Technical Reports Server (NTRS)

    Galin, Natalia; Worby, Anthony; Markus, Thorsten; Leuschen, Carl; Gogineni, Prasad

    2012-01-01

    Antarctic sea ice and its snow cover are integral components of the global climate system, yet many aspects of their vertical dimensions are poorly understood, making their representation in global climate models poor. Remote sensing is the key to monitoring the dynamic nature of sea ice and its snow cover. Reliable and accurate snow thickness data are currently a highly sought after data product. Remotely sensed snow thickness measurements can provide an indication of precipitation levels, predicted to increase with effects of climate change in the polar regions. Airborne techniques provide a means for regional-scale estimation of snow depth and distribution. Accurate regional-scale snow thickness data will also facilitate an increase in the accuracy of sea ice thickness retrieval from satellite altimeter freeboard estimates. The airborne data sets are easier to validate with in situ measurements and are better suited to validating satellite algorithms when compared with in situ techniques. This is primarily due to two factors: better chance of getting coincident in situ and airborne data sets and the tractability of comparison between an in situ data set and the airborne data set averaged over the footprint of the antennas. A 28-GHz frequency modulated continuous wave (FMCW) radar loaned by the Center for Remote Sensing of Ice Sheets to the Australian Antarctic Division is used to measure snow thickness over sea ice in East Antarctica. Provided with the radar design parameters, the expected performance parameters of the radar are summarized. The necessary conditions for unambiguous identification of the airsnow and snowice layers for the radar are presented. Roughnesses of the snow and ice surfaces are found to be dominant determinants in the effectiveness of layer identification for this radar. Finally, this paper presents the first in situ validated snow thickness estimates over sea ice in Antarctica derived from an FMCW radar on a helicopterborne platform.

  5. Snow depth on Arctic and Antarctic sea ice derived from autonomous (Snow Buoy) measurements

    NASA Astrophysics Data System (ADS)

    Nicolaus, Marcel; Arndt, Stefanie; Hendricks, Stefan; Heygster, Georg; Huntemann, Marcus; Katlein, Christian; Langevin, Danielle; Rossmann, Leonard; Schwegmann, Sandra

    2016-04-01

    The snow cover on sea ice received more and more attention in recent sea ice studies and model simulations, because its physical properties dominate many sea ice and upper ocean processes. In particular; the temporal and spatial distribution of snow depth is of crucial importance for the energy and mass budgets of sea ice, as well as for the interaction with the atmosphere and the oceanic freshwater budget. Snow depth is also a crucial parameter for sea ice thickness retrieval algorithms from satellite altimetry data. Recent time series of Arctic sea ice volume only use monthly snow depth climatology, which cannot take into account annual changes of the snow depth and its properties. For Antarctic sea ice, no such climatology is available. With a few exceptions, snow depth on sea ice is determined from manual in-situ measurements with very limited coverage of space and time. Hence the need for more consistent observational data sets of snow depth on sea ice is frequently highlighted. Here, we present time series measurements of snow depths on Antarctic and Arctic sea ice, recorded by an innovative and affordable platform. This Snow Buoy is optimized to autonomously monitor the evolution of snow depth on sea ice and will allow new insights into its seasonality. In addition, the instruments report air temperature and atmospheric pressure directly into different international networks, e.g. the Global Telecommunication System (GTS) and the International Arctic Buoy Programme (IABP). We introduce the Snow Buoy concept together with technical specifications and results on data quality, reliability, and performance of the units. We highlight the findings from four buoys, which simultaneously drifted through the Weddell Sea for more than 1.5 years, revealing unique information on characteristic regional and seasonal differences. Finally, results from seven snow buoys co-deployed on Arctic sea ice throughout the winter season 2015/16 suggest the great importance of local

  6. Analysis of Airborne Radar Altimetry Measurements of the Greenland Ice Sheet

    NASA Technical Reports Server (NTRS)

    Ferraro, Ellen J.

    1994-01-01

    This dissertation presents an analysis of airborne altimetry measurements taken over the Greenland ice sheet with the 13.9 GHz Advanced Application Flight Experiment (AAFE) pulse compression radar altimeter. This Ku-band instrument was refurbished in 1990 by the Microwave Remote Sensing Laboratory at the University of Massachusetts to obtain high-resolution altitude measurements and to improve the tracking, speed, storage and display capabilities of the radar. In 1991 and 1993, the AAFE altimeter took part in the NASA Multisensor Airborne Altimetry Experiments over Greenland, along with two NASA laser altimeters. Altitude results from both experiments are presented along with comparisons to the laser altimeter and calibration passes over the Sondrestroem runway in Greenland. Although it is too early to make a conclusion about the growth or decay of the ice sheet, these results show that the instrument is capable of measuring small-scale surface changes to within 14 centimeters. In addition, results from these experiments reveal that the radar is sensitive to the different diagenetic regions of the ice sheet. Return waveforms from the wet- snow, percolation and dry-snow zones show varying effects of both surface scattering and sub-surface or volume scattering. Models of each of the diagenetic regions of Greenland are presented along with parameters such as rms surface roughness, rms surface slope and attenuation coefficient of the snow pack obtained by fitting the models to actual return waveforms.

  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. The extreme melt across the Greenland ice sheet in 2012

    NASA Astrophysics Data System (ADS)

    Nghiem, S. V.; Hall, D. K.; Mote, T. L.; Tedesco, M.; Albert, M. R.; Keegan, K.; Shuman, C. A.; DiGirolamo, N. E.; Neumann, G.

    2012-10-01

    The discovery of the 2012 extreme melt event across almost the entire surface of the Greenland ice sheet is presented. Data from three different satellite sensors - including the Oceansat-2 scatterometer, the Moderate-resolution Imaging Spectroradiometer, and the Special Sensor Microwave Imager/Sounder - are combined to obtain composite melt maps, representing the most complete melt conditions detectable across the ice sheet. Satellite observations reveal that melt occurred at or near the surface of the Greenland ice sheet across 98.6% of its entire extent on 12 July 2012, including the usually cold polar areas at high altitudes like Summit in the dry snow facies of the ice sheet. This melt event coincided with an anomalous ridge of warm air that became stagnant over Greenland. As seen in melt occurrences from multiple ice core records at Summit reported in the published literature, such a melt event is rare with the last significant one occurring in 1889 and the next previous one around seven centuries earlier in the Medieval Warm Period. Given its rarity, the 2012 extreme melt across Greenland provides an exceptional opportunity for new studies in broad interdisciplinary geophysical research.

  9. Arctic Circle Traverse 2010 (ACT-10): South East Greenland snow accumulation variability from firn coring and ice sounding radar

    NASA Astrophysics Data System (ADS)

    Forster, R. R.; Miege, C.; Box, J. E.; McConnell, J.; Spikes, V. B.; Burgess, E. W.

    2010-12-01

    The Greenland Ice Sheet plays an important role in Earth’s climate system evolution. The snow accumulation rate is the largest single mass budget term. With only 14% of the ice sheet area, Southeast Greenland contains the highest accumulation rates, accounting for one third of the total snow accumulation and annual variability. The high accumulation rates have made the region less desirable for long climate record ice cores and therefore, contain relatively very few in situ measurements to constrain the ice sheet mass budget. We present annual snow accumulation rates from the Arctic Circle Traverse 2010 (ACT-10). During April and May 2010 we acquired three 50 m firn cores connected by surface-based 400 MHz ground penetrating radar (GPR) in Southeast Greenland. The traverse repeated and extended the original Arctic Circle Traverse in 2004 (Spikes et al., 2004). Dating is achieved using geochemical analysis of the cores to identify isochronal layers detected by the GPR yielding annual accumulation estimates along the traverse between the core sites. The 300 km ACT-10 GPR snowmobile traverse extended the ACT-04 path 80 km to the lowest elevation core site at 1776 m. Meanwhile, airborne radars, operating as part of NASA’s Operation IceBridge also acquired data over the full length of the ACT-10 path, simultaneously with a portion of the traverse and within days for the remaining segments. The IceBridge and ACT-10 data are to be combined in a calibration effort such that snow accumulation rates may be mapped elsewhere in Greenland and even in Antarctica.

  10. Entrainment, transport and concentration of meteorites in polar ice sheets

    NASA Technical Reports Server (NTRS)

    Drewry, D. J.

    1986-01-01

    Glaciers and ice sheets act as slow-moving conveyancing systems for material added to both their upper and lower surfaces. Because the transit time for most materials is extremely long the ice acts as a major global storage facility. The effects of horizontal and vertical motions on the flow patterns of Antarctic ice sheets are summarized. The determination of the source areas of meteorites and their transport paths is a problem of central importance since it relates not only directly to concentration mechanisms but also to the wider issues in glaciology and meteorites. The ice and snow into which a meteorite falls, and which moves with it to the concentration area, encodes information about the infall area. The principle environmental conditions being former elevation, temperature (also related to elevation), and age of the ice. This encoded information could be used to identify the infall area.

  11. Variability of Surface Temperature and Melt on the Greenland Ice Sheet, 2000-2011

    NASA Technical Reports Server (NTRS)

    Hall, Dorothy K.; Comiso, Josefino, C.; Shuman, Christopher A.; Koenig, Lora S.; DiGirolamo, Nicolo E.

    2012-01-01

    Enhanced melting along with surface-temperature increases measured using infrared satellite data, have been documented for the Greenland Ice Sheet. Recently we developed a climate-quality data record of ice-surface temperature (IST) of the Greenland Ice Sheet using the Moderate-Resolution Imaging Spectroradiometer (MODIS) 1ST product -- http://modis-snow-ice.gsfc.nasa.gov. Using daily and mean monthly MODIS 1ST maps from the data record we show maximum extent of melt for the ice sheet and its six major drainage basins for a 12-year period extending from March of 2000 through December of 2011. The duration of the melt season on the ice sheet varies in different drainage basins with some basins melting progressively earlier over the study period. Some (but not all) of the basins also show a progressively-longer duration of melt. The short time of the study period (approximately 12 years) precludes an evaluation of statistically-significant trends. However the dataset provides valuable information on natural variability of IST, and on the ability of the MODIS instrument to capture changes in IST and melt conditions indifferent drainage basins of the ice sheet.

  12. Climate Variability, Melt-Flow Acceleration, and Ice Quakes at the Western Slope of the Greenland Ice Sheet

    NASA Astrophysics Data System (ADS)

    Steffen, K.; Zwally, J. H.; Rial, J. A.; Behar, A.; Huff, R.

    2006-12-01

    The Greenland ice sheet experienced surface melt increase over the past 15 years with record melt years in 1987, 1991, 1998, 2002 and 2005. For the western part of the ice sheet the melt area increased by 30 percent (1979-2005). Monthly mean air temperatures increased in spring and fall by 0.23 deg. C per year since 1990, extending the length of melt and total ablation. Winter air temperatures increased by as much as 0.5 deg. C per year during the past 15 years. The equilibrium line altitude ranged between 400 and 1530 m above sea level at 70 deg. north along the western slope of the ice sheet for the past 15 years, equaling a horizontal distance of 100 km. The ELA has been below the Swiss Camp (1100 m elevation) in the nineties, and since 1997 moved above the Swiss Camp height. An increase in ELA leads to an increase in melt water run-off which has been verified by regional model studies (high-resolution re-analysis). Interannual variability of snow accumulation varies from 0.3 to 2.0 m, whereas snow and ice ablation ranges from 0 to 1.5 m water equivalent at Swiss Camp during 1990-2005. A GPS network (10 stations) monitors ice velocity, acceleration, and surface height change at high temporal resolution throughout the year. The network covers a range of 500 and 1500 m above sea level, close to the Ilulissat Icefjord World Heritage region. The ice sheet continued to accelerate during the height of the melt season with short-term velocity increases up to 100 percent, and vertical uplift rates of 0.5 m. There seems to be a good correlation between the change in ice velocity and total surface melt, suggesting that melt water penetrates to great depth through moulins and cracks, lubricating the bottom of the ice sheet. A new bore-hole video movie will be shown from a 110 m deep moulin close to Swiss Camp. A PASSCAL array of 10 portable, 3-component seismic stations deployed around Swiss Camp from May to August 2006 detected numerous microearthquakes within the ice

  13. Performance evaluation of snow and ice plows.

    DOT National Transportation Integrated Search

    2015-11-01

    Removal of ice and snow from road surfaces is a critical task in the northern tier of the United States, : including Illinois. Highways with high levels of traffic are expected to be cleared of snow and ice quickly : after each snow storm. This is ne...

  14. MODIS Snow and Ice Products from the NSIDC DAAC

    NASA Technical Reports Server (NTRS)

    Scharfen, Greg R.; Hall, Dorothy K.; Riggs, George A.

    1997-01-01

    The National Snow and Ice Data Center (NSIDC) Distributed Active Archive Center (DAAC) provides data and information on snow and ice processes, especially pertaining to interactions among snow, ice, atmosphere and ocean, in support of research on global change detection and model validation, and provides general data and information services to cryospheric and polar processes research community. The NSIDC DAAC is an integral part of the multi-agency-funded support for snow and ice data management services at NSIDC. The Moderate Resolution Imaging Spectroradiometer (MODIS) will be flown on the first Earth Observation System (EOS) platform (AM-1) in 1998. The MODIS Instrument Science Team is developing geophysical products from data collected by the MODIS instrument, including snow and ice products which will be archived and distributed by NSIDC DAAC. The MODIS snow and ice mapping algorithms will generate global snow, lake ice, and sea ice cover products on a daily basis. These products will augment the existing record of satellite-derived snow cover and sea ice products that began about 30 years ago. The characteristics of these products, their utility, and comparisons to other data set are discussed. Current developments and issues are summarized.

  15. Ice shelf snow accumulation rates from the Amundsen-Bellingshausen Sea sector of West Antarctica derived from airborne radar

    NASA Astrophysics Data System (ADS)

    Medley, B.; Kurtz, N. T.; Brunt, K. M.

    2015-12-01

    The large ice shelves surrounding the Antarctic continent buttress inland ice, limiting the grounded ice-sheet flow. Many, but not all, of the thick ice shelves located along the Amundsen-Bellingshausen Seas are experiencing rapid thinning due to enhanced basal melting driven by the intrusion of warm circumpolar deep water. Determination of their mass balance provides an indicator as to the future of the shelves buttressing capability; however, measurements of surface accumulation are few, limiting the precision of the mass balance estimates. Here, we present new radar-derived measurements of snow accumulation primarily over the Getz and Abbott Ice Shelves, as well as the Dotson and Crosson, which have been the focus of several of NASA's Operation IceBridge airborne surveys between 2009 and 2014. Specifically, we use the Center for Remote Sensing of Ice Sheets (CReSIS) snow radar to map the near-surface (< 30 m) internal stratigraphy to measure snow accumulation. Due to the complexities of the local topography (e.g., ice rises and rumples) and their relative proximity to the ocean, the spatial pattern of accumulation can be equally varied. Therefore, atmospheric models might not be able to reproduce these small-scale features because of their limited spatial resolution. To evaluate whether this is the case over these narrow shelves, we will compare the radar-derived accumulation rates with those from atmospheric models.

  16. Climate Sensitivity Studies of the Greenland Ice Sheet Using Satellite AVHRR, SMMR, SSM/I and in Situ Data

    NASA Technical Reports Server (NTRS)

    Steffen, K.; Abdalati, W.; Stroeve, J.

    1993-01-01

    The feasibility of using satellite data for climate research over the Greenland ice sheet is discussed. In particular, we demonstrate the usefulness of Advanced Very High Resolution Radiometer (AVHRR) Local Area Coverage (LAC) and Global Area Coverage (GAC) data for narrow-band albedo retrieval. Our study supports the use of lower resolution AVHRR (GAC) data for process studies over most of the Greenland ice sheet. Based on LAC data time series analysis, we can resolve relative albedo changes on the order of 2-5%. In addition, we examine Scanning Multichannel Microwave Radiometer (SMMR) and Special Sensor Microwave Imager (SSM/I) passive microwave data for snow typing and other signals of climatological significance. Based on relationships between in situ measurements and horizontally polarized 19 and 37 GHz observations, wet snow regions are identified. The wet snow regions increase in aerial percentage from 9% of the total ice surface in June to a maximum of 26% in August 1990. Furthermore, the relationship between brightness temperatures and accumulation rates in the northeastern part of Greenland is described. We found a consistent increase in accumulation rate for the northeastern part of the ice sheet from 1981 to 1986.

  17. 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.

  18. Snowmelt on the Greenland Ice Sheet as Derived From Passive Microwave Satellite Data

    NASA Technical Reports Server (NTRS)

    Abdalati, Waleed; Steffen, Konrad

    1997-01-01

    The melt extent of the snow on the Greenland ice sheet is of considerable importance to the ice sheet's mass and energy balance, as well as Arctic and global climates. By comparing passive microwave satellite data to field observations, variations 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 variations in snowmelt extent of the ice sheet are studied. The melt is found to be most extensive on the western side of the ice 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.

  19. Snow and ice ecosystems: not so extreme.

    PubMed

    Maccario, Lorrie; Sanguino, Laura; Vogel, Timothy M; Larose, Catherine

    2015-12-01

    Snow and ice environments cover up to 21% of the Earth's surface. They have been regarded as extreme environments because of their low temperatures, high UV irradiation, low nutrients and low water availability, and thus, their microbial activity has not been considered relevant from a global microbial ecology viewpoint. In this review, we focus on why snow and ice habitats might not be extreme from a microbiological perspective. Microorganisms interact closely with the abiotic conditions imposed by snow and ice habitats by having diverse adaptations, that include genetic resistance mechanisms, to different types of stresses in addition to inhabiting various niches where these potential stresses might be reduced. The microbial communities inhabiting snow and ice are not only abundant and taxonomically diverse, but complex in terms of their interactions. Altogether, snow and ice seem to be true ecosystems with a role in global biogeochemical cycles that has likely been underestimated. Future work should expand past resistance studies to understanding the function of these ecosystems. Copyright © 2015 Institut Pasteur. Published by Elsevier Masson SAS. All rights reserved.

  20. Ice sheet altimetry

    NASA Technical Reports Server (NTRS)

    Brooks, R. L.

    1981-01-01

    Generalized surface slopes were computed for the Antarctic and Greenland ice sheets by differencing plotted contour levels and dividing them by the distance between the contours. It was observed that more than 90% of the ice sheets have surface slopes less than 1%. Seasat test mode-1 Seasat altimeter measurements over Greenland were analyzed by comparisons with collinear and intersecting normal mode Seasat altimeter passes. Over the ice sheet, the computed surface elevations from test mode-1 measurements were consistently lower by about 45 m and the AGC levels were down by approximately 6 dB. No test mode-1 data were acquired over Antarctica. It is concluded that analysis of the existing altimeter data base over the two ice sheets is crucial in designing a future improved altimeter tracking capability. It is recommended that additional waveform retracking be performed to characterize ice sheet topography as a function of geographic area and elevation.

  1. Spatiotemporal Variability of Meltwater Refreezing in Southwest Greenland Ice Sheet Firn

    NASA Astrophysics Data System (ADS)

    Rennermalm, A. K.; Hock, R.; Tedesco, M.; Corti, G.; Covi, F.; Miège, C.; Kingslake, J.; Leidman, S. Z.; Munsell, S.

    2017-12-01

    A substantial fraction of the summer meltwater formed on the surface of the Greenland ice sheet is retained in firn, while the remaining portion runs to the ocean through surface and subsurface channels. Refreezing of meltwater in firn can create impenetrable ice lenses, hence being a crucial process in the redistribution of surface runoff. To quantify the impact of refreezing on runoff and current and future Greenland surface mass balance, a three year National Science Foundation funded project titled "Refreezing in the firn of the Greenland ice sheet: Spatiotemporal variability and implications for ice sheet mass balance" started this past year. Here we present an overview of the project and some initial results from the first field season in May 2017 conducted in proximity of the DYE-2 site in the percolation zone of the Southwest Greenland ice sheet at elevations between 1963 and 2355 m a.s.l.. During this fieldwork two automatic weather stations were deployed, outfitted with surface energy balance sensors and 16 m long thermistor strings, over 300 km of ground penetrating radar data were collected, and five 20-26 m deep firn cores were extracted and analyzed for density and stratigraphy. Winter snow accumulation was measured along the radar tracks. Preliminary work on the firn-core data reveals increasing frequency and thickness of ice lenses at lower ice-sheet elevations, in agreement with other recent work in the area. Data collected within this project will facilitate advances in our understanding of the spatiotemporal variability of firn refreezing and its role in the hydrology and surface mass balance of the Greenland Ice Sheet.

  2. Recent Changes in Arctic Glaciers, Ice Caps, and the Greenland Ice Sheet: Cold Facts About Warm Ice

    NASA Astrophysics Data System (ADS)

    Abdalati, W.

    2005-12-01

    One of the major manifestations of Arctic change can be observed in the state of balance of Arctic glaciers and ice caps and the Greenland ice sheet. These ice masses are estimated to contain nearly 3 million cubic kilometers of ice, 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 ice masses have been shrinking in recent in years, but their mass balance is highly variable on a wide range of spatial and temporal scales. On the Greenland ice 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 ice sheet change to a warming climate. At the same time, however, the vast interior regions of the Greenland ice 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 ice caps have been shrinking in the past few decades, and in Canada and Alaska, the rate of ice 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 ice mass 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.

  3. Winter snow conditions on Arctic sea ice north of Svalbard during the Norwegian young sea ICE (N-ICE2015) expedition

    NASA Astrophysics Data System (ADS)

    Merkouriadi, Ioanna; Gallet, Jean-Charles; Graham, Robert M.; Liston, Glen E.; Polashenski, Chris; Rösel, Anja; Gerland, Sebastian

    2017-10-01

    Snow is a crucial component of the Arctic sea ice system. Its thickness and thermal properties control heat conduction and radiative fluxes across the ocean, ice, and atmosphere interfaces. Hence, observations of the evolution of snow depth, density, thermal conductivity, and stratigraphy are crucial for the development of detailed snow numerical models predicting energy transfer through the snow pack. Snow depth is also a major uncertainty in predicting ice thickness using remote sensing algorithms. Here we examine the winter spatial and temporal evolution of snow physical properties on first-year (FYI) and second-year ice (SYI) in the Atlantic sector of the Arctic Ocean, during the Norwegian young sea ICE (N-ICE2015) expedition (January to March 2015). During N-ICE2015, the snow pack consisted of faceted grains (47%), depth hoar (28%), and wind slab (13%), indicating very different snow stratigraphy compared to what was observed in the Pacific sector of the Arctic Ocean during the SHEBA campaign (1997-1998). Average snow bulk density was 345 kg m-3 and it varied with ice type. Snow depth was 41 ± 19 cm in January and 56 ± 17 cm in February, which is significantly greater than earlier suggestions for this region. The snow water equivalent was 14.5 ± 5.3 cm over first-year ice and 19 ± 5.4 cm over second-year ice.

  4. An Ultra-Wideband, Microwave Radar for Measuring Snow Thickness on Sea Ice and Mapping Near-Surface Internal Layers in Polar Firn

    NASA Technical Reports Server (NTRS)

    Panzer, Ben; Gomez-Garcia, Daniel; Leuschen, Carl; Paden, John; Rodriguez-Morales, Fernando; Patel, Azsa; Markus, Thorsten; Holt, Benjamin; Gogineni, Prasad

    2013-01-01

    Sea ice is generally covered with snow, which can vary in thickness from a few centimeters to >1 m. Snow cover acts as a thermal insulator modulating the heat exchange between the ocean and the atmosphere, and it impacts sea-ice growth rates and overall thickness, a key indicator of climate change in polar regions. Snow depth is required to estimate sea-ice thickness using freeboard measurements made with satellite altimeters. The snow cover also acts as a mechanical load that depresses ice freeboard (snow and ice above sea level). Freeboard depression can result in flooding of the snow/ice interface and the formation of a thick slush layer, particularly in the Antarctic sea-ice cover. The Center for Remote Sensing of Ice Sheets (CReSIS) has developed an ultra-wideband, microwave radar capable of operation on long-endurance aircraft to characterize the thickness of snow over sea ice. The low-power, 100mW signal is swept from 2 to 8GHz allowing the air/snow and snow/ ice interfaces to be mapped with 5 c range resolution in snow; this is an improvement over the original system that worked from 2 to 6.5 GHz. From 2009 to 2012, CReSIS successfully operated the radar on the NASA P-3B and DC-8 aircraft to collect data on snow-covered sea ice in the Arctic and Antarctic for NASA Operation IceBridge. The radar was found capable of snow depth retrievals ranging from 10cm to >1 m. We also demonstrated that this radar can be used to map near-surface internal layers in polar firn with fine range resolution. Here we describe the instrument design, characteristics and performance of the radar.

  5. First Moderate Resolution Imaging Spectroradiometer (MODIS) Snow and Ice Workshop

    NASA Technical Reports Server (NTRS)

    Hall, Dorothy K. (Editor)

    1995-01-01

    This document is a compilation of summaries of talks presented at a 2-day workshop on Moderate Resolution maging Spectroradiometer (MODIS) snow and ice products. The objectives of the workshop were to: inform the snow and ce community of potential MODIS products, seek advice from the participants regarding the utility of the products, and letermine the needs for future post-launch MODIS snow and ice products. Four working groups were formed to discuss at-launch snow products, at-launch ice products, post-launch snow and ice products and utility of MODIS snow and ice products, respectively. Each working group presented recommendations at the conclusion of the workshop.

  6. Coupled energy-balance/ice-sheet model simulations of the glacial cycle: A possible connection between terminations and terrigenous dust

    NASA Astrophysics Data System (ADS)

    Peltier, W. Richard; Marshall, Shawn

    1995-07-01

    We apply a coupled energy-balance/ice-sheet climate model in an investigation of northern hemisphere ice-sheet advance and retreat over the last glacial cycle. When driven only by orbital insolation variations, the model predicts ice-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 ice masses. The orbital forcing alone, however, is unable to induce the observed rapid ice-sheet retreat, and we conclude that additional climatic feedbacks not explicitly included in the basic model must be acting. In the analyses presented here we have parameterized a number of potentially important effects in order to test their relative influence on the process of glacial termination. These include marine instability, thermohaline circulation effects, carbon dioxide variations, and snow albedo changes caused by dust loading during periods of high atmospheric aerosol concentration. For the purpose of these analyses the temporal changes in the latter two variables were inferred from ice core records. Of these various influences, our analyses suggest that the albedo variations in the ice-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 ice sheet ensues. The last glacial maximum configurations of the Laurentide and Fennoscandian complexes are also brought into much closer accord with the ICE-3G reconstruction of Tushingham and Peltier (1991,1992) and the ICE-4G reconstruction of Peltier (1994) when this effect is reasonably introduced.

  7. The Rapid Ice Sheet Change Observatory (RISCO)

    NASA Astrophysics Data System (ADS)

    Morin, P.; Howat, I. M.; Ahn, Y.; Porter, C.; McFadden, E. M.

    2010-12-01

    The recent expansion of observational capacity from space has revealed dramatic, rapid changes in the Earth’s ice cover. These discoveries have fundamentally altered how scientists view ice-sheet change. Instead of just slow changes in snow accumulation and melting over centuries or millennia, important changes can occur in sudden events lasting only months, weeks, or even a single day. Our understanding of these short time- and space-scale processes, which hold important implications for future global sea level rise, has been impeded by the low temporal and spatial resolution, delayed sensor tasking, incomplete coverage, inaccessibility and/or high cost of data available to investigators. New cross-agency partnerships and data access policies provide the opportunity to dramatically improve the resolution of ice sheet observations by an order of magnitude, from timescales of months and distances of 10’s of meters, to days and meters or less. Advances in image processing technology also enable application of currently under-utilized datasets. The infrastructure for systematically gathering, processing, analyzing and distributing these data does not currently exist. Here we present the development of a multi-institutional, multi-platform observatory for rapid ice change with the ultimate objective of helping to elucidate the relevant timescales and processes of ice sheet dynamics and response to climate change. The Rapid Ice Sheet Observatory (RISCO) gathers observations of short time- and space-scale Cryosphere events and makes them easily accessible to investigators, media and general public. As opposed to existing data centers, which are structured to archive and distribute diverse types of raw data to end users with the specialized software and skills to analyze them, RISCO focuses on three types of geo-referenced raster (image) data products in a format immediately viewable with commonly available software. These three products are (1) sequences of images

  8. Sensitivities of Greenland ice sheet volume inferred from an ice sheet adjoint model

    NASA Astrophysics Data System (ADS)

    Heimbach, P.; Bugnion, V.

    2009-04-01

    We present a new and original approach to understanding the sensitivity of the Greenland ice sheet to key model parameters and environmental conditions. At the heart of this approach is the use of an adjoint ice sheet model. Since its introduction by MacAyeal (1992), the adjoint method has become widespread to fit ice stream models to the increasing number and diversity of satellite observations, and to estimate uncertain model parameters such as basal conditions. However, no attempt has been made to extend this method to comprehensive ice sheet models. As a first step toward the use of adjoints of comprehensive three-dimensional ice sheet models we have generated an adjoint of the ice sheet model SICOPOLIS of Greve (1997). The adjoint was generated by means of the automatic differentiation (AD) tool TAF. The AD tool generates exact source code representing the tangent linear and adjoint model of the nonlinear parent model provided. Model sensitivities are given by the partial derivatives of a scalar-valued model diagnostic with respect to the controls, and can be efficiently calculated via the adjoint. By way of example, we determine the sensitivity of the total Greenland ice volume to various control variables, such as spatial fields of basal flow parameters, surface and basal forcings, and initial conditions. Reliability of the adjoint was tested through finite-difference perturbation calculations for various control variables and perturbation regions. Besides confirming qualitative aspects of ice sheet sensitivities, such as expected regional variations, we detect regions where model sensitivities are seemingly unexpected or counter-intuitive, albeit ``real'' in the sense of actual model behavior. An example is inferred regions where sensitivities of ice sheet volume to basal sliding coefficient are positive, i.e. where a local increase in basal sliding parameter increases the ice sheet volume. Similarly, positive ice temperature sensitivities in certain parts

  9. Snow and Ice Applications of AVHRR in Polar Regions: Report of a Workshop

    NASA Technical Reports Server (NTRS)

    Steffen, K.; Bindschadler, R.; Casassa, G.; Comiso, J.; Eppler, D.; Fetterer, F.; Hawkins, J.; Key, J.; Rothrock, D.; Thomas, R.; hide

    1993-01-01

    The third symposium on Remote Sensing of Snow and Ice, organized by the International Glaciological Society, took place in Boulder, Colorado, 17-22 May 1992. As part of this meeting a total of 21 papers was presented on snow and ice applications of Advanced Very High Resolution Radiometer (AVHRR) satellite data in polar regions. Also during this meeting a NASA sponsored Workshop was held to review the status of polar surface measurements from AVHRR. In the following we have summarized the ideas and recommendations from the workshop, and the conclusions of relevant papers given during the regular symposium sessions. The seven topics discussed include cloud masking, ice surface temperature, narrow-band albedo, ice concentration, lead statistics, sea-ice motion and ice-sheet studies with specifics on applications, algorithms and accuracy, following recommendations for future improvements. In general, we can affirm the strong potential of AVHRR for studying sea ice and snow covered surfaces, and we highly recommend this satellite data set for long-term monitoring of polar process studies. However, progress is needed to reduce the uncertainty of the retrieved parameters for all of the above mentioned topics to make this data set useful for direct climate applications such as heat balance studies and others. Further, the acquisition and processing of polar AVHRR data must become better coordinated between receiving stations, data centers and funding agencies to guarantee a long-term commitment to the collection and distribution of high quality data.

  10. Snow Radar Derived Surface Elevations and Snow Depths Multi-Year Time Series over Greenland Sea-Ice During IceBridge Campaigns

    NASA Astrophysics Data System (ADS)

    Perkovic-Martin, D.; Johnson, M. P.; Holt, B.; Panzer, B.; Leuschen, C.

    2012-12-01

    This paper presents estimates of snow depth over sea ice from the 2009 through 2011 NASA Operation IceBridge [1] spring campaigns over Greenland and the Arctic Ocean, derived from Kansas University's wideband Snow Radar [2] over annually repeated sea-ice transects. We compare the estimates of the top surface interface heights between NASA's Atmospheric Topographic Mapper (ATM) [3] and the Snow Radar. We follow this by comparison of multi-year snow depth records over repeated sea-ice transects to derive snow depth changes over the area. For the purpose of this paper our analysis will concentrate on flights over North/South basin transects off Greenland, which are the closest overlapping tracks over this time period. The Snow Radar backscatter returns allow for surface and interface layer types to be differentiated between snow, ice, land and water using a tracking and classification algorithm developed and discussed in the paper. The classification is possible due to different scattering properties of surfaces and volumes at the radar's operating frequencies (2-6.5 GHz), as well as the geometries in which they are viewed by the radar. These properties allow the returns to be classified by a set of features that can be used to identify the type of the surface or interfaces preset in each vertical profile. We applied a Support Vector Machine (SVM) learning algorithm [4] to the Snow Radar data to classify each detected interface into one of four types. The SVM algorithm was trained on radar echograms whose interfaces were visually classified and verified against coincident aircraft data obtained by CAMBOT [5] and DMS [6] imaging sensors as well as the scanning ATM lidar. Once the interface locations were detected for each vertical profile we derived a range to each interface that was used to estimate the heights above the WGS84 ellipsoid for direct comparisons with ATM. Snow Radar measurements were calibrated against ATM data over areas free of snow cover and over GPS

  11. Assessment of climate variability of the Greenland Ice Sheet: Integration of in situ and satellite data

    NASA Technical Reports Server (NTRS)

    Steffen, K.; Abdalati, W.; Stroeve, J.; Key, J.

    1994-01-01

    The proposed research involves the application of multispectral satellite data in combination with ground truth measurements to monitor surface properties of the Greenland Ice Sheet which are essential for describing the energy and mass of the ice sheet. Several key components of the energy balance are parameterized using satellite data and in situ measurements. The analysis will be done for a ten year time period in order to get statistics on the seasonal and interannual variations of the surface processes and the climatology. Our goal is to investigate to what accuracy and over what geographic areas large scale snow properties and radiative fluxes can be derived based upon a combination of available remote sensing and meteorological data sets. Operational satellite sensors are calibrated based on ground measurements and atmospheric modeling prior to large scale analysis to ensure the quality of the satellite data. Further, several satellite sensors of different spatial and spectral resolution are intercompared to access the parameter accuracy. Proposed parameterization schemes to derive key component of the energy balance from satellite data are validated. For the understanding of the surface processes a field program was designed to collect information on spectral albedo, specular reflectance, soot content, grain size and the physical properties of different snow types. Further, the radiative and turbulent fluxes at the ice/snow surface are monitored for the parameterization and interpretation of the satellite data. The expected results include several baseline data sets of albedo, surface temperature, radiative fluxes, and different snow types of the entire Greenland Ice Sheet. These climatological data sets will be of potential use for climate sensitivity studies in the context of future climate change.

  12. An ice sheet model validation framework for the Greenland ice sheet

    NASA Astrophysics Data System (ADS)

    Price, Stephen F.; Hoffman, Matthew J.; Bonin, Jennifer A.; Howat, Ian M.; Neumann, Thomas; Saba, Jack; Tezaur, Irina; Guerber, Jeffrey; Chambers, Don P.; Evans, Katherine J.; Kennedy, Joseph H.; Lenaerts, Jan; Lipscomb, William H.; Perego, Mauro; Salinger, Andrew G.; Tuminaro, Raymond S.; van den Broeke, Michiel R.; Nowicki, Sophie M. J.

    2017-01-01

    We propose a new ice sheet model validation framework - the Cryospheric Model Comparison Tool (CmCt) - that takes advantage of ice sheet altimetry and gravimetry observations collected over the past several decades and is applied here to modeling of the Greenland ice sheet. We use realistic simulations performed with the Community Ice Sheet Model (CISM) along with two idealized, non-dynamic models to demonstrate the framework and its use. Dynamic simulations with CISM are forced from 1991 to 2013, using combinations of reanalysis-based surface mass balance and observations of outlet glacier flux change. We propose and demonstrate qualitative and quantitative metrics for use in evaluating the different model simulations against the observations. We find that the altimetry observations used here are largely ambiguous in terms of their ability to distinguish one simulation from another. Based on basin-scale and whole-ice-sheet-scale metrics, we find that simulations using both idealized conceptual models and dynamic, numerical models provide an equally reasonable representation of the ice sheet surface (mean elevation differences of < 1 m). This is likely due to their short period of record, biases inherent to digital elevation models used for model initial conditions, and biases resulting from firn dynamics, which are not explicitly accounted for in the models or observations. On the other hand, we find that the gravimetry observations used here are able to unambiguously distinguish between simulations of varying complexity, and along with the CmCt, can provide a quantitative score for assessing a particular model and/or simulation. The new framework demonstrates that our proposed metrics can distinguish relatively better from relatively worse simulations and that dynamic ice sheet models, when appropriately initialized and forced with the right boundary conditions, demonstrate a predictive skill with respect to observed dynamic changes that have occurred on

  13. An ice sheet model validation framework for the Greenland ice sheet

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

    Price, Stephen F.; Hoffman, Matthew J.; Bonin, Jennifer A.

    We propose a new ice sheet model validation framework the Cryospheric Model Comparison Tool (CMCT) that takes advantage of ice sheet altimetry and gravimetry observations collected over the past several decades and is applied here to modeling of the Greenland ice sheet. We use realistic simulations performed with the Community Ice Sheet Model (CISM) along with two idealized, non-dynamic models to demonstrate the framework and its use. Dynamic simulations with CISM are forced from 1991 to 2013 using combinations of reanalysis-based surface mass balance and observations of outlet glacier flux change. We propose and demonstrate qualitative and quanti- tative metricsmore » for use in evaluating the different model simulations against the observations. We find 10 that the altimetry observations used here are largely ambiguous in terms of their ability to distinguish one simulation from another. Based on basin- and whole-ice-sheet scale metrics, the model initial condition as well as output from idealized and dynamic models all provide an equally reasonable representation of the ice sheet surface (mean elevation differences of <1 m). This is likely due to their short period of record, biases inherent to digital elevation models used for model initial conditions, and biases resulting from firn dynamics, which are not explicitly accounted for in the models or observations. On the other hand, we find that the gravimetry observations used here are able to unambiguously distinguish between simulations of varying complexity, and along with the CMCT, can provide a quantitative score for assessing a particular model and/or simulation. The new framework demonstrates that our proposed metrics can distinguish relatively better from relatively worse simulations and that dynamic ice sheet models, when appropriately initialized and forced with the right boundary conditions, demonstrate predictive skill with respect to observed dynamic changes occurring on Greenland over the past few

  14. An ice sheet model validation framework for the Greenland ice sheet

    PubMed Central

    Price, Stephen F.; Hoffman, Matthew J.; Bonin, Jennifer A.; Howat, Ian M.; Neumann, Thomas; Saba, Jack; Tezaur, Irina; Guerber, Jeffrey; Chambers, Don P.; Evans, Katherine J.; Kennedy, Joseph H.; Lenaerts, Jan; Lipscomb, William H.; Perego, Mauro; Salinger, Andrew G.; Tuminaro, Raymond S.; van den Broeke, Michiel R.; Nowicki, Sophie M. J.

    2018-01-01

    We propose a new ice sheet model validation framework – the Cryospheric Model Comparison Tool (CmCt) – that takes advantage of ice sheet altimetry and gravimetry observations collected over the past several decades and is applied here to modeling of the Greenland ice sheet. We use realistic simulations performed with the Community Ice Sheet Model (CISM) along with two idealized, non-dynamic models to demonstrate the framework and its use. Dynamic simulations with CISM are forced from 1991 to 2013 using combinations of reanalysis-based surface mass balance and observations of outlet glacier flux change. We propose and demonstrate qualitative and quantitative metrics for use in evaluating the different model simulations against the observations. We find that the altimetry observations used here are largely ambiguous in terms of their ability to distinguish one simulation from another. Based on basin- and whole-ice-sheet scale metrics, we find that simulations using both idealized conceptual models and dynamic, numerical models provide an equally reasonable representation of the ice sheet surface (mean elevation differences of <1 m). This is likely due to their short period of record, biases inherent to digital elevation models used for model initial conditions, and biases resulting from firn dynamics, which are not explicitly accounted for in the models or observations. On the other hand, we find that the gravimetry observations used here are able to unambiguously distinguish between simulations of varying complexity, and along with the CmCt, can provide a quantitative score for assessing a particular model and/or simulation. The new framework demonstrates that our proposed metrics can distinguish relatively better from relatively worse simulations and that dynamic ice sheet models, when appropriately initialized and forced with the right boundary conditions, demonstrate predictive skill with respect to observed dynamic changes occurring on Greenland over the

  15. An ice sheet model validation framework for the Greenland ice sheet.

    PubMed

    Price, Stephen F; Hoffman, Matthew J; Bonin, Jennifer A; Howat, Ian M; Neumann, Thomas; Saba, Jack; Tezaur, Irina; Guerber, Jeffrey; Chambers, Don P; Evans, Katherine J; Kennedy, Joseph H; Lenaerts, Jan; Lipscomb, William H; Perego, Mauro; Salinger, Andrew G; Tuminaro, Raymond S; van den Broeke, Michiel R; Nowicki, Sophie M J

    2017-01-01

    We propose a new ice sheet model validation framework - the Cryospheric Model Comparison Tool (CmCt) - that takes advantage of ice sheet altimetry and gravimetry observations collected over the past several decades and is applied here to modeling of the Greenland ice sheet. We use realistic simulations performed with the Community Ice Sheet Model (CISM) along with two idealized, non-dynamic models to demonstrate the framework and its use. Dynamic simulations with CISM are forced from 1991 to 2013 using combinations of reanalysis-based surface mass balance and observations of outlet glacier flux change. We propose and demonstrate qualitative and quantitative metrics for use in evaluating the different model simulations against the observations. We find that the altimetry observations used here are largely ambiguous in terms of their ability to distinguish one simulation from another. Based on basin- and whole-ice-sheet scale metrics, we find that simulations using both idealized conceptual models and dynamic, numerical models provide an equally reasonable representation of the ice sheet surface (mean elevation differences of <1 m). This is likely due to their short period of record, biases inherent to digital elevation models used for model initial conditions, and biases resulting from firn dynamics, which are not explicitly accounted for in the models or observations. On the other hand, we find that the gravimetry observations used here are able to unambiguously distinguish between simulations of varying complexity, and along with the CmCt, can provide a quantitative score for assessing a particular model and/or simulation. The new framework demonstrates that our proposed metrics can distinguish relatively better from relatively worse simulations and that dynamic ice sheet models, when appropriately initialized and forced with the right boundary conditions, demonstrate predictive skill with respect to observed dynamic changes occurring on Greenland over the past

  16. An ice sheet model validation framework for the Greenland ice sheet

    DOE PAGES

    Price, Stephen F.; Hoffman, Matthew J.; Bonin, Jennifer A.; ...

    2017-01-17

    We propose a new ice sheet model validation framework the Cryospheric Model Comparison Tool (CMCT) that takes advantage of ice sheet altimetry and gravimetry observations collected over the past several decades and is applied here to modeling of the Greenland ice sheet. We use realistic simulations performed with the Community Ice Sheet Model (CISM) along with two idealized, non-dynamic models to demonstrate the framework and its use. Dynamic simulations with CISM are forced from 1991 to 2013 using combinations of reanalysis-based surface mass balance and observations of outlet glacier flux change. We propose and demonstrate qualitative and quanti- tative metricsmore » for use in evaluating the different model simulations against the observations. We find 10 that the altimetry observations used here are largely ambiguous in terms of their ability to distinguish one simulation from another. Based on basin- and whole-ice-sheet scale metrics, the model initial condition as well as output from idealized and dynamic models all provide an equally reasonable representation of the ice sheet surface (mean elevation differences of <1 m). This is likely due to their short period of record, biases inherent to digital elevation models used for model initial conditions, and biases resulting from firn dynamics, which are not explicitly accounted for in the models or observations. On the other hand, we find that the gravimetry observations used here are able to unambiguously distinguish between simulations of varying complexity, and along with the CMCT, can provide a quantitative score for assessing a particular model and/or simulation. The new framework demonstrates that our proposed metrics can distinguish relatively better from relatively worse simulations and that dynamic ice sheet models, when appropriately initialized and forced with the right boundary conditions, demonstrate predictive skill with respect to observed dynamic changes occurring on Greenland over the past few

  17. An Ice Sheet Model Validation Framework for the Greenland Ice Sheet

    NASA Technical Reports Server (NTRS)

    Price, Stephen F.; Hoffman, Matthew J.; Bonin, Jennifer A.; Howat, Ian M.; Neumann, Thomas A.; Saba, Jack; Tezaur, Irina; Guerber, Jeffrey R.; Chambers, Don P.; Evans, Katherine J.; hide

    2017-01-01

    We propose a new ice sheet model validation framework - the Cryospheric Model Comparison Tool (CmCt) - that takes advantage of ice sheet altimetry and gravimetry observations collected over the past several decades and is applied here to modeling of the Greenland ice sheet. We use realistic simulations performed with the Community Ice Sheet Model (CISM) along with two idealized, non-dynamic models to demonstrate the framework and its use. Dynamic simulations with CISM are forced from 1991 to 2013, using combinations of reanalysis-based surface mass balance and observations of outlet glacier flux change. We propose and demonstrate qualitative and quantitative metrics for use in evaluating the different model simulations against the observations. We find that the altimetry observations used here are largely ambiguous in terms of their ability to distinguish one simulation from another. Based on basin-scale and whole-ice-sheet-scale metrics, we find that simulations using both idealized conceptual models and dynamic, numerical models provide an equally reasonable representation of the ice sheet surface (mean elevation differences of less than 1 meter). This is likely due to their short period of record, biases inherent to digital elevation models used for model initial conditions, and biases resulting from firn dynamics, which are not explicitly accounted for in the models or observations. On the other hand, we find that the gravimetry observations used here are able to unambiguously distinguish between simulations of varying complexity, and along with the CmCt, can provide a quantitative score for assessing a particular model and/or simulation. The new framework demonstrates that our proposed metrics can distinguish relatively better from relatively worse simulations and that dynamic ice sheet models, when appropriately initialized and forced with the right boundary conditions, demonstrate a predictive skill with respect to observed dynamic changes that have occurred

  18. On the influence of recrystallization on snow fabric and microstructure: study of a snow profile in Central East Antarctica

    NASA Astrophysics Data System (ADS)

    Calonne, Neige; Schneebeli, Martin; Montagnat, Maurine; Matzl, Margret

    2016-04-01

    Temperature gradient metamorphism affects the Antarctic snowpack up to 5 meters depth, which lead to a recrystallization of the ice grains by sublimation of ice and deposition of water vapor. By this way, it is well known that the snow microstructure evolves (geometrical changes). Also, a recent study shows an evolution of the snow fabric, based on a cold laboratory experiment. Both fabric and microstructure are required to better understand mechanical behavior and densification of snow, firn and ice, given polar climatology. The fabric of firn and ice has been extensively investigated, but the publications by Stephenson (1967, 1968) are to our knowledge the only ones describing the snow fabric in Antarctica. In this context, our work focuses on snow microstructure and fabric in the first meters depth of the Antarctic ice sheet, where temperature gradients driven recrystallization occurs. Accurate details of the snow microstructure are observed using micro-computed tomography. Snow fabrics were measured at various depths from thin sections of impregnated snow with an Automatic Ice Texture Analyzer (AITA). A definite relationship between microstructure and fabric is found and highlights the influence of metamorphism on both properties. Our results also show that the metamorphism enhances the differences between the snow layers properties. Our work stresses the significant and complex evolution of snow properties in the upper meters of the ice sheet and opens the question of how these layer properties will evolve at depth and may influence the densification.

  19. The Effects of Snow Depth Forcing on Southern Ocean Sea Ice Simulations

    NASA Technical Reports Server (NTRS)

    Powel, Dylan C.; Markus, Thorsten; Stoessel, Achim

    2003-01-01

    The spatial and temporal distribution of snow on sea ice is an important factor for sea ice and climate models. First, it acts as an efficient insulator between the ocean and the atmosphere, and second, snow is a source of fresh water for altering the already weak Southern Ocean stratification. For the Antarctic, where the ice thickness is relatively thin, snow can impact the ice thickness in two ways: a) As mentioned above snow on sea ice reduces the ocean-atmosphere heat flux and thus reduces freezing at the base of the ice flows; b) a heavy snow load can suppress the ice below sea level which causes flooding and, with subsequent freezing, a thickening of the sea ice (snow-to-ice conversion). In this paper, we compare different snow fall paramterizations (incl. the incorporation of satellite-derived snow depth) and study the effect on the sea ice using a sea ice model.

  20. Canadian snow and sea ice: historical trends and projections

    NASA Astrophysics Data System (ADS)

    Mudryk, Lawrence R.; Derksen, Chris; Howell, Stephen; Laliberté, Fred; Thackeray, Chad; Sospedra-Alfonso, Reinel; Vionnet, Vincent; Kushner, Paul J.; Brown, Ross

    2018-04-01

    The Canadian Sea Ice and Snow Evolution (CanSISE) Network is a climate research network focused on developing and applying state of the art observational data to advance dynamical prediction, projections, and understanding of seasonal snow cover and sea ice in Canada and the circumpolar Arctic. Here, we present an assessment from the CanSISE Network on trends in the historical record of snow cover (fraction, water equivalent) and sea ice (area, concentration, type, and thickness) across Canada. We also assess projected changes in snow cover and sea ice likely to occur by mid-century, as simulated by the Coupled Model Intercomparison Project Phase 5 (CMIP5) suite of Earth system models. The historical datasets show that the fraction of Canadian land and marine areas covered by snow and ice is decreasing over time, with seasonal and regional variability in the trends consistent with regional differences in surface temperature trends. In particular, summer sea ice cover has decreased significantly across nearly all Canadian marine regions, and the rate of multi-year ice loss in the Beaufort Sea and Canadian Arctic Archipelago has nearly doubled over the last 8 years. The multi-model consensus over the 2020-2050 period shows reductions in fall and spring snow cover fraction and sea ice concentration of 5-10 % per decade (or 15-30 % in total), with similar reductions in winter sea ice concentration in both Hudson Bay and eastern Canadian waters. Peak pre-melt terrestrial snow water equivalent reductions of up to 10 % per decade (30 % in total) are projected across southern Canada.

  1. Assessing the Impact of Laurentide Ice-sheet Topography on Glacial Climate

    NASA Technical Reports Server (NTRS)

    Ullman, D. J.; LeGrande, A. N.; Carlson, A. E.; Anslow, F. S.; Licciardi, J. M.

    2014-01-01

    Simulations of past climates require altered boundary conditions to account for known shifts in the Earth system. For the Last Glacial Maximum (LGM) and subsequent deglaciation, the existence of large Northern Hemisphere ice sheets caused profound changes in surface topography and albedo. While ice-sheet extent is fairly well known, numerous conflicting reconstructions of ice-sheet topography suggest that precision in this boundary condition is lacking. Here we use a high-resolution and oxygen-isotopeenabled fully coupled global circulation model (GCM) (GISS ModelE2-R), along with two different reconstructions of the Laurentide Ice Sheet (LIS) that provide maximum and minimum estimates of LIS elevation, to assess the range of climate variability in response to uncertainty in this boundary condition.We present this comparison at two equilibrium time slices: the LGM, when differences in ice-sheet topography are maximized, and 14 ka, when differences in maximum ice-sheet height are smaller but still exist. Overall, we find significant differences in the climate response to LIS topography, with the larger LIS resulting in enhanced Atlantic Meridional Overturning Circulation and warmer surface air temperatures, particularly over northeastern Asia and the North Pacific. These up- and downstream effects are associated with differences in the development of planetary waves in the upper atmosphere, with the larger LIS resulting in a weaker trough over northeastern Asia that leads to the warmer temperatures and decreased albedo from snow and sea-ice cover. Differences between the 14 ka simulations are similar in spatial extent but smaller in magnitude, suggesting that climate is responding primarily to the larger difference in maximum LIS elevation in the LGM simulations. These results suggest that such uncertainty in ice-sheet boundary conditions alone may significantly impact the results of paleoclimate simulations and their ability to successfully simulate past climates

  2. Coupled ice sheet-ocean modelling to investigate ocean driven melting of marine ice sheets in Antarctica

    NASA Astrophysics Data System (ADS)

    Jong, Lenneke; Gladstone, Rupert; Galton-Fenzi, Ben

    2017-04-01

    Ocean induced melting below the ice shelves of marine ice sheets is a major source of uncertainty for predictions of ice mass loss and Antarctica's resultant contribution to future sea level rise. The floating ice shelves provide a buttressing force against the flow of ice across the grounding line into the ocean. Thinning of these ice shelves due to an increase in melting reduces this force and can lead to an increase in the discharge of grounded ice. Fully coupled modelling of ice sheet-ocean interactions is key to improving understanding the influence of the Southern ocean on the evolution of the Antarctic ice sheet, and to predicting its future behaviour under changing climate conditions. Coupling of ocean and ice sheet models is needed to provide more realistic melt rates at the base of ice shelves and hence make better predictions of the behaviour of the grounding line and the shape of the ice-shelf cavity as the ice sheet evolves. The Framework for Ice Sheet - Ocean Coupling (FISOC) has been developed to provide a flexible platform for performing coupled ice sheet - ocean modelling experiments. We present preliminary results using FISOC to couple the Regional Ocean Modelling System (ROMS) with Elmer/Ice in idealised experiments Marine Ice Sheet-Ocean Model Intercomparison Project (MISOMIP). These experiments use an idealised geometry motivated by that of Pine Island glacier and the adjacent Amundsen Sea in West Antarctica, a region which has shown shown signs of thinning ice and grounding line retreat.

  3. Assessment of Climate Variability of the Greenland Ice Sheet: Integration of In Situ and Satellite Data

    NASA Technical Reports Server (NTRS)

    Steffen, K.; Abdalati, W.; Stroeve, J.; Nolin, A.; Box, J.; Key, J.; Zwally, J.; Stober, M.; Kreuter, J.

    1996-01-01

    The proposed research involves the application of multispectral satellite data in combination with ground truth measurements to monitor surface properties of the Greenland Ice Sheet which are essential for describing the energy and mass of the ice sheet. Several key components of the energy balance are parameterized using satellite data and in situ measurements. The analysis has been done for a 6 to 17 year time period in order to analyze the seasonal and interannual variations of the surface processes and the climatology. Our goal was to investigate to what accuracy and over what geographic areas large scale snow properties and radiative fluxes can be derived based upon a combination of available remote sensing and meteorological data sets. For the understanding of the surface processes a field program was designed to collect information on spectral albedo, specular reflectance, soot content, grain size and the physical properties of different snow types. Further, the radiative and turbulent fluxes at the ice/snow surface were monitored for the parameterization and interpretation of the satellite data. Highlights include AVHRR time series and surface based radiation measurements, passive microwave time series, and geodetic results from the ETH/CU camp.

  4. How much can Greenland melt? An upper bound on mass loss from the Greenland Ice Sheet through surface melting

    NASA Astrophysics Data System (ADS)

    Liu, X.; Bassis, J. N.

    2015-12-01

    With observations showing accelerated mass loss from the Greenland Ice Sheet due to surface melt, the Greenland Ice Sheet is becoming one of the most significant contributors to sea level rise. The contribution of the Greenland Ice 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 Ice Sheet both due to uncertainty in atmospheric forcing and the ice 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 ice volume loss and related sea-level rise associated with surface melting. To estimate the upper bound, we assume the Greenland Ice Sheet is perpetually covered in thick clouds, which maximize longwave radiation to the ice sheet. We further assume that deposition of black carbon darkens the ice 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 ice sheet increases mass loss in the short term, refreezing of retained water warms the ice 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 Ice 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

  5. Satellite-derived, melt-season surface temperature of the Greenland Ice Sheet (2000-2005) and its relationship to mass balance

    USGS Publications Warehouse

    Hall, D.K.; Williams, R.S.; Casey, K.A.; DiGirolamo, N.E.; Wan, Z.

    2006-01-01

    Mean, clear-sky surface temperature of the Greenland Ice 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 ice 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 ice sheet; a reduction in area of the dry-snow facies would indicate a more-negative mass 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.

  6. Assessment of climate variability of the Greenland ice sheet: Integration of in situ and satellite data

    NASA Technical Reports Server (NTRS)

    Steffen, K.; Abdalati, W.; Stroeve, J.; Stober, M.; Nolin, A.; Key, J.

    1995-01-01

    The proposed research involves the application of multispectral satellite data in combination with ground truth measurements to monitor surface properties of the Greenland ice sheet which are essential for describing the energy and mass of the ice sheet. Several key components of the energy balance are parameterized using satellite data and in situ measurements. The analysis will be done for a ten year time period in order to get statistics on the seasonal and interannual variations of the surface processes and the climatology. Our goal is to investigate to what accuracy and over what geographic areas large scale snow properties and radiative fluxes can be derived based upon a combination of available remote sensing and meterological data sets. Data analysis showed the following results: (1)cloud classification based on longwave sky radiation revealed that overcast sky occurred for 25% of the time in winter, and for 15% in spring and summer respectively (winter and summer both show the same occurrence of clear sky of approximately 26%); (2) comparison of aerodynamic profile method with eddy correlation method to derive sensible and latent heat flux showed good agreement in the diurnal cycle and the turbulent fluxes were underestimated with the aerodynamic method by 10 - 30% as compared to the in situ eddy flux method; (3) the katabatic wind shows a distinct diurnal cycle with a maximum in the morning (7-9 h solar time) and a minimum in the later afternoon (18 h solar time); (4) snow grain size was modeled with a surface energy balance model (SNTHERM) and compared with in situ measurements. Sharp decreases in the modeled snow grain size, caused by accumulation events such as precipitation and deposition, could be verified with observational data; (4) radiative transfer modeling of firn supports our beliefs that the observed trends in 18 and 19 GHz passive microwave brightness temperatures are attributable to accumulation rate changes (modeling also indicates the

  7. Annual Greenland Accumulation Rates (2009-2012) from Airborne Snow Radar

    NASA Technical Reports Server (NTRS)

    Koenig, Lora S.; Ivanoff, Alvaro; Alexander, Patrick M.; MacGregor, Joseph A.; Fettweis, Xavier; Panzer, Ben; Paden, John D.; Forster, Richard R.; Das, Indrani; McConnell, Joseph R.; hide

    2016-01-01

    Contemporary climate warming over the Arctic is accelerating mass loss from the Greenland Ice Sheet through increasing surface melt, emphasizing the need to closely monitor its surface mass balance in order to improve sea-level rise predictions. Snow accumulation is the largest component of the ice sheet's surface mass balance, but in situ observations thereof are inherently sparse and models are difficult to evaluate at large scales. Here, we quantify recent Greenland accumulation rates using ultra-wideband (2-6.5 gigahertz) airborne snow radar data collected as part of NASA's Operation IceBridge between 2009 and 2012. We use a semi-automated method to trace the observed radiostratigraphy and then derive annual net accumulation rates for 2009-2012. The uncertainty in these radar-derived accumulation rates is on average 14 percent. A comparison of the radarderived accumulation rates and contemporaneous ice cores shows that snow radar captures both the annual and longterm mean accumulation rate accurately. A comparison with outputs from a regional climate model (MAR - Modele Atmospherique Regional for Greenland and vicinity) shows that this model matches radar-derived accumulation rates in the ice sheet interior but produces higher values over southeastern Greenland. Our results demonstrate that snow radar can efficiently and accurately map patterns of snow accumulation across an ice sheet and that it is valuable for evaluating the accuracy of surface mass balance models.

  8. The Darkening of the Greenland Ice Sheet: Trends, Drivers and Projections (1981-2100)

    NASA Technical Reports Server (NTRS)

    Tedesco, Marco; Doherty, Sarah; Fettweis, Xavier; Alexander, Patrick; Jeyaratnam, Jeyavinoth; Stroeve, Julienne

    2016-01-01

    The surface energy balance and meltwater production of the Greenland ice sheet (GrIS) are modulated by snow and ice albedo through the amount of absorbed solar radiation. Here we show, using space-borne multispectral data collected during the 3 decades from 1981 to 2012, that summertime surface albedo over the GrIS decreased at a statistically significant (99 %) rate of 0.02 decade(sup -1) between 1996 and 2012. Over the same period, albedo modelled by the Modele Atmospherique Regionale (MAR) also shows a decrease, though at a lower rate (approximately -0.01 decade(sup -1)) than that obtained from space-borne data. We suggest that the discrepancy between modelled and measured albedo trends can be explained by the absence in the model of processes associated with the presence of light-absorbing impurities. The negative trend in observed albedo is confined to the regions of the GrIS that undergo melting in summer, with the dry snow zone showing no trend. The period 1981-1996 also showed no statistically significant trend over the whole GrIS. Analysis of MAR outputs indicates that the observed albedo decrease is attributable to the combined effects of increased near-surface air temperatures, which enhanced melt and promoted growth in snow grain size and the expansion of bare ice areas, and to trends in light-absorbing impurities (LAI) on the snow and ice surfaces. Neither aerosol models nor in situ and remote sensing observations indicate increasing trends in LAI in the atmosphere over Greenland. Similarly, an analysis of the number of fires and BC emissions from fires points to the absence of trends for such quantities. This suggests that the apparent increase of LAI in snow and ice might be related to the exposure of a "dark band" of dirty ice and to increased consolidation of LAI at the surface with melt, not to increased aerosol deposition. Albedo projections through to the end of the century under different warming scenarios consistently point to continued

  9. Ice sheet radar altimetry

    NASA Technical Reports Server (NTRS)

    Zwally, J.

    1988-01-01

    The surface topography of the Greenland and Antarctic ice 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 ice flow, changes in the position of floating ice-shelf fronts, and ultimately to measure temporal changes in ice surface elevation indicative of ice sheet mass balance.

  10. 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.

  11. Spring snow conditions on Arctic sea ice north of Svalbard, during the Norwegian Young Sea ICE (N-ICE2015) expedition

    NASA Astrophysics Data System (ADS)

    Gallet, Jean-Charles; Merkouriadi, Ioanna; Liston, Glen E.; Polashenski, Chris; Hudson, Stephen; Rösel, Anja; Gerland, Sebastian

    2017-10-01

    Snow is crucial over sea ice due to its conflicting role in reflecting the incoming solar energy and reducing the heat transfer so that its temporal and spatial variability are important to estimate. During the Norwegian Young Sea ICE (N-ICE2015) campaign, snow physical properties and variability were examined, and results from April until mid-June 2015 are presented here. Overall, the snow thickness was about 20 cm higher than the climatology for second-year ice, with an average of 55 ± 27 cm and 32 ± 20 cm on first-year ice. The average density was 350-400 kg m-3 in spring, with higher values in June due to melting. Due to flooding in March, larger variability in snow water equivalent was observed. However, the snow structure was quite homogeneous in spring due to warmer weather and lower amount of storms passing over the field camp. The snow was mostly consisted of wind slab, faceted, and depth hoar type crystals with occasional fresh snow. These observations highlight the more dynamic character of evolution of snow properties over sea ice compared to previous observations, due to more variable sea ice and weather conditions in this area. The snowpack was isothermal as early as 10 June with the first onset of melt clearly identified in early June. Based on our observations, we estimate than snow could be accurately represented by a three to four layers modeling approach, in order to better consider the high variability of snow thickness and density together with the rapid metamorphose of the snow in springtime.

  12. Modelling the climate and surface mass balance of polar ice sheets using RACMO2 - Part 1: Greenland (1958-2016)

    NASA Astrophysics Data System (ADS)

    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.

    2018-03-01

    We evaluate modelled Greenland ice sheet (GrIS) near-surface climate, surface energy balance (SEB) and surface mass 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 ice 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 ice sheet percolation zone. The ice albedo prescribed in the updated model is lower at the ice sheet margins, increasing ice 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.

  13. Greenland ice sheet retreat since the Little Ice Age

    NASA Astrophysics Data System (ADS)

    Beitch, Marci J.

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

  14. Greenland Ice Sheet Monitoring Network (GLISN): Contributions to Science and Society

    NASA Astrophysics Data System (ADS)

    Anderson, K. R.; Bonaime, S.; Clinton, J. F.; Dahl-Jensen, T.; Debski, W. M.; Giardini, D.; Govoni, A.; Kanao, M.; Larsen, T. B.; Lasocki, S.; Lee, W. S.; McCormack, D. A.; Mykkeltveit, S.; Nettles, M.; Stutzmann, E.; Strollo, A.; Sweet, J. R.; Tsuboi, S.; Vallee, M.

    2017-12-01

    The Greenland Ice Sheet Monitoring Network (GLISN) is a broadband, multi-use seismological network, enhanced by selected geodetic observations, designed with the capability to allow researchers to understand the changes currently occurring in the Arctic, and with the operational characteristics necessary to enable response to those changes as understanding improves. GLISN was established through an international collaboration, with 10 nations coordinating their efforts to develop the current 34-station observing network during the last eight years. All of the data collected are freely and openly available in near-real time. The network was designed to transform the community capability for recording, analysis, and interpretation of seismic signals generated by discrete events in Greenland and the Arctic, as well as those traversing the region. Data from the network support a wide range of uses, including estimation of the properties of the solid Earth that control isostatic adjustment rates and set key boundary conditions for ice-sheet evolution; analysis of tectonic earthquakes throughout Greenland and the Arctic; study of the seismic signals associated with large calving events and changing glacier dynamics; and variations in ice and snow properties within the Greenland Ice Sheet. Recordings from the network have also provided invaluable data for rapid evaluation and understanding of the devastating landslide and tsunami that occurred near Nuugaatsiaq, Greenland, in June, 2017. The GLISN strategy of maximizing data quality from a network of approximately evenly distributed stations, delivering data in near-real time, and archiving a continuous data stream easily accessible to researchers, allows continuous discovery of new uses while also facilitating the generation of data products, such as catalogs of tectonic and glacial earthquakes and GPS-based estimates of snow height, that allow for assessment of change over time.

  15. Assimilation of MODIS Ice Surface Temperature and Albedo into the Snow and Ice Model CROCUS Over the Greenland Ice Sheet Along the K-transect Stations

    NASA Astrophysics Data System (ADS)

    Navari, M.; Margulis, S. A.; Bateni, S. M.; Alexander, P. M.; Tedesco, M.

    2016-12-01

    Estimating the Greenland Ice Sheet (GrIS) surface mass balance (SMB) is an important component of current and future projections of sea level rise. In situ measurement provides direct estimates of the SMB, but are inherently limited by their spatial extent and representativeness. Given this limitation, physically based regional climate models (RCMs) are critical for understanding GrIS physical processes and estimating of the GrIS SMB. However, the uncertainty in estimates of SMB from RCMs is still high. Surface remote sensing (RS) has been used as a complimentary tool to characterize various aspects related to the SMB. The difficulty of using these data streams is that the links between them and the SMB terms are most often indirect and implicit. Given the lack of in situ information, imperfect models, and under-utilized RS data it is critical to merge the available data in a systematic way to better characterize the spatial and temporal variation of the GrIS SMB. This work proposes a data assimilation (DA) framework that yields temporally-continuous and physically consistent SMB estimates that benefit from state-of-the-art models and relevant remote sensing data streams. Ice surface temperature (IST) is the most important factor that regulates partitioning of the net radiation into the subsurface snow/ice, sensible and latent heat fluxes and plays a key role in runoff generation. Therefore it can be expected that a better estimate of surface temperature from a data assimilation system would contribute to a better estimate of surface mass fluxes. Albedo plays an important role in the surface energy balance of the GrIS. However, even advanced albedo modules are not adequate to simulate albedo over the GrIS. Therefore, merging remotely sensed albedo product into a physically based model has a potential to improve the estimates of the GrIS SMB. In this work a MODIS-derived IST and a 16-day albedo product are independently assimilated into the snow and ice model CROCUS

  16. A Transient Initialization Routine of the Community Ice Sheet Model for the Greenland Ice Sheet

    NASA Astrophysics Data System (ADS)

    van der Laan, Larissa; van den Broeke, Michiel; Noël, Brice; van de Wal, Roderik

    2017-04-01

    The Community Ice Sheet Model (CISM) is to be applied in future simulations of the Greenland Ice Sheet under a range of climate change scenarios, determining the sensitivity of the ice sheet to individual climatic forcings. In order to achieve reliable results regarding ice sheet stability and assess the probability of future occurrence of tipping points, a realistic initial ice sheet geometry is essential. The current work describes and evaluates the development of a transient initialization routine, using NGRIP 18O isotope data to create a temperature anomaly field. Based on the latter, surface mass balance components runoff and precipitation are perturbed for the past 125k years. The precipitation and runoff fields originate from a downscaled 1 km resolution version of the regional climate model RACMO2.3 for the period 1961-1990. The result of the initialization routine is a present-day ice sheet with a transient memory of the last glacial-interglacial cycle, which will serve as the future runs' initial condition.

  17. Routine Mapping of the Snow Depth Distribution on Sea Ice

    NASA Astrophysics Data System (ADS)

    Farrell, S. L.; Newman, T.; Richter-Menge, J.; Dattler, M.; Paden, J. D.; Yan, S.; Li, J.; Leuschen, C.

    2016-12-01

    The annual growth and retreat of the polar sea ice cover is influenced by the seasonal accumulation, redistribution and melt of snow on sea ice. Due to its high albedo and low thermal conductivity, snow is also a controlling parameter in the mass and energy budgets of the polar climate system. Under a changing climate scenario it is critical to obtain reliable and routine measurements of snow depth, across basin scales, and long time periods, so as to understand regional, seasonal and inter-annual variability, and the subsequent impacts on the sea ice cover itself. Moreover the snow depth distribution remains a significant source of uncertainty in the derivation of sea ice thickness from remote sensing measurements, as well as in numerical model predictions of future climate state. Radar altimeter systems flown onboard NASA's Operation IceBridge (OIB) mission now provide annual measurements of snow across both the Arctic and Southern Ocean ice packs. We describe recent advances in the processing techniques used to interpret airborne radar waveforms and produce accurate and robust snow depth results. As a consequence of instrument effects and data quality issues associated with the initial release of the OIB airborne radar data, the entire data set was reprocessed to remove coherent noise and sidelobes in the radar echograms. These reprocessed data were released to the community in early 2016, and are available for improved derivation of snow depth. Here, using the reprocessed data, we present the results of seven years of radar measurements collected over Arctic sea ice at the end of winter, just prior to melt. Our analysis provides the snow depth distribution on both seasonal and multi-year sea ice. We present the inter-annual variability in snow depth for both the Central Arctic and the Beaufort/Chukchi Seas. We validate our results via comparison with temporally and spatially coincident in situ measurements gathered during many of the OIB surveys. The results

  18. The seasonal cycle of snow cover, sea ice and surface albedo

    NASA Technical Reports Server (NTRS)

    Robock, A.

    1980-01-01

    The paper examines satellite data used to construct mean snow cover caps for the Northern Hemisphere. The zonally averaged snow cover from these maps is used to calculate the seasonal cycle of zonally averaged surface albedo. The effects of meltwater on the surface, solar zenith angle, and cloudiness are parameterized and included in the calculations of snow and ice albedo. The data allows a calculation of surface albedo for any land or ocean 10 deg latitude band as a function of surface temperature ice and snow cover; the correct determination of the ice boundary is more important than the snow boundary for accurately simulating the ice and snow albedo feedback.

  19. Active volcanism beneath the West Antarctic ice sheet and implications for ice-sheet stability

    USGS Publications Warehouse

    Blankenship, D.D.; Bell, R.E.; Hodge, S.M.; Brozena, J.M.; Behrendt, John C.; Finn, C.A.

    1993-01-01

    IT is widely understood that the collapse of the West Antarctic ice sheet (WAIS) would cause a global sea level rise of 6 m, yet there continues to be considerable debate about the detailed response of this ice sheet to climate change1-3. Because its bed is grounded well below sea level, the stability of the WAIS may depend on geologically controlled conditions at the base which are independent of climate. In particular, heat supplied to the base of the ice sheet could increase basal melting and thereby trigger ice streaming, by providing the water for a lubricating basal layer of till on which ice streams are thought to slide4,5. Ice streams act to protect the reservoir of slowly moving inland ice from exposure to oceanic degradation, thus enhancing ice-sheet stability. Here we present aerogeophysical evidence for active volcanism and associated elevated heat flow beneath the WAIS near the critical region where ice streaming begins. If this heat flow is indeed controlling ice-stream formation, then penetration of ocean waters inland of the thin hot crust of the active portion of the West Antarctic rift system could lead to the disappearance of ice streams, and possibly trigger a collapse of the inland ice reservoir.

  20. Reconstructing the last Irish Ice Sheet 2: a geomorphologically-driven model of ice sheet growth, retreat and dynamics

    NASA Astrophysics Data System (ADS)

    Greenwood, Sarah L.; Clark, Chris D.

    2009-12-01

    The ice sheet that once covered Ireland has a long history of investigation. Much prior work focussed on localised evidence-based reconstructions and ice-marginal dynamics and chronologies, with less attention paid to an ice sheet wide view of the first order properties of the ice sheet: centres of mass, ice divide structure, ice 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 ice sheet reconstruction yielding these fundamental ice sheet properties. We present a seven stage model of ice sheet evolution, from initiation to demise, in the form of palaeo-geographic maps. An early incursion of ice from Scotland likely coalesced with local ice caps and spread in a south-westerly direction 200 km across Ireland. A semi-independent Irish Ice Sheet was then established during ice sheet growth, with a branching ice divide structure whose main axis migrated up to 140 km from the west coast towards the east. Ice 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. Ice cover is reconstructed as extending to the continental shelf break. The Irish Ice Sheet became autonomous (i.e. separate from the British Ice Sheet) during deglaciation and fragmented into multiple ice masses, each decaying towards the west. Final sites of demise were likely over the mountains of Donegal, Leitrim and Connemara. Patterns of growth and decay of the ice sheet are shown to be radically different: asynchronous and asymmetric in both spatial and temporal domains. We implicate collapse of the ice stream system in the North Channel - Irish Sea Basin in driving such asymmetry, since rapid

  1. The Physics of Ice Sheets

    ERIC Educational Resources Information Center

    Bassis, J. N.

    2008-01-01

    The great ice sheets in Antarctica and Greenland are vast deposits of frozen freshwater that contain enough to raise sea level by approximately 70 m if they were to completely melt. Because of the potentially catastrophic impact that ice sheets can have, it is important that we understand how ice sheets have responded to past climate changes and…

  2. Large Ice Discharge From the Greenland Ice Sheet

    NASA Technical Reports Server (NTRS)

    Rignot, Eric

    1999-01-01

    The objectives of this work are to measure the ice discharge of the Greenland Ice Sheet close to the grounding line and/or calving front, and compare the results with mass accumulation and ablation in the interior to estimate the ice sheet mass balance.

  3. Ice shelf fracture parameterization in an ice sheet model

    NASA Astrophysics Data System (ADS)

    Sun, Sainan; Cornford, Stephen L.; Moore, John C.; Gladstone, Rupert; Zhao, Liyun

    2017-11-01

    Floating ice shelves exert a stabilizing force onto the inland ice sheet. However, this buttressing effect is diminished by the fracture process, which on large scales effectively softens the ice, accelerating its flow, increasing calving, and potentially leading to ice shelf breakup. We add a continuum damage model (CDM) to the BISICLES ice sheet model, which is intended to model the localized opening of crevasses under stress, the transport of those crevasses through the ice sheet, and the coupling between crevasse depth and the ice flow field and to carry out idealized numerical experiments examining the broad impact on large-scale ice sheet and shelf dynamics. In each case we see a complex pattern of damage evolve over time, with an eventual loss of buttressing approximately equivalent to halving the thickness of the ice shelf. We find that it is possible to achieve a similar ice flow pattern using a simple rule of thumb: introducing an enhancement factor ˜ 10 everywhere in the model domain. However, spatially varying damage (or equivalently, enhancement factor) fields set at the start of prognostic calculations to match velocity observations, as is widely done in ice sheet simulations, ought to evolve in time, or grounding line retreat can be slowed by an order of magnitude.

  4. Origin and sources of dissolved organic matter in snow on the East Antarctic ice sheet.

    PubMed

    Antony, Runa; Grannas, Amanda M; Willoughby, Amanda S; Sleighter, Rachel L; Thamban, Meloth; Hatcher, Patrick G

    2014-06-03

    Polar ice sheets hold a significant pool of the world's carbon reserve and are an integral component of the global carbon cycle. Yet, organic carbon composition and cycling in these systems is least understood. Here, we use ultrahigh resolution mass spectrometry to elucidate, at an unprecedented level, molecular details of dissolved organic matter (DOM) in Antarctic snow. Tens of thousands of distinct molecular species are identified, providing clues to the nature and sources of organic carbon in Antarctica. We show that many of the identified supraglacial organic matter formulas are consistent with material from microbial sources, and terrestrial inputs of vascular plant-derived materials are likely more important sources of organic carbon to Antarctica than previously thought. Black carbon-like material apparently originating from biomass burning in South America is also present, while a smaller fraction originated from soil humics and appears to be photochemically or microbially modified. In addition to remote continental sources, we document signals of oceanic emissions of primary aerosols and secondary organic aerosol precursors. The new insights on the diversity of organic species in Antarctic snowpack reinforce the importance of studying organic carbon associated with the Earth's polar regions in the face of changing climate.

  5. Ice_Sheets_CCI: Essential Climate Variables for the Greenland Ice Sheet

    NASA Astrophysics Data System (ADS)

    Forsberg, R.; Sørensen, L. S.; Khan, A.; Aas, C.; Evansberget, D.; Adalsteinsdottir, G.; Mottram, R.; Andersen, S. B.; Ahlstrøm, A.; Dall, J.; Kusk, A.; Merryman, J.; Hvidberg, C.; Khvorostovsky, K.; Nagler, T.; Rott, H.; Scharrer, M.; Shepard, A.; Ticconi, F.; Engdahl, M.

    2012-04-01

    As part of the ESA Climate Change Initiative (www.esa-cci.org) a long-term project "ice_sheets_cci" started January 1, 2012, in addition to the existing 11 projects already generating Essential Climate Variables (ECV) for the Global Climate Observing System (GCOS). The "ice_sheets_cci" goal is to generate a consistent, long-term and timely set of key climate parameters for the Greenland ice sheet, to maximize the impact of European satellite data on climate research, from missions such as ERS, Envisat and the future Sentinel satellites. The climate parameters to be provided, at first in a research context, and in the longer perspective by a routine production system, would be grids of Greenland ice sheet elevation changes from radar altimetry, ice velocity from repeat-pass SAR data, as well as time series of marine-terminating glacier calving front locations and grounding lines for floating-front glaciers. The ice_sheets_cci project will involve a broad interaction of the relevant cryosphere and climate communities, first through user consultations and specifications, and later in 2012 optional participation in "best" algorithm selection activities, where prototype climate parameter variables for selected regions and time frames will be produced and validated using an objective set of criteria ("Round-Robin intercomparison"). This comparative algorithm selection activity will be completely open, and we invite all interested scientific groups with relevant experience to participate. The results of the "Round Robin" exercise will form the algorithmic basis for the future ECV production system. First prototype results will be generated and validated by early 2014. The poster will show the planned outline of the project and some early prototype results.

  6. 30 CFR 56.11016 - Snow and ice on walkways and travelways.

    Code of Federal Regulations, 2010 CFR

    2010-07-01

    ... 30 Mineral Resources 1 2010-07-01 2010-07-01 false Snow and ice on walkways and travelways. 56... Travelways § 56.11016 Snow and ice on walkways and travelways. Regularly used walkways and travelways shall be sanded, salted, or cleared of snow and ice as soon as practicable. ...

  7. 30 CFR 56.11016 - Snow and ice on walkways and travelways.

    Code of Federal Regulations, 2011 CFR

    2011-07-01

    ... 30 Mineral Resources 1 2011-07-01 2011-07-01 false Snow and ice on walkways and travelways. 56... Travelways § 56.11016 Snow and ice on walkways and travelways. Regularly used walkways and travelways shall be sanded, salted, or cleared of snow and ice as soon as practicable. ...

  8. 30 CFR 56.11016 - Snow and ice on walkways and travelways.

    Code of Federal Regulations, 2012 CFR

    2012-07-01

    ... 30 Mineral Resources 1 2012-07-01 2012-07-01 false Snow and ice on walkways and travelways. 56... Travelways § 56.11016 Snow and ice on walkways and travelways. Regularly used walkways and travelways shall be sanded, salted, or cleared of snow and ice as soon as practicable. ...

  9. 30 CFR 56.11016 - Snow and ice on walkways and travelways.

    Code of Federal Regulations, 2013 CFR

    2013-07-01

    ... 30 Mineral Resources 1 2013-07-01 2013-07-01 false Snow and ice on walkways and travelways. 56... Travelways § 56.11016 Snow and ice on walkways and travelways. Regularly used walkways and travelways shall be sanded, salted, or cleared of snow and ice as soon as practicable. ...

  10. 30 CFR 56.11016 - Snow and ice on walkways and travelways.

    Code of Federal Regulations, 2014 CFR

    2014-07-01

    ... 30 Mineral Resources 1 2014-07-01 2014-07-01 false Snow and ice on walkways and travelways. 56... Travelways § 56.11016 Snow and ice on walkways and travelways. Regularly used walkways and travelways shall be sanded, salted, or cleared of snow and ice as soon as practicable. ...

  11. Exposure age and ice-sheet model constraints on Pliocene East Antarctic ice sheet dynamics.

    PubMed

    Yamane, Masako; Yokoyama, Yusuke; Abe-Ouchi, Ayako; Obrochta, Stephen; Saito, Fuyuki; Moriwaki, Kiichi; Matsuzaki, Hiroyuki

    2015-04-24

    The Late Pliocene epoch is a potential analogue for future climate in a warming world. Here we reconstruct Plio-Pleistocene East Antarctic Ice Sheet (EAIS) variability using cosmogenic nuclide exposure ages and model simulations to better understand ice sheet behaviour under such warm conditions. New and previously published exposure ages indicate interior-thickening during the Pliocene. An ice sheet model with mid-Pliocene boundary conditions also results in interior thickening and suggests that both the Wilkes Subglacial and Aurora Basins largely melted, offsetting increased ice volume. Considering contributions from West Antarctica and Greenland, this is consistent with the most recent IPCC AR5 estimate, which indicates that the Pliocene sea level likely did not exceed +20 m on Milankovitch timescales. The inception of colder climate since ∼3 Myr has increased the sea ice cover and inhibited active moisture transport to Antarctica, resulting in reduced ice sheet thickness, at least in coastal areas.

  12. Evaluation of Surface and Near-Surface Melt Characteristics on the Greenland Ice Sheet using MODIS and QuikSCAT Data

    NASA Technical Reports Server (NTRS)

    Hall, Dorothy K.; Nghiem, Son V.; Schaaf, Crystal B.; DiGirolamo, Nicolo E.

    2009-01-01

    The Greenland Ice Sheet has been the focus of much attention recently because of increasing melt in response to regional climate warming. To improve our ability to measure surface melt, we use remote-sensing data products to study surface and near-surface melt characteristics of the Greenland Ice Sheet for the 2007 melt season when record melt extent and runoff occurred. Moderate Resolution Imaging Spectroradiometer (MODIS) daily land-surface temperature (LST), MODIS daily snow albedo, and a special diurnal melt product derived from QuikSCAT (QS) scatterometer data, are all effective in measuring the evolution of melt on the ice sheet. These daily products, produced from different parts of the electromagnetic spectrum, are sensitive to different geophysical features, though QS- and MODIS-derived melt generally show excellent correspondence when surface melt is present on the ice sheet. Values derived from the daily MODIS snow albedo product drop in response to melt, and change with apparent grain-size changes. For the 2007 melt season, the QS and MODIS LST products detect 862,769 square kilometers and 766,184 square kilometers of melt, respectively. The QS product detects about 11% greater melt extent than is detected by the MODIS LST product probably because QS is more sensitive to surface melt, and can detect subsurface melt. The consistency of the response of the different products demonstrates unequivocally that physically-meaningful melt/freeze boundaries can be detected. We have demonstrated that these products, used together, can improve the precision in mapping surface and near-surface melt extent on the Greenland Ice Sheet.

  13. Snow and Ice Products from the Moderate Resolution Imaging Spectroradiometer

    NASA Technical Reports Server (NTRS)

    Hall, Dorothy K.; Salomonson, Vincent V.; Riggs, George A.; Klein, Andrew G.

    2003-01-01

    Snow and sea ice products, derived from the Moderate Resolution Imaging Spectroradiometer (MODIS) instrument, flown on the Terra and Aqua satellites, are or will be available through the National Snow and Ice Data Center Distributed Active Archive Center (DAAC). The algorithms that produce the products are automated, thus providing a consistent global data set that is suitable for climate studies. The suite of MODIS snow products begins with a 500-m resolution, 2330-km swath snow-cover map that is then projected onto a sinusoidal grid to produce daily and 8-day composite tile products. The sequence proceeds to daily and 8-day composite climate-modeling grid (CMG) products at 0.05 resolution. A daily snow albedo product will be available in early 2003 as a beta test product. The sequence of sea ice products begins with a swath product at 1-km resolution that provides sea ice extent and ice-surface temperature (IST). The sea ice swath products are then mapped onto the Lambert azimuthal equal area or EASE-Grid projection to create a daily and 8-day composite sea ice tile product, also at 1 -km resolution. Climate-Modeling Grid (CMG) sea ice products in the EASE-Grid projection at 4-km resolution are planned for early 2003.

  14. Snow and ice volume on Mount Spurr Volcano, Alaska, 1981

    USGS Publications Warehouse

    March, Rod S.; Mayo, Lawrence R.; Trabant, Dennis C.

    1997-01-01

    Mount Spurr (3,374 meters altitude) is an active volcano 130 kilometers west of Anchorage, Alaska, with an extensive covering of seasonal and perennial snow, and glaciers. Knowledge of the volume and distribution of snow and ice on a volcano aids in assessing hydrologic hazards such as floods, mudflows, and debris flows. In July 1981, ice thickness was measured at 68 locations on the five main glaciers of Mount Spurr: 64 of these measurements were made using a portable 1.7 megahertz monopulse ice-radar system, and 4 measurements were made using the helicopter altimeter where the glacier bed was exposed by ice avalanching. The distribution of snow and ice derived from these measurements is depicted on contour maps and in tables compiled by altitude and by drainage basins. Basal shear stresses at 20 percent of the measured locations ranged from 200 to 350 kilopascals, which is significantly higher than the 50 to 150 kilopascals commonly referred to in the literature as the 'normal' range for glaciers. Basal shear stresses higher than 'normal' have also been found on steep glaciers on volcanoes in the Cascade Range in the western United States. The area of perennial snow and ice coverage on Mount Spurr was 360 square kilometers in 1981, with an average thickness of 190?50 meters. Seasonal snow increases the volume about 1 percent and increases the area about 30 percent with a maximum in May or June. Runoff from Mount Spurr feeds the Chakachatna River and the Chichantna River (a tributary of the Beluga River). The Chakachatna River drainage contains 14 cubic kilometers of snow and ice and the Chichantna River drainage contains 53 cubic kilometers. The snow and ice volume on the mountain was 67?17 cubic kilometers, approximately 350 times more snow and ice than was on Mount St. Helens before its May 18, 1980, eruption, and 15 times more snow and ice than on Mount Rainier, the most glacierized of the measured volcanoes in the Cascade Range. On the basis of these relative

  15. Branch breakage under snow and ice loads.

    PubMed

    Cannell, M G; Morgan, J

    1989-09-01

    Measurements were made on branches and trunks of Picea sitchensis (Bong.) Carr. to determine the relationship between (i) the bending moment at the bases of branches that cause breakage, and (ii) midpoint diameter cubed. The theory for cantilever beams was then used to calculate the basal bending moments and midpoint diameters of branches with different numbers of laterals and endpoint deflections, given previously measured values of Young's modulus, taper and weights of foliage and wood. Snow and ice loads (equal to 2 and 4 g cm(-1) of shoot, respectively) were then included in the calculation to determine whether the basal bending moments exceeded the breakage values. The likelihood of breakage increased with an increase in (i) number of laterals, and (ii) endpoint deflection under self weight (without snow or ice)-features that had previously been shown to lessen the amount of branch wood required to support a unit of foliage. However, branches which deflected moderately (> 10% of their length) under their own weight deflected greatly under snow or ice loads and might shed powdery snow before breakage occurs.

  16. Satellite remote sensing over ice

    NASA Technical Reports Server (NTRS)

    Thomas, R. H.

    1984-01-01

    Satellite remote sensing provides unique opportunities for observing ice-covered terrain. Passive-microwave data give information on snow extent on land, sea-ice extent and type, and zones of summer melting on the polar ice sheets, with the potential for estimating snow-accumulation rates on these ice sheets. All weather, high-resolution imagery of sea ice is obtained using synthetic aperture radars, and ice-movement vectors can be deduced by comparing sequential images of the same region. Radar-altimetry data provide highly detailed information on ice-sheet topography, with the potential for deducing thickening/thinning rates from repeat surveys. The coastline of Antarctica can be mapped accurately using altimetry data, and the size and spatial distribution of icebergs can be monitored. Altimetry data also distinguish open ocean from pack ice and they give an indication of sea-ice characteristics.

  17. Satellite remote sensing over ice

    NASA Technical Reports Server (NTRS)

    Thomas, R. H.

    1986-01-01

    Satellite remote sensing provides unique opportunities for observing ice-covered terrain. Passive-microwave data give information on snow extent on land, sea-ice extent and type, and zones of summer melting on the polar ice sheets, with the potential for estimating snow-accumulation rates on these ice sheets. All weather, high-resolution imagery of sea ice is obtained using synthetic aperture radars, and ice-movement vectors can be deduced by comparing sequential images of the same region. Radar-altimetry data provide highly detailed information on ice-sheet topography, with the potential for deducing thickening/thinning rates from repeat surveys. The coastline of Antarctica can be mapped accurately using altimetry data, and the size and spatial distribution of icebergs can be monitored. Altimetry data also distinguish open ocean from pack ice and they give an indication of sea-ice characteristics.

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

    NASA Technical Reports Server (NTRS)

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

    1986-01-01

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

  19. Snow depth on Arctic sea ice from historical in situ data

    NASA Astrophysics Data System (ADS)

    Shalina, Elena V.; Sandven, Stein

    2018-06-01

    The snow data from the Soviet airborne expeditions Sever in the Arctic collected over several decades in March, April and May have been analyzed in this study. The Sever data included more measurements and covered a much wider area, particularly in the Eurasian marginal seas (Kara Sea, Laptev Sea, East Siberian Sea and Chukchi Sea), compared to the Soviet North Pole drifting stations. The latter collected data mainly in the central part of the Arctic Basin. The following snow parameters have been analyzed: average snow depth on the level ice (undisturbed snow) height and area of sastrugi, depth of snow dunes attached to ice ridges and depth of snow on hummocks. In the 1970s-1980s, in the central Arctic, the average depth of undisturbed snow was 21.2 cm, the depth of sastrugi (that occupied about 30 % of the ice surface) was 36.2 cm and the average depth of snow near hummocks and ridges was about 65 cm. For the marginal seas, the average depth of undisturbed snow on the level ice varied from 9.8 cm in the Laptev Sea to 15.3 cm in the East Siberian Sea, which had a larger fraction of multiyear ice. In the marginal seas the spatial variability of snow depth was characterized by standard deviation varying between 66 and 100 %. The average height of sastrugi varied from 23 cm to about 32 cm with standard deviation between 50 and 56 %. The average area covered by sastrugi in the marginal seas was estimated to be 36.5 % of the total ice area where sastrugi were observed. The main result of the study is a new snow depth climatology for the late winter using data from both the Sever expeditions and the North Pole drifting stations. The snow load on the ice observed by Sever expeditions has been described as a combination of the depth of undisturbed snow on the level ice and snow depth of sastrugi weighted in proportion to the sastrugi area. The height of snow accumulated near the ice ridges was not included in the calculations because there are no estimates of the area

  20. 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

  1. Thin Sea Ice, Thick Snow, and Widespread Negative Freeboard Observed During N-ICE2015 North of Svalbard

    NASA Astrophysics Data System (ADS)

    Rösel, Anja; Itkin, Polona; King, Jennifer; Divine, Dmitry; Wang, Caixin; Granskog, Mats A.; Krumpen, Thomas; Gerland, Sebastian

    2018-02-01

    In recent years, sea-ice conditions in the Arctic Ocean changed substantially toward a younger and thinner sea-ice cover. To capture the scope of these changes and identify the differences between individual regions, in situ observations from expeditions are a valuable data source. We present a continuous time series of in situ measurements from the N-ICE2015 expedition from January to June 2015 in the Arctic Basin north of Svalbard, comprising snow buoy and ice mass balance buoy data and local and regional data gained from electromagnetic induction (EM) surveys and snow probe measurements from four distinct drifts. The observed mean snow depth of 0.53 m for April to early June is 73% above the average value of 0.30 m from historical and recent observations in this region, covering the years 1955-2017. The modal total ice and snow thicknesses, of 1.6 and 1.7 m measured with ground-based EM and airborne EM measurements in April, May, and June 2015, respectively, lie below the values ranging from 1.8 to 2.7 m, reported in historical observations from the same region and time of year. The thick snow cover slows thermodynamic growth of the underlying sea ice. In combination with a thin sea-ice cover this leads to an imbalance between snow and ice thickness, which causes widespread negative freeboard with subsequent flooding and a potential for snow-ice formation. With certainty, 29% of randomly located drill holes on level ice had negative freeboard.

  2. Greenland ice-sheet contribution to sea-level rise buffered by meltwater storage in firn.

    PubMed

    Harper, J; Humphrey, N; Pfeffer, W T; Brown, J; Fettweis, X

    2012-11-08

    Surface melt on the Greenland ice sheet has shown increasing trends in areal extent and duration since the beginning of the satellite era. Records for melt were broken in 2005, 2007, 2010 and 2012. Much of the increased surface melt is occurring in the percolation zone, a region of the accumulation area that is perennially covered by snow and firn (partly compacted snow). The fate of melt water in the percolation zone is poorly constrained: some may travel away from its point of origin and eventually influence the ice sheet's flow dynamics and mass balance and the global sea level, whereas some may simply infiltrate into cold snow or firn and refreeze with none of these effects. Here we quantify the existing water storage capacity of the percolation zone of the Greenland ice sheet and show the potential for hundreds of gigatonnes of meltwater storage. We collected in situ observations of firn structure and meltwater retention along a roughly 85-kilometre-long transect of the melting accumulation area. Our data show that repeated infiltration events in which melt water penetrates deeply (more than 10 metres) eventually fill all pore space with water. As future surface melt intensifies under Arctic warming, a fraction of melt water that would otherwise contribute to sea-level rise will fill existing pore space of the percolation zone. We estimate the lower and upper bounds of this storage sink to be 322 ± 44 gigatonnes and  1,289(+388)(-252) gigatonnes, respectively. Furthermore, we find that decades are required to fill this pore space under a range of plausible future climate conditions. Hence, routing of surface melt water into filling the pore space of the firn column will delay expansion of the area contributing to sea-level rise, although once the pore space is filled it cannot quickly be regenerated.

  3. Ice Sheet Temperature Records - Satellite and In Situ Data from Antarctica and Greenland

    NASA Astrophysics Data System (ADS)

    Shuman, C. A.; Comiso, J. C.

    2001-12-01

    Recently completed decadal-length surface temperature records from Antarctica and Greenland are providing insights into the challenge of detecting climate change. Ice and snow cover at high latitudes influence the global climate system by reflecting much of the incoming solar energy back to space. An expected consequence of global warming is a decrease in area covered by snow and ice and an increase in Earth's absorption of solar radiation. Models have predicted that the effects of climate warming may be amplified at high latitudes; thinning of the Greenland ice sheet margins and the breakup of Antarctic Peninsula ice shelves suggest this process may have begun. Satellite data provide an excellent means of observing climate parameters across both long temporal and remote spatial domains but calibration and validation of their data remains a challenge. Infrared sensors can provide excellent temperature information but cloud cover and calibration remain as problems. Passive-microwave sensors can obtain data during the long polar night and through clouds but have calibration issues and a much lower spatial resolution. Automatic weather stations are generally spatially- and temporally-restricted and may have long gaps due to equipment failure. Stable isotopes of oxygen and hydrogen from ice sheet locations provide another means of determining temperature variations with time but are challenging to calibrate to observed temperatures and also represent restricted areas. This presentation will discuss these issues and elaborate on the development and limitations of composite satellite, automatic weather station, and proxy temperature data from selected sites in Antarctica and Greenland.

  4. Global ice sheet/RSL simulations using the higher-order Ice Sheet System Model.

    NASA Astrophysics Data System (ADS)

    Larour, E. Y.; Ivins, E. R.; Adhikari, S.; Schlegel, N.; Seroussi, H. L.; Morlighem, M.

    2017-12-01

    Relative sea-level rise is driven by processes that are intimately linked to the evolution ofglacial areas and ice sheets in particular. So far, most Earth System models capable of projecting theevolution of RSL on decadal to centennial time scales have relied on offline interactions between RSL andice sheets. In particular, grounding line and calving front dynamics have not been modeled in a way that istightly coupled with Elasto-Static Adjustment (ESA) and/or Glacial-Isostatic Adjustment (GIA). Here, we presenta new simulation of the entire Earth System in which both Greenland and Antarctica ice sheets are tightly coupledto an RSL model that includes both ESA and GIA at resolutions and time scales compatible with processes suchas grounding line dynamics for Antarctica ice shelves and calving front dynamics for Greenland marine-terminatingglaciers. The simulations rely on the Ice Sheet System Model (ISSM) and show the impact of higher-orderice flow dynamics and coupling feedbacks between ice flow and RSL. We quantify the exact impact of ESA andGIA inclusion on grounding line evolution for large ice shelves such as the Ronne and Ross ice shelves, as well asthe Agasea Embayment ice streams, and demonstate how offline vs online RSL simulations diverge in the long run,and the consequences for predictions of sea-level rise.This work was performed at the California Institute of Technology's Jet Propulsion Laboratory undera contract with the National Aeronautics and Space Administration's Cryosphere Science Program.

  5. Nitrate deposition and preservation in the snowpack along a traverse from coast to the ice sheet summit (Dome A) in East Antarctica

    NASA Astrophysics Data System (ADS)

    Shi, Guitao; Hastings, Meredith G.; Yu, Jinhai; Ma, Tianming; Hu, Zhengyi; An, Chunlei; Li, Chuanjin; Ma, Hongmei; Jiang, Su; Li, Yuansheng

    2018-04-01

    Antarctic ice core nitrate (NO3-) can provide a unique record of the atmospheric reactive nitrogen cycle. However, the factors influencing the deposition and preservation of NO3- at the ice sheet surface must first be understood. Therefore, an intensive program of snow and atmospheric sampling was made on a traverse from the coast to the ice sheet summit, Dome A, East Antarctica. Snow samples in this observation include 120 surface snow samples (top ˜ 3 cm), 20 snow pits with depths of 150 to 300 cm, and 6 crystal ice samples (the topmost needle-like layer on Dome A plateau). The main purpose of this investigation is to characterize the distribution pattern and preservation of NO3- concentrations in the snow in different environments. Results show that an increasing trend of NO3- concentrations with distance inland is present in surface snow, and NO3- is extremely enriched in the topmost crystal ice (with a maximum of 16.1 µeq L-1). NO3- concentration profiles for snow pits vary between coastal and inland sites. On the coast, the deposited NO3- was largely preserved, and the archived NO3- fluxes are dominated by snow accumulation. The relationship between the archived NO3- and snow accumulation rate can be depicted well by a linear model, suggesting a homogeneity of atmospheric NO3- levels. It is estimated that dry deposition contributes 27-44 % of the archived NO3- fluxes, and the dry deposition velocity and scavenging ratio for NO3- were relatively constant near the coast. Compared to the coast, the inland snow shows a relatively weak correlation between archived NO3- and snow accumulation, and the archived NO3- fluxes were more dependent on concentration. The relationship between NO3- and coexisting ions (nssSO42-, Na+ and Cl-) was also investigated, and the results show a correlation between nssSO42- (fine aerosol particles) and NO3- in surface snow, while the correlation between NO3- and Na+ (mainly associated with coarse aerosol particles) is not

  6. 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.

  7. CO2 flux over young and snow-covered Arctic pack ice in winter and spring

    NASA Astrophysics Data System (ADS)

    Nomura, Daiki; Granskog, Mats A.; Fransson, Agneta; Chierici, Melissa; Silyakova, Anna; Ohshima, Kay I.; Cohen, Lana; Delille, Bruno; Hudson, Stephen R.; Dieckmann, Gerhard S.

    2018-06-01

    Rare CO2 flux measurements from Arctic pack ice show that two types of ice contribute to the release of CO2 from the ice to the atmosphere during winter and spring: young, thin ice with a thin layer of snow and older (several weeks), thicker ice with thick snow cover. Young, thin sea ice is characterized by high salinity and high porosity, and snow-covered thick ice remains relatively warm ( > -7.5 °C) due to the insulating snow cover despite air temperatures as low as -40 °C. Therefore, brine volume fractions of these two ice types are high enough to provide favorable conditions for gas exchange between sea ice and the atmosphere even in mid-winter. Although the potential CO2 flux from sea ice decreased due to the presence of the snow, the snow surface is still a CO2 source to the atmosphere for low snow density and thin snow conditions. We found that young sea ice that is formed in leads without snow cover produces CO2 fluxes an order of magnitude higher than those in snow-covered older ice (+1.0 ± 0.6 mmol C m-2 day-1 for young ice and +0.2 ± 0.2 mmol C m-2 day-1 for older ice).

  8. Small scale variability of snow properties on Antarctic sea ice

    NASA Astrophysics Data System (ADS)

    Wever, Nander; Leonard, Katherine; Paul, Stephan; Jacobi, Hans-Werner; Proksch, Martin; Lehning, Michael

    2016-04-01

    Snow on sea ice plays an important role in air-ice-sea interactions, as snow accumulation may for example increase the albedo. Snow is also able to smooth the ice surface, thereby reducing the surface roughness, while at the same time it may generate new roughness elements by interactions with the wind. Snow density is a key property in many processes, for example by influencing the thermal conductivity of the snow layer, radiative transfer inside the snow as well as the effects of aerodynamic forcing on the snowpack. By comparing snow density and grain size from snow pits and snow micro penetrometer (SMP) measurements, highly resolved density and grain size profiles were acquired during two subsequent cruises of the RV Polarstern in the Weddell Sea, Antarctica, between June and October 2013. During the first cruise, SMP measurements were done along two approximately 40 m transects with a horizontal resolution of approximately 30 cm. During the second cruise, one transect was made with approximately 7.5 m resolution over a distance of 500 m. Average snow densities are about 300 kg/m3, but the analysis also reveals a high spatial variability in snow density on sea ice in both horizontal and vertical direction, ranging from roughly 180 to 360 kg/m3. This variability is expressed by coherent snow structures over several meters. On the first cruise, the measurements were accompanied by terrestrial laser scanning (TLS) on an area of 50x50 m2. The comparison with the TLS data indicates that the spatial variability is exhibiting similar spatial patterns as deviations in surface topology. This suggests a strong influence from surface processes, for example wind, on the temporal development of density or grain size profiles. The fundamental relationship between variations in snow properties, surface roughness and changes therein as investigated in this study is interpreted with respect to large-scale ice movement and the mass balance.

  9. Interpretation of Passive Microwave Imagery of Surface Snow and Ice: Harding Lake, Alaska

    DTIC Science & Technology

    1991-06-01

    Circle conditions in microwave imagery depends on the char- (Fig. 1). The lake is roughly circular in shape and has a acteristics of the sensor system...local oscillator frequency 33.6 0Hz IF bandwidth Greaterthan 500 MHz cracks in the ice sheet. The incursion process is de - video bandwidth 1.7 kHz...using pas- surface snow had oct.urred on these similarly sized sive microwave sensors . IEEE/Transactions on Geo- lakes. Additional field verifications

  10. 30 CFR 57.11016 - Snow and ice on walkways and travelways.

    Code of Federal Regulations, 2014 CFR

    2014-07-01

    ... 30 Mineral Resources 1 2014-07-01 2014-07-01 false Snow and ice on walkways and travelways. 57... MINES Travelways and Escapeways Travelways-Surface and Underground § 57.11016 Snow and ice on walkways... ice as soon as practicable. ...

  11. 30 CFR 57.11016 - Snow and ice on walkways and travelways.

    Code of Federal Regulations, 2010 CFR

    2010-07-01

    ... 30 Mineral Resources 1 2010-07-01 2010-07-01 false Snow and ice on walkways and travelways. 57... MINES Travelways and Escapeways Travelways-Surface and Underground § 57.11016 Snow and ice on walkways... ice as soon as practicable. ...

  12. 30 CFR 57.11016 - Snow and ice on walkways and travelways.

    Code of Federal Regulations, 2012 CFR

    2012-07-01

    ... 30 Mineral Resources 1 2012-07-01 2012-07-01 false Snow and ice on walkways and travelways. 57... MINES Travelways and Escapeways Travelways-Surface and Underground § 57.11016 Snow and ice on walkways... ice as soon as practicable. ...

  13. 30 CFR 57.11016 - Snow and ice on walkways and travelways.

    Code of Federal Regulations, 2013 CFR

    2013-07-01

    ... 30 Mineral Resources 1 2013-07-01 2013-07-01 false Snow and ice on walkways and travelways. 57... MINES Travelways and Escapeways Travelways-Surface and Underground § 57.11016 Snow and ice on walkways... ice as soon as practicable. ...

  14. 30 CFR 57.11016 - Snow and ice on walkways and travelways.

    Code of Federal Regulations, 2011 CFR

    2011-07-01

    ... 30 Mineral Resources 1 2011-07-01 2011-07-01 false Snow and ice on walkways and travelways. 57... MINES Travelways and Escapeways Travelways-Surface and Underground § 57.11016 Snow and ice on walkways... ice as soon as practicable. ...

  15. Sea Ice Thickness, Freeboard, and Snow Depth products from Operation IceBridge Airborne Data

    NASA Technical Reports Server (NTRS)

    Kurtz, N. T.; Farrell, S. L.; Studinger, M.; Galin, N.; Harbeck, J. P.; Lindsay, R.; Onana, V. D.; Panzer, B.; Sonntag, J. G.

    2013-01-01

    The study of sea ice using airborne remote sensing platforms provides unique capabilities to measure a wide variety of sea ice properties. These measurements are useful for a variety of topics including model evaluation and improvement, assessment of satellite retrievals, and incorporation into climate data records for analysis of interannual variability and long-term trends in sea ice properties. In this paper we describe methods for the retrieval of sea ice thickness, freeboard, and snow depth using data from a multisensor suite of instruments on NASA's Operation IceBridge airborne campaign. We assess the consistency of the results through comparison with independent data sets that demonstrate that the IceBridge products are capable of providing a reliable record of snow depth and sea ice thickness. We explore the impact of inter-campaign instrument changes and associated algorithm adaptations as well as the applicability of the adapted algorithms to the ongoing IceBridge mission. The uncertainties associated with the retrieval methods are determined and placed in the context of their impact on the retrieved sea ice thickness. Lastly, we present results for the 2009 and 2010 IceBridge campaigns, which are currently available in product form via the National Snow and Ice Data Center

  16. Snow Micro-Structure Model

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

    Micah Johnson, Andrew Slaughter

    PIKA is a MOOSE-based application for modeling micro-structure evolution of seasonal snow. The model will be useful for environmental, atmospheric, and climate scientists. Possible applications include application to energy balance models, ice sheet modeling, and avalanche forecasting. The model implements physics from published, peer-reviewed articles. The main purpose is to foster university and laboratory collaboration to build a larger multi-scale snow model using MOOSE. The main feature of the code is that it is implemented using the MOOSE framework, thus making features such as multiphysics coupling, adaptive mesh refinement, and parallel scalability native to the application. PIKA implements three equations:more » the phase-field equation for tracking the evolution of the ice-air interface within seasonal snow at the grain-scale; the heat equation for computing the temperature of both the ice and air within the snow; and the mass transport equation for monitoring the diffusion of water vapor in the pore space of the snow.« less

  17. Multi-modal albedo distributions in the ablation area of the southwestern Greenland Ice Sheet

    NASA Astrophysics Data System (ADS)

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

    2015-05-01

    Surface albedo is a key variable controlling solar radiation absorbed at the Greenland Ice Sheet (GrIS) surface and, thus, meltwater production. Recent decline in surface albedo over the GrIS has been linked to enhanced snow grain metamorphic rates, earlier snowmelt, and amplified melt-albedo feedback from atmospheric warming. However, the importance of distinct surface types on ablation area albedo and meltwater production is still relatively unknown. In this study, we analyze albedo and ablation rates using in situ and remotely sensed data. Observations include (1) a new high-quality in situ spectral albedo data set collected with an Analytical Spectral Devices Inc. spectroradiometer measuring at 325-1075 nm along a 1.25 km transect during 3 days in June 2013; (2) broadband albedo at two automatic weather stations; and (3) daily MODerate Resolution Imaging Spectroradiometer (MODIS) albedo (MOD10A1) between 31 May and 30 August 2012 and 2013. We find that seasonal ablation area albedos in 2013 have a bimodal distribution, with snow and ice facies characterizing the two peaks. Our results show that a shift from a distribution dominated by high to low albedos corresponds to an observed melt rate increase of 51.5% (between 10-14 July and 20-24 July 2013). In contrast, melt rate variability caused by albedo changes before and after this shift was much lower and varied between ~10 and 30% in the melting season. Ablation area albedos in 2012 exhibited a more complex multimodal distribution, reflecting a transition from light to dark-dominated surface, as well as sensitivity to the so called "dark-band" region in southwest Greenland. In addition to a darkening surface from ice crystal growth, our findings demonstrate that seasonal changes in GrIS ablation area albedos are controlled by changes in the fractional coverage of snow, bare ice, and impurity-rich surface types. Thus, seasonal variability in ablation area albedos appears to be regulated primarily as a function

  18. On the extraordinary snow on the sea ice off East Antarctica in late winter, 2012

    NASA Astrophysics Data System (ADS)

    Toyota, Takenobu; Massom, Robert; Lecomte, Olivier; Nomura, Daiki; Heil, Petra; Tamura, Takeshi; Fraser, Alexander D.

    2016-09-01

    In late winter-early spring 2012, the second Sea Ice Physics and Ecosystems Experiment (SIPEX II) was conducted off Wilkes Land, East Antarctica, onboard R/V Aurora Australis. The sea-ice conditions were characterized by significantly thick first-year ice and snow, trapping the ship for about 10 days in the near coastal region. The deep snow cover was particularly remarkable, in that its average value of 0.45 m was almost three times that observed between 1992 and 2007 in the region. To reveal factors responsible, we used in situ observations and ERA-Interim reanalysis (1990-2012) to examine the relative contribution of the different components of the local-regional snow mass balance equation i.e., snow accumulation on sea ice, precipitation minus evaporation (P-E), and loss by (i) snow-ice formation and (ii) entering into leads due to drifting snow. Results show no evidence for significantly high P-E in the winter of 2012. Ice core analysis has shown that although the snow-ice layer was relatively thin, indicating less transformation from snow to snow-ice in 2012 as compared to measurements from 2007, the difference was not enough to explain the extraordinarily deep snow. Based on these results, we deduce that lower loss of snow into leads was probably responsible for the extraordinary snow in 2012. Statistical analysis and satellite images suggest that the reduction in loss of snow into leads is attributed to rough ice surface associated with active deformation processes and larger floe size due to sea-ice expansion. This highlights the importance of snow-sea ice interaction in determining the mean snow depth on Antarctic sea ice.

  19. Measurements of thermal infrared spectral reflectance of frost, snow, and ice

    NASA Technical Reports Server (NTRS)

    Salisbury, John W.; D'Aria, Dana M.; Wald, Andrew

    1994-01-01

    Because much of Earth's surface is covered by frost, snow, and ice, the spectral emissivities of these materials are a significant input to radiation balance calculations in global atmospheric circulation and climate change models. Until now, however, spectral emissivities of frost and snow have been calculated from the optical constants of ice. We have measured directional hemispherical reflectance spectra of frost, snow, and ice from which emissivities can be predicted using Kirchhoff's law (e = 1-R). These measured spectra show that contrary to conclusions about the emissivity of snow drawn from previously calculated spectra, snow emissivity departs significantly from blackbody behavior in the 8-14 micrometer region of the spectrum; snow emissivity decreases with both increasing particle size and increasing density due to packing or grain welding; while snow emissivity increases due to the presence of meltwater.

  20. Rewriting Ice Sheet "Glacier-ology"

    NASA Astrophysics Data System (ADS)

    Bindschadler, R.

    2006-12-01

    The revolution in glaciology driven by the suite of increasingly sophisticated satellite instruments has been no more extreme than in the area of ice dynamics. Years ago, glaciologists were (probably unwittingly) selective in what properties of mountain glaciers were also applied to ice sheets. This reinforced the view that they responded slowly to their environment. Notions of rapid response driven by the ideas of John Mercer, Bill Budd and Terry Hughes were politely rejected by the centrists of mainstream glaciological thought. How the tables have turned--and by the ice sheets themselves, captured in the act of rapidly changing by modern remote sensors! The saw-toothed record of sea-level change over past glacial-interglacial cycles required the existence of rapid ice loss processes. Satellite based observations, supported by hard-earned field observations have extended the time scale over which ice sheets can suddenly change to ever shorter intervals: from centuries, to decades, to years to even minutes. As changes continue to be observed, the scientific community is forced to consider new or previously ignored processes to explain these observations. The penultimate goal of ice-sheet dynamics is to credibly predict the future of both the Greenland and Antarctic ice sheets. In this important endeavor, there is no substitute for our ability to observe. Without the extensive data sets provided by remote sensing, numerical models can be neither tested nor improved. The impact of remote sensing on our existing ability to predict the future must be compared to our probable state of knowledge and ability were these data never collected. Among many satellite observed phenomena we would be largely or wholly ignorant of are the recent acceleration of ice throughout much of coastal Greenland; the sudden disintegration of multiple ice shelves along the Antarctic Peninsula; and the dramatic thinning and acceleration of the Amundsen Sea sector of West Antarctica. These

  1. Ice-sheet response to oceanic forcing.

    PubMed

    Joughin, Ian; Alley, Richard B; Holland, David M

    2012-11-30

    The ice sheets of Greenland and Antarctica are losing ice at accelerating rates, much of which is a response to oceanic forcing, especially of the floating ice shelves. Recent observations establish a clear correspondence between the increased delivery of oceanic heat to the ice-sheet margin and increased ice loss. In Antarctica, most of these processes are reasonably well understood but have not been rigorously quantified. In Greenland, an understanding of the processes by which warmer ocean temperatures drive the observed retreat remains elusive. Experiments designed to identify the relevant processes are confounded by the logistical difficulties of instrumenting ice-choked fjords with actively calving glaciers. For both ice sheets, multiple challenges remain before the fully coupled ice-ocean-atmosphere models needed for rigorous sea-level projection are available.

  2. Balance of the West Antarctic Ice Sheet

    NASA Technical Reports Server (NTRS)

    2002-01-01

    For several decades, measurements of the West Antarctic Ice Sheet showed it to be retreating rapidly. But new data derived from satellite-borne radar sensors show the ice sheet to be growing. Changing Antarctic ice sheets remains an area of high scientific interest, particularly in light of recent global warming concerns. These new findings are significant because scientists estimate that sea level would rise 5-6 meters (16-20 feet) if the ice sheet collapsed into the sea. Do these new measurements signal the end of the ice sheet's 10,000-year retreat? Or, are these new satellite data simply much more accurate than the sparse ice core and surface measurements that produced the previous estimates? Another possibility is that the ice accumulation may simply indicate that the ice sheet naturally expands and retreats in regular cycles. Cryologists will grapple with these questions, and many others, as they examine the new data. The image above depicts the region of West Antarctica where scientists measured ice speed. The fast-moving central ice streams are shown in red. Slower tributaries feeding the ice streams are shown in blue. Green areas depict slow-moving, stable areas. Thick black lines depict the areas that collect snowfall to feed their respective ice streams. Reference: Ian Joughin and Slawek Tulaczyk Science Jan 18 2002: 476-480. Image courtesy RADARSAT Antarctic Mapping Project

  3. Validation of Modelled Ice Dynamics of the Greenland Ice Sheet using Historical Forcing

    NASA Astrophysics Data System (ADS)

    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.

    2015-12-01

    Although ice 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 ice sheets. Here we describe a validation framework for the Greenland Ice Sheet applied to the Community Ice Sheet Model by forcing the model annually with flux anomalies at the major outlet glaciers (Enderlin et al., 2014, observed from Landsat/ASTER/Operation IceBridge) and surface mass balance (van Angelen et al., 2013, calculated from RACMO2) for the period 1991-2012. The ice sheet model output is compared to ice surface elevation observations from ICESat and ice sheet mass change observations from GRACE. Early results show promise for assessing the performance of different model configurations. Additionally, we explore the effect of ice sheet model resolution on validation skill.

  4. Microwave signatures of snow and fresh water ice

    NASA Technical Reports Server (NTRS)

    Schmugge, T.; Wilheit, T. T.; Gloersen, P.; Meier, M. F.; Frank, D.; Dirmhirn, I.

    1973-01-01

    During March of 1971, the NASA Convair 990 Airborne Observatory carrying microwave radiometers in the wavelength range 0.8 to 21 cm was flown over dry snow with different substrata: Lake ice at Bear Lake in Utah; wet soil in the Yampa River Valley near Steamboat Springs, Colorado; and glacier ice, firm and wet snow on the South Cascade Glacier in Washington. The data presented indicate that the transparency of the snow cover is a function of wavelength. False-color images of microwave brightness temperatures obtained from a scanning radiometer operating at a wavelength of 1.55 cm demonstrate the capability of scanning radiometers for mapping snowfields.

  5. Variability of AVHRR-Derived Clear-Sky Surface Temperature over the Greenland Ice Sheet.

    NASA Astrophysics Data System (ADS)

    Stroeve, Julienne; Steffen, Konrad

    1998-01-01

    The Advanced Very High Resolution Radiometer is used to derive surface temperatures for one satellite pass under clear skies over the Greenland ice sheet from 1989 through 1993. The results of these temperatures are presented as monthly means, and their spatial and temporal variability are discussed. Accuracy of the dry snow surface temperatures is estimated to be better than 1 K during summer. This error is expected to increase during polar night due to problems in cloud identification. Results indicate the surface temperature of the Greenland ice sheet is strongly dominated by topography, with minimum surface temperatures associated with the high elevation regions. In the summer, maximum surface temperatures occur during July along the western coast and southern tip of the ice sheet. Minimum temperatures are found at the summit during summer and move farther north during polar night. Large interannual variability in surface temperatures occurs during winter associated with katabatic storm events. Summer temperatures show little variation, although 1992 stands out as being colder than the other years. The reason for the lower temperatures during 1992 is believed to be a result of the 1991 eruption of Mount Pinatubo.

  6. Quantifying bioalbedo: a new physically based model and discussion of empirical methods for characterising biological influence on ice and snow albedo

    NASA Astrophysics Data System (ADS)

    Cook, Joseph M.; Hodson, Andrew J.; Gardner, Alex S.; Flanner, Mark; Tedstone, Andrew J.; Williamson, Christopher; Irvine-Fynn, Tristram D. L.; Nilsson, Johan; Bryant, Robert; Tranter, Martyn

    2017-11-01

    The darkening effects of biological impurities on ice and snow have been recognised as a control on the surface energy balance of terrestrial snow, sea ice, glaciers and ice sheets. With a heightened interest in understanding the impacts of a changing climate on snow and ice processes, quantifying the impact of biological impurities on ice and snow albedo (bioalbedo) and its evolution through time is a rapidly growing field of research. However, rigorous quantification of bioalbedo has remained elusive because of difficulties in isolating the biological contribution to ice albedo from that of inorganic impurities and the variable optical properties of the ice itself. For this reason, isolation of the biological signature in reflectance data obtained from aerial/orbital platforms has not been achieved, even when ground-based biological measurements have been available. This paper provides the cell-specific optical properties that are required to model the spectral signatures and broadband darkening of ice. Applying radiative transfer theory, these properties provide the physical basis needed to link biological and glaciological ground measurements with remotely sensed reflectance data. Using these new capabilities we confirm that biological impurities can influence ice albedo, then we identify 10 challenges to the measurement of bioalbedo in the field with the aim of improving future experimental designs to better quantify bioalbedo feedbacks. These challenges are (1) ambiguity in terminology, (2) characterising snow or ice optical properties, (3) characterising solar irradiance, (4) determining optical properties of cells, (5) measuring biomass, (6) characterising vertical distribution of cells, (7) characterising abiotic impurities, (8) surface anisotropy, (9) measuring indirect albedo feedbacks, and (10) measurement and instrument configurations. This paper aims to provide a broad audience of glaciologists and biologists with an overview of radiative

  7. Effect of en-glacial water on ice sheet temperatures in a warming climate - a model approach

    NASA Astrophysics Data System (ADS)

    Phillips, T. P.; Rajaram, H.; Steffen, K.

    2009-12-01

    Each summer, significant amount of melt is generated in the ablation zones of large glaciers and ice sheets. This melt does not run off on the surface of the glacier or ice sheet. In fact a significant fraction enters the glacier and flows through en-glacial and sub-glacial hydrologic systems. Correspondingly, the en-glacial and sub-glacial hydrologic systems are brought to a temperature close to the pressure melting point of ice. The thermal influence of these hydrologic processes is seldom incorporated in heat transfer models for glaciers and ice sheets. In a warming climate, as melt water generation is amplified, en-glacial and sub-glacial hydrologic processes can influence the thermal dynamics of an ice sheet significantly, a feedback which is missed in current models. Although the role of refreezing melt water in the firn of the accumulation zone is often accounted for to explain warmer near-surface temperatures, the role of melt water flow within a glacier is not considered in large ice sheet models. We propose a simple parameterization of the influence of en-glacial and sub-glacial hydrology on the thermal dynamics of ice sheets, in the form of a dual-column model. Our model basically modifies the classical Budd column model for temperature variations in ice sheets by introducing an interaction with an en-glacial column, where the temperature is brought to the melting point during the melt season, and winter-time refreezing is influenced by latent heat effects associated with water retained within the en-glacial and sub-glacial systems. A cryo-hydraulic heat exchange coefficient ς is defined, as a parameter that quantifies this interaction. The parameter ς is related to k/R^2, where R is the characteristic spacing between en-glacial passages. The general behavior of the dual-column model is influenced by the competition between cooling by horizontal advection and warming by cryo-hydraulic exchange. We present a dimensionless parameter to quantify this

  8. Towards development of an operational snow on sea ice product

    NASA Astrophysics Data System (ADS)

    Stroeve, J.; Liston, G. E.; Barrett, A. P.; Tschudi, M. A.; Stewart, S.

    2017-12-01

    Sea ice has been visibly changing over the past couple of decades; most notably the annual minimum extent which has shown a distinct downward, and recently accelerating, trend. September mean sea ice extent was over 7×106 km2 in the 1980's, but has averaged less than 5×106 km2 in the last decade. Should this loss continue, there will be wide-ranging impacts on marine ecosystems, coastal communities, prospects for resource extraction and marine activity, and weather conditions in the Arctic and beyond. While changes in the spatial extent of sea ice have been routinely monitored since the 1970s, less is known about how the thickness of the ice cover has changed. While estimates of ice thickness across the Arctic Ocean have become available over the past 20 years based on data from ERS-1/2, Envisat, ICESat, CryoSat-2 satellites and Operation IceBridge aircraft campaigns, the variety of these different measurement approaches, sensor technologies and spatial coverage present formidable challenges. Key among these is that measurement techniques do not measure ice thickness directly - retrievals also require snow depth and density. Towards that end, a sophisticated snow accumulation model is tested in a Lagrangian framework to map daily snow depths across the Arctic sea ice cover using atmospheric reanalysis data as input. Accuracy of the snow accumulation is assessed through comparison with Operation IceBridge data and ice mass balance buoys (IMBs). Impacts on ice thickness retrievals are further discussed.

  9. Seasonal variations of the backscattering coefficient measured by radar altimeters over the Antarctic Ice Sheet

    NASA Astrophysics Data System (ADS)

    Ibrahime Adodo, Fifi; Remy, Frédérique; Picard, Ghislain

    2018-05-01

    Spaceborne radar altimeters are a valuable tool for observing the Antarctic Ice Sheet. The radar wave interaction with the snow provides information on both the surface and the subsurface of the snowpack due to its dependence on the snow properties. However, the penetration of the radar wave within the snowpack also induces a negative bias on the estimated surface elevation. Empirical corrections of this space- and time-varying bias are usually based on the backscattering coefficient variability. We investigate the spatial and seasonal variations of the backscattering coefficient at the S (3.2 GHz ˜ 9.4 cm), Ku (13.6 GHz ˜ 2.3 cm) and Ka (37 GHz ˜ 0.8 cm) bands. We identified that the backscattering coefficient at Ku band reaches a maximum in winter in part of the continent (Region 1) and in the summer in the remaining (Region 2), while the evolution at other frequencies is relatively uniform over the whole continent. To explain this contrasting behavior between frequencies and between regions, we studied the sensitivity of the backscattering coefficient at three frequencies to several parameters (surface snow density, snow temperature and snow grain size) using an electromagnetic model. The results show that the seasonal cycle of the backscattering coefficient at Ka frequency is dominated by the volume echo and is mainly driven by snow temperature evolution everywhere. In contrast, at S band, the cycle is dominated by the surface echo. At Ku band, the seasonal cycle is dominated by the volume echo in Region 1 and by the surface echo in Region 2. This investigation provides new information on the seasonal dynamics of the Antarctic Ice Sheet surface and provides new clues to build more accurate corrections of the radar altimeter surface elevation signal in the future.

  10. Advances in Airborne Altimetric Techniques for the Measurement of Snow on Arctic Sea Ice

    NASA Astrophysics Data System (ADS)

    Newman, T.; Farrell, S. L.; Richter-Menge, J.; Elder, B. C.; Ruth, J.; Connor, L. N.

    2014-12-01

    Current sea ice observations and models indicate a transition towards a more seasonal Arctic ice pack with a smaller, and geographically more variable, multiyear ice component. To gain a comprehensive understanding of the processes governing this transition it is important to include the impact of the snow cover, determining the mechanisms by which snow is both responding to and forcing changes to the sea ice pack. Data from NASA's Operation IceBridge (OIB) snow radar system, which has been making yearly surveys of the western Arctic since 2009, offers a key resource for investigating the snow cover. In this work, we characterize the OIB snow radar instrument response to ascertain the location of 'side-lobes', aiding the interpretation of snow radar data. We apply novel wavelet-based techniques to identify the primary reflecting interfaces within the snow pack from which snow depth estimates are derived. We apply these techniques to the range of available snow radar data collected over the last 6 years during the NASA OIB mission. Our results are validated through comparison with a range of in-situ data. We discuss the impact of sea ice surface morphology on snow radar returns (with respect to ice type) and the topographic conditions over which accurate snow-radar-derived snow depths may be obtained. Finally we present improvements to in situ survey design that will allow for both an improved sampling of the snow radar footprint and more accurate assessment of the uncertainties in radar-derived snow depths in the future.

  11. Canadian snow and sea ice: assessment of snow, sea ice, and related climate processes in Canada's Earth system model and climate-prediction system

    NASA Astrophysics Data System (ADS)

    Kushner, Paul J.; Mudryk, Lawrence R.; Merryfield, William; Ambadan, Jaison T.; Berg, Aaron; Bichet, Adéline; Brown, Ross; Derksen, Chris; Déry, Stephen J.; Dirkson, Arlan; Flato, Greg; Fletcher, Christopher G.; Fyfe, John C.; Gillett, Nathan; Haas, Christian; Howell, Stephen; Laliberté, Frédéric; McCusker, Kelly; Sigmond, Michael; Sospedra-Alfonso, Reinel; Tandon, Neil F.; Thackeray, Chad; Tremblay, Bruno; Zwiers, Francis W.

    2018-04-01

    The Canadian Sea Ice and Snow Evolution (CanSISE) Network is a climate research network focused on developing and applying state-of-the-art observational data to advance dynamical prediction, projections, and understanding of seasonal snow cover and sea ice in Canada and the circumpolar Arctic. This study presents an assessment from the CanSISE Network of the ability of the second-generation Canadian Earth System Model (CanESM2) and the Canadian Seasonal to Interannual Prediction System (CanSIPS) to simulate and predict snow and sea ice from seasonal to multi-decadal timescales, with a focus on the Canadian sector. To account for observational uncertainty, model structural uncertainty, and internal climate variability, the analysis uses multi-source observations, multiple Earth system models (ESMs) in Phase 5 of the Coupled Model Intercomparison Project (CMIP5), and large initial-condition ensembles of CanESM2 and other models. It is found that the ability of the CanESM2 simulation to capture snow-related climate parameters, such as cold-region surface temperature and precipitation, lies within the range of currently available international models. Accounting for the considerable disagreement among satellite-era observational datasets on the distribution of snow water equivalent, CanESM2 has too much springtime snow mass over Canada, reflecting a broader northern hemispheric positive bias. Biases in seasonal snow cover extent are generally less pronounced. CanESM2 also exhibits retreat of springtime snow generally greater than observational estimates, after accounting for observational uncertainty and internal variability. Sea ice is biased low in the Canadian Arctic, which makes it difficult to assess the realism of long-term sea ice trends there. The strengths and weaknesses of the modelling system need to be understood as a practical tradeoff: the Canadian models are relatively inexpensive computationally because of their moderate resolution, thus enabling their

  12. Leads in Arctic pack ice enable early phytoplankton blooms below snow-covered sea ice

    PubMed Central

    Assmy, Philipp; Fernández-Méndez, Mar; Duarte, Pedro; Meyer, Amelie; Randelhoff, Achim; Mundy, Christopher J.; Olsen, Lasse M.; Kauko, Hanna M.; Bailey, Allison; Chierici, Melissa; Cohen, Lana; Doulgeris, Anthony P.; Ehn, Jens K.; Fransson, Agneta; Gerland, Sebastian; Hop, Haakon; Hudson, Stephen R.; Hughes, Nick; Itkin, Polona; Johnsen, Geir; King, Jennifer A.; Koch, Boris P.; Koenig, Zoe; Kwasniewski, Slawomir; Laney, Samuel R.; Nicolaus, Marcel; Pavlov, Alexey K.; Polashenski, Christopher M.; Provost, Christine; Rösel, Anja; Sandbu, Marthe; Spreen, Gunnar; Smedsrud, Lars H.; Sundfjord, Arild; Taskjelle, Torbjørn; Tatarek, Agnieszka; Wiktor, Jozef; Wagner, Penelope M.; Wold, Anette; Steen, Harald; Granskog, Mats A.

    2017-01-01

    The Arctic icescape is rapidly transforming from a thicker multiyear ice cover to a thinner and largely seasonal first-year ice cover with significant consequences for Arctic primary production. One critical challenge is to understand how productivity will change within the next decades. Recent studies have reported extensive phytoplankton blooms beneath ponded sea ice during summer, indicating that satellite-based Arctic annual primary production estimates may be significantly underestimated. Here we present a unique time-series of a phytoplankton spring bloom observed beneath snow-covered Arctic pack ice. The bloom, dominated by the haptophyte algae Phaeocystis pouchetii, caused near depletion of the surface nitrate inventory and a decline in dissolved inorganic carbon by 16 ± 6 g C m−2. Ocean circulation characteristics in the area indicated that the bloom developed in situ despite the snow-covered sea ice. Leads in the dynamic ice cover provided added sunlight necessary to initiate and sustain the bloom. Phytoplankton blooms beneath snow-covered ice might become more common and widespread in the future Arctic Ocean with frequent lead formation due to thinner and more dynamic sea ice despite projected increases in high-Arctic snowfall. This could alter productivity, marine food webs and carbon sequestration in the Arctic Ocean. PMID:28102329

  13. Comparison of Retracking Algorithms Using Airborne Radar and Laser Altimeter Measurements of the Greenland Ice Sheet

    NASA Technical Reports Server (NTRS)

    Ferraro, Ellen J.; Swift, Calvin T.

    1995-01-01

    This paper compares four continental ice sheet radar altimeter retracking algorithms using airborne radar and laser altimeter data taken over the Greenland ice sheet in 1991. The refurbished Advanced Application Flight Experiment (AAFE) airborne radar altimeter has a large range window and stores the entire return waveform during flight. Once the return waveforms are retracked, or post-processed to obtain the most accurate altitude measurement possible, they are compared with the high-precision Airborne Oceanographic Lidar (AOL) altimeter measurements. The AAFE waveforms show evidence of varying degrees of both surface and volume scattering from different regions of the Greenland ice sheet. The AOL laser altimeter, however, obtains a return only from the surface of the ice sheet. Retracking altimeter waveforms with a surface scattering model results in a good correlation with the laser measurements in the wet and dry-snow zones, but in the percolation region of the ice sheet, the deviation between the two data sets is large due to the effects of subsurface and volume scattering. The Martin et al model results in a lower bias than the surface scattering model, but still shows an increase in the noise level in the percolation zone. Using an Offset Center of Gravity algorithm to retrack altimeter waveforms results in measurements that are only slightly affected by subsurface and volume scattering and, despite a higher bias, this algorithm works well in all regions of the ice sheet. A cubic spline provides retracked altitudes that agree with AOL measurements over all regions of Greenland. This method is not sensitive to changes in the scattering mechanisms of the ice sheet and it has the lowest noise level and bias of all the retracking methods presented.

  14. Snow crystal imaging using scanning electron microscopy: III. Glacier ice, snow and biota

    USGS Publications Warehouse

    Rango, A.; Wergin, W.P.; Erbe, E.F.; Josberger, E.G.

    2000-01-01

    Low-temperature scanning electron microscopy (SEM) was used to observe metamorphosed snow, glacial firn, and glacial ice obtained from South Cascade Glacier in Washington State, USA. Biotic samples consisting of algae (Chlamydomonas nivalis) and ice worms (a species of oligochaetes) were also collected and imaged. In the field, the snow and biological samples were mounted on copper plates, cooled in liquid nitrogen, and stored in dry shipping containers which maintain a temperature of -196??C. The firn and glacier ice samples were obtained by extracting horizontal ice cores, 8 mm in diameter, at different levels from larger standard glaciological (vertical) ice cores 7.5 cm in diameter. These samples were cooled in liquid nitrogen and placed in cryotubes, were stored in the same dry shipping container, and sent to the SEM facility. In the laboratory, the samples were sputter coated with platinum and imaged by a low-temperature SEM. To image the firn and glacier ice samples, the cores were fractured in liquid nitrogen, attached to a specimen holder, and then imaged. While light microscope images of snow and ice are difficult to interpret because of internal reflection and refraction, the SEM images provide a clear and unique view of the surface of the samples because they are generated from electrons emitted or reflected only from the surface of the sample. In addition, the SEM has a great depth of field with a wide range of magnifying capabilities. The resulting images clearly show the individual grains of the seasonal snowpack and the bonding between the snow grains. Images of firn show individual ice crystals, the bonding between the crystals, and connected air spaces. Images of glacier ice show a crystal structure on a scale of 1-2 mm which is considerably smaller than the expected crystal size. Microscopic air bubbles, less than 15 ??m in diameter, clearly marked the boundaries between these crystal-like features. The life forms associated with the glacier were

  15. Snow accumulation on Arctic sea ice: is it a matter of how much or when?

    NASA Astrophysics Data System (ADS)

    Webster, M.; Petty, A.; Boisvert, L.; Markus, T.

    2017-12-01

    Snow on sea ice plays an important, yet sometimes opposing role in sea ice mass balance depending on the season. In autumn and winter, snow reduces the heat exchange from the ocean to the atmosphere, reducing sea ice growth. In spring and summer, snow shields sea ice from solar radiation, delaying sea ice surface melt. Changes in snow depth and distribution in any season therefore directly affect the mass balance of Arctic sea ice. In the western Arctic, a decreasing trend in spring snow depth distribution has been observed and attributed to the combined effect of peak snowfall rates in autumn and the coincident delay in sea ice freeze-up. Here, we build on this work and present an in-depth analysis on the relationship between snow accumulation and the timing of sea ice freeze-up across all Arctic regions. A newly developed two-layer snow model is forced with eight reanalysis precipitation products to: (1) identify the seasonal distribution of snowfall accumulation for different regions, (2) highlight which regions are most sensitive to the timing of sea ice freeze-up with regard to snow accumulation, and (3) show, if precipitation were to increase, which regions would be most susceptible to thicker snow covers. We also utilize a comprehensive sensitivity study to better understand the factors most important in controlling winter/spring snow depths, and to explore what could happen to snow depth on sea ice in a warming Arctic climate.

  16. Snow depth of the Weddell and Bellingshausen sea ice covers from IceBridge surveys in 2010 and 2011: An examination

    NASA Astrophysics Data System (ADS)

    Kwok, R.; Maksym, T.

    2014-07-01

    We examine the snow radar data from the Weddell and Bellingshausen Seas acquired by eight IceBridge (OIB) flightlines in October of 2010 and 2011. In snow depth retrieval, the sidelobes from the stronger scattering snow-ice (s-i) interfaces could be misidentified as returns from the weaker air-snow (a-s) interfaces. In this paper, we first introduce a retrieval procedure that accounts for the structure of the radar system impulse response followed by a survey of the snow depths in the Weddell and Bellingshausen Seas. Limitations and potential biases in our approach are discussed. Differences between snow depth estimates from a repeat survey of one Weddell Sea track separated by 12 days, without accounting for variability due to ice motion, is -0.7 ± 13.6 cm. Average snow depth is thicker in coastal northwestern Weddell and thins toward Cape Norvegia, a decrease of >30 cm. In the Bellingshausen, the thickest snow is found nearshore in both Octobers and is thickest next to the Abbot Ice Shelf. Snow depth is linearly related to freeboard when freeboards are low but diverge as the freeboard increases especially in the thicker/rougher ice of the western Weddell. We find correlations of 0.71-0.84 between snow depth and surface roughness suggesting preferential accumulation over deformed ice. Retrievals also seem to be related to radar backscatter through surface roughness. Snow depths reported here, generally higher than those from in situ records, suggest dissimilarities in sample populations. Implications of these differences on Antarctic sea ice thickness are discussed.

  17. History of the Greenland Ice Sheet: paleoclimatic insights

    USGS Publications Warehouse

    Alley, Richard B.; Andrews, John T.; Brigham-Grette, J.; Clarke, G.K.C.; Cuffey, Kurt M.; Fitzpatrick, J.J.; Funder, S.; Marshall, S.J.; Miller, G.H.; Mitrovica, J.X.; Muhs, D.R.; Otto-Bliesner, B. L.; Polyak, L.; White, J.W.C.

    2010-01-01

    Paleoclimatic records show that the GreenlandIce Sheet consistently has lost mass in response to warming, and grown in response to cooling. Such changes have occurred even at times of slow or zero sea-level change, so changing sea level cannot have been the cause of at least some of the ice-sheet changes. In contrast, there are no documented major ice-sheet changes that occurred independent of temperature changes. Moreover, snowfall has increased when the climate warmed, but the ice sheet lost mass nonetheless; increased accumulation in the ice sheet's center has not been sufficient to counteract increased melting and flow near the edges. Most documented forcings and ice-sheet responses spanned periods of several thousand years, but limited data also show rapid response to rapid forcings. In particular, regions near the ice margin have responded within decades. However, major changes of central regions of the ice sheet are thought to require centuries to millennia. The paleoclimatic record does not yet strongly constrain how rapidly a major shrinkage or nearly complete loss of the ice sheet could occur. The evidence suggests nearly total ice-sheet loss may result from warming of more than a few degrees above mean 20th century values, but this threshold is poorly defined (perhaps as little as 2 °C or more than 7 °C). Paleoclimatic records are sufficiently sketchy that the ice sheet may have grown temporarily in response to warming, or changes may have been induced by factors other than temperature, without having been recorded.

  18. Capabilities and performance of Elmer/Ice, a new generation ice-sheet model

    NASA Astrophysics Data System (ADS)

    Gagliardini, O.; Zwinger, T.; Gillet-Chaulet, F.; Durand, G.; Favier, L.; de Fleurian, B.; Greve, R.; Malinen, M.; Martín, C.; Råback, P.; Ruokolainen, J.; Sacchettini, M.; Schäfer, M.; Seddik, H.; Thies, J.

    2013-03-01

    The Fourth IPCC Assessment Report concluded that ice-sheet flow models are unable to forecast the current increase of polar ice sheet discharge and the associated contribution to sea-level rise. Since then, the glaciological community has undertaken a huge effort to develop and improve a new generation of ice-flow models, and as a result, a significant number of new ice-sheet models have emerged. Among them is the parallel finite-element model Elmer/Ice, based on the open-source multi-physics code Elmer. It was one of the first full-Stokes models used to make projections for the evolution of the whole Greenland ice sheet for the coming two centuries. Originally developed to solve local ice flow problems of high mechanical and physical complexity, Elmer/Ice has today reached the maturity to solve larger scale problems, earning the status of an ice-sheet model. Here, we summarise almost 10 yr of development performed by different groups. We present the components already included in Elmer/Ice, its numerical performance, selected applications, as well as developments planned for the future.

  19. Response of the Antarctic ice sheet to ocean forcing using the POPSICLES coupled ice sheet-ocean model

    NASA Astrophysics Data System (ADS)

    Martin, D. F.; Asay-Davis, X.; Price, S. F.; Cornford, S. L.; Maltrud, M. E.; Ng, E. G.; Collins, W.

    2014-12-01

    We present the response of the continental Antarctic ice sheet to sub-shelf-melt forcing derived from POPSICLES simulation results covering the full Antarctic Ice Sheet and the Southern Ocean spanning the period 1990 to 2010. Simulations are performed at 0.1 degree (~5 km) ocean resolution and ice sheet resolution as fine as 500 m using adaptive mesh refinement. A comparison of fully-coupled and comparable standalone ice-sheet model results demonstrates the importance of two-way coupling between the ice sheet and the ocean. The POPSICLES model couples the POP2x ocean model, a modified version of the Parallel Ocean Program (Smith and Gent, 2002), and the BISICLES ice-sheet model (Cornford et al., 2012). BISICLES makes use of adaptive mesh refinement to fully resolve dynamically-important regions like grounding lines and employs a momentum balance similar to the vertically-integrated formulation of Schoof and Hindmarsh (2009). Results of BISICLES simulations have compared favorably to comparable simulations with a Stokes momentum balance in both idealized tests like MISMIP3D (Pattyn et al., 2013) and realistic configurations (Favier et al. 2014). POP2x includes sub-ice-shelf circulation using partial top cells (Losch, 2008) and boundary layer physics following Holland and Jenkins (1999), Jenkins (2001), and Jenkins et al. (2010). Standalone POP2x output compares well with standard ice-ocean test cases (e.g., ISOMIP; Losch, 2008) and other continental-scale simulations and melt-rate observations (Kimura et al., 2013; Rignot et al., 2013). A companion presentation, "Present-day circum-Antarctic simulations using the POPSICLES coupled land ice-ocean model" in session C027 describes the ocean-model perspective of this work, while we focus on the response of the ice sheet and on details of the model. The figure shows the BISICLES-computed vertically-integrated ice velocity field about 1 month into a 20-year coupled Antarctic run. Groundling lines are shown in green.

  20. Windblown Snow

    NASA Image and Video Library

    2011-04-11

    On April 11, 2011, IceBridge finally got the clear weather necessary to fly over glaciers in southeast Greenland, but with clear skies came winds of up to 70 knots. What looks like clouds is actually wind-blown snow. The data could help scientists to evaluate the impact of wind-blown snow on satellite-based laser altimetry measurements. Operation IceBridge, now in its third year, makes annual campaigns in the Arctic and Antarctic where science flights monitor glaciers, ice sheets and sea ice. Credit: NASA/GSFC/Michael Studinger To learn more about Ice Bridge go to: www.nasa.gov/mission_pages/icebridge/news/spr11/index.html NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. Follow us on Twitter Join us on Facebook

  1. Snow and ice: Chapter 3

    USGS Publications Warehouse

    Littell, Jeremy; McAfee, Stephanie A.; O'Neel, Shad; Sass, Louis; Burgess, Evan; Colt, Steve; Clark, Paul; Hayward, Gregory D.; Colt, Steve; McTeague, Monica L.; Hollingsworth, Teresa N.

    2017-01-01

    Temperature and precipitation are key determinants of snowpack levels. Therefore, climate change is likely to affect the role of snow and ice in the landscapes and hydrology of the Chugach National Forest region.Downscaled climate projections developed by Scenarios Network for Alaska and Arctic Planning (SNAP) are useful for examining projected changes in snow at relatively fine resolution using a variable called “snowday fraction (SDF),” the percentage of days with precipitation falling as snow.We summarized SNAP monthly SDF from five different global climate models for the Chugach region by 500 m elevation bands, and compared historical (1971–2000) and future (2030–2059) SDF. We found that:Snow-day fraction and snow-water equivalent (SWE) are projected to decline most in late autumn (October to November) and at lower elevations.Snow-day fraction is projected to decrease 23 percent (averaged across five climate models) from October to March, between sea level and 500 m. Between sea level and 1000 m, SDF is projected to decrease by 17 percent between October and March.Snow-water equivalent is projected to decrease most in autumn (October and November) and at lower elevations (below 1500 m), an average of -26 percent for the 2030–2059 period compared to 1971– 2000. Averaged across the cool season and the entire domain, SWE is projected to decrease at elevations below 1000 m because of increased temperature, but increase at higher elevations because of increased precipitation.Compared to 1971–2000, the percentage of the landscape that is snowdominant in 2030–2059 is projected to decrease, and the percentage in which rain and snow are co-dominant (transient hydrology) is projected to increase from 27 to 37 percent. Most of this change is at lower elevations.Glaciers on the Chugach National Forest are currently losing about 6 km3 of ice per year; half of this loss comes from Columbia Glacier (Berthier et al. 2010).Over the past decade, almost all

  2. Snow and Ice Crust Changes over Northern Eurasia since 1966

    NASA Astrophysics Data System (ADS)

    Bulygina, O.; Groisman, P. Y.; Razuvaev, V.; Radionov, V.

    2009-12-01

    When temperature of snow cover reaches zero Celsius first time since its establishment, snowmelt starts. In many parts of the world this process can be lengthy. The initial amount of heat that “arrives” to the snowpack might be insufficient for complete snowmelt, during the colder nights re-freeze of the melted snow may occur (thus creating the ice crust layers), and a new cold front (or the departure of the warm front that initiated melt) can decrease temperatures below the freezing point again and stop the snowmelt completely. It well can be that first such snowmelt occurs in winter (thaw day) and for several months thereafter snowpack stays on the ground. However, even the first such melt initiates a process of snow metamorphosis on its surface changing snow albedo and generating snow crust as well as on its bottom generating ice crust. Once emerged, the crusts will not disappear until the complete snowmelt. Furthermore, these crusts have numerous pathways of impact on the wild birds and animals in the Arctic environment as well as on domesticated reindeers. In extreme cases, the crusts may kill some wild species and prevent reindeers’ migration and feeding. Ongoing warming in high latitudes created situations when in the western half of Eurasian continent days with thaw became more frequent. Keeping in mind potential detrimental impacts of winter thaws and associated with them snow/ice crust development, it is worthwhile to study directly what are the major features of snow and ice crust over Eurasia and what is their dynamics. For the purpose of this study, we employed the national snow survey data set archived at the Russian Institute for Hydrometeorological Information. The dataset has routine snow surveys run throughout the cold season each decade (during the intense snowmelt, each 5 days) at all meteorological stations of the former USSR, thereafter, in Russia since 1966. Prior to 1966 snow surveys are also available but the methodology of

  3. Quantifying Local Ablation Rates for the Greenland Ice Sheet Using Terrestrial LIDAR

    NASA Astrophysics Data System (ADS)

    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.

    2016-12-01

    Quantifying accurate ice surface ablation or melt rates for the Greenland Ice Sheet is important for calibrating and validating surface mass balance models and constraining sea level rise estimates. Common practice is to monitor surface ablation at defined points by manually measuring ice surface lowering in relation to stakes inserted into the ice / snow. However, this method does not account for the effects of local topography, solar zenith angle, and local variations in ice 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 Ice 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 IceBridge and NASA's Land, Vegetation & Ice Sensor - LVIS) and forthcoming spaceborne sensors (e.g. NASA's ICESat-2).

  4. Role of ice sheet dynamics in the collapse of the early-Holocene Laurentide Ice Sheet

    NASA Astrophysics Data System (ADS)

    Matero, I. S. O.; Gregoire, L. J.; Cornford, S. L.; Ivanovic, R. F.

    2017-12-01

    The last stage of the deglaciation of the Laurentide Ice Sheet (LIS) during the early Holocene Thermal Maximum ( 9000 to 7000 years ago) provides an analogy and insight to the possible responses of contemporary ice sheets in a warming climate. What makes LIS particularly interesting is that meltwater from the collapse of an ice saddle over Hudson Bay was recently shown to be the primary forcing for the period of abrupt northern hemisphere cooling known as the 8.2 ka event. The evolution of the LIS during this period was likely influenced by its interaction with marginal lakes and the ocean, and its major ice stream, which exported ice towards Hudson Strait. Accurately simulating the early Holocene LIS evolution thus requires a model such as BISICLES, capable of accurately and efficiently resolving ice stream dynamics and grounding line migration thanks to the combined use of higher order physics and adaptive mesh refinement. We drive the BISICLES model using a positive degree day mass balance scheme with monthly precipitation and temperature from the HadCM3 climate model under climatic conditions from 10,000 to 8,000 years ago. We test the effect of varying the initial topographies and ice thicknesses from different timeslices in the ICE-6Gc reconstruction. We also test different parameterisations for the basal friction based on the thicknesses of the underlying sediments. These simulations evaluate the role of the Hudson Strait ice stream, ice sheet dynamics and interactions with the adjacent proglacial Lake Agassiz and North Atlantic Ocean in the collapse of the LIS. Our results highlight that the choice of parameterisation for basal friction has major effects on ice sheet dynamics and evolution.

  5. Capabilities and performance of the new generation ice-sheet model Elmer/Ice

    NASA Astrophysics Data System (ADS)

    Gagliardini, O.; Zwinger, T.; Durand, G.; Favier, L.; de Fleurian, B.; Gillet-chaulet, F.; Seddik, H.; Greve, R.; Mallinen, M.; Martin, C.; Raback, P.; Ruokolainen, J.; Schäfer, M.; Thies, J.

    2012-12-01

    Since the Fourth IPCC Assessment Report, and its conclusion about the inability of ice-sheet flow models to forecast the current increase of polar ice sheet discharge and associated contribution to sea-level rise, a huge development effort has been undertaken by the glaciological community. All around the world, models have been improved and, interestingly, a significant number of new ice-sheet models have emerged. Among them, the parallel finite-element model Elmer/Ice (based on the open-source multi-physics code Elmer) was one of the first full-Stokes models used to make projections of the future of the whole Greenland ice sheet for the coming two centuries. Originally developed to solve dedicated local ice flow problems of high mechanical and physical complexity, Elmer/Ice has today reached the maturity to solve larger scale problems, earning the status of an ice-sheet model. In this presentation, we summarise the almost 10 years of development performed by different groups. We present the components already included in Elmer/Ice, its numerical performance, selected applications, as well as developments planed for the future.

  6. Water, ice and mud: Lahars and lahar hazards at ice- and snow-clad volcanoes

    USGS Publications Warehouse

    Waythomas, Christopher F.

    2014-01-01

    Large-volume lahars are significant hazards at ice and snow covered volcanoes. Hot eruptive products produced during explosive eruptions can generate a substantial volume of melt water that quickly evolves into highly mobile flows of ice, sediment and water. At present it is difficult to predict the size of lahars that can form at ice and snow covered volcanoes due to their complex flow character and behaviour. However, advances in experiments and numerical approaches are producing new conceptual models and new methods for hazard assessment. Eruption triggered lahars that are ice-dominated leave behind thin, almost unrecognizable sedimentary deposits, making them likely to be under-represented in the geological record.

  7. Modes of supraglacial lake drainage and dynamic ice sheet response

    NASA Astrophysics Data System (ADS)

    Das, S. B.; Behn, M. D.; Joughin, I. R.

    2011-12-01

    We investigate modes of supraglacial lake drainage using geophysical, ground, and remote sensing observations over the western margin of the Greenland ice sheet. Lakes exhibit a characteristic life cycle defined by a pre-drainage, drainage, and post-drainage phase. In the pre-drainage phase winter snow fills pre-existing cracks and stream channels, efficiently blocking past drainage conduits. As temperatures increase in the spring, surface melting commences, initially saturating the snow pack and subsequently forming a surface network of streams that fills the lake basins. Basins continue to fill until lake drainage commences, which for individual lakes occurs at different times depending on the previous winter snow accumulation and summer temperatures. Three styles of drainage behavior have been observed: (1) no drainage, (2) slow drainage over the side into an adjacent pre-existing crack, and (3) rapid drainage through a new crack formed beneath the lake basin. Moreover, from year-to-year individual lakes exhibit different drainage behaviors. Lakes that drain slowly often utilize the same outflow channel for multiple years, creating dramatic canyons in the ice. Ultimately, these surface channels are advected out of the lake basin and a new channel forms. In the post-drainage phase, melt water continues to access the bed typically through a small conduit (e.g. moulin) formed near a local topographic minimum along the main drainage crack, draining the lake catchment throughout the remainder of the melt season. This melt water input to the bed leads to continued basal lubrication and enhanced ice flow compared to background velocities. Lakes that do not completely drain freeze over to form a surface ice layer that persists into the following year. Our results show that supraglacial lakes show a spectrum of drainage behaviors and that these styles of drainage lead to varying rates and timing of surface meltwater delivery to the bed resulting in different dynamic ice

  8. Holocene deceleration of the Greenland Ice Sheet.

    PubMed

    MacGregor, Joseph A; Colgan, William T; Fahnestock, Mark A; Morlighem, Mathieu; Catania, Ginny A; Paden, John D; Gogineni, S Prasad

    2016-02-05

    Recent peripheral thinning of the Greenland Ice Sheet is partly offset by interior thickening and is overprinted on its poorly constrained Holocene evolution. On the basis of the ice sheet's radiostratigraphy, ice flow in its interior is slower now than the average speed over the past nine millennia. Generally higher Holocene accumulation rates relative to modern estimates can only partially explain this millennial-scale deceleration. The ice sheet's dynamic response to the decreasing proportion of softer ice from the last glacial period and the deglacial collapse of the ice bridge across Nares Strait also contributed to this pattern. Thus, recent interior thickening of the Greenland Ice Sheet is partly an ongoing dynamic response to the last deglaciation that is large enough to affect interpretation of its mass balance from altimetry. Copyright © 2016, American Association for the Advancement of Science.

  9. Optimizing Observations of Sea Ice Thickness and Snow Depth in the Arctic

    DTIC Science & Technology

    2015-09-30

    Region Research and Engineering Laboratory (CRREL), Naval Research Laboratory (NRL) and National Aeronautics and Space Administration ( NASA ) in...and results from this focused effort with data collected during related national and international activities (e.g. other NASA IceBridge sea ice...surface elevation of the snow or ice/air interface, and radar altimetry measurements of the snow/ice interface, taken by NASA IceBridge and NRL

  10. Ultra-Wideband Radar Measurements of Thickness of Snow Over Sea Ice

    NASA Technical Reports Server (NTRS)

    Kanagaratnam, P.; Markus, T.; Lytle, V.; Heavey, B.; Jansen, P.; Prescott, G.; Gogineni, S.

    2007-01-01

    An accurate knowledge of snow thickness and its variability over sea ice is crucial for determining the overall polar heat and freshwater budget, which influences the global climate. Recently, algorithms have been developed to extract snow thicknesses from passive microwave satellite data. However, validation of these data over the large footprint of the passive microwave sensor has been a challenge. The only method used thus far has been with meter sticks during ship cruises. To address this problem, we developed an ultra wideband frequency-modulated continuous-wave (FM-CW) radar to measure snow thickness over sea ice. We made snow-thickness measurements over Antarctic sea ice by operating the radar from a sled during September and October, 2003. We performed radar measurements over 11 stations with varying snow thickness between 4 and 85 cm. We observed excellent agreement between radar estimates of snow thickness with physical measurements, achieving a correlation coefficient of 0.95 and a vertical resolution of about 3 cm.

  11. Simulation of the Greenland Ice Sheet over two glacial-interglacial cycles: investigating a sub-ice-shelf melt parameterization and relative sea level forcing in an ice-sheet-ice-shelf model

    NASA Astrophysics Data System (ADS)

    Bradley, Sarah L.; Reerink, Thomas J.; van de Wal, Roderik S. W.; Helsen, Michiel M.

    2018-05-01

    Observational evidence, including offshore moraines and sediment cores, confirm that at the Last Glacial Maximum (LGM) the Greenland ice sheet (GrIS) expanded to a significantly larger spatial extent than seen at present, grounding into Baffin Bay and out onto the continental shelf break. Given this larger spatial extent and its close proximity to the neighbouring Laurentide Ice Sheet (LIS) and Innuitian Ice Sheet (IIS), it is likely these ice sheets will have had a strong non-local influence on the spatial and temporal behaviour of the GrIS. Most previous paleo ice-sheet modelling simulations recreated an ice sheet that either did not extend out onto the continental shelf or utilized a simplified marine ice parameterization which did not fully include the effect of ice shelves or neglected the sensitivity of the GrIS to this non-local bedrock signal from the surrounding ice sheets. In this paper, we investigated the evolution of the GrIS over the two most recent glacial-interglacial cycles (240 ka BP to the present day) using the ice-sheet-ice-shelf model IMAU-ICE. We investigated the solid earth influence of the LIS and IIS via an offline relative sea level (RSL) forcing generated by a glacial isostatic adjustment (GIA) model. The RSL forcing governed the spatial and temporal pattern of sub-ice-shelf melting via changes in the water depth below the ice shelves. In the ensemble of simulations, at the glacial maximums, the GrIS coalesced with the IIS to the north and expanded to the continental shelf break to the southwest but remained too restricted to the northeast. In terms of the global mean sea level contribution, at the Last Interglacial (LIG) and LGM the ice sheet added 1.46 and -2.59 m, respectively. This LGM contribution by the GrIS is considerably higher (˜ 1.26 m) than most previous studies whereas the contribution to the LIG highstand is lower (˜ 0.7 m). The spatial and temporal behaviour of the northern margin was highly variable in all simulations

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

    NASA Technical Reports Server (NTRS)

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

    1997-01-01

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

  13. Perennial snow and ice volumes on Iliamna Volcano, Alaska, estimated with ice radar and volume modeling

    USGS Publications Warehouse

    Trabant, Dennis C.

    1999-01-01

    The volume of four of the largest glaciers on Iliamna Volcano was estimated using the volume model developed for evaluating glacier volumes on Redoubt Volcano. The volume model is controlled by simulated valley cross sections that are constructed by fitting third-order polynomials to the shape of the valley walls exposed above the glacier surface. Critical cross sections were field checked by sounding with ice-penetrating radar during July 1998. The estimated volumes of perennial snow and glacier ice for Tuxedni, Lateral, Red, and Umbrella Glaciers are 8.6, 0.85, 4.7, and 0.60 cubic kilometers respectively. The estimated volume of snow and ice on the upper 1,000 meters of the volcano is about 1 cubic kilometer. The volume estimates are thought to have errors of no more than ?25 percent. The volumes estimated for the four largest glaciers are more than three times the total volume of snow and ice on Mount Rainier and about 82 times the total volume of snow and ice that was on Mount St. Helens before its May 18, 1980 eruption. Volcanoes mantled by substantial snow and ice covers have produced the largest and most catastrophic lahars and floods. Therefore, it is prudent to expect that, during an eruptive episode, flooding and lahars threaten all of the drainages heading on Iliamna Volcano. On the other hand, debris avalanches can happen any time. Fortunately, their influence is generally limited to the area within a few kilometers of the summit.

  14. North American study on contracting snow and ice response : final report.

    DOT National Transportation Integrated Search

    2017-01-01

    Snow and ice control operations are a vital function often conducted by state and local transportation agencies. Many states are choosing to contract snow and ice response services, instead of or in addition to the use of in-house forces, to maintain...

  15. Operational satellites and the global monitoring of snow and ice

    NASA Technical Reports Server (NTRS)

    Walsh, John E.

    1991-01-01

    The altitudinal dependence of the global warming projected by global climate models is at least partially attributable to the albedo-temperature feedback involving snow and ice, which must be regarded as key variables in the monitoring for global change. Statistical analyses of data from IR and microwave sensors monitoring the areal coverage and extent of sea ice have led to mixed conclusions about recent trends of hemisphere sea ice coverage. Seasonal snow cover has been mapped for over 20 years by NOAA/NESDIS on the basis of imagery from a variety of satellite sensors. Multichannel passive microwave data show some promise for the routine monitoring of snow depth over unforested land areas.

  16. MODIS Collection 6 Data at the National Snow and Ice Data Center (NSIDC)

    NASA Astrophysics Data System (ADS)

    Fowler, D. K.; Steiker, A. E.; Johnston, T.; Haran, T. M.; Fowler, C.; Wyatt, P.

    2015-12-01

    For over 15 years, the NASA National Snow and Ice Data Center Distributed Active Archive Center (NSIDC DAAC) has archived and distributed snow and sea ice products derived from the Moderate Resolution Imaging Spectroradiometer (MODIS) instruments on the NASA Earth Observing System (EOS) Aqua and Terra satellites. Collection 6 represents the next revision to NSIDC's MODIS archive, mainly affecting the snow-cover products. Collection 6 specifically addresses the needs of the MODIS science community by targeting the scenarios that have historically confounded snow detection and introduced errors into the snow-cover and fractional snow-cover maps even though MODIS snow-cover maps are typically 90 percent accurate or better under good observing conditions, Collection 6 uses revised algorithms to discriminate between snow and clouds, resolve uncertainties along the edges of snow-covered regions, and detect summer snow cover in mountains. Furthermore, Collection 6 applies modified and additional snow detection screens and new Quality Assessment protocols that enhance the overall accuracy of the snow maps compared with Collection 5. Collection 6 also introduces several new MODIS snow products, including a daily Climate Modelling Grid (CMG) cloud gap-filled (CGF) snow-cover map which generates cloud-free maps by using the most recent clear observations.. The MODIS Collection 6 sea ice extent and ice surface temperature algorithms and products are much the same as Collection 5; however, Collection 6 updates to algorithm inputs—in particular, the L1B calibrated radiances, land and water mask, and cloud mask products—have improved the sea ice outputs. The MODIS sea ice products are currently available at NSIDC, and the snow cover products are soon to follow in 2016 NSIDC offers a variety of methods for obtaining these data. Users can download data directly from an online archive or use the NASA Reverb Search & Order Tool to perform spatial, temporal, and parameter

  17. Ice sheet topography by satellite altimetry

    USGS Publications Warehouse

    Brooks, R.L.; Campbell, W.J.; Ramseier, R.O.; Stanley, H.R.; Zwally, H.J.

    1978-01-01

    The surface elevation of the southern Greenland ice sheet and surface features of the ice 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 ice volume, the mass balance of the present ice sheets could be determined by repetitive mapping of the surface elevation and the surface could be monitored to detect surging or significant changes in ice flow. ?? 1978 Nature Publishing Group.

  18. Enhanced ice sheet growth in Eurasia owing to adjacent ice-dammed lakes.

    PubMed

    Krinner, G; Mangerud, J; Jakobsson, M; Crucifix, M; Ritz, C; Svendsen, J I

    2004-01-29

    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 ice-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 ice sheet centred over the Barents and Kara seas blocked the large northbound Russian rivers. Here we present high-resolution simulations with an atmospheric general circulation model that explicitly simulates the surface mass balance of the ice sheet. We show that the main influence of the Eurasian proglacial lakes was a significant reduction of ice sheet melting at the southern margin of the Barents-Kara ice 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 ice sheet growth and delayed ice sheet decay in Eurasia and probably also in North America.

  19. The Response of Ice Sheets to Climate Variability

    NASA Astrophysics Data System (ADS)

    Snow, K.; Goldberg, D. N.; Holland, P. R.; Jordan, J. R.; Arthern, R. J.; Jenkins, A.

    2017-12-01

    West Antarctic Ice Sheet loss is a significant contributor to sea level rise. While the ice loss is thought to be triggered by fluctuations in oceanic heat at the ice shelf bases, ice sheet response to ocean variability remains poorly understood. Using a synchronously coupled ice-ocean model permitting grounding line migration, this study evaluates the response of an ice sheet to periodic variations in ocean forcing. Resulting oscillations in grounded ice 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 ice sheets. The ice shelf residence time offers a critical time scale, above which the ice response amplitude is a linear function of ocean forcing period and below which it is quadratic. These results highlight the sensitivity of West Antarctic ice streams to perturbations in heat fluxes occurring at decadal time scales.

  20. ICESat: Ice, Cloud and Land Elevation Satellite

    NASA Technical Reports Server (NTRS)

    Zwally, Jay; Shuman, Christopher

    2002-01-01

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

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

    PubMed

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

    2012-04-25

    Accurate prediction of global sea-level rise requires that we understand the cause of recent, widespread and intensifying glacier acceleration along Antarctic ice-sheet coastal margins. Atmospheric and oceanic forcing have the potential to reduce the thickness and extent of floating ice shelves, potentially limiting their ability to buttress the flow of grounded tributary glaciers. Indeed, recent ice-shelf collapse led to retreat and acceleration of several glaciers on the Antarctic Peninsula. But the extent and magnitude of ice-shelf thickness change, the underlying causes of such change, and its link to glacier flow rate are so poorly understood that its future impact on the ice sheets cannot yet be predicted. Here we use satellite laser altimetry and modelling of the surface firn layer to reveal the circum-Antarctic pattern of ice-shelf thinning through increased basal melt. We deduce that this increased melt is the primary control of Antarctic ice-sheet loss, through a reduction in buttressing of the adjacent ice sheet leading to accelerated glacier flow. The highest thinning rates occur where warm water at depth can access thick ice shelves via submarine troughs crossing the continental shelf. Wind forcing could explain the dominant patterns of both basal melting and the surface melting and collapse of Antarctic ice shelves, through ocean upwelling in the Amundsen and Bellingshausen seas, and atmospheric warming on the Antarctic Peninsula. This implies that climate forcing through changing winds influences Antarctic ice-sheet mass balance, and hence global sea level, on annual to decadal timescales.

  2. Enhancement of the MODIS Snow and Ice Product Suite Utilizing Image Segmentation

    NASA Technical Reports Server (NTRS)

    Tilton, James C.; Hall, Dorothy K.; Riggs, George A.

    2006-01-01

    A problem has been noticed with the current NODIS Snow and Ice Product in that fringes of certain snow fields are labeled as "cloud" whereas close inspection of the data indicates that the correct labeling is a non-cloud category such as snow or land. This occurs because the current MODIS Snow and Ice Product generation algorithm relies solely on the MODIS Cloud Mask Product for the labeling of image pixels as cloud. It is proposed here that information obtained from image segmentation can be used to determine when it is appropriate to override the cloud indication from the cloud mask product. Initial tests show that this approach can significantly reduce the cloud "fringing" in modified snow cover labeling. More comprehensive testing is required to determine whether or not this approach consistently improves the accuracy of the snow and ice product.

  3. Snow depth retrieval from L-band satellite measurements on Arctic and Antarctic sea ice

    NASA Astrophysics Data System (ADS)

    Maaß, N.; Kaleschke, L.; Wever, N.; Lehning, M.; Nicolaus, M.; Rossmann, H. L.

    2017-12-01

    The passive microwave mission SMOS provides daily coverage of the polar regions and measures at a low frequency of 1.4 GHz (L-band). SMOS observations have been used to operationally retrieve sea ice thickness up to 1 m and to estimate snow depth in the Arctic for thicker ice. Here, we present how SMOS-retrieved snow depths compare with airborne measurements from NASA's Operation IceBridge mission (OIB) and with AMSR-2 satellite retrievals at higher frequencies, and we show first applications to Antarctic sea ice. In previous studies, SMOS and OIB snow depths showed good agreement on spatial scales from 50 to 1000 km for some days and disagreement for other days. Here, we present a more comprehensive comparison of OIB and SMOS snow depths in the Arctic for 2011 to 2015. We find that the SMOS retrieval works best for cold conditions and depends on auxiliary information on ice surface temperature, here provided by MODIS thermal imagery satellite data. However, comparing SMOS and OIB snow depths is difficult because of the different spatial resolutions (SMOS: 40 km, OIB: 40 m). Spatial variability within the SMOS footprint can lead to different snow conditions as seen from SMOS and OIB. Ideally the comparison is made for uniform conditions: Low lead and open water fraction, low spatial and temporal variability of ice surface temperature, no mixture of multi- and first-year ice. Under these conditions and cold temperatures (surface temperatures below -25°C), correlation coefficients between SMOS and OIB snow depths increase from 0.3 to 0.6. A finding from the comparison with AMSR-2 snow depths is that the SMOS-based maps depend less on the age of the sea ice than the maps derived from higher frequencies. Additionally, we show first results of SMOS snow depths for Antarctic sea ice. SMOS observations are compared to measurements of autonomous snow buoys drifting in the Weddell Sea since 2014. For a better comparability of these point measurements with SMOS data, we use

  4. Extensive massive basal-ice structures in West Antarctica relate to ice-sheet anisotropy and ice-flow

    NASA Astrophysics Data System (ADS)

    Ross, N.; Bingham, R. G.; Corr, H. F. J.; Siegert, M. J.

    2016-12-01

    Complex structures identified within both the East Antarctic and Greenland ice sheets are thought to be generated by the action of basal water freezing to the ice-sheet base, evolving under ice flow. Here, we use ice-penetrating radar to image an extensive series of similarly complex basal ice facies in West Antarctica, revealing a thick (>500 m) tectonised unit in an area of cold-based and relatively slow-flowing ice. We show that major folding and overturning of the unit perpendicular to ice flow elevates deep, warm ice into the mid ice-sheet column. Fold axes align with present ice flow, and axis amplitudes increase down-ice, suggesting long-term consistency in the direction and convergence of flow. In the absence of basal water, and the draping of the tectonised unit over major subglacial mountain ranges, the formation of the unit must be solely through the deformation of meteoric ice. Internal layer radar reflectivity is consistently greater parallel to flow compared with the perpendicular direction, revealing ice-sheet crystal anisotropy is associated with the folding. By linking layers to the Byrd ice-core site, we show the basal ice dates to at least the last glacial cycle and may be as old as the last interglacial. Deformation of deep-ice in this sector of WAIS, and potentially elsewhere in Antarctica, may be caused by differential shearing at interglacial-glacial boundaries, in a process analogous to that proposed for interior Greenland. The scale and heterogeneity of the englacial structures, and their subsequent impact on ice sheet rheology, means that the nature of ice flow across the bulk of West Antarctica must be far more complex that is currently accounted for by any numerical ice sheet model.

  5. The Potsdam Parallel Ice Sheet Model (PISM-PIK) - Part 2: Dynamic equilibrium simulation of the Antarctic ice sheet

    NASA Astrophysics Data System (ADS)

    Martin, M. A.; Winkelmann, R.; Haseloff, M.; Albrecht, T.; Bueler, E.; Khroulev, C.; Levermann, A.

    2010-08-01

    We present a dynamic equilibrium simulation of the ice sheet-shelf system on Antarctica with the Potsdam Parallel Ice Sheet Model (PISM-PIK). The simulation is initialized with present-day conditions for topography and ice thickness and then run to steady state with constant present-day surface mass balance. Surface temperature and basal melt distribution are parameterized. Grounding lines and calving fronts are free to evolve, and their modeled equilibrium state is compared to observational data. A physically-motivated dynamic calving law based on horizontal spreading rates allows for realistic calving fronts for various types of shelves. Steady-state dynamics including surface velocity and ice flux are analyzed for whole Antarctica and the Ronne-Filchner and Ross ice shelf areas in particular. The results show that the different flow regimes in sheet and shelves, and the transition zone between them, are captured reasonably well, supporting the approach of superposition of SIA and SSA for the representation of fast motion of grounded ice. This approach also leads to a natural emergence of streams in this new 3-D marine ice sheet model.

  6. An automated approach for mapping persistent ice and snow cover over high latitude regions

    USGS Publications Warehouse

    Selkowitz, David J.; Forster, Richard R.

    2016-01-01

    We developed an automated approach for mapping persistent ice and snow cover (glaciers and perennial snowfields) from Landsat TM and ETM+ data across a variety of topography, glacier types, and climatic conditions at high latitudes (above ~65°N). Our approach exploits all available Landsat scenes acquired during the late summer (1 August–15 September) over a multi-year period and employs an automated cloud masking algorithm optimized for snow and ice covered mountainous environments. Pixels from individual Landsat scenes were classified as snow/ice covered or snow/ice free based on the Normalized Difference Snow Index (NDSI), and pixels consistently identified as snow/ice covered over a five-year period were classified as persistent ice and snow cover. The same NDSI and ratio of snow/ice-covered days to total days thresholds applied consistently across eight study regions resulted in persistent ice and snow cover maps that agreed closely in most areas with glacier area mapped for the Randolph Glacier Inventory (RGI), with a mean accuracy (agreement with the RGI) of 0.96, a mean precision (user’s accuracy of the snow/ice cover class) of 0.92, a mean recall (producer’s accuracy of the snow/ice cover class) of 0.86, and a mean F-score (a measure that considers both precision and recall) of 0.88. We also compared results from our approach to glacier area mapped from high spatial resolution imagery at four study regions and found similar results. Accuracy was lowest in regions with substantial areas of debris-covered glacier ice, suggesting that manual editing would still be required in these regions to achieve reasonable results. The similarity of our results to those from the RGI as well as glacier area mapped from high spatial resolution imagery suggests it should be possible to apply this approach across large regions to produce updated 30-m resolution maps of persistent ice and snow cover. In the short term, automated PISC maps can be used to rapidly

  7. Programme for Monitoring of the Greenland Ice Sheet - Ice Surface Velocities

    NASA Astrophysics Data System (ADS)

    Andersen, S. B.; Ahlstrom, A. P.; Boncori, J. M.; Dall, J.

    2011-12-01

    In 2007, the Danish Ministry of Climate and Energy launched the Programme for Monitoring of the Greenland Ice Sheet (PROMICE) as an ongoing effort to assess changes in the mass budget of the Greenland Ice Sheet. Iceberg calving from the outlet glaciers of the Greenland Ice Sheet, often termed the ice-dynamic mass loss, is responsible for an important part of the mass loss during the last decade. To quantify this part of the mass loss, we combine airborne surveys yielding ice-sheet thickness along the entire margin, with surface velocities derived from satellite synthetic-aperture radar (SAR). In order to derive ice 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 Ice-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.

  8. Intercomparison of snow depth retrievals over Arctic sea ice from radar data acquired by Operation IceBridge

    NASA Astrophysics Data System (ADS)

    Kwok, Ron; Kurtz, Nathan T.; Brucker, Ludovic; Ivanoff, Alvaro; Newman, Thomas; Farrell, Sinead L.; King, Joshua; Howell, Stephen; Webster, Melinda A.; Paden, John; Leuschen, Carl; MacGregor, Joseph A.; Richter-Menge, Jacqueline; Harbeck, Jeremy; Tschudi, Mark

    2017-11-01

    Since 2009, the ultra-wideband snow radar on Operation IceBridge (OIB; a NASA airborne mission to survey the polar ice covers) has acquired data in annual campaigns conducted during the Arctic and Antarctic springs. Progressive improvements in radar hardware and data processing methodologies have led to improved data quality for subsequent retrieval of snow depth. Existing retrieval algorithms differ in the way the air-snow (a-s) and snow-ice (s-i) interfaces are detected and localized in the radar returns and in how the system limitations are addressed (e.g., noise, resolution). In 2014, the Snow Thickness On Sea Ice Working Group (STOSIWG) was formed and tasked with investigating how radar data quality affects snow depth retrievals and how retrievals from the various algorithms differ. The goal is to understand the limitations of the estimates and to produce a well-documented, long-term record that can be used for understanding broader changes in the Arctic climate system. Here, we assess five retrieval algorithms by comparisons with field measurements from two ground-based campaigns, including the BRomine, Ozone, and Mercury EXperiment (BROMEX) at Barrow, Alaska; a field program by Environment and Climate Change Canada at Eureka, Nunavut; and available climatology and snowfall from ERA-Interim reanalysis. The aim is to examine available algorithms and to use the assessment results to inform the development of future approaches. We present results from these assessments and highlight key considerations for the production of a long-term, calibrated geophysical record of springtime snow thickness over Arctic sea ice.

  9. Probability based hydrologic catchments of the Greenland Ice Sheet

    NASA Astrophysics Data System (ADS)

    Hudson, B. D.

    2015-12-01

    Greenland Ice Sheet melt water impacts ice sheet flow dynamics, fjord and coastal circulation, and sediment and biogeochemical fluxes. Melt water exiting the ice sheet also is a key term in its mass balance. Because of this, knowledge of the area of the ice sheet that contributes melt water to a given outlet (its hydrologic catchment) is important to many ice sheet studies and is especially critical to methods using river runoff to assess ice sheet mass balance. Yet uncertainty in delineating ice sheet hydrologic catchments is a problem that is rarely acknowledged. Ice 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 ice sheet catchments that quantifies the impact of uncertain basal topography. In this scheme, over many iterations I randomly vary the ice sheet bed elevation within published error bounds (using Morlighem et al., 2014 bed and bed error datasets). For each iteration of ice 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 variations 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 ice sheet hydrology would be the most successful, allows reinterpretation of past results, and points to where future radar surveys would be most advantageous.

  10. Multi-decadal evolution of ice/snow covers in the Mont-Blanc massif (France)

    NASA Astrophysics Data System (ADS)

    Guillet, Grégoire; Ravanel, Ludovic

    2017-04-01

    Dynamics and evolution of the major glaciers of the Mont-Blanc massif have been vastly studied since the XXth century. Ice/snow covers on steep rock faces as part of the cryosphere however remain poorly studied with only qualitative descriptions existing. The study of ice/snow covers is primordial to further understand permafrost degradation throughout the Mont-Blanc massif and to improve safety and prevention for mountain sports practitioners. This study focuses on quantifying the evolution of ice/snow covers surface during the past century using a specially developed monoplotting tool using Bayesian statistics and Markov Chain Monte Carlo algorithms. Combining digital elevation models and photographs covering a time-span of 110 years, we calculated the ice/snow cover surface for 3 study sites — North faces of the Tour Ronde (3792 m a.s.l.) and the Grandes Jorasses (4208 m a.s.l.) and Triangle du Tacul (3970 m a.s.l.) — and deduced the evolution of their area throughout the XXth century. First results are showing several increase/decrease periods. The first decrease in ice/snow cover surface occurs between the 1940's and the 1950's. It is followed by an increase up to the 1980's. Since then, ice/snow covers show a general decrease in surface which is faster since the 2010's. Furthermore, the gain/loss during the increase/decrease periods varies with the considered ice/snow cover, making it an interesting cryospheric entity of its own.

  11. Ice Sheet Roughness Estimation Based on Impulse Responses Acquired in the Global Ice Sheet Mapping Orbiter Mission

    NASA Astrophysics Data System (ADS)

    Niamsuwan, N.; Johnson, J. T.; Jezek, K. C.; Gogineni, P.

    2008-12-01

    The Global Ice Sheet Mapping Orbiter (GISMO) mission was developed to address scientific needs to understand the polar ice subsurface structure. This NASA Instrument Incubator Program project is a collaboration between Ohio State University, the University of Kansas, Vexcel Corporation and NASA. The GISMO design utilizes an interferometric SAR (InSAR) strategy in which ice sheet reflected signals received by a dual-antenna system are used to produce an interference pattern. The resulting interferogram can be used to filter out surface clutter so as to reveal the signals scattered from the base of the ice sheet. These signals are further processed to produce 3D-images representing basal topography of the ice sheet. In the past three years, the GISMO airborne field campaigns that have been conducted provide a set of useful data for studying geophysical properties of the Greenland ice sheet. While topography information can be obtained using interferometric SAR processing techniques, ice sheet roughness statistics can also be derived by a relatively simple procedure that involves analyzing power levels and the shape of the radar impulse response waveforms. An electromagnetic scattering model describing GISMO impulse responses has previously been proposed and validated. This model suggested that rms-heights and correlation lengths of the upper surface profile can be determined from the peak power and the decay rate of the pulse return waveform, respectively. This presentation will demonstrate a procedure for estimating the roughness of ice surfaces by fitting the GISMO impulse response model to retrieved waveforms from selected GISMO flights. Furthermore, an extension of this procedure to estimate the scattering coefficient of the glacier bed will be addressed as well. Planned future applications involving the classification of glacier bed conditions based on the derived scattering coefficients will also be described.

  12. Algae Drive Enhanced Darkening of Bare Ice on the Greenland Ice Sheet

    NASA Astrophysics Data System (ADS)

    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.

    2017-11-01

    Surface ablation of the Greenland ice 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 ice 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 ice sheet. The impact of algae on bare ice 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 ice darkening, and incorporating the algal darkening effect will improve mass balance and sea level projections of the Greenland ice sheet and ice masses elsewhere.

  13. How robust are in situ observations for validating satellite-derived albedo over the dark zone of the Greenland Ice Sheet?

    NASA Astrophysics Data System (ADS)

    Ryan, J. C.; Hubbard, A.; Irvine-Fynn, T. D.; Doyle, S. H.; Cook, J. M.; Stibal, M.; Box, J. E.

    2017-06-01

    Calibration and validation of satellite-derived ice sheet albedo data require high-quality, in situ measurements commonly acquired by up and down facing pyranometers mounted on automated weather stations (AWS). However, direct comparison between ground and satellite-derived albedo can only be justified when the measured surface is homogeneous at the length-scale of both satellite pixel and in situ footprint. Here we use digital imagery acquired by an unmanned aerial vehicle to evaluate point-to-pixel albedo comparisons across the western, ablating margin of the Greenland Ice Sheet. Our results reveal that in situ measurements overestimate albedo by up to 0.10 at the end of the melt season because the ground footprints of AWS-mounted pyranometers are insufficient to capture the spatial heterogeneity of the ice surface as it progressively ablates and darkens. Statistical analysis of 21 AWS across the entire Greenland Ice Sheet reveals that almost half suffer from this bias, including some AWS located within the wet snow zone.

  14. How robust are in situ observations for validating satellite-derived albedo over the dark zone of the Greenland Ice Sheet?

    NASA Astrophysics Data System (ADS)

    Ryan, J.; Hubbard, A., II; Irvine-Fynn, T. D.; Doyle, S. H.; Cook, J.; Stibal, M.; Smith, L. C.; Box, J. E.

    2017-12-01

    Calibration and validation of satellite-derived ice sheet albedo data require high-quality, in situ measurements commonly acquired by up and down facing pyranometers mounted on automated weather stations (AWS). However, direct comparison between ground and satellite-derived albedo can only be justified when the measured surface is homogeneous at the length-scale of both satellite pixel and in situ footprint. We used digital imagery acquired by an unmanned aerial vehicle to evaluate point-to-pixel albedo comparisons across the western, ablating margin of the Greenland Ice Sheet. Our results reveal that in situ measurements overestimate albedo by up to 0.10 at the end of the melt season because the ground footprints of AWS-mounted pyranometers are insufficient to capture the spatial heterogeneity of the ice surface as it progressively ablates and darkens. Statistical analysis of 21 AWS across the entire Greenland Ice Sheet reveals that almost half suffer from this bias, including some AWS located within the wet snow zone.

  15. Ice sheets play important role in climate change

    NASA Astrophysics Data System (ADS)

    Clark, Peter U.; MacAyeal, Douglas R.; Andrews, John T.; Bartlein, Patrick J.

    Ice sheets once were viewed as passive elements in the climate system enslaved to orbitally generated variations in solar radiation. Today, modeling results and new geologic records suggest that ice 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 ice volume were ultimately caused by orbital variations (the Milankovitch hypothesis), once in existence, the former ice 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 ice sheets' climatic significance. Manabe and Broccoli [1985], for example, found that the topographic and albedo effects of ice sheets alone explain much of the Northern Hemisphere cooling identified in paleoclimatic records of the last glacial maximum (˜21 ka).

  16. Snow Climatology of Arctic Sea Ice: Comparison of Reanalysis and Climate Model Data with In Situ Measurements

    NASA Astrophysics Data System (ADS)

    Chevooruvalappil Chandran, B.; Pittana, M.; Haas, C.

    2015-12-01

    Snow on sea ice is a critical and complex factor influencing sea ice processes. Deep snow with a high albedo and low thermal conductivity inhibits ice growth in winter and minimizes ice loss in summer. Very shallow or absent snow promotes ice growth in winter and ice loss in summer. The timing of snow ablation critically impacts summer sea ice mass balance. Here we assess the accuracy of various snow on sea ice data products from reanalysis and modeling comparing them with in situ measurements. The latter are based on the Warren et al. (1999) monthly climatology derived from snow ruler measurements between 1954-1991, and on daily snow depth retrievals from few drifting ice mass balance buoys (IMB) with sufficiently long observations spanning the summer season. These were compared with snow depth data from the National Center for Environmental Prediction Department of Energy Reanalysis 2 (NCEP), the Community Climate System Model 4 (CCSM4), and the Canadian Earth System Model 2 (CanESM2). Results are quite variable in different years and regions. However, there is often good agreement between CanESM2 and IMB snow depth during the winter accumulation and spring melt periods. Regional analyses show that over the western Arctic covered primarily with multiyear ice NCEP snow depths are in good agreement with the Warren climatology while CCSM4 overestimates snow depth. However, in the Eastern Arctic which is dominated by first-year ice the opposite behavior is observed. Compared to the Warren climatology CanESM2 underestimates snow depth in all regions. Differences between different snow depth products are as large as 10 to 20 cm, with large consequences for the sea ice mass balance. However, it is also very difficult to evaluate the accuracy of reanalysis and model snow depths due to a lack of extensive, continuous in situ measurements.

  17. Interhemispheric ice-sheet synchronicity during the Last Glacial Maximum

    NASA Astrophysics Data System (ADS)

    Weber, M. E.; Clark, P. U.; Ricken, W.; Mitrovica, J. X.; Hostetler, S. W.; Kuhn, G.

    2012-04-01

    The timing of the last maximum extent of the Antarctic ice sheets relative to those in the Northern Hemisphere remains poorly understood because only a few findings with robust chronologies exist for Antarctic ice sheets. We developed a chronology for the Weddell Sea sector of the East Antarctic ice sheet that, combined with ages from other Antarctic ice-sheet sectors, indicates the advance to their maximum extent at 29 -28 ka, and retreat from their maximum extent at 19 ka was nearly synchronous with Northern Hemisphere ice sheets (Weber, M.E., Clark, P. U., Ricken, W., Mitrovica, J. X., Hostetler, S. W., and Kuhn, G. (2011): Interhemispheric ice-sheet synchronicity during the Last Glacial Maximum. - Science, 334, 1265-1269, doi: 10.1126:science.1209299). As for the deglaciation, modeling studies suggest a late ice-sheet retreat starting around 14 ka BP and ending around 7 ka BP with a large impact of an unstable West Antarctic Ice Sheet (WAIS) and a small impact of a stable East Antarctic Ice Sheet (EAIS). However, the Weddell Sea sites studied here, as well as sites from the Scotia Sea, provide evidence that specifically the EAIS responded much earlier, possibly provided a significant contribution to the last sea-level rise, and was much more dynamic than previously thought. Using the results of an atmospheric general circulation we conclude that surface climate forcing of Antarctic ice mass balance would likely cause an opposite response, whereby a warming climate would increase accumulation but not surface melting. Furthermore, our new data support teleconnections involving a sea-level fingerprint forced from Northern Hemisphere ice sheets as indicated by gravitational modeling. Also, changes in North Atlantic Deepwater formation and attendant heat flux to Antarctic grounding lines may have contributed to synchronizing the hemispheric ice sheets.

  18. Dirty snow after nuclear war

    NASA Technical Reports Server (NTRS)

    Warren, S. G.; Wiscombe, W. J.

    1985-01-01

    It is shown that smoke from fires started by nuclear explosions could continue to cause significant disruption even after it has fallen from the atmosphere, by lowering the reflectivity of snow and sea ice surfaces, with possible effects on climate in northern latitudes caused by enhanced absorption of sunlight. The reduced reflectivity could persist for several years on Arctic sea ice and on the ablation area of the Greenland ice sheet.

  19. The Potsdam Parallel Ice Sheet Model (PISM-PIK) - Part 2: Dynamic equilibrium simulation of the Antarctic ice sheet

    NASA Astrophysics Data System (ADS)

    Martin, M. A.; Winkelmann, R.; Haseloff, M.; Albrecht, T.; Bueler, E.; Khroulev, C.; Levermann, A.

    2011-09-01

    We present a dynamic equilibrium simulation of the ice sheet-shelf system on Antarctica with the Potsdam Parallel Ice Sheet Model (PISM-PIK). The simulation is initialized with present-day conditions for bed topography and ice thickness and then run to steady state with constant present-day surface mass balance. Surface temperature and sub-shelf basal melt distribution are parameterized. Grounding lines and calving fronts are free to evolve, and their modeled equilibrium state is compared to observational data. A physically-motivated calving law based on horizontal spreading rates allows for realistic calving fronts for various types of shelves. Steady-state dynamics including surface velocity and ice flux are analyzed for whole Antarctica and the Ronne-Filchner and Ross ice shelf areas in particular. The results show that the different flow regimes in sheet and shelves, and the transition zone between them, are captured reasonably well, supporting the approach of superposition of SIA and SSA for the representation of fast motion of grounded ice. This approach also leads to a natural emergence of sliding-dominated flow in stream-like features in this new 3-D marine ice sheet model.

  20. Greenland ice sheet motion insensitive to exceptional meltwater forcing.

    PubMed

    Tedstone, Andrew J; Nienow, Peter W; Sole, Andrew J; Mair, Douglas W F; Cowton, Thomas R; Bartholomew, Ian D; King, Matt A

    2013-12-03

    Changes to the dynamics of the Greenland ice sheet can be forced by various mechanisms including surface-melt-induced ice acceleration and oceanic forcing of marine-terminating glaciers. We use observations of ice motion to examine the surface melt-induced dynamic response of a land-terminating outlet glacier in southwest Greenland to the exceptional melting observed in 2012. During summer, meltwater generated on the Greenland ice sheet surface accesses the ice sheet bed, lubricating basal motion and resulting in periods of faster ice flow. However, the net impact of varying meltwater volumes upon seasonal and annual ice flow, and thus sea level rise, remains unclear. We show that two extreme melt events (98.6% of the Greenland ice sheet surface experienced melting on July 12, the most significant melt event since 1889, and 79.2% on July 29) and summer ice sheet runoff ~3.9 σ above the 1958-2011 mean resulted in enhanced summer ice motion relative to the average melt year of 2009. However, despite record summer melting, subsequent reduced winter ice motion resulted in 6% less net annual ice motion in 2012 than in 2009. Our findings suggest that surface melt-induced acceleration of land-terminating regions of the ice sheet will remain insignificant even under extreme melting scenarios.

  1. 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 <span class="hlt">snow</span> in sea <span class="hlt">ice</span> mass 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 <span class="hlt">snow</span> cover is turned into <span class="hlt">ice</span>. The latter is largely a consequence of high mass of <span class="hlt">snow</span> 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 <span class="hlt">snow</span> 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 <span class="hlt">snow</span> 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/2016APS..DFDR13007H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..DFDR13007H"><span><span class="hlt">Ice</span> <span class="hlt">sheets</span> on plastically-yielding beds</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hewitt, Ian</p> <p>2016-11-01</p> <p>Many fast flowing regions of <span class="hlt">ice</span> <span class="hlt">sheets</span> are underlain by a layer of water-saturated sediments, or till. The rheology of the till has been the subject of some controversy, with laboratory tests suggesting almost perfectly plastic behaviour (stress independent of strain rate), but many models adopting a pseudo-viscous description. In this work, we consider the behaviour of glaciers underlain by a plastic bed. The <span class="hlt">ice</span> is treated as a viscous gravity current, on a bed that allows unconstrained slip above a critical yield stress. This simplified description allows rapid sliding, and aims to investigate 'worst-case' scenarios of possible <span class="hlt">ice-sheet</span> disintegration. The plastic bed results in an approximate <span class="hlt">ice-sheet</span> geometry that is primarily controlled by force balance, whilst <span class="hlt">ice</span> velocity is determined from mass conservation (rather than the other way around, as standard models would hold). The stability of various states is considered, and particular attention is given to the pace at which transitions between unstable states can occur. Finally, we observe that the strength of basal tills depends strongly on pore pressure, and combine the model with a description of subglacial hydrology. Implications for the present-day <span class="hlt">ice</span> <span class="hlt">sheets</span> in Greenland and Antarctica will be discussed. Funding: ERC Marie Curie FP7 Career Integration Grant.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://dx.doi.org/10.1126/science.1209299','USGSPUBS'); return false;" href="http://dx.doi.org/10.1126/science.1209299"><span>Interhemispheric <span class="hlt">ice-sheet</span> synchronicity during the last glacial maximum</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Weber, Michael E.; Clark, Peter U.; Ricken, Werner; Mitrovica, Jerry X.; Hostetler, Steven W.; Kuhn, Gerhard</p> <p>2011-01-01</p> <p>The timing of the last maximum extent of the Antarctic <span class="hlt">ice</span> <span class="hlt">sheets</span> relative to those in the Northern Hemisphere remains poorly understood. We develop a chronology for the Weddell Sea sector of the East Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> that, combined with ages from other Antarctic <span class="hlt">ice-sheet</span> sectors, indicates that the advance to and retreat from their maximum extent was within dating uncertainties synchronous with most sectors of Northern Hemisphere <span class="hlt">ice</span> <span class="hlt">sheets</span>. Surface climate forcing of Antarctic mass balance would probably cause an opposite response, whereby a warming climate would increase accumulation but not surface melting. Our new data support teleconnections involving sea-level forcing from Northern Hemisphere <span class="hlt">ice</span> <span class="hlt">sheets</span> and changes in North Atlantic deep-water formation and attendant heat flux to Antarctic grounding lines to synchronize the hemispheric <span class="hlt">ice</span> <span class="hlt">sheets</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22144623','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22144623"><span>Interhemispheric <span class="hlt">ice-sheet</span> synchronicity during the Last Glacial Maximum.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Weber, Michael E; Clark, Peter U; Ricken, Werner; Mitrovica, Jerry X; Hostetler, Steven W; Kuhn, Gerhard</p> <p>2011-12-02</p> <p>The timing of the last maximum extent of the Antarctic <span class="hlt">ice</span> <span class="hlt">sheets</span> relative to those in the Northern Hemisphere remains poorly understood. We develop a chronology for the Weddell Sea sector of the East Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> that, combined with ages from other Antarctic <span class="hlt">ice-sheet</span> sectors, indicates that the advance to and retreat from their maximum extent was within dating uncertainties synchronous with most sectors of Northern Hemisphere <span class="hlt">ice</span> <span class="hlt">sheets</span>. Surface climate forcing of Antarctic mass balance would probably cause an opposite response, whereby a warming climate would increase accumulation but not surface melting. Our new data support teleconnections involving sea-level forcing from Northern Hemisphere <span class="hlt">ice</span> <span class="hlt">sheets</span> and changes in North Atlantic deep-water formation and attendant heat flux to Antarctic grounding lines to synchronize the hemispheric <span class="hlt">ice</span> <span class="hlt">sheets</span>.</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> <span class="hlt">sheet</span> 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> <span class="hlt">sheet</span> deglaciation are critical to our understanding of glacial-interglacial cycles and <span class="hlt">ice</span> <span class="hlt">sheet</span> sensitivity to climate change. The precise mechanisms of deglaciation are also relevant to our understanding of modern-day <span class="hlt">ice</span> <span class="hlt">sheet</span> stability and concerns over global sea level rise. Mass loss from <span class="hlt">ice</span> <span class="hlt">sheets</span> 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> <span class="hlt">sheet</span> mass 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-sheet</span> 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 mass 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> <span class="hlt">Sheet</span> 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('http://hdl.handle.net/2060/20140011040','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140011040"><span><span class="hlt">Snow</span> Dunes: A Controlling Factor of Melt Pond Distribution on Arctic Sea <span class="hlt">Ice</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Petrich, Chris; Eicken, Hajo; Polashenski, Christopher M.; Sturm, Matthew; Harbeck, Jeremy P.; Perovich, Donald K.; Finnegan, David C.</p> <p>2012-01-01</p> <p>The location of <span class="hlt">snow</span> dunes over the course of the <span class="hlt">ice</span>-growth season 2007/08 was mapped on level landfast first-year sea <span class="hlt">ice</span> near Barrow, Alaska. Landfast <span class="hlt">ice</span> formed in mid-December and exhibited essentially homogeneous <span class="hlt">snow</span> depths of 4-6 cm in mid-January; by early February distinct <span class="hlt">snow</span> dunes were observed. Despite additional snowfall and wind redistribution throughout the season, the location of the dunes was fixed by March, and these locations were highly correlated with the distribution of meltwater ponds at the beginning of June. Our observations, including ground-based light detection and ranging system (lidar) measurements, show that melt ponds initially form in the interstices between <span class="hlt">snow</span> dunes, and that the outline of the melt ponds is controlled by <span class="hlt">snow</span> depth contours. The resulting preferential surface ablation of ponded <span class="hlt">ice</span> creates the surface topography that later determines the melt pond evolution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010E%26PSL.291..138B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010E%26PSL.291..138B"><span>Multiple sources supply eolian mineral dust to the Atlantic sector of coastal Antarctica: Evidence from recent <span class="hlt">snow</span> layers at the top of Berkner Island <span class="hlt">ice</span> <span class="hlt">sheet</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bory, Aloys; Wolff, Eric; Mulvaney, Robert; Jagoutz, Emil; Wegner, Anna; Ruth, Urs; Elderfield, Harry</p> <p>2010-03-01</p> <p>The Sr and Nd isotopic composition of dust extracted from recent <span class="hlt">snow</span> layers at the top of Berkner Island <span class="hlt">ice</span> <span class="hlt">sheet</span> (located within the Filchner-Ronne <span class="hlt">Ice</span> Shelf at the southern end of the Weddell Sea) enables us, for the first time, to document dust provenance in Antarctica outside the East Antarctic Plateau (EAP) where all previous studies based on isotopic fingerprinting were carried out. Berkner dust displays an overall crust-like isotopic signature, characterized by more radiogenic 87Sr/ 86Sr and much less radiogenic 143Nd/ 144Nd compared to dust deposited on the EAP during glacial periods. Differences with EAP interglacial dust are not as marked but still significant, indicating that present-day Berkner dust provenance is distinct, at least to some extent, from that of the dust reaching the EAP. The fourteen <span class="hlt">snow</span>-pit sub-seasonal samples that were obtained span a two-year period (2002-2003) and their dust Sr and Nd isotopic composition reveals that multiple sources are at play over a yearly time period. Southern South America, Patagonia in particular, likely accounts for part of the observed spring/summer dust deposition maxima, when isotopic composition is shifted towards "younger" isotopic signatures. In the spring, possible additional inputs from Australian sources would also be supported by the data. Most of the year, however, the measured isotopic signatures would be best explained by a sustained background supply from putative local sources in East Antarctica, which carry old-crust-like isotopic fingerprints. Whether the restricted East Antarctic <span class="hlt">ice</span>-free areas produce sufficient eolian material has yet to be substantiated however. The fact that large (> 5 μm) particles represent a significant fraction of the samples throughout the entire time-series supports scenarios that involve contributions from proximal sources, either in Patagonia and/or Antarctica (possibly including <span class="hlt">snow</span>-free areas in the Antarctic Peninsula and other areas as well). This also</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70035675','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70035675"><span>Sensitivity of Pliocene <span class="hlt">ice</span> <span class="hlt">sheets</span> to orbital forcing</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Dolan, A.M.; Haywood, A.M.; Hill, D.J.; Dowsett, H.J.; Hunter, S.J.; Lunt, D.J.; Pickering, S.J.</p> <p>2011-01-01</p> <p>The stability of the Earth's major <span class="hlt">ice</span> <span class="hlt">sheets</span> is a critical uncertainty in predictions of future climate and sea level change. One method of investigating the behaviour of the Greenland and the Antarctic <span class="hlt">ice</span> <span class="hlt">sheets</span> in a warmer-than-modern climate is to look back at past warm periods of Earth history, for example the Pliocene. This paper presents climate and <span class="hlt">ice</span> <span class="hlt">sheet</span> modelling results for the mid-Pliocene warm period (mPWP; 3.3 to 3.0 million years ago), which has been identified as a key interval for understanding warmer-than-modern climates (Jansen et al., 2007). Using boundary conditions supplied by the United States Geological Survey PRISM Group (Pliocene Research, Interpretation and Synoptic Mapping), the Hadley Centre coupled ocean–atmosphere climate model (HadCM3) and the British Antarctic Survey <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model (BASISM), we show large reductions in the Greenland and East Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheets</span> (GrIS and EAIS) compared to modern in standard mPWP experiments. We also present the first results illustrating the variability of the <span class="hlt">ice</span> <span class="hlt">sheets</span> due to realistic orbital forcing during the mid-Pliocene. While GrIS volumes are lower than modern under even the most extreme (cold) mid-Pliocene orbit (losing at least 35% of its <span class="hlt">ice</span> mass), the EAIS can both grow and shrink, losing up to 20% or gaining up to 10% of its present-day volume. The changes in <span class="hlt">ice</span> <span class="hlt">sheet</span> volume incurred by altering orbital forcing alone means that global sea level can vary by more than 25 m during the mid-Pliocene. However, we have also shown that the response of the <span class="hlt">ice</span> <span class="hlt">sheets</span> to mPWP orbital hemispheric forcing can be in anti-phase, whereby the greatest reductions in EAIS volume are concurrent with the smallest reductions of the GrIS. If this anti-phase relationship is in operation throughout the mPWP, then the total eustatic sea level response would be dampened compared to the <span class="hlt">ice</span> <span class="hlt">sheet</span> fluctuations that are theoretically possible. This suggests that maximum eustatic sea level rise does not</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013GMD.....6.1299G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013GMD.....6.1299G"><span>Capabilities and performance of Elmer/<span class="hlt">Ice</span>, a new-generation <span class="hlt">ice</span> <span class="hlt">sheet</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>Gagliardini, O.; Zwinger, T.; Gillet-Chaulet, F.; Durand, G.; Favier, L.; de Fleurian, B.; Greve, R.; Malinen, M.; Martín, C.; Råback, P.; Ruokolainen, J.; Sacchettini, M.; Schäfer, M.; Seddik, H.; Thies, J.</p> <p>2013-08-01</p> <p>The Fourth IPCC Assessment Report concluded that <span class="hlt">ice</span> <span class="hlt">sheet</span> flow models, in their current state, were unable to provide accurate forecast for the increase of polar <span class="hlt">ice</span> <span class="hlt">sheet</span> discharge and the associated contribution to sea level rise. Since then, the glaciological community has undertaken a huge effort to develop and improve a new generation of <span class="hlt">ice</span> flow models, and as a result a significant number of new <span class="hlt">ice</span> <span class="hlt">sheet</span> models have emerged. Among them is the parallel finite-element model Elmer/<span class="hlt">Ice</span>, based on the open-source multi-physics code Elmer. It was one of the first full-Stokes models used to make projections for the evolution of the whole Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> for the coming two centuries. Originally developed to solve local <span class="hlt">ice</span> flow problems of high mechanical and physical complexity, Elmer/<span class="hlt">Ice</span> has today reached the maturity to solve larger-scale problems, earning the status of an <span class="hlt">ice</span> <span class="hlt">sheet</span> model. Here, we summarise almost 10 yr of development performed by different groups. Elmer/<span class="hlt">Ice</span> solves the full-Stokes equations, for isotropic but also anisotropic <span class="hlt">ice</span> rheology, resolves the grounding line dynamics as a contact problem, and contains various basal friction laws. Derived fields, like the age of the <span class="hlt">ice</span>, the strain rate or stress, can also be computed. Elmer/<span class="hlt">Ice</span> includes two recently proposed inverse methods to infer badly known parameters. Elmer is a highly parallelised code thanks to recent developments and the implementation of a block preconditioned solver for the Stokes system. In this paper, all these components are presented in detail, as well as the numerical performance of the Stokes solver and developments planned for the future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.C41A0504B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.C41A0504B"><span>Managing <span class="hlt">Ice</span>Bridge Airborne Mission Data at the National <span class="hlt">Snow</span> and <span class="hlt">Ice</span> Data Center</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brodzik, M.; Kaminski, M. L.; Deems, J. S.; Scambos, T. A.</p> <p>2010-12-01</p> <p> a map-based interface. This portal will provide flight line rendering and multi-instrument data previewing capabilities to facilitate use of the wide array of data types, resolutions, and configurations in this dynamic airborne mission. Together with the <span class="hlt">Ice</span>Bridge Science Team and <span class="hlt">Ice</span> Bridge Science Working Groups, NSIDC is generating value-added products from the <span class="hlt">Ice</span> Bridge data streams and other ancillary data. These products will provide simple, useful combinations of <span class="hlt">Ice</span> Bridge products and regional maps of important geophysical parameters from other sources. Planned value-added products include: (1) gridded products in which new profiles from <span class="hlt">Ice</span> Bridge (e.g. elevation or <span class="hlt">ice</span> thickness) are combined with existing DEMs or bed maps to produce revised grids and (2) flight-profile multi-instrument products in which data from several instruments are combined into <span class="hlt">ice</span> <span class="hlt">sheet</span> profiles (surface elevation, <span class="hlt">ice</span> thickness, internal reflection data, bed reflection intensity, and gravimetry), sea <span class="hlt">ice</span> profiles (freeboard, <span class="hlt">snow</span> cover, and thickness), and surface data profiles (elevation, slope, roughness, near-surface layering, and imagery).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1239510-sph-non-newtonian-model-ice-sheet-ice-shelf-dynamics','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1239510-sph-non-newtonian-model-ice-sheet-ice-shelf-dynamics"><span>SPH non-Newtonian Model for <span class="hlt">Ice</span> <span class="hlt">Sheet</span> and <span class="hlt">Ice</span> Shelf Dynamics</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>Tartakovsky, Alexandre M.; Pan, Wenxiao; Monaghan, Joseph J.</p> <p>2012-07-07</p> <p>We propose a new three-dimensional smoothed particle hydrodynamics (SPH) non-Newtonian model to study coupled <span class="hlt">ice</span> <span class="hlt">sheet</span> and <span class="hlt">ice</span> shelf dynamics. Most existing <span class="hlt">ice</span> <span class="hlt">sheet</span> numerical models use a grid-based Eulerian approach, and are usually restricted to shallow <span class="hlt">ice</span> <span class="hlt">sheet</span> and <span class="hlt">ice</span> shelf approximations of the momentum conservation equation. SPH, a fully Lagrangian particle method, solves the full momentum conservation equation. SPH method also allows modeling of free-surface flows, large material deformation, and material fragmentation without employing complex front-tracking schemes, and does not require re-meshing. As a result, SPH codes are highly scalable. Numerical accuracy of the proposed SPH model ismore » first verified by simulating a plane shear flow with a free surface and the propagation of a blob of <span class="hlt">ice</span> along a horizontal surface. Next, the SPH model is used to investigate the grounding line dynamics of <span class="hlt">ice</span> <span class="hlt">sheet</span>/shelf. The steady position of the grounding line, obtained from our SPH simulations, is in good agreement with laboratory observations for a wide range of bedrock slopes, <span class="hlt">ice</span>-to-fluid density ratios, and flux. We examine the effect of non-Newtonian behavior of <span class="hlt">ice</span> on the grounding line dynamics. The non-Newtonian constitutive model is based on Glen's law for a creeping flow of a polycrystalline <span class="hlt">ice</span>. Finally, we investigate the effect of a bedrock geometry on a steady-state position of the grounding line.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20170007832&hterms=sensors&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dsensors','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20170007832&hterms=sensors&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dsensors"><span>Impact of MODIS Sensor Calibration Updates on Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Surface Reflectance and Albedo Trends</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Casey, Kimberly A.; Polashenski, Chris M.; Chen, Justin; Tedesco, Marco</p> <p>2017-01-01</p> <p>We evaluate Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (GrIS) surface reflectance and albedo trends using the newly released Collection 6 (C6) MODIS (Moderate Resolution Imaging Spectroradiometer) products over the period 2001-2016. We find that the correction of MODIS sensor degradation provided in the new C6 data products reduces the magnitude of the surface reflectance and albedo decline trends obtained from previous MODIS data (i.e., Collection 5, C5). Collection 5 and 6 data product analysis over GrIS is characterized by surface (i.e., wet vs. dry) and elevation (i.e., 500-2000 m, 2000 m and greater) conditions over the summer season from 1 June to 31 August. Notably, the visible-wavelength declining reflectance trends identified in several bands of MODIS C5 data from previous studies are only slightly detected at reduced magnitude in the C6 versions over the dry <span class="hlt">snow</span> area. Declining albedo in the wet <span class="hlt">snow</span> and <span class="hlt">ice</span> area remains over the MODIS record in the C6 product, albeit at a lower magnitude than obtained using C5 data. Further analyses of C6 spectral reflectance trends show both reflectance increases and decreases in select bands and regions, suggesting that several competing processes are contributing to Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> albedo change. Investigators using MODIS data for other ocean, atmosphere and/or land analyses are urged to consider similar re-examinations of trends previously established using C5 data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C51A0947C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C51A0947C"><span><span class="hlt">Ice-sheet</span> thinning and acceleration at Camp Century, Greenlan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Colgan, W. T.</p> <p>2017-12-01</p> <p>Camp Century, Greenland (77.18 °N, 61.12 °W, 1900 m), is located approximately 150 km inland from the <span class="hlt">ice-sheet</span> margin in Northwest Greenland. In-situ and remotely-sensed measurements of <span class="hlt">ice-sheet</span> elevation at Camp Century exhibit a thinning trend between 1964 and the present. A comparison of 1966 and 2017 firn density profiles indicates that a portion of this <span class="hlt">ice-sheet</span> thinning is attributable to increased firn compaction rate. In-situ measurements of increasing <span class="hlt">ice</span> surface velocity over the 1977-2017 period indicate that enhanced horizontal divergence of <span class="hlt">ice</span> flux is also contributing to <span class="hlt">ice</span> dynamic thinning at Camp Century. This apparent <span class="hlt">ice</span> dynamic thinning could potentially result from a migrating local flow divide or decreasing effective <span class="hlt">ice</span> viscosity. In a shorter-term context, observations of decadal-scale <span class="hlt">ice-sheet</span> thinning and acceleration at Camp Century highlights underappreciated transience in inland <span class="hlt">ice</span> form and flow during the satellite era. In a longer-term context, these multi-decadal observations contrast with inferences of millennial-scale <span class="hlt">ice-sheet</span> thickening and deceleration at Camp Century.</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> <span class="hlt">sheet</span> 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> <span class="hlt">sheet</span> 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> <span class="hlt">sheets</span> had melted and that the evidence for the time of original growth of these <span class="hlt">ice</span> masses 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> <span class="hlt">sheets</span> 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> <span class="hlt">sheet</span>. If the present-day <span class="hlt">ice</span> masses began their growth during the last interglacial, the <span class="hlt">ice</span> <span class="hlt">sheet</span> 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> <span class="hlt">sheet</span>, as has been suggested.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19980017810','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19980017810"><span>Measuring Geophysical Parameters of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> using Airborne Radar Altimetry</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ferraro, Ellen J.; Swift. Calvin T.</p> <p>1995-01-01</p> <p>This paper presents radar-altimeter scattering models for each of the diagenetic zones of the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span>. AAFE radar- altimeter waveforms obtained during the 1991 and 1993 NASA multi-sensor airborne altimetry experiments over Greenland reveal that the Ku-band return pulse changes significantly with the different diagenetic zones. These changes are due to varying amounts of surface and volume scattering in the return waveform. In the ablation and soaked zones, where surface scattering dominates the AAFE return, geophysical parameters such as rms surface height and rms surface slope are obtained by fitting the waveforms to a surface-scattering model. Waveforms from the percolation zone show that the sub-surface <span class="hlt">ice</span> features have a much more significant effect on the return pulse than the surrounding snowpack. Model percolation waveforms, created using a combined surface- and volume-scattering model and an <span class="hlt">ice</span>-feature distribution obtained during the 1993 field season, agree well with actual AAFE waveforms taken in the same time period. Using a combined surface- and volume-scattering model for the dry-<span class="hlt">snow</span>-zone return waveforms, the rms surface height and slope and the attenuation coefficient of the snowpack are obtained. These scattering models not only allow geophysical parameters of the <span class="hlt">ice</span> <span class="hlt">sheet</span> to be measured but also help in the understanding of satellite radar-altimeter data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA....13008H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA....13008H"><span>Glaciological constraints on current <span class="hlt">ice</span> mass changes from modelling the <span class="hlt">ice</span> <span class="hlt">sheets</span> over the glacial cycles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huybrechts, P.</p> <p>2003-04-01</p> <p>The evolution of continental <span class="hlt">ice</span> <span class="hlt">sheets</span> introduces a long time scale in the climate system. Large <span class="hlt">ice</span> <span class="hlt">sheets</span> have a memory of millenia, hence the present-day <span class="hlt">ice</span> <span class="hlt">sheets</span> 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 <span class="hlt">ice</span> mass changes is to model the past history of the <span class="hlt">ice</span> <span class="hlt">sheets</span> and their underlying beds over the glacial cycles. Such calculations assist to distinguish between the longer-term <span class="hlt">ice</span>-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 <span class="hlt">ice-sheet</span>/lithosphere/bedrock models applied to the Antarctic and Greenland <span class="hlt">ice</span> <span class="hlt">sheets</span>. The simulations are forced by time-dependent boundary conditions derived from sediment and <span class="hlt">ice</span> core records and are constrained by geomorphological and glacial-geological data of past <span class="hlt">ice</span> <span class="hlt">sheet</span> and sea-level stands. Current simulations suggest that the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> is close to balance, while the Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> is still losing mass, mainly due to incomplete grounding-line retreat of the West Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> since the LGM. The results indicate that altimetry trends are likely dominated by <span class="hlt">ice</span> thickness changes but that the gravitational signal mainly reflects postglacial rebound.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20090038693','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20090038693"><span>Estimation of Sea <span class="hlt">Ice</span> Thickness Distributions through the Combination of <span class="hlt">Snow</span> Depth and Satellite Laser Altimetry Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kurtz, Nathan T.; Markus, Thorsten; Cavalieri, Donald J.; Sparling, Lynn C.; Krabill, William B.; Gasiewski, Albin J.; Sonntag, John G.</p> <p>2009-01-01</p> <p>Combinations of sea <span class="hlt">ice</span> freeboard and <span class="hlt">snow</span> depth measurements from satellite data have the potential to provide a means to derive global sea <span class="hlt">ice</span> thickness values. However, large differences in spatial coverage and resolution between the measurements lead to uncertainties when combining the data. High resolution airborne laser altimeter retrievals of <span class="hlt">snow-ice</span> freeboard and passive microwave retrievals of <span class="hlt">snow</span> depth taken in March 2006 provide insight into the spatial variability of these quantities as well as optimal methods for combining high resolution satellite altimeter measurements with low resolution <span class="hlt">snow</span> depth data. The aircraft measurements show a relationship between freeboard and <span class="hlt">snow</span> depth for thin <span class="hlt">ice</span> allowing the development of a method for estimating sea <span class="hlt">ice</span> thickness from satellite laser altimetry data at their full spatial resolution. This method is used to estimate <span class="hlt">snow</span> and <span class="hlt">ice</span> thicknesses for the Arctic basin through the combination of freeboard data from ICESat, <span class="hlt">snow</span> depth data over first-year <span class="hlt">ice</span> from AMSR-E, and <span class="hlt">snow</span> depth over multiyear <span class="hlt">ice</span> from climatological data. Due to the non-linear dependence of heat flux on <span class="hlt">ice</span> thickness, the impact on heat flux calculations when maintaining the full resolution of the ICESat data for <span class="hlt">ice</span> thickness estimates is explored for typical winter conditions. Calculations of the basin-wide mean heat flux and <span class="hlt">ice</span> growth rate using <span class="hlt">snow</span> and <span class="hlt">ice</span> thickness values at the 70 m spatial resolution of ICESat are found to be approximately one-third higher than those calculated from 25 km mean <span class="hlt">ice</span> thickness values.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C41C1235L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C41C1235L"><span>Sensitivity of an Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model to Sub-<span class="hlt">Ice</span>-Shelf Melting</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lipscomb, W. H.; Leguy, G.; Urban, N. M.; Berdahl, M.</p> <p>2017-12-01</p> <p>Theory and observations suggest that marine-based sectors of the Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> could retreat rapidly under ocean warming and increased melting beneath <span class="hlt">ice</span> shelves. Numerical models of marine <span class="hlt">ice</span> <span class="hlt">sheets</span> vary widely in sensitivity, depending on grid resolution and the parameterization of key processes (e.g., calving and hydrofracture). Here we study the sensitivity of the Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> to ocean warming and sub-shelf melting in standalone simulations of the Community <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model (CISM). Melt rates either are prescribed based on observations and high-resolution ocean model output, or are derived from a plume model forced by idealized ocean temperature profiles. In CISM, we vary the model resolution (between 1 and 8 km), Stokes approximation (shallow-shelf, depth-integrated higher-order, or 3D higher-order) and calving scheme to create an ensemble of plausible responses to sub-shelf melting. This work supports a broader goal of building statistical and reduced models that can translate large-scale Earth-system model projections to changes in Antarctic ocean temperatures and <span class="hlt">ice</span> <span class="hlt">sheet</span> discharge, thus better quantifying uncertainty in Antarctic-sourced sea-level rise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19278447','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19278447"><span>Bacteria beneath the West Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lanoil, Brian; Skidmore, Mark; Priscu, John C; Han, Sukkyun; Foo, Wilson; Vogel, Stefan W; Tulaczyk, Slawek; Engelhardt, Hermann</p> <p>2009-03-01</p> <p>Subglacial environments, particularly those that lie beneath polar <span class="hlt">ice</span> <span class="hlt">sheets</span>, are beginning to be recognized as an important part of Earth's biosphere. However, except for indirect indications of microbial assemblages in subglacial Lake Vostok, Antarctica, no sub-<span class="hlt">ice</span> <span class="hlt">sheet</span> environments have been shown to support microbial ecosystems. Here we report 16S rRNA gene and isolate diversity in sediments collected from beneath the Kamb <span class="hlt">Ice</span> Stream, West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> and stored for 15 months at 4 degrees C. This is the first report of microbes in samples from the sediment environment beneath the Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span>. The cells were abundant ( approximately 10(7) cells g(-1)) but displayed low diversity (only five phylotypes), likely as a result of enrichment during storage. Isolates were cold tolerant and the 16S rRNA gene diversity was a simplified version of that found in subglacial alpine and Arctic sediments and water. Although in situ cell abundance and the extent of wet sediments beneath the Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> can only be roughly extrapolated on the basis of this sample, it is clear that the subglacial ecosystem contains a significant and previously unrecognized pool of microbial cells and associated organic carbon that could potentially have significant implications for global geochemical processes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('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> <span class="hlt">sheet</span> oscillations.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Naish, T; Powell, R; Levy, R; Wilson, G; Scherer, R; Talarico, F; Krissek, L; Niessen, F; Pompilio, M; Wilson, T; Carter, L; DeConto, R; Huybers, P; McKay, R; Pollard, D; Ross, J; Winter, D; Barrett, P; Browne, G; Cody, R; Cowan, E; Crampton, J; Dunbar, G; Dunbar, N; Florindo, F; Gebhardt, C; Graham, I; Hannah, M; Hansaraj, D; Harwood, D; Helling, D; Henrys, S; Hinnov, L; Kuhn, G; Kyle, P; Läufer, A; Maffioli, P; Magens, D; Mandernack, K; McIntosh, W; Millan, C; Morin, R; Ohneiser, C; Paulsen, T; Persico, D; Raine, I; Reed, J; Riesselman, C; Sagnotti, L; Schmitt, D; Sjunneskog, C; Strong, P; Taviani, M; Vogel, S; Wilch, T; Williams, T</p> <p>2009-03-19</p> <p>Thirty years after oxygen isotope records from microfossils deposited in ocean sediments confirmed the hypothesis that variations in the Earth's orbital geometry control the <span class="hlt">ice</span> ages, fundamental questions remain over the response of the Antarctic <span class="hlt">ice</span> <span class="hlt">sheets</span> to orbital cycles. Furthermore, an understanding of the behaviour of the marine-based West Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> (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-sheet</span> behaviour in the context of future global warming. Here we present a marine glacial record from the upper 600 m of the AND-1B sediment core recovered from beneath the northwest part of the Ross <span class="hlt">ice</span> shelf by the ANDRILL programme and demonstrate well-dated, approximately 40-kyr cyclic variations in <span class="hlt">ice-sheet</span> 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> <span class="hlt">sheet</span>, 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> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_12 --> <div id="page_13" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="241"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16782607','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16782607"><span><span class="hlt">Ice-sheet</span> 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-sheet</span> surface mass balance requires higher spatial resolution than is afforded by typical atmosphere-ocean general circulation models (AOGCMs), owing, in particular, to the need to resolve the narrow and steep margins where the majority of precipitation and ablation occurs. We have developed a method for calculating mass-balance changes by combining <span class="hlt">ice-sheet</span> 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-sheet</span> mass-balance model. Antarctica contributes negatively to sea level on account of increased accumulation, while Greenland contributes positively because ablation increases more rapidly. The uncertainty in the results is about 20% for Antarctica and 35% for Greenland. Changes in <span class="hlt">ice-sheet</span> topography and dynamics are not included, but we discuss their possible effects. For an annual- and area-average warming exceeding 4.5+/-0.9K in Greenland and 3.1+/-0.8K in the global average, the net surface mass balance of the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> becomes negative, in which case it is likely that the <span class="hlt">ice</span> <span class="hlt">sheet</span> 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.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> <span class="hlt">Sheet</span></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>Mass loss from the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> now exceeds 260 Gt/year, raising global sea level by >0.7 mm annually. Approximately two-thirds of this total mass loss is now driven by negative <span class="hlt">ice</span> <span class="hlt">sheet</span> surface mass balance (SMB), attributed mainly to production and runoff of meltwater from the <span class="hlt">ice</span> <span class="hlt">sheet</span> surface. This new dominance of runoff as a driver of GrIS total mass loss will likely persist owing to anticipated further increases in surface melting, reduced meltwater storage in firn, and the waning importance of dynamical mass losses (<span class="hlt">ice</span> calving) as the <span class="hlt">ice</span> <span class="hlt">sheets</span> 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> <span class="hlt">sheet</span> 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> <span class="hlt">sheet</span>. 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> <span class="hlt">sheet</span> dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900033212&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=19900033212&hterms=balance+sheet&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dbalance%2Bsheet"><span>Growth of Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> - Interpretation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zwally, H. Jay</p> <p>1989-01-01</p> <p>An observed 0.23 m/year thickening of the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> indicates a 25 percent to 45 percent excess <span class="hlt">ice</span> accumulation over the amount required to balance the outward <span class="hlt">ice</span> flow. The implied global sea-level depletion is 0.2 to 0.4 mm/year, depending on whether the thickening is only recent (5 to 10 years) or longer term (less than 100 years). If there is a similar imbalance in the northern 60 percent of the <span class="hlt">ice-sheet</span> area, the depletion is 0.35 to 0.7 mm/year. Increasing <span class="hlt">ice</span> thickness suggests that the precipitation is higher than the long-term average; higher precipitation may be a characteristic of warmer climates in polar regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.C33A0669O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.C33A0669O"><span>Recent Increases in <span class="hlt">Snow</span> Accumulation and Decreases in Sea-<span class="hlt">Ice</span> Concentration Recorded in a Coastal NW Greenland <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>Osterberg, E. C.; Thompson, J. T.; Wong, G. J.; Hawley, R. L.; Kelly, M. A.; Lutz, E.; Howley, J.; Ferris, D. G.</p> <p>2013-12-01</p> <p>A significant rise in summer temperatures over the past several decades has led to widespread retreat of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (GIS) margin and surrounding sea <span class="hlt">ice</span>. Recent observations from geodetic stations and GRACE show that <span class="hlt">ice</span> mass loss progressed from South Greenland up to Northwest Greenland by 2005 (Khan et al., 2010). Observations from meteorological stations at the U.S. Thule Air Force Base, remote sensing platforms, and climate reanalyses indicate a 3.5C mean annual warming in the Thule region and a 44% decrease in summer (JJAS) sea-<span class="hlt">ice</span> concentrations in Baffin Bay from 1980-2010. Mean annual precipitation near Thule increased by 12% over this interval, with the majority of the increase occurring in fall (SON). To improve projections of future <span class="hlt">ice</span> loss and sea-level rise in a warming climate, we are currently developing multi-proxy records (lake sediment cores, <span class="hlt">ice</span> cores, glacial geologic data, glaciological models) of Holocene climate variability and cryospheric response in NW Greenland, with a focus on past warm periods. As part of our efforts to develop a millennial-length <span class="hlt">ice</span> core paleoclimate record from the Thule region, we collected and analyzed <span class="hlt">snow</span> pit samples and short firn cores (up to 20 m) from the coastal region of the GIS (2Barrel site; 76.9317 N, 63.1467 W) and the summit of North <span class="hlt">Ice</span> Cap (76.938 N, 67.671 W) in 2011 and 2012, respectively. The 2Barrel <span class="hlt">ice</span> core was sampled using a continuous <span class="hlt">ice</span> core melting system at Dartmouth, and subsequently analyzed for major anion and trace element concentrations and stable water isotope ratios. Here we show that the 2Barrel <span class="hlt">ice</span> core spanning 1990-2010 records a 25% increase in mean annual <span class="hlt">snow</span> accumulation, and is positively correlated (r = 0.52, p<0.01) with ERA-Interim precipitation. The 2Barrel annual sea-salt Na concentration is strongly correlated (r = 0.5-0.8, p<0.05) with summer and fall sea-<span class="hlt">ice</span> concentrations in northern Baffin Bay near Thule (Figure 1). We hypothesize that the positive</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1813272G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1813272G"><span>ISMIP6 - initMIP: Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> model initialisation experiments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goelzer, Heiko; Nowicki, Sophie; Payne, Tony; Larour, Eric; Abe Ouchi, Ayako; Gregory, Jonathan; Lipscomb, William; Seroussi, Helene; Shepherd, Andrew; Edwards, Tamsin</p> <p>2016-04-01</p> <p>Earlier large-scale Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> sea-level projections e.g. those run during <span class="hlt">ice</span>2sea and SeaRISE initiatives have shown that <span class="hlt">ice</span> <span class="hlt">sheet</span> initialisation can have a large effect on the projections and gives rise to important uncertainties. This intercomparison exercise (initMIP) aims at comparing, evaluating and improving the initialization techniques used in the <span class="hlt">ice</span> <span class="hlt">sheet</span> modeling community and to estimate the associated uncertainties. It is the first in a series of <span class="hlt">ice</span> <span class="hlt">sheet</span> model intercomparison activities within ISMIP6 (<span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model Intercomparison Project for CMIP6). The experiments are conceived for the large-scale Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> and are designed to allow intercomparison between participating models of 1) the initial present-day state of the <span class="hlt">ice</span> <span class="hlt">sheet</span> and 2) the response in two schematic forward experiments. The latter experiments serve to evaluate the initialisation in terms of model drift (forward run without any forcing) and response to a large perturbation (prescribed surface mass balance anomaly). We present and discuss first results of the intercomparison and highlight important uncertainties with respect to projections of the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> sea-level contribution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004AGUFM.C31A0292F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUFM.C31A0292F"><span>Climate Sensitivity to Realistic Solar Heating of <span class="hlt">Snow</span> and <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>Flanner, M.; Zender, C. S.</p> <p>2004-12-01</p> <p><span class="hlt">Snow</span> and <span class="hlt">ice</span>-covered surfaces are highly reflective and play an integral role in the planetary radiation budget. However, GCMs typically prescribe <span class="hlt">snow</span> reflection and absorption based on minimal knowledge of <span class="hlt">snow</span> physical characteristics. We performed climate sensitivity simulations with the NCAR CCSM including a new physically-based multi-layer <span class="hlt">snow</span> radiative transfer model. The model predicts the effects of vertically resolved heating, absorbing aerosol, and snowpack transparency on snowpack evolution and climate. These processes significantly reduce the model's near-infrared albedo bias over deep snowpacks. While the current CCSM implementation prescribes all solar radiative absorption to occur in the top 2 cm of <span class="hlt">snow</span>, we estimate that about 65% occurs beneath this level. Accounting for the vertical distribution of snowpack heating and more realistic reflectance significantly alters snowpack depth, surface albedo, and surface air temperature over Northern Hemisphere regions. Implications for the strength of the <span class="hlt">ice</span>-albedo feedback will be discussed.</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-sheet</span> 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-sheet</span> 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 variations of this <span class="hlt">ice-sheet</span> 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> <span class="hlt">Sheet</span>, thus fitting the concept of a globally interlocked <span class="hlt">ice-sheet</span> 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> <span class="hlt">Sheet</span> strongly influenced Southern Hemisphere climate and terminated the last <span class="hlt">ice</span> age simultaneously in both polar hemispheres. Atmospheric carbon dioxide linked to high-latitude oceans is the most likely candidate ( Shackleton and Pisias, 1985, Atmospheric carbon dioxide, orbital forcing, and climate. In "The Carbon Cycle and Atmospheric CO 2: Natural Variations Archean to Present" (E. T. Sundquest and W. S. Broecker, Eds.), pp. 303-318. Geophysical Monograph 32, American Geophysical Union, Washington, D.C.), but another potential influence was high-frequency climatic oscillations (2500 yr). It is postulated that variations in atmospheric carbon dioxide acted through an Antarctic <span class="hlt">ice</span> shelf linked to the grounded <span class="hlt">ice</span> <span class="hlt">sheet</span> 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-sheet</span> 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://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-sheet</span> 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 mass balance stability of the Laurentide <span class="hlt">ice</span> <span class="hlt">sheet</span>--the largest glacial <span class="hlt">ice</span> mass 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 mass balance of the Laurentide <span class="hlt">ice</span> <span class="hlt">sheet</span> was positive throughout much of the deglaciation, and suggest that dynamic discharge was mainly responsible for mass loss during this time. Total surface mass 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> <span class="hlt">sheet</span> remained a viable <span class="hlt">ice</span> <span class="hlt">sheet</span> before the Holocene and began to fully deglaciate only once summer temperatures and radiative forcing over the <span class="hlt">ice</span> <span class="hlt">sheet</span> 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://adsabs.harvard.edu/abs/2014EGUGA..1614162B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1614162B"><span>The role of <span class="hlt">ice</span> shelves in the Holocene evolution of the Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bernales, Jorge; Rogozhina, Irina; Thomas, Maik</p> <p>2014-05-01</p> <p>Using the continental-scale <span class="hlt">ice</span> <span class="hlt">sheet</span>-shelf model SICOPOLIS (Greve, 1997 [1]; Sato and Greve, 2012 [2]), we assess the influence of <span class="hlt">ice</span> shelves on the Holocene evolution and present-day geometry of the Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span>. We have designed a series of paleoclimate simulations driven by a time-evolved climate forcing that couples the surface temperature record from the Vostok <span class="hlt">ice</span> core with precipitation pattern using an empirical relation of Dahl-Jensen et al., (1998) [3]. Our numerical experiments show that the geometry of <span class="hlt">ice</span> shelves is determined by the evolution of climate and ocean conditions over time scales of 15 to 25 kyr. This implies that the initial configuration of <span class="hlt">ice</span> shelves at the Last Glacial Maximum (LGM, about 21 kyr before present) has a significant effect on the modelled Early Holocene volume of <span class="hlt">ice</span> shelves (up to 20%) that gradually diminishes to a negligible level for the present-day <span class="hlt">ice</span> shelf configuration. Thus, the present-day geometry of the Antarctic <span class="hlt">ice</span> shelves can be attained even if an <span class="hlt">ice</span>-shelf-free initial condition is chosen at the LGM. However, the grounded <span class="hlt">ice</span> volume, thickness and dynamic states are found to be sensitive to the <span class="hlt">ice</span> shelf dynamics over a longer history spanning several tens of thousands of years. A presence of extensive marine <span class="hlt">ice</span> at the LGM, supported by sediment core reconstructions (e.g. Naish et al., 2009 [4]), has a clear buttressing effect on the grounded <span class="hlt">ice</span> that remains significant over a period of 30 to 50 kyr. If <span class="hlt">ice</span>-shelf-free conditions are prescribed at the LGM, the modelled Early Holocene and present-day grounded <span class="hlt">ice</span> volumes are underestimated by up to 10%, as opposed to simulations incorporating <span class="hlt">ice</span> shelf dynamics over longer periods. The use of <span class="hlt">ice</span>-shelf-free LGM conditions thus results in 50 to over 200 meters thinner <span class="hlt">ice</span> <span class="hlt">sheet</span> across much of East Antarctica. References [1] Greve, R. (1997). Application of a polythermal three-dimensional <span class="hlt">ice</span> <span class="hlt">sheet</span> model to the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span>: response to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140006009','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140006009"><span>A Supplementary Clear-Sky <span class="hlt">Snow</span> and <span class="hlt">Ice</span> Recognition Technique for CERES Level 2 Products</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Radkevich, Alexander; Khlopenkov, Konstantin; Rutan, David; Kato, Seiji</p> <p>2013-01-01</p> <p>Identification of clear-sky <span class="hlt">snow</span> and <span class="hlt">ice</span> is an important step in the production of cryosphere radiation budget products, which are used in the derivation of long-term data series for climate research. In this paper, a new method of clear-sky <span class="hlt">snow/ice</span> identification for Moderate Resolution Imaging Spectroradiometer (MODIS) is presented. The algorithm's goal is to enhance the identification of <span class="hlt">snow</span> and <span class="hlt">ice</span> within the Clouds and the Earth's Radiant Energy System (CERES) data after application of the standard CERES scene identification scheme. The input of the algorithm uses spectral radiances from five MODIS bands and surface skin temperature available in the CERES Single Scanner Footprint (SSF) product. The algorithm produces a cryosphere rating from an aggregated test: a higher rating corresponds to a more certain identification of the clear-sky <span class="hlt">snow/ice</span>-covered scene. Empirical analysis of regions of interest representing distinctive targets such as <span class="hlt">snow</span>, <span class="hlt">ice</span>, <span class="hlt">ice</span> and water clouds, open waters, and <span class="hlt">snow</span>-free land selected from a number of MODIS images shows that the cryosphere rating of <span class="hlt">snow/ice</span> targets falls into 95% confidence intervals lying above the same confidence intervals of all other targets. This enables recognition of clear-sky cryosphere by using a single threshold applied to the rating, which makes this technique different from traditional branching techniques based on multiple thresholds. Limited tests show that the established threshold clearly separates the cryosphere rating values computed for the cryosphere from those computed for noncryosphere scenes, whereas individual tests applied consequently cannot reliably identify the cryosphere for complex scenes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ISPAr41B8..481B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ISPAr41B8..481B"><span>Mass Balance Changes and <span class="hlt">Ice</span> Dynamics of Greenland and Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheets</span> from Laser Altimetry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Babonis, G. S.; Csatho, B.; Schenk, T.</p> <p>2016-06-01</p> <p>During the past few decades the Greenland and Antarctic <span class="hlt">ice</span> <span class="hlt">sheets</span> have lost <span class="hlt">ice</span> at accelerating rates, caused by increasing surface temperature. The melting of the two big <span class="hlt">ice</span> <span class="hlt">sheets</span> has a big impact on global sea level rise. If the <span class="hlt">ice</span> <span class="hlt">sheets</span> would melt down entirely, the sea level would rise more than 60 m. Even a much smaller rise would cause dramatic damage along coastal regions. In this paper we report about a major upgrade of surface elevation changes derived from laser altimetry data, acquired by NASA's <span class="hlt">Ice</span>, Cloud and land Elevation Satellite mission (ICESat) and airborne laser campaigns, such as Airborne Topographic Mapper (ATM) and Land, Vegetation and <span class="hlt">Ice</span> Sensor (LVIS). For detecting changes in <span class="hlt">ice</span> <span class="hlt">sheet</span> elevations we have developed the Surface Elevation Reconstruction And Change detection (SERAC) method. It computes elevation changes of small surface patches by keeping the surface shape constant and considering the absolute values as surface elevations. We report about important upgrades of earlier results, for example the inclusion of local <span class="hlt">ice</span> caps and the temporal extension from 1993 to 2014 for the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> and for a comprehensive reconstruction of <span class="hlt">ice</span> thickness and mass changes for the Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheets</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://rosap.ntl.bts.gov/view/dot/27184','DOTNTL'); return false;" href="https://rosap.ntl.bts.gov/view/dot/27184"><span>Evaluation of the effectiveness of salt neutralizers for washing <span class="hlt">snow</span> and <span class="hlt">ice</span> equipment.</span></a></p> <p><a target="_blank" href="http://ntlsearch.bts.gov/tris/index.do">DOT National Transportation Integrated Search</a></p> <p></p> <p>2014-01-01</p> <p>In winter maintenance, the chloride-based deicers used to keep roadways clear of : <span class="hlt">snow</span> and <span class="hlt">ice</span> are highly corrosive to vehicles and equipment. Corrosion of <span class="hlt">snow</span> and <span class="hlt">ice</span> equipment : is a major issue causing increased maintenance and repair costs, red...</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> <span class="hlt">sheets</span> modulate global sea level by storing water deposited as <span class="hlt">snow</span> on the surface, and discharging water back into the ocean through melting. Their physical state can be characterized in terms of their mass balance and dynamics. To estimate the current <span class="hlt">ice</span> mass balance, and to predict future changes in the motion of the Greenland and Antarctic <span class="hlt">ice</span> <span class="hlt">sheets</span>, it is necessary to know the <span class="hlt">ice</span> <span class="hlt">sheet</span> thickness and the physical conditions of the <span class="hlt">ice</span> <span class="hlt">sheet</span> surface and bed. This information is required at fine resolution and over extensive portions of the <span class="hlt">ice</span> <span class="hlt">sheets</span>. 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> <span class="hlt">sheet</span> 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('https://rosap.ntl.bts.gov/view/dot/3912','DOTNTL'); return false;" href="https://rosap.ntl.bts.gov/view/dot/3912"><span>Southeast Michigan <span class="hlt">Snow</span> and <span class="hlt">Ice</span> Management (SEMSIM)</span></a></p> <p><a target="_blank" href="http://ntlsearch.bts.gov/tris/index.do">DOT National Transportation Integrated Search</a></p> <p></p> <p>2001-07-01</p> <p>The Southeast Michigan <span class="hlt">Snow</span> and <span class="hlt">Ice</span> Management (SEMSIM) partnership includes the Detroit Department of Public Works, the Road Commission of Macomb County, the Road Commission for Oakland County, and the Wayne County Department of Public Services. The...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C23D..01R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C23D..01R"><span><span class="hlt">Ice</span> <span class="hlt">sheet</span> systems and sea level change.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rignot, E. J.</p> <p>2015-12-01</p> <p>Modern views of <span class="hlt">ice</span> <span class="hlt">sheets</span> provided by satellites, airborne surveys, in situ data and paleoclimate records while transformative of glaciology have not fundamentally changed concerns about <span class="hlt">ice</span> <span class="hlt">sheet</span> stability and collapse that emerged in the 1970's. Motivated by the desire to learn more about <span class="hlt">ice</span> <span class="hlt">sheets</span> using new technologies, we stumbled on an unexplored field of science and witnessed surprising changes before realizing that most were coming too fast, soon and large. <span class="hlt">Ice</span> <span class="hlt">sheets</span> are integrant part of the Earth system; they interact vigorously with the atmosphere and the oceans, yet most of this interaction is not part of current global climate models. Since we have never witnessed the collapse of a marine <span class="hlt">ice</span> <span class="hlt">sheet</span>, observations and exploration remain critical sentinels. At present, these observations suggest that Antarctica and Greenland have been launched into a path of multi-meter sea level rise caused by rapid climate warming. While the current loss of <span class="hlt">ice</span> <span class="hlt">sheet</span> mass to the ocean remains a trickle, every mm of sea level change will take centuries of climate reversal to get back, several major marine-terminating sectors have been pushed out of equilibrium, and <span class="hlt">ice</span> shelves are irremediably being lost. As glaciers retreat from their salty, warm, oceanic margins, they will melt away and retreat slower, but concerns remain about sea level change from vastly marine-based sectors: 2-m sea level equivalent in Greenland and 23-m in Antarctica. Significant changes affect 2/4 marine-based sectors in Greenland - Jakobshavn Isb. and the northeast stream - with Petermann Gl. not far behind. Major changes have affected the Amundsen Sea sector of West Antarctica since the 1980s. Smaller yet significant changes affect the marine-based Wilkes Land sector of East Antarctica, a reminder that not all marine-based <span class="hlt">ice</span> is in West Antarctica. Major advances in reducing uncertainties in sea level projections will require massive, interdisciplinary efforts that are not currently in place</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C32B..05S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C32B..05S"><span>The <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Mass Balance Inter-comparison Exercise</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shepherd, A.; Ivins, E. R.</p> <p>2015-12-01</p> <p>Fluctuations in the mass of <span class="hlt">ice</span> stored in Antarctica and Greenland are of considerable societal importance. The <span class="hlt">Ice</span> <span class="hlt">Sheet</span> 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 <span class="hlt">ice</span> <span class="hlt">sheet</span> losses. Within IMBIE, estimates of <span class="hlt">ice</span> <span class="hlt">sheet</span> 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 <span class="hlt">ice</span> <span class="hlt">sheet</span> mass balance to date. In its first phase, IMBIE involved 27 science teams, and delivered a first community assessment of <span class="hlt">ice</span> <span class="hlt">sheet</span> 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 <span class="hlt">ice</span> <span class="hlt">sheet</span> mass balance, (ii) combining satellite data sets leads to significant improvement in certainty, (iii) the polar <span class="hlt">ice</span> <span class="hlt">sheets</span> contributed 11 ± 4 mm to global sea levels between 1992 and 2012, and (iv) that combined <span class="hlt">ice</span> 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 <span class="hlt">ice</span> dynamical imbalance - information that is of critical importance for climate modelling. This presentation outlines the approach</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70191516','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70191516"><span>The effects of <span class="hlt">snow</span> and salt on <span class="hlt">ice</span> table stability in University Valley, 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>Williams, Kaj; Heldmann, Jennifer L.; McKay, Christopher P.; Mellon, Michael T.</p> <p>2018-01-01</p> <p>The Antarctic Dry Valleys represent a unique environment where it is possible to study dry permafrost overlaying an <span class="hlt">ice</span>-rich permafrost. In this paper, two opposing mechanisms for <span class="hlt">ice</span> table stability in University Valley are addressed: i) diffusive recharge via thin seasonal <span class="hlt">snow</span> deposits and ii) desiccation via salt deposits in the upper soil column. A high-resolution time-marching soil and <span class="hlt">snow</span> model was constructed and applied to University Valley, driven by meteorological station atmospheric measurements. It was found that periodic thin surficial <span class="hlt">snow</span> deposits (observed in University Valley) are capable of drastically slowing (if not completely eliminating) the underlying <span class="hlt">ice</span> table ablation. The effects of NaCl, CaCl2 and perchlorate deposits were then modelled. Unlike the <span class="hlt">snow</span> cover, however, the presence of salt in the soil surface (but no periodic <span class="hlt">snow</span>) results in a slight increase in the <span class="hlt">ice</span> table recession rate, due to the hygroscopic effects of salt sequestering vapour from the <span class="hlt">ice</span> table below. Near-surface pore <span class="hlt">ice</span> frequently forms when large amounts of salt are present in the soil due to the suppression of the saturation vapour pressure. Implications for Mars high latitudes are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5911933','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5911933"><span><span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model Intercomparison Project (ISMIP6) contribution to CMIP6</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Nowicki, Sophie M.J.; Payne, Tony; Larour, Eric; Seroussi, Helene; Goelzer, Heiko; Lipscomb, William; Gregory, Jonathan; Abe-Ouchi, Ayako; Shepherd, Andrew</p> <p>2018-01-01</p> <p>Reducing the uncertainty in the past, present and future contribution of <span class="hlt">ice</span> <span class="hlt">sheets</span> to sea-level change requires a coordinated effort between the climate and glaciology communities. The <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model Intercomparison Project for CMIP6 (ISMIP6) is the primary activity within the Coupled Model Intercomparison Project – phase 6 (CMIP6) focusing on the Greenland and Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheets</span>. In this paper, we describe the framework for ISMIP6 and its relationship to other activities within CMIP6. The ISMIP6 experimental design relies on CMIP6 climate models and includes, for the first time within CMIP, coupled <span class="hlt">ice</span> <span class="hlt">sheet</span> – climate models as well as standalone <span class="hlt">ice</span> <span class="hlt">sheet</span> models. To facilitate analysis of the multi-model ensemble and to generate a set of standard climate inputs for standalone <span class="hlt">ice</span> <span class="hlt">sheet</span> models, ISMIP6 defines a protocol for all variables related to <span class="hlt">ice</span> <span class="hlt">sheets</span>. ISMIP6 will provide a basis for investigating the feedbacks, impacts, and sea-level changes associated with dynamic <span class="hlt">ice</span> <span class="hlt">sheets</span> and for quantifying the uncertainty in <span class="hlt">ice-sheet</span>-sourced global sea-level change. PMID:29697697</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRE..122.2250B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRE..122.2250B"><span>Preservation of Midlatitude <span class="hlt">Ice</span> <span class="hlt">Sheets</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>Bramson, A. M.; Byrne, S.; Bapst, J.</p> <p>2017-11-01</p> <p>Excess <span class="hlt">ice</span> with a minimum age of tens of millions of years is widespread in Arcadia Planitia on Mars, and a similar deposit has been found in Utopia Planitia. The conditions that led to the formation and preservation of these midlatitude <span class="hlt">ice</span> <span class="hlt">sheets</span> hold clues to past climate and subsurface structure on Mars. We simulate the thermal stability and retreat of buried excess <span class="hlt">ice</span> <span class="hlt">sheets</span> over 21 Myr of Martian orbital solutions and find that the <span class="hlt">ice</span> <span class="hlt">sheets</span> can be orders of magnitude older than the obliquity cycles that are typically thought to drive midlatitude <span class="hlt">ice</span> deposition and sublimation. Retreat of this <span class="hlt">ice</span> in the last 4 Myr could have contributed 6% of the volume of the north polar layered deposits (NPLD) and more than 10% if the NPLD are older than 4 Myr. Matching the measured dielectric constants of the Arcadia and Utopia Planitia deposits requires <span class="hlt">ice</span> porosities of 25-35%. We model geothermally driven vapor migration through porous <span class="hlt">ice</span> under Martian temperatures and find that Martian firn may be able to maintain porosity for timescales longer than we predict for retreat of the <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014ESD.....5..271L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014ESD.....5..271L"><span>Projecting Antarctic <span class="hlt">ice</span> discharge using response functions from SeaRISE <span class="hlt">ice-sheet</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>Levermann, A.; Winkelmann, R.; Nowicki, S.; Fastook, J. L.; Frieler, K.; Greve, R.; Hellmer, H. H.; Martin, M. A.; Meinshausen, M.; Mengel, M.; Payne, A. J.; Pollard, D.; Sato, T.; Timmermann, R.; Wang, W. L.; Bindschadler, R. A.</p> <p>2014-08-01</p> <p>The largest uncertainty in projections of future sea-level change results from the potentially changing dynamical <span class="hlt">ice</span> discharge from Antarctica. Basal <span class="hlt">ice</span>-shelf melting induced by a warming ocean has been identified as a major cause for additional <span class="hlt">ice</span> flow across the grounding line. Here we attempt to estimate the uncertainty range of future <span class="hlt">ice</span> discharge from Antarctica by combining uncertainty in the climatic forcing, the oceanic response and the <span class="hlt">ice-sheet</span> model response. The uncertainty in the global mean temperature increase is obtained from historically constrained emulations with the MAGICC-6.0 (Model for the Assessment of Greenhouse gas Induced Climate Change) model. The oceanic forcing is derived from scaling of the subsurface with the atmospheric warming from 19 comprehensive climate models of the Coupled Model Intercomparison Project (CMIP-5) and two ocean models from the EU-project <span class="hlt">Ice</span>2Sea. The dynamic <span class="hlt">ice-sheet</span> response is derived from linear response functions for basal <span class="hlt">ice</span>-shelf melting for four different Antarctic drainage regions using experiments from the Sea-level Response to <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Evolution (SeaRISE) intercomparison project with five different Antarctic <span class="hlt">ice-sheet</span> models. The resulting uncertainty range for the historic Antarctic contribution to global sea-level rise from 1992 to 2011 agrees with the observed contribution for this period if we use the three <span class="hlt">ice-sheet</span> models with an explicit representation of <span class="hlt">ice</span>-shelf dynamics and account for the time-delayed warming of the oceanic subsurface compared to the surface air temperature. The median of the additional <span class="hlt">ice</span> loss for the 21st century is computed to 0.07 m (66% range: 0.02-0.14 m; 90% range: 0.0-0.23 m) of global sea-level equivalent for the low-emission RCP-2.6 (Representative Concentration Pathway) scenario and 0.09 m (66% range: 0.04-0.21 m; 90% range: 0.01-0.37 m) for the strongest RCP-8.5. Assuming no time delay between the atmospheric warming and the oceanic subsurface, these</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_13 --> <div id="page_14" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="261"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC43H1150W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC43H1150W"><span>Geoengineering Marine <span class="hlt">Ice</span> <span class="hlt">Sheets</span></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>Mass 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 mass loss and sea-level rise. If the grounding line enters a section of overdeepened bed the <span class="hlt">ice</span> <span class="hlt">sheet</span> may even enter a runaway collapse via the marine <span class="hlt">ice</span> <span class="hlt">sheet</span> 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> <span class="hlt">sheet</span> 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/2017AGUFM.C33C1213N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C33C1213N"><span>On the Impact of <span class="hlt">Snow</span> Salinity on CryoSat-2 First-Year Sea <span class="hlt">Ice</span> Thickness Retrievals</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nandan, V.; Yackel, J.; Geldsetzer, T.; Mahmud, M.</p> <p>2017-12-01</p> <p>European Space Agency's Ku-band altimeter CryoSat-2 (CS-2) has demonstrated its potential to provide extensive basin-scale spatial and temporal measurements of Arctic sea <span class="hlt">ice</span> freeboard. It is assumed that CS-2 altimetric returns originate from the <span class="hlt">snow</span>/sea <span class="hlt">ice</span> interface (assumed to be the main scattering horizon). However, in newly formed thin <span class="hlt">ice</span> ( 0.6 m) through to thick first-year sea <span class="hlt">ice</span> (FYI) ( 2 m), upward wicking of brine into the <span class="hlt">snow</span> cover from the underlying sea <span class="hlt">ice</span> surface produces saline <span class="hlt">snow</span> layers, especially in the bottom 6-8 cm of a <span class="hlt">snow</span> cover. This in turn modifies the brine volume at/or near the <span class="hlt">snow</span>/sea <span class="hlt">ice</span> interface, altering the dielectric and scattering properties of the <span class="hlt">snow</span> cover, leading to strong Ku-band microwave attenuation within the upper <span class="hlt">snow</span> volume. Such significant reductions in Ku-band penetration may substantially affect CS-2 FYI freeboard retrievals. Therefore, the goal of this study is to evaluate a theoretical approach to estimate <span class="hlt">snow</span> salinity induced uncertainty on CS-2 Arctic FYI freeboard measurements. Using the freeboard-to-thickness hydrostatic equilibrium equation, we quantify the error differences between the CS-2 FYI thickness, (assuming complete penetration of CS-2 radar signals to the <span class="hlt">snow</span>/FYI interface), and the FYI thickness based on the modeled Ku-band main scattering horizon for different <span class="hlt">snow</span> cover cases. We utilized naturally occurring saline and non-saline <span class="hlt">snow</span> cover cases ranging between 6 cm to 32 cm from the Canadian Arctic, observed during late-winter from 1993 to 2017, on newly-formed <span class="hlt">ice</span> ( 0.6 m), medium ( 1.5 m) and thick FYI ( 2 m). Our results suggest that irrespective of the thickness of the <span class="hlt">snow</span> cover overlaying FYI, the thickness of brine-wetted <span class="hlt">snow</span> layers and actual FYI freeboard strongly influence the amount with which CS-2 FYI freeboard estimates and thus thickness calculations are overestimated. This effect is accentuated for increasingly thicker saline <span class="hlt">snow</span> covers overlaying newly-formed <span class="hlt">ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4822592','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4822592"><span>Dynamic Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> during the early to mid-Miocene</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>DeConto, Robert M.; Pollard, David; Levy, Richard H.</p> <p>2016-01-01</p> <p>Geological data indicate that there were major variations in Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> volume and extent during the early to mid-Miocene. Simulating such large-scale changes is problematic because of a strong hysteresis effect, which results in stability once the <span class="hlt">ice</span> <span class="hlt">sheets</span> have reached continental size. A relatively narrow range of atmospheric CO2 concentrations indicated by proxy records exacerbates this problem. Here, we are able to simulate large-scale variability of the early to mid-Miocene Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> because of three developments in our modeling approach. (i) We use a climate–<span class="hlt">ice</span> <span class="hlt">sheet</span> coupling method utilizing a high-resolution atmospheric component to account for <span class="hlt">ice</span> sheet–climate feedbacks. (ii) The <span class="hlt">ice</span> <span class="hlt">sheet</span> model includes recently proposed mechanisms for retreat into deep subglacial basins caused by <span class="hlt">ice</span>-cliff failure and <span class="hlt">ice</span>-shelf hydrofracture. (iii) We account for changes in the oxygen isotopic composition of the <span class="hlt">ice</span> <span class="hlt">sheet</span> by using isotope-enabled climate and <span class="hlt">ice</span> <span class="hlt">sheet</span> models. We compare our modeling results with <span class="hlt">ice</span>-proximal records emerging from a sedimentological drill core from the Ross Sea (Andrill-2A) that is presented in a companion article. The variability in Antarctic <span class="hlt">ice</span> volume that we simulate is equivalent to a seawater oxygen isotope signal of 0.52–0.66‰, or a sea level equivalent change of 30–36 m, for a range of atmospheric CO2 between 280 and 500 ppm and a changing astronomical configuration. This result represents a substantial advance in resolving the long-standing model data conflict of Miocene Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> and sea level variability. PMID:26903645</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23739423','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23739423"><span><span class="hlt">Ice-sheet</span> mass balance and climate change.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>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</p> <p>2013-06-06</p> <p>Since the 2007 Intergovernmental Panel on Climate Change Fourth Assessment Report, new observations of <span class="hlt">ice-sheet</span> mass balance and improved computer simulations of <span class="hlt">ice-sheet</span> response to continuing climate change have been published. Whereas Greenland is losing <span class="hlt">ice</span> mass at an increasing pace, current Antarctic <span class="hlt">ice</span> loss is likely to be less than some recently published estimates. It remains unclear whether East Antarctica has been gaining or losing <span class="hlt">ice</span> mass over the past 20 years, and uncertainties in <span class="hlt">ice</span>-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.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017E%26PSL.460..293C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017E%26PSL.460..293C"><span>The layered evolution of fabric and microstructure of <span class="hlt">snow</span> at Point Barnola, Central East Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Calonne, Neige; Montagnat, Maurine; Matzl, Margret; Schneebeli, Martin</p> <p>2017-02-01</p> <p><span class="hlt">Snow</span> fabric, defined as the distribution of the c-axis orientations of the <span class="hlt">ice</span> crystals in <span class="hlt">snow</span>, is poorly known. So far, only one study exits that measured <span class="hlt">snow</span> fabric based on a statistically representative technique. This recent study has revealed the impact of temperature gradient metamorphism on the evolution of fabric in natural <span class="hlt">snow</span>, based on cold laboratory experiments. On polar <span class="hlt">ice</span> <span class="hlt">sheets</span>, <span class="hlt">snow</span> properties are currently investigated regarding their strong variability in time and space, notably because of their potential influence on firn processes and consequently on <span class="hlt">ice</span> core analysis. Here, we present measurements of fabric and microstructure of <span class="hlt">snow</span> from Point Barnola, East Antarctica (close to Dome C). We analyzed a <span class="hlt">snow</span> profile from 0 to 3 m depth, where temperature gradients occur. The main contributions of the paper are (1) a detailed characterization of <span class="hlt">snow</span> in the upper meters of the <span class="hlt">ice</span> <span class="hlt">sheet</span>, especially by providing data on <span class="hlt">snow</span> fabric, and (2) the study of a fundamental <span class="hlt">snow</span> process, never observed up to now in a natural snowpack, namely the role of temperature gradient metamorphism on the evolution of the <span class="hlt">snow</span> fabric. <span class="hlt">Snow</span> samples were scanned by micro-tomography to measure continuous profiles of microstructural properties (density, specific surface area and pore thickness). Fabric analysis was performed using an automatic <span class="hlt">ice</span> texture analyzer on 77 representative thin sections cut out from the samples. Different types of <span class="hlt">snow</span> fabric could be identified and persist at depth. <span class="hlt">Snow</span> fabric is significantly correlated with <span class="hlt">snow</span> microstructure, pointing to the simultaneous influence of temperature gradient metamorphism on both properties. We propose a mechanism based on preferential grain growth to explain the fabric evolution under temperature gradients. Our work opens the question of how such a layered profile of fabric and microstructure evolves at depth and further influences the physical and mechanical properties of <span class="hlt">snow</span> and firn. More generally</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA103734','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA103734"><span>Review of Thermal Properties of <span class="hlt">Snow</span>, <span class="hlt">Ice</span> and Sea <span class="hlt">Ice</span>,</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1981-06-01</p> <p>AD-AL03 734 COLD RE61ONS RESEARCH AND ENGINEERING LAS HANOVER NH F/G 8/12AI3 3REVIEW OF THERMAL PROPERTIES OF <span class="hlt">SNOW</span>. <span class="hlt">ICE</span> AND SEA <span class="hlt">ICE</span>,(U)UNCLASSIFIlED...Distribution/ Availability Codes Avail and/or D~ Dis~t Special D 1 7 C- T > L) UNITED STATES ARMY CORPS OF ENGINEERS COLD REGIONS RESEARCH AND ENGINEERING...PROGRAM ELEMENT, PROJECT. TASK AREA A WORK UNIT NUMBERS U.S. Army Cold Regions Research and Engineering Laboratory Hanover, New Hampshire 03755 DA Pr</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70034736','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70034736"><span>Obliquity-paced Pliocene West Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> oscillations</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Naish, T.; Powell, R.; Levy, R.; Wilson, G.; Scherer, R.; Talarico, F.; Krissek, L.; Niessen, F.; Pompilio, M.; Wilson, T.; Carter, L.; DeConto, R.; Huybers, P.; McKay, R.; Pollard, D.; Ross, J.; Winter, D.; Barrett, P.; Browne, G.; Cody, R.; Cowan, E.; Crampton, J.; Dunbar, G.; Dunbar, N.; Florindo, F.; Gebhardt, C.; Graham, I.; Hannah, M.; Hansaraj, D.; Harwood, D.; Helling, D.; Henrys, S.; Hinnov, L.; Kuhn, G.; Kyle, P.; Laufer, A.; Maffioli, P.; Magens, D.; Mandernack, K.; McIntosh, W.; Millan, C.; Morin, R.; Ohneiser, C.; Paulsen, T.; Persico, D.; Raine, I.; Reed, J.; Riesselman, C.; Sagnotti, L.; Schmitt, D.; Sjunneskog, C.; Strong, P.; Taviani, M.; Vogel, S.; Wilch, T.; Williams, T.</p> <p>2009-01-01</p> <p>Thirty years after oxygen isotope records from microfossils deposited in ocean sediments confirmed the hypothesis that variations in the Earth's orbital geometry control the <span class="hlt">ice</span> ages1, fundamental questions remain over the response of the Antarctic <span class="hlt">ice</span> <span class="hlt">sheets</span> to orbital cycles2. Furthermore, an understanding of the behaviour of the marine-based West Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> (WAIS) during the 'warmer-than-present' early-Pliocene epoch (5–3 Myr ago) is needed to better constrain the possible range of <span class="hlt">ice-sheet</span> behaviour in the context of future global warming3. Here we present a marine glacial record from the upper 600 m of the AND-1B sediment core recovered from beneath the northwest part of the Ross <span class="hlt">ice</span> shelf by the ANDRILL programme and demonstrate well-dated, 40-kyr cyclic variations in <span class="hlt">ice-sheet</span> extent linked to cycles in insolation influenced by changes in the Earth's axial tilt (obliquity) during the Pliocene. Our data provide direct evidence for orbitally induced oscillations in the WAIS, which periodically collapsed, resulting in a switch from grounded <span class="hlt">ice</span>, or <span class="hlt">ice</span> shelves, to open waters in the Ross embayment when planetary temperatures were up to 3 °C warmer than today4 and atmospheric CO2 concentration was as high as 400 p.p.m.v. (refs 5, 6). The evidence is consistent with a new <span class="hlt">ice-sheet/ice</span>-shelf model7 that simulates fluctuations in 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> <span class="hlt">sheet</span>, in response to ocean-induced melting paced by obliquity. During interglacial times, diatomaceous sediments indicate high surface-water productivity, minimal summer sea <span class="hlt">ice</span> and air temperatures above freezing, suggesting an additional influence of surface melt8 under conditions of elevated CO2.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AtmEn.140..415H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AtmEn.140..415H"><span>Effects of different temperature treatments on biological <span class="hlt">ice</span> nuclei in <span class="hlt">snow</span> samples</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hara, Kazutaka; Maki, Teruya; Kakikawa, Makiko; Kobayashi, Fumihisa; Matsuki, Atsushi</p> <p>2016-09-01</p> <p>The heat tolerance of biological <span class="hlt">ice</span> nucleation activity (INA) depends on their types. Different temperature treatments may cause varying degrees of inactivation on biological <span class="hlt">ice</span> nuclei (IN) in precipitation samples. In this study, we measured IN concentration and bacterial INA in <span class="hlt">snow</span> samples using a drop freezing assay, and compared the results for unheated <span class="hlt">snow</span> and <span class="hlt">snow</span> treated at 40 °C and 90 °C. At a measured temperature of -7 °C, the concentration of IN in untreated <span class="hlt">snow</span> was 100-570 L-1, whereas the concentration in <span class="hlt">snow</span> treated at 40 °C and 90 °C was 31-270 L-1 and 2.5-14 L-1, respectively. In the present study, heat sensitive IN inactivated by heating at 40 °C were predominant, and ranged 23-78% of IN at -7 °C compared with untreated samples. <span class="hlt">Ice</span> nucleation active Pseudomonas strains were also isolated from the <span class="hlt">snow</span> samples, and heating at 40 °C and 90 °C inactivated these microorganisms. Consequently, different temperature treatments induced varying degrees of inactivation on IN in <span class="hlt">snow</span> samples. Differences in the concentration of IN across a range of treatment temperatures might reflect the abundance of different heat sensitive biological IN components.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.C24A..08P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.C24A..08P"><span>Global mountain <span class="hlt">snow</span> and <span class="hlt">ice</span> loss driven by dust and black carbon radiative forcing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Painter, T. H.</p> <p>2014-12-01</p> <p>Changes in mountain <span class="hlt">snow</span> and glaciers have been our strongest indicators of the effects of changing climate. Earlier melt of <span class="hlt">snow</span> and losses of glacier mass have perturbed regional water cycling, regional climate, and ecosystem dynamics, and contributed strongly to sea level rise. Recent studies however have revealed that in some regions, the reduction of albedo by light absorbing impurities in <span class="hlt">snow</span> and <span class="hlt">ice</span> such as dust and black carbon can be distinctly more powerful than regional warming at melting <span class="hlt">snow</span> and <span class="hlt">ice</span>. In the Rocky Mountains, dust deposition has increased 5 to 7 fold in the last 150 years, leading to ~3 weeks earlier loss of <span class="hlt">snow</span> cover from forced melt. In absolute terms, in some years dust radiative forcing there can shorten <span class="hlt">snow</span> cover duration by nearly two months. Remote sensing retrievals are beginning to reveal powerful dust and black carbon radiative forcing in the Hindu Kush through Himalaya. In light of recent <span class="hlt">ice</span> cores that show pronounced increases in loading of dust and BC during the Anthropocene, these forcings may have contributed far more to glacier retreat than previously thought. For example, we have shown that the paradoxical end of the Little <span class="hlt">Ice</span> Age in the European Alps beginning around 1850 (when glaciers began to retreat but temperatures continued to decline and precipitation was unchanged) very likely was driven by the massive increases in deposition to <span class="hlt">snow</span> and <span class="hlt">ice</span> of black carbon from industrialization in surrounding nations. A more robust understanding of changes in mountain <span class="hlt">snow</span> and <span class="hlt">ice</span> during the Anthropocene requires that we move past simplistic treatments (e.g. temperature-index modeling) to energy balance approaches that assess changes in the individual forcings such as the most powerful component for melt - net solar radiation. Remote sensing retrievals from imaging spectrometers and multispectral sensors are giving us more powerful insights into the time-space variation of <span class="hlt">snow</span> and <span class="hlt">ice</span> albedo.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170003153','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170003153"><span><span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model Intercomparison Project (ISMIP6) Contribution to CMIP6</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nowicki, Sophie M. J.; Payne, Tony; Larour, Eric; Seroussi, Helene; Goelzer, Heiko; Lipscomb, William; Gregory, Jonathan; Abe-Ouchi, Ayako; Shepherd, Andrew</p> <p>2016-01-01</p> <p>Reducing the uncertainty in the past, present, and future contribution of <span class="hlt">ice</span> <span class="hlt">sheets</span> to sea-level change requires a coordinated effort between the climate and glaciology communities. The <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model Intercomparison Project for CMIP6 (ISMIP6) is the primary activity within the Coupled Model Intercomparison Project phase 6 (CMIP6) focusing on the Greenland and Antarctic <span class="hlt">ice</span> <span class="hlt">sheets</span>. In this paper, we describe the framework for ISMIP6 and its relationship with other activities within CMIP6. The ISMIP6 experimental design relies on CMIP6 climate models and includes, for the first time within CMIP, coupled <span class="hlt">ice</span>-sheetclimate models as well as standalone <span class="hlt">ice-sheet</span> models. To facilitate analysis of the multi-model ensemble and to generate a set of standard climate inputs for standalone <span class="hlt">ice-sheet</span> models, ISMIP6 defines a protocol for all variables related to <span class="hlt">ice</span> <span class="hlt">sheets</span>. ISMIP6 will provide a basis for investigating the feedbacks, impacts, and sea-level changes associated with dynamic <span class="hlt">ice</span> <span class="hlt">sheets</span> and for quantifying the uncertainty in <span class="hlt">ice-sheet</span>-sourced global sea-level change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015CliPa..11.1467B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015CliPa..11.1467B"><span>How might the North American <span class="hlt">ice</span> <span class="hlt">sheet</span> influence the northwestern Eurasian climate?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Beghin, P.; Charbit, S.; Dumas, C.; Kageyama, M.; Ritz, C.</p> <p>2015-10-01</p> <p>It is now widely acknowledged that past Northern Hemisphere <span class="hlt">ice</span> <span class="hlt">sheets</span> covering Canada and northern Europe at the Last Glacial Maximum (LGM) exerted a strong influence on climate by causing changes in atmospheric and oceanic circulations. In turn, these changes may have impacted the development of the <span class="hlt">ice</span> <span class="hlt">sheets</span> themselves through a combination of different feedback mechanisms. The present study is designed to investigate the potential impact of the North American <span class="hlt">ice</span> <span class="hlt">sheet</span> on the surface mass balance (SMB) of the Eurasian <span class="hlt">ice</span> <span class="hlt">sheet</span> driven by simulated changes in the past glacial atmospheric circulation. Using the LMDZ5 atmospheric circulation model, we carried out 12 experiments under constant LGM conditions for insolation, greenhouse gases and ocean. In these experiments, the Eurasian <span class="hlt">ice</span> <span class="hlt">sheet</span> is removed. The 12 experiments differ in the North American <span class="hlt">ice-sheet</span> topography, ranging from a white and flat (present-day topography) <span class="hlt">ice</span> <span class="hlt">sheet</span> to a full-size LGM <span class="hlt">ice</span> <span class="hlt">sheet</span>. This experimental design allows the albedo and the topographic impacts of the North American <span class="hlt">ice</span> <span class="hlt">sheet</span> onto the climate to be disentangled. The results are compared to our baseline experiment where both the North American and the Eurasian <span class="hlt">ice</span> <span class="hlt">sheets</span> have been removed. In summer, the sole albedo effect of the American <span class="hlt">ice</span> <span class="hlt">sheet</span> modifies the pattern of planetary waves with respect to the no-<span class="hlt">ice-sheet</span> case, resulting in a cooling of the northwestern Eurasian region. By contrast, the atmospheric circulation changes induced by the topography of the North American <span class="hlt">ice</span> <span class="hlt">sheet</span> lead to a strong decrease of this cooling. In winter, the Scandinavian and the Barents-Kara regions respond differently to the American <span class="hlt">ice-sheet</span> albedo effect: in response to atmospheric circulation changes, Scandinavia becomes warmer and total precipitation is more abundant, whereas the Barents-Kara area becomes cooler with a decrease of convective processes, causing a decrease of total precipitation. The gradual increase of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://rosap.ntl.bts.gov/view/dot/21787','DOTNTL'); return false;" href="https://rosap.ntl.bts.gov/view/dot/21787"><span><span class="hlt">Snow</span> and <span class="hlt">ice</span> control at extreme temperatures.</span></a></p> <p><a target="_blank" href="http://ntlsearch.bts.gov/tris/index.do">DOT National Transportation Integrated Search</a></p> <p></p> <p>2011-04-25</p> <p>As expected, most state and provincial DOTs that we spoke with are using traditional methods to prevent and : remove <span class="hlt">snow</span> and <span class="hlt">ice</span> at very low temperatures. In addition to a review of current research, we spoke with six winter : maintenance profession...</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> <span class="hlt">Sheets</span></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> <span class="hlt">sheets</span> 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> <span class="hlt">sheets</span> 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> <span class="hlt">sheet</span> mass balance and dynamics. In this review, we summarize in situ and satellite-based measurements of the tidal response of <span class="hlt">ice</span> shelves and grounded <span class="hlt">ice</span>, and spatial variability of ocean tide heights and currents around the <span class="hlt">ice</span> <span class="hlt">sheets</span>. We review sensitivity of tide heights and currents as ocean geometry responds to variations in sea level, <span class="hlt">ice</span> shelf thickness, and <span class="hlt">ice</span> <span class="hlt">sheet</span> mass and extent. We then describe coupled <span class="hlt">ice</span>-ocean models and analytical glacier models that quantify the effect of ocean tides on lower-frequency <span class="hlt">ice</span> <span class="hlt">sheet</span> mass loss and motion. We suggest new observations and model developments to improve the representation of tides in coupled models that are used to predict future <span class="hlt">ice</span> <span class="hlt">sheet</span> mass loss and the associated contribution to sea level change. The most critical need is for new data to improve maps of bathymetry, <span class="hlt">ice</span> shelf draft, spatial variability of the drag coefficient at the <span class="hlt">ice</span>-ocean interface, and higher-resolution models with improved representation of tidal energy sinks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.nsf.gov/pubs/2005/nsf0539/nsf0539_5.pdf','USGSPUBS'); return false;" href="http://www.nsf.gov/pubs/2005/nsf0539/nsf0539_5.pdf"><span>Correlated declines in Pacific arctic <span class="hlt">snow</span> and sea <span class="hlt">ice</span> cover</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Stone, Robert P.; Douglas, David C.; Belchansky, Gennady I.; Drobot, Sheldon</p> <p>2005-01-01</p> <p>Simulations of future climate suggest that global warming will reduce Arctic <span class="hlt">snow</span> and <span class="hlt">ice</span> cover, resulting in decreased surface albedo (reflectivity). Lowering of the surface albedo leads to further warming by increasing solar absorption at the surface. This phenomenon is referred to as “temperature–albedo feedback.” Anticipation of such a feedback is one reason why scientists look to the Arctic for early indications of global warming. Much of the Arctic has warmed significantly. Northern Hemisphere <span class="hlt">snow</span> cover has decreased, and sea <span class="hlt">ice</span> has diminished in area and thickness. As reported in the Arctic Climate Impact Assessment in 2004, the trends are considered to be outside the range of natural variability, implicating global warming as an underlying cause. Changing climatic conditions in the high northern latitudes have influenced biogeochemical cycles on a broad scale. Warming has already affected the sea <span class="hlt">ice</span>, the tundra, the plants, the animals, and the indigenous populations that depend on them. Changing annual cycles of <span class="hlt">snow</span> and sea <span class="hlt">ice</span> also affect sources and sinks of important greenhouse gases (such as carbon dioxide and methane), further complicating feedbacks involving the global budgets of these important constituents. For instance, thawing permafrost increases the extent of tundra wetlands and lakes, releasing greater amounts of methane into the atmosphere. Variable sea <span class="hlt">ice</span> cover may affect the hemispheric carbon budget by altering the ocean–atmosphere exchange of carbon dioxide. There is growing concern that amplification of global warming in the Arctic will have far-reaching effects on lower latitude climate through these feedback mechanisms. Despite the diverse and convincing observational evidence that the Arctic environment is changing, it remains unclear whether these changes are anthropogenically forced or result from natural variations of the climate system. A better understanding of what controls the seasonal distributions of <span class="hlt">snow</span> and <span class="hlt">ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27386524','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27386524"><span>Monitoring southwest Greenland's <span class="hlt">ice</span> <span class="hlt">sheet</span> melt with ambient seismic noise.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mordret, Aurélien; Mikesell, T Dylan; Harig, Christopher; Lipovsky, Bradley P; Prieto, Germán A</p> <p>2016-05-01</p> <p>The Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> presently accounts for ~70% of global <span class="hlt">ice</span> <span class="hlt">sheet</span> 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 <span class="hlt">ice</span> <span class="hlt">sheet</span> 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 <span class="hlt">ice</span> <span class="hlt">sheet</span> 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) <span class="hlt">ice</span> <span class="hlt">sheet</span> mass balance, yielding new constraints on <span class="hlt">ice</span> <span class="hlt">sheet</span> evolution and its contribution to global sea-level changes. An increased number of seismic stations in the vicinity of <span class="hlt">ice</span> <span class="hlt">sheets</span> will enhance our ability to create detailed space-time records of <span class="hlt">ice</span> mass variations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4508962','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4508962"><span>Radiostratigraphy and age structure of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>MacGregor, Joseph A; Fahnestock, Mark A; Catania, Ginny A; Paden, John D; Prasad Gogineni, S; Young, S Keith; Rybarski, Susan C; Mabrey, Alexandria N; Wagman, Benjamin M; Morlighem, Mathieu</p> <p>2015-01-01</p> <p>Several decades of <span class="hlt">ice</span>-penetrating radar surveys of the Greenland and Antarctic <span class="hlt">ice</span> <span class="hlt">sheets</span> have observed numerous widespread internal reflections. Analysis of this radiostratigraphy has produced valuable insights into <span class="hlt">ice</span> <span class="hlt">sheet</span> dynamics and motivates additional mapping of these reflections. Here we present a comprehensive deep radiostratigraphy of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> from airborne deep <span class="hlt">ice</span>-penetrating radar data collected over Greenland by The University of Kansas between 1993 and 2013. To map this radiostratigraphy efficiently, we developed new techniques for predicting reflection slope from the phase recorded by coherent radars. When integrated along track, these slope fields predict the radiostratigraphy and simplify semiautomatic reflection tracing. Core-intersecting reflections were dated using synchronized depth-age relationships for six deep <span class="hlt">ice</span> cores. Additional reflections were dated by matching reflections between transects and by extending reflection-inferred depth-age relationships using the local effective vertical strain rate. The oldest reflections, dating to the Eemian period, are found mostly in the northern part of the <span class="hlt">ice</span> <span class="hlt">sheet</span>. Within the onset regions of several fast-flowing outlet glaciers and <span class="hlt">ice</span> streams, reflections typically do not conform to the bed topography. Disrupted radiostratigraphy is also observed in a region north of the Northeast Greenland <span class="hlt">Ice</span> Stream that is not presently flowing rapidly. Dated reflections are used to generate a gridded age volume for most of the <span class="hlt">ice</span> <span class="hlt">sheet</span> and also to determine the depths of key climate transitions that were not observed directly. This radiostratigraphy provides a new constraint on the dynamics and history of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span>. Key Points Phase information predicts reflection slope and simplifies reflection tracing Reflections can be dated away from <span class="hlt">ice</span> cores using a simple <span class="hlt">ice</span> flow model Radiostratigraphy is often disrupted near the onset of fast <span class="hlt">ice</span> flow PMID:26213664</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRC..123.1907W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123.1907W"><span>Estimation of Antarctic Land-Fast Sea <span class="hlt">Ice</span> Algal Biomass and <span class="hlt">Snow</span> Thickness From Under-<span class="hlt">Ice</span> Radiance Spectra in Two Contrasting Areas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wongpan, P.; Meiners, K. M.; Langhorne, P. J.; Heil, P.; Smith, I. J.; Leonard, G. H.; Massom, R. A.; Clementson, L. A.; Haskell, T. G.</p> <p>2018-03-01</p> <p>Fast <span class="hlt">ice</span> is an important component of Antarctic coastal marine ecosystems, providing a prolific habitat for <span class="hlt">ice</span> algal communities. This work examines the relationships between normalized difference indices (NDI) calculated from under-<span class="hlt">ice</span> radiance measurements and sea <span class="hlt">ice</span> algal biomass and <span class="hlt">snow</span> thickness for Antarctic fast <span class="hlt">ice</span>. While this technique has been calibrated to assess biomass in Arctic fast <span class="hlt">ice</span> and pack <span class="hlt">ice</span>, as well as Antarctic pack <span class="hlt">ice</span>, relationships are currently lacking for Antarctic fast <span class="hlt">ice</span> characterized by bottom <span class="hlt">ice</span> algae communities with high algal biomass. We analyze measurements along transects at two contrasting Antarctic fast <span class="hlt">ice</span> sites in terms of platelet <span class="hlt">ice</span> presence: near and distant from an <span class="hlt">ice</span> shelf, i.e., in McMurdo Sound and off Davis Station, respectively. <span class="hlt">Snow</span> and <span class="hlt">ice</span> thickness, and <span class="hlt">ice</span> salinity and temperature measurements support our paired in situ optical and biological measurements. Analyses show that NDI wavelength pairs near the first chlorophyll a (chl a) absorption peak (≈440 nm) explain up to 70% of the total variability in algal biomass. Eighty-eight percent of <span class="hlt">snow</span> thickness variability is explained using an NDI with a wavelength pair of 648 and 567 nm. Accounting for pigment packaging effects by including the ratio of chl a-specific absorption coefficients improved the NDI-based algal biomass estimation only slightly. Our new observation-based algorithms can be used to estimate Antarctic fast <span class="hlt">ice</span> algal biomass and <span class="hlt">snow</span> thickness noninvasively, for example, by using moored sensors (time series) or mapping their spatial distributions using underwater vehicles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeCoA.231....1S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeCoA.231....1S"><span>Distinguishing summertime atmospheric production of nitrate across the East Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shi, G.; Buffen, A. M.; Ma, H.; Hu, Z.; Sun, B.; Li, C.; Yu, J.; Ma, T.; An, C.; Jiang, S.; Li, Y.; Hastings, M. G.</p> <p>2018-06-01</p> <p>Surface <span class="hlt">snow</span> and atmospheric samples collected along a traverse from the coast to the <span class="hlt">ice</span> <span class="hlt">sheet</span> summit (Dome A) are used to investigate summertime atmospheric production of nitrate (NO3-) across East Antarctica. The strong relationship observed between δ15N and δ18O of nitrate in the surface <span class="hlt">snow</span> suggests a large (lesser) extent of nitrate photolysis in the interior (coastal) region. A linear correlation between the oxygen isotopes of nitrate (δ18O and Δ17O) indicates mixing of various oxidants that react with NOx (NOx = NO + NO2) to produce atmospheric nitrate. On the plateau, the isotopes of <span class="hlt">snow</span> nitrate are best explained by local reoxidation chemistry of NOx, possibly occurring in both condensed and gas phases. Nitrate photolysis results in redistribution of <span class="hlt">snow</span> nitrate, and the plateau <span class="hlt">snow</span> is a net exporter of nitrate and its precursors. Our results suggest that while <span class="hlt">snow</span>-sourced NOx from the plateau due to photolysis is a significant input to the nitrate budget in coastal <span class="hlt">snow</span> (up to ∼35%), tropospheric transport from mid-low latitudes dominates (∼65%) coastal <span class="hlt">snow</span> nitrate. The linear relationship of δ18O vs. Δ17O of the <span class="hlt">snow</span> nitrate suggests a predominant role of hydroxyl radical (OH) and ozone (O3) in nitrate production, although a high Δ17O(O3) is required to explain the observations. Across Antarctica the oxygen isotope composition of OH appears to be dominated by exchange with water vapor, despite the very dry environment. One of the largest uncertainties in quantifying nitrate production pathways is the limited knowledge of atmospheric oxidant isotopic compositions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.4266C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.4266C"><span>BRITICE-CHRONO: Constraining rates and style of marine-influenced <span class="hlt">ice</span> <span class="hlt">sheet</span> decay to provide a data-rich playground for <span class="hlt">ice</span> <span class="hlt">sheet</span> modellers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clark, Chris</p> <p>2014-05-01</p> <p>Uncertainty exists regarding the fate of the Antarctic and Greenland <span class="hlt">ice</span> <span class="hlt">sheets</span> and how they will respond to forcings from sea level and atmospheric and ocean temperatures. If we want to know more about the mechanisms and rate of change of shrinking <span class="hlt">ice</span> <span class="hlt">sheets</span>, then why not examine an <span class="hlt">ice</span> <span class="hlt">sheet</span> that has fully disappeared and track its retreat through time? If achieved in enough detail such information could become a data-rich playground for improving the next breed of numerical <span class="hlt">ice</span> <span class="hlt">sheet</span> models to be used in <span class="hlt">ice</span> and sea level forecasting. We regard that the last British-Irish <span class="hlt">Ice</span> <span class="hlt">Sheet</span> is a good target for this work, on account of its small size, density of information and with its numerous researchers already investigating it. BRITICE-CHRONO is a large (>45 researchers) NERC-funded consortium project comprising Quaternary scientists and glaciologists who will search the seafloor around Britain and Ireland and parts of the landmass in order to find and extract samples of sand, rock and organic matter that can be dated (OSL; Cosmogenic; 14C) to reveal the timing and rate of change of the collapsing British-Irish <span class="hlt">Ice</span> <span class="hlt">Sheet</span>. The purpose is to produce a high resolution dataset on the demise on an <span class="hlt">ice</span> <span class="hlt">sheet</span> - from the continental shelf edge and across the marine to terrestrial transition. Some 800 new date assessments will be added to those that already exist. This poster reports on the hypotheses that underpin the work. Data on retreat will be collected by focusing on 8 transects running from the continental shelf edge to a short distance (10s km) onshore and acquiring marine and terrestrial samples for geochronometric dating. The project includes funding for 587 radiocarbon, 140 OSL and 158 TCN samples for surface exposure dating; with sampling accomplished by two research cruises and 16 fieldwork campaigns. Results will reveal the timing and rate of change of <span class="hlt">ice</span> margin recession for each transect, and combined with existing landform and dating databases, will be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4987822','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4987822"><span>Stochastic <span class="hlt">ice</span> stream dynamics</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Bertagni, Matteo Bernard; Ridolfi, Luca</p> <p>2016-01-01</p> <p><span class="hlt">Ice</span> streams are narrow corridors of fast-flowing <span class="hlt">ice</span> that constitute the arterial drainage network of <span class="hlt">ice</span> <span class="hlt">sheets</span>. Therefore, changes in <span class="hlt">ice</span> stream flow are key to understanding paleoclimate, sea level changes, and rapid disintegration of <span class="hlt">ice</span> <span class="hlt">sheets</span> during deglaciation. The dynamics of <span class="hlt">ice</span> flow are tightly coupled to the climate system through atmospheric temperature and <span class="hlt">snow</span> recharge, which are known exhibit stochastic variability. Here we focus on the interplay between stochastic climate forcing and <span class="hlt">ice</span> stream temporal dynamics. Our work demonstrates that realistic climate fluctuations are able to (i) induce the coexistence of dynamic behaviors that would be incompatible in a purely deterministic system and (ii) drive <span class="hlt">ice</span> stream flow away from the regime expected in a steady climate. We conclude that environmental noise appears to be crucial to interpreting the past behavior of <span class="hlt">ice</span> <span class="hlt">sheets</span>, as well as to predicting their future evolution. PMID:27457960</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_14 --> <div id="page_15" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="281"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1810332R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1810332R"><span>Trends in annual minimum exposed <span class="hlt">snow</span> and <span class="hlt">ice</span> cover in High Mountain Asia from MODIS</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rittger, Karl; Brodzik, Mary J.; Painter, Thomas H.; Racoviteanu, Adina; Armstrong, Richard; Dozier, Jeff</p> <p>2016-04-01</p> <p>Though a relatively short record on climatological scales, data from the Moderate Resolution Imaging Spectroradiometer (MODIS) from 2000-2014 can be used to evaluate changes in the cryosphere and provide a robust baseline for future observations from space. We use the MODIS <span class="hlt">Snow</span> Covered Area and Grain size (MODSCAG) algorithm, based on spectral mixture analysis, to estimate daily fractional <span class="hlt">snow</span> and <span class="hlt">ice</span> cover and the MODICE Persistent <span class="hlt">Ice</span> (MODICE) algorithm to estimate the annual minimum <span class="hlt">snow</span> and <span class="hlt">ice</span> fraction (fSCA) for each year from 2000 to 2014 in High Mountain Asia. We have found that MODSCAG performs better than other algorithms, such as the Normalized Difference Index (NDSI), at detecting <span class="hlt">snow</span>. We use MODICE because it minimizes false positives (compared to maximum extents), for example, when bright soils or clouds are incorrectly classified as <span class="hlt">snow</span>, a common problem with optical satellite <span class="hlt">snow</span> mapping. We analyze changes in area using the annual MODICE maps of minimum <span class="hlt">snow</span> and <span class="hlt">ice</span> cover for over 15,000 individual glaciers as defined by the Randolph Glacier Inventory (RGI) Version 5, focusing on the Amu Darya, Syr Darya, Upper Indus, Ganges, and Brahmaputra River basins. For each glacier with an area of at least 1 km2 as defined by RGI, we sum the total minimum <span class="hlt">snow</span> and <span class="hlt">ice</span> covered area for each year from 2000 to 2014 and estimate the trends in area loss or gain. We find the largest loss in annual minimum <span class="hlt">snow</span> and <span class="hlt">ice</span> extent for 2000-2014 in the Brahmaputra and Ganges with 57% and 40%, respectively, of analyzed glaciers with significant losses (p-value<0.05). In the Upper Indus River basin, we see both gains and losses in minimum <span class="hlt">snow</span> and <span class="hlt">ice</span> extent, but more glaciers with losses than gains. Our analysis shows that a smaller proportion of glaciers in the Amu Darya and Syr Darya are experiencing significant changes in minimum <span class="hlt">snow</span> and <span class="hlt">ice</span> extent (3.5% and 12.2%), possibly because more of the glaciers in this region are smaller than 1 km2 than in the Indus</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JAMES...9..854K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JAMES...9..854K"><span>LIVVkit: An extensible, python-based, land <span class="hlt">ice</span> verification and validation toolkit for <span class="hlt">ice</span> <span class="hlt">sheet</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>Kennedy, Joseph H.; Bennett, Andrew R.; Evans, Katherine J.; Price, Stephen; Hoffman, Matthew; Lipscomb, William H.; Fyke, Jeremy; Vargo, Lauren; Boghozian, Adrianna; Norman, Matthew; Worley, Patrick H.</p> <p>2017-06-01</p> <p>To address the pressing need to better understand the behavior and complex interaction of <span class="hlt">ice</span> <span class="hlt">sheets</span> within the global Earth system, significant development of continental-scale, dynamical <span class="hlt">ice</span> <span class="hlt">sheet</span> models is underway. Concurrent to the development of the Community <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model (CISM), the corresponding verification and validation (V&V) process is being coordinated through a new, robust, Python-based extensible software package, the Land <span class="hlt">Ice</span> Verification and Validation toolkit (LIVVkit). Incorporated into the typical <span class="hlt">ice</span> <span class="hlt">sheet</span> model development cycle, it provides robust and automated numerical verification, software verification, performance validation, and physical validation analyses on a variety of platforms, from personal laptops to the largest supercomputers. LIVVkit operates on sets of regression test and reference data sets, and provides comparisons for a suite of community prioritized tests, including configuration and parameter variations, bit-for-bit evaluation, and plots of model variables to indicate where differences occur. LIVVkit also provides an easily extensible framework to incorporate and analyze results of new intercomparison projects, new observation data, and new computing platforms. LIVVkit is designed for quick adaptation to additional <span class="hlt">ice</span> <span class="hlt">sheet</span> models via abstraction of model specific code, functions, and configurations into an <span class="hlt">ice</span> <span class="hlt">sheet</span> model description bundle outside the main LIVVkit structure. Ultimately, through shareable and accessible analysis output, LIVVkit is intended to help developers build confidence in their models and enhance the credibility of <span class="hlt">ice</span> <span class="hlt">sheet</span> models overall.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C41D0740M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C41D0740M"><span>Shape-from-shading using Landsat 8 and airborne laser altimetry over <span class="hlt">ice</span> <span class="hlt">sheets</span>: toward new regional DEMs of Greenland and Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moussavi, M. S.; Scambos, T.; Haran, T. M.; Klinger, M. J.; Abdalati, W.</p> <p>2015-12-01</p> <p>We investigate the capability of Landsat 8's Operational Land Imager (OLI) instrument to quantify subtle <span class="hlt">ice</span> <span class="hlt">sheet</span> topography of Greenland and Antarctica. We use photoclinometry, or 'shape-from-shading', a method of deriving surface topography from local variations in image brightness due to varying surface slope. Photoclinomeetry is applicable over <span class="hlt">ice</span> <span class="hlt">sheet</span> areas with highly uniform albedo such as regions covered by recent snowfall. OLI imagery is available from both ascending and descending passes near the summer solstice period for both <span class="hlt">ice</span> <span class="hlt">sheets</span>. This provides two views of the surface features from two distinct solar azimuth illumination directions. Airborne laser altimetry data from the Airborne Topographic Mapper (ATM) instrument (flying on the Operation <span class="hlt">Ice</span> Bridge program) are used to quantitatively convert the image brightness variations of surface undulations to surface slope. To validate the new DEM products, we use additional laser altimetry profiles collected over independent sites from <span class="hlt">Ice</span> Bridge and ICESat, and high-resolution WorldView-2 DEMs. The photoclinometry-derived DEM products will be useful for studying surface elevation changes, enhancing bedrock elevation maps through inversion of surface topography, and inferring local variations in <span class="hlt">snow</span> accumulation rates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120009085','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120009085"><span>Modeling of Firn Compaction for Estimating <span class="hlt">Ice-Sheet</span> Mass Change from Observed <span class="hlt">Ice-Sheet</span> Elevation Change</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Li, Jun; Zwally, H. Jay</p> <p>2011-01-01</p> <p>Changes in <span class="hlt">ice-sheet</span> surface elevation are caused by a combination of <span class="hlt">ice</span>-dynamic imbalance, ablation, temporal variations in accumulation rate, firn compaction and underlying bedrock motion. Thus, deriving the rate of <span class="hlt">ice-sheet</span> 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 <span class="hlt">ice</span> <span class="hlt">sheet</span> in order to separate the accumulation-driven changes from the <span class="hlt">ice</span>-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.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/14699053','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/14699053"><span>Soot climate forcing via <span class="hlt">snow</span> and <span class="hlt">ice</span> albedos.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hansen, James; Nazarenko, Larissa</p> <p>2004-01-13</p> <p>Plausible estimates for the effect of soot on <span class="hlt">snow</span> and <span class="hlt">ice</span> albedos (1.5% in the Arctic and 3% in Northern Hemisphere land areas) yield a climate forcing of +0.3 W/m(2) in the Northern Hemisphere. The "efficacy" of this forcing is approximately 2, i.e., for a given forcing it is twice as effective as CO(2) in altering global surface air temperature. This indirect soot forcing may have contributed to global warming of the past century, including the trend toward early springs in the Northern Hemisphere, thinning Arctic sea <span class="hlt">ice</span>, and melting land <span class="hlt">ice</span> and permafrost. If, as we suggest, melting <span class="hlt">ice</span> and sea level rise define the level of dangerous anthropogenic interference with the climate system, then reducing soot emissions, thus restoring <span class="hlt">snow</span> albedos to pristine high values, would have the double benefit of reducing global warming and raising the global temperature level at which dangerous anthropogenic interference occurs. However, soot contributions to climate change do not alter the conclusion that anthropogenic greenhouse gases have been the main cause of recent global warming and will be the predominant climate forcing in the future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C31A..06R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C31A..06R"><span>The impact of the <span class="hlt">snow</span> cover on sea-<span class="hlt">ice</span> thickness products retrieved by Ku-band radar altimeters</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ricker, R.; Hendricks, S.; Helm, V.; Perovich, D. K.</p> <p>2015-12-01</p> <p><span class="hlt">Snow</span> on sea <span class="hlt">ice</span> is a relevant polar climate parameter related to ocean-atmospheric interactions and surface albedo. It also remains an important factor for sea-<span class="hlt">ice</span> thickness products retrieved from Ku-band satellite radar altimeters like Envisat or CryoSat-2, which is currently on its mission and the subject of many recent studies. Such satellites sense the height of the sea-<span class="hlt">ice</span> surface above the sea level, which is called sea-<span class="hlt">ice</span> freeboard. By assuming hydrostatic equilibrium and that the main scattering horizon is given by the <span class="hlt">snow-ice</span> interface, the freeboard can be transformed into sea-<span class="hlt">ice</span> thickness. Therefore, information about the <span class="hlt">snow</span> load on hemispherical scale is crucial. Due to the lack of sufficient satellite products, only climatological values are used in current studies. Since such values do not represent the high variability of <span class="hlt">snow</span> distribution in the Arctic, they can be a substantial contributor to the total sea-<span class="hlt">ice</span> thickness uncertainty budget. Secondly, recent studies suggest that the <span class="hlt">snow</span> layer cannot be considered as homogenous, but possibly rather featuring a complex stratigraphy due to wind compaction and/or <span class="hlt">ice</span> lenses. Therefore, the Ku-band radar signal can be scattered at internal layers, causing a shift of the main scattering horizon towards the <span class="hlt">snow</span> surface. This alters the freeboard and thickness retrieval as the assumption that the main scattering horizon is given by the <span class="hlt">snow-ice</span> interface is no longer valid and introduces a bias. Here, we present estimates for the impact of <span class="hlt">snow</span> depth uncertainties and <span class="hlt">snow</span> properties on CryoSat-2 sea-<span class="hlt">ice</span> thickness retrievals. We therefore compare CryoSat-2 freeboard measurements with field data from <span class="hlt">ice</span> mass-balance buoys and aircraft campaigns from the CryoSat Validation Experiment. This unique validation dataset includes airborne laser scanner and radar altimeter measurements in spring coincident to CryoSat-2 overflights, and allows us to evaluate how the main scattering horizon is altered by the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.C41D0434C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.C41D0434C"><span><span class="hlt">Ice</span> <span class="hlt">Sheet</span> and Sea <span class="hlt">Ice</span> Observations from Unmanned Aircraft Systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Crocker, R. I.; Maslanik, J. A.</p> <p>2011-12-01</p> <p>A suite of sensors has been assembled to map <span class="hlt">ice</span> <span class="hlt">sheet</span> and sea <span class="hlt">ice</span> surface topography with fine-resolution from small unmanned aircraft systems (UAS). This payload is optimized to provide coincident surface elevation and imagery data, and with its low cost and ease of reproduction, it has the potential to become a widely-distributed observational resource to complement polar manned-aircraft and satellite missions. To date, it has been deployed to map <span class="hlt">ice</span> <span class="hlt">sheet</span> elevations near Jakobshavn Isbræ in Greenland, and to measure sea <span class="hlt">ice</span> freeboard and roughness in Fram Strait off the coast of Svalbard. Data collected during these campaigns have facilitate a detailed assessment of the system's surface elevation measurement accuracy, and provide a glimpse of the summer 2009 Fram Strait sea <span class="hlt">ice</span> conditions. These findings are presented, along with a brief overview of our future Arctic UAS operations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150021875','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150021875"><span>ISMIP6: <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model Intercomparison Project for CMIP6</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nowicki, S.</p> <p>2015-01-01</p> <p>ISMIP6 (<span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model Intercomparison Project for CMIP6) targets the Cryosphere in a Changing Climate and the Future Sea Level Grand Challenges of the WCRP (World Climate Research Program). Primary goal is to provide future sea level contribution from the Greenland and Antarctic <span class="hlt">ice</span> <span class="hlt">sheets</span>, along with associated uncertainty. Secondary goal is to investigate feedback due to dynamic <span class="hlt">ice</span> <span class="hlt">sheet</span> models. Experiment design uses and augment the existing CMIP6 (Coupled Model Intercomparison Project Phase 6) DECK (Diagnosis, Evaluation, and Characterization of Klima) experiments. Additonal MIP (Model Intercomparison Project)- specific experiments will be designed for ISM (<span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model). Effort builds on the <span class="hlt">Ice</span>2sea, SeaRISE (Sea-level Response to <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Evolution) and COMBINE (Comprehensive Modelling of the Earth System for Better Climate Prediction and Projection) efforts.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C21D1150M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C21D1150M"><span>Improved climate model evaluation using a new, 750-year Antarctic-wide <span class="hlt">snow</span> accumulation product</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Medley, B.; Thomas, E. R.</p> <p>2017-12-01</p> <p><span class="hlt">Snow</span> that accumulates over the cold, dry grounded <span class="hlt">ice</span> of Antarctica is an important component of its mass balance, mitigating the <span class="hlt">ice</span> <span class="hlt">sheet</span>'s contribution to sea level. Secular trends in accumulation not only result trends in the mass balance of the Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span>, but also directly and indirectly impact surface height changes. Long-term and spatiotemporally complete records of <span class="hlt">snow</span> accumulation are needed to understand part and present Antarctic-wide mass balance, to convert from altimetry derived volume change to mass change, and to evaluate the ability of climate models to reproduce the observed climate change. We need measurements in both time and space, yet they typically sample one dimension at the expense of the other. Here, we develop a spatially complete, annually resolved <span class="hlt">snow</span> accumulation product for the Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> over the past 750 years by combining a newly compiled database of <span class="hlt">ice</span> core accumulation records with climate model output. We mainly focus on climate model evaluation. Because the product spans several centuries, we can evaluate model ability in representing the preindustrial as well as present day accumulation change. Significant long-term trends in <span class="hlt">snow</span> accumulation are found over the Ross and Bellingshausen Sea sectors of West Antarctica, the Antarctic Peninsula, and several sectors in East Antarctica. These results suggest that change is more complex over the Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> than a simple uniform change (i.e., more snowfall in a warming world), which highlights the importance of atmospheric circulation as a major driver of change. By evaluating several climate models' ability to reproduce the observed trends, we can deduce whether their projections are reasonable or potentially biased where the latter would result in a misrepresentation of the Antarctic contribution to sea level.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C11E..05F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C11E..05F"><span>Eastern Ross <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Deglacial History inferred from the Roosevelt Island <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>Fudge, T. J.; Buizert, C.; Lee, J.; Waddington, E. D.; Bertler, N. A. N.; Conway, H.; Brook, E.; Severinghaus, J. P.</p> <p>2017-12-01</p> <p>The Ross <span class="hlt">Ice</span> <span class="hlt">Sheet</span> drains large portions of both West and East Antarctica. Understanding the retreat of the Ross <span class="hlt">Ice</span> <span class="hlt">Sheet</span> following the Last Glacial Maximum is particularly difficult in the eastern Ross area where there is no exposed rock and the Ross <span class="hlt">Ice</span> Shelf prevents extensive bathymetric mapping. Coastal domes, by preserving old <span class="hlt">ice</span>, can be used to infer the establishment of grounded <span class="hlt">ice</span> and be used to infer past <span class="hlt">ice</span> thickness. Here we focus on Roosevelt Island, in the eastern Ross Sea, where the Roosevelt Island Climate Evolution project recently completed an <span class="hlt">ice</span> core to bedrock. Using <span class="hlt">ice</span>-flow modeling constrained by the depth-age relationship and an independent estimate of accumulation rate from firn-densification measurements and modeling, we infer <span class="hlt">ice</span> thickness histories for the LGM (20ka) to present. Preliminary results indicate thinning of 300m between 15ka and 12ka is required. This is similar to the amount and timing of thinning inferred at Siple Dome, in the central Ross Sea (Waddington et al., 2005; Price et al., 2007) and supports the presence of active <span class="hlt">ice</span> streams throughout the Ross <span class="hlt">Ice</span> <span class="hlt">Sheet</span> advance during the LGM.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16782602','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16782602"><span>Geological and geomorphological insights into Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> evolution.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sugden, David E; Bentley, Michael J; O Cofaigh, Colm</p> <p>2006-07-15</p> <p>Technical advances in the study of <span class="hlt">ice</span>-free parts of Antarctica can provide quantitative records that are useful for constraining and refining models of <span class="hlt">ice</span> <span class="hlt">sheet</span> evolution and behaviour. Such records improve our understanding of system trajectory, influence the questions we ask about system stability and help to define the <span class="hlt">ice-sheet</span> processes that are relevant on different time-scales. Here, we illustrate the contribution of cosmogenic isotope analysis of exposed bedrock surfaces and marine geophysical surveying to the understanding of Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> evolution on a range of time-scales. In the Dry Valleys of East Antarctica, 3He dating of subglacial flood deposits that are now exposed on mountain summits provide evidence of an expanded and thicker Mid-Miocene <span class="hlt">ice</span> <span class="hlt">sheet</span>. The survival of surface boulders for approximately 14Myr, the oldest yet measured, demonstrates exceptionally low rates of subsequent erosion and points to the persistence and stability of the dry polar desert climate since that time. Increasingly, there are constraints on West Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> fluctuations during Quaternary glacial cycles. In the Sarnoff Mountains of Marie Byrd Land in West Antarctica, 10Be and 26Al cosmogenic isotope analysis of glacial erratics and bedrock reveal steady thinning of the <span class="hlt">ice</span> <span class="hlt">sheet</span> from 10400 years ago to the present, probably as a result of grounding line retreat. In the Antarctic Peninsula, offshore analysis reveals an extensive <span class="hlt">ice</span> <span class="hlt">sheet</span> at the last glacial maximum. Based on radiocarbon dating, deglaciation began by 17000cal yr BP and was complete by 9500cal yr BP. Deglaciation of the west and east sides of the Antarctic Peninsula <span class="hlt">ice</span> <span class="hlt">sheet</span> occurred at different times and rates, but was largely complete by the Early Holocene. At that time <span class="hlt">ice</span> shelves were less extensive on the west side of the Antarctic Peninsula than they are today. The message from the past is that individual glacier drainage basins in Antarctica respond in different and distinctive</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70186956','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70186956"><span><span class="hlt">Snow</span> and <span class="hlt">ice</span> perturbation during historical volcanic eruptions and the formation of lahars and floods</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Major, Jon J.; Newhall, Christopher G.</p> <p>1989-01-01</p> <p>Historical eruptions have produced lahars and floods by perturbing <span class="hlt">snow</span> and <span class="hlt">ice</span> at more than 40 volcanoes worldwide. Most of these volcanoes are located at latitudes higher than 35°; those at lower latitudes reach altitudes generally above 4000 m. Volcanic events can perturb mantles of <span class="hlt">snow</span> and <span class="hlt">ice</span> in at least five ways: (1) scouring and melting by flowing pyroclastic debris or blasts of hot gases and pyroclastic debris, (2) surficial melting by lava flows, (3) basal melting of glacial <span class="hlt">ice</span> or <span class="hlt">snow</span> by subglacial eruptions or geothermal activity, (4) ejection of water by eruptions through a crater lake, and (5) deposition of tephra fall. Historical records of volcanic eruptions at <span class="hlt">snow</span>-clad volcanoes show the following: (1) Flowing pyroclastic debris (pyroclastic flows and surges) and blasts of hot gases and pyroclastic debris are the most common volcanic events that generate lahars and floods; (2) Surficial lava flows generally cannot melt <span class="hlt">snow</span> and <span class="hlt">ice</span> rapidly enough to form large lahars or floods; (3) Heating the base of a glacier or snowpack by subglacial eruptions or by geothermal activity can induce basal melting that may result in ponding of water and lead to sudden outpourings of water or sediment-rich debris flows; (4) Tephra falls usually alter ablation rates of <span class="hlt">snow</span> and <span class="hlt">ice</span> but generally produce little meltwater that results in the formation of lahars and floods; (5) Lahars and floods generated by flowing pyroclastic debris, blasts of hot gases and pyroclastic debris, or basal melting of <span class="hlt">snow</span> and <span class="hlt">ice</span> commonly have volumes that exceed 105 m3.The glowing lava (pyroclastic flow) which flowed with force over ravines and ridges...gathered in the basin quickly and then forced downwards. As a result, tremendously wide and deep pathways in the <span class="hlt">ice</span> and <span class="hlt">snow</span> were made and produced great streams of water (Wolf 1878).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1989BVol...52....1M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1989BVol...52....1M"><span><span class="hlt">Snow</span> and <span class="hlt">ice</span> perturbation during historical volcanic eruptions and the formation of lahars and floods</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Major, Jon J.; Newhall, Christopher G.</p> <p>1989-10-01</p> <p>Historical eruptions have produced lahars and floods by perturbing <span class="hlt">snow</span> and <span class="hlt">ice</span> at more than 40 volcanoes worldwide. Most of these volcanoes are located at latitudes higher than 35°; those at lower latitudes reach altitudes generally above 4000 m. Volcanic events can perturb mantles of <span class="hlt">snow</span> and <span class="hlt">ice</span> in at least five ways: (1) scouring and melting by flowing pyroclastic debris or blasts of hot gases and pyroclastic debris, (2) surficial melting by lava flows, (3) basal melting of glacial <span class="hlt">ice</span> or <span class="hlt">snow</span> by subglacial eruptions or geothermal activity, (4) ejection of water by eruptions through a crater lake, and (5) deposition of tephra fall. Historical records of volcanic eruptions at <span class="hlt">snow</span>-clad volcanoes show the following: (1) Flowing pyroclastic debris (pyroclastic flows and surges) and blasts of hot gases and pyroclastic debris are the most common volcanic events that generate lahars and floods; (2) Surficial lava flows generally cannot melt <span class="hlt">snow</span> and <span class="hlt">ice</span> rapidly enough to form large lahars or floods; (3) Heating the base of a glacier or snowpack by subglacial eruptions or by geothermal activity can induce basal melting that may result in ponding of water and lead to sudden outpourings of water or sediment-rich debris flows; (4) Tephra falls usually alter ablation rates of <span class="hlt">snow</span> and <span class="hlt">ice</span> but generally produce little meltwater that results in the formation of lahars and floods; (5) Lahars and floods generated by flowing pyroclastic debris, blasts of hot gases and pyroclastic debris, or basal melting of <span class="hlt">snow</span> and <span class="hlt">ice</span> commonly have volumes that exceed 105 m3. The glowing lava (pyroclastic flow) which flowed with force over ravines and ridges...gathered in the basin quickly and then forced downwards. As a result, tremendously wide and deep pathways in the <span class="hlt">ice</span> and <span class="hlt">snow</span> were made and produced great streams of water (Wolf 1878).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70148418','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70148418"><span>Radar attenuation and temperature within the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>MacGregor, Joseph A; Li, Jilu; Paden, John D; Catania, Ginny A; Clow, Gary D.; Fahnestock, Mark A; Gogineni, Prasad S.; Grimm, Robert E.; Morlighem, Mathieu; Nandi, Soumyaroop; Seroussi, Helene; Stillman, David E</p> <p>2015-01-01</p> <p>The flow of <span class="hlt">ice</span> is temperature-dependent, but direct measurements of englacial temperature are sparse. The dielectric attenuation of radio waves through <span class="hlt">ice</span> is also temperature-dependent, and radar sounding of <span class="hlt">ice</span> <span class="hlt">sheets</span> is sensitive to this attenuation. Here we estimate depth-averaged radar-attenuation rates within the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> from airborne radar-sounding data and its associated radiostratigraphy. Using existing empirical relationships between temperature, chemistry, and radar attenuation, we then infer the depth-averaged englacial temperature. The dated radiostratigraphy permits a correction for the confounding effect of spatially varying <span class="hlt">ice</span> chemistry. Where radar transects intersect boreholes, radar-inferred temperature is consistently higher than that measured directly. We attribute this discrepancy to the poorly recognized frequency dependence of the radar-attenuation rate and correct for this effect empirically, resulting in a robust relationship between radar-inferred and borehole-measured depth-averaged temperature. Radar-inferred englacial temperature is often lower than modern surface temperature and that of a steady state <span class="hlt">ice-sheet</span> model, particularly in southern Greenland. This pattern suggests that past changes in surface boundary conditions (temperature and accumulation rate) affect the <span class="hlt">ice</span> <span class="hlt">sheet</span>'s present temperature structure over a much larger area than previously recognized. This radar-inferred temperature structure provides a new constraint for thermomechanical models of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013TCry....7.1161B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013TCry....7.1161B"><span>Data assimilation and prognostic whole <span class="hlt">ice</span> <span class="hlt">sheet</span> modelling with the variationally derived, higher order, open source, and fully parallel <span class="hlt">ice</span> <span class="hlt">sheet</span> model VarGlaS</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brinkerhoff, D. J.; Johnson, J. V.</p> <p>2013-07-01</p> <p>We introduce a novel, higher order, finite element <span class="hlt">ice</span> <span class="hlt">sheet</span> model called VarGlaS (Variational Glacier Simulator), which is built on the finite element framework FEniCS. Contrary to standard procedure in <span class="hlt">ice</span> <span class="hlt">sheet</span> modelling, VarGlaS formulates <span class="hlt">ice</span> <span class="hlt">sheet</span> motion as the minimization of an energy functional, conferring advantages such as a consistent platform for making numerical approximations, a coherent relationship between motion and heat generation, and implicit boundary treatment. VarGlaS also solves the equations of enthalpy rather than temperature, avoiding the solution of a contact problem. Rather than include a lengthy model spin-up procedure, VarGlaS possesses an automated framework for model inversion. These capabilities are brought to bear on several benchmark problems in <span class="hlt">ice</span> <span class="hlt">sheet</span> modelling, as well as a 500 yr simulation of the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> at high resolution. VarGlaS performs well in benchmarking experiments and, given a constant climate and a 100 yr relaxation period, predicts a mass evolution of the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> that matches present-day observations of mass loss. VarGlaS predicts a thinning in the interior and thickening of the margins of the <span class="hlt">ice</span> <span class="hlt">sheet</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=igneous+AND+rock&pg=2&id=EJ275135','ERIC'); return false;" href="https://eric.ed.gov/?q=igneous+AND+rock&pg=2&id=EJ275135"><span>Winter <span class="hlt">Ice</span> and <span class="hlt">Snow</span> as Models of Igneous Rock Formation.</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>Romey, William D.</p> <p>1983-01-01</p> <p>Examines some features of <span class="hlt">ice</span> and <span class="hlt">snow</span> that offer teachers and researchers help in understanding many aspects of igneous processes and configurations. Careful observation of such processes as melting, decay, evolution, and <span class="hlt">snow</span> accumulation provide important clues to understanding processes by which many kinds of rocks form. (Author/JN)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.2523T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.2523T"><span>Current and future darkening of the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tedesco, Marco; Stroeve, Julienne; Fettweis, Xavier; Warren, Stephen; Doherty, Sarah; Noble, Erik; Alexander, Patrick</p> <p>2015-04-01</p> <p>Surface melting over the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> (GIS) promotes <span class="hlt">snow</span> grains growth, reducing albedo and further enhancing melting through the increased amount of absorbed solar radiation. Using a combination of remote sensing data and outputs of a regional climate model, we show that albedo over the GIS decreased significantly from 1996 to 2012. Further, we show that most of this darkening can be accounted for by enhanced <span class="hlt">snow</span> grain growth and the expansion of areas where bare <span class="hlt">ice</span> is exposed, both of which are driven by increases in <span class="hlt">snow</span> warming. An analysis of the impact of light-absorbing impurities on albedo trends detected from spaceborne measurements was inconclusive because the estimated impact for concentrations of impurities of order of magnitude found in Greenland is within the albedo uncertainty retrievable from space-based instruments. However, neither models nor observations show an increase in pollutants (black carbon and associated organics) in the atmosphere over the GIS in this time period. Additionally, we could not identify trends in the number of fires over North America and Russia, assumed to be among the sources of soot for Greenland. We did find that a 'dark band' of tilted <span class="hlt">ice</span> plays a crucial role in decreasing albedo along the west margin, and there is some indication that dust deposition to the GIS may be decreasing albedo in this region but this is not conclusive. In addition to looking at the direct impact of impurities on albedo, we estimated the impact of impurities on albedo via their influence on grain growth and found it is relatively small (~ 1- 2 %), though more sophisticated analysis needs to be carried out. Projections obtained under different warming scenarios consistently point to a continued darkening, with anomalies in albedo driven solely by the effects of climate warming of as much as -0.12 along the west margin of the GIS by the end of this century (with respect to year 2000). Projected darkening is likely underestimated</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1352451-livvkit-extensible-python-based-land-ice-verification-validation-toolkit-ice-sheet-models','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1352451-livvkit-extensible-python-based-land-ice-verification-validation-toolkit-ice-sheet-models"><span>LIVVkit: An extensible, python-based, land <span class="hlt">ice</span> verification and validation toolkit for <span class="hlt">ice</span> <span class="hlt">sheet</span> models</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Kennedy, Joseph H.; Bennett, Andrew R.; Evans, Katherine J.</p> <p></p> <p>To address the pressing need to better understand the behavior and complex interaction of <span class="hlt">ice</span> <span class="hlt">sheets</span> within the global Earth system, significant development of continental-scale, dynamical <span class="hlt">ice</span> <span class="hlt">sheet</span> models is underway. Concurrent to the development of the Community <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model (CISM), the corresponding verification and validation (V&V) process is being coordinated through a new, robust, Python-based extensible software package, the Land <span class="hlt">Ice</span> Verification and Validation toolkit (LIVVkit). Incorporated into the typical <span class="hlt">ice</span> <span class="hlt">sheet</span> model development cycle, it provides robust and automated numerical verification, software verification, performance validation, and physical validation analyses on a variety of platforms, from personal laptopsmore » to the largest supercomputers. LIVVkit operates on sets of regression test and reference data sets, and provides comparisons for a suite of community prioritized tests, including configuration and parameter variations, bit-for-bit evaluation, and plots of model variables to indicate where differences occur. LIVVkit also provides an easily extensible framework to incorporate and analyze results of new intercomparison projects, new observation data, and new computing platforms. LIVVkit is designed for quick adaptation to additional <span class="hlt">ice</span> <span class="hlt">sheet</span> models via abstraction of model specific code, functions, and configurations into an <span class="hlt">ice</span> <span class="hlt">sheet</span> model description bundle outside the main LIVVkit structure. Furthermore, through shareable and accessible analysis output, LIVVkit is intended to help developers build confidence in their models and enhance the credibility of <span class="hlt">ice</span> <span class="hlt">sheet</span> models overall.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1352451-livvkit-extensible-python-based-land-ice-verification-validation-toolkit-ice-sheet-models','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1352451-livvkit-extensible-python-based-land-ice-verification-validation-toolkit-ice-sheet-models"><span>LIVVkit: An extensible, python-based, land <span class="hlt">ice</span> verification and validation toolkit for <span class="hlt">ice</span> <span class="hlt">sheet</span> models</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Kennedy, Joseph H.; Bennett, Andrew R.; Evans, Katherine J.; ...</p> <p>2017-03-23</p> <p>To address the pressing need to better understand the behavior and complex interaction of <span class="hlt">ice</span> <span class="hlt">sheets</span> within the global Earth system, significant development of continental-scale, dynamical <span class="hlt">ice</span> <span class="hlt">sheet</span> models is underway. Concurrent to the development of the Community <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model (CISM), the corresponding verification and validation (V&V) process is being coordinated through a new, robust, Python-based extensible software package, the Land <span class="hlt">Ice</span> Verification and Validation toolkit (LIVVkit). Incorporated into the typical <span class="hlt">ice</span> <span class="hlt">sheet</span> model development cycle, it provides robust and automated numerical verification, software verification, performance validation, and physical validation analyses on a variety of platforms, from personal laptopsmore » to the largest supercomputers. LIVVkit operates on sets of regression test and reference data sets, and provides comparisons for a suite of community prioritized tests, including configuration and parameter variations, bit-for-bit evaluation, and plots of model variables to indicate where differences occur. LIVVkit also provides an easily extensible framework to incorporate and analyze results of new intercomparison projects, new observation data, and new computing platforms. LIVVkit is designed for quick adaptation to additional <span class="hlt">ice</span> <span class="hlt">sheet</span> models via abstraction of model specific code, functions, and configurations into an <span class="hlt">ice</span> <span class="hlt">sheet</span> model description bundle outside the main LIVVkit structure. Furthermore, through shareable and accessible analysis output, LIVVkit is intended to help developers build confidence in their models and enhance the credibility of <span class="hlt">ice</span> <span class="hlt">sheet</span> models overall.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2011-02-09/pdf/2011-2837.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2011-02-09/pdf/2011-2837.pdf"><span>76 FR 7238 - Pipeline Safety: Dangers of Abnormal <span class="hlt">Snow</span> and <span class="hlt">Ice</span> Build-Up on Gas Distribution Systems</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2011-02-09</p> <p>... been related to either the stress of <span class="hlt">snow</span> and <span class="hlt">ice</span> or the malfunction of pressure control equipment due... to have been related to either the stress of <span class="hlt">snow</span> and <span class="hlt">ice</span> or malfunction of pressure control... from the stresses imposed by the additional loading of the <span class="hlt">snow</span> or <span class="hlt">ice</span>. Damage to facilities may also...</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.osti.gov/biblio/984088-modeling-fracture-ice-sheets-parallel-computers','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/984088-modeling-fracture-ice-sheets-parallel-computers"><span>Modeling the fracture of <span class="hlt">ice</span> <span class="hlt">sheets</span> on parallel computers.</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Waisman, Haim; Bell, Robin; Keyes, David</p> <p>2010-03-01</p> <p>The objective of this project is to investigate the complex fracture of <span class="hlt">ice</span> and understand its role within larger <span class="hlt">ice</span> <span class="hlt">sheet</span> simulations and global climate change. At the present time, <span class="hlt">ice</span> fracture is not explicitly considered within <span class="hlt">ice</span> <span class="hlt">sheet</span> models due in part to large computational costs associated with the accurate modeling of this complex phenomena. However, fracture not only plays an extremely important role in regional behavior but also influences <span class="hlt">ice</span> dynamics over much larger zones in ways that are currently not well understood. Dramatic illustrations of fracture-induced phenomena most notably include the recent collapse of <span class="hlt">ice</span> shelves inmore » Antarctica (e.g. partial collapse of the Wilkins shelf in March of 2008 and the diminishing extent of the Larsen B shelf from 1998 to 2002). Other fracture examples include <span class="hlt">ice</span> calving (fracture of icebergs) which is presently approximated in simplistic ways within <span class="hlt">ice</span> <span class="hlt">sheet</span> models, and the draining of supraglacial lakes through a complex network of cracks, a so called <span class="hlt">ice</span> <span class="hlt">sheet</span> plumbing system, that is believed to cause accelerated <span class="hlt">ice</span> <span class="hlt">sheet</span> flows due essentially to lubrication of the contact surface with the ground. These dramatic changes are emblematic of the ongoing change in the Earth's polar regions and highlight the important role of fracturing <span class="hlt">ice</span>. To model <span class="hlt">ice</span> fracture, a simulation capability will be designed centered around extended finite elements and solved by specialized multigrid methods on parallel computers. In addition, appropriate dynamic load balancing techniques will be employed to ensure an approximate equal amount of work for each processor.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018TCry...12.1479M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018TCry...12.1479M"><span>Modelling the climate and surface mass balance of polar <span class="hlt">ice</span> <span class="hlt">sheets</span> using RACMO2 - Part 2: Antarctica (1979-2016)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Melchior van Wessem, Jan; van de Berg, Willem Jan; Noël, Brice P. Y.; van Meijgaard, Erik; Amory, Charles; Birnbaum, Gerit; Jakobs, Constantijn L.; Krüger, Konstantin; Lenaerts, Jan T. M.; Lhermitte, Stef; Ligtenberg, Stefan R. M.; Medley, Brooke; Reijmer, Carleen H.; van Tricht, Kristof; Trusel, Luke D.; van Ulft, Lambertus H.; Wouters, Bert; Wuite, Jan; van den Broeke, Michiel R.</p> <p>2018-04-01</p> <p>We evaluate modelled Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> (AIS) near-surface climate, surface mass balance (SMB) and surface energy balance (SEB) from the updated polar version of the regional atmospheric climate model, RACMO2 (1979-2016). The updated model, referred to as RACMO2.3p2, incorporates upper-air relaxation, a revised topography, tuned parameters in the cloud scheme to generate more precipitation towards the AIS interior and modified <span class="hlt">snow</span> properties reducing drifting <span class="hlt">snow</span> sublimation and increasing surface snowmelt. Comparisons of RACMO2 model output with several independent observational data show that the existing biases in AIS temperature, radiative fluxes and SMB components are further reduced with respect to the previous model version. The model-integrated annual average SMB for the <span class="hlt">ice</span> <span class="hlt">sheet</span> including <span class="hlt">ice</span> shelves (minus the Antarctic Peninsula, AP) now amounts to 2229 Gt y-1, with an interannual variability of 109 Gt y-1. The largest improvement is found in modelled surface snowmelt, which now compares well with satellite and weather station observations. For the high-resolution ( ˜ 5.5 km) AP simulation, results remain comparable to earlier studies. The updated model provides a new, high-resolution data set of the contemporary near-surface climate and SMB of the AIS; this model version will be used for future climate scenario projections in a forthcoming study.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C53A0693M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C53A0693M"><span>Multi-channel <span class="hlt">Ice</span> Penetrating Radar Traverse for Estimates of Firn Density in the Percolation Zone, Western Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Meehan, T.; Osterberg, E. C.; Lewis, G.; Overly, T. B.; Hawley, R. L.; Bradford, J.; Marshall, H. P.</p> <p>2016-12-01</p> <p>To better predict the response of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (GrIS) to future warming, leading edge Regional Climate Models (RCM) must be calibrated with in situ measurements of recent accumulation and melt. Mass balance estimates averaged across the entire Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (GrIS) vary between models by more than 30 percent, and regional comparisons of mass balance reconstructions in Greenland vary by 100 percent or more. Greenland Traverse for Accumulation and Climate Studies (GreenTrACS) is a multi-year and multi-disciplinary 1700 km science traverse from Raven/Dye2 in SW Greenland, to Summit Station. Multi-offset radar measurements can provide high accuracy electromagnetic (EM) velocity estimates of the firn to within (+-) 0.002 to 0.003 m/ns. EM velocity, in turn, can be used to estimate bulk firn density. Using a mixing equation such as the CRIM Equation we use the measured EM velocity, along with the known EM velocity in air and <span class="hlt">ice</span>, to estimate bulk density. During spring 2016, we used multi-channel 500MHz radar in a multi-offset configuration to survey more than 800 km from Raven towards summit. Preliminary radar-derived <span class="hlt">snow</span> density estimates agree with density estimates from a firn core measurement ( 50 kg/m3), despite the lateral heterogeneity of the firn across the length of the antenna array (12 m).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC53A0867D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC53A0867D"><span>Impacts of 1, 1.5, and 2 Degree Warming on Arctic Terrestrial <span class="hlt">Snow</span> and 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>Derksen, C.; Mudryk, L.; Howell, S.; Flato, G. M.; Fyfe, J. C.; Gillett, N. P.; Sigmond, M.; Kushner, P. J.; Dawson, J.; Zwiers, F. W.; Lemmen, D.; Duguay, C. R.; Zhang, X.; Fletcher, C. G.; Dery, S. J.</p> <p>2017-12-01</p> <p>The 2015 Paris Agreement of the United Nations Framework Convention on Climate Change (UNFCCC) established the global temperature goal of "holding the increase in the global average temperature to below 2°C above pre-industrial levels and pursuing efforts to limit the temperature increase to 1.5°C above pre-industrial levels." In this study, we utilize multiple gridded <span class="hlt">snow</span> and sea <span class="hlt">ice</span> products (satellite retrievals; assimilation systems; physical models driven by reanalyses) and ensembles of climate model simulations to determine the impacts of observed warming, and project the relative impacts of the UNFCC future warming targets on Arctic seasonal terrestrial <span class="hlt">snow</span> and sea <span class="hlt">ice</span> cover. Observed changes during the satellite era represent the response to approximately 1°C of global warming. Consistent with other studies, analysis of the observational record (1970's to present) identifies changes including a shorter <span class="hlt">snow</span> cover duration (due to later <span class="hlt">snow</span> onset and earlier <span class="hlt">snow</span> melt), significant reductions in spring <span class="hlt">snow</span> cover and summer sea <span class="hlt">ice</span> extent, and the loss of a large proportion of multi-year sea <span class="hlt">ice</span>. The spatial patterns of observed <span class="hlt">snow</span> and sea <span class="hlt">ice</span> loss are coherent across adjacent terrestrial/marine regions. There are strong pattern correlations between <span class="hlt">snow</span> and temperature trends, with weaker association between sea <span class="hlt">ice</span> and temperature due to the additional influence of dynamical effects such wind-driven redistribution of sea <span class="hlt">ice</span>. Climate model simulations from the Coupled Model Inter-comparison Project Phase 5(CMIP-5) multi-model ensemble, large initial condition ensembles of the Community Earth System Model (CESM) and Canadian Earth System Model (CanESM2) , and warming stabilization simulations from CESM were used to identify changes in <span class="hlt">snow</span> and <span class="hlt">ice</span> under further increases to 1.5°C and 2°C warming. The model projections indicate these levels of warming will be reached over the coming 2-4 decades. Warming to 1.5°C results in an increase in the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1813508S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1813508S"><span>The Impact of Geothermal Heat on the Scandinavian <span class="hlt">Ice</span> <span class="hlt">Sheet</span>'s LGM Extent</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Szuman, Izabela; Ewertowski, Marek W.; Kalita, Jakub Z.</p> <p>2016-04-01</p> <p>The last Scandinavian <span class="hlt">ice</span> <span class="hlt">sheet</span> attained its most southern extent over Poland and Germany, protruding c. 200 km south of the main <span class="hlt">ice</span> <span class="hlt">sheet</span> mass. There are number of factors that may control <span class="hlt">ice</span> <span class="hlt">sheet</span> dynamics and extent. One of the less recognised is geothermal heat, which is heat that is supplied to the base of the <span class="hlt">ice</span> <span class="hlt">sheet</span>. A heat at the <span class="hlt">ice</span>/bed interface plays a crucial role in controlling <span class="hlt">ice</span> <span class="hlt">sheet</span> stability, as well as impacting basal temperatures, melting, and <span class="hlt">ice</span> flow velocities. However, the influence of geothermal heat is still virtually neglected in reconstructions and modelling of paleo-<span class="hlt">ice</span> <span class="hlt">sheets</span> behaviour. Only in a few papers is geothermal heat recalled though often in the context of past climatic conditions. Thus, the major question is if and how spatial differences in geothermal heat had influenced paleo-<span class="hlt">ice</span> <span class="hlt">sheet</span> dynamics and in consequence their extent. Here, we assumed that the configuration of the <span class="hlt">ice</span> <span class="hlt">sheet</span> along its southern margin was moderately to strongly correlated with geothermal heat for Poland and non or negatively correlated for Germany.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29066736','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29066736"><span>Enhanced <span class="hlt">ice</span> <span class="hlt">sheet</span> melting driven by volcanic eruptions during the last deglaciation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Muschitiello, Francesco; Pausata, Francesco S R; Lea, James M; Mair, Douglas W F; Wohlfarth, Barbara</p> <p>2017-10-24</p> <p>Volcanic eruptions can impact the mass balance of <span class="hlt">ice</span> <span class="hlt">sheets</span> through changes in climate and the radiative properties of the <span class="hlt">ice</span>. Yet, empirical evidence highlighting the sensitivity of ancient <span class="hlt">ice</span> <span class="hlt">sheets</span> to volcanism is scarce. Here we present an exceptionally well-dated annual glacial varve chronology recording the melting history of the Fennoscandian <span class="hlt">Ice</span> <span class="hlt">Sheet</span> at the end of the last deglaciation (∼13,200-12,000 years ago). Our data indicate that abrupt <span class="hlt">ice</span> melting events coincide with volcanogenic aerosol emissions recorded in Greenland <span class="hlt">ice</span> cores. We suggest that enhanced <span class="hlt">ice</span> <span class="hlt">sheet</span> runoff is primarily associated with albedo effects due to deposition of ash sourced from high-latitude volcanic eruptions. Climate and snowpack mass-balance simulations show evidence for enhanced <span class="hlt">ice</span> <span class="hlt">sheet</span> runoff under volcanically forced conditions despite atmospheric cooling. The sensitivity of past <span class="hlt">ice</span> <span class="hlt">sheets</span> to volcanic ashfall highlights the need for an accurate coupling between atmosphere and <span class="hlt">ice</span> <span class="hlt">sheet</span> components in climate models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140011343','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140011343"><span>First Satellite-detected Perturbations of Outgoing Longwave Radiation Associated with Blowing <span class="hlt">Snow</span> Events over Antarctica</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Yang, Yuekui; Palm, Stephen P.; Marshak, Alexander; Wu, Dong L.; Yu, Hongbin; Fu, Qiang</p> <p>2014-01-01</p> <p>We present the first satellite-detected perturbations of the outgoing longwave radiation (OLR) associated with blowing <span class="hlt">snow</span> events over the Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> using data from Cloud-Aerosol Lidar with Orthogonal Polarization and Clouds and the Earth's Radiant Energy System. Significant cloud-free OLR differences are observed between the clear and blowing <span class="hlt">snow</span> sky, with the sign andmagnitude depending on season and time of the day. During nighttime, OLRs are usually larger when blowing <span class="hlt">snow</span> is present; the average difference in OLRs between without and with blowing <span class="hlt">snow</span> over the East Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> is about 5.2 W/m2 for the winter months of 2009. During daytime, in contrast, the OLR perturbation is usually smaller or even has the opposite sign. The observed seasonal variations and day-night differences in the OLR perturbation are consistent with theoretical calculations of the influence of blowing <span class="hlt">snow</span> on OLR. Detailed atmospheric profiles are needed to quantify the radiative effect of blowing <span class="hlt">snow</span> from the satellite observations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.G52A..06D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.G52A..06D"><span>Polar <span class="hlt">ice-sheet</span> contributions to sea level during past warm periods</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dutton, A.</p> <p>2015-12-01</p> <p>Recent sea-level rise has been dominated by thermal expansion and glacier loss, but the contribution from mass loss from the Greenland and Antarctic <span class="hlt">ice</span> <span class="hlt">sheets</span> is expected to exceed other contributions under future sustained warming. Due to limitations of existing <span class="hlt">ice</span> <span class="hlt">sheet</span> models and the lack of relevant analogues in the historical record, projecting the timing and magnitude of polar <span class="hlt">ice</span> <span class="hlt">sheet</span> mass loss in the future remains challenging. One approach to improving our understanding of how polar <span class="hlt">ice-sheet</span> retreat will unfold is to integrate observations and models of sea level, <span class="hlt">ice</span> <span class="hlt">sheets</span>, and climate during past intervals of warmth when the polar <span class="hlt">ice</span> <span class="hlt">sheets</span> contributed to higher sea levels. A recent review evaluated the evidence of polar <span class="hlt">ice</span> <span class="hlt">sheet</span> mass loss during several warm periods, including interglacials during the mid-Pliocene warm period, Marine Isotope Stage (MIS) 11, 5e (Last Interglacial), and 1 (Holocene). Sea-level benchmarks of <span class="hlt">ice-sheet</span> retreat during the first of these three periods, when global mean climate was ~1 to 3 deg. C warmer than preindustrial, are useful for understanding the long-term potential for future sea-level rise. Despite existing uncertainties in these reconstructions, it is clear that our present climate is warming to a level associated with significant polar <span class="hlt">ice-sheet</span> loss in the past, resulting in a conservative estimate for a global mean sea-level rise of 6 meters above present (or more). This presentation will focus on identifying the approaches that have yielded significant advances in terms of past sea level and <span class="hlt">ice</span> <span class="hlt">sheet</span> reconstruction as well as outstanding challenges. A key element of recent advances in sea-level reconstructions is the ability to recognize and quantify the imprint of geophysical processes, such as glacial isostatic adjustment (GIA) and dynamic topography, that lead to significant spatial variability in sea level reconstructions. Identifying specific <span class="hlt">ice-sheet</span> sources that contributed to higher sea levels</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C41C0706G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C41C0706G"><span>Potential Elevation Biases for Laser Altimeters from Subsurface Scattered Photons: Laboratory and Model Exploration of Green Light Scattering in <span class="hlt">Snow</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Greeley, A.; Neumann, T.; Markus, T.; Kurtz, N. T.; Cook, W. B.</p> <p>2015-12-01</p> <p>Existing visible light laser altimeters such as MABEL (Multiple Altimeter Beam Experimental Lidar) - a single photon counting simulator for ATLAS (Advanced Topographic Laser Altimeter System) on NASA's upcoming ICESat-2 mission - and ATM (Airborne Topographic Mapper) on NASA's Operation <span class="hlt">Ice</span>Bridge mission provide scientists a view of Earth's <span class="hlt">ice</span> <span class="hlt">sheets</span>, glaciers, and sea <span class="hlt">ice</span> with unprecedented detail. Precise calibration of these instruments is needed to understand rapidly changing parameters like sea <span class="hlt">ice</span> freeboard and to measure optical properties of surfaces like <span class="hlt">snow</span> covered <span class="hlt">ice</span> <span class="hlt">sheets</span> using subsurface scattered photons. Photons travelling into <span class="hlt">snow</span>, <span class="hlt">ice</span>, or water before scattering back to the altimeter receiving system (subsurface photons) travel farther and longer than photons scattering off the surface only, causing a bias in the measured elevation. We seek to identify subsurface photons in a laboratory setting using a flight-tested laser altimeter (MABEL) and to quantify their effect on surface elevation estimates for laser altimeter systems. We also compare these estimates with previous laboratory measurements of green laser light transmission through <span class="hlt">snow</span>, as well as Monte Carlo simulations of backscattered photons from <span class="hlt">snow</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018QSRv..179...87E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018QSRv..179...87E"><span><span class="hlt">Ice</span> streams of the Late Wisconsin Cordilleran <span class="hlt">Ice</span> <span class="hlt">Sheet</span> in western North America</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Eyles, Nick; Arbelaez Moreno, Lina; Sookhan, Shane</p> <p>2018-01-01</p> <p>The Late Wisconsin Cordilleran <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (CIS) of western North America is thought to have reached its maximum extent (∼2.5 × 106 km2) as late at c. 14.5 ka. Most (80%) of the <span class="hlt">ice</span> <span class="hlt">sheet</span>'s bed consists of high mountains but its 'core zone' sited on plateaux of the Intermontane Belt of British Columbia and coterminous parts of the USA, shows broad swaths of subglacially-streamlined rock and sediment. Broad scale mapping from new digital imagery data identifies three subglacial bed types: 1) 'hard beds' of variably streamlined bedrock; 2) drumlinized 'soft beds' of deformation till reworked from antecedent sediment, and 3) 'mixed beds' of variably-streamlined bedrock protruding through drumlinized sediment. Drumlins on soft beds appear to be erosional features cut into till and antecedent sediments, and identify the catchment areas of paleo <span class="hlt">ice</span> streams expressed downglacier as flow sets of megascale glacial lineations (MSGLs). 'Grooved' and 'cloned' drumlins appear to record the transition from drumlins to MSGLs. The location of paleo <span class="hlt">ice</span> streams reflects topographic funneling of <span class="hlt">ice</span> from plateau surfaces through outlet valleys and a soft bed that sustained fast flow; rock-cut MSGLs are also present locally on the floors of outlet valleys. CIS disintegrated in <1000 years shortly after c. 13.0 ka releasing very large volumes of meltwater and sediment to the Pacific coast. Abrupt deglaciation may reflect unsustainable calving of marine-based <span class="hlt">ice</span> streams along the glacio-isostatically depressed coast; large deep 'fiord lakes' in the <span class="hlt">ice</span> <span class="hlt">sheet</span>'s interior may have played an analogous role. Mapping of the broad scale distribution of bed types across the Cordilleran <span class="hlt">Ice</span> <span class="hlt">Sheet</span> provides key information for paleoglaciological modelling and also for understanding the beds of modern <span class="hlt">ice</span> masses such as the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> which is of a comparable topographic setting.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22419155','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22419155"><span>Collapse of polar <span class="hlt">ice</span> <span class="hlt">sheets</span> during the stage 11 interglacial.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Raymo, Maureen E; Mitrovica, Jerry X</p> <p>2012-03-14</p> <p>Contentious observations of Pleistocene shoreline features on the tectonically stable islands of Bermuda and the Bahamas have suggested that sea level about 400,000 years ago was more than 20 metres higher than it is today. Geochronologic and geomorphic evidence indicates that these features formed during interglacial marine isotope stage (MIS) 11, an unusually long interval of warmth during the <span class="hlt">ice</span> age. Previous work has advanced two divergent hypotheses for these shoreline features: first, significant melting of the East Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span>, in addition to the collapse of the West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> and the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span>; or second, emplacement by a mega-tsunami during MIS 11 (ref. 4, 5). Here we show that the elevations of these features are corrected downwards by ∼10 metres when we account for post-glacial crustal subsidence of these sites over the course of the anomalously long interglacial. On the basis of this correction, we estimate that eustatic sea level rose to ∼6-13 m above the present-day value in the second half of MIS 11. This suggests that both the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> and the West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> collapsed during the protracted warm period while changes in the volume of the East Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> were relatively minor, thereby resolving the long-standing controversy over the stability of the East Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> during MIS 11.</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> <span class="hlt">sheet</span> 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> <span class="hlt">sheet</span> mass 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 mass 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> <span class="hlt">sheet</span> in three ways: 1.) sensible heating given the water temperature exceeds that of the <span class="hlt">ice</span> <span class="hlt">sheet</span> 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> <span class="hlt">sheet</span>, 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> <span class="hlt">sheet</span> 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> <span class="hlt">sheet</span> loss reversible only through much slower <span class="hlt">ice</span> <span class="hlt">sheet</span> growth in an <span class="hlt">ice</span> age environment. As the inland <span class="hlt">ice</span> <span class="hlt">sheet</span> 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('https://pubs.er.usgs.gov/publication/70179581','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70179581"><span>Final Laurentide <span class="hlt">ice-sheet</span> deglaciation and Holocene climate-sea level change</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Ullman, David J.; Carlson, Anders E.; Hostetler, Steven W.; Clark, Peter U.; Cuzzone, Joshua; Milne, Glenn A.; Winsor, Kelsey; Caffee, Marc A.</p> <p>2016-01-01</p> <p>Despite elevated summer insolation forcing during the early Holocene, global <span class="hlt">ice</span> <span class="hlt">sheets</span> retained nearly half of their volume from the Last Glacial Maximum, as indicated by deglacial records of global mean sea level (GMSL). Partitioning the GMSL rise among potential sources requires accurate dating of <span class="hlt">ice-sheet</span> extent to estimate <span class="hlt">ice-sheet</span> volume. Here, we date the final retreat of the Laurentide <span class="hlt">Ice</span> <span class="hlt">Sheet</span> with 10Be surface exposure ages for the Labrador Dome, the largest of the remnant Laurentide <span class="hlt">ice</span> domes during the Holocene. We show that the Labrador Dome deposited moraines during North Atlantic cold events at ∼10.3 ka, 9.3 ka and 8.2 ka, suggesting that these regional climate events helped stabilize the retreating Labrador Dome in the early Holocene. After Hudson Bay became seasonally <span class="hlt">ice</span> free at ∼8.2 ka, the majority of Laurentide <span class="hlt">ice-sheet</span> melted abruptly within a few centuries. We demonstrate through high-resolution regional climate model simulations that the thermal properties of a seasonally <span class="hlt">ice</span>-free Hudson Bay would have increased Laurentide <span class="hlt">ice-sheet</span> ablation and thus contributed to the subsequent rapid Labrador Dome retreat. Finally, our new 10Be chronology indicates full Laurentide <span class="hlt">ice-sheet</span> had completely deglaciated by 6.7 ± 0.4 ka, which re quires that Antarctic <span class="hlt">ice</span> <span class="hlt">sheets</span> contributed 3.6–6.5 m to GMSL rise since 6.3–7.1 ka.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..1512466B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..1512466B"><span>Monitoring <span class="hlt">Snow</span> and Land <span class="hlt">Ice</span> Using Satellite data in the GMES Project CryoLand</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bippus, Gabriele; Nagler, Thomas</p> <p>2013-04-01</p> <p>The main objectives of the project "CryoLand - GMES Service <span class="hlt">Snow</span> and Land <span class="hlt">Ice</span>" are to develop, implement and validate services for <span class="hlt">snow</span>, glaciers and lake and river <span class="hlt">ice</span> products as a Downstream Service within the Global Monitoring for Environment and Security (GMES) program of the European Commission. CryoLand exploits Earth Observation data from current optical and microwave sensors and of the upcoming GMES Sentinel satellite family. The project prepares also the basis for the cryospheric component of the GMES Land Monitoring services. The CryoLand project team consists of 10 partner organisations from Austria, Finland, Norway, Sweden, Switzerland and Romania and is funded by the 7th Framework Program of the European Commission. The CryoLand baseline products for <span class="hlt">snow</span> include fractional <span class="hlt">snow</span> extent from optical satellite data, the extent of melting <span class="hlt">snow</span> from SAR data, and coarse resolution <span class="hlt">snow</span> water equivalent maps from passive microwave data. Experimental products include maps of <span class="hlt">snow</span> surface wetness and temperature. The products range from large scale coverage at medium resolution to regional products with high resolution, in order to address a wide user community. Medium resolution optical data (e.g. MODIS, in the near future Sentinel-3) and SAR (ENVISAT ASAR, in the near future Sentinel-1) are the main sources of EO data for generating large scale products in near real time. For generation of regional products high resolution satellite data are used. Glacier products are based on high resolution optical (e.g. SPOT-5, in the near future Sentinel-2) and SAR (TerraSAR-X, in the near future Sentinel-1) data and include glacier outlines, mapping of glacier facies, glacier lakes and <span class="hlt">ice</span> velocity. The glacier products are generated on users demand. Current test areas are located in the Alps, Norway, Greenland and the Himalayan Mountains. The lake and river <span class="hlt">ice</span> products include <span class="hlt">ice</span> extent and its temporal changes and <span class="hlt">snow</span> extent on <span class="hlt">ice</span>. The algorithms for these</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27665449','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27665449"><span>Water-soluble elements in <span class="hlt">snow</span> and <span class="hlt">ice</span> on Mt. Yulong.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Niu, Hewen; Kang, Shichang; Shi, Xiaofei; He, Yuanqing; Lu, Xixi; Shi, Xiaoyi; Paudyal, Rukumesh; Du, Jiankuo; Wang, Shijin; Du, Jun; Chen, Jizu</p> <p>2017-01-01</p> <p>Melting of high-elevation glaciers can be accelerated by the deposition of light-absorbing aerosols (e.g., organic carbon, mineral dust), resulting in significant reductions of the surface albedo on glaciers. Organic carbon deposited in glaciers is of great significance to global carbon cycles, <span class="hlt">snow</span> photochemistry, and air-<span class="hlt">snow</span> exchange processes. In this work, various <span class="hlt">snow</span> and <span class="hlt">ice</span> samples were collected at high elevation sites (4300-4850masl) from Mt. Yulong on the southeastern Tibetan Plateau in 2015. These samples were analyzed for water-soluble organic carbon (DOC), total nitrogen (TN), and water-soluble inorganic ions (WSIs) to elucidate the chemical species and compositions of the glaciers in the Mt. Yulong region. Generally, glacial meltwater had the lowest DOC content (0.39mgL -1 ), while fresh <span class="hlt">snow</span> had the highest (2.03mgL -1 ) among various types of <span class="hlt">snow</span> and <span class="hlt">ice</span> samples. There were obvious spatial and temporal trends of DOC and WSIs in glaciers. The DOC and TN concentrations decreased in the order of fresh <span class="hlt">snow</span>, <span class="hlt">snow</span> meltwater, snowpit, and surface <span class="hlt">snow</span>, resulting from the photolysis of DOC and <span class="hlt">snow</span>'s quick-melt effects. The surface <span class="hlt">snow</span> had low DOC and TN depletion ratios in the melt season; specifically, the ratios were -0.79 and -0.19mgL -1 d -1 , respectively. In the winter season, the ratios of DOC and TN were remarkably higher, with values of -0.20mgL -1 d -1 and -0.08mgL -1 d -1 , respectively. A reduction of the DOC and TN content in glaciers was due to <span class="hlt">snow</span>'s quick melt and sublimation. Deposition of these light-absorbing impurities (LAPs) in glaciers might accelerate snowmelt and even glacial retreat. Copyright © 2016 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.4366H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.4366H"><span>Deciphering the evolution of the last Eurasian <span class="hlt">ice</span> <span class="hlt">sheets</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hughes, Anna; Gyllencreutz, Richard; Mangerud, Jan; Svendsen, John Inge</p> <p>2016-04-01</p> <p>Glacial geologists need <span class="hlt">ice</span> <span class="hlt">sheet</span>-scale chronological reconstructions of former <span class="hlt">ice</span> extent to set individual records in a wider context and compare interpretations of <span class="hlt">ice</span> <span class="hlt">sheet</span> response to records of past environmental changes. <span class="hlt">Ice</span> <span class="hlt">sheet</span> modellers require empirical reconstructions on size and volume of past <span class="hlt">ice</span> <span class="hlt">sheets</span> that are fully documented, specified in time and include uncertainty estimates for model validation or constraints. Motivated by these demands, in 2005 we started a project (Database of the Eurasian Deglaciation, DATED) to compile and archive all published dates relevant to constraining the build-up and retreat of the last Eurasian <span class="hlt">ice</span> <span class="hlt">sheets</span>, including the British-Irish, Scandinavian and Svalbard-Barents-Kara Seas <span class="hlt">ice</span> <span class="hlt">sheets</span> (BIIS, SIS and SBKIS respectively). Over 5000 dates were assessed for reliability and used together with published <span class="hlt">ice-sheet</span> margin positions to reconstruct time-slice maps of the <span class="hlt">ice</span> <span class="hlt">sheets</span>' extent, with uncertainty bounds, every 1000 years between 25-10 kyr ago and at four additional periods back to 40 kyr ago. Ten years after the idea for a database was conceived, the first version of results (DATED-1) has now been released (Hughes et al. 2016). We observe that: i) both the BIIS and SBKIS achieve maximum extent, and commence retreat earlier than the larger SIS; ii) the eastern terrestrial margin of the SIS reached its maximum extent up to 7000 years later than the westernmost marine margin; iii) the combined maximum <span class="hlt">ice</span> volume (~24 m sea-level equivalent) was reached c. 21 ka; iv) large uncertainties exist; predominantly across marine sectors (e.g. the timing of coalescence and separation of the SIS and BKIS) but also in well-studied areas due to conflicting yet equally robust data. In just three years since the DATED-1 census (1 January 2013), the volume of new information (from both dates and mapped glacial geomorphology) has grown significantly (~1000 new dates). Here, we present the DATED-1 results in the context of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1714301S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1714301S"><span>Validating Cryosat-2 elevation estimates with airborne laser scanner data for the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span>, Austfonna and Devon <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>Simonsen, Sebastian B.; Sandberg Sørensen, Louise; Nilsson, Johan; Helm, Veit; Langley, Kirsty A.; Forsberg, Rene; Hvidegaard, Sine M.; Skourup, Henriette</p> <p>2015-04-01</p> <p>The ESA CryoSat-2 satellite, launched in late 2010, carries a new type of radar altimeter especially designed for monitoring changes of sea and land <span class="hlt">ice</span>. The radar signal might penetrate into the <span class="hlt">snow</span> pack and the depth of the radar reflecting surface depends on the ratio between the surface and the volume backscatter, which is a function of several different properties such as <span class="hlt">snow</span> density, crystal structure and surface roughness. In case of large volume scatter, the radar waveforms become broad and the determination of the range (surface elevation) becomes more difficult. Different algorithms (retrackers) are used for the range determination, and estimated surface penetration is highly dependent on the applied retracker. As part of the ESA-CryoVEx/CryoVal-Land <span class="hlt">Ice</span> projects, DTU Space has gathered accurate airborne laser scanner elevation measurements. Sites on the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span>, Austfonna and Devon <span class="hlt">ice</span> caps, has been surveyed repeatedly, aligned with Cryosat-2 ground tracks and surface experiments. Here, we utilize elevation estimates from available Cryosat-2 retrackers (ESA level-2 retracker, DTU retracker, etc.) and validate the elevation measurements against ESA-CryoVEx campaigns. A difference between laser and radar elevations is expected due to radar penetration issues, however an inter-comparison between retrackers will shed light on individual performances and biases. Additionally, the geo-location of the radar return will also be a determining factor for the precision. Ultimately, the use of multiple retrackers can provide information about subsurface conditions and utilize more of the waveform information than presently used in radar altimetry.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014PhDT........38L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014PhDT........38L"><span>A model of the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> deglaciation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lecavalier, Benoit</p> <p></p> <p>The goal of this thesis is to improve our understanding of the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> (GrIS) and how it responds to climate change. This was achieved using <span class="hlt">ice</span> core records to infer elevation changes of the GrIS during the Holocene (11.7 ka BP to Present). The inferred elevation changes show the response of the <span class="hlt">ice</span> <span class="hlt">sheet</span> interior to the Holocene Thermal Maximum (HTM; 9-5 ka BP) when temperatures across Greenland were warmer than present. These <span class="hlt">ice</span>-core derived thinning curves act as a new set of key constraints on the deglacial history of the GrIS. Furthermore, a calibration was conducted on a three-dimensional thermomechanical <span class="hlt">ice</span> <span class="hlt">sheet</span>, glacial isostatic adjustment, and relative sea-level model of GrIS evolution during the most recent deglaciation (21 ka BP to present). The model was data-constrained to a variety of proxy records from paleoclimate archives and present-day observations of <span class="hlt">ice</span> thickness and extent.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017TCry...11.1371V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017TCry...11.1371V"><span>Hypsometric amplification and routing moderation of Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> meltwater release</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>van As, Dirk; Mikkelsen, Andreas Bech; Holtegaard Nielsen, Morten; Box, Jason E.; Claesson Liljedahl, Lillemor; Lindbäck, Katrin; Pitcher, Lincoln; Hasholt, Bent</p> <p>2017-06-01</p> <p>Concurrent <span class="hlt">ice</span> <span class="hlt">sheet</span> surface runoff and proglacial discharge monitoring are essential for understanding Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> meltwater release. We use an updated, well-constrained river discharge time series from the Watson River in southwest Greenland, with an accurate, observation-based <span class="hlt">ice</span> <span class="hlt">sheet</span> surface mass balance model of the ˜ 12 000 km2 <span class="hlt">ice</span> <span class="hlt">sheet</span> area feeding the river. For the 2006-2015 decade, we find a large range of a factor of 3 in interannual variability in discharge. The amount of discharge is amplified ˜ 56 % by the <span class="hlt">ice</span> <span class="hlt">sheet</span>'s hypsometry, i.e., area increase with elevation. A good match between river discharge and <span class="hlt">ice</span> <span class="hlt">sheet</span> surface meltwater production is found after introducing elevation-dependent transit delays that moderate diurnal variability in meltwater release by a factor of 10-20. The routing lag time increases with <span class="hlt">ice</span> <span class="hlt">sheet</span> elevation and attains values in excess of 1 week for the upper reaches of the runoff area at ˜ 1800 m above sea level. These multi-day routing delays ensure that the highest proglacial discharge levels and thus overbank flooding events are more likely to occur after multi-day melt episodes. Finally, for the Watson River <span class="hlt">ice</span> <span class="hlt">sheet</span> catchment, we find no evidence of meltwater storage in or release from the en- and subglacial environments in quantities exceeding our methodological uncertainty, based on the good match between <span class="hlt">ice</span> <span class="hlt">sheet</span> runoff and proglacial discharge.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C51E..02K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C51E..02K"><span>The self-organization of <span class="hlt">snow</span> surfaces and the growth of sastrugi</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kochanski, K.; Bertholet, C.; Anderson, R. S.; Tucker, G. E.</p> <p>2017-12-01</p> <p>Seasonal <span class="hlt">snow</span> covers approximately 15% of the surface of the Earth. The majority of this <span class="hlt">snow</span> is found on tundra, <span class="hlt">ice</span> <span class="hlt">sheets</span>, and sea <span class="hlt">ice</span>. These windswept <span class="hlt">snow</span> surfaces self-organize into depositional bedforms, such as ripples, barchan dunes, and transverse waves, and erosional bedforms, such as anvil-shaped sastrugi. Previous researchers have shown that these bedforms influence the reflectivity, thermal conductivity, and aerodynamic roughness of the surface. For the past two winters, we have observed the growth and movement of <span class="hlt">snow</span> bedforms on Niwot Ridge, Colorado, at an elevation of 3500m. We have observed that (1) when wind speeds are below 3m/s, <span class="hlt">snow</span> surfaces can be smooth, (2) when winds are higher than 3m/s during and immediately following a storm, the smooth surface is unstable and self-organizes into a field of dunes, (3) as <span class="hlt">snow</span> begins to harden, it forms erosional bedforms that are characterized by vertical edges facing upwind (4) between 12 and 48 hours after each snowfall, alternating stripes of erosional and depositional bedforms occur, and (5) within 60 hours of each storm, the surface self-organizes into a field of sastrugi, which remains stable until it melts or becomes buried by the next snowfall. Polar researchers should therefore expect <span class="hlt">snow</span>-covered surfaces to be characterized by fields of bedforms, which evolve in response to variations in <span class="hlt">snow</span> delivery, windspeed, and periods of sintering. Smooth drifts may be found in sheltered and forested regions. On most <span class="hlt">ice</span> <span class="hlt">sheets</span> and sea <span class="hlt">ice</span> where snowfall is frequent, the typical surface is likely to consist of an evolving mix of depositional and erosional bedforms. Where snowfall is infrequent, for example in Antarctica, the surface will be dominated by sastrugi fields.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_16 --> <div id="page_17" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="321"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110008252','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110008252"><span>Recent Changes in the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> as Seen from Space</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hall, Dorothy K.</p> <p>2011-01-01</p> <p>Many changes in the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> have been reported in the recent scientific literature and have been attributed to various responses of the <span class="hlt">ice</span> <span class="hlt">sheet</span> due to regional (and global) warming. Because melting of the <span class="hlt">ice</span> <span class="hlt">sheet</span> would contribute approximately 7 m to sea-level rise, the lives and habitat of hundreds of millions of people worldwide would be directly and indirectly affected if continued <span class="hlt">ice-sheet</span> melting occurs. As mean-annual global temperatures have increased, there has been an increasing focus on studying the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> using available satellite data, and numerous expeditions have been undertaken. Regional "clear-sky" surface temperature increases since the early 1980s in the Arctic, measured using Advanced Very High Resolution Radiometer (AVHRR) infrared data, range from 0.57+/-0.02 C to 0.72+/-0.10 C per decade. Arctic warming has important implications for <span class="hlt">ice-sheet</span> mass balance because much of the periphery of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> is already near O C during the melt season, and is thus vulnerable to more extensive melting if temperatures continue to increase. An increase in melting of the <span class="hlt">ice</span> <span class="hlt">sheet</span> would accelerate sea-level rise, an issue of increasing concern to billions of people worldwide. The surface temperature of the <span class="hlt">ice</span> <span class="hlt">sheet</span> has been studied in even greater detail using Moderate-Resolution Imaging Spectroradiometer (MODIS) data in the six individual drainage basins as well as for the <span class="hlt">ice</span> <span class="hlt">sheet</span> as a whole. Surface temperature trends in the decade of the 2000s have not been strong, according to the MODIS measurements. In addition to surface-temperature increases over the last few decades as measured by AVHRR, other changes have been observed such as accelerated movement of many of Greenland's outlet glaciers and sudden draining of supraglacial lakes. Decreasing mass of the <span class="hlt">ice</span> <span class="hlt">sheet</span> since (at least) 2002 has been measured using Gravity Recovery and Climate Experiment (GRACE) data, along with an build-up of <span class="hlt">ice</span> at the higher</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.8570A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.8570A"><span>Design of the MISMIP+, ISOMIP+, and MISOMIP <span class="hlt">ice-sheet</span>, ocean, and coupled <span class="hlt">ice</span> <span class="hlt">sheet</span>-ocean intercomparison projects</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Asay-Davis, Xylar; Cornford, Stephen; Martin, Daniel; Gudmundsson, Hilmar; Holland, David; Holland, Denise</p> <p>2015-04-01</p> <p>The MISMIP and MISMIP3D marine <span class="hlt">ice</span> <span class="hlt">sheet</span> model intercomparison exercises have become popular benchmarks, and several modeling groups have used them to show how their models compare to both analytical results and other models. Similarly, the ISOMIP (<span class="hlt">Ice</span> Shelf-Ocean Model Intercomparison Project) experiments have acted as a proving ground for ocean models with sub-<span class="hlt">ice</span>-shelf cavities.As coupled <span class="hlt">ice</span> <span class="hlt">sheet</span>-ocean models become available, an updated set of benchmark experiments is needed. To this end, we propose sequel experiments, MISMIP+ and ISOMIP+, with an end goal of coupling the two in a third intercomparison exercise, MISOMIP (the Marine <span class="hlt">Ice</span> <span class="hlt">Sheet</span>-Ocean Model Intercomparison Project). Like MISMIP3D, the MISMIP+ experiments take place in an idealized, three-dimensional setting and compare full 3D (Stokes) and reduced, hydrostatic models. Unlike the earlier exercises, the primary focus will be the response of models to sub-shelf melting. The chosen configuration features an <span class="hlt">ice</span> shelf that experiences substantial lateral shear and buttresses the upstream <span class="hlt">ice</span>, and so is well suited to melting experiments. Differences between the steady states of each model are minor compared to the response to melt-rate perturbations, reflecting typical real-world applications where parameters are chosen so that the initial states of all models tend to match observations. The three ISOMIP+ experiments have been designed to to make use of the same bedrock topography as MISMIP+ and using <span class="hlt">ice</span>-shelf geometries from MISMIP+ results produced by the BISICLES <span class="hlt">ice-sheet</span> model. The first two experiments use static <span class="hlt">ice</span>-shelf geometries to simulate the evolution of ocean dynamics and resulting melt rates to a quasi-steady state when far-field forcing changes in either from cold to warm or from warm to cold states. The third experiment prescribes 200 years of dynamic <span class="hlt">ice</span>-shelf geometry (with both retreating and advancing <span class="hlt">ice</span>) based on a BISICLES simulation along with similar flips between warm and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C11F..05G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C11F..05G"><span>Microwave Observations of <span class="hlt">Snow</span>-Covered Freshwater Lake <span class="hlt">Ice</span> obtained during the Great Lakes Winter EXperiment (GLAWEX), 2017</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gunn, G. E.; Hall, D. K.; Nghiem, S. V.</p> <p>2017-12-01</p> <p>Studies observing lake <span class="hlt">ice</span> using active microwave acquisitions suggest that the dominant scattering mechanism in <span class="hlt">ice</span> is caused by double-bounce of the signal off vertical tubular bubble inclusions. Recent polarimetric SAR observations and target decomposition algorithms indicate single-bounce interactions may be the dominant source of returns, and in the absence of field observations, has been hypothesized to be the result of roughness at the <span class="hlt">ice</span>-water interface on the order of incident wavelengths. This study presents in-situ physical observations of <span class="hlt">snow</span>-covered lake <span class="hlt">ice</span> in western Michigan and Wisconsin acquired during the Great Lakes Winter EXperiment in 2017 (GLAWEX'17). In conjunction with NASA's <span class="hlt">Snow</span>Ex airborne <span class="hlt">snow</span> campaign in Colorado (http://<span class="hlt">snow</span>.nasa.gov), C- (Sentinel-1, RADARSAT-2) and X-band (TerraSAR-X) synthetic aperture radar (SAR) observations were acquired coincidently to surface physical <span class="hlt">snow</span> and <span class="hlt">ice</span> observations. Small/large scale roughness features at the <span class="hlt">ice</span>-water interface are quantified through auger transects and used as an input variable in lake <span class="hlt">ice</span> backscatter models to assess the relative contributions from different scattering mechanisms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910017261','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910017261"><span>Sea-level response to <span class="hlt">ice</span> <span class="hlt">sheet</span> evolution: An ocean perspective</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jacobs, Stanley S.</p> <p>1991-01-01</p> <p>The ocean's influence upon and response to Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> changes is considered in relation to sea level rise over recent and future decades. Assuming present day <span class="hlt">ice</span> fronts are in approximate equilibrium, a preliminary budget for the <span class="hlt">ice</span> <span class="hlt">sheet</span> is estimated from accumulation vs. iceberg calving and the basal melting that occurs beneath floating <span class="hlt">ice</span> shelves. Iceberg calving is derived from the volume of large bergs identified and tracked by the Navy/NOAA Joint <span class="hlt">Ice</span> Center and from shipboard observations. Basal melting exceeds 600 cu km/yr and is concentrated near the <span class="hlt">ice</span> fronts and <span class="hlt">ice</span> shelf grounding lines. An apparent negative mass balance for the Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> may result from an anomalous calving rate during the past decade, but there are large uncertainties associated with all components of the <span class="hlt">ice</span> budget. The results from general circulation models are noted in the context of projected precipitation increases and ocean temperature changes on and near the continent. An ocean research program that could help refine budget estimates is consistent with goals of the West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Initiative.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013QSRv...64...33I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013QSRv...64...33I"><span>The Svalbard-Barents Sea <span class="hlt">ice-sheet</span> - Historical, current and future perspectives</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ingólfsson, Ólafur; Landvik, Jon Y.</p> <p>2013-03-01</p> <p>The history of research on the Late Quaternary Svalbard-Barents Sea <span class="hlt">ice</span> <span class="hlt">sheet</span> mirrors the developments of ideas and the shifts of paradigms in glacial theory over the past 150 years. Since the onset of scientific research there in the early 19th Century, Svalbard has been a natural laboratory where ideas and concepts have been tested, and played an important (but rarely acknowledged) role in the break-through of the <span class="hlt">Ice</span> Age theory in the 1870's. The history of how the scientific perception of the Svalbard-Barents sea <span class="hlt">ice</span> <span class="hlt">sheet</span> developed in the mid-20th Century also tells a story of how a combination of fairly scattered and often contradictory observational data, and through both deductive and inductive reasoning, could outline a major <span class="hlt">ice</span> <span class="hlt">sheet</span> that had left but few tangible fingerprints. Since the 1980's, with increased terrestrial stratigraphical data, ever more marine geological evidence and better chronological control of glacial events, our perception of the Svalbard-Barents Sea <span class="hlt">ice</span> <span class="hlt">sheet</span> has changed. The first reconstructions depicted it as a static, concentric, single-domed <span class="hlt">ice</span> <span class="hlt">sheet</span>, with <span class="hlt">ice</span> flowing from an <span class="hlt">ice</span> divide over the central northern Barents Sea that expanded and declined in response to large-scale, Late Quaternary climate fluctuations, and which was more or less in tune with other major Northern Hemisphere <span class="hlt">ice</span> <span class="hlt">sheets</span>. We now increasingly perceive it as a very dynamic, multidomed <span class="hlt">ice</span> <span class="hlt">sheet</span>, controlled by climate fluctuations, relative sea-level change, as well as subglacial topography, substrate properties and basal temperature. In this respect, the Svalbard-Barents Sea <span class="hlt">ice</span> <span class="hlt">sheet</span> will increasingly hold the key for understanding the dynamics and processes of how marine-based <span class="hlt">ice</span> <span class="hlt">sheets</span> build-up and decay.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040085502','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040085502"><span>Interannual Variability of <span class="hlt">Snow</span> and <span class="hlt">Ice</span> and Impact on the Carbon Cycle</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Yung, Yuk L.</p> <p>2004-01-01</p> <p>The goal of this research is to assess the impact of the interannual variability in <span class="hlt">snow/ice</span> using global satellite data sets acquired in the last two decades. This variability will be used as input to simulate the CO2 interannual variability at high latitudes using a biospheric model. The progress in the past few years is summarized as follows: 1) Albedo decrease related to spring <span class="hlt">snow</span> retreat; 2) Observed effects of interannual summertime sea <span class="hlt">ice</span> variations on the polar reflectance; 3) The Northern Annular Mode response to Arctic sea <span class="hlt">ice</span> loss and the sensitivity of troposphere-stratosphere interaction; 4) The effect of Arctic warming and sea <span class="hlt">ice</span> loss on the growing season in northern terrestrial ecosystem.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1013735','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1013735"><span><span class="hlt">Snow</span> on Sea <span class="hlt">Ice</span> Workshop - An Icy Meeting of the Minds: Modelers and Measurers</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2015-09-30</p> <p>1 DISTRIBUTION STATEMENT A. Approved for public release; distribution is unlimited. <span class="hlt">Snow</span> on Sea <span class="hlt">Ice</span> Workshop - An Icy Meeting of the Minds...workshop was to promote more seamless and better integration between measurements and modeling of <span class="hlt">snow</span> on sea <span class="hlt">ice</span> , thereby improving our predictive...capabilities for sea <span class="hlt">ice</span> . OBJECTIVES The key objective was to improve the ability of modelers and measurers work together closely. To that end, we</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27873793','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27873793"><span>Empirical Retrieval of Surface Melt Magnitude from Coupled MODIS Optical and Thermal Measurements over the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> during the 2001 Ablation Season.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lampkin, Derrick; Peng, Rui</p> <p>2008-08-22</p> <p>Accelerated <span class="hlt">ice</span> flow near the equilibrium line of west-central Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (GIS) has been attributed to an increase in infiltrated surface melt water as a response to climate warming. The assessment of surface melting events must be more than the detection of melt onset or extent. Retrieval of surface melt magnitude is necessary to improve understanding of <span class="hlt">ice</span> <span class="hlt">sheet</span> flow and surface melt coupling. In this paper, we report on a new technique to quantify the magnitude of surface melt. Cloud-free dates of June 10, July 5, 7, 9, and 11, 2001 Moderate Resolution Imaging Spectroradiometer (MODIS) daily reflectance Band 5 (1.230-1.250μm) and surface temperature images rescaled to 1km over western Greenland were used in the retrieval algorithm. An optical-thermal feature space partitioned as a function of melt magnitude was derived using a one-dimensional thermal snowmelt model (SNTHERM89). SNTHERM89 was forced by hourly meteorological data from the Greenland Climate Network (GC-Net) at reference sites spanning dry <span class="hlt">snow</span>, percolation, and wet <span class="hlt">snow</span> zones in the Jakobshavn drainage basin in western GIS. Melt magnitude or effective melt (E-melt) was derived for satellite composite periods covering May, June, and July displaying low fractions (0-1%) at elevations greater than 2500m and fractions at or greater than 15% at elevations lower than 1000m assessed for only the upper 5 cm of the <span class="hlt">snow</span> surface. Validation of E-melt involved comparison of intensity to dry and wet zones determined from QSCAT backscatter. Higher intensities (> 8%) were distributed in wet <span class="hlt">snow</span> zones, while lower intensities were grouped in dry zones at a first order accuracy of ~ ±2%.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GeoRL..4311295S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GeoRL..4311295S"><span>Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> flow response to runoff variability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stevens, Laura A.; Behn, Mark D.; Das, Sarah B.; Joughin, Ian; Noël, Brice P. Y.; Broeke, Michiel R.; Herring, Thomas</p> <p>2016-11-01</p> <p>We use observations of <span class="hlt">ice</span> <span class="hlt">sheet</span> surface motion from a Global Positioning System network operating from 2006 to 2014 around North Lake in west Greenland to investigate the dynamical response of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span>'s ablation area to interannual variability in surface melting. We find no statistically significant relationship between runoff season characteristics and <span class="hlt">ice</span> flow velocities within a given year or season. Over the 7 year time series, annual velocities at North Lake decrease at an average rate of -0.9 ± 1.1 m yr-2, consistent with the negative trend in annual velocities observed in neighboring regions over recent decades. We find that net runoff integrated over several preceding years has a negative correlation with annual velocities, similar to findings from the two other available decadal records of <span class="hlt">ice</span> velocity in western Greenland. However, we argue that this correlation is not necessarily evidence for a direct hydrologic mechanism acting on the timescale of multiple years but could be a statistical construct. Finally, we stress that neither the decadal slowdown trend nor the negative correlation between velocity and integrated runoff is predicted by current <span class="hlt">ice-sheet</span> models, underscoring that these models do not yet capture all the relevant feedbacks between runoff and <span class="hlt">ice</span> dynamics needed to predict long-term trends in <span class="hlt">ice</span> <span class="hlt">sheet</span> flow.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017QSRv..169...13D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017QSRv..169...13D"><span>Current state and future perspectives on coupled <span class="hlt">ice-sheet</span> - sea-level modelling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>de Boer, Bas; Stocchi, Paolo; Whitehouse, Pippa L.; van de Wal, Roderik S. W.</p> <p>2017-08-01</p> <p>The interaction between <span class="hlt">ice-sheet</span> growth and retreat and sea-level change has been an established field of research for many years. However, recent advances in numerical modelling have shed new light on the precise interaction of marine <span class="hlt">ice</span> <span class="hlt">sheets</span> with the change in near-field sea level, and the related stability of the grounding line position. Studies using fully coupled <span class="hlt">ice-sheet</span> - sea-level models have shown that accounting for gravitationally self-consistent sea-level change will act to slow down the retreat and advance of marine <span class="hlt">ice-sheet</span> grounding lines. Moreover, by simultaneously solving the 'sea-level equation' and modelling <span class="hlt">ice-sheet</span> flow, coupled models provide a global field of relative sea-level change that is consistent with dynamic changes in <span class="hlt">ice-sheet</span> extent. In this paper we present an overview of recent advances, possible caveats, methodologies and challenges involved in coupled <span class="hlt">ice-sheet</span> - sea-level modelling. We conclude by presenting a first-order comparison between a suite of relative sea-level data and output from a coupled <span class="hlt">ice-sheet</span> - sea-level model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhDT.......190B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhDT.......190B"><span>Machine Learning Algorithms for Automated Satellite <span class="hlt">Snow</span> and Sea <span class="hlt">Ice</span> Detection</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bonev, George</p> <p></p> <p>The continuous mapping of <span class="hlt">snow</span> and <span class="hlt">ice</span> cover, particularly in the arctic and poles, are critical to understanding the earth and atmospheric science. Much of the world's sea <span class="hlt">ice</span> and <span class="hlt">snow</span> covers the most inhospitable places, making measurements from satellite-based remote sensors essential. Despite the wealth of data from these instruments many challenges remain. For instance, remote sensing instruments reside on-board different satellites and observe the earth at different portions of the electromagnetic spectrum with different spatial footprints. Integrating and fusing this information to make estimates of the surface is a subject of active research. In response to these challenges, this dissertation will present two algorithms that utilize methods from statistics and machine learning, with the goal of improving on the quality and accuracy of current <span class="hlt">snow</span> and sea <span class="hlt">ice</span> detection products. The first algorithm aims at implementing <span class="hlt">snow</span> detection using optical/infrared instrument data. The novelty in this approach is that the classifier is trained using ground station measurements of <span class="hlt">snow</span> depth that are collocated with the reflectance observed at the satellite. Several classification methods are compared using this training data to identify the one yielding the highest accuracy and optimal space/time complexity. The algorithm is then evaluated against the current operational NASA <span class="hlt">snow</span> product and it is found that it produces comparable and in some cases superior accuracy results. The second algorithm presents a fully automated approach to sea <span class="hlt">ice</span> detection that integrates data obtained from passive microwave and optical/infrared satellite instruments. For a particular region of interest the algorithm generates sea <span class="hlt">ice</span> maps of each individual satellite overpass and then aggregates them to a daily composite level, maximizing the amount of high resolution information available. The algorithm is evaluated at both, the individual satellite overpass level, and at the daily</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> <span class="hlt">sheets</span> 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> <span class="hlt">sheets</span>: Once these <span class="hlt">ice</span> masses 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> <span class="hlt">sheet</span> and the West Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span>.</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> <span class="hlt">Sheet</span></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> <span class="hlt">Sheet</span> (LIS; including the Innuitian <span class="hlt">Ice</span> <span class="hlt">Sheet</span>) from the Last Glacial Maximum (LGM), with a particular focus on the spatial and temporal variations 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> <span class="hlt">sheet</span> 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> <span class="hlt">sheet</span> 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 mass balance are viewed as more likely drivers. Retreat</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20030062151&hterms=Ali&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DAli','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20030062151&hterms=Ali&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DAli"><span>Advancing Glaciological Applications of Remote Sensing with EO-1: (1) Mapping <span class="hlt">Snow</span> Grain Size and Albedo on the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Using an Imaging Spectrometer, and (2) ALI Evaluation for Subtle Surface Topographic Mapping via Shape-from Shading</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>2003-01-01</p> <p>The Hyperion sensor, onboard NASA's Earth Observing-1 (EO-1) satellite,is an imaging spectroradiometer with 220 spectral bands over the spectral range from 0.4 - 2.5 microns. Over the course of summer 2001, the instrument acquired numerous images over the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span>. Our main motivation is to develop an accurate and robust approach for measuring the broadband albedo of <span class="hlt">snow</span> from satellites. Satellite-derived estimates of broadband have typically been plagued with three problems: errors resulting from inaccurate atmospheric correction, particularly in the visible wavelengths from the conversion of reflectance to albedo (accounting for <span class="hlt">snow</span> BRDE); and errors resulting from regression-based approaches used to convert narrowband albedo to broadband albedo. A typerspectral method has been developed that substantially reduces these three main sources of error and produces highly accurate estimates of <span class="hlt">snow</span> albedo. This technique uses hyperspectral data from 0.98 - 1.06 microns, spanning a spectral absorption feature centered at 1.03 microns. A key aspect of this work is that this spectral range is within an atmospheric transmission window and reflectances are largely unaffected by atmospheric aerosols, water vapor, or ozone. In this investigation, we make broadband albedo measurements at four sites on the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span>: Summit, a high altitude station in central Greenland; the ETH/CU camp, a camp on the equilibrium line in western Greenland; Crawford Point, a site located between Summit and the ETH/CU camp; and Tunu, a site located in northeastern Greenland at 2000 m. altitude. Each of these sites has an automated weather station (AWS) that continually measures broadband albedo thereby providing validation data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.C31A0603R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.C31A0603R"><span>Comparison between AVHRR surface temperature data and in-situ weather station temperatures over the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rezvanbehbahani, S.; Csatho, B. M.; Comiso, J. C.; Babonis, G. S.</p> <p>2011-12-01</p> <p>Advanced Very-High Resolution Radiometer (AVHRR) images have been exhaustively used to measure surface temperature time series of the Greenland <span class="hlt">Ice</span> <span class="hlt">sheet</span>. The purpose of this study is to assess the accuracy of monthly average <span class="hlt">ice</span> <span class="hlt">sheet</span> surface temperatures, derived from thermal infrared AVHRR satellite imagery on a 6.25 km grid. In-situ temperature data sets are from the Greenland Collection Network (GC-Net). GC-Net stations comprise sensors monitoring air temperature at 1 and 2 meter above the <span class="hlt">snow</span> surface, gathered at every 60 seconds and monthly averaged to match the AVHRR temporal resolution. Our preliminary results confirm the good agreement between satellite and in-situ temperature measurements reported by previous studies. However, some large discrepancies still exist. While AVHRR provides <span class="hlt">ice</span> surface temperature, in-situ stations measure air temperatures at different elevations above the <span class="hlt">snow</span> surface. Since most in-situ data on <span class="hlt">ice</span> <span class="hlt">sheets</span> are collected by Automatic Weather Station (AWS) instruments, it is important to characterize the difference between surface and air temperatures. Therefore, we compared and analyzed average monthly AVHRR <span class="hlt">ice</span> surface temperatures using data collected in 2002. Differences between these temperatures correlate with in-situ temperatures and GC-Net station elevations, with increasing differences at lower elevations and higher temperatures. The Summit Station (3199 m above sea level) and the Swiss Camp (1176 m above sea level) results were compared as high altitude and low altitude stations for 2002, respectively. Our results show that AVHRR derived temperatures were 0.5°K warmer than AWS temperature at the Summit Station, while this difference was 2.8°K in the opposite direction for the Swiss Camp with surface temperatures being lower than air temperatures. The positive bias of 0.5°K at the high altitude Summit Station (surface warmer than air) is within the retrieval error of AVHRR temperatures and might be in part due to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-GSFC_20171208_Archive_e000258.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-GSFC_20171208_Archive_e000258.html"><span>NASA: First Map Of Thawed Areas Under Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2017-12-08</p> <p>NASA researchers have helped produce the first map showing what parts of the bottom of the massive Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> are thawed – key information in better predicting how the <span class="hlt">ice</span> <span class="hlt">sheet</span> will react to a warming climate. Greenland’s thick <span class="hlt">ice</span> <span class="hlt">sheet</span> insulates the bedrock below from the cold temperatures at the surface, so the bottom of the <span class="hlt">ice</span> is often tens of degrees warmer than at the top, because the <span class="hlt">ice</span> bottom is slowly warmed by heat coming from the Earth’s depths. Knowing whether Greenland’s <span class="hlt">ice</span> lies on wet, slippery ground or is anchored to dry, frozen bedrock is essential for predicting how this <span class="hlt">ice</span> will flow in the future, But scientists have very few direct observations of the thermal conditions beneath the <span class="hlt">ice</span> <span class="hlt">sheet</span>, obtained through fewer than two dozen boreholes that have reached the bottom. Now, a new study synthesizes several methods to infer the Greenland <span class="hlt">Ice</span> Sheet’s basal thermal state –whether the bottom of the <span class="hlt">ice</span> is melted or not– leading to the first map that identifies frozen and thawed areas across the whole <span class="hlt">ice</span> <span class="hlt">sheet</span>. Map caption: This first-of-a-kind map, showing which parts of the bottom of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> are likely thawed (red), frozen (blue) or still uncertain (gray), will help scientists better predict how the <span class="hlt">ice</span> will flow in a warming climate. Credit: NASA Earth Observatory/Jesse Allen Read more: go.nasa.gov/2avKgl2 NASA image use policy. NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. Follow us on Twitter Like us on Facebook Find us on Instagram</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMED12A..06H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMED12A..06H"><span>Improving Climate Literacy Using The <span class="hlt">Ice</span> <span class="hlt">Sheet</span> System Model (ISSM): A Prototype Virtual <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Laboratory For Use In K-12 Classrooms</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Halkides, D. J.; Larour, E. Y.; Perez, G.; Petrie, K.; Nguyen, L.</p> <p>2013-12-01</p> <p>Statistics indicate that most Americans learn what they will know about science within the confines of our public K-12 education system and the media. Next Generation Science Standards (NGSS) aim to remedy science illiteracy and provide guidelines to exceed the Common Core State Standards that most U.S. state governments have adopted, by integrating disciplinary cores with crosscutting ideas and real life practices. In this vein, we present a prototype ';Virtual <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Laboratory' (I-Lab), geared to K-12 students, educators and interested members of the general public. I-Lab will allow users to perform experiments using a state-of-the-art dynamical <span class="hlt">ice</span> <span class="hlt">sheet</span> model and provide detailed downloadable lesson plans, which incorporate this model and are consistent with NGSS Physical Science criteria for different grade bands (K-2, 3-5, 6-8, and 9-12). The ultimate goal of this website is to improve public climate science literacy, especially in regards to the crucial role of the polar <span class="hlt">ice</span> <span class="hlt">sheets</span> in Earth's climate and sea level. The model used will be the <span class="hlt">Ice</span> <span class="hlt">Sheet</span> System Model (ISSM), an <span class="hlt">ice</span> flow model developed at NASA's Jet Propulsion Laboratory and UC Irvine, that simulates the near-term evolution of polar <span class="hlt">ice</span> <span class="hlt">sheets</span> (Greenland and Antarctica) and includes high spatial resolution capabilities and data assimilation to produce realistic simulations of <span class="hlt">ice</span> <span class="hlt">sheet</span> dynamics at the continental scale. Open sourced since 2011, ISSM is used in cutting edge cryosphere research around the globe. Thru I-Lab, students will be able to access ISSM using a simple, online graphical interface that can be launched from a web browser on a computer, tablet or smart phone. The interface will allow users to select different climate conditions and watch how the polar <span class="hlt">ice</span> <span class="hlt">sheets</span> evolve in time under those conditions. Lesson contents will include links to background material and activities that teach observation recording, concept articulation, hypothesis formulation and testing, and</p> </li> <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> <span class="hlt">sheets</span> 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> <span class="hlt">sheets</span>: Once these <span class="hlt">ice</span> masses 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> <span class="hlt">sheet</span> and the West Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span>. PMID:19884496</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/10903198','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/10903198"><span>Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span>: High-Elevation Balance and Peripheral Thinning.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Krabill; Abdalati; Frederick; Manizade; Martin; Sonntag; Swift; Thomas; Wright; Yungel</p> <p>2000-07-21</p> <p>Aircraft laser-altimeter surveys over northern Greenland in 1994 and 1999 have been coupled with previously reported data from southern Greenland to analyze the recent mass-balance of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span>. Above 2000 meters elevation, the <span class="hlt">ice</span> <span class="hlt">sheet</span> is in balance on average but has some regions of local thickening or thinning. Thinning predominates at lower elevations, with rates exceeding 1 meter per year close to the coast. Interpolation of our results between flight lines indicates a net loss of about 51 cubic kilometers of <span class="hlt">ice</span> per year from the entire <span class="hlt">ice</span> <span class="hlt">sheet</span>, sufficient to raise sea level by 0.13 millimeter per year-approximately 7% of the observed rise.</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> <span class="hlt">Sheet</span></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>Mass-balance analysis of the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> 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 mass loss at lower elevations (<2000 m) of the <span class="hlt">ice</span> <span class="hlt">sheet</span>, 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 mass loss at the <span class="hlt">ice-sheet</span> 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> <span class="hlt">sheet</span> agrees with the observations, which implies that the strong mass loss since the early 2000s at low elevations has had a dynamic impact on the entire <span class="hlt">ice</span> <span class="hlt">sheet</span>. The modeling results also suggest that even if the large mass loss at the margins stopped, the interior <span class="hlt">ice</span> <span class="hlt">sheet</span> 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_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/2060/20110008454','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110008454"><span>Freeboard, <span class="hlt">Snow</span> Depth and Sea-<span class="hlt">Ice</span> Roughness in East Antarctica from In Situ and Multiple Satellite Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Markus, Thorsten; Masson, Robert; Worby, Anthony; Lytle, Victoria; Kurtz, Nathan; Maksym, Ted</p> <p>2011-01-01</p> <p>In October 2003 a campaign on board the Australian icebreaker Aurora Australis had the objective to validate standard Aqua Advanced Microwave Scanning Radiometer (AMSR-E) sea-<span class="hlt">ice</span> products. Additionally, the satellite laser altimeter on the <span class="hlt">Ice</span>, Cloud and land Elevation Satellite (ICESat) was in operation. To capture the large-scale information on the sea-<span class="hlt">ice</span> conditions necessary for satellite validation, the measurement strategy was to obtain large-scale sea-<span class="hlt">ice</span> statistics using extensive sea-<span class="hlt">ice</span> measurements in a Lagrangian approach. A drifting buoy array, spanning initially 50 km 100 km, was surveyed during the campaign. In situ measurements consisted of 12 transects, 50 500 m, with detailed <span class="hlt">snow</span> and <span class="hlt">ice</span> measurements as well as random <span class="hlt">snow</span> depth sampling of floes within the buoy array using helicopters. In order to increase the amount of coincident in situ and satellite data an approach has been developed to extrapolate measurements in time and in space. Assuming no change in <span class="hlt">snow</span> depth and freeboard occurred during the period of the campaign on the floes surveyed, we use buoy <span class="hlt">ice</span>-drift information as well as daily estimates of thin-<span class="hlt">ice</span> fraction and rough-<span class="hlt">ice</span> vs smooth-<span class="hlt">ice</span> fractions from AMSR-E and QuikSCAT, respectively, to estimate kilometer-scale <span class="hlt">snow</span> depth and freeboard for other days. The results show that ICESat freeboard estimates have a mean difference of 1.8 cm when compared with the in situ data and a correlation coefficient of 0.6. Furthermore, incorporating ICESat roughness information into the AMSR-E <span class="hlt">snow</span> depth algorithm significantly improves <span class="hlt">snow</span> depth retrievals. <span class="hlt">Snow</span> depth retrievals using a combination of AMSR-E and ICESat data agree with in situ data with a mean difference of 2.3 cm and a correlation coefficient of 0.84 with a negligible bias.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.B13K..05H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.B13K..05H"><span>Inorganic carbon addition stimulates <span class="hlt">snow</span> algae primary productivity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hamilton, T. L.; Havig, J. R.</p> <p>2017-12-01</p> <p>Earth has experienced glacial/interglacial oscillations throughout its history. Today over 15 million square kilometers (5.8 million square miles) of Earth's land surface is covered in <span class="hlt">ice</span> including glaciers, <span class="hlt">ice</span> caps, and the <span class="hlt">ice</span> <span class="hlt">sheets</span> of Greenland and Antarctica, most of which are retreating as a consequence of increased atmospheric CO2. Glaciers are teeming with life and supraglacial <span class="hlt">snow</span> and <span class="hlt">ice</span> surfaces are often red due to blooms of photoautotrophic algae. Recent evidence suggests the red pigmentation, secondary carotenoids produced in part to thrive under high irradiation, lowers albedo and accelerates melt. However, there are relatively few studies that report the productivity of <span class="hlt">snow</span> algae communities and the parameters that constrain their growth on <span class="hlt">snow</span> and <span class="hlt">ice</span> surfaces. Here, we demonstrate that <span class="hlt">snow</span> algae primary productivity can be stimulated by the addition of inorganic carbon. We found an increase in light-dependent carbon assimilation in <span class="hlt">snow</span> algae microcosms amended with increasing amounts of inorganic carbon. Our <span class="hlt">snow</span> algae communities were dominated by typical cosmopolitan <span class="hlt">snow</span> algae species recovered from Alpine and Arctic environments. The climate feedbacks necessary to enter and exit glacial/interglacial oscillations are poorly understood. Evidence and models agree that global Snowball events are accompanied by changes in atmospheric CO2 with increasing CO2 necessary for entering periods of interglacial time. Our results demonstrate a positive feedback between increased CO2 and <span class="hlt">snow</span> algal productivity and presumably growth. With the recent call for bio-albedo effects to be considered in climate models, our results underscore the need for robust climate models to include feedbacks between supraglacial primary productivity, albedo, and atmospheric CO2.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C13E0999L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C13E0999L"><span>Supporting <span class="hlt">Snow</span> Research: <span class="hlt">Snow</span>Ex Data and Services at the NASA National <span class="hlt">Snow</span> and <span class="hlt">Ice</span> Data Center DAAC</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Leon, A.; Tanner, S.; Deems, J. S.</p> <p>2017-12-01</p> <p>The National <span class="hlt">Snow</span> and <span class="hlt">Ice</span> Data Center Distributed Active Archive Center (NSIDC DAAC), part of the Cooperative Institute for Research in Environmental Sciences (CIRES) at the University of Colorado Boulder, will archive and distribute all primary data sets collected during the NASA <span class="hlt">Snow</span>Ex campaigns. NSIDC DAAC's overarching goal for <span class="hlt">Snow</span>Ex data management is to steward the diverse <span class="hlt">Snow</span>Ex data sets to provide a reliable long-term archive, to enable effective data discovery, retrieval, and usage, and to support end user engagement. This goal will be achieved though coordination and collaboration with <span class="hlt">Snow</span>Ex project management and investigators. NSIDC DAAC's core functions for <span class="hlt">Snow</span>Ex data management include: Data Creation: Advise investigators on data formats and structure as well as metadata creation and content to enable preservation, usability, and discoverability. Data Documentation: Develop comprehensive data set documentation describing the instruments, data collection and derivation methods, and data file contents. Data Distribution: Provide discovery and access through NSIDC and NASA data portals to make <span class="hlt">Snow</span>Ex data available to a broad user community Data & User Support: Assist user communities with the selection and usage of <span class="hlt">Snow</span>Ex data products. In an effort to educate and broaden the <span class="hlt">Snow</span>Ex user community, we will present an overview of the <span class="hlt">Snow</span>Ex data products, tools, and services which will be available at the NSIDC DAAC. We hope to gain further insight into how the DAAC can enable the user community to seamlessly and effectively utilize <span class="hlt">Snow</span>Ex data in their research and applications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12208033','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12208033"><span>Influence of <span class="hlt">ice</span> and <span class="hlt">snow</span> covers on the UV exposure of terrestrial microbial communities: dosimetric studies.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cockell, Charles S; Rettberg, Petra; Horneck, Gerda; Wynn-Williams, David D; Scherer, Kerstin; Gugg-Helminger, Anton</p> <p>2002-08-01</p> <p>Bacillus subtilis spore biological dosimeters and electronic dosimeters were used to investigate the exposure of terrestrial microbial communities in micro-habitats covered by <span class="hlt">snow</span> and <span class="hlt">ice</span> in Antarctica. The melting of <span class="hlt">snow</span> covers of between 5- and 15-cm thickness, depending on age and heterogeneity, could increase B. subtilis spore inactivation by up to an order of magnitude, a relative increase twice that caused by a 50% ozone depletion. Within the <span class="hlt">snow</span>-pack at depths of less than approximately 3 cm <span class="hlt">snow</span> algae could receive two to three times the DNA-weighted irradiance they would receive on bare ground. At the edge of the <span class="hlt">snow</span>-pack, warming of low albedo soils resulted in the formation of overhangs that provided transient UV protection to thawed and growing microbial communities on the soils underneath. In shallow aquatic habitats, thin layers of heterogeneous <span class="hlt">ice</span> of a few millimetres thickness were found to reduce DNA-weighted irradiances by up to 55% compared to full-sky values with equivalent DNA-weighted diffuse attenuation coefficients (K(DNA)) of >200 m(-1). A 2-mm <span class="hlt">snow</span>-encrusted <span class="hlt">ice</span> cover on a pond was equivalent to 10 cm of <span class="hlt">ice</span> on a perennially <span class="hlt">ice</span> covered lake. <span class="hlt">Ice</span> covers also had the effect of stabilizing the UV exposure, which was often subject to rapid variations of up to 33% of the mean value caused by wind-rippling of the water surface. These data show that changing <span class="hlt">ice</span> and <span class="hlt">snow</span> covers cause relative changes in microbial UV exposure at least as great as those caused by changing ozone column abundance. Copyright 2002 Elsevier Science B.V.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AREPS..43..207A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AREPS..43..207A"><span>Oceanic Forcing of <span class="hlt">Ice-Sheet</span> Retreat: West Antarctica and More</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alley, Richard B.; Anandakrishnan, Sridhar; Christianson, Knut; Horgan, Huw J.; Muto, Atsu; Parizek, Byron R.; Pollard, David; Walker, Ryan T.</p> <p>2015-05-01</p> <p>Ocean-<span class="hlt">ice</span> interactions have exerted primary control on the Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> and parts of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span>, and will continue to do so in the near future, especially through melting of <span class="hlt">ice</span> shelves and calving cliffs. Retreat in response to increasing marine melting typically exhibits threshold behavior, with little change for forcing below the threshold but a rapid, possibly delayed shift to a reduced state once the threshold is exceeded. For Thwaites Glacier, West Antarctica, the threshold may already have been exceeded, although rapid change may be delayed by centuries, and the reduced state will likely involve loss of most of the West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span>, causing >3 m of sea-level rise. Because of shortcomings in physical understanding and available data, uncertainty persists about this threshold and the subsequent rate of change. Although sea-level histories and physical understanding allow the possibility that <span class="hlt">ice-sheet</span> response could be quite fast, no strong constraints are yet available on the worst-case scenario. Recent work also suggests that the Greenland and East Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheets</span> share some of the same vulnerabilities to shrinkage from marine influence.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.C13D..06G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.C13D..06G"><span>The response of grounded <span class="hlt">ice</span> to ocean temperature forcing in a coupled <span class="hlt">ice</span> <span class="hlt">sheet-ice</span> shelf-ocean cavity model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goldberg, D. N.; Little, C. M.; Sergienko, O. V.; Gnanadesikan, A.</p> <p>2010-12-01</p> <p><span class="hlt">Ice</span> shelves provide a pathway for the heat content of the ocean to influence continental <span class="hlt">ice</span> <span class="hlt">sheets</span>. Changes in the rate or location of basal melting can alter their geometry and effect changes in stress conditions at the grounding line, leading to a grounded <span class="hlt">ice</span> response. Recent observations of <span class="hlt">ice</span> streams and <span class="hlt">ice</span> shelves in the Amundsen Sea sector of West Antarctica have been consistent with this story. On the other hand, <span class="hlt">ice</span> dynamics in the grounding zone control flux into the shelf and thus <span class="hlt">ice</span> shelf geometry, which has a strong influence on the circulation in the cavity beneath the shelf. Thus the coupling between the two systems, ocean and <span class="hlt">ice</span> <span class="hlt">sheet-ice</span> shelf, can be quite strong. We examine the response of the <span class="hlt">ice</span> <span class="hlt">sheet-ice</span> shelf-ocean cavity system to changes in ocean temperature using a recently developed coupled model. The coupled model consists a 3-D ocean model (GFDL's Generalized Ocean Layered Dynamics model, or GOLD) to a two-dimensional <span class="hlt">ice</span> <span class="hlt">sheet-ice</span> shelf model (Goldberg et al, 2009), and allows for changing cavity geometry and a migrating grounding line. Steady states of the coupled system are found even under considerable forcing. The <span class="hlt">ice</span> shelf morphology and basal melt rate patterns of the steady states exhibit detailed structure, and furthermore seem to be unique and robust. The relationship between temperature forcing and area-averaged melt rate is influenced by the response of <span class="hlt">ice</span> shelf morphology to thermal forcing, and is found to be sublinear in the range of forcing considered. However, results suggest that area-averaged melt rate is not the best predictor of overall system response, as grounding line stability depends on local aspects of the basal melt field. Goldberg, D N, D M Holland and C G Schoof, 2009. Grounding line movement and <span class="hlt">ice</span> shelf buttressing in marine <span class="hlt">ice</span> <span class="hlt">sheets</span>, Journal of Geophysical Research-Earth Surfaces, 114, F04026.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014SolE....5..569A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014SolE....5..569A"><span>Future Antarctic bed topography and its implications for <span class="hlt">ice</span> <span class="hlt">sheet</span> dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Adhikari, S.; Ivins, E. R.; Larour, E.; Seroussi, H.; Morlighem, M.; Nowicki, S.</p> <p>2014-06-01</p> <p>The Antarctic bedrock is evolving as the solid Earth responds to the past and ongoing evolution of the <span class="hlt">ice</span> <span class="hlt">sheet</span>. A recently improved <span class="hlt">ice</span> loading history suggests that the Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (AIS) has generally been losing its mass since the Last Glacial Maximum. In a sustained warming climate, the AIS is predicted to retreat at a greater pace, primarily via melting beneath the <span class="hlt">ice</span> shelves. We employ the glacial isostatic adjustment (GIA) capability of the <span class="hlt">Ice</span> <span class="hlt">Sheet</span> System Model (ISSM) to combine these past and future <span class="hlt">ice</span> loadings and provide the new solid Earth computations for the AIS. We find that past loading is relatively less important than future loading for the evolution of the future bed topography. Our computations predict that the West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (WAIS) may uplift by a few meters and a few tens of meters at years AD 2100 and 2500, respectively, and that the East Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> is likely to remain unchanged or subside minimally except around the Amery <span class="hlt">Ice</span> Shelf. The Amundsen Sea Sector in particular is predicted to rise at the greatest rate; one hundred years of <span class="hlt">ice</span> evolution in this region, for example, predicts that the coastline of Pine Island Bay will approach roughly 45 mm yr-1 in viscoelastic vertical motion. Of particular importance, we systematically demonstrate that the effect of a pervasive and large GIA uplift in the WAIS is generally associated with the flattening of reverse bed slope, reduction of local sea depth, and thus the extension of grounding line (GL) towards the continental shelf. Using the 3-D higher-order <span class="hlt">ice</span> flow capability of ISSM, such a migration of GL is shown to inhibit the <span class="hlt">ice</span> flow. This negative feedback between the <span class="hlt">ice</span> <span class="hlt">sheet</span> and the solid Earth may promote stability in marine portions of the <span class="hlt">ice</span> <span class="hlt">sheet</span> in the future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014SolED...6..191A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014SolED...6..191A"><span>Future Antarctic bed topography and its implications for <span class="hlt">ice</span> <span class="hlt">sheet</span> dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Adhikari, S.; Ivins, E.; Larour, E.; Seroussi, H.; Morlighem, M.; Nowicki, S.</p> <p>2014-01-01</p> <p>The Antarctic bedrock is evolving as the solid Earth responds to the past and ongoing evolution of the <span class="hlt">ice</span> <span class="hlt">sheet</span>. A~recently improved <span class="hlt">ice</span> loading history suggests that the Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (AIS) is generally losing its mass since the last glacial maximum (LGM). In a sustained warming climate, the AIS is predicted to retreat at a greater pace primarily via melting beneath the <span class="hlt">ice</span> shelves. We employ the glacial isostatic adjustment (GIA) capability of the <span class="hlt">Ice</span> <span class="hlt">Sheet</span> System Model (ISSM) to combine these past and future <span class="hlt">ice</span> loadings and provide the new solid Earth computations for the AIS. We find that the past loading is relatively less important than future loading on the evolution of the future bed topography. Our computations predict that the West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (WAIS) may uplift by a few meters and a few tens of meters at years 2100 and 2500 AD, respectively, and that the East Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (EAIS) is likely to remain unchanged or subside minimally except around the Amery <span class="hlt">Ice</span> Shelf. The Amundsen Sea Sector in particular is predicted to rise at the greatest rate; one hundred years of <span class="hlt">ice</span> evolution in this region, for example, predicts that the coastline of Pine Island Bay approaches roughly 45 mm yr-1 in viscoelastic vertical motion. Of particular importance, we systematically demonstrate that the effect of a pervasive and large GIA uplift in the WAIS is associated with the flattening of reverse bed, reduction of local sea depth, and thus the extension of grounding line (GL) towards the continental shelf. Using the 3-D higher-order <span class="hlt">ice</span> flow capability of ISSM, such a migration of GL is shown to inhibit the <span class="hlt">ice</span> flow. This negative feedback between the <span class="hlt">ice</span> <span class="hlt">sheet</span> and the solid Earth may promote the stability to marine portions of the <span class="hlt">ice</span> <span class="hlt">sheet</span> in future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140017427','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140017427"><span>Future Antarctic Bed Topography and Its Implications for <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Dynamics</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Adhikari, Surendra; Ivins, Erik R.; Larour, Eric Y.; Seroussi, Helene L.; Morlighem, Mathieu; Nowicki, S.</p> <p>2014-01-01</p> <p>The Antarctic bedrock is evolving as the solid Earth responds to the past and ongoing evolution of the <span class="hlt">ice</span> <span class="hlt">sheet</span>. A recently improved <span class="hlt">ice</span> loading history suggests that the Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (AIS) has generally been losing its mass since the Last Glacial Maximum. In a sustained warming climate, the AIS is predicted to retreat at a greater pace, primarily via melting beneath the <span class="hlt">ice</span> shelves.We employ the glacial isostatic adjustment (GIA) capability of the <span class="hlt">Ice</span> <span class="hlt">Sheet</span> System Model (ISSM) to combine these past and future <span class="hlt">ice</span> loadings and provide the new solid Earth computations for the AIS.We find that past loading is relatively less important than future loading for the evolution of the future bed topography. Our computations predict that the West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (WAIS) may uplift by a few meters and a few tens of meters at years AD 2100 and 2500, respectively, and that the East Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> is likely to remain unchanged or subside minimally except around the Amery <span class="hlt">Ice</span> Shelf. The Amundsen Sea Sector in particular is predicted to rise at the greatest rate; one hundred years of <span class="hlt">ice</span> evolution in this region, for example, predicts that the coastline of Pine Island Bay will approach roughly 45mmyr-1 in viscoelastic vertical motion. Of particular importance, we systematically demonstrate that the effect of a pervasive and large GIA uplift in the WAIS is generally associated with the flattening of reverse bed slope, reduction of local sea depth, and thus the extension of grounding line (GL) towards the continental shelf. Using the 3-D higher-order <span class="hlt">ice</span> flow capability of ISSM, such a migration of GL is shown to inhibit the <span class="hlt">ice</span> flow. This negative feedback between the <span class="hlt">ice</span> <span class="hlt">sheet</span> and the solid Earth may promote stability in marine portions of the <span class="hlt">ice</span> <span class="hlt">sheet</span> in the future.</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> <span class="hlt">Sheet</span> 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> <span class="hlt">Sheet</span> for 1978-2014, partitioned into changes due to surface processes and <span class="hlt">ice</span> dynamics. Elevation changes are computed from all available stereoscopic DEMs, and laser altimetry data (ICESat, ATM, LVIS). Surface Mass Balance and firn-compaction estimates are from RACMO2.3. Originating nearly at the divide of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (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> <span class="hlt">sheet</span> 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> <span class="hlt">sheet</span>. These thickness changes, often occurring at the onset of fast flow, could indicate rapid variations of basal lubrication due to rerouting of subglacial drainage. We investigate the possible causes of the observed spatiotemporal pattern of <span class="hlt">ice</span> <span class="hlt">sheet</span> elevation changes using the <span class="hlt">Ice</span> <span class="hlt">Sheet</span> 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/2014TCD.....8.4737M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014TCD.....8.4737M"><span>Bimodal albedo distributions in the ablation zone of the southwestern Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moustafa, S. E.; Rennermalm, A. K.; Smith, L. C.; Miller, M. A.; Mioduszewski, J. R.</p> <p>2014-09-01</p> <p>Surface albedo is a key variable controlling solar radiation absorbed at the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (GrIS) surface, and thus, meltwater production. Recent decline in surface albedo over the GrIS has been linked to enhanced <span class="hlt">snow</span> grain metamorphic rates and amplified <span class="hlt">ice</span>-albedo feedback from atmospheric warming. However, the importance of distinct surface types on ablation zone albedo and meltwater production is still relatively unknown, and excluded in surface mass balance models. In this study, we analyze albedo and ablation rates using in situ and remotely-sensed data. Observations include: (1) a new high-quality in situ spectral albedo dataset collected with an Analytical Spectral Devices (ASD) spectroradiometer measuring at 325-1075 nm, along a 1.25 km transect during three days in June 2013; (2) broadband albedo at two automatic weather stations; and (3) daily MODerate Resolution Imaging Spectroradiometer (MODIS) albedo (MOD10A1) between 31 May and 30 August. We find that seasonal ablation zone albedos have a bimodal distribution, with two alternate states. This suggests that an abrupt switch from high to low albedo can be triggered by a modest melt event, resulting in amplified surface ablation rates. Our results show that such a shift corresponds to an observed melt rate percent difference increase of 51.6% during peak melt season (between 10-14 and 20-24 July 2013). Furthermore, our findings demonstrate that seasonal changes in GrIS ablation zone albedo are not exclusively a function of a darkening surface from <span class="hlt">ice</span> crystal growth, but rather are controlled by changes in the fractional coverage of <span class="hlt">snow</span>, bare <span class="hlt">ice</span>, and impurity-rich surface types. As the climate continues to warm, regional climate models should consider the seasonal evolution of <span class="hlt">ice</span> surface types in Greenland's ablation zone to improve projections of mass loss contributions to sea level rise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.C13A0407M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.C13A0407M"><span>Bimodal Albedo Distributions in the Ablation Zone of the Southwestern Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moustafa, S.; Rennermalm, A. K.; Smith, L. C.; Miller, M. A.; Mioduszewski, J.; Koenig, L.</p> <p>2014-12-01</p> <p>Surface albedo is a key variable controlling solar radiation absorbed at the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (GrIS) surface, and thus meltwater production. Recent decline in surface albedo over the GrIS has been linked to enhanced <span class="hlt">snow</span> grain metamorphic rates and amplified <span class="hlt">ice</span>-albedo feedback from atmospheric warming. However, the importance of distinct surface types on ablation zone albedo and meltwater production is still relatively unknown, and excluded in surface mass balance models. In this study, we analyze albedo and ablation rates (m d-1) using in situ and remotely-sensed data. Observations include: 1) a new high-quality in situ spectral albedo dataset collected with an Analytical Spectral Devices (ASD) spectroradiometer measuring at 325-1075 nm, along a 1.25 km transect during three days in June 2013; 2) broadband albedo at two automatic weather stations; and 3) daily MODerate Resolution Imaging Spectroradiometer (MODIS) albedo (MOD10A1) between 31 May and 30 August. We find that seasonal ablation zone albedos have a bimodal distribution, with two alternate states. This suggests that an abrupt switch from high to low albedo can be triggered by a modest melt event, resulting in amplified ablation rates. Our results show that such a shift corresponds to an observed melt rate percent difference increase of 51.6% during peak melt season (between 10-14 July and 20-24 July, 2013). Furthermore, our findings demonstrate that seasonal changes in GrIS ablation zone albedo are not exclusively a function of a darkening surface from <span class="hlt">ice</span> crystal growth, but rather are controlled by changes in the fractional coverage of <span class="hlt">snow</span>, bare <span class="hlt">ice</span>, and impurity-rich surface types. As the climate continues to warm, regional climate models should consider the seasonal evolution of <span class="hlt">ice</span> surface types in Greenland's ablation zone to improve projections of mass loss contributions to sea level rise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.U22A..02H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.U22A..02H"><span>An Imminent Revolution in Modeling Interactions of <span class="hlt">Ice</span> <span class="hlt">Sheets</span> With Climate</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hughes, T.</p> <p>2008-12-01</p> <p>Modeling continental <span class="hlt">ice</span> <span class="hlt">sheets</span> was inaugurated by meteorologists William Budd and Uwe Radok, with mathematician Richard Jenssen, in 1971. Their model calculated the thermal and mechanical regime using measured surface accumulation rates, temperatures, and elevations, and bed topography. This top-down approach delivered a basal thermal regime of temperatures or melting rates for an assumed basal geothermal heat flux. When Philippe Huybrechts and others incorporated time, largely unknownpast surface conditions had a major effect on present basal thermal conditions. This approach produced <span class="hlt">ice-sheet</span> models with only a slow response to external forcing, whereas the glacial geological record and climate records from <span class="hlt">ice</span> and ocean cores show that <span class="hlt">ice</span> <span class="hlt">sheets</span> can have rapid changes in size and shape independent of external forcing. These top-down models were wholly inadequate for reconstructing former <span class="hlt">ice</span> <span class="hlt">sheets</span> at the LGM for CLIMAP in 1981. <span class="hlt">Ice-sheet</span> areas,elevations, and volumes provided the albedo, surface topography, and sea-surface area as input to climate models. A bottom-up model based on dated glacial geology was developed to provide the areal extent and basal thermal regime of <span class="hlt">ice</span> <span class="hlt">sheets</span> at the LGM. Basal thermal conditions determined <span class="hlt">ice</span>-bed coupling and therefore the elevation of <span class="hlt">ice</span> <span class="hlt">sheets</span>. High convex <span class="hlt">ice</span> surfaces for slow <span class="hlt">sheet</span> flow lower about 20 percent when a frozen bed becomes thawed. As further basal melting drowns bedrock bumps that "pin" basal <span class="hlt">ice</span>, the <span class="hlt">ice</span> surface becomes concave in fast stream flow that ends as low floating <span class="hlt">ice</span> shelves at marine <span class="hlt">ice</span> margins. A revolution in modeling interactions between glaciation, climate, and sea level is driven by new Greenland and Antarctic data from Earth-orbiting satellites, airborne and surface traverses, and deep drilling. We anticipate continuous data acquisition of surface albedo, accumulation/ablation rates, elevations, velocities, and temperatures over a whole <span class="hlt">ice</span> <span class="hlt">sheet</span>, mapping basal thermal conditions</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C41B0670T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C41B0670T"><span>Estimating the impact of internal climate variability on <span class="hlt">ice</span> <span class="hlt">sheet</span> model simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tsai, C. Y.; Forest, C. E.; Pollard, D.</p> <p>2016-12-01</p> <p>Rising sea level threatens human societies and coastal habitats and melting <span class="hlt">ice</span> <span class="hlt">sheets</span> are a major contributor to sea level rise (SLR). Thus, understanding uncertainty of both forcing and variability within the climate system is essential for assessing long-term risk of SLR given their impact on <span class="hlt">ice</span> <span class="hlt">sheet</span> evolution. The predictability of polar climate is limited by uncertainties from the given forcing, the climate model response to this forcing, and the internal variability from feedbacks within the fully coupled climate system. Among those sources of uncertainty, the impact of internal climate variability on <span class="hlt">ice</span> <span class="hlt">sheet</span> changes has not yet been robustly assessed. Here we investigate how internal variability affects <span class="hlt">ice</span> <span class="hlt">sheet</span> projections using climate fields from two Community Earth System Model (CESM) large-ensemble (LE) experiments to force a three-dimensional <span class="hlt">ice</span> <span class="hlt">sheet</span> model. Each ensemble member in an LE experiment undergoes the same external forcings but with unique initial conditions. We find that for both LEs, 2m air temperature variability over Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> (GrIS) can lead to significantly different <span class="hlt">ice</span> <span class="hlt">sheet</span> responses. Our results show that the internal variability from two fully coupled CESM LEs can cause about 25 35 mm differences of GrIS's contribution to SLR in 2100 compared to present day (about 20% of the total change), and 100m differences of SLR in 2300. Moreover, only using ensemble-mean climate fields as the forcing in <span class="hlt">ice</span> <span class="hlt">sheet</span> model can significantly underestimate the melt of GrIS. As the Arctic region becomes warmer, the role of internal variability is critical given the complex nonlinear interactions between surface temperature and <span class="hlt">ice</span> <span class="hlt">sheet</span>. Our results demonstrate that internal variability from coupled atmosphere-ocean general circulation model can affect <span class="hlt">ice</span> <span class="hlt">sheet</span> simulations and the resulting sea-level projections. This study highlights an urgent need to reassess associated uncertainties of projecting <span class="hlt">ice</span> <span class="hlt">sheet</span> loss over the next few</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Natur.541...72B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Natur.541...72B"><span>Centennial-scale Holocene climate variations amplified by Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> 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> <span class="hlt">sheets</span> 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> <span class="hlt">Sheet</span> 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> <span class="hlt">Sheet</span> 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> <span class="hlt">Sheet</span>, and performed both high-spatial-resolution <span class="hlt">ice-sheet</span> modelling of the Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> and multi-millennial global climate model simulations. <span class="hlt">Ice-sheet</span> 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> <span class="hlt">Sheet</span> 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('http://adsabs.harvard.edu/abs/2004AGUFM.C34A..02S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUFM.C34A..02S"><span>Landform Formation Under <span class="hlt">Ice</span> <span class="hlt">Sheets</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schoof, C. G.; Ng, F. S.; Hallet, B.</p> <p>2004-12-01</p> <p>We present a new mathematical model for the formation of subglacial landforms such as drumlins under a warm-based, soft-bedded <span class="hlt">ice</span> <span class="hlt">sheet</span>. At the heart of the model is a channelized drainage system in which smaller channels grow at the expense of larger ones, leading to the continuous creation and extinction of drainage paths, and to a spatially distributed imprint on the landscape. We demonstrate how interactions between such a drainage system, bed topography and <span class="hlt">ice</span> flow can lead to the spontaneous formation of subglacial landforms, and discuss the effect of different sediment transport characteristics in the drainage system on the shape and migration of these landforms. This mathematical model is the first component of a study of landscape/<span class="hlt">ice-sheet</span> self-organization, which is inspired and guided, in part, by new digital topographic data (LIDAR) that are revealing with unprecedented detail the striking grain of glacially scoured topography on length scales ranging from 0.5 to 20 km.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C21A0687M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C21A0687M"><span>Decadal-Scale Response of the Antarctic <span class="hlt">Ice</span> <span class="hlt">sheet</span> to a Warming Ocean using the POPSICLES Coupled <span class="hlt">Ice</span> <span class="hlt">Sheet</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>Martin, D. F.; Asay-Davis, X.; Cornford, S. L.; Price, S. F.; Ng, E. G.; Collins, W.</p> <p>2015-12-01</p> <p>We present POPSICLES simulation results covering the full Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> and the Southern Ocean spanning the period from 1990 to 2010. We use the CORE v. 2 interannual forcing data to force the ocean model. Simulations are performed at 0.1o(~5 km) ocean resolution with adaptive <span class="hlt">ice</span> <span class="hlt">sheet</span> resolution as fine as 500 m to adequately resolve the grounding line dynamics. We discuss the effect of improved ocean mixing and subshelf bathymetry (vs. the standard Bedmap2 bathymetry) on the behavior of the coupled system, comparing time-averaged melt rates below a number of major <span class="hlt">ice</span> shelves with those reported in the literature. We also present seasonal variability and decadal melting trends from several Antarctic regions, along with the response of the <span class="hlt">ice</span> shelves and the consequent dynamic response of the grounded <span class="hlt">ice</span> <span class="hlt">sheet</span>.POPSICLES couples the POP2x ocean model, a modified version of the Parallel Ocean Program, and the BISICLES <span class="hlt">ice-sheet</span> model. POP2x includes sub-<span class="hlt">ice</span>-shelf circulation using partial top cells and the commonly used three-equation boundary layer physics. Standalone POP2x output compares well with standard <span class="hlt">ice</span>-ocean test cases (e.g., ISOMIP) and other continental-scale simulations and melt-rate observations. BISICLES makes use of adaptive mesh refinement and a 1st-order accurate momentum balance similar to the L1L2 model of Schoof and Hindmarsh to accurately model regions of dynamic complexity, such as <span class="hlt">ice</span> streams, outlet glaciers, and grounding lines. Results of BISICLES simulations have compared favorably to comparable simulations with a Stokes momentum balance in both idealized tests (MISMIP-3d) and realistic configurations.The figure shows the BISICLES-computed vertically-integrated grounded <span class="hlt">ice</span> velocity field 5 years into a 20-year coupled full-continent Antarctic-Southern-Ocean simulation. Submarine melt rates are painted onto the surface of the floating <span class="hlt">ice</span> shelves. Grounding lines are shown in green.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004AGUSM.C42A..01S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUSM.C42A..01S"><span>ICESat's First Year of Measurements Over the Polar <span class="hlt">Ice</span> <span class="hlt">Sheets</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shuman, C. A.</p> <p>2004-05-01</p> <p>NASA's <span class="hlt">Ice</span>, Cloud and Land Elevation Satellite (ICESat) mission was developed to measure changes in elevation of the Greenland and Antarctic <span class="hlt">ice</span> <span class="hlt">sheets</span>. Its primary mission goal is to significantly refine estimates of polar <span class="hlt">ice</span> <span class="hlt">sheet</span> mass balance. Obtaining precise, spatially dense, <span class="hlt">ice</span> <span class="hlt">sheet</span> elevations through time is the first step towards this goal. ICESat data will then enable study of associations between observed <span class="hlt">ice</span> changes and dynamic or climatic forcing factors, and thus enable improved estimation of the present and future contributions of the <span class="hlt">ice</span> <span class="hlt">sheets</span> to global sea level rise. ICESat was launched on January 12, 2003 and acquired science data from February 20th to March 29th with the first of the three lasers of the Geoscience Laser Altimeter System (GLAS). Data acquisition with the second laser began on September 25th and continued until November 18th, 2003. For one-year change detection, the second laser is scheduled for operation from approximately February 17th to March 20th, 2004. Additional operational periods will be selected to 1) enable periodic measurements through the year, and 2) to support of other NASA Earth Science Enterprise missions and activities. To obtain these precise <span class="hlt">ice</span> <span class="hlt">sheet</span> elevations, GLAS has a 1064 nm wavelength laser operating at 40 Hz with a designed range precision of about 10 cm. The laser footprints are about 70 m in diameter on the Earth's surface and are spaced every 172 m along-track. The on-board GPS receiver enables radial orbit determinations to an accuracy better than 5 cm. The star-tracking attitude-determination system will enable laser footprints to be located to 6 m horizontally when attitude calibration is completed. The orbital altitude averages 600 km at an inclination of 94 degrees with coverage extending from 86 degrees N and S latitude. The spacecraft attitude can be controlled to point the laser beam to within 50 m of surface reference tracks over the <span class="hlt">ice</span> <span class="hlt">sheets</span> and to point off-nadir up to 5 degrees to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C33C1209N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C33C1209N"><span>A full year of <span class="hlt">snow</span> on sea <span class="hlt">ice</span> observations and simulations - Plans for MOSAiC 2019/20</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nicolaus, M.; Geland, S.; Perovich, D. K.</p> <p>2017-12-01</p> <p>The <span class="hlt">snow</span> cover on sea on sea <span class="hlt">ice</span> dominates many exchange processes and properties of the <span class="hlt">ice</span> covered polar oceans. It is a major interface between the atmosphere and the sea <span class="hlt">ice</span> with the ocean underneath. <span class="hlt">Snow</span> on sea <span class="hlt">ice</span> is known for its extraordinarily large spatial and temporal variability from micro scales and minutes to basin wide scales and decades. At the same time, <span class="hlt">snow</span> cover properties and even <span class="hlt">snow</span> depth distributions are among the least known and most difficult to observe climate variables. Starting in October 2019 and ending in October 2020, the international MOSAiC drift experiment will allow to observe the evolution of a <span class="hlt">snow</span> pack on Arctic sea <span class="hlt">ice</span> over a full annual cycle. During the drift with one <span class="hlt">ice</span> floe along the transpolar drift, we will study <span class="hlt">snow</span> processes and interactions as one of the main topics of the MOSAiC research program. Thus we will, for the first time, be able to perform such studies on seasonal sea <span class="hlt">ice</span> and relate it to previous expeditions and parallel observations at different locations. Here we will present the current status of our planning of the MOSAiC <span class="hlt">snow</span> program. We will summarize the latest implementation ideas to combine the field observations with numerical simulations. The field program will include regular manual observations and sampling on the main floe of the central observatory, autonomous recordings in the distributed network, airborne observations in the surrounding of the central observatory, and retrievals of satellite remote sensing products. Along with the field program, numerical simulations of the MOSAiC <span class="hlt">snow</span> cover will be performed on different scales, including large-scale interaction with the atmosphere and the sea <span class="hlt">ice</span>. The <span class="hlt">snow</span> studies will also bridge between the different disciplines, including physical, chemical, biological, and geochemical measurements, samples, and fluxes. The main challenge of all measurements will be to accomplish the description of the full annual cycle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C53B1040K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C53B1040K"><span>Spatio-Temporal Variability of Recent <span class="hlt">Snow</span> Accumulation Across the West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Divide Using Ultra-High Frequency Radar and Shallow Firn Cores</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Keeler, D. G.; Rupper, S.; Forster, R. R.; Miège, C.; Brewer, S.; Koenig, L.</p> <p>2017-12-01</p> <p>The West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (WAIS) could be a substantial source of future sea level rise, with 3+ meters of potential increase stored in the <span class="hlt">ice</span> <span class="hlt">sheet</span>. Adequate predictions of WAIS contributions, however, depend on well-constrained surface mass balance estimates for the region. Given the sparsity of available data, such estimates are tenuous. Although new data are periodically added, further research (both to collect more data and better utilize existing data) is critical to addressing these issues. Here we present accumulation data from 9 shallow firn cores and 600 km of Ku band radar traces collected as part of the Satellite Era Antarctic Traverse (SEAT) 2011/2012 field season. Using these data, combined with similar data collected during the SEAT 2010/2011 field season, we investigate the spatial variability in accumulation across the WAIS Divide and surrounding regions. We utilize seismic interpretation and 3D visualization tools to investigate the extent and variations of laterally continuous internal horizons in the radar profiles, and compare the results to nearby firn cores. Previous results show that clearly visible, laterally continuous horizons in radar returns in this area do not always represent annual accumulation isochrones, but can instead represent multi-year or sub-annual events. The automated application of Bayesian inference techniques to averaged estimates of multiple adjacent radar traces, however, can estimate annually-resolved independent age-depth scales for these radar data. We use these same automated techniques on firn core isotopic records to infer past <span class="hlt">snow</span> accumulation rates, allowing a direct comparison with the radar-derived results. Age-depth scales based on manual annual-layer counting of geochemical and isotopic species from these same cores provide validation for the automated approaches. Such techniques could theoretically be applied to additional radar/core data sets in polar regions (e.g. Operation <span class="hlt">Ice</span>Bridge), thereby</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://adsabs.harvard.edu/abs/2011AGUFM.C23B0489B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.C23B0489B"><span>Response of Arctic <span class="hlt">Snow</span> and Sea <span class="hlt">Ice</span> Extents to Melt Season Atmospheric Forcing Across the Land-Ocean Boundary</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bliss, A. C.; Anderson, M. R.</p> <p>2011-12-01</p> <p>Little research has gone into studying the concurrent variations in the annual loss of continental <span class="hlt">snow</span> cover and sea <span class="hlt">ice</span> extent across the land-ocean boundary, however, the analysis of these data averaged spatially over three study regions located in North America and Eastern and Western Russia, reveals a distinct difference in the response of anomalous <span class="hlt">snow</span> and sea <span class="hlt">ice</span> conditions to the atmospheric forcing. This study compares the monthly continental <span class="hlt">snow</span> cover and sea <span class="hlt">ice</span> extent loss in the Arctic, during the melt season months (May-August) for the period 1979-2007, with regional atmospheric conditions known to influence summer melt including: mean sea level pressures, 925 hPa air temperatures, and mean 2 m U and V wind vectors from NCEP/DOE Reanalysis 2. The monthly hemispheric <span class="hlt">snow</span> cover extent data used are from the Rutgers University Global <span class="hlt">Snow</span> Lab and sea <span class="hlt">ice</span> extents for this study are derived from the monthly passive microwave satellite Bootstrap algorithm sea <span class="hlt">ice</span> concentrations available from the National <span class="hlt">Snow</span> and <span class="hlt">Ice</span> Data Center. Three case study years (1985, 1996, and 2007) are used to compare the direct response of monthly anomalous sea <span class="hlt">ice</span> and <span class="hlt">snow</span> cover areal extents to monthly mean atmospheric forcing averaged spatially over the extent of each study region. This comparison is then expanded for all summer months over the 29 year study period where the monthly persistence of sea <span class="hlt">ice</span> and <span class="hlt">snow</span> cover extent anomalies and changes in the sea <span class="hlt">ice</span> and <span class="hlt">snow</span> conditions under differing atmospheric conditions are explored further. The monthly anomalous atmospheric conditions are classified into four categories including: warmer temperatures with higher pressures, warmer temperatures with lower pressures, cooler temperatures with higher pressures, and cooler temperatures with lower pressures. Analysis of the atmospheric conditions surrounding anomalous loss of <span class="hlt">snow</span> and <span class="hlt">ice</span> cover over the independent study regions indicates that conditions of warmer temperatures</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040172041&hterms=balance+sheet&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dbalance%2Bsheet','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040172041&hterms=balance+sheet&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dbalance%2Bsheet"><span>Advances in Measuring Antarctic Sea-<span class="hlt">Ice</span> Thickness and <span class="hlt">Ice-Sheet</span> Elevations with ICESat Laser Altimetry</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zwally, H. Jay</p> <p>2004-01-01</p> <p>NASA's <span class="hlt">Ice</span>, Cloud and Land Elevation Satellite (ICESat) has been measuring elevations of the Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> and sea-<span class="hlt">ice</span> freeboard elevations with unprecedented accuracy. Since February 20,2003, data has been acquired during three periods of laser operation varying from 36 to 54 days, which is less than the continuous operation of 3 to 5 years planned for the mission. The primary purpose of ICESat is to measure time-series of <span class="hlt">ice-sheet</span> elevation changes for determination of the present-day mass balance of the <span class="hlt">ice</span> <span class="hlt">sheets</span>, study of associations between observed <span class="hlt">ice</span> changes and polar climate, and estimation of the present and future contributions of the <span class="hlt">ice</span> <span class="hlt">sheets</span> to global sea level rise. ICESat data will continue to be acquired for approximately 33 days periods at 3 to 6 month intervals with the second of ICESat's three lasers, and eventually with the third laser. The laser footprints are about 70 m on the surface and are spaced at 172 m along-track. The on-board GPS receiver enables radial orbit determinations to an accuracy better than 5 cm. The orbital altitude is around 600 km at an inclination of 94 degrees with a 8-day repeat pattern for the calibration and validation period, followed by a 91 -day repeat period for the rest of the mission. The expected range precision of single footprint measurements was 10 cm, but the actual range precision of the data has been shown to be much better at 2 to 3 cm. The star-tracking attitude-determination system should enable footprints to be located to 6 m horizontally when attitude calibrations are completed. With the present attitude calibration, the elevation accuracy over the <span class="hlt">ice</span> <span class="hlt">sheets</span> ranges from about 30 cm over the low-slope areas to about 80 cm over areas with slopes of 1 to 2 degrees, which is much better than radar altimetry. After the first period of data collection, the spacecraft attitude was controlled to point the laser beam to within 50 m of reference surface tracks over the <span class="hlt">ice</span> <span class="hlt">sheets</span>. Detection of <span class="hlt">ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21637255','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21637255"><span>A dynamic early East Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> suggested by <span class="hlt">ice</span>-covered fjord landscapes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Young, Duncan A; Wright, Andrew P; Roberts, Jason L; Warner, Roland C; Young, Neal W; Greenbaum, Jamin S; Schroeder, Dustin M; Holt, John W; Sugden, David E; Blankenship, Donald D; van Ommen, Tas D; Siegert, Martin J</p> <p>2011-06-02</p> <p>The first Cenozoic <span class="hlt">ice</span> <span class="hlt">sheets</span> initiated in Antarctica from the Gamburtsev Subglacial Mountains and other highlands as a result of rapid global cooling ∼34 million years ago. In the subsequent 20 million years, at a time of declining atmospheric carbon dioxide concentrations and an evolving Antarctic circumpolar current, sedimentary sequence interpretation and numerical modelling suggest that cyclical periods of <span class="hlt">ice-sheet</span> expansion to the continental margin, followed by retreat to the subglacial highlands, occurred up to thirty times. These fluctuations were paced by orbital changes and were a major influence on global sea levels. <span class="hlt">Ice-sheet</span> models show that the nature of such oscillations is critically dependent on the pattern and extent of Antarctic topographic lowlands. Here we show that the basal topography of the Aurora Subglacial Basin of East Antarctica, at present overlain by 2-4.5 km of <span class="hlt">ice</span>, is characterized by a series of well-defined topographic channels within a mountain block landscape. The identification of this fjord landscape, based on new data from <span class="hlt">ice</span>-penetrating radar, provides an improved understanding of the topography of the Aurora Subglacial Basin and its surroundings, and reveals a complex surface sculpted by a succession of <span class="hlt">ice-sheet</span> configurations substantially different from today's. At different stages during its fluctuations, the edge of the East Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> lay pinned along the margins of the Aurora Subglacial Basin, the upland boundaries of which are currently above sea level and the deepest parts of which are more than 1 km below sea level. Although the timing of the channel incision remains uncertain, our results suggest that the fjord landscape was carved by at least two iceflow regimes of different scales and directions, each of which would have over-deepened existing topographic depressions, reversing valley floor slopes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C41B0663K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C41B0663K"><span>Using paleoclimate data to improve models of the Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>King, M. A.; Phipps, S. J.; Roberts, J. L.; White, D.</p> <p>2016-12-01</p> <p><span class="hlt">Ice</span> <span class="hlt">sheet</span> models are the most descriptive tools available to simulate the future evolution of the Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (AIS), including its contribution towards changes in global sea level. However, our knowledge of the dynamics of the coupled <span class="hlt">ice</span>-ocean-lithosphere system is inevitably limited, in part due to a lack of observations. Furthemore, to build computationally efficient models that can be run for multiple millennia, it is necessary to use simplified descriptions of <span class="hlt">ice</span> dynamics. <span class="hlt">Ice</span> <span class="hlt">sheet</span> modeling is therefore an inherently uncertain exercise. The past evolution of the AIS provides an opportunity to constrain the description of physical processes within <span class="hlt">ice</span> <span class="hlt">sheet</span> models and, therefore, to constrain our understanding of the role of the AIS in driving changes in global sea level. We use the Parallel <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model (PISM) to demonstrate how paleoclimate data can improve our ability to predict the future evolution of the AIS. A large, perturbed-physics ensemble is generated, spanning uncertainty in the parameterizations of four key physical processes within <span class="hlt">ice</span> <span class="hlt">sheet</span> models: <span class="hlt">ice</span> rheology, <span class="hlt">ice</span> shelf calving, and the stress balances within <span class="hlt">ice</span> <span class="hlt">sheets</span> and <span class="hlt">ice</span> shelves. A Latin hypercube approach is used to optimally sample the range of uncertainty in parameter values. This perturbed-physics ensemble is used to simulate the evolution of the AIS from the Last Glacial Maximum ( 21,000 years ago) to present. Paleoclimate records are then used to determine which ensemble members are the most realistic. This allows us to use data on past climates to directly constrain our understanding of the past contribution of the AIS towards changes in global sea level. Critically, it also allows us to determine which ensemble members are likely to generate the most realistic projections of the future evolution of the AIS.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20000038172&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=20000038172&hterms=BALANCE+SHEET&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DBALANCE%2BSHEET"><span>Balance Velocities of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Joughin, Ian; Fahnestock, Mark; Ekholm, Simon; Kwok, Ron</p> <p>1997-01-01</p> <p>We present a map of balance velocities for the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span>. The resolution of the underlying DEM, which was derived primarily from radar altimetry data, yields far greater detail than earlier balance velocity estimates for Greenland. The velocity contours reveal in striking detail the location of an <span class="hlt">ice</span> stream in northeastern Greenland, which was only recently discovered using satellite imagery. Enhanced flow associated with all of the major outlets is clearly visible, although small errors in the source data result in less accurate estimates of the absolute flow speeds. Nevertheless, the balance map is useful for <span class="hlt">ice-sheet</span> modelling, mass balance studies, and field planning.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017CliPa..13.1243S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017CliPa..13.1243S"><span>The influence of <span class="hlt">ice</span> <span class="hlt">sheets</span> on temperature during the past 38 million years inferred from a one-dimensional <span class="hlt">ice</span> <span class="hlt">sheet</span>-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>Stap, Lennert B.; van de Wal, Roderik S. W.; de Boer, Bas; Bintanja, Richard; Lourens, Lucas J.</p> <p>2017-09-01</p> <p>Since the inception of the Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> at the Eocene-Oligocene transition (˜ 34 Myr ago), land <span class="hlt">ice</span> has played a crucial role in Earth's climate. Through feedbacks in the climate system, land <span class="hlt">ice</span> variability modifies atmospheric temperature changes induced by orbital, topographical, and greenhouse gas variations. Quantification of these feedbacks on long timescales has hitherto scarcely been undertaken. In this study, we use a zonally averaged energy balance climate model bidirectionally coupled to a one-dimensional <span class="hlt">ice</span> <span class="hlt">sheet</span> model, capturing the <span class="hlt">ice</span>-albedo and surface-height-temperature feedbacks. Potentially important transient changes in topographic boundary conditions by tectonics and erosion are not taken into account but are briefly discussed. The relative simplicity of the coupled model allows us to perform integrations over the past 38 Myr in a fully transient fashion using a benthic oxygen isotope record as forcing to inversely simulate CO2. Firstly, we find that the results of the simulations over the past 5 Myr are dependent on whether the model run is started at 5 or 38 Myr ago. This is because the relation between CO2 and temperature is subject to hysteresis. When the climate cools from very high CO2 levels, as in the longer transient 38 Myr run, temperatures in the lower CO2 range of the past 5 Myr are higher than when the climate is initialised at low temperatures. Consequently, the modelled CO2 concentrations depend on the initial state. Taking the realistic warm initialisation into account, we come to a best estimate of CO2, temperature, <span class="hlt">ice</span>-volume-equivalent sea level, and benthic δ18O over the past 38 Myr. Secondly, we study the influence of <span class="hlt">ice</span> <span class="hlt">sheets</span> on the evolution of global temperature and polar amplification by comparing runs with <span class="hlt">ice</span> <span class="hlt">sheet</span>-climate interaction switched on and off. By passing only albedo or surface height changes to the climate model, we can distinguish the separate effects of the <span class="hlt">ice</span>-albedo and surface</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3705479','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3705479"><span>Empirical Retrieval of Surface Melt Magnitude from Coupled MODIS Optical and Thermal Measurements over the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> during the 2001 Ablation Season</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Lampkin, Derrick; Peng, Rui</p> <p>2008-01-01</p> <p>Accelerated <span class="hlt">ice</span> flow near the equilibrium line of west-central Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (GIS) has been attributed to an increase in infiltrated surface melt water as a response to climate warming. The assessment of surface melting events must be more than the detection of melt onset or extent. Retrieval of surface melt magnitude is necessary to improve understanding of <span class="hlt">ice</span> <span class="hlt">sheet</span> flow and surface melt coupling. In this paper, we report on a new technique to quantify the magnitude of surface melt. Cloud-free dates of June 10, July 5, 7, 9, and 11, 2001 Moderate Resolution Imaging Spectroradiometer (MODIS) daily reflectance Band 5 (1.230-1.250μm) and surface temperature images rescaled to 1km over western Greenland were used in the retrieval algorithm. An optical-thermal feature space partitioned as a function of melt magnitude was derived using a one-dimensional thermal snowmelt model (SNTHERM89). SNTHERM89 was forced by hourly meteorological data from the Greenland Climate Network (GC-Net) at reference sites spanning dry <span class="hlt">snow</span>, percolation, and wet <span class="hlt">snow</span> zones in the Jakobshavn drainage basin in western GIS. Melt magnitude or effective melt (E-melt) was derived for satellite composite periods covering May, June, and July displaying low fractions (0-1%) at elevations greater than 2500m and fractions at or greater than 15% at elevations lower than 1000m assessed for only the upper 5 cm of the <span class="hlt">snow</span> surface. Validation of E-melt involved comparison of intensity to dry and wet zones determined from QSCAT backscatter. Higher intensities (> 8%) were distributed in wet <span class="hlt">snow</span> zones, while lower intensities were grouped in dry zones at a first order accuracy of ∼ ±2%. PMID:27873793</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C51F..01D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C51F..01D"><span>The geomorphic signature of past <span class="hlt">ice</span> <span class="hlt">sheets</span> in the marine record</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dowdeswell, J. A.</p> <p>2016-12-01</p> <p>The deglaciation of high-latitude continental shelves since the Last Glacial Maximum has revealed suites of subglacial and <span class="hlt">ice</span>-contact landforms that have remained well-preserved beneath tens to hundreds of metres of water. Once <span class="hlt">ice</span> has retreated, sedimentation is generally low on polar shelves during interglacials and the submarine landforms have not, therefore, been buried by subsequent sedimentation. By contrast, the beds of modern <span class="hlt">ice</span> <span class="hlt">sheets</span> are hidden by several thousand metres of <span class="hlt">ice</span>, which is much more difficult than water to penetrate using geophysical methods. These submarine glacial landforms provide insights into past <span class="hlt">ice-sheet</span> form and flow, and information on the processes that have taken place beneath former <span class="hlt">ice</span> <span class="hlt">sheets</span>. Examples will be shown of streamlined subglacial landforms that indicate the distribution and dimensions of former <span class="hlt">ice</span> streams on high-latitde continental margins. Distinctive landform assemblages characterise <span class="hlt">ice</span> stream and inter-<span class="hlt">ice</span> stream areas. Landforms, including subglacially formed channel systems in inner- and mid-shelf areas, and the lack of them on sedimentary outer shelves, allow inferences to be made about subglacial hydrology. The distribution of grounding-zone wedges and other transverse moraine ridges also provides evidence on the nature of <span class="hlt">ice-sheet</span> retreat - whether by rapid collapse, episodic retreat or by the slow retreat of grounded <span class="hlt">ice</span>. Such information can be used to test the predictive capability of <span class="hlt">ice-sheet</span> numerical models. These marine geophysical and geological observations of submarine glacial landforms enhance our understanding of the form and flow of past <span class="hlt">ice</span> masses at scales ranging from <span class="hlt">ice</span> <span class="hlt">sheets</span> (1000s of km in flow-line and margin length), through <span class="hlt">ice</span> streams (100s of km long), to surge-type glaciers (10s of km long).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1714074E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1714074E"><span>Observationally constrained projections of Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> instability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Edwards, Tamsin; Ritz, Catherine; Durand, Gael; Payne, Anthony; Peyaud, Vincent; Hindmarsh, Richard</p> <p>2015-04-01</p> <p>Large parts of the Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> lie on bedrock below sea level and may be vulnerable to a positive feedback known as Marine <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Instability (MISI), a self-sustaining retreat of the grounding line triggered by oceanic or atmospheric changes. There is growing evidence MISI may be underway throughout the Amundsen Sea Embayment (ASE) of West Antarctica, induced by circulation of warm Circumpolar Deep Water. If this retreat is sustained the region could contribute up to 1-2 m to global mean sea level, and if triggered in other areas the potential contribution to sea level on centennial to millennial timescales could be two to three times greater. However, physically plausible projections of Antarctic MISI are challenging: numerical <span class="hlt">ice</span> <span class="hlt">sheet</span> models are too low in spatial resolution to resolve grounding line processes or else too computationally expensive to assess modelling uncertainties, and no dynamical models exist of the ocean-atmosphere-<span class="hlt">ice</span> <span class="hlt">sheet</span> system. Furthermore, previous numerical <span class="hlt">ice</span> <span class="hlt">sheet</span> model projections for Antarctica have not been calibrated with observations, which can reduce uncertainties. Here we estimate the probability of dynamic mass loss in the event of MISI under a medium climate scenario, assessing 16 modelling uncertainties and calibrating the projections with observed mass losses in the ASE from 1992-2011. We project losses of up to 30 cm sea level equivalent (SLE) by 2100 and 72 cm SLE by 2200 (95% credibility interval: CI). Our results are substantially lower than previous estimates. The ASE sustains substantial losses, 83% of the continental total by 2100 and 67% by 2200 (95% CI), but in other regions losses are limited by <span class="hlt">ice</span> dynamical theory, observations, or a lack of projected triggers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('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 Mass Balance for the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span></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> <span class="hlt">Sheet</span> 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> <span class="hlt">sheet</span> surface mass balance (SMB), but lack spatial resolution needed to resolve ablation areas along the periphery of the <span class="hlt">ice</span> <span class="hlt">sheet</span>. 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> <span class="hlt">Sheet</span>. MERRA-2 is produced for the period 1980 to the present at a grid spacing of ½° latitude by ⅝° longitude, and includes <span class="hlt">snow</span> 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> <span class="hlt">sheets</span>. The surface coupling is performed such that mass 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/2014AGUFM.V11B4717I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.V11B4717I"><span>Phreatomagmatic eruptions under the West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span>: potential hazard for <span class="hlt">ice</span> <span class="hlt">sheet</span> stability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Iverson, N. A.; Dunbar, N. W.; Lieb-Lappen, R.; Kim, E. J.; Golden, E. J.; Obbard, R. W.</p> <p>2014-12-01</p> <p>Volcanic tephra layers have been seen in most <span class="hlt">ice</span> cores in Antarctica. These tephra layers are deposited almost instantaneously across wide areas of <span class="hlt">ice</span> <span class="hlt">sheets</span>, creating horizons that can provide "pinning points" to adjust <span class="hlt">ice</span> time scales that may otherwise be lacking detailed chronology. A combination of traditional particle morphology characterization by SEM with new non-destructive X-ray micro-computed tomography (Micro-CT) has been used to analyze selected coarse grained tephra in the West Antarctica <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (WAIS) Divide WDC06A <span class="hlt">ice</span> core. Micro-CT has the ability to image particles as small as 50µm in length (15µm resolution), quantifying both particle shape and size. The WDC06A contains hundreds of dusty layers of which 36 have so far been identified as primary tephra layers. Two of these tephra layers have been characterized as phreatomagmatic eruptions based on SEM imagery and are blocky and platy in nature, with rare magmatic particles. These layers are strikingly different in composition from the typical phonolitic and trachytic tephra produced from West Antarctic volcanoes. These two layers are coarser in grain size, with many particles (including feldspar crystals) exceeding 100µm in length. One tephra layer found at 3149.138m deep in the <span class="hlt">ice</span> core is a coarse ~1mm thick basanitic tephra layer with a WDC06-7 <span class="hlt">ice</span> core age of 45,381±2000yrs. The second layer is a ~1.3 cm thick zoned trachyandesite to trachydacite tephra found at 2569.205m deep with an <span class="hlt">ice</span> core age 22,470±835yrs. Micro-CT analysis shows that WDC06A-3149.138 has normal grading with the largest particles at the bottom of the sample (~160μm). WDC06A-2569.205 has a bimodal distribution of particles with large particles at the top and bottom of the layer. These large particles are more spherical in shape at the base and become more irregular and finer grained higher in the layer, likely showing changes in eruption dynamics. The distinct chemistry as well as the blocky and large grain size</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.C23B..08K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.C23B..08K"><span>Monitoring <span class="hlt">Snow</span> on <span class="hlt">ice</span> as Critical Habitat for Ringed Seals</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kelly, B. P.; Moran, J.; Douglas, D. C.; Nghiem, S. V.</p> <p>2007-12-01</p> <p>Ringed seals are the primary prey of polar bears, and they are found in all seasonally <span class="hlt">ice</span> covered seas of the northern hemisphere as well as in several freshwater lakes. The presence of <span class="hlt">snow</span> covered sea <span class="hlt">ice</span> is essential for successful ringed seal reproduction. Ringed seals abrade holes in the <span class="hlt">ice</span> allowing them to surface and breathe under the <span class="hlt">snow</span> cover. Where <span class="hlt">snow</span> accumulates to sufficient depths, ringed seals excavate subnivean lairs above breathing holes. They rest, give birth, and nurse their young in those lairs. Temperatures within the lairs remain within a few degrees of freezing, well within the zone of thermal neutrality for newborn ringed seals, even at ambient temperatures of -30° C. High rates of seal mortality have been recorded when early <span class="hlt">snow</span> melt caused lairs to collapse exposing newborn seals to predators and to subsequent extreme cold events. As melt onset dates come earlier in the Arctic Ocean, ringed seal populations (and the polar bears that depend upon them) will be increasingly challenged. We determined dates of lair abandonment by ringed seals fitted with radio transmitters in the Beaufort Sea (n = 60). We compared abandonment dates to melt onset dates measured in the field, as well as estimated dates derived from active (Ku-band backscatter) and passive (SSM/I) microwave satellite imagery. Date of <span class="hlt">snow</span> melt significantly improved models of environmental influences on the timing of lair abandonment. We used an algorithm based on multi-channel means and variances of passive microwave data to detect melt onset dates. Those melt onset dates predicted the date of lair abandonment ± 3 days (r 2 = 0.982, p = 0.001). The predictive power of passive microwave proxies combined with their historical record suggest they could serve to monitor critical changes to ringed seal habitat.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C12A..02G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C12A..02G"><span>Analysis of Light Absorbing Aerosols in Northern Pakistan: Concentration on <span class="hlt">Snow/Ice</span>, their Source Regions and Impacts on <span class="hlt">Snow</span> Albedo</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gul, C.; Praveen, P. S.; Shichang, K.; Adhikary, B.; Zhang, Y.; Ali, S.</p> <p>2016-12-01</p> <p>Elemental carbon (EC) and light absorbing organic carbon (OC) are important particulate impurities in <span class="hlt">snow</span> and <span class="hlt">ice</span> which significantly reduce the albedo of glaciers and accelerate their melting. <span class="hlt">Snow</span> and <span class="hlt">ice</span> samples were collected from Karakorum-Himalayan region of North Pakistan during the summer campaign (May-Jun) 2015 and only <span class="hlt">snow</span> samples were collected during winter (Dec 2015- Jan 2016). Total 41 surface <span class="hlt">snow/ice</span> samples were collected during summer campaign along different elevation ranges (2569 to 3895 a.m.s.l) from six glaciers: Sachin, Henarche, Barpu, Mear, Gulkin and Passu. Similarly 18 <span class="hlt">snow</span> samples were collected from Sust, Hoper, Tawas, Astore, Shangla, and Kalam regions during the winter campaign. Quartz filters were used for filtering of melted <span class="hlt">snow</span> and <span class="hlt">ice</span> samples which were then analyzed by thermal optical reflectance (TOR) method to determine the concentration of EC and OC. The average concentration of EC (ng/g), OC (ng/g) and dust (ppm) were found as follows: Passu (249.5, 536.8, 475), Barpu (1190, 397.6, 1288), Gulkin (412, 793, 761), Sachin (911, 2130, 358), Mear (678, 2067, 83) and Henarche (755, 1868, 241) respectively during summer campaign. Similarly, average concentration of EC (ng/g), OC (ng/g) and dust (ppm) was found in the samples of Sust (2506, 1039, 131), Hoper (646, 1153, 76), Tawas (650, 1320, 16), Astore (1305, 2161, 97), Shangla (739, 2079, 31) and Kalam (107, 347, 5) respectively during winter campaign. Two methods were adopted to identify the source regions: one coupled emissions inventory with back trajectories, second with a simple region tagged chemical transport modeling analysis. In addition, CALIPSO subtype aerosol composition indicated that frequency of smoke in the atmosphere over the region was highest followed by dust and then polluted dust. SNICAR model was used to estimate the <span class="hlt">snow</span> albedo reduction from our in-situ measurements. <span class="hlt">Snow</span> albedo reduction was observed to be 0.3% to 27.6%. The derived results were used</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.C11A0465M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.C11A0465M"><span>Characteristics of basal <span class="hlt">ice</span> and subglacial water at Dome Fuji, Antarctica <span class="hlt">ice</span> <span class="hlt">sheet</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Motoyama, H.; Uemura, R.; Hirabayashi, M.; Miyake, T.; Kuramoto, T.; Tanaka, Y.; Dome Fuji Ice Core Project, M.</p> <p>2008-12-01</p> <p>(Introduction): The second deep <span class="hlt">ice</span> coring project at Dome Fuji, Antarctica reached a depth of 3035.22 m during the austral summer season in 2006/2007. The recovered <span class="hlt">ice</span> cores contain records of global environmental changes going back about 720,000 years. (Estimation of basal <span class="hlt">ice</span> melt): The borehole measurement was carried out on January 2nd in 2007 when the temperature disturbance in the borehole calmed down by the rest of drilling for 2 days. Temperature measurement was performed after 0 C thermometer test was done in the ground. The temperature sensor of pt100 installed in the skate-like anti-torque was used. We did not have the enough time until the temperature of thermometer was matched with the temperature of <span class="hlt">ice</span> <span class="hlt">sheet</span>. Some error was included in <span class="hlt">ice</span> temperature data. The resistance of pt100 sensor was converted to temperature in the borehole measurement machine. But we used only two electrical lines for pt100 sensor. Rate of heat flow in the <span class="hlt">ice</span> <span class="hlt">sheet</span> was calculated using the vertical temperature gradient of the <span class="hlt">ice</span> <span class="hlt">sheet</span> and rate of heat conductivity of <span class="hlt">ice</span>. The deepest part of heat flux using temperatures at 3000m and 3030m was about 45mW/m2. We assumed that this value was the heat flux from the bedrock in the <span class="hlt">ice</span> <span class="hlt">sheet</span>. Heat flux to the bedrock surface in the ground was assumed 54.6mW/m2 adopted by <span class="hlt">ice</span> <span class="hlt">sheet</span> model (P. Huybrechts, 2006). Then the heat flux for basal <span class="hlt">ice</span> melt was about 10mW/m2. This value was equaled to melting of 1.1mm of <span class="hlt">ice</span> thickness per year. On the other hand, the annual layer thickness under 2500m was not changed so much and its average was 1.3mm of <span class="hlt">ice</span> thickness. So the annual layer thickness and melting rate of basal <span class="hlt">ice</span> was the same in ordering way. Or <span class="hlt">ice</span> equivalent in annual layer is melting every year. The age of the deepest part of <span class="hlt">ice</span> core is guessed at 720,000 years old and the <span class="hlt">ice</span> older than basal <span class="hlt">ice</span> has melted away. (The state of basal <span class="hlt">ice</span>): When the <span class="hlt">ice</span> core drilling depth passed 3031.44m, amount of <span class="hlt">ice</span> chip more abundant</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060038062&hterms=flower&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dflower','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060038062&hterms=flower&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dflower"><span>(abstract) A Polarimetric Model for Effects of Brine Infiltrated <span class="hlt">Snow</span> Cover and Frost Flowers on Sea <span class="hlt">Ice</span> Backscatter</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nghiem, S. V.; Kwok, R.; Yueh, S. H.</p> <p>1995-01-01</p> <p>A polarimetric scattering model is developed to study effects of <span class="hlt">snow</span> cover and frost flowers with brine infiltration on thin sea <span class="hlt">ice</span>. Leads containing thin sea <span class="hlt">ice</span> in the Artic icepack are important to heat exchange with the atmosphere and salt flux into the upper ocean. Surface characteristics of thin sea <span class="hlt">ice</span> in leads are dominated by the formation of frost flowers with high salinity. In many cases, the thin sea <span class="hlt">ice</span> layer is covered by <span class="hlt">snow</span>, which wicks up brine from sea <span class="hlt">ice</span> due to capillary force. <span class="hlt">Snow</span> and frost flowers have a significant impact on polarimetric signatures of thin <span class="hlt">ice</span>, which needs to be studied for accessing the retrieval of geophysical parameters such as <span class="hlt">ice</span> thickness. Frost flowers or <span class="hlt">snow</span> layer is modeled with a heterogeneous mixture consisting of randomly oriented ellipsoids and brine infiltration in an air background. <span class="hlt">Ice</span> crystals are characterized with three different axial lengths to depict the nonspherical shape. Under the covering multispecies medium, the columinar sea-<span class="hlt">ice</span> layer is an inhomogeneous anisotropic medium composed of ellipsoidal brine inclusions preferentially oriented in the vertical direction in an <span class="hlt">ice</span> background. The underlying medium is homogeneous sea water. This configuration is described with layered inhomogeneous media containing multiple species of scatterers. The species are allowed to have different size, shape, and permittivity. The strong permittivity fluctuation theory is extended to account for the multispecies in the derivation of effective permittivities with distributions of scatterer orientations characterized by Eulerian rotation angles. Polarimetric backscattering coefficients are obtained consistently with the same physical description used in the effective permittivity calculation. The mulitspecies model allows the inclusion of high-permittivity species to study effects of brine infiltrated <span class="hlt">snow</span> cover and frost flowers on thin <span class="hlt">ice</span>. The results suggest that the frost cover with a rough interface</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030020763','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030020763"><span>Understanding Recent Mass Balance Changes of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>vanderVeen, Cornelius</p> <p>2003-01-01</p> <p>The ultimate goal of this project is to better understand the current transfer of mass between the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span>, the world's oceans and the atmosphere, and to identify processes controlling the rate of this transfer, to be able to predict with greater confidence future contributions to global sea level rise. During the first year of this project, we focused on establishing longer-term records of change of selected outlet glaciers, reevaluation of mass input to the <span class="hlt">ice</span> <span class="hlt">sheet</span> and analysis of climate records derived from <span class="hlt">ice</span> cores, and modeling meltwater production and runoff from the margins of the <span class="hlt">ice</span> <span class="hlt">sheet</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..11.1261G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..11.1261G"><span>Buttressing and stability of marine <span class="hlt">Ice</span> <span class="hlt">sheets</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goldberg, D.; Holland, D. M.; Schoof, C.</p> <p>2009-04-01</p> <p>The West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> is marine in nature, meaning most of its base is below sea level. At the grounding line (where it becomes thin enough to float), its outlet streams flow into large <span class="hlt">ice</span> shelves. Gravitational stress in the shelf is transmitted back to the grounding line, and largely balanced by basal friction in the transition zone. The details of this force balance control the evolution of both the thickness and grounded extent of the <span class="hlt">ice</span> <span class="hlt">sheet</span>, and can lead to Weertman's (1974) Marine Instability for a foredeepened bedrock (one that deepens inland). However, the presence of rigid sidewalls and locally grounded regions in the shelf can reduce the longitudinal stresses felt at the grounding line (a phenomenon called buttressing). Thomas (1979) and others pointed out that Marine Instability may be lessened or reversed by <span class="hlt">ice</span> shelf buttressing. When modelling marine <span class="hlt">ice</span> <span class="hlt">sheets</span> numerically, the physics of the grounded-to-floating transition must be represented and the associated small length scales must be resolved (Schoof, 2007). Failing to do so can result in nonphysical or numerically inconsistent behavior (Vieli and Payne, 2005). While several methods have been developed to treat these issues (Vieli and Payne, 2005; Pattyn et al, 2006; Schoof, 2007) they are limited to flowline models. We present a model that represents the physics of the grounded-to-floating transition in a time-dependent three-dimensional marine <span class="hlt">ice</span> <span class="hlt">sheet</span>, using mesh adaption to resolve the transition zone. We show that in the special case of a two-dimensional <span class="hlt">sheet</span> our model reproduces the theoretical results of the MISMIP experiments, and that it produces robust results when both horizontal dimensions are resolved. In idealized experiments in a channel with rigid sidewalls and a foredeepened bed, we narrow the channel to determine whether buttressing is sufficient to reverse instability. We find that for strong beds (high friction coefficients), while the timescales and dynamics are</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017QSRv..169..148P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017QSRv..169..148P"><span>Deglaciation of the Eurasian <span class="hlt">ice</span> <span class="hlt">sheet</span> complex</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Patton, Henry; Hubbard, Alun; Andreassen, Karin; Auriac, Amandine; Whitehouse, Pippa L.; Stroeven, Arjen P.; Shackleton, Calvin; Winsborrow, Monica; Heyman, Jakob; Hall, Adrian M.</p> <p>2017-08-01</p> <p>The Eurasian <span class="hlt">ice</span> <span class="hlt">sheet</span> complex (EISC) was the third largest <span class="hlt">ice</span> mass during the Last Glacial Maximum with a span of over 4500 km and responsible for around 20 m of eustatic sea-level lowering. Whilst recent terrestrial and marine empirical insights have improved understanding of the chronology, pattern and rates of retreat of this vast <span class="hlt">ice</span> <span class="hlt">sheet</span>, a concerted attempt to model the deglaciation of the EISC honouring these new constraints is conspicuously lacking. Here, we apply a first-order, thermomechanical <span class="hlt">ice</span> <span class="hlt">sheet</span> model, validated against a diverse suite of empirical data, to investigate the retreat of the EISC after 23 ka BP, directly extending the work of Patton et al. (2016) who modelled the build-up to its maximum extent. Retreat of the <span class="hlt">ice</span> <span class="hlt">sheet</span> complex was highly asynchronous, reflecting contrasting regional sensitivities to climate forcing, oceanic influence, and internal dynamics. Most rapid retreat was experienced across the Barents Sea sector after 17.8 ka BP when this marine-based <span class="hlt">ice</span> <span class="hlt">sheet</span> disintegrated at a rate of ∼670 gigatonnes per year (Gt a-1) through enhanced calving and interior dynamic thinning, driven by oceanic/atmospheric warming and exacerbated by eustatic sea-level rise. From 14.9 to 12.9 ka BP the EISC lost on average 750 Gt a-1, peaking at rates >3000 Gt a-1, roughly equally partitioned between surface melt and dynamic losses, and potentially contributing up to 2.5 m to global sea-level rise during Meltwater Pulse 1A. Independent glacio-isostatic modelling constrained by an extensive inventory of relative sea-level change corroborates our <span class="hlt">ice</span> <span class="hlt">sheet</span> loading history of the Barents Sea sector. Subglacial conditions were predominately temperate during deglaciation, with over 6000 subglacial lakes predicted along with an extensive subglacial drainage network. Moreover, the maximum EISC and its isostatic footprint had a profound impact on the proglacial hydrological network, forming the Fleuve Manche mega-catchment which had an area of </p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.7407K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.7407K"><span>Sea-level and solid-Earth deformation feedbacks in <span class="hlt">ice</span> <span class="hlt">sheet</span> modelling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Konrad, Hannes; Sasgen, Ingo; Klemann, Volker; Thoma, Malte; Grosfeld, Klaus; Martinec, Zdeněk</p> <p>2014-05-01</p> <p>The interactions of <span class="hlt">ice</span> <span class="hlt">sheets</span> with the sea level and the solid Earth are important factors for the stability of the <span class="hlt">ice</span> shelves and the tributary inland <span class="hlt">ice</span> (e.g. Thomas and Bentley, 1978; Gomez et al, 2012). First, changes in <span class="hlt">ice</span> extent and <span class="hlt">ice</span> thickness induce viscoelastic deformation of the Earth surface and Earth's gravity field. In turn, global and local changes in sea level and bathymetry affect the grounding line and, subsequently, alter the <span class="hlt">ice</span> dynamic behaviour. Here, we investigate these feedbacks for a synthetic <span class="hlt">ice</span> <span class="hlt">sheet</span> configuration as well as for the Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> using a three-dimensional thermomechanical <span class="hlt">ice</span> <span class="hlt">sheet</span> and shelf model, coupled to a viscoelastic solid-Earth and gravitationally self-consistent sea-level model. The respective <span class="hlt">ice</span> <span class="hlt">sheet</span> undergoes a forcing from rising sea level, warming ocean, and/or changing surface mass balance. The coupling is realized by exchanging <span class="hlt">ice</span> thickness, Earth surface deformation and sea level periodically. We apply several sets of viscoelastic Earth parameters to our coupled model, e.g. simulating a low-viscous upper mantle present at the Antarctic Peninsula (Ivins et al., 2011). Special focus of our study lies on the evolution of Earth surface deformation and local sea level changes, as well as on the accompanying grounding line evolution. N. Gomez, D. Pollard, J. X. Mitrovica, P. Huybers, and P. U. Clark 2012. Evolution of a coupled marine <span class="hlt">ice</span> <span class="hlt">sheet</span>-sea level model, J. Geophys. Res., 117, F01013, doi:10.1029/2011JF002128. E. R. Ivins, M. M. Watkins, D.-N. Yuan, R. Dietrich, G. Casassa, and A. Rülke 2011. On-land <span class="hlt">ice</span> loss and glacial isostatic adjustment at the Drake Passage: 2003-2009, J. Geophys. Res. 116, B02403, doi: 10.1029/2010JB007607 R. H. Thomas and C. R. Bentley 1978. A model for Holocene retreat of the West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span>, Quaternary Research, 10 (2), pages 150-170, doi: 10.1016/0033-5894(78)90098-4.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060033521&hterms=extremophile&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dextremophile','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060033521&hterms=extremophile&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dextremophile"><span>Issues in subsurface exploration of <span class="hlt">ice</span> <span class="hlt">sheets</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>French, L.; Carsey, F.; Zimmerman, W.</p> <p>2000-01-01</p> <p>Exploration of the deep subsurface <span class="hlt">ice</span> <span class="hlt">sheets</span> of Earth, Mars, Europa, and Titan has become a major consideration in addressing scientific objectives in climate change, extremophile biology, exobiology,chemical weathering, planetary evolution and <span class="hlt">ice</span> dynamics.</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://pubs.er.usgs.gov/publication/70024064','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70024064"><span>Discharge of debris from <span class="hlt">ice</span> at the margin of the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Knight, P.G.; Waller, R.I.; Patterson, C.J.; Jones, A.P.; Robinson, Z.P.</p> <p>2002-01-01</p> <p>Sediment production at a terrestrial section of the <span class="hlt">ice-sheet</span> margin in West Greenland is dominated by debris released through the basal <span class="hlt">ice</span> layer. The debris flux through the basal <span class="hlt">ice</span> at the margin is estimated to be 12-45 m3 m-1 a-1. This is three orders of magnitude higher than that previously reported for East Antarctica, an order of magnitude higher than sites reported from in Norway, Iceland and Switzerland, but an order of magnitude lower than values previously reported from tidewater glaciers in Alaska and other high-rate environments such as surging glaciers. At our site, only negligible amounts of debris are released through englacial, supraglacial or subglacial sediment transfer. Glacio-fluvial sediment production is highly localized, and long sections of the <span class="hlt">ice-sheet</span> margin receive no sediment from glaciofluvial sources. These findings differ from those of studies at more temperate glacial settings where glaciofluvial routes are dominant and basal <span class="hlt">ice</span> contributes only a minor percentage of the debris released at the margin. These data on debris flux through the terrestrial margin of an outlet glacier contribute to our limited knowledge of debris production from the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29055575','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29055575"><span>Review of levoglucosan in glacier <span class="hlt">snow</span> and <span class="hlt">ice</span> studies: Recent progress and future perspectives.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>You, Chao; Xu, Chao</p> <p>2018-03-01</p> <p>Levoglucosan (LEV) in glacier <span class="hlt">snow</span> and <span class="hlt">ice</span> layers provides a fingerprint of fire activity, ranging from modern air pollution to ancient fire emissions. In this study, we review recent progress in our understanding and application of LEV in glaciers, including analytical methods, transport and post-depositional processes, and historical records. We firstly summarize progress in analytical methods for determination of LEV in glacier <span class="hlt">snow</span> and <span class="hlt">ice</span>. Then, we discuss the processes influencing the records of LEV in <span class="hlt">snow</span> and <span class="hlt">ice</span> layers. Finally, we make some recommendations for future work, such as assessing the stability of LEV and obtaining continuous records, to increase reliability of the reconstructed ancient fire activity. This review provides an update for researchers working with LEV and will facilitate the further use of LEV as a biomarker in paleo-fire studies based on <span class="hlt">ice</span> core records. Copyright © 2017 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14.9151B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.9151B"><span>A sensitivity analysis for a thermomechanical model of the Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> and <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>Baratelli, F.; Castellani, G.; Vassena, C.; Giudici, M.</p> <p>2012-04-01</p> <p>The outcomes of an <span class="hlt">ice</span> <span class="hlt">sheet</span> model depend on a number of parameters and physical quantities which are often estimated with large uncertainty, because of lack of sufficient experimental measurements in such remote environments. Therefore, the efforts to improve the accuracy of the predictions of <span class="hlt">ice</span> <span class="hlt">sheet</span> models by including more physical processes and interactions with atmosphere, hydrosphere and lithosphere can be affected by the inaccuracy of the fundamental input data. A sensitivity analysis can help to understand which are the input data that most affect the different predictions of the model. In this context, a finite difference thermomechanical <span class="hlt">ice</span> <span class="hlt">sheet</span> model based on the Shallow-<span class="hlt">Ice</span> Approximation (SIA) and on the Shallow-Shelf Approximation (SSA) has been developed and applied for the simulation of the evolution of the Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> and <span class="hlt">ice</span> shelves for the last 200 000 years. The sensitivity analysis of the model outcomes (e.g., the volume of the <span class="hlt">ice</span> <span class="hlt">sheet</span> and of the <span class="hlt">ice</span> shelves, the basal melt rate of the <span class="hlt">ice</span> <span class="hlt">sheet</span>, the mean velocity of the Ross and Ronne-Filchner <span class="hlt">ice</span> shelves, the wet area at the base of the <span class="hlt">ice</span> <span class="hlt">sheet</span>) with respect to the model parameters (e.g., the basal sliding coefficient, the geothermal heat flux, the present-day surface accumulation and temperature, the mean <span class="hlt">ice</span> shelves viscosity, the melt rate at the base of the <span class="hlt">ice</span> shelves) has been performed by computing three synthetic numerical indices: two local sensitivity indices and a global sensitivity index. Local sensitivity indices imply a linearization of the model and neglect both non-linear and joint effects of the parameters. The global variance-based sensitivity index, instead, takes into account the complete variability of the input parameters but is usually conducted with a Monte Carlo approach which is computationally very demanding for non-linear complex models. Therefore, the global sensitivity index has been computed using a development of the model outputs in a</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> <span class="hlt">Sheet</span> 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> <span class="hlt">sheets</span> (Hays et al., 1976). However, variations 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> <span class="hlt">sheet</span> 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> <span class="hlt">sheet</span> sensitivity to a range of commonly used <span class="hlt">ice</span> <span class="hlt">sheet</span> model parameters, including mass balance and albedo, to optimize simulations for Pleistocene orbital cycles. Our tests indicate that choice of mass balance and albedo parameterizations can lead to significant differences in <span class="hlt">ice</span> <span class="hlt">sheet</span> behavior and volume. For instance, use of an insolation-temperature mass balance scheme (van den Berg, 2008) allows for a larger <span class="hlt">ice</span> <span class="hlt">sheet</span> 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> <span class="hlt">sheet</span> sensitivity. Careful tuning of mass balance and albedo parameterizations can help alleviate the problem of insufficient <span class="hlt">ice</span> <span class="hlt">sheet</span> 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/2018TCry...12...39B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018TCry...12...39B"><span>Influence of temperature fluctuations on equilibrium <br class="break"/><span class="hlt">ice</span> <span class="hlt">sheet</span> volume</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bøgeholm Mikkelsen, Troels; Grinsted, Aslak; Ditlevsen, Peter</p> <p>2018-01-01</p> <p>Forecasting the future sea level relies on accurate modeling of the response of the Greenland and Antarctic <span class="hlt">ice</span> <span class="hlt">sheets</span> to changing temperatures. The surface mass balance (SMB) of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (GrIS) has a nonlinear response to warming. Cold and warm anomalies of equal size do not cancel out and it is therefore important to consider the effect of interannual fluctuations in temperature. We find that the steady-state volume of an <span class="hlt">ice</span> <span class="hlt">sheet</span> is biased toward larger size if interannual temperature fluctuations are not taken into account in numerical modeling of the <span class="hlt">ice</span> <span class="hlt">sheet</span>. We illustrate this in a simple <span class="hlt">ice</span> <span class="hlt">sheet</span> model and find that the equilibrium <span class="hlt">ice</span> volume is approximately 1 m SLE (meters sea level equivalent) smaller when the simple model is forced with fluctuating temperatures as opposed to a stable climate. It is therefore important to consider the effect of interannual temperature fluctuations when designing long experiments such as paleo-spin-ups. We show how the magnitude of the potential bias can be quantified statistically. For recent simulations of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span>, we estimate the bias to be 30 Gt yr-1 (24-59 Gt yr-1, 95 % credibility) for a warming of 3 °C above preindustrial values, or 13 % (10-25, 95 % credibility) of the present-day rate of <span class="hlt">ice</span> loss. Models of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> show a collapse threshold beyond which the <span class="hlt">ice</span> <span class="hlt">sheet</span> becomes unsustainable. The proximity of the threshold will be underestimated if temperature fluctuations are not taken into account. We estimate the bias to be 0.12 °C (0.10-0.18 °C, 95 % credibility) for a recent estimate of the threshold. In light of our findings it is important to gauge the extent to which this increased variability will influence the mass balance of the <span class="hlt">ice</span> <span class="hlt">sheets</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.V21A2763E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.V21A2763E"><span>Experimental Insights on Natural Lava-<span class="hlt">Ice/Snow</span> Interactions and Their Implications for Glaciovolcanic and Submarine Eruptions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Edwards, B. R.; Karson, J.; Wysocki, R.; Lev, E.; Bindeman, I. N.; Kueppers, U.</p> <p>2012-12-01</p> <p>Lava-<span class="hlt">ice-snow</span> interactions have recently gained global attention through the eruptions of <span class="hlt">ice</span>-covered volcanoes, particularly from Eyjafjallajokull in south-central Iceland, with dramatic effects on local communities and global air travel. However, as with most submarine eruptions, direct observations of lava-<span class="hlt">ice/snow</span> interactions are rare. Only a few hundred potentially active volcanoes are presently <span class="hlt">ice</span>-covered, these volcanoes are generally in remote places, and their associated hazards make close observation and measurements dangerous. Here we report the results of the first large-scale experiments designed to provide new constraints on natural interactions between lava and <span class="hlt">ice/snow</span>. The experiments comprised controlled effusion of tens of kilograms of melted basalt on top of <span class="hlt">ice/snow</span>, and provide insights about observations from natural lava-<span class="hlt">ice-snow</span> interactions including new constraints for: 1) rapid lava advance along the <span class="hlt">ice</span>-lava interface; 2) rapid downwards melting of lava flows through <span class="hlt">ice</span>; 3) lava flow exploitation of pre-existing discontinuities to travel laterally beneath and within <span class="hlt">ice</span>; and 4) formation of abundant limu o Pele and non-explosive vapor transport from the base to the top of the lava flow with minor O isotope exchange. The experiments are consistent with observations from eruptions showing that lava is more efficient at melting <span class="hlt">ice</span> when emplaced on top of the <span class="hlt">ice</span> as opposed to beneath the <span class="hlt">ice</span>, as well as the efficacy of tephra cover for slowing melting. The experimental extrusion rates are as within the range of those for submarine eruptions as well, and reproduce some features seen in submarine eruptions including voluminous production of gas rich cavities within initially anhydrous lavas and limu on lava surfaces. Our initial results raise questions about the possibility of secondary ingestion of water by submarine and glaciovolcanic lava flows, and the origins of apparent primary gas cavities in those flows. Basaltic melt moving down</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160013723','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160013723"><span>A Synthesis of the Basal Thermal State of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Macgregor, J. A.; Fahnestock, M. A.; Catania, G. A.; Aschwanden, A.; Clow, G. D.; Colgan, W. T.; Gogineni, S. P.; Morlighem, M.; Nowicki, S. M. J.; Paden, J. D.; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20160013723'); toggleEditAbsImage('author_20160013723_show'); toggleEditAbsImage('author_20160013723_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20160013723_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20160013723_hide"></p> <p>2016-01-01</p> <p>Greenland's thick <span class="hlt">ice</span> <span class="hlt">sheet</span> insulates the bedrock below from the cold temperatures at the surface, so the bottom of the <span class="hlt">ice</span> is often tens of degrees warmer than at the top, because the <span class="hlt">ice</span> bottom is slowly warmed by heat coming from the Earth's depths. Knowing whether Greenland's <span class="hlt">ice</span> lies on wet, slippery ground or is anchored to dry, frozen bedrock is essential for predicting how this <span class="hlt">ice</span> will flow in the future. But scientists have very few direct observations of the thermal conditions beneath the <span class="hlt">ice</span> <span class="hlt">sheet</span>, obtained through fewer than two dozen boreholes that have reached the bottom. Our study synthesizes several independent methods to infer the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span>'s basal thermal state -whether the bottom of the <span class="hlt">ice</span> is melted or not-leading to the first map that identifies frozen and thawed areas across the whole <span class="hlt">ice</span> <span class="hlt">sheet</span>. This map will guide targets for future investigations of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> toward the most vulnerable and poorly understood regions, ultimately improving our understanding of its dynamics and contribution to future sea-level rise. It is of particular relevance to ongoing Operation <span class="hlt">Ice</span>Bridge activities and future large-scale airborne missions over Greenland.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050139693','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050139693"><span>Earth Observing System (EOS) <span class="hlt">Snow</span> and <span class="hlt">Ice</span> Products for Observation and Modeling</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hall, D.; Kaminski, M.; Cavalieri, D.; Dickinson, R.; Marquis, M.; Riggs, G.; Robinson, D.; VanWoert, M.; Wolfe, R.</p> <p>2005-01-01</p> <p><span class="hlt">Snow</span> and <span class="hlt">ice</span> are the key components of the Earth's cryosphere, and their influence on the Earth's energy balance is very significant due at least in part to the large areal extent and high albedo characterizing these features. Large changes in the cryosphere have been measured over the last century and especially over the past decade, and remote sensing plays a pivotal role in documenting these changes. Many of NASA's Earth Observing System (EOS) products derived from instruments on the Terra, Aqua, and <span class="hlt">Ice</span>, Cloud and land Elevation Satellite (ICESat) satellites are useful for measuring changes in features that are associated with climate change. The utility of the products is continually enhanced as the length of the time series increases. To gain a more coherent view of the cryosphere and its historical and recent changes, the EOS products may be employed together, in conjunction with other sources of data, and in models. To further this goal, the first EOS <span class="hlt">Snow</span> and <span class="hlt">Ice</span> Products Workshop was convened. The specific goals of the workshop were to provide current and prospective users of EOS <span class="hlt">snow</span> and <span class="hlt">ice</span> products up-to-date information on the products, their validation status and future enhancements, to help users utilize the data products through hands-on demonstrations, and to facilitate the integration of EOS products into models. Oral and poster sessions representing a wide variety of <span class="hlt">snow</span> and <span class="hlt">ice</span> topics were held; three panels were also convened to discuss workshop themes. Panel discussions focused on data fusion and assimilation of the products into models. Approximately 110 people attended, representing a wide array of interests and organizations in the cryospheric community.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.G52B..03B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.G52B..03B"><span>The East Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> and the Gamburtsev Subglacial Mountains (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bell, R. E.; Studinger, M.; Ferraccioli, F.; Damaske, D.; Finn, C.; Braaten, D. A.; Fahnestock, M. A.; Jordan, T. A.; Corr, H.; Elieff, S.; Frearson, N.; Block, A. E.; Rose, K.</p> <p>2009-12-01</p> <p>Models of the onset of glaciation in Antarctica routinely document the early growth of the <span class="hlt">ice</span> <span class="hlt">sheet</span> on the summit of the Gamburtsev Subglacial Mountains in the center of the East Antarctic Craton. While <span class="hlt">ice</span> <span class="hlt">sheet</span> models replicate the formation of the East Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> 35 million years ago, the age, evolution and structure of the Gamburtsev Mountains remain completely unresolved. During the International Polar Year scientists from seven nations have launched a major collaborative program (AGAP) to explore the Gamburtsev Subglacial Mountains buried by the East Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> and bounded by numerous subglacial lakes. The AGAP umbrella is a multi-national, multi-disciplinary effort and includes aerogeophysics, passive seismology, traverse programs and will be complimented by future <span class="hlt">ice</span> core and bedrock drilling. A major new airborne data set including gravity; magnetics; <span class="hlt">ice</span> thickness; SAR images of the <span class="hlt">ice</span>-bed interface; near-surface and deep internal layers; and <span class="hlt">ice</span> surface elevation is providing insights into a more dynamic East Antarctica. More than 120,000 km of aerogeophysical data have been acquired from two remote field camps during the 2008/09 field season. AGAP effort was designed to address several fundamental questions including: 1) What role does topography play in the nucleation of continental <span class="hlt">ice</span> <span class="hlt">sheets</span>? 2) How do tectonic processes control the formation, distribution, and stability of subglacial lakes? The preliminary analysis of this major new data set indicated these 3000m high mountains are deeply dissected by a dendritic system. The northern margin of the mountain range terminates against the inland extent of the Lambert Graben. Evidence of the onset of glaciation is preserved as cirques and U shaped valleys along the axis of the uplifted massifs. The geomorphology reflects the interaction between the <span class="hlt">ice</span> <span class="hlt">sheet</span> and the Gamburtsev Mountains. Bright reflectors in the radar data in the deep valleys indicate the presence of water that has</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA....12815H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA....12815H"><span>Data sets for <span class="hlt">snow</span> cover monitoring and modelling from the National <span class="hlt">Snow</span> and <span class="hlt">Ice</span> Data Center</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Holm, M.; Daniels, K.; Scott, D.; McLean, B.; Weaver, R.</p> <p>2003-04-01</p> <p>A wide range of <span class="hlt">snow</span> cover monitoring and modelling data sets are pending or are currently available from the National <span class="hlt">Snow</span> and <span class="hlt">Ice</span> Data Center (NSIDC). In-situ observations support validation experiments that enhance the accuracy of remote sensing data. In addition, remote sensing data are available in near-real time, providing coarse-resolution <span class="hlt">snow</span> monitoring capability. Time series data beginning in 1966 are valuable for modelling efforts. NSIDC holdings include SMMR and SSM/I <span class="hlt">snow</span> cover data, MODIS <span class="hlt">snow</span> cover extent products, in-situ and satellite data collected for NASA's recent Cold Land Processes Experiment, and soon-to-be-released ASMR-E passive microwave products. The AMSR-E and MODIS sensors are part of NASA's Earth Observing System flying on the Terra and Aqua satellites Characteristics of these NSIDC-held data sets, appropriateness of products for specific applications, and data set access and availability will be presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1616351A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1616351A"><span>Future Antarctic bed topography and its implications for <span class="hlt">ice</span> <span class="hlt">sheet</span> dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Adhikari, Surendra; Ivins, Erik; Larour, Eric; Seroussi, Helene; Morlighem, Mathieu; Nowicki, Sophie</p> <p>2014-05-01</p> <p>A recently improved <span class="hlt">ice</span> loading history suggests that the Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (AIS) has been generally losing its mass since the last glacial maximum. In a sustained warming climate, the AIS is predicted to retreat at a greater pace primarily via melting beneath the <span class="hlt">ice</span> shelves. We employ the glacial isostatic adjustment (GIA) capability of the <span class="hlt">Ice</span> <span class="hlt">Sheet</span> System Model (ISSM) to combine these past and future <span class="hlt">ice</span> loadings and provide the new solid Earth computations for the AIS. We find that the past loading is relatively less important than future loading on the evolution of the future bed topography. Our computations predict that the West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (WAIS) may uplift by a few meters and a few tens of meters at years 2100 and 2500 AD, respectively, and that the East Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (EAIS) is likely to remain unchanged or subside minimally except around the Amery <span class="hlt">Ice</span> Shelf. The Amundsen Sea Sector of WAIS in particular is predicted to rise at the greatest rate; one hundred years of <span class="hlt">ice</span> evolution in this region, for example, predicts that the coastline of Pine Island Bay approaches roughly 45 mm/yr in viscoelastic vertical motion. Of particular importance, we systematically demonstrate that the effect of a pervasive and large GIA uplift in the WAIS is associated with the flattening of reverse bed, reduction of local sea depth, and thus the extension of grounding line (GL) towards the continental shelf. Using the 3-D higher-order <span class="hlt">ice</span> flow capability of ISSM, such a migration of GL is shown to inhibit the <span class="hlt">ice</span> flow. This negative feedback between the <span class="hlt">ice</span> <span class="hlt">sheet</span> and the solid Earth may promote the stability to marine portions of the <span class="hlt">ice</span> <span class="hlt">sheet</span> in the future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-GSFC_20171208_Archive_e000832.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-GSFC_20171208_Archive_e000832.html"><span>Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> in 3D Cutaway</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2017-12-08</p> <p>Peering into the thousands of frozen layers inside Greenland’s <span class="hlt">ice</span> <span class="hlt">sheet</span> is like looking back in time. Each layer provides a record of what Earth’s climate was like at the dawn of civilization, or during the last <span class="hlt">ice</span> age, or during an ancient period of warmth similar to the one we experience today. Scientists using <span class="hlt">ice</span>-penetrating radar data collected by NASA’s Operation <span class="hlt">Ice</span>Bridge and earlier airborne campaigns have built the first-ever comprehensive map of layers deep inside the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span>. View the full video: youtu.be/u0VbPE0TOtQ Credit: NASA’s Goddard Space Flight Center NASA image use policy. NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. Follow us on Twitter Like us on Facebook Find us on Instagram</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150001448','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150001448"><span>Preservation of a Preglacial Landscape Under the Center of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bierman, Paul R.; Corbett, Lee B.; Graly, Joseph A.; Neumann, Thomas Allen; Lini, Andrea; Crosby, Benjamin T.; Rood, Dylan H.</p> <p>2014-01-01</p> <p>Continental <span class="hlt">ice</span> <span class="hlt">sheets</span> typically sculpt landscapes via erosion; under certain conditions, ancient landscapes can be preserved beneath <span class="hlt">ice</span> and can survive extensive and repeated glaciation. We used concentrations of atmospherically produced cosmogenic beryllium-10, carbon, and nitrogen to show that ancient soil has been preserved in basal <span class="hlt">ice</span> for millions of years at the center of the <span class="hlt">ice</span> <span class="hlt">sheet</span> at Summit, Greenland. This finding suggests <span class="hlt">ice</span> <span class="hlt">sheet</span> stability through the Pleistocene (i.e., the past 2.7 million years). The preservation of this soil implies that the <span class="hlt">ice</span> has been non-erosive and frozen to the bed for much of that time, that there was no substantial exposure of central Greenland once the <span class="hlt">ice</span> <span class="hlt">sheet</span> became fully established, and that preglacial landscapes can remain preserved for long periods under continental <span class="hlt">ice</span> <span class="hlt">sheets</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMIN43B0087W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMIN43B0087W"><span>Alaska Testbed for the Fusion of Citizen Science and Remote Sensing of Sea <span class="hlt">Ice</span> and <span class="hlt">Snow</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Walsh, J. E.; Sparrow, E.; Lee, O. A.; Brook, M.; Brubaker, M.; Casas, J.</p> <p>2017-12-01</p> <p>Citizen science, remote sensing and related environmental information sources for the Alaskan Arctic are synthesized with the objectives of (a) placing local observations into a broader geospatial framework and (b) enabling the use of local observations to evaluate sea <span class="hlt">ice</span>, <span class="hlt">snow</span> and land surface products obtained from remote sensing. In its initial phase, the project instituted a coordinated set of community-based observations of sea <span class="hlt">ice</span> and <span class="hlt">snow</span> in three coastal communities in western and northern Alaska: Nome, Point Hope and Barrow. Satellite maps of sea <span class="hlt">ice</span> concentration have been consolidated with the in situ reports, leading to a three-part depiction of surface conditions at each site: narrative reports, surface-based photos, and satellite products. The project has developed a prototype visualization package, enabling users to select a location and date for which the three information sources can be viewed. Visual comparisons of the satellite products and the local reports show generally consistent depictions of the sea <span class="hlt">ice</span> concentrations in the vicinity of the coastlines, although the satellite products are generally biased low, especially in coastal regions where shorefast <span class="hlt">ice</span> persists after the appearance of open water farther offshore. A preliminary comparison of the local <span class="hlt">snow</span> reports and the MODIS daily North American <span class="hlt">snow</span> cover images indicates that areas of <span class="hlt">snow</span> persisted in the satellite images beyond the date of <span class="hlt">snow</span> disappearance reported by the observers. The "in-town" location of most of the <span class="hlt">snow</span> reports is a factor that must be addressed in further reporting and remote sensing comparisons.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5510715','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5510715"><span>West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> retreat driven by Holocene warm water incursions</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Hillenbrand, Claus-Dieter; Smith, James A.; Hodell, David A.; Greaves, Mervyn; Poole, Christopher R.; Kender, Sev; Williams, Mark; Andersen, Thorbjørn Joest; Jernas, Patrycja E.; Klages, Johann P.; Roberts, Stephen J.; Gohl, Karsten; Larter, Robert D.; Kuhn, Gerhard</p> <p>2017-01-01</p> <p>Glaciological and oceanographic observations coupled with numerical models show that warm Circumpolar Deep Water (CDW) upwelling onto the West Antarctic continental shelf causes melting of the undersides of floating <span class="hlt">ice</span> shelves. Because these <span class="hlt">ice</span> shelves buttress glaciers feeding into them, their ocean-induced thinning is driving Antarctic <span class="hlt">ice-sheet</span> loss today. Here we present the first multi-proxy data based reconstruction of variability in CDW inflow to the Amundsen Sea sector, the most vulnerable part of the West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span>, during the last 11,000 years. The chemical composition of foraminifer shells and benthic foraminifer assemblages in marine sediments indicate that enhanced CDW upwelling, controlled by the latitudinal position of the Southern Hemisphere westerly winds, forced deglaciation of this sector both until 7,500 years ago, when an <span class="hlt">ice</span>-shelf collapse may have caused rapid <span class="hlt">ice-sheet</span> thinning further upstream, and since the 1940s. These results increase confidence in the predictive capability of current <span class="hlt">ice-sheet</span> models. PMID:28682333</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C51A0950M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C51A0950M"><span>SPICE: Sentinel-3 Performance Improvement for <span class="hlt">Ice</span> <span class="hlt">Sheets</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McMillan, M.; Escola, R.; Roca, M.; Thibaut, P.; Aublanc, J.; Shepherd, A.; Remy, F.; Benveniste, J.; Ambrózio, A.; Restano, M.</p> <p>2017-12-01</p> <p>For the past 25 years, polar-orbiting satellite radar altimeters have provided a valuable record of <span class="hlt">ice</span> <span class="hlt">sheet</span> elevation change and mass balance. One of the principle challenges associated with radar altimetry comes from the relatively large ground footprint of conventional pulse-limited radars, which reduces their capacity to make measurements in areas of complex topographic terrain. In recent years, progress has been made towards improving ground resolution, through the implementation of Synthetic Aperture Radar (SAR), or Delay-Doppler, techniques. In 2010, the launch of CryoSat-2 heralded the start of a new era of SAR Interferometric (SARIn) altimetry. However, because the satellite operated in SARIn and LRM mode over the <span class="hlt">ice</span> <span class="hlt">sheets</span>, many of the non-interferometric SAR altimeter processing techniques have been optimized for water and sea <span class="hlt">ice</span> surfaces only. The launch of Sentinel-3, which provides full non-interferometric SAR coverage of the <span class="hlt">ice</span> <span class="hlt">sheets</span>, therefore presents the opportunity to further develop these SAR processing methodologies over <span class="hlt">ice</span> <span class="hlt">sheets</span>. Here we present results from SPICE, a 2 year study that focuses on (1) developing and evaluating Sentinel-3 SAR altimetry processing methodologies over the Polar <span class="hlt">ice</span> <span class="hlt">sheets</span>, and (2) investigating radar wave penetration through comparisons of Ku- and Ka-band satellite measurements. The project, which is funded by ESA's SEOM (Scientific Exploitation of Operational Missions) programme, has worked in advance of the operational phase of Sentinel-3, to emulate Sentinel-3 SAR and pseudo-LRM data from dedicated CryoSat-2 SAR acquisitions made at the Lake Vostok, Dome C and Spirit sites in East Antarctica, and from reprocessed SARIn data in Greenland. In Phase 1 of the project we have evaluated existing processing methodologies, and in Phase 2 we are investigating new evolutions to the Delay-Doppler Processing (DDP) and retracking chains. In this presentation we (1) evaluate the existing Sentinel-3 processing chain by</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017TCry...11.3011H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017TCry...11.3011H"><span>The significance of vertical moisture diffusion on drifting <span class="hlt">snow</span> sublimation near <span class="hlt">snow</span> surface</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huang, Ning; Shi, Guanglei</p> <p>2017-12-01</p> <p>Sublimation of blowing <span class="hlt">snow</span> is an important parameter not only for the study of polar <span class="hlt">ice</span> <span class="hlt">sheets</span> and glaciers, but also for maintaining the ecology of arid and semi-arid lands. However, sublimation of near-surface blowing <span class="hlt">snow</span> has often been ignored in previous studies. To study sublimation of near-surface blowing <span class="hlt">snow</span>, we established a sublimation of blowing <span class="hlt">snow</span> model containing both a vertical moisture diffusion equation and a heat balance equation. The results showed that although sublimation of near-surface blowing <span class="hlt">snow</span> was strongly reduced by a negative feedback effect, due to vertical moisture diffusion, the relative humidity near the surface does not reach 100 %. Therefore, the sublimation of near-surface blowing <span class="hlt">snow</span> does not stop. In addition, the sublimation rate near the surface is 3-4 orders of magnitude higher than that at 10 m above the surface and the mass of <span class="hlt">snow</span> sublimation near the surface accounts for more than half of the total <span class="hlt">snow</span> sublimation when the friction wind velocity is less than about 0.55 m s-1. Therefore, the sublimation of near-surface blowing <span class="hlt">snow</span> should not be neglected.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23197528','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23197528"><span>A reconciled estimate of <span class="hlt">ice-sheet</span> mass balance.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>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</p> <p>2012-11-30</p> <p>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 <span class="hlt">ice</span> <span class="hlt">sheets</span>. 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 <span class="hlt">ice</span> <span class="hlt">sheets</span> 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 <span class="hlt">ice</span> <span class="hlt">sheets</span> have contributed, on average, 0.59 ± 0.20 millimeter year(-1) to the rate of global sea-level rise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.C44A..06B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.C44A..06B"><span>Widespread Refreezing of Both Surface and Basal Melt Water Beneath the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bell, R. E.; Tinto, K. J.; Das, I.; Wolovick, M.; Chu, W.; Creyts, T. T.; Frearson, N.</p> <p>2013-12-01</p> <p>The isotopically and chemically distinct, bubble-free <span class="hlt">ice</span> observed along the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> margin both in the Russell Glacier and north of Jacobshavn must have formed when water froze from subglacial networks. Where this refreezing occurs and what impact it has on <span class="hlt">ice</span> <span class="hlt">sheet</span> processes remain unclear. We use airborne radar data to demonstrate that freeze-on to the <span class="hlt">ice</span> <span class="hlt">sheet</span> base and associated deformation produce large <span class="hlt">ice</span> units up to 700 m thick throughout northern Greenland. Along the <span class="hlt">ice</span> <span class="hlt">sheet</span> margin, in the ablation zone, surface meltwater, delivered via moulins, refreezes to the <span class="hlt">ice</span> <span class="hlt">sheet</span> base over rugged topography. In the interior, water melted from the <span class="hlt">ice</span> <span class="hlt">sheet</span> base is refrozen and surrounded by folded <span class="hlt">ice</span>. A significant fraction of the <span class="hlt">ice</span> <span class="hlt">sheet</span> is modified by basal freeze-on and associated deformation. For the Eqip and Petermann catchments, representing the <span class="hlt">ice</span> <span class="hlt">sheet</span> margin and interior respectively, extensive airborne radar datasets show that 10%-13% of the base of the <span class="hlt">ice</span> <span class="hlt">sheet</span> and up to a third of the catchment width is modified by basal freeze-on. The interior units develop over relatively subdued topography with modest water flux from basal melt where conductive cooling likely dominates. Steps in the bed topography associated with subglacial valley networks may foster glaciohydraulic supercooling. The ablation zone units develop where both surface melt and crevassing are widespread and large volumes of surface meltwater will reach the base of the <span class="hlt">ice</span> <span class="hlt">sheet</span>. The relatively steep topography at the upslope edge of the ablation zone units combined with the larger water flux suggests that supercooling plays a greater role in their formation. The <span class="hlt">ice</span> qualities of the ablation zone units should reflect the relatively fresh surface melt whereas the chemistry of the interior units should reflect solute-rich basal melt. Changes in basal conditions such as the presence of till patches may contribute to the formation of the large basal units near the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19790015307','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19790015307"><span>Remote sensing of <span class="hlt">snow</span> and <span class="hlt">ice</span>: A review of the research in the United States 1975 - 1978</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rango, A.</p> <p>1979-01-01</p> <p>Research work in the United States from 1975-1978 in the field of remote sensing of <span class="hlt">snow</span> and <span class="hlt">ice</span> is reviewed. Topics covered include snowcover mapping, snowmelt runoff forecasting, demonstration projects, <span class="hlt">snow</span> water equivalent and free water content determination, glaciers, river and lake <span class="hlt">ice</span>, and sea <span class="hlt">ice</span>. A bibliography of 200 references is included.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_20 --> <div id="page_21" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="401"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.4464P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.4464P"><span>Reconstructing the post-LGM decay of the Eurasian <span class="hlt">Ice</span> <span class="hlt">Sheets</span> with <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Models; data-model comparison and focus on the Storfjorden (Svalbard) <span class="hlt">ice</span> stream dynamics history</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Petrini, Michele; Kirchner, Nina; Colleoni, Florence; Camerlenghi, Angelo; Rebesco, Michele; Lucchi, Renata G.; Forte, Emanuele; Colucci, Renato R.</p> <p>2017-04-01</p> <p>The challenge of reconstructing palaeo-<span class="hlt">ice</span> <span class="hlt">sheets</span> past growth and decay represent a critical task to better understand mechanisms of present and future global climate change. Last Glacial Maximum (LGM), and the subsequent deglaciation until Pre-Industrial time (PI) represent an excellent testing ground for numerical <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Models (ISMs), due to the abundant data available that can be used in an ISM as boundary conditions, forcings or constraints to test the ISMs results. In our study, we simulate with ISMs the post-LGM decay of the Eurasian <span class="hlt">Ice</span> <span class="hlt">Sheets</span>, with a focus on the marine-based Svalbard-Barents Sea-Kara Sea <span class="hlt">Ice</span> <span class="hlt">Sheet</span>. In particular, we aim to reconstruct the Storfjorden <span class="hlt">ice</span> stream dynamics history by comparing the model results with the marine geological data (MSGLs, GZWs, sediment cores analysis) available from the area, e.g., Pedrosa et al. 2011, Rebesco et al. 2011, 2013, Lucchi et al. 2013. Two hybrid SIA/SSA ISMs are employed, GRISLI, Ritz et al. 2001, and PSU, Pollard&DeConto 2012. These models differ mainly in the complexity with which grounding line migration is treated. Climate forcing is interpolated by means of climate indexes between LGM and PI climate. Regional climate indexes are constructed based on the non-accelerated deglaciation transient experiment carried out with CCSM3, Liu et al. 2009. Indexes representative of the climate evolution over Siberia, Svalbard and Scandinavia are employed. The impact of such refined representation as opposed to the common use of the NGRIP δ18O index for transient experiments is analysed. In this study, the <span class="hlt">ice</span>-ocean interaction is crucial to reconstruct the Storfjorden <span class="hlt">ice</span> stream dynamics history. To investigate the sensitivity of the <span class="hlt">ice</span> shelf/stream retreat to ocean temperature, we allow for a space-time variation of basal melting under the <span class="hlt">ice</span> shelves by testing two-equations implementations based on Martin et al. 2011 forced with simulated ocean temperature and salinity from the TraCE-21ka coupled</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA629258','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA629258"><span>Passive Polarimetric Remote Sensing of <span class="hlt">Snow</span> and <span class="hlt">Ice</span></span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1997-09-30</p> <p>In recent years, polarimetric radiometry has shown great potential to revolutionize passive remote sensing of the ocean surface. As a result, several...polarimetric radiometer, in 2001. This project explores the possibility of applying this new technology to remote sensing in the Polar Regions by investigating the polarimetric signature of <span class="hlt">ice</span> and <span class="hlt">snow</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014CliPa..10.2135S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014CliPa..10.2135S"><span>Interaction of <span class="hlt">ice</span> <span class="hlt">sheets</span> and climate during the past 800 000 years</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stap, L. B.; van de Wal, R. S. W.; de Boer, B.; Bintanja, R.; Lourens, L. J.</p> <p>2014-12-01</p> <p>During the Cenozoic, land <span class="hlt">ice</span> and climate interacted on many different timescales. On long timescales, the effect of land <span class="hlt">ice</span> on global climate and sea level is mainly set by large <span class="hlt">ice</span> <span class="hlt">sheets</span> in North America, Eurasia, Greenland and Antarctica. The climatic forcing of these <span class="hlt">ice</span> <span class="hlt">sheets</span> is largely determined by the meridional temperature profile resulting from radiation and greenhouse gas (GHG) forcing. As a response, the <span class="hlt">ice</span> <span class="hlt">sheets</span> cause an increase in albedo and surface elevation, which operates as a feedback in the climate system. To quantify the importance of these climate-land <span class="hlt">ice</span> processes, a zonally averaged energy balance climate model is coupled to five one-dimensional <span class="hlt">ice</span> <span class="hlt">sheet</span> models, representing the major <span class="hlt">ice</span> <span class="hlt">sheets</span>. In this study, we focus on the transient simulation of the past 800 000 years, where a high-confidence CO2 record from <span class="hlt">ice</span> core samples is used as input in combination with Milankovitch radiation changes. We obtain simulations of atmospheric temperature, <span class="hlt">ice</span> volume and sea level that are in good agreement with recent proxy-data reconstructions. We examine long-term climate-<span class="hlt">ice-sheet</span> interactions by a comparison of simulations with uncoupled and coupled <span class="hlt">ice</span> <span class="hlt">sheets</span>. We show that these interactions amplify global temperature anomalies by up to a factor of 2.6, and that they increase polar amplification by 94%. We demonstrate that, on these long timescales, the <span class="hlt">ice</span>-albedo feedback has a larger and more global influence on the meridional atmospheric temperature profile than the surface-height-temperature feedback. Furthermore, we assess the influence of CO2 and insolation by performing runs with one or both of these variables held constant. We find that atmospheric temperature is controlled by a complex interaction of CO2 and insolation, and both variables serve as thresholds for northern hemispheric glaciation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016Icar..271..237C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016Icar..271..237C"><span>Lava heating and loading of <span class="hlt">ice</span> <span class="hlt">sheets</span> on early Mars: Predictions for meltwater generation, groundwater recharge, and resulting landforms</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cassanelli, James P.; Head, James W.</p> <p>2016-06-01</p> <p> accumulate to a sufficient thickness to raise the <span class="hlt">ice</span>-melting isotherm to the base of the superposed lavas. In these locations, if lava accumulation occurs rapidly, bottom-up melting of the <span class="hlt">ice</span> <span class="hlt">sheet</span> can continue, or begin, after lava accumulation has completed in a process we term "deferred melting". Subsurface mass loss through melting of the buried <span class="hlt">ice</span> <span class="hlt">sheets</span> is predicted to cause substantial subsidence in the superposed lavas, leading to the formation of associated collapse features including fracture systems, depressions, surface faulting and folding, wrinkle-ridge formation, and chaos terrain. In addition, if meltwater generated from the lava heating and loading process becomes trapped at the lava flow margins due to the presence of impermeable confining units, large highly pressurized episodic flooding events could occur. Examination of the study area reveals geological features which are generally consistent with those predicted to form as a result of the <span class="hlt">ice</span> <span class="hlt">sheet</span> lava heating and loading process, suggesting the presence of surface <span class="hlt">snow</span> and <span class="hlt">ice</span> during the Late Noachian to Early Hesperian period.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.A23C0165M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.A23C0165M"><span>Influence of projected <span class="hlt">snow</span> and sea-<span class="hlt">ice</span> changes on future climate in heavy snowfall region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Matsumura, S.; Sato, T.</p> <p>2011-12-01</p> <p><span class="hlt">Snow/ice</span> albedo and cloud feedbacks are critical for climate change projection in cryosphere regions. However, future <span class="hlt">snow</span> and sea-<span class="hlt">ice</span> distributions are significantly different in each GCM. Thus, surface albedo in cryosphere regions is one of the causes of the uncertainty for climate change projection. Northern Japan is one of the heaviest snowfall regions in the world. In particular, Hokkaido is bounded on the north by the Okhotsk Sea, where is the southernmost ocean in the Northern Hemisphere that is covered with sea <span class="hlt">ice</span> during winter. Wintertime climate around Hokkaido is highly sensitive to fluctuations in <span class="hlt">snow</span> and sea-<span class="hlt">ice</span>. The purpose of this study is to evaluate the influence of global warming on future climate around Hokkaido, using the Pseudo-Global-Warming method (PGW) by a regional climate model. The boundary conditions of the PGW run were obtained by adding the difference between the future (2090s) and past (1990s) climates simulated by coupled general circulation model (MIROC3.2 medres), which is from the CMIP3 multi-model dataset, into the 6-hourly NCEP reanalysis (R-2) and daily OISST data in the past climate (CTL) run. The PGW experiments show that <span class="hlt">snow</span> depth significantly decreases over mountainous areas and <span class="hlt">snow</span> cover mainly decreases over plain areas, contributing to higher surface warming due to the decreased <span class="hlt">snow</span> albedo. Despite the <span class="hlt">snow</span> reductions, precipitation mainly increases over the mountainous areas because of enhanced water vapor content. However, precipitation decreases over the Japan Sea and the coastal areas, indicating the weakening of a convergent cloud band, which is formed by convergence between cold northwesteries from the Eurasian continent and anticyclonic circulation over the Okhotsk Sea. These results suggest that Okhotsk sea-<span class="hlt">ice</span> decline may change the atmospheric circulation and the resulting effect on cloud formation, resulting in changes in winter <span class="hlt">snow</span> or precipitation. We will also examine another CMIP3 model (MRI-CGCM2</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45.1481D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45.1481D"><span>Limited Impact of Subglacial Supercooling Freeze-on for Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Stratigraphy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dow, Christine F.; Karlsson, Nanna B.; Werder, Mauro A.</p> <p>2018-02-01</p> <p>Large units of disrupted radiostratigraphy (UDR) are visible in many radio-echo sounding data sets from the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span>. This study investigates whether supercooling freeze-on rates at the bed can cause the observed UDR. We use a subglacial hydrology model to calculate both freezing and melting rates at the base of the <span class="hlt">ice</span> <span class="hlt">sheet</span> in a distributed <span class="hlt">sheet</span> and within basal channels. We find that while supercooling freeze-on is a phenomenon that occurs in many areas of the <span class="hlt">ice</span> <span class="hlt">sheet</span>, there is no discernible correlation with the occurrence of UDR. The supercooling freeze-on rates are so low that it would require tens of thousands of years with minimal downstream <span class="hlt">ice</span> motion to form the hundreds of meters of disrupted radiostratigraphy. Overall, the melt rates at the base of the <span class="hlt">ice</span> <span class="hlt">sheet</span> greatly overwhelm the freeze-on rates, which has implications for mass balance calculations of Greenland <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20170010244&hterms=sea&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsea','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20170010244&hterms=sea&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsea"><span>Improvements in <span class="hlt">Ice-Sheet</span> Sea-Level Projections</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Shepherd, Andrew; Nowicki, Sophie</p> <p>2017-01-01</p> <p><span class="hlt">Ice</span> losses from Antarctica and Greenland are the largest uncertainty in sea-level projections. Nevertheless, improvements in <span class="hlt">ice-sheet</span> models over recent decades have led to closer agreement with satellite observations, keeping track with their increasing contribution to global sea-level rise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C23A1213G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C23A1213G"><span>The frequency response of a coupled <span class="hlt">ice</span> <span class="hlt">sheet-ice</span> shelf-ocean system to climate forcing variability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goldberg, D.; Snow, K.; Jordan, J. R.; Holland, P.; Arthern, R. J.</p> <p>2017-12-01</p> <p>Changes at the West Antarctic <span class="hlt">ice</span>-ocean boundary in recent decades has triggered significant increases in the regions contribution to global sea-level rise, coincident with large scale, and in some cases potentially unstable, grounding line retreat. Much of the induced change is thought to be driven by fluctuations in the oceanic heat available at the <span class="hlt">ice</span>-ocean boundary, transported on-shelf via warm Circumpolar Deep Water (CDW). However, the processes in which ocean heat drives <span class="hlt">ice-sheet</span> loss remains poorly understood, with observational studies routinely hindered by the extreme environment notorious to the Antarctic region. In this study we apply a novel synchronous coupled <span class="hlt">ice</span>-ocean model, developed within the MITgcm, and are thus able to provide detailed insight into the impacts of short time scale (interannual to decadal) climate variability and feedbacks within the <span class="hlt">ice</span>-ocean system. Feedbacks and response are assessed in an idealised <span class="hlt">ice-sheet</span>/ocean-cavity configuration in which the far field ocean condition is adjusted to emulate periodic climate variability patterns. We reveal a non-linear response of the <span class="hlt">ice-sheet</span> to periodic variations in thermocline depth. These non-linearities illustrate the heightened sensitivity of fast flowing <span class="hlt">ice</span>-shelves to periodic perturbations in heat fluxes occurring at interannual and decadal time scales. The results thus highlight how small perturbations in variable climate forcing, like that of ENSO, may trigger large changes in <span class="hlt">ice-sheet</span> response.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..11.8790H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..11.8790H"><span>Study of elevation changes along a profile crossing the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hvidegaard, S. M.; Sandberg, L.</p> <p>2009-04-01</p> <p>In recent years much research has focused on determining how the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> is responding to the observed climate changes. There is wide agreement on the fact that the <span class="hlt">Ice</span> <span class="hlt">Sheet</span> is currently loosing mass, and studies have shown that the mass loss is found near the <span class="hlt">ice</span> edge and that no significant changes are found in the central part of the <span class="hlt">Ice</span> <span class="hlt">Sheet</span>. As a part of European Space Agency's CryoSat Validation Experiment (CryoVEx) running from 2004 to 2008, the National Space Institute (DTU Space) measured the elevations along a profile crossing the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span>. The elevation observations were carried out in 2004, 2006 and 2008 using airborne laser altimetry from a Twin Otter aircraft. The observed profile follows the old EGIG line (Expédition Glaciologique au Groenland, measured in the 1950's) situated between 69-71N, heading nearly east-west. This unique dataset gives the opportunity to study elevation changes along the profile crossing the <span class="hlt">ice</span> <span class="hlt">sheet</span>. With this work, we outline the observed elevation changes from the different zones of the <span class="hlt">ice</span> <span class="hlt">sheet</span>. We furthermore compare elevation changes based on coincident ICESat and airborne laser altimeter data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C51A0962S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C51A0962S"><span>A 25-year Record of Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Elevation and Mass Change</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shepherd, A.; Muir, A. S.; Sundal, A.; McMillan, M.; Briggs, K.; Hogg, A.; Engdahl, M.; Gilbert, L.</p> <p>2017-12-01</p> <p>Since 1992, the European Remote-Sensing (ERS-1 and ERS-2), ENVISAT, and CryoSat-2 satellite radar altimeters have measured the Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> surface elevation, repeatedly, at approximately monthly intervals. These data constitute the longest continuous record of <span class="hlt">ice</span> <span class="hlt">sheet</span> 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 <span class="hlt">ice</span> <span class="hlt">sheets</span>, and of parts of the Antarctic Peninsula <span class="hlt">ice</span> <span class="hlt">sheet</span>, over a 25-year period. The root mean square difference between elevation rates computed from our survey and 257,296 estimates determined from airborne laser measurements is 54 cm/yr. The longevity of the satellite altimeter data record allows to identify and chart the evolution of changes associated with meteorology and <span class="hlt">ice</span> flow, and we estimate that 3.6 % of the continental <span class="hlt">ice</span> <span class="hlt">sheet</span>, 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 <span class="hlt">ice</span> <span class="hlt">sheet</span> drainage basins and the root mean square difference between these and independent estimates derived from satellite gravimetry is less than 5 Gt yr-1.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014QSRv...87...60H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014QSRv...87...60H"><span>The sea-level fingerprints of <span class="hlt">ice-sheet</span> collapse during interglacial periods</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hay, Carling; Mitrovica, Jerry X.; Gomez, Natalya; Creveling, Jessica R.; Austermann, Jacqueline; E. Kopp, Robert</p> <p>2014-03-01</p> <p>Studies of sea level during previous interglacials provide insight into the stability of polar <span class="hlt">ice</span> <span class="hlt">sheets</span> in the face of global climate change. Commonly, these studies correct ancient sea-level highstands for the contaminating effect of isostatic adjustment associated with past <span class="hlt">ice</span> age cycles, and interpret the residuals as being equivalent to the peak eustatic sea level associated with excess melting, relative to present day, of ancient polar <span class="hlt">ice</span> <span class="hlt">sheets</span>. However, the collapse of polar <span class="hlt">ice</span> <span class="hlt">sheets</span> produces a distinct geometry, or fingerprint, of sea-level change, which must be accounted for to accurately infer peak eustatic sea level from site-specific residual highstands. To explore this issue, we compute fingerprints associated with the collapse of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span>, West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span>, and marine sectors of the East Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> in order to isolate regions that would have been subject to greater-than-eustatic sea-level change for all three cases. These fingerprints are more robust than those associated with modern melting events, when applied to infer eustatic sea level, because: (1) a significant collapse of polar <span class="hlt">ice</span> <span class="hlt">sheets</span> reduces the sensitivity of the computed fingerprints to uncertainties in the geometry of the melt regions; and (2) the sea-level signal associated with the collapse will dominate the signal from steric effects. We evaluate these fingerprints at a suite of sites where sea-level records from interglacial marine isotopes stages (MIS) 5e and 11 have been obtained. Using these results, we demonstrate that previously discrepant estimates of peak eustatic sea level during MIS5e based on sea-level markers in Australia and the Seychelles are brought into closer accord.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19990025392','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19990025392"><span>Satellite Detection of Smoke Aerosols Over a <span class="hlt">Snow/Ice</span> Surface by TOMS</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hsu, N. Christina; Herman, Jay R.; Gleason, J. F.; Torres, O.; Seftor, C. J.</p> <p>1998-01-01</p> <p>The use of TOMS (Total Ozone Mapping Spectrometer) satellite data demonstrates the recently developed technique of using satellite UV radiance measurements to detect absorbing tropospheric aerosols is effective over <span class="hlt">snow/ice</span> surfaces. Instead of the traditional single wavelength (visible or infrared) method of measuring tropospheric aerosols, this method takes advantage of the wavelength dependent reduction in the backscattered radiance due to the presence of absorbing aerosols over <span class="hlt">snow/ice</span> surfaces. An example of the resulting aerosol distribution derived from TOMS data is shown for an August 1998 event in which smoke generated by Canadian forest fires drifts over and across Greenland. As the smoke plume moved over Greenland, the TOMS observed 380 nm reflectivity over the <span class="hlt">snow/ice</span> surface dropped drastically from 90-100% down to 30-40%. To study the effects of this smoke plume in both the UV and visible regions of the spectrum, we compared a smoke-laden spectrum taken over Greenland by the high spectral resolution (300 to 800 nm) GOME instrument with one that is aerosol-free. We also discuss the results of modeling the darkening effects of various types of absorbing aerosols over <span class="hlt">snow/ice</span> surfaces using a radiative transfer code. Finally, we investigated the history of such events by looking at the nearly twenty year record of TOMS aerosol index measurements and found that there is a large interannual variability in the amount of smoke aerosols observed over Greenland. This information will be available for studies of radiation and transport properties in the Arctic.</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> <span class="hlt">sheet</span> <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> <span class="hlt">sheet</span> 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> <span class="hlt">sheet</span> 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 mass flux that satisfies the contact conditions. When no sliding is allowed at the bed, however, we find a range of mass fluxes satisfy the contact conditions. The effect of 'backpressure' on the solutions is investigated, and is found to have no affect on the qualitative behaviour of the junctions. To the extent that the numerical, linearly viscous treatment may be applied to the case of <span class="hlt">ice</span> flowing out over the ocean, we conclude that when sliding is present, Weertman's 'instability' hypothesis holds.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ACP....18.4981G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ACP....18.4981G"><span>Concentrations and source regions of light-absorbing particles in <span class="hlt">snow/ice</span> in northern Pakistan and their impact on <span class="hlt">snow</span> albedo</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gul, Chaman; Praveen Puppala, Siva; Kang, Shichang; Adhikary, Bhupesh; Zhang, Yulan; Ali, Shaukat; Li, Yang; Li, Xiaofei</p> <p>2018-04-01</p> <p>Black carbon (BC), water-insoluble organic carbon (OC), and mineral dust are important particles in <span class="hlt">snow</span> and <span class="hlt">ice</span> which significantly reduce albedo and accelerate melting. Surface <span class="hlt">snow</span> and <span class="hlt">ice</span> samples were collected from the Karakoram-Himalayan region of northern Pakistan during 2015 and 2016 in summer (six glaciers), autumn (two glaciers), and winter (six mountain valleys). The average BC concentration overall was 2130 ± 1560 ng g-1 in summer samples, 2883 ± 3439 ng g-1 in autumn samples, and 992 ± 883 ng g-1 in winter samples. The average water-insoluble OC concentration overall was 1839 ± 1108 ng g-1 in summer samples, 1423 ± 208 ng g-1 in autumn samples, and 1342 ± 672 ng g-1 in winter samples. The overall concentration of BC, OC, and dust in aged <span class="hlt">snow</span> samples collected during the summer campaign was higher than the concentration in <span class="hlt">ice</span> samples. The values are relatively high compared to reports by others for the Himalayas and the Tibetan Plateau. This is probably the result of taking more representative samples at lower elevation where deposition is higher and the effects of ageing and enrichment are more marked. A reduction in <span class="hlt">snow</span> albedo of 0.1-8.3 % for fresh <span class="hlt">snow</span> and 0.9-32.5 % for aged <span class="hlt">snow</span> was calculated for selected solar zenith angles during daytime using the <span class="hlt">Snow</span>, <span class="hlt">Ice</span>, and Aerosol Radiation (SNICAR) model. The daily mean albedo was reduced by 0.07-12.0 %. The calculated radiative forcing ranged from 0.16 to 43.45 W m-2 depending on <span class="hlt">snow</span> type, solar zenith angle, and location. The potential source regions of the deposited pollutants were identified using spatial variance in wind vector maps, emission inventories coupled with backward air trajectories, and simple region-tagged chemical transport modeling. Central, south, and west Asia were the major sources of pollutants during the sampling months, with only a small contribution from east Asia. Analysis based on the Weather Research and Forecasting (WRF-STEM) chemical transport model identified a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140006608','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140006608"><span>A Reconciled Estimate of <span class="hlt">Ice-Sheet</span> Mass Balance</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>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; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20140006608'); toggleEditAbsImage('author_20140006608_show'); toggleEditAbsImage('author_20140006608_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20140006608_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20140006608_hide"></p> <p>2012-01-01</p> <p>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 <span class="hlt">ice</span> <span class="hlt">sheets</span>. 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 <span class="hlt">ice</span> <span class="hlt">sheets</span> 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 <span class="hlt">ice</span> <span class="hlt">sheets</span> have contributed, on average, 0.59 plus or minus 0.20 millimeter year(sup -1) to the rate of global sea-level rise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17829380','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17829380"><span>Satellite radar interferometry for monitoring <span class="hlt">ice</span> <span class="hlt">sheet</span> motion: application to 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>Goldstein, R M; Engelhardt, H; Kamb, B; Frolich, R M</p> <p>1993-12-03</p> <p>Satellite radar interferometry (SRI) provides a sensitive means of monitoring the flow velocities and grounding-line positions of <span class="hlt">ice</span> streams, which are indicators of response of the <span class="hlt">ice</span> <span class="hlt">sheets</span> to climatic change or internal instability. The detection limit is about 1.5 millimeters for vertical motions and about 4 millimeters for horizontal motions in the radar beam direction. The grounding line, detected by tidal motions where the <span class="hlt">ice</span> goes afloat, can be mapped at a resolution of approximately 0.5 kilometer. The SRI velocities and grounding line of the Rutford <span class="hlt">Ice</span> Stream, Antarctica, agree fairly well with earlier ground-based data. The combined use of SRI and other satellite methods is expected to provide data that will enhance the understanding of <span class="hlt">ice</span> stream mechanics and help make possible the prediction of <span class="hlt">ice</span> <span class="hlt">sheet</span> behavior.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C41A1187C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C41A1187C"><span>Formation and interpretation of eskers beneath retreating <span class="hlt">ice</span> <span class="hlt">sheets</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Creyts, T. T.; Hewitt, I.</p> <p>2017-12-01</p> <p>The retreat of the <span class="hlt">ice</span> <span class="hlt">sheets</span> during the Pleistocene left large and spectacular subglacial features exposed. Understanding these features gives us insight into how the <span class="hlt">ice</span> <span class="hlt">sheets</span> retreated, how meltwater influenced retreat, and can help inform our understanding of potential future rates of <span class="hlt">ice</span> <span class="hlt">sheet</span> retreat. Among these features, eskers, long sinuous ridges primarily composed of clastic sediments, lack a detailed explanation of how surface melt rates and <span class="hlt">ice</span> <span class="hlt">sheet</span> retreat rates influence their growth and spatial distribution. Here, we develop a theory for esker formation based on the initial work of Rothlisberger modified for sediment transport and inclusion of surface meltwater forcing. The primary subglacial ingredients include water flow through subglacial tunnels with the addition of mass balances for sediment transport. We show how eskers when water flow slows below a critical stress for sediment motion. This implies that eskers are deposited in a localized region near the snout of the <span class="hlt">ice</span> <span class="hlt">sheet</span>. Our findings suggest that very long eskers form sequentially as the <span class="hlt">ice</span> front retreats. The position of the esker follows the path of the channel mouth through time, which does not necessarily coincide with the instantaneous route of the feeding channel. However, in most cases, we expect those locations to be similar. The role of surface meltwater and the climatology associated with the forcing is crucial to the lateral spacing of the eskers. We predict that high surface melt rates lead to narrower catchments but that the greater extent of the ablation area means that channels are likely larger. At the same time, for a given channel size (and hence sediment flux), the size of a deposited esker depends on a margin retreat rate. Hence, the size of the eskers is related delicately to the balance between surface melt rates and margin retreat rates. We discuss how our theory can be combined with observed esker distributions to infer the relationship between these two rates</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C31C..05G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C31C..05G"><span>Results of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model Initialisation Experiments ISMIP6 - initMIP-Greenland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goelzer, H.; Nowicki, S.; Edwards, T.; Beckley, M.; Abe-Ouchi, A.; Aschwanden, A.; Calov, R.; Gagliardini, O.; Gillet-chaulet, F.; Golledge, N. R.; Gregory, J. M.; Greve, R.; Humbert, A.; Huybrechts, P.; Larour, E. Y.; Lipscomb, W. H.; Le ´h, S.; Lee, V.; Kennedy, J. H.; Pattyn, F.; Payne, A. J.; Rodehacke, C. B.; Rückamp, M.; Saito, F.; Schlegel, N.; Seroussi, H. L.; Shepherd, A.; Sun, S.; Vandewal, R.; Ziemen, F. A.</p> <p>2016-12-01</p> <p>Earlier large-scale Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> sea-level projections e.g. those run during <span class="hlt">ice</span>2sea and SeaRISE initiatives have shown that <span class="hlt">ice</span> <span class="hlt">sheet</span> initialisation can have a large effect on the projections and gives rise to important uncertainties. The goal of this intercomparison exercise (initMIP-Greenland) is to compare, evaluate and improve the initialization techniques used in the <span class="hlt">ice</span> <span class="hlt">sheet</span> modeling community and to estimate the associated uncertainties. It is the first in a series of <span class="hlt">ice</span> <span class="hlt">sheet</span> model intercomparison activities within ISMIP6 (<span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model Intercomparison Project for CMIP6). Two experiments for the large-scale Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> have been designed to allow intercomparison between participating models of 1) the initial present-day state of the <span class="hlt">ice</span> <span class="hlt">sheet</span> and 2) the response in two schematic forward experiments. The forward experiments serve to evaluate the initialisation in terms of model drift (forward run without any forcing) and response to a large perturbation (prescribed surface mass balance anomaly). We present and discuss final results of the intercomparison and highlight important uncertainties with respect to projections of the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> sea-level contribution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28682333','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28682333"><span>West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> retreat driven by Holocene warm water incursions.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hillenbrand, Claus-Dieter; Smith, James A; Hodell, David A; Greaves, Mervyn; Poole, Christopher R; Kender, Sev; Williams, Mark; Andersen, Thorbjørn Joest; Jernas, Patrycja E; Elderfield, Henry; Klages, Johann P; Roberts, Stephen J; Gohl, Karsten; Larter, Robert D; Kuhn, Gerhard</p> <p>2017-07-05</p> <p>Glaciological and oceanographic observations coupled with numerical models show that warm Circumpolar Deep Water (CDW) incursions onto the West Antarctic continental shelf cause melting of the undersides of floating <span class="hlt">ice</span> shelves. Because these <span class="hlt">ice</span> shelves buttress glaciers feeding into them, their ocean-induced thinning is driving Antarctic <span class="hlt">ice-sheet</span> retreat today. Here we present a multi-proxy data based reconstruction of variability in CDW inflow to the Amundsen Sea sector, the most vulnerable part of the West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span>, during the Holocene epoch (from 11.7 thousand years ago to the present). The chemical compositions of foraminifer shells and benthic foraminifer assemblages in marine sediments indicate that enhanced CDW upwelling, controlled by the latitudinal position of the Southern Hemisphere westerly winds, forced deglaciation of this sector from at least 10,400 years ago until 7,500 years ago-when an <span class="hlt">ice</span>-shelf collapse may have caused rapid <span class="hlt">ice-sheet</span> thinning further upstream-and since the 1940s. These results increase confidence in the predictive capability of current <span class="hlt">ice-sheet</span> models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910017259','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910017259"><span>West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Initiative. Volume 2: Discipline Reviews</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bindschadler, Robert A. (Editor)</p> <p>1991-01-01</p> <p>Seven discipline review papers are presented on the state of the knowledge of West Antarctica and opinions on how that knowledge must be increased to predict the future behavior of this <span class="hlt">ice</span> <span class="hlt">sheet</span> and to assess its potential to collapse, rapidly raising the global sea level. These are the goals of the West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Initiative (WAIS).</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_21 --> <div id="page_22" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="421"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C31D..03C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C31D..03C"><span>Modulation of Sea <span class="hlt">Ice</span> Melt Onset and Retreat in the Laptev Sea by the Timing of <span class="hlt">Snow</span> Retreat in the West Siberian Plain</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Crawford, A. D.; Stroeve, J.; Serreze, M. C.; Rajagopalan, B.; Horvath, S.</p> <p>2017-12-01</p> <p>As much of the Arctic Ocean transitions to <span class="hlt">ice</span>-free conditions in summer, efforts have increased to improve seasonal forecasts of not only sea <span class="hlt">ice</span> extent, but also the timing of melt onset and retreat. This research investigates the potential of regional terrestrial <span class="hlt">snow</span> retreat in spring as a predictor for subsequent sea <span class="hlt">ice</span> melt onset and retreat in Arctic seas. One pathway involves earlier <span class="hlt">snow</span> retreat enhancing atmospheric moisture content, which increases downwelling longwave radiation over sea <span class="hlt">ice</span> cover downstream. Another pathway involves manipulation of jet stream behavior, which may affect the sea <span class="hlt">ice</span> pack via both dynamic and thermodynamic processes. Although several possible connections between <span class="hlt">snow</span> and sea <span class="hlt">ice</span> regions are identified using a mutual information criterion, the physical mechanisms linking <span class="hlt">snow</span> retreat and sea <span class="hlt">ice</span> phenology are most clearly exemplified by variability of <span class="hlt">snow</span> retreat in the West Siberian Plain impacting melt onset and sea <span class="hlt">ice</span> retreat in the Laptev Sea. The detrended time series of <span class="hlt">snow</span> retreat in the West Siberian Plain explains 26% of the detrended variance in Laptev Sea melt onset (29% for sea <span class="hlt">ice</span> retreat). With modest predictive skill and an average time lag of 53 (88) days between <span class="hlt">snow</span> retreat and sea <span class="hlt">ice</span> melt onset (retreat), West Siberian Plains <span class="hlt">snow</span> retreat is useful for refining seasonal sea <span class="hlt">ice</span> predictions in the Laptev Sea.</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-Sheet</span> 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> <span class="hlt">Sheet</span> (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-sheet</span> extent are used to spin-up predictive <span class="hlt">ice-sheet</span> models and correct mass-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-sheet</span> model simulations suggest played a key role in Holocene <span class="hlt">ice</span>-mass 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-sheet</span> 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-sheet</span> mass 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://ntrs.nasa.gov/search.jsp?R=20040171463&hterms=SSM&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DSSM','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040171463&hterms=SSM&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DSSM"><span>Analysis of Summer 2002 Melt Extent on the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> using MODIS and SSM/I Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hall, Dorothy K.; Williams, Richard S., Jr.; Steffen, Konrad; Chien, Y. L.; Foster, James L.; Robinson, David A.; Riggs, George A.</p> <p>2004-01-01</p> <p>Previous work has shown that the summer of 2002 had the greatest area of <span class="hlt">snow</span> melt extent on the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> ever recorded using passive-microwave data. In this paper, we compare the 0 degree isotherm derived from the Moderate-Resolution Imaging Spectroradiometer (MODIS) instrument, with Special Sensor Microwave/Imager (SSM/I)-derived melt, at the time of the maximum melt extent in 2002. To validate the MODIS-derived land-surface temperatures (LSTs), we compared the MODIS LSTs with air temperatures from nine stations (using 11 different data points) and found that they agreed to within 2.3 plus or minus 2.09 C, with station temperatures consistently lower than the MODIS LSTs. According to the MODIS LST, the maximum surface melt extended to approximately 2300 m in southern Greenland; while the SSM/I measurements showed that the maximum melt extended to nearly 2700 m in southeastern Greenland. The MODIS and SSM/I data are complementary in providing detailed information about the progression of surface and near-surface melt on the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040171217','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040171217"><span>Analysis of Summer 2002 Melt Extent on the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> using MODIS and SSM/I Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hall, Dorothy K.; Williams, Richard S.; Steffen, Konrad; Chien, Janet Y. L.</p> <p>2004-01-01</p> <p>Previous work has shown that the summer of 2002 had the greatest area of <span class="hlt">snow</span> melt extent on the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> ever recorded using passive-microwave data. In this paper, we compare the 0 deg. isotherm derived from the Moderate-Resolution Imaging Spectroradiometer (MODIS) instrument, with Special Sensor Microwave/Imager (SSM/I)-derived melt, at the time of the maximum melt extent in 2002. To validate the MODIS derived land-surface temperatures (LSTs), we compared the MODIS LSTs with air temperatures from nine stations (using 11 different data points) and found that they agreed to within 2.3 +/- 2.09 C, with station temperatures consistently lower than the MODIS LSTs. According to the MODIS LST, the maximum surface melt extended to approx. 2300 m in southern Greenland; while the SSM/I measurements showed that the maximum melt extended to nearly 2700 m in southeastern Greenland. The MODIS and SSM/I data are complementary in providing detailed information about the progression of surface and near- surface melt on the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70026165','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70026165"><span>Analysis of summer 2002 melt extent on the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> using MODIS and SSM/I 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>Hall, D.K.; Williams, R.S.; Steffen, K.; Chien, Janet Y.L.</p> <p>2004-01-01</p> <p>Previous work has shown that the summer of 2002 had the greatest area of <span class="hlt">snow</span> melt extent on the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> ever recorded using passive-microwave data. In this paper, we compare the 0?? isotherm derived from the Moderate-Resolution Imaging Spectroradiometer (MODIS) instrument, with Special Sensor Microwave/Imager (SSM/I)-derived melt, at the time of the maximum melt extent in 2002. To validate the MODIS-derived land-surface temperatures (LSTs), we compared the MODIS LSTs with air temperatures from nine stations (using 11 different data points) and found that they agreed to within 2.3??2.09??C, with station temperatures consistently lower than the MODIS LSTs. According to the MODIS LST, the maximum surface melt extended to ???2300 m in southern Greenland; while the SSM/I measurements showed that the maximum melt extended to nearly 2700 m in southeastern Greenland. The MODIS and SSM/I data are complementary in providing detailed information about the progression of surface and near-surface melt on the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70191437','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70191437"><span>Analysis of summer 2002 melt extent on the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> using MODIS and SSM/I 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>Hall, D. K.; Williams, R.S.; Steffen, K.; Chien, Janet Y.L.</p> <p>2004-01-01</p> <p>Previous work has shown that the summer of 2002 had the greatest area of <span class="hlt">snow</span> melt extent on the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> ever recorded using passive-microwave data. In this paper, we compare the 0deg isotherm derived from the Moderate-Resolution Imaging Spectroradiometer (MODIS) instrument, with Special Sensor Microwave/Imager (SSM/I)-derived melt, at the time of the maximum melt extent in 2002. To validate the MODIS-derived land-surface temperatures (LSTs), we compared the MODIS LSTs with air temperatures from nine stations (using 11 different data points) and found that they agreed to within 2.3 plusmn 2.09 degC, with station temperatures consistently lower than the MODIS LSTs. According to the MODIS LST, the maximum surface melt extended to ~2300 m in southern Greenland; while the SSM/I measurements showed that the maximum melt extended to nearly 2700 m in southeastern Greenland. The MODIS and SSM/I data are complementary in providing detailed information about the progression of surface and near-surface melt on the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018TCry...12..955C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018TCry...12..955C"><span>Meltwater storage in low-density near-surface bare <span class="hlt">ice</span> in the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> ablation zone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cooper, Matthew G.; Smith, Laurence C.; Rennermalm, Asa K.; Miège, Clément; Pitcher, Lincoln H.; Ryan, Jonathan C.; Yang, Kang; Cooley, Sarah W.</p> <p>2018-03-01</p> <p>We document the density and hydrologic properties of bare, ablating <span class="hlt">ice</span> in a mid-elevation (1215 m a.s.l.) supraglacial internally drained catchment in the Kangerlussuaq sector of the western Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span>. We find low-density (0.43-0.91 g cm-3, μ = 0.69 g cm-3) <span class="hlt">ice</span> to at least 1.1 m depth below the <span class="hlt">ice</span> <span class="hlt">sheet</span> surface. This near-surface, low-density <span class="hlt">ice</span> consists of alternating layers of water-saturated, porous <span class="hlt">ice</span> and clear solid <span class="hlt">ice</span> lenses, overlain by a thin (< 0.5 m), even lower density (0.33-0.56 g cm-3, μ = 0.45 g cm-3) unsaturated weathering crust. <span class="hlt">Ice</span> density data from 10 shallow (0.9-1.1 m) <span class="hlt">ice</span> cores along an 800 m transect suggest an average 14-18 cm of specific meltwater storage within this low-density <span class="hlt">ice</span>. Water saturation of this <span class="hlt">ice</span> is confirmed through measurable water levels (1-29 cm above hole bottoms, μ = 10 cm) in 84 % of cryoconite holes and rapid refilling of 83 % of 1 m drilled holes sampled along the transect. These findings are consistent with descriptions of shallow, depth-limited aquifers on the weathered surface of glaciers worldwide and confirm the potential for substantial transient meltwater storage within porous low-density <span class="hlt">ice</span> on the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> ablation zone surface. A conservative estimate for the ˜ 63 km2 supraglacial catchment yields 0.009-0.012 km3 of liquid meltwater storage in near-surface, porous <span class="hlt">ice</span>. Further work is required to determine if these findings are representative of broader areas of the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> ablation zone, and to assess the implications for sub-seasonal mass balance processes, surface lowering observations from airborne and satellite altimetry, and supraglacial runoff processes.</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> <span class="hlt">sheet</span> beyond 2100: Simulating its evolution and influence using the coupled climate-<span class="hlt">ice</span> <span class="hlt">sheet</span> 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> <span class="hlt">sheet</span> (GrIS) is observed undergoing a rapid change in the recent decades, with an increasing area of surface melting and ablation and a speeding mass 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> <span class="hlt">sheet</span> 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> <span class="hlt">sheet</span> 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> <span class="hlt">Sheet</span> 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 mass slowly in the 21st century, but the <span class="hlt">ice</span> retreat accelerates substantially after 2100 and <span class="hlt">ice</span> mass 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 mass balance that leads to GrIS retreat are investigated</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C13F1014L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C13F1014L"><span>The Effect of Topographic Shadowing by <span class="hlt">Ice</span> on Irradiance in the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Ablation Zone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Leidman, S. Z.; Rennermalm, A. K.; Ryan, J.; Cooper, M. G.; Smith, L. C.</p> <p>2017-12-01</p> <p>Accurately predicting runoff contributions to global sea level rise requires more refined surface mass balance (SMB) models of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (GrIS). Topographic shadowing has shown to be important in the SMB of <span class="hlt">snow</span>-covered regions, yet SMB models for the GrIS generally ignore how surface topography affects spatial variability of incoming solar radiation on a surface. In the ablation zone of Southwest Greenland, deeply incised supraglacial drainage features, fracturing, and large-scale bed deformation result in extensive areas of rough surface topography. This topography blocks direct radiation such that shadowed areas receive less energy for melting while other topographic features such as peaks recieve more energy. In this study, we quantify how shadowing from local topography features changes incoming solar radiation. We apply the ArcGIS Pro Solar Radiation Toolset to calculate the direct and diffuse irradiance in sunlit and shadowed areas by determining the sun's movement for every half hour increment of 2016. Multiple digital elevation models (DEMs) with spatial resolutions ranging from 0.06 to 5m were derived from fixed wing and quadcopter UAV imagery collected in summer 2016 and the ArcticDEM dataset. Our findings show that shadowing significantly decreases irradiance compared to smoothed surfaces where local topography is removed. This decrease is exponentially proportional to the DEM pixel sized with 5m DEMs only able to capture a small percentage of the effect. Applying these calculations to the ArcticDEM to cover a larger study area indicates that decreases in irradiance are nonlinearly proportional to elevation with highly crevassed areas showing a larger effect from shadowing. Even so, shading at higher elevations reduces irradiance enough to result in several centimeters <span class="hlt">snow</span> water equivalence (SWE) per year of over-prediction of runoff in SMB models. Furthermore, analysis of solar radiation products shows that shadowing predicts albedo</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016SPIE.9839E..0LC','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016SPIE.9839E..0LC"><span>Mapping of <span class="hlt">ice</span>, <span class="hlt">snow</span> and water using aircraft-mounted LiDAR</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Church, Philip; Matheson, Justin; Owens, Brett</p> <p>2016-05-01</p> <p>Neptec Technologies Corp. has developed a family of obscurant-penetrating 3D laser scanners (OPAL 2.0) that are being adapted for airborne platforms for operations in Degraded Visual Environments (DVE). The OPAL uses a scanning mechanism based on the Risley prism pair. Data acquisition rates can go as high as 200kHz for ranges within 240m and 25kHz for ranges exceeding 240m. The scan patterns are created by rotating two prisms under independent motor control producing a conical Field-Of-View (FOV). An OPAL laser scanner with 90° FOV was installed on a Navajo aircraft, looking down through an aperture in the aircraft floor. The rotation speeds of the Risley prisms were selected to optimize a uniformity of the data samples distribution on the ground. Flight patterns simulating a landing approach over <span class="hlt">snow</span> and <span class="hlt">ice</span> in an unprepared Arctic environment were also performed to evaluate the capability of the OPAL LiDAR to map <span class="hlt">snow</span> and <span class="hlt">ice</span> elevation distribution in real-time and highlight potential obstacles. Data was also collected to evaluate the detection of wires when flying over water, <span class="hlt">snow</span> and <span class="hlt">ice</span>. Main results and conclusions obtained from the flight data analysis are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C33D1232R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C33D1232R"><span>The Contribution to High Asia Runoff from <span class="hlt">Ice</span> and <span class="hlt">Snow</span> (CHARIS): Understanding the source and trends of cryospheric contributions to the water balance</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rittger, K.; Armstrong, R. L.; Bair, N.; Racoviteanu, A.; Brodzik, M. J.; Hill, A. F.; Wilson, A. M.; Khan, A. L.; Ramage, J. M.; Khalsa, S. J. S.; Barrett, A. P.; Raup, B. H.; Painter, T. H.</p> <p>2017-12-01</p> <p>The Contribution to High Asia Runoff from <span class="hlt">Ice</span> and <span class="hlt">Snow</span>, or CHARIS, project is systematically assessing the role that glaciers and seasonal <span class="hlt">snow</span> play in the freshwater resources of Central and South Asia. The study area encompasses roughly 3 million square kilometers of the Himalaya, Karakoram, Hindu Kush, Pamir and Tien Shan mountain ranges that drain to five major rivers: the Ganges, Brahmaputra, Indus, Amu Darya and Syr Darya. We estimate daily <span class="hlt">snow</span> and glacier <span class="hlt">ice</span> contributions to the water balance. Our automated partitioning method generates daily maps of 1) <span class="hlt">snow</span> over <span class="hlt">ice</span> (SOI), 2) exposed glacier <span class="hlt">ice</span> (EGI), 3) debris covered glacier <span class="hlt">ice</span> (DGI) and 4) <span class="hlt">snow</span> over land (SOL) using fractional <span class="hlt">snow</span> cover, <span class="hlt">snow</span> grain size, and annual minimum <span class="hlt">ice</span> and <span class="hlt">snow</span> from the 500 m MODIS-derived MODSCAG and MODICE products. Maps of <span class="hlt">snow</span> and <span class="hlt">ice</span> cover are validated using high-resolution (30 m) maps of <span class="hlt">snow</span>, <span class="hlt">ice</span>, and debris cover from Landsat. The probability of detection is 0.91 and precision is 0.85 for MODICE. We examine trends in annual and monthly <span class="hlt">snow</span> and <span class="hlt">ice</span> maps and use daily maps as inputs to a calibrated temperature-index model and an uncalibrated energy balance model, ParBal. Melt model results and measurements of isotopes and specific ions used as an independent validation of melt modeling indicate a sharp geographic contrast in the role of <span class="hlt">snow</span> and <span class="hlt">ice</span> melt to downstream water supplies between the arid Tien Shan and Pamir ranges of Central Asia, where melt water dominates dry season flows, and the monsoon influenced central and eastern Himalaya where rain controls runoff. We also compare melt onset and duration from the melt models to the Calibrated, Enhanced Resolution Passive Microwave Brightness Temperature Earth Science Data Record. Trend analysis of annual and monthly area of permanent <span class="hlt">snow</span> and <span class="hlt">ice</span> (the union of SOI and EGI) for 2000 to 2016 shows statistically significant negative trends in the Ganges and Brahmaputra basins. There are no statistically significant</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C12B..04B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C12B..04B"><span>Uncertainty Quantification for <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Science and Sea Level Projections</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Boening, C.; Schlegel, N.; Limonadi, D.; Schodlok, M.; Seroussi, H. L.; Larour, E. Y.; Watkins, M. M.</p> <p>2017-12-01</p> <p>In order to better quantify uncertainties in global mean sea level rise projections and in particular upper bounds, we aim at systematically evaluating the contributions from <span class="hlt">ice</span> <span class="hlt">sheets</span> and potential for extreme sea level rise due to sudden <span class="hlt">ice</span> mass loss. Here, we take advantage of established uncertainty quantification tools embedded within the <span class="hlt">Ice</span> <span class="hlt">Sheet</span> System Model (ISSM) as well as sensitivities to <span class="hlt">ice</span>/ocean interactions using melt rates and melt potential derived from MITgcm/ECCO2. With the use of these tools, we conduct Monte-Carlo style sampling experiments on forward simulations of the Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span>, by varying internal parameters and boundary conditions of the system over both extreme and credible worst-case ranges. Uncertainty bounds for climate forcing are informed by CMIP5 ensemble precipitation and <span class="hlt">ice</span> melt estimates for year 2100, and uncertainty bounds for ocean melt rates are derived from a suite of regional sensitivity experiments using MITgcm. Resulting statistics allow us to assess how regional uncertainty in various parameters affect model estimates of century-scale sea level rise projections. The results inform efforts to a) isolate the processes and inputs that are most responsible for determining <span class="hlt">ice</span> <span class="hlt">sheet</span> contribution to sea level; b) redefine uncertainty brackets for century-scale projections; and c) provide a prioritized list of measurements, along with quantitative information on spatial and temporal resolution, required for reducing uncertainty in future sea level rise projections. Results indicate that <span class="hlt">ice</span> <span class="hlt">sheet</span> mass loss is dependent on the spatial resolution of key boundary conditions - such as bedrock topography and melt rates at the <span class="hlt">ice</span>-ocean interface. This work is performed at and supported by the California Institute of Technology's Jet Propulsion Laboratory. Supercomputing time is also supported through a contract with the National Aeronautics and Space Administration's Cryosphere program.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C33G..01D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C33G..01D"><span>What color should <span class="hlt">snow</span> algae be and what does it mean for glacier melt?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dial, R. J.; Ganey, G. Q.; Loso, M.; Burgess, A. B.; Skiles, M.</p> <p>2017-12-01</p> <p>Specialized microbes colonize glaciers and <span class="hlt">ice</span> <span class="hlt">sheets</span> worldwide and, like all organisms, they are unable to metabolize water in its solid form. It is well understood that net solar radiation controls melt in almost all <span class="hlt">snow</span> and <span class="hlt">ice</span> covered environments, and theoretical and empirical studies have documented the substantial reduction of albedo by these microbes both on <span class="hlt">ice</span> and on <span class="hlt">snow</span>, implicating a microbial role in glacier melt. If glacial microbiomes are limited by liquid water, and the albedo-reducing properties of individual cells enhance melt rates, then natural selection should favor those microbes that melt <span class="hlt">ice</span> and <span class="hlt">snow</span> crystals most efficiently. Here we: (1) argue that natural selection favors a red color on <span class="hlt">snow</span> and a near-black color on <span class="hlt">ice</span> based on instantaneous radiative forcing. (2) Review results of the first replicated, controlled field experiment to both quantify the impact of microbes on snowmelt in "red-<span class="hlt">snow</span>" communities and demonstrate their water-limitation and (3) show the extent of <span class="hlt">snow</span>-algae's spatial distribution and estimate their contribution to snowmelt across a large Alaskan icefield using remote sensing. On the 700 km2 of a 2,000 km2 maritime icefield in Alaska where red-<span class="hlt">snow</span> was present, microbes increased snowmelt over 20% by volume, a percentage likely to increase as the climate warms and particulate pollution intensifies with important implications for models of sea level rise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.G43A1033W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.G43A1033W"><span>Combustion of available fossil-fuel resources sufficient to eliminate the Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Winkelmann, R.; Levermann, A.; Ridgwell, A.; Caldeira, K.</p> <p>2015-12-01</p> <p>The Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> stores water equivalent to 58 meters in global sea-level rise. Here we show in simulations with the Parallel <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model that burning the currently attainable fossil-fuel resources is sufficient to eliminate the <span class="hlt">ice</span> <span class="hlt">sheet</span>. With cumulative fossil-fuel emissions of 10 000 GtC, Antarctica is projected to become almost <span class="hlt">ice</span>-free with an average contribution to sea-level rise exceeding 3 meters per century during the first millennium. Consistent with recent observations and simulations, the West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> becomes unstable with 600 to 800 GtC of additional carbon emissions. Beyond this additional carbon release, the destabilization of <span class="hlt">ice</span> basins in both West- and East Antarctica results in a threshold-increase in global sea level. Unabated carbon emissions thus threaten the Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> in its entirety with associated sea-level rise that far exceeds that of all other possible sources.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1810135J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1810135J"><span>Eskers in the Keewatin region of the Laurentide <span class="hlt">Ice</span> <span class="hlt">Sheet</span> - inventory comparisons</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jorge, Marco G.; Brennand, Tracy A.; Storrar, Robert D.; Dinney, Meaghan; Perkins, Andrew</p> <p>2016-04-01</p> <p> ridge density vary spatially and sometimes exceed the differences that could be expected to result from cell-size differences and variations in image quality alone. Such non-systematic differences may be due to differences in land cover (lakes, <span class="hlt">snow</span> and vegetation) and to mapper subjectivity. An example of relatively large differences between the two inventories is a 41,000 km2 area of the Athabasca region in northern Saskatchewan, where mean length is 8x lower, and number of ridges, total length, and mean sinuosity are 21.3x, 2.4x and 1.13x higher, respectively, for inventory B. In contrast, at the <span class="hlt">ice</span> <span class="hlt">sheet</span> scale, chronological trends in morphometric indices (e.g., number of ridges per 100 km of <span class="hlt">ice</span> margin, per 1000-year time step) are similar between the two inventories. Particularly prone to subjectivity and important for glacio-hydrological interpretations, is the expert's interpretation of the nature of the gaps (e.g., post- or non-depositional) between esker ridges, which directly influences the definition of esker networks; whether two ridges mediated by a gap are assigned to a single esker or to separate eskers, depends on that interpretation. Reference: Storrar RD, Stokes CR, Evans DJ. A map of large Canadian eskers from Landsat satellite imagery. Journal of maps. 2013 Sep 1;9(3):456-73.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.C51B..07B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.C51B..07B"><span>Linking <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Freshwater Discharge and Marine production in Greenland via Fiord Circulation. 'FreshLink', an Interdisciplinary Project Involving Researchers from Multiple Countries.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bøggild, C. E.; Rysgaard, S.; Mortensen, J.; Kallenborn, R.; Truffer, M.; Forsberg, R.; Ahlstrøm, A. P.; Petersen, D.</p> <p>2008-12-01</p> <p>This interdisciplinary and international project has recently been initiated mainly with IPY funding from Denmark and Greenland. In short the project investigates the linkage between <span class="hlt">ice</span> <span class="hlt">sheet</span> freshwater release to a fiord near Nuuk (South-western Greenland) and the resulting fiord circulation. The low density melt water draining into the innermost of the long fiord forms a brackish outward sloping top layer, which exits the fiord and is balanced by entrance of nutritious salty oceanic water below. Such nutritious water, in turn, favors marine production in the fiord. The perspectives of a warmer climate, where more <span class="hlt">ice</span> <span class="hlt">sheet</span> melt water will increase the marine production, is of vital interest to investigate for the Greenland society because the present export from the country is totally dominated by living resources of the oceans. This interdisciplinary research project involves scientists from Greenland, Norway, Denmark and USA. Scientific disciplines presently covered are; marine ecology (biological production), cryospheric sciences (<span class="hlt">ice</span> <span class="hlt">sheet</span> and <span class="hlt">snow</span>-water release), pollution chemistry (separating present from ancient precipitation), marine geology (history of freshwater input), oceanography (fiord circulation), geodesy (cryospheric elevation changes), and hydrology (land runoff). First field results will be presented together with the perspectives for linking each fresh water component coming from land and <span class="hlt">ice</span> to the observed freshwater budget in the fiord.</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 Mass Balance Model for Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> 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> <span class="hlt">Sheet</span> contains nearly 3 million cubic kilometers of glacial <span class="hlt">ice</span>. If the entire <span class="hlt">ice</span> <span class="hlt">sheet</span> completely melted, sea level would raise by nearly 7 meters. There is thus considerable interest in monitoring the mass balance of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span>. Each year, the <span class="hlt">ice</span> <span class="hlt">sheet</span> 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 mass balance of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span>. 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> <span class="hlt">sheet</span> surface temperature and melt production. The englacial model predicts the evolution of temperature and meltwater within the <span class="hlt">ice</span> <span class="hlt">sheet</span>. These two models can be combined with estimates of precipitation (snowfall) to estimate the mass balance over the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span>. 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> <span class="hlt">Sheet</span>. 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> <span class="hlt">sheet</span> 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/2014APS..MARG40002H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014APS..MARG40002H"><span><span class="hlt">Ice</span> <span class="hlt">sheet</span>-ocean interactions and sea level change</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Heimbach, Patrick</p> <p>2014-03-01</p> <p>Mass loss from the Greenland and Antarctic <span class="hlt">ice</span> <span class="hlt">sheets</span> has increased rapidly since the mid-1990s. Their combined loss now accounts for about one-third of global sea level rise. In Greenland, a growing body of evidence points to the marine margins of these glaciers as the region from which this dynamic response originated. Similarly, <span class="hlt">ice</span> streams in West Antarctica that feed vast floating <span class="hlt">ice</span> shelves have exhibited large decadal changes. We review observational evidence and present physical mechanisms that might explain the observed changes, in particular in the context of <span class="hlt">ice</span> <span class="hlt">sheet</span>-ocean interactions. Processes involve cover 7 orders of magnitudes of scales, ranging from mm boundary-layer processes to basin-scale coupled atmosphere-ocean variability. We discuss observational needs to fill the gap in our mechanistic understanding.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5559208','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5559208"><span>Seismic evidence for complex sedimentary control of Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> flow</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; Hubbard, Alun L.; Booth, Adam D.; Bougamont, Marion; Dow, Christine F.; Doyle, Samuel H.; Christoffersen, Poul; Lindbäck, Katrin; Pettersson, Rickard; Fitzpatrick, Andrew A. W.; Jones, Glenn A.</p> <p>2017-01-01</p> <p>The land-terminating margin of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> has slowed down in recent decades, although the causes and implications for future <span class="hlt">ice</span> flow are unclear. Explained originally by a self-regulating mechanism where basal slip reduces as drainage evolves from low to high efficiency, recent numerical modeling invokes a sedimentary control of <span class="hlt">ice</span> <span class="hlt">sheet</span> flow as an alternative hypothesis. Although both hypotheses can explain the recent slowdown, their respective forecasts of a long-term deceleration versus an acceleration of <span class="hlt">ice</span> flow are contradictory. We present amplitude-versus-angle seismic data as the first observational test of the alternative hypothesis. We document transient modifications of basal sediment strengths by rapid subglacial drainages of supraglacial lakes, the primary current control on summer <span class="hlt">ice</span> <span class="hlt">sheet</span> flow according to our numerical model. Our observations agree with simulations of initial postdrainage sediment weakening and <span class="hlt">ice</span> flow accelerations, and subsequent sediment restrengthening and <span class="hlt">ice</span> flow decelerations, and thus confirm the alternative hypothesis. Although simulated melt season acceleration of <span class="hlt">ice</span> flow due to weakening of subglacial sediments does not currently outweigh winter slowdown forced by self-regulation, they could dominate over the longer term. Subglacial sediments beneath the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> must therefore be mapped and characterized, and a sedimentary control of <span class="hlt">ice</span> flow must be evaluated against competing self-regulation mechanisms. PMID:28835915</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28835915','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28835915"><span>Seismic evidence for complex sedimentary control of Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> flow.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kulessa, Bernd; Hubbard, Alun L; Booth, Adam D; Bougamont, Marion; Dow, Christine F; Doyle, Samuel H; Christoffersen, Poul; Lindbäck, Katrin; Pettersson, Rickard; Fitzpatrick, Andrew A W; Jones, Glenn A</p> <p>2017-08-01</p> <p>The land-terminating margin of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> has slowed down in recent decades, although the causes and implications for future <span class="hlt">ice</span> flow are unclear. Explained originally by a self-regulating mechanism where basal slip reduces as drainage evolves from low to high efficiency, recent numerical modeling invokes a sedimentary control of <span class="hlt">ice</span> <span class="hlt">sheet</span> flow as an alternative hypothesis. Although both hypotheses can explain the recent slowdown, their respective forecasts of a long-term deceleration versus an acceleration of <span class="hlt">ice</span> flow are contradictory. We present amplitude-versus-angle seismic data as the first observational test of the alternative hypothesis. We document transient modifications of basal sediment strengths by rapid subglacial drainages of supraglacial lakes, the primary current control on summer <span class="hlt">ice</span> <span class="hlt">sheet</span> flow according to our numerical model. Our observations agree with simulations of initial postdrainage sediment weakening and <span class="hlt">ice</span> flow accelerations, and subsequent sediment restrengthening and <span class="hlt">ice</span> flow decelerations, and thus confirm the alternative hypothesis. Although simulated melt season acceleration of <span class="hlt">ice</span> flow due to weakening of subglacial sediments does not currently outweigh winter slowdown forced by self-regulation, they could dominate over the longer term. Subglacial sediments beneath the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> must therefore be mapped and characterized, and a sedimentary control of <span class="hlt">ice</span> flow must be evaluated against competing self-regulation mechanisms.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_22 --> <div id="page_23" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="441"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=67188&keyword=LAKE+AND+ICE&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=67188&keyword=LAKE+AND+ICE&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>ALBEDO MODELS FOR <span class="hlt">SNOW</span> AND <span class="hlt">ICE</span> ON A FRESHWATER LAKE. (R824801)</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p><h2>Abstract</h2><p><span class="hlt">Snow</span> and <span class="hlt">ice</span> albedo measurements were taken over a freshwater lake in Minnesota for three months during the winter of 1996<sub>¯</sub>1997 for use in a winter lake water quality model. The mean albedo of new <span class="hlt">snow</span> was measured as 0.83±0.028, while the...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMPP54A..03M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMPP54A..03M"><span>Modelled Growth and Decay of the Cordilleran <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Through the Last Glacial Cycle</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marshall, S. J.; Banwell, A.</p> <p>2015-12-01</p> <p>The Cordilleran <span class="hlt">Ice</span> <span class="hlt">Sheet</span> in western North America had an enigmatic evolution during the last glacial cycle, developing out of sync with the larger Laurentide and global glaciation. The geological record suggests that the <span class="hlt">ice</span> <span class="hlt">sheet</span> emerged late, ca. 45 ka, growing to be a fully-established <span class="hlt">ice</span> <span class="hlt">sheet</span> in isotope stages 3 and 2 and deglaciating late in the glacial cycle. This has been a challenge to model, and is a paleoclimatic curiosity, because the western Cordillera of North America is heavily glacierized today, and one would intuitively expect it to act as an inception centre for the Pleistocene <span class="hlt">ice</span> <span class="hlt">sheets</span>. The region receives heavy precipitation, and modest cooling should induce large-scale glacier expansion. Indeed, a Cordilleran <span class="hlt">Ice</span> <span class="hlt">Sheet</span> quickly nucleates in isotope substage 5d in most <span class="hlt">ice</span> <span class="hlt">sheet</span> modeling studies to date, and is a resilient feature throughout the glaciation. The fact that a full-scale Cordilleran <span class="hlt">Ice</span> <span class="hlt">Sheet</span> did not develop until relatively late argues for either: (a) <span class="hlt">ice</span> <span class="hlt">sheet</span> models that have been inadequate in resolving the process of alpine-style glaciation, i.e., the coalescence of alpine icefields, or (b) a climatic history in western North America that deviated strongly from the hemispheric-scale cooling which drove the growth of the Laurentide and Scandinavian <span class="hlt">Ice</span> <span class="hlt">Sheets</span>, as recorded in Greenland. We argue that reasonable reconstructions of Cordilleran <span class="hlt">Ice</span> <span class="hlt">Sheet</span> growth and decay implicate a combination of these two considerations. Sufficient model resolution is required to capture the valley-bottom melt that suppresses icefield coalescence, while early-glacial cooling must have been modest in the Pacific sector of North America. We argue for a persistent warm, dry climate relative to that in eastern North America and the Atlantic sector, likely associated with positive feedbacks between atmospheric circulation and the nascent Laurentide <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (i.e., peristent circulation patterns similar to those of 2014-2015). This must have been</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSHE34A1450N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSHE34A1450N"><span>Export of Algal Communities from Land Fast Arctic Sea <span class="hlt">Ice</span> Influenced by Overlying <span class="hlt">Snow</span> Depth and Episodic Rain Events</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Neuer, S.; Juhl, A. R.; Aumack, C.; McHugh, C.; Wolverton, M. A.; Kinzler, K.</p> <p>2016-02-01</p> <p>Sea <span class="hlt">ice</span> algal communities dominate primary production of the coastal Arctic Ocean in spring. As the sea <span class="hlt">ice</span> bloom terminates, algae are released from the <span class="hlt">ice</span> into the underlying, nutrient-rich waters, potentially seeding blooms and feeding higher trophic levels in the water column and benthos. We studied the sea <span class="hlt">ice</span> community including export events over four consecutive field seasons (2011-2014) during the spring <span class="hlt">ice</span> algae bloom in land-fast <span class="hlt">ice</span> near Barrow, Alaska, allowing us to investigate both seasonal and interannual differences. Within each year, we observed a delay in algal export from <span class="hlt">ice</span> in areas covered by thicker <span class="hlt">snow</span> compared to areas with thinner <span class="hlt">snow</span> coverage. Variability in <span class="hlt">snow</span> cover therefore resulted in a prolonged supply of organic matter to the underlying water column. Earlier export in 2012 was followed by a shift in the diatom community within the <span class="hlt">ice</span> from pennates to centrics. During an unusual warm period in early May 2014, precipitation falling as rain substantially decreased the <span class="hlt">snow</span> cover thickness (from <span class="hlt">snow</span> depth > 20 cm down to 0-2 cm). After the early snowmelt, algae were rapidly lost from the sea <span class="hlt">ice</span>, and a subsequent bloom of taxonomically-distinct, under-<span class="hlt">ice</span> phytoplankton developed a few days later. The typical immured sea <span class="hlt">ice</span> diatoms never recovered in terms of biomass, though pennate diatoms (predominantly Nitzschia frigida) did regrow to some extent near the <span class="hlt">ice</span> bottom. Sinking rates of the under-<span class="hlt">ice</span> phytoplankton were much more variable than those of <span class="hlt">ice</span> algae particles, which would potentially impact residence time in the water column, and fluxes to the benthos. Thus, the early melt episode, triggered by rain, transitioned directly into the seasonal melt and the release of biomass from the <span class="hlt">ice</span>, shifting production from sea <span class="hlt">ice</span> to the water column, with as-of-yet unknown consequences for the springtime Arctic food web.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.C53A0279G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.C53A0279G"><span>Rapid Access <span class="hlt">Ice</span> Drill: A New Tool for Exploration of the Deep Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheets</span> and Subglacial Geology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goodge, J. W.; Severinghaus, J. P.</p> <p>2014-12-01</p> <p>The Rapid Access <span class="hlt">Ice</span> Drill (RAID) will penetrate the Antarctic <span class="hlt">ice</span> <span class="hlt">sheets</span> in order to core through deep <span class="hlt">ice</span>, the glacial bed, and into bedrock below. This new technology will provide a critical first look at the interface between major <span class="hlt">ice</span> caps and their subglacial geology. Currently in construction, RAID is a mobile drilling system capable of making several long boreholes in a single field season in Antarctica. RAID is interdisciplinary and will allow access to polar paleoclimate records in <span class="hlt">ice</span> >1 Ma, direct observation at the base of the <span class="hlt">ice</span> <span class="hlt">sheets</span>, and recovery of rock cores from the <span class="hlt">ice</span>-covered East Antarctic craton. RAID uses a diamond rock-coring system as in mineral exploration. Threaded drill-pipe with hardened metal bits will cut through <span class="hlt">ice</span> using reverse circulation of Estisol for pressure-compensation, maintenance of temperature, and removal of <span class="hlt">ice</span> cuttings. Near the bottom of the <span class="hlt">ice</span> <span class="hlt">sheet</span>, a wireline bottom-hole assembly will enable diamond coring of <span class="hlt">ice</span>, the glacial bed, and bedrock below. Once complete, boreholes will be kept open with fluid, capped, and made available for future down-hole measurement of thermal gradient, heat flow, <span class="hlt">ice</span> chronology, and <span class="hlt">ice</span> deformation. RAID will also sample for extremophile microorganisms. RAID is designed to penetrate up to 3,300 meters of <span class="hlt">ice</span> and take sample cores in less than 200 hours. This rapid performance will allow completion of a borehole in about 10 days before moving to the next drilling site. RAID is unique because it can provide fast borehole access through thick <span class="hlt">ice</span>; take short <span class="hlt">ice</span> cores for paleoclimate study; sample the glacial bed to determine <span class="hlt">ice</span>-flow conditions; take cores of subglacial bedrock for age dating and crustal history; and create boreholes for use as an observatory in the <span class="hlt">ice</span> <span class="hlt">sheets</span>. Together, the rapid drilling capability and mobility of the drilling system, along with <span class="hlt">ice</span>-penetrating imaging methods, will provide a unique 3D picture of the interior Antarctic <span class="hlt">ice</span> <span class="hlt">sheets</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20060013398','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20060013398"><span>Recent Changes in High-Latitude Glaciers, <span class="hlt">Ice</span> Caps, and <span class="hlt">Ice</span> <span class="hlt">Sheets</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Abdalati, Waleed</p> <p>2006-01-01</p> <p>The glaciers and <span class="hlt">ice</span> <span class="hlt">sheets</span> of the world contain enough <span class="hlt">ice</span> to raise sea level by approximately 70 meters if they were to disappear entirely, and most of this <span class="hlt">ice</span> is located in the climatically sensitive polar regions. Fortunately changes of this magnitude would probably take many thousands of years to occur, but recent discoveries indicate that these <span class="hlt">ice</span> masses are responding to changes in today s climate more rapidly than previously thought. These responses are likely to be of great societal significance, primarily in terms of their implications for sea level, but also in terms of how their discharge of freshwater, through melting or calving, may impact ocean circulation. For millions of years, oceans have risen and fallen as the Earth has warmed and cooled, and <span class="hlt">ice</span> on land has shrunk and grown. Today is no different in that respect, as sea levels have been rising at a rate of nearly 2 m per year during the last century (Miller and Douglas 2004), and 3 mm/yr in the last 12 years (Leuliette et al. 2004). What is different today, however, is that tens - perhaps hundreds - of millions of people live in coastal areas that are vulnerable to changes in sea level. Rising seas erode beaches, increase flood potential, and reduce the ability of barrier islands and coastal wetlands to mitigate the effects of major storms and hurricanes. The costs associated with a one-meter rise in sea level are estimated to be in the hundreds of billions of dollars in the United States alone. The worldwide costs in human terms would be far greater as some vulnerable low-lying coastal regions would become inundated, especially in poorer nations that do not have the resources to deal with such changes. Such considerations are particularly important in light of the fact that a one meter sea level rise is not significantly outside the 0.09 to 0.88 range of predictions for this century (IPCC 2001), and rises of this magnitude have occurred in the past in as little as 20 years (Fairbanks 1989</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17..233W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17..233W"><span>The Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> during the last Interglaciation: Insights from my Thesis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Whipple, Matthew; Lunt, Dan; Singarayer, Joy; Bradley, Sarah; Milne, Glenn; Wolff, Eric; Siddall, Mark</p> <p>2015-04-01</p> <p>The last interglaciation represents a period of warmer climates and higher sea levels, and a useful analogue to future climate. While many studies have focussed on the response of the Greenland <span class="hlt">Ice</span> <span class="hlt">sheet</span>, far less is known about the response of the Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span>. Here, I present the summarised results of my PhD thesis "Constraints on the minimum extent of the Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> during the last interglaciation". Firstly, I cover the timings of interglaciation in Antarctica, and their differences with respect to the Northern Hemisphere timings, based on paleo sea level indicators, and oceanic temperature records. I move on to cover climate forcings, and how they influence the <span class="hlt">ice</span> <span class="hlt">sheet</span>, relative to present, and early Holocene. Secondly, I present thesis results, from looking at <span class="hlt">ice</span> core stable water isotopes. These are compared with Isostatic and Climatic modelling results, for various different <span class="hlt">Ice</span> <span class="hlt">sheet</span> scenarios, as to the resulting Climate, from changes in Elevation, Temperature, Precipitation, and Sublimation, all contributing to the recorded stable water isotope record. Thirdly, I move on to looking at the mid-field relative sea level records, from Australia and Argentina. Using isostatic modelling, these are used to assess the relative contribution of the Eastern and Western Antarctic <span class="hlt">Ice</span> <span class="hlt">sheets</span>. Although data uncertainties result in us being to identify the contribution from West Antarctica. Overall, using model-data comparison, we find a lack of evidence for a substantial retreat of the Wilkes Subglacial basin. No data location is close enough to determine the existence of the marine based West Antarctic <span class="hlt">Ice</span> <span class="hlt">sheet</span>. Model uncertainty is unable to constrain evidence of variations in <span class="hlt">ice</span> thickness in East Antarctica.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1911256P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1911256P"><span>Using palaeoclimate data to improve models of the Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Phipps, Steven; King, Matt; Roberts, Jason; White, Duanne</p> <p>2017-04-01</p> <p><span class="hlt">Ice</span> <span class="hlt">sheet</span> models are the most descriptive tools available to simulate the future evolution of the Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (AIS), including its contribution towards changes in global sea level. However, our knowledge of the dynamics of the coupled <span class="hlt">ice</span>-ocean-lithosphere system is inevitably limited, in part due to a lack of observations. Furthemore, to build computationally efficient models that can be run for multiple millennia, it is necessary to use simplified descriptions of <span class="hlt">ice</span> dynamics. <span class="hlt">Ice</span> <span class="hlt">sheet</span> modelling is therefore an inherently uncertain exercise. The past evolution of the AIS provides an opportunity to constrain the description of physical processes within <span class="hlt">ice</span> <span class="hlt">sheet</span> models and, therefore, to constrain our understanding of the role of the AIS in driving changes in global sea level. We use the Parallel <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model (PISM) to demonstrate how palaeoclimate data can improve our ability to predict the future evolution of the AIS. A 50-member perturbed-physics ensemble is generated, spanning uncertainty in the parameterisations of three key physical processes within the model: (i) the stress balance within the <span class="hlt">ice</span> <span class="hlt">sheet</span>, (ii) basal sliding and (iii) calving of <span class="hlt">ice</span> shelves. A Latin hypercube approach is used to optimally sample the range of uncertainty in parameter values. This perturbed-physics ensemble is used to simulate the evolution of the AIS from the Last Glacial Maximum ( 21,000 years ago) to present. Palaeoclimate records are then used to determine which ensemble members are the most realistic. This allows us to use data on past climates to directly constrain our understanding of the past contribution of the AIS towards changes in global sea level. Critically, it also allows us to determine which ensemble members are likely to generate the most realistic projections of the future evolution of the AIS.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013ERL.....8a5017R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013ERL.....8a5017R"><span>Understanding Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> hydrology using an integrated multi-scale approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rennermalm, A. K.; Moustafa, S. E.; Mioduszewski, J.; Chu, V. W.; Forster, R. R.; Hagedorn, B.; Harper, J. T.; Mote, T. L.; Robinson, D. A.; Shuman, C. A.; Smith, L. C.; Tedesco, M.</p> <p>2013-03-01</p> <p>Improved understanding of Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> hydrology is critically important for assessing its impact on current and future <span class="hlt">ice</span> <span class="hlt">sheet</span> dynamics and global sea level rise. This has motivated the collection and integration of in situ observations, model development, and remote sensing efforts to quantify meltwater production, as well as its phase changes, transport, and export. Particularly urgent is a better understanding of albedo feedbacks leading to enhanced surface melt, potential positive feedbacks between <span class="hlt">ice</span> <span class="hlt">sheet</span> hydrology and dynamics, and meltwater retention in firn. These processes are not isolated, but must be understood as part of a continuum of processes within an integrated system. This letter describes a systems approach to the study of Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> hydrology, emphasizing component interconnections and feedbacks, and highlighting research and observational needs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C41B0695B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C41B0695B"><span>Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> albedo variability and feedback: 2000-2015</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.; van As, D.; Fausto, R. S.; Mottram, R.; Langen, P. P.; Steffen, K.</p> <p>2015-12-01</p> <p>Absorbed solar irradiance represents the dominant source of surface melt energy for Greenland <span class="hlt">ice</span>. Surface melting has increased as part of a positive feedback amplifier due to surface darkening. The 16 most recent summers of observations from the NASA MODIS sensor indicate a darkening exceeding 6% in July when most melting occurs. Without the darkening, the increase in surface melting would be roughly half as large. A minority of the albedo decline signal may be from sensor degradation. So, in this study, MOD10A1 and MCD43 albedo products from MODIS are evaluated for sensor degradation and anisotropic reflectance errors. Errors are minimized through calibration to GC-Net and PROMICE Greenland <span class="hlt">snow</span> and <span class="hlt">ice</span> ground control data. The seasonal and spatial variability in Greenland <span class="hlt">snow</span> and <span class="hlt">ice</span> albedo over a 16 year period is presented, including quantifying changing absorbed solar irradiance and melt enhancement due to albedo feedback using the DMI HIRHAM5 5 km model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1918952H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1918952H"><span>Demonstration of Sparse Signal Reconstruction for Radar Imaging of <span class="hlt">Ice</span> <span class="hlt">Sheets</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Heister, Anton; Scheiber, Rolf</p> <p>2017-04-01</p> <p>Conventional processing of <span class="hlt">ice</span>-sounder data produces 2-D images of the <span class="hlt">ice</span> <span class="hlt">sheet</span> and bed, where the two dimensions are along-track and depth, while the across-track direction is fixed to nadir. The 2-D images contain information about the topography and radar reflectivity of the <span class="hlt">ice</span> <span class="hlt">sheet</span>'s surface, bed, and internal layers in the along-track direction. Having multiple antenna phase centers in the across-track direction enables the production of 3-D images of the <span class="hlt">ice</span> <span class="hlt">sheet</span> and bed. Compared to conventional 2-D images, these contain additional information about the surface and bed topography, and orientation of the internal layers over a swath in the across-track direction. We apply a 3-D SAR tomographic <span class="hlt">ice</span>-sounding method based on sparse signal reconstruction [1] to the data collected by Center for Remote Sensing of <span class="hlt">Ice</span> <span class="hlt">Sheets</span> (CReSIS) in 2008 in Greenland [2] using their multichannel coherent radar depth sounder (MCoRDS). The MCoRDS data have 16 effective phase centers which allows us to better understand the performance of the method. Lastly we offer sparsity improvement by including wavelet dictionaries into the reconstruction.The results show improved scene feature resolvability in across-track direction compared to MVDR beamformer. References: [1] A. Heister, R. Scheiber, "First Analysis of Sparse Signal Reconstruction for Radar Imaging of <span class="hlt">Ice</span> <span class="hlt">Sheets</span>". In: Proceedings of EUSAR, pp. 788-791, June 2016. [2] X. Wu, K. C. Jezek, E. Rodriguez, S. Gogineni, F. Rodriguez-Morales, and A. Freeman, "<span class="hlt">Ice</span> <span class="hlt">sheet</span> bed mapping with airborne SAR tomography". IEEE Transactions on Geoscience and Remote Sensing, vol. 49, no. 10 Part 1, pp. 3791-3802, 2011.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.A23I..05F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.A23I..05F"><span>Arctic Sea Salt Aerosol from Blowing <span class="hlt">Snow</span> and Sea <span class="hlt">Ice</span> Surfaces - a Missing Natural Source in Winter</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Frey, M. M.; Norris, S. J.; Brooks, I. M.; Nishimura, K.; Jones, A. E.</p> <p>2015-12-01</p> <p>Atmospheric particles in the polar regions consist mostly of sea salt aerosol (SSA). SSA plays an important role in regional climate change through influencing the surface energy balance either directly or indirectly via cloud formation. SSA irradiated by sunlight also releases very reactive halogen radicals, which control concentrations of ozone, a pollutant and greenhouse gas. However, models under-predict SSA concentrations in the Arctic during winter pointing to a missing source. It has been recently suggested that salty blowing <span class="hlt">snow</span> above sea <span class="hlt">ice</span>, which is evaporating, to be that source as it may produce more SSA than equivalent areas of open ocean. Participation in the 'Norwegian Young Sea <span class="hlt">Ice</span> Cruise (N-<span class="hlt">ICE</span> 2015)' on board the research vessel `Lance' allowed to test this hypothesis in the Arctic sea <span class="hlt">ice</span> zone during winter. Measurements were carried out from the ship frozen into the pack <span class="hlt">ice</span> North of 80º N during February to March 2015. Observations at ground level (0.1-2 m) and from the ship's crows nest (30 m) included number concentrations and size spectra of SSA (diameter range 0.3-10 μm) as well as <span class="hlt">snow</span> particles (diameter range 50-500 μm). During and after blowing <span class="hlt">snow</span> events significant SSA production was observed. In the aerosol and <span class="hlt">snow</span> phase sulfate is fractionated with respect to sea water, which confirms sea <span class="hlt">ice</span> surfaces and salty <span class="hlt">snow</span>, and not the open ocean, to be the dominant source of airborne SSA. Aerosol shows depletion in bromide with respect to sea water, especially after sunrise, indicating photochemically driven release of bromine. We discuss the SSA source strength from blowing <span class="hlt">snow</span> in light of environmental conditions (wind speed, atmospheric turbulence, temperature and <span class="hlt">snow</span> salinity) and recommend improved model parameterisations to estimate regional aerosol production. N-<span class="hlt">ICE</span> 2015 results are then compared to a similar study carried out previously in the Weddell Sea during the Antarctic winter.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4643791','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4643791"><span>Combustion of available fossil fuel resources sufficient to eliminate the Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Winkelmann, Ricarda; Levermann, Anders; Ridgwell, Andy; Caldeira, Ken</p> <p>2015-01-01</p> <p>The Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> stores water equivalent to 58 m in global sea-level rise. We show in simulations using the Parallel <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model that burning the currently attainable fossil fuel resources is sufficient to eliminate the <span class="hlt">ice</span> <span class="hlt">sheet</span>. With cumulative fossil fuel emissions of 10,000 gigatonnes of carbon (GtC), Antarctica is projected to become almost <span class="hlt">ice</span>-free with an average contribution to sea-level rise exceeding 3 m per century during the first millennium. Consistent with recent observations and simulations, the West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> becomes unstable with 600 to 800 GtC of additional carbon emissions. Beyond this additional carbon release, the destabilization of <span class="hlt">ice</span> basins in both West and East Antarctica results in a threshold increase in global sea level. Unabated carbon emissions thus threaten the Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> in its entirety with associated sea-level rise that far exceeds that of all other possible sources. PMID:26601273</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26601273','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26601273"><span>Combustion of available fossil fuel resources sufficient to eliminate the Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Winkelmann, Ricarda; Levermann, Anders; Ridgwell, Andy; Caldeira, Ken</p> <p>2015-09-01</p> <p>The Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> stores water equivalent to 58 m in global sea-level rise. We show in simulations using the Parallel <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model that burning the currently attainable fossil fuel resources is sufficient to eliminate the <span class="hlt">ice</span> <span class="hlt">sheet</span>. With cumulative fossil fuel emissions of 10,000 gigatonnes of carbon (GtC), Antarctica is projected to become almost <span class="hlt">ice</span>-free with an average contribution to sea-level rise exceeding 3 m per century during the first millennium. Consistent with recent observations and simulations, the West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> becomes unstable with 600 to 800 GtC of additional carbon emissions. Beyond this additional carbon release, the destabilization of <span class="hlt">ice</span> basins in both West and East Antarctica results in a threshold increase in global sea level. Unabated carbon emissions thus threaten the Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> in its entirety with associated sea-level rise that far exceeds that of all other possible sources.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C41E0717L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C41E0717L"><span>Albedo Spatial Variability and Causes on the Western Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Percolation Zone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lewis, G.; Osterberg, E. C.; Hawley, R. L.; Koffman, B. G.; Marshall, H. P.; Birkel, S. D.; Dibb, J. E.</p> <p>2016-12-01</p> <p>Many recent studies have concluded that Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (GIS) mass loss has been accelerating over recent decades, but spatial and temporal variations in GIS mass balance remain poorly understood due to a complex relationship among precipitation and temperature changes, increasing melt and runoff, <span class="hlt">ice</span> discharge, and surface albedo. Satellite measurements from MODerate resolution Imaging Spectroradiometer (MODIS) indicate that albedo has been declining over the past decade, but the cause and extent of GIS albedo change remains poorly constrained by field data. As fresh <span class="hlt">snow</span> (albedo > 0.85) warms and melts, its albedo decreases due to <span class="hlt">snow</span> grain growth, promoting solar absorption, higher snowpack temperatures and further melt. However, dark impurities like soot and dust can also significantly reduce <span class="hlt">snow</span> albedo, even in the dry <span class="hlt">snow</span> zone. While many regional climate models (e.g. the Regional Atmospheric Climate MOdel - RACMO2) calculate albedo spatial resolutions on the order of 10-30 km, and MODIS averages albedo over 500 m, surface features like sastrugi can affect albedo on much smaller scales. Here we assess the relative importance of grain size and shape vs. impurity concentrations on albedo in the western GIS percolation zone. We collected broadband albedo measurements (300-2500 nm at 3-8 nm resolution) at 35 locations using an ASD FieldSpec4 spectroradiometer to simultaneously quantify radiative fluxes and spectral reflectance. Measurements were collected on 10 x 10 m, 1 x 1 km, 5 x 5 km, and 10 x 10 km grids to determine the spatial variability of albedo as part of the 850-km Greenland Traverse for Accumulation and Climate Studies (GreenTrACS) traverse from Raven/Dye 2 to Summit. Additionally, we collected shallow (0-50 cm) <span class="hlt">snow</span> pit samples every 5 cm at ASD measurement sites to quantify black carbon and mineral dust concentrations and size distributions using a Single Particle Soot Photometer and Coulter Counter, respectively. Preliminary results</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018TCry...12..993Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018TCry...12..993Z"><span>On the retrieval of sea <span class="hlt">ice</span> thickness and <span class="hlt">snow</span> depth using concurrent laser altimetry and L-band 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>Zhou, Lu; Xu, Shiming; Liu, Jiping; Wang, Bin</p> <p>2018-03-01</p> <p>The accurate knowledge of sea <span class="hlt">ice</span> parameters, including sea <span class="hlt">ice</span> thickness and <span class="hlt">snow</span> depth over the sea <span class="hlt">ice</span> cover, is key to both climate studies and data assimilation in operational forecasts. Large-scale active and passive remote sensing is the basis for the estimation of these parameters. In traditional altimetry or the retrieval of <span class="hlt">snow</span> depth with passive microwave remote sensing, although the sea <span class="hlt">ice</span> thickness and the <span class="hlt">snow</span> depth are closely related, the retrieval of one parameter is usually carried out under assumptions over the other. For example, climatological <span class="hlt">snow</span> depth data or as derived from reanalyses contain large or unconstrained uncertainty, which result in large uncertainty in the derived sea <span class="hlt">ice</span> thickness and volume. In this study, we explore the potential of combined retrieval of both sea <span class="hlt">ice</span> thickness and <span class="hlt">snow</span> depth using the concurrent active altimetry and passive microwave remote sensing of the sea <span class="hlt">ice</span> cover. Specifically, laser altimetry and L-band passive remote sensing data are combined using two forward models: the L-band radiation model and the isostatic relationship based on buoyancy model. Since the laser altimetry usually features much higher spatial resolution than L-band data from the Soil Moisture Ocean Salinity (SMOS) satellite, there is potentially covariability between the observed <span class="hlt">snow</span> freeboard by altimetry and the retrieval target of <span class="hlt">snow</span> depth on the spatial scale of altimetry samples. Statistically significant correlation is discovered based on high-resolution observations from Operation <span class="hlt">Ice</span>Bridge (OIB), and with a nonlinear fitting the covariability is incorporated in the retrieval algorithm. By using fitting parameters derived from large-scale surveys, the retrievability is greatly improved compared with the retrieval that assumes flat <span class="hlt">snow</span> cover (i.e., no covariability). Verifications with OIB data show good match between the observed and the retrieved parameters, including both sea <span class="hlt">ice</span> thickness and <span class="hlt">snow</span> depth. With</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12.2878B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12.2878B"><span>Modelling large-scale <span class="hlt">ice-sheet</span>-climate interactions at the last glacial inception</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Browne, O. J. H.; Gregory, J. M.; Payne, A. J.; Ridley, J. K.; Rutt, I. C.</p> <p>2010-05-01</p> <p>In order to investigate the interactions between coevolving climate and <span class="hlt">ice-sheets</span> on multimillenial timescales, a low-resolution atmosphere-ocean general circulation model (AOGCM) has been coupled to a three-dimensional thermomechanical <span class="hlt">ice-sheet</span> model. We use the FAMOUS AOGCM, which is almost identical in formulation to the widely used HadCM3 AOGCM, but on account of its lower resolution (7.5° longitude × 5° latitude in the atmosphere, 3.75°× 2.5° in the ocean) it runs about ten times faster. We use the community <span class="hlt">ice-sheet</span> model Glimmer at 20 km resolution, with the shallow <span class="hlt">ice</span> approximation and an annual degree-day scheme for surface mass balance. With the FAMOUS-Glimmer coupled model, we have simulated the growth of the Laurentide and Fennoscandian <span class="hlt">ice</span> <span class="hlt">sheets</span> at the last glacial inception, under constant orbital forcing and atmospheric composition for 116 ka BP. <span class="hlt">Ice</span> grows in both regions, totalling 5.8 m of sea-level equivalent in 10 ka, slower than proxy records suggest. Positive climate feedbacks reinforce this growth at local scales (order hundreds of kilometres), where changes are an order of magnitude larger than on the global average. The albedo feedback (higher local albedo means a cooler climate) is important in the initial expansion of the <span class="hlt">ice-sheet</span> area. The topography feedback (higher surface means a cooler climate) affects <span class="hlt">ice-sheet</span> thickness and is not noticeable for the first 1 ka. These two feedbacks reinforce each other. Without them, the <span class="hlt">ice</span> volume is ~90% less after 10 ka. In Laurentia, <span class="hlt">ice</span> expands initially on the Canadian Arctic islands. The glaciation of the islands eventually cools the nearby mainland climate sufficiently to produce a positive mass balance there. Adjacent to the <span class="hlt">ice-sheets</span>, cloud feedbacks tend to reduce the surface mass balance and restrain <span class="hlt">ice</span> growth; this is an example of a local feedback whose simulation requires a model that includes detailed atmospheric physics.</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> <span class="hlt">Sheet</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>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> <span class="hlt">Sheet</span> Model, simulating the flow of a three-dimensional, inherently buttressed <span class="hlt">ice-sheet</span>-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 variation of surface mass balance and basal roughness suggest that <span class="hlt">ice</span> <span class="hlt">sheets</span> 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-sheet</span> surging, such as the surging of the Laurentide <span class="hlt">Ice</span> <span class="hlt">Sheet</span>, 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/2013NatGe...6..765C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013NatGe...6..765C"><span>Dynamic behaviour of the East Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> during Pliocene warmth</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cook, Carys P.; van de Flierdt, Tina; Williams, Trevor; Hemming, Sidney R.; Iwai, Masao; Kobayashi, Munemasa; Jimenez-Espejo, Francisco J.; Escutia, Carlota; González, Jhon Jairo; Khim, Boo-Keun; McKay, Robert M.; Passchier, Sandra; Bohaty, Steven M.; Riesselman, Christina R.; Tauxe, Lisa; Sugisaki, Saiko; Galindo, Alberto Lopez; Patterson, Molly O.; Sangiorgi, Francesca; Pierce, Elizabeth L.; Brinkhuis, Henk; Klaus, Adam; Fehr, Annick; Bendle, James A. P.; Bijl, Peter K.; Carr, Stephanie A.; Dunbar, Robert B.; Flores, José Abel; Hayden, Travis G.; Katsuki, Kota; Kong, Gee Soo; Nakai, Mutsumi; Olney, Matthew P.; Pekar, Stephen F.; Pross, Jörg; Röhl, Ursula; Sakai, Toyosaburo; Shrivastava, Prakash K.; Stickley, Catherine E.; Tuo, Shouting; Welsh, Kevin; Yamane, Masako</p> <p>2013-09-01</p> <p>Warm intervals within the Pliocene epoch (5.33-2.58 million years ago) were characterized by global temperatures comparable to those predicted for the end of this century and atmospheric CO2 concentrations similar to today. Estimates for global sea level highstands during these times imply possible retreat of the East Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span>, but <span class="hlt">ice</span>-proximal evidence from the Antarctic margin is scarce. Here we present new data from Pliocene marine sediments recovered offshore of Adélie Land, East Antarctica, that reveal dynamic behaviour of the East Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> in the vicinity of the low-lying Wilkes Subglacial Basin during times of past climatic warmth. Sedimentary sequences deposited between 5.3 and 3.3 million years ago indicate increases in Southern Ocean surface water productivity, associated with elevated circum-Antarctic temperatures. The geochemical provenance of detrital material deposited during these warm intervals suggests active erosion of continental bedrock from within the Wilkes Subglacial Basin, an area today buried beneath the East Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span>. We interpret this erosion to be associated with retreat of the <span class="hlt">ice</span> <span class="hlt">sheet</span> margin several hundreds of kilometres inland and conclude that the East Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> was sensitive to climatic warmth during the Pliocene.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.G23B..01S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.G23B..01S"><span>Trends in <span class="hlt">ice</span> <span class="hlt">sheet</span> mass balance, 1992 to 2017</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shepherd, A.; 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.</p> <p>2017-12-01</p> <p>The <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Mass Balance Inter-Comparison Exercise (IMBIE) is a community effort, jointly supported by ESA and NASA, that aims to provide a consensus estimate of <span class="hlt">ice</span> <span class="hlt">sheet</span> 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 <span class="hlt">ice</span> <span class="hlt">sheet</span> 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 <span class="hlt">ice</span> <span class="hlt">sheet</span> mass balance derived from the individual techniques were then compared and combined. The result is single estimates of <span class="hlt">ice</span> <span class="hlt">sheet</span> 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.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP13E..02A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP13E..02A"><span>Possible contribution of <span class="hlt">ice-sheet</span>/lithosphere interactions to past glaciological changes 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>Alley, R. B.; Parizek, B. R.; Anandakrishnan, S.; Pollard, D.; Stevens, N. T.; Pourpoint, M.</p> <p>2017-12-01</p> <p><span class="hlt">Ice</span>-lithosphere interactions may have influenced the history of <span class="hlt">ice-sheet</span> sensitivity to climate change. The Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> (GIS) is sensitive to warming, and is likely to be largely removed if subjected to relatively small additional temperature increases. The recent report (Schaefer et al., 2016, Nature) of near-complete GIS removal under modest Pleistocene forcing suggests that GIS sensitivity may be even greater than generally modeled, but lack of major Holocene retreat is more consistent with existing models. As shown by Stevens et al. (2016, JGR), peak lithospheric flexural stresses associated with <span class="hlt">ice</span>-age GIS cycling are of the same order as dike-driving stresses in plutonic systems, and migrate over <span class="hlt">ice</span>-age cycles. The full analysis by Stevens et al. suggests the possibility that the onset of cyclic <span class="hlt">ice-sheet</span> loading allowed deep melt associated with the passage of the Icelandic hot spot beneath Greenland to work up though the crust to or near the base of the <span class="hlt">ice</span> <span class="hlt">sheet</span>, helping explain the anomalous geothermal heat fluxes observed at the head of the Northeast Greenland <span class="hlt">Ice</span> Stream and elsewhere in the northern part of GIS. If <span class="hlt">ice</span>-age cycling aided extraction of an existing reservoir of melted rock, then geothermal heat flux would have risen with the onset of extraction and migration, but with a subsequent fall associated with reservoir depletion. Simple parameterized flow-model simulations confirm intuition that a higher geothermal flux makes deglaciation easier, with the northern part of the <span class="hlt">ice</span> <span class="hlt">sheet</span> especially important. Large uncertainties remain in quantification, but we suggest the hypothesis that, following the onset of <span class="hlt">ice</span>-age cycling, deglaciation of the GIS first became easier and then more difficult in response to feedbacks involving the <span class="hlt">ice</span> <span class="hlt">sheet</span> and the geological system beneath. In turn, this suggests that evidence of past deglaciation under moderate forcing is consistent with existing <span class="hlt">ice-sheet</span> models.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_23 --> <div id="page_24" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="461"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.9548T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.9548T"><span>Biogeochemical Impact of <span class="hlt">Snow</span> Cover and Cyclonic Intrusions on the Winter Weddell Sea <span class="hlt">Ice</span> Pack</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tison, J.-L.; Schwegmann, S.; Dieckmann, G.; Rintala, J.-M.; Meyer, H.; Moreau, S.; Vancoppenolle, M.; Nomura, D.; Engberg, S.; Blomster, L. J.; Hendrickx, S.; Uhlig, C.; Luhtanen, A.-M.; de Jong, J.; Janssens, J.; Carnat, G.; Zhou, J.; Delille, B.</p> <p>2017-12-01</p> <p>Sea <span class="hlt">ice</span> is a dynamic biogeochemical reactor and a double interface actively interacting with both the atmosphere and the ocean. However, proper understanding of its annual impact on exchanges, and therefore potentially on the climate, notably suffer from the paucity of autumnal and winter data sets. Here we present the results of physical and biogeochemical investigations on winter Antarctic pack <span class="hlt">ice</span> in the Weddell Sea (R. V. Polarstern AWECS cruise, June-August 2013) which are compared with those from two similar studies conducted in the area in 1986 and 1992. The winter 2013 was characterized by a warm sea <span class="hlt">ice</span> cover due to the combined effects of deep <span class="hlt">snow</span> and frequent warm cyclones events penetrating southward from the open Southern Ocean. These conditions were favorable to high <span class="hlt">ice</span> permeability and cyclic events of brine movements within the sea <span class="hlt">ice</span> cover (brine tubes), favoring relatively high chlorophyll-a (Chl-a) concentrations. We discuss the timing of this algal activity showing that arguments can be presented in favor of continued activity during the winter due to the specific physical conditions. Large-scale sea <span class="hlt">ice</span> model simulations also suggest a context of increasingly deep <span class="hlt">snow</span>, warm <span class="hlt">ice</span>, and large brine fractions across the three observational years, despite the fact that the model is forced with a snowfall climatology. This lends support to the claim that more severe Antarctic sea <span class="hlt">ice</span> conditions, characterized by a longer <span class="hlt">ice</span> season, thicker, and more concentrated <span class="hlt">ice</span> are sufficient to increase the <span class="hlt">snow</span> depth and, somehow counterintuitively, to warm the <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP33C1338B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP33C1338B"><span>Inception of the Laurentide <span class="hlt">Ice</span> <span class="hlt">Sheet</span> using asynchronous coupling of a regional atmospheric model and an <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>Birch, L.; Cronin, T.; Tziperman, E.</p> <p>2017-12-01</p> <p>The climate over the past 0.8 million years has been dominated by <span class="hlt">ice</span> ages. <span class="hlt">Ice</span> <span class="hlt">sheets</span> have grown about every 100 kyrs, starting from warm interglacials, until they spanned continents. State-of-the-art global climate models (GCMs) have difficulty simulating glacial inception, or the transition of Earth's climate from an interglacial to a glacial state. It has been suggested that this failure may be related to their poorly resolved local mountain topography, due to their coarse spatial resolution. We examine this idea as well as the possible role of <span class="hlt">ice</span> flow dynamics missing in GCMs. We investigate the growth of the Laurentide <span class="hlt">Ice</span> <span class="hlt">Sheet</span> at 115 kya by focusing on the mountain glaciers of Canada's Baffin Island, where geologic evidence indicates the last inception occurred. We use the Weather Research and Forecasting model (WRF) in a regional, cloud-resolving configuration with resolved mountain terrain to explore how quickly Baffin Island could become glaciated with the favorable yet realizable conditions of 115 kya insolation, cool summers, and wet winters. Using the model-derived mountain glacier mass balance, we force an <span class="hlt">ice</span> <span class="hlt">sheet</span> model based on the shallow-<span class="hlt">ice</span> approximation, capturing the <span class="hlt">ice</span> flow that may be critical to the spread of <span class="hlt">ice</span> <span class="hlt">sheets</span> away from mountain <span class="hlt">ice</span> caps. The <span class="hlt">ice</span> <span class="hlt">sheet</span> model calculates the surface area newly covered by <span class="hlt">ice</span> and the change in the <span class="hlt">ice</span> surface elevation, which we then use to run WRF again. Through this type of iterated asynchronous coupling, we investigate how the regional climate responds to both larger areas of <span class="hlt">ice</span> cover and changes in <span class="hlt">ice</span> surface elevation. In addition, we use the NOAH-MP Land model to characterize the importance of land processes, like refreezing. We find that initial <span class="hlt">ice</span> growth on the Penny <span class="hlt">Ice</span> Cap causes regional cooling that increases the accumulation on the Barnes <span class="hlt">Ice</span> Cap. We investigate how <span class="hlt">ice</span> and topography changes on Baffin Island may impact both the regional climate and the large-scale circulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013TCry....7.1721L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013TCry....7.1721L"><span>Potential subglacial lake locations and meltwater drainage pathways beneath the Antarctic and Greenland <span class="hlt">ice</span> <span class="hlt">sheets</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Livingstone, S. J.; Clark, C. D.; Woodward, J.; Kingslake, J.</p> <p>2013-11-01</p> <p>We use the Shreve hydraulic potential equation as a simplified approach to investigate potential subglacial lake locations and meltwater drainage pathways beneath the Antarctic and Greenland <span class="hlt">ice</span> <span class="hlt">sheets</span>. We validate the method by demonstrating its ability to recall the locations of >60% of the known subglacial lakes beneath the Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span>. This is despite uncertainty in the <span class="hlt">ice-sheet</span> bed elevation and our simplified modelling approach. However, we predict many more lakes than are observed. Hence we suggest that thousands of subglacial lakes remain to be found. Applying our technique to the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span>, where very few subglacial lakes have so far been observed, recalls 1607 potential lake locations, covering 1.2% of the bed. Our results will therefore provide suitable targets for geophysical surveys aimed at identifying lakes beneath Greenland. We also apply the technique to modelled past <span class="hlt">ice-sheet</span> configurations and find that during deglaciation both <span class="hlt">ice</span> <span class="hlt">sheets</span> likely had more subglacial lakes at their beds. These lakes, inherited from past <span class="hlt">ice-sheet</span> configurations, would not form under current surface conditions, but are able to persist, suggesting a retreating <span class="hlt">ice-sheet</span> will have many more subglacial lakes than advancing ones. We also investigate subglacial drainage pathways of the present-day and former Greenland and Antarctic <span class="hlt">ice</span> <span class="hlt">sheets</span>. Key sectors of the <span class="hlt">ice</span> <span class="hlt">sheets</span>, such as the Siple Coast (Antarctica) and NE Greenland <span class="hlt">Ice</span> Stream system, are suggested to have been susceptible to subglacial drainage switching. We discuss how our results impact our understanding of meltwater drainage, basal lubrication and <span class="hlt">ice</span>-stream formation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.4409G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.4409G"><span>Results of the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> model initialisation experiments: ISMIP6 - initMIP-Greenland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goelzer, Heiko; Nowicki, Sophie; Edwards, Tamsin; Beckley, Matthew</p> <p>2017-04-01</p> <p><span class="hlt">Ice</span> <span class="hlt">sheet</span> model initialisation has a large effect on projected future sea-level contributions and gives rise to important uncertainties. The goal of this intercomparison exercise for the continental-scale Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> is therefore to compare, evaluate and improve the initialisation techniques used in the <span class="hlt">ice</span> <span class="hlt">sheet</span> modelling community. The initMIP-Greenland project is the first in a series of <span class="hlt">ice</span> <span class="hlt">sheet</span> model intercomparison activities within ISMIP6 (<span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model Intercomparison Project for CMIP6). The experimental set-up has been designed to allow comparison of the initial present-day state of the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> between participating models and against observations. Furthermore, the initial states are tested with two schematic forward experiments to evaluate the initialisation in terms of model drift (forward run without any forcing) and response to a large perturbation (prescribed surface mass balance anomaly). We present and discuss results that highlight the wide diversity of data sets, boundary conditions and initialisation techniques used in the community to generate initial states of the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/48384','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/48384"><span>Sulfur dioxide reactions on <span class="hlt">ice</span> surfaces: Implications for dry deposition to <span class="hlt">snow</span></span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Martha H. Conklin; Richard A. Sommerfeld; S. Kay Laird; John E. Villinski</p> <p>1993-01-01</p> <p>Controlled exposure of <span class="hlt">ice</span> to a reactive gas, SO2, demonstrated the importance of the chemical composition of the <span class="hlt">ice</span> surface on the accumulation of acidity in <span class="hlt">snow</span>. In a series of bench-scale continuous-flow column experiments run at four temperatures (-1, -8, -30 and -60°C), SO2 was shown to dissolve and to react with other species in the <span class="hlt">ice</span>-air interfacial region...</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> <span class="hlt">sheet</span> Including Shelves and Regional Sea Level Variations</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> <span class="hlt">sheet</span> (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> <span class="hlt">sheet</span> (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> <span class="hlt">sheets</span> to eustatic sea level (ESL). Most previous paleo <span class="hlt">ice</span> <span class="hlt">sheet</span> modelling simulations of the GIS recreated an <span class="hlt">ice</span> <span class="hlt">sheet</span> 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> <span class="hlt">sheet</span> 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> <span class="hlt">sheet</span> 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> <span class="hlt">sheet</span> Including Shelves and Regional Sea Level Variations</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> <span class="hlt">sheet</span> (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> <span class="hlt">sheet</span> (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> <span class="hlt">sheets</span> to eustatic sea level (ESL). Most previous paleo <span class="hlt">ice</span> <span class="hlt">sheet</span> modelling simulations of the GIS recreated an <span class="hlt">ice</span> <span class="hlt">sheet</span> 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> <span class="hlt">sheet</span> 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> <span class="hlt">sheet</span> 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('http://hdl.handle.net/2060/20140001444','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140001444"><span>ISSM: <span class="hlt">Ice</span> <span class="hlt">Sheet</span> System Model</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Larour, Eric; Schiermeier, John E.; Seroussi, Helene; Morlinghem, Mathieu</p> <p>2013-01-01</p> <p>In order to have the capability to use satellite data from its own missions to inform future sea-level rise projections, JPL needed a full-fledged <span class="hlt">ice-sheet</span>/iceshelf flow model, capable of modeling the mass balance of Antarctica and Greenland into the near future. ISSM was developed with such a goal in mind, as a massively parallelized, multi-purpose finite-element framework dedicated to <span class="hlt">ice-sheet</span> modeling. ISSM features unstructured meshes (Tria in 2D, and Penta in 3D) along with corresponding finite elements for both types of meshes. Each finite element can carry out diagnostic, prognostic, transient, thermal 3D, surface, and bed slope simulations. Anisotropic meshing enables adaptation of meshes to a certain metric, and the 2D Shelfy-Stream, 3D Blatter/Pattyn, and 3D Full-Stokes formulations capture the bulk of the <span class="hlt">ice</span>-flow physics. These elements can be coupled together, based on the Arlequin method, so that on a large scale model such as Antarctica, each type of finite element is used in the most efficient manner. For each finite element referenced above, ISSM implements an adjoint. This adjoint can be used to carry out model inversions of unknown model parameters, typically <span class="hlt">ice</span> rheology and basal drag at the <span class="hlt">ice</span>/bedrock interface, using a metric such as the observed InSAR surface velocity. This data assimilation capability is crucial to allow spinning up of <span class="hlt">ice</span> flow models using available satellite data. ISSM relies on the PETSc library for its vectors, matrices, and solvers. This allows ISSM to run efficiently on any parallel platform, whether shared or distrib- ISSM: <span class="hlt">Ice</span> <span class="hlt">Sheet</span> System Model NASA's Jet Propulsion Laboratory, Pasadena, California uted. It can run on the largest clusters, and is fully scalable. This allows ISSM to tackle models the size of continents. ISSM is embedded into MATLAB and Python, both open scientific platforms. This improves its outreach within the science community. It is entirely written in C/C++, which gives it flexibility in its</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17937301','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17937301"><span>Modeling the effect of <span class="hlt">snow</span> and <span class="hlt">ice</span> on the global environmental fate and long-range transport potential of semivolatile organic compounds.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Stocker, Judith; Scheringer, Martin; Wegmann, Fabio; Hungerbuhler, Konrad</p> <p>2007-09-01</p> <p><span class="hlt">Snow</span> and <span class="hlt">ice</span> have been implemented in a global multimedia box model to investigate the influence of these media on the environmental fate and long-range transport (LRT) of semivolatile organic compounds (SOCs). Investigated compounds include HCB, PCB28, PCB180, PBDE47, PBDE209, alpha-HCH, and dacthal. In low latitudes, <span class="hlt">snow</span> acts as a transfer medium taking up chemicals from air and releasing them to water or soil during snowmelt. In high latitudes, <span class="hlt">snow</span> and <span class="hlt">ice</span> shield water, soil, and vegetation from chemical deposition. In the model version including <span class="hlt">snow</span> and <span class="hlt">ice</span> (scenario 2), the mass of chemicals in soil in high latitudes is between 27% (HCB) and 97% (alpha-HCH) of the mass calculated with the model version without <span class="hlt">snow</span> and <span class="hlt">ice</span> (scenario 1). Amounts in Arctic seawater in scenario 2 are 8% (alpha-HCH) to 21% (dacthal) of the amounts obtained in scenario 1. For all investigated chemicals except alpha-HCH, presence of <span class="hlt">snow</span> and <span class="hlt">ice</span> in the model increases the concentration in air by a factor of 2 (HCB)to 10 (PBDE209). Because of reduced net deposition to <span class="hlt">snow</span>-covered surfaces in high latitudes, LRT to the Arctic is reduced for most chemicals whereas transport to the south is more pronounced than in scenario 1 ("southward shift"). The presence of <span class="hlt">snow</span> and <span class="hlt">ice</span> thus considerably changes the environmental fate of SOCs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.C41A0448F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.C41A0448F"><span>Operational Products Archived at the National <span class="hlt">Snow</span> and <span class="hlt">Ice</span> Data Center</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fetterer, F. M.; Ballagh, L.; Gergely, K.; Kovarik, J.; Wallace, A.; Windnagel, A.</p> <p>2009-12-01</p> <p>Sea <span class="hlt">ice</span> charts for shipping interests from the Navy/NOAA/Coast Guard National <span class="hlt">Ice</span> Center are often laboriously produced by manually interpreting and synthesizing data from many sources, both satellite and in situ. They are generally more accurate than similar products from single sources. Upward looking sonar data from U.S. Navy submarines operating in the Arctic provides information on <span class="hlt">ice</span> thickness. Similarly extensive data were available from no other source prior to the recently established reliability of <span class="hlt">ice</span> thickness estimates from polar orbiting instruments like the Geoscience Laser Altimeter System (GLAS). <span class="hlt">Snow</span> Data Assimilation System (SNODAS) products from the NOAA NWS National Operational Hydrologic Remote Sensing Center give researchers the best possible estimates of <span class="hlt">snow</span> cover and associated variables to support hydrologic modeling and analysis for the continental U.S. These and other <span class="hlt">snow</span> and <span class="hlt">ice</span> data products are produced by the U.S. Navy, the NOAA National Weather Service, and other agency entities to serve users who have an operational need: to get a ship safely to its destination, for example, or to predict stream flow. NOAA supports work at NSIDC with data from operational sources that can be used for climate research and change detection. We make these products available to a new user base, by archiving operational data, making data available online, providing documentation, and fielding questions from researchers about the data. These data demand special consideration: often they are advantageous because they are available on a schedule in near real time, but their use in climate studies is problematic since many are produced with regard for ‘best now’ and without regard for time series consistency. As arctic climate changes rapidly, operational and semi-operational products have an expanding science support role to play.</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> <span class="hlt">Sheet</span> 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> <span class="hlt">Sheet</span> (GrIS) to atmospheric variations. However, several studies suggest that the enhanced <span class="hlt">ice</span> mass loss experienced by the GrIS in the past decades is directly connected to the increasing North Atlantic temperatures. Melting of GrIS outlet glaciers triggers grounding-line retreat increasing <span class="hlt">ice</span> discharge into the ocean. This new evidence leads to consider the ocean as a relevant driver to be taken into account when modeling the evolution of the GrIS. The <span class="hlt">ice</span>-ocean interaction is a primary factor controling not only the likely future retreat of GrIS outlet glaciers, or the huge <span class="hlt">ice</span> loss in past warming climates, but also, and more strongly, the past GrIS glacial expansion. The latter assumption is supported by reconstructions which propose the GrIS to be fully marine-based during glacials, and thus more exposed to the influence of the ocean. Here, for the first time, we investigate the response of the GrIS to past oceanic changes using a three-dimensional hybrid <span class="hlt">ice-sheet/ice</span>-shelf model, which combines the Shallow <span class="hlt">Ice</span> Approximation (SIA) for slow grounded <span class="hlt">ice</span> <span class="hlt">sheets</span> and the Shallow Shelf Approximation (SSA) in <span class="hlt">ice</span> shelves and <span class="hlt">ice</span> streams. The model accounts for a time-dependent parametrisation of the marine basal melting rate, which is used to reproduce past oceanic variations. In this work simulations of the last two glacial cycles are performed. Our results show that the GrIS is very sensitive to the ocean-triggered submarine melting (freezing). Mild oceanic temperature variations lead to a rapid retreat (expansion) of the GrIS margins, which, inducing a dynamic adjustment of the grounded <span class="hlt">ice</span> <span class="hlt">sheet</span>, drive the evolution of the whole <span class="hlt">ice</span> <span class="hlt">sheet</span>. Our results strongly suggest the need to consider the ocean as an active forcing in paleo <span class="hlt">ice</span> <span class="hlt">sheet</span> models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013SolED...5.2345S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013SolED...5.2345S"><span>Comparing a thermo-mechanical Weichselian <span class="hlt">ice</span> <span class="hlt">sheet</span> reconstruction to GIA driven reconstructions: aspects of earth response and <span class="hlt">ice</span> configuration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schmidt, P.; Lund, B.; Näslund, J.-O.</p> <p>2013-12-01</p> <p>In this study we compare a recent reconstruction of the Weichselian <span class="hlt">ice-sheet</span> as simulated by the University of Main <span class="hlt">ice-sheet</span> model (UMISM) to two reconstructions commonly used in glacial isostatic adjustment (GIA) modeling: <span class="hlt">ICE</span>-5G and ANU (also known as RSES). The UMISM reconstruction is carried out on a regional scale based on thermo-mechanical modelling whereas ANU and <span class="hlt">ICE</span>-5G are global models based on the sea-level equation. The Weichselian <span class="hlt">ice-sheet</span> in the three models are compared directly in terms of <span class="hlt">ice</span> volume, extent and thickness, as well as in terms of predicted glacial isostatic adjustment in Fennoscandia. The three reconstructions display significant differences. UMISM and ANU includes phases of pronounced advance and retreat prior to the last glacial maximum (LGM), whereas the thickness and areal extent of the <span class="hlt">ICE</span>-5G <span class="hlt">ice-sheet</span> is more or less constant up until LGM. The final retreat of the <span class="hlt">ice-sheet</span> initiates at earliest time in <span class="hlt">ICE</span>-5G and latest in UMISM, while <span class="hlt">ice</span> free conditions are reached earliest in UMISM and latest in <span class="hlt">ICE</span>-5G. The post-LGM deglaciation style also differs notably between the <span class="hlt">ice</span> models. While the UMISM simulation includes two temporary halts in the deglaciation, the later during the Younger Dryas, ANU only includes a decreased deglaciation rate during Younger Dryas and <span class="hlt">ICE</span>-5G retreats at a relatively constant pace after an initial slow phase. Moreover, ANU and <span class="hlt">ICE</span>-5G melt relatively uniformly over the entire <span class="hlt">ice-sheet</span> in contrast to UMISM which melts preferentially from the edges. We find that all three reconstructions fit the present day uplift rates over Fennoscandia and the observed relative sea-level curve along the Ångerman river equally well, albeit with different optimal earth model parameters. Given identical earth models, <span class="hlt">ICE</span>-5G predicts the fastest present day uplift rates and ANU the slowest, ANU also prefers the thinnest lithosphere. Moreover, only for ANU can a unique best fit model be determined. For UMISM and <span class="hlt">ICE</span></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> <span class="hlt">Sheet</span> Mass Balance - Evolution of Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span> 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> <span class="hlt">sheet</span> mass 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> <span class="hlt">sheets</span> 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> <span class="hlt">sheet</span> 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> <span class="hlt">Sheet</span> between 2003 and 2009 on a high-resolution grid. Our reconstruction, consistent with GRACE results, shows <span class="hlt">ice</span> <span class="hlt">sheet</span> thinning propagating</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4890806','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4890806"><span>The <span class="hlt">Snow</span> Must Go On: Ground <span class="hlt">Ice</span> Encasement, <span class="hlt">Snow</span> Compaction and Absence of <span class="hlt">Snow</span> Differently Cause Soil Hypoxia, CO2 Accumulation and Tree Seedling Damage in 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>Vuosku, Jaana; Ovaskainen, Anu; Stark, Sari; Rautio, Pasi</p> <p>2016-01-01</p> <p>At high latitudes, the climate has warmed at twice the rate of the global average with most changes observed in autumn, winter and spring. Increasing winter temperatures and wide temperature fluctuations are leading to more frequent rain-on-<span class="hlt">snow</span> events and freeze-thaw cycles causing <span class="hlt">snow</span> compaction and formation of <span class="hlt">ice</span> layers in the snowpack, thus creating <span class="hlt">ice</span> encasement (IE). By decreasing the snowpack insulation capacity and restricting soil-atmosphere gas exchange, modification of the <span class="hlt">snow</span> properties may lead to colder soil but also to hypoxia and accumulation of trace gases in the subnivean environment. To test the effects of these overwintering conditions changes on plant winter survival and growth, we established a <span class="hlt">snow</span> manipulation experiment in a coniferous forest in Northern Finland with Norway spruce and Scots pine seedlings. In addition to ambient conditions and prevention of IE, we applied three <span class="hlt">snow</span> manipulation levels: IE created by artificial rain-on-<span class="hlt">snow</span> events, <span class="hlt">snow</span> compaction and complete <span class="hlt">snow</span> removal. <span class="hlt">Snow</span> removal led to deeper soil frost during winter, but no clear effect of IE or <span class="hlt">snow</span> compaction done in early winter was observed on soil temperature. Hypoxia and accumulation of CO2 were highest in the IE plots but, more importantly, the duration of CO2 concentration above 5% was 17 days in IE plots compared to 0 days in ambient plots. IE was the most damaging winter condition for both species, decreasing the proportion of healthy seedlings by 47% for spruce and 76% for pine compared to ambient conditions. Seedlings in all three treatments tended to grow less than seedlings in ambient conditions but only IE had a significant effect on spruce growth. Our results demonstrate a negative impact of winter climate change on boreal forest regeneration and productivity. Changing <span class="hlt">snow</span> conditions may thus partially mitigate the positive effect of increasing growing season temperatures on boreal forest productivity. PMID:27254100</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27254100','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27254100"><span>The <span class="hlt">Snow</span> Must Go On: Ground <span class="hlt">Ice</span> Encasement, <span class="hlt">Snow</span> Compaction and Absence of <span class="hlt">Snow</span> Differently Cause Soil Hypoxia, CO2 Accumulation and Tree Seedling Damage in Boreal Forest.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Martz, Françoise; Vuosku, Jaana; Ovaskainen, Anu; Stark, Sari; Rautio, Pasi</p> <p>2016-01-01</p> <p>At high latitudes, the climate has warmed at twice the rate of the global average with most changes observed in autumn, winter and spring. Increasing winter temperatures and wide temperature fluctuations are leading to more frequent rain-on-<span class="hlt">snow</span> events and freeze-thaw cycles causing <span class="hlt">snow</span> compaction and formation of <span class="hlt">ice</span> layers in the snowpack, thus creating <span class="hlt">ice</span> encasement (IE). By decreasing the snowpack insulation capacity and restricting soil-atmosphere gas exchange, modification of the <span class="hlt">snow</span> properties may lead to colder soil but also to hypoxia and accumulation of trace gases in the subnivean environment. To test the effects of these overwintering conditions changes on plant winter survival and growth, we established a <span class="hlt">snow</span> manipulation experiment in a coniferous forest in Northern Finland with Norway spruce and Scots pine seedlings. In addition to ambient conditions and prevention of IE, we applied three <span class="hlt">snow</span> manipulation levels: IE created by artificial rain-on-<span class="hlt">snow</span> events, <span class="hlt">snow</span> compaction and complete <span class="hlt">snow</span> removal. <span class="hlt">Snow</span> removal led to deeper soil frost during winter, but no clear effect of IE or <span class="hlt">snow</span> compaction done in early winter was observed on soil temperature. Hypoxia and accumulation of CO2 were highest in the IE plots but, more importantly, the duration of CO2 concentration above 5% was 17 days in IE plots compared to 0 days in ambient plots. IE was the most damaging winter condition for both species, decreasing the proportion of healthy seedlings by 47% for spruce and 76% for pine compared to ambient conditions. Seedlings in all three treatments tended to grow less than seedlings in ambient conditions but only IE had a significant effect on spruce growth. Our results demonstrate a negative impact of winter climate change on boreal forest regeneration and productivity. Changing <span class="hlt">snow</span> conditions may thus partially mitigate the positive effect of increasing growing season temperatures on boreal forest productivity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C43A..05D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C43A..05D"><span>Minimum and Maximum Potential Contributions to Future Sea Level Rise from Polar <span class="hlt">Ice</span> <span class="hlt">Sheets</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Deconto, R. M.; Pollard, D.</p> <p>2017-12-01</p> <p>New climate and <span class="hlt">ice-sheet</span> modeling, calibrated to past changes in sea-level, is painting a stark picture of the future fate of the great polar <span class="hlt">ice</span> <span class="hlt">sheets</span> if greenhouse gas emissions continue unabated. This is especially true for Antarctica, where a substantial fraction of the <span class="hlt">ice</span> <span class="hlt">sheet</span> rests on bedrock more than 500-meters below sea level. Here, we explore the sensitivity of the polar <span class="hlt">ice</span> <span class="hlt">sheets</span> to a warming atmosphere and ocean under a range of future greenhouse gas emissions scenarios. The <span class="hlt">ice</span> <span class="hlt">sheet</span>-climate-ocean model used here considers time-evolving changes in surface mass balance and sub-<span class="hlt">ice</span> oceanic melting, <span class="hlt">ice</span> deformation, grounding line retreat on reverse-sloped bedrock (Marine <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Instability), and newly added processes including hydrofracturing of <span class="hlt">ice</span> shelves in response to surface meltwater and rain, and structural collapse of thick, marine-terminating <span class="hlt">ice</span> margins with tall <span class="hlt">ice</span>-cliff faces (Marine <span class="hlt">Ice</span> Cliff Instability). The simulations improve on previous work by using 1) improved atmospheric forcing from a Regional Climate Model and 2) a much wider range of model physical parameters within the bounds of modern observations of <span class="hlt">ice</span> dynamical processes (particularly calving rates) and paleo constraints on past <span class="hlt">ice-sheet</span> response to warming. Approaches to more precisely define the climatic thresholds capable of triggering rapid and potentially irreversible <span class="hlt">ice-sheet</span> retreat are also discussed, as is the potential for aggressive mitigation strategies like those discussed at the 2015 Paris Climate Conference (COP21) to substantially reduce the risk of extreme sea-level rise. These results, including physics that consider both <span class="hlt">ice</span> deformation (creep) and calving (mechanical failure of marine terminating <span class="hlt">ice</span>) expand on previously estimated limits of maximum rates of future sea level rise based solely on kinematic constraints of glacier flow. At the high end, the new results show the potential for more than 2m of global mean sea level rise by 2100</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.S52A..02A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.S52A..02A"><span>Acoustic Gravity Waves Generated by an Oscillating <span class="hlt">Ice</span> <span class="hlt">Sheet</span> in Arctic Zone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Abdolali, A.; Kadri, U.; Kirby, J. T., Jr.</p> <p>2016-12-01</p> <p>We investigate the formation of acoustic-gravity waves due to oscillations of large <span class="hlt">ice</span> blocks, possibly triggered by atmospheric and ocean currents, <span class="hlt">ice</span> block shrinkage or storms and <span class="hlt">ice</span>-quakes.For the idealized case of a homogeneous weakly compressible water bounded at the surface by <span class="hlt">ice</span> <span class="hlt">sheet</span> and a rigid bed, the description of the infinite family of acoustic modes is characterized by the water depth h and angular frequency of oscillating <span class="hlt">ice</span> <span class="hlt">sheet</span> ω ; The acoustic wave field is governed by the leading mode given by: Nmax=\\floor {(ω h)/(π c)} where c is the sound speed in water and the special brackets represent the floor function (Fig1). Unlike the free-surface setting, the higher acoustic modes might exhibit a larger contribution and therefore all progressive acoustic modes have to be considered.This study focuses on the characteristics of acoustic-gravity waves generated by an oscillating elastic <span class="hlt">ice</span> <span class="hlt">sheet</span> in a weakly compressible fluid coupled with a free surface model [Abdolali et al. 2015] representing shrinking <span class="hlt">ice</span> blocks in realistic sea state, where the randomly oriented <span class="hlt">ice</span> <span class="hlt">sheets</span> cause inter modal transition and multidirectional reflections. A theoretical solution and a 3D numerical model have been developed for the study purposes. The model is first validated against the theoretical solution [Kadri, 2016]. To overcome the computational difficulties of 3D models, we derive a depth-integrated equation valid for spatially varying <span class="hlt">ice</span> <span class="hlt">sheet</span> thickness and water depth. We show that the generated acoustic-gravity waves contribute significantly to deep ocean currents compared to other mechanisms. In addition, these waves travel at the sound speed in water carrying information on <span class="hlt">ice</span> <span class="hlt">sheet</span> motion, providing various implications for ocean monitoring and detection of <span class="hlt">ice</span>-quakes. Fig1:Snapshots of dynamic pressure given by an oscillating <span class="hlt">ice</span> <span class="hlt">sheet</span>; h=4500m, c=1500m/s, semi-length b=10km, ζ =1m, omega=π rad/s. Abdolali, A., Kirby, J. T. and Bellotti, G</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-Sheet</span> mass 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> <span class="hlt">Sheet</span> (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> <span class="hlt">sheet</span> has a stabilizing influence on the <span class="hlt">ice</span> <span class="hlt">sheets</span>, 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-sheet</span> retreat significantly reduces AIS mass 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/2017ERL....12h4010L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ERL....12h4010L"><span>Improved simulation of Antarctic sea <span class="hlt">ice</span> due to the radiative effects of falling <span class="hlt">snow</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, J.-L. F.; Richardson, Mark; Hong, Yulan; Lee, Wei-Liang; Wang, Yi-Hui; Yu, Jia-Yuh; Fetzer, Eric; Stephens, Graeme; Liu, Yinghui</p> <p>2017-08-01</p> <p>Southern Ocean sea-<span class="hlt">ice</span> cover exerts critical control on local albedo and Antarctic precipitation, but simulated Antarctic sea-<span class="hlt">ice</span> concentration commonly disagrees with observations. Here we show that the radiative effects of precipitating <span class="hlt">ice</span> (falling <span class="hlt">snow</span>) contribute substantially to this discrepancy. Many models exclude these radiative effects, so they underestimate both shortwave albedo and downward longwave radiation. Using two simulations with the climate model CESM1, we show that including falling-<span class="hlt">snow</span> radiative effects improves the simulations relative to cloud properties from CloudSat-CALIPSO, radiation from CERES-EBAF and sea-<span class="hlt">ice</span> concentration from passive microwave sensors. From 50-70°S, the simulated sea-<span class="hlt">ice</span>-area bias is reduced by 2.12 × 106 km2 (55%) in winter and by 1.17 × 106 km2 (39%) in summer, mainly because increased wintertime longwave heating restricts sea-<span class="hlt">ice</span> growth and so reduces summer albedo. Improved Antarctic sea-<span class="hlt">ice</span> simulations will increase confidence in projected Antarctic sea level contributions and changes in global warming driven by long-term changes in Southern Ocean feedbacks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMED51A3424L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMED51A3424L"><span>Outreach/education interface for Cryosphere models using the Virtual <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Laboratory</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.; Halkides, D. J.; Romero, V.; Cheng, D. L.; Perez, G.</p> <p>2014-12-01</p> <p>In the past decade, great strides have been made in the development of models capable of projecting the future evolution of glaciers and the polar <span class="hlt">ice</span> <span class="hlt">sheets</span> in a changing climate. These models are now capable of replicating some of the trends apparent in satellite observations. However, because this field is just now maturing, very few efforts have been dedicated to adapting these capabilities to education. Technologies that have been used in outreach efforts in Atmospheric and Oceanic sciences still have not been extended to Cryospheric Science. We present a cutting-edge, technologically driven virtual laboratory, geared towards outreach and k-12 education, dedicated to the polar <span class="hlt">ice</span> <span class="hlt">sheets</span> on Antarctica and Greenland, and their role as major contributors to sea level rise in coming decades. VISL (Virtual <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Laboratory) relies on state-of-the art Web GL rendering of polar <span class="hlt">ice</span> <span class="hlt">sheets</span>, Android/iPhone and web portability using Javascript, as well as C++ simulations (back-end) based on the <span class="hlt">Ice</span> <span class="hlt">Sheet</span> System Model, the NASA model for simulating the evolution of polar <span class="hlt">ice</span> <span class="hlt">sheets</span>. Using VISL, educators and students can have an immersive experience into the world of polar <span class="hlt">ice</span> <span class="hlt">sheets</span>, while at the same exercising the capabilities of a state-of-the-art climate model, all of it embedded into an education experience that follows the new STEM standards for education.This work was performed at the California Institute of Technology's Jet Propulsion Laboratory under a contract with the National Aeronautics and Space Administration's Cryosphere Science Program.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_24 --> <div id="page_25" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="481"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1366350','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1366350"><span>West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> cloud cover and surface radiation budget from NASA A-Train satellites</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Scott, Ryan C.; Lubin, Dan; Vogelmann, Andrew M.</p> <p></p> <p>Clouds are an essential parameter of the surface energy budget influencing the West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (WAIS) response to atmospheric warming and net contribution to global sea-level rise. A four-year record of NASA A-Train cloud observations is combined with surface radiation measurements to quantify the WAIS radiation budget and constrain the three-dimensional occurrence frequency, thermodynamic phase partitioning, and surface radiative effect of clouds over West Antarctica (WA). The skill of satellite-modeled radiative fluxes is confirmed through evaluation against measurements at four Antarctic sites (WAIS Divide <span class="hlt">Ice</span> Camp, Neumayer, Syowa, and Concordia Stations). And due to perennial high-albedo <span class="hlt">snow</span> and icemore » cover, cloud infrared emission dominates over cloud solar reflection/absorption leading to a positive net all-wave cloud radiative effect (CRE) at the surface, with all monthly means and 99.15% of instantaneous CRE values exceeding zero. The annual-mean CRE at theWAIS surface is 34 W m -2, representing a significant cloud-induced warming of the <span class="hlt">ice</span> <span class="hlt">sheet</span>. Low-level liquid-containing clouds, including thin liquid water clouds implicated in radiative contributions to surface melting, are widespread and most frequent in WA during the austral summer. Clouds warm the WAIS by 26 W m -2, in summer, on average, despite maximum offsetting shortwave CRE. Glaciated cloud systems are strongly linked to orographic forcing, with maximum incidence on the WAIS continuing downstream along the Transantarctic Mountains.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1366350-west-antarctic-ice-sheet-cloud-cover-surface-radiation-budget-from-nasa-train-satellites','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1366350-west-antarctic-ice-sheet-cloud-cover-surface-radiation-budget-from-nasa-train-satellites"><span>West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> cloud cover and surface radiation budget from NASA A-Train satellites</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Scott, Ryan C.; Lubin, Dan; Vogelmann, Andrew M.; ...</p> <p>2017-04-26</p> <p>Clouds are an essential parameter of the surface energy budget influencing the West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (WAIS) response to atmospheric warming and net contribution to global sea-level rise. A four-year record of NASA A-Train cloud observations is combined with surface radiation measurements to quantify the WAIS radiation budget and constrain the three-dimensional occurrence frequency, thermodynamic phase partitioning, and surface radiative effect of clouds over West Antarctica (WA). The skill of satellite-modeled radiative fluxes is confirmed through evaluation against measurements at four Antarctic sites (WAIS Divide <span class="hlt">Ice</span> Camp, Neumayer, Syowa, and Concordia Stations). And due to perennial high-albedo <span class="hlt">snow</span> and icemore » cover, cloud infrared emission dominates over cloud solar reflection/absorption leading to a positive net all-wave cloud radiative effect (CRE) at the surface, with all monthly means and 99.15% of instantaneous CRE values exceeding zero. The annual-mean CRE at theWAIS surface is 34 W m -2, representing a significant cloud-induced warming of the <span class="hlt">ice</span> <span class="hlt">sheet</span>. Low-level liquid-containing clouds, including thin liquid water clouds implicated in radiative contributions to surface melting, are widespread and most frequent in WA during the austral summer. Clouds warm the WAIS by 26 W m -2, in summer, on average, despite maximum offsetting shortwave CRE. Glaciated cloud systems are strongly linked to orographic forcing, with maximum incidence on the WAIS continuing downstream along the Transantarctic Mountains.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMPP11E..02G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMPP11E..02G"><span>Simulating a Dynamic Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> in the Early to Middle Miocene</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gasson, E.; DeConto, R.; Pollard, D.; Levy, R. H.</p> <p>2015-12-01</p> <p>There are a variety of sources of geological data that suggest major variations in the volume and extent of the Antarctic <span class="hlt">ice</span> <span class="hlt">sheet</span> during the early to middle Miocene. Simulating such variability using coupled climate-<span class="hlt">ice</span> <span class="hlt">sheet</span> models is problematic due to a strong hysteresis effect caused by height-mass balance feedback and albedo feedback. This results in limited retreat of the <span class="hlt">ice</span> <span class="hlt">sheet</span> 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> <span class="hlt">sheet</span>-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> <span class="hlt">sheet</span> in the Miocene. This variability is equivalent to a seawater oxygen isotope signal of ~0.5 ‰, or a sea level equivalent change of ~35 m, for a range of atmospheric CO2 between 280 - 500 ppm.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29899456','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29899456"><span>Extensive retreat and re-advance of the West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> during the Holocene.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kingslake, J; Scherer, R P; Albrecht, T; Coenen, J; Powell, R D; Reese, R; Stansell, N D; Tulaczyk, S; Wearing, M G; Whitehouse, P L</p> <p>2018-06-01</p> <p>To predict the future contributions of the Antarctic <span class="hlt">ice</span> <span class="hlt">sheets</span> to sea-level rise, numerical models use reconstructions of past <span class="hlt">ice-sheet</span> retreat after the Last Glacial Maximum to tune model parameters 1 . Reconstructions of the West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> have assumed that it retreated progressively throughout the Holocene epoch (the past 11,500 years or so) 2-4 . Here we show, however, that over this period the grounding line of the West Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (which marks the point at which it is no longer in contact with the ground and becomes a floating <span class="hlt">ice</span> shelf) retreated several hundred kilometres inland of today's grounding line, before isostatic rebound caused it to re-advance to its present position. Our evidence includes, first, radiocarbon dating of sediment cores recovered from beneath the <span class="hlt">ice</span> streams of the Ross Sea sector, indicating widespread Holocene marine exposure; and second, <span class="hlt">ice</span>-penetrating radar observations of englacial structure in the Weddell Sea sector, indicating <span class="hlt">ice</span>-shelf grounding. We explore the implications of these findings with an <span class="hlt">ice-sheet</span> model. Modelled re-advance of the grounding line in the Holocene requires <span class="hlt">ice</span>-shelf grounding caused by isostatic rebound. Our findings overturn the assumption of progressive retreat of the grounding line during the Holocene in West Antarctica, and corroborate previous suggestions of <span class="hlt">ice-sheet</span> re-advance 5 . Rebound-driven stabilizing processes were apparently able to halt and reverse climate-initiated <span class="hlt">ice</span> loss. Whether these processes can reverse present-day <span class="hlt">ice</span> loss 6 on millennial timescales will depend on bedrock topography and mantle viscosity-parameters that are difficult to measure and to incorporate into <span class="hlt">ice-sheet</span> models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C22C..03R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C22C..03R"><span>Isostasy as a Driver of Paleo Retreat of the Greenland <span class="hlt">Ice</span> <span class="hlt">Sheet</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Robinson, A.; Tabone, I.; Alvarez-Solas, J.; Montoya, M.</p> <p>2016-12-01</p> <p>During glacial times, the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> (GrIS) extended onto the continental shelf, and thus was much more directly affected by changing ocean temperatures through basal melt of the marine <span class="hlt">ice</span> margins than it is today. The larger glacial <span class="hlt">ice</span> <span class="hlt">sheet</span> also induced lithospheric depression of several hundred meters in regions that are near sea level today. As the <span class="hlt">ice</span> <span class="hlt">sheet</span> retreated inland under interglacial climatic forcing, the regions significantly affected by local isostatic changes in elevation were exposed to much higher basal melt rates than they would have been given the present-day topography. Here we explore this effect using a hybrid <span class="hlt">ice</span> <span class="hlt">sheet</span> model that represents both grounded and floating <span class="hlt">ice</span>, as well as local isostatic effects, and is driven by both atmospheric and oceanic temperature anomalies. We find that when transient oceanic forcing is included in the model, isostasy plays an important role in allowing oceanic melting to drive GrIS retreat in some regions. During the last interglacial, for example, this effect can account for a significant additional sea-level contribution, as well as an increase in the rate of sea-level rise. Our results highlight the importance of accounting for <span class="hlt">ice</span>-ocean-lithosphere interactions in the past, in order to be able to properly reconstruct the evolution of the <span class="hlt">ice</span> <span class="hlt">sheet</span>, and for estimating its sensitivity to potential changes in climate in the future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1711590F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1711590F"><span>Chemical Atmosphere-<span class="hlt">Snow</span>-Sea <span class="hlt">Ice</span> Interactions: defining future research in the field, lab and modeling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Frey, Markus</p> <p>2015-04-01</p> <p>The air-<span class="hlt">snow</span>-sea <span class="hlt">ice</span> system plays an important role in the global cycling of nitrogen, halogens, trace metals or carbon, including greenhouse gases (e.g. CO2 air-sea flux), and therefore influences also climate. Its impact on atmospheric composition is illustrated for example by dramatic ozone and mercury depletion events which occur within or close to the sea <span class="hlt">ice</span> zone (SIZ) mostly during polar spring and are catalysed by halogens released from SIZ <span class="hlt">ice</span>, <span class="hlt">snow</span> or aerosol. Recent field campaigns in the high Arctic (e.g. BROMEX, OASIS) and Antarctic (Weddell sea cruises) highlight the importance of <span class="hlt">snow</span> on sea <span class="hlt">ice</span> as a chemical reservoir and reactor, even during polar night. However, many processes, participating chemical species and their interactions are still poorly understood and/or lack any representation in current models. Furthermore, recent lab studies provide a lot of detail on the chemical environment and processes but need to be integrated much better to improve our understanding of a rapidly changing natural environment. During a 3-day workshop held in Cambridge/UK in October 2013 more than 60 scientists from 15 countries who work on the physics, chemistry or biology of the atmosphere-<span class="hlt">snow</span>-sea <span class="hlt">ice</span> system discussed research status and challenges, which need to be addressed in the near future. In this presentation I will give a summary of the main research questions identified during this workshop as well as ways forward to answer them through a community-based interdisciplinary approach.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23925242','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23925242"><span>Insolation-driven 100,000-year glacial cycles and hysteresis of <span class="hlt">ice-sheet</span> volume.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Abe-Ouchi, Ayako; Saito, Fuyuki; Kawamura, Kenji; Raymo, Maureen E; Okuno, Jun'ichi; Takahashi, Kunio; Blatter, Heinz</p> <p>2013-08-08</p> <p>The growth and reduction of Northern Hemisphere <span class="hlt">ice</span> <span class="hlt">sheets</span> over the past million years is dominated by an approximately 100,000-year periodicity and a sawtooth pattern (gradual growth and fast termination). Milankovitch theory proposes that summer insolation at high northern latitudes drives the glacial cycles, and statistical tests have demonstrated that the glacial cycles are indeed linked to eccentricity, obliquity and precession cycles. Yet insolation alone cannot explain the strong 100,000-year cycle, suggesting that internal climatic feedbacks may also be at work. Earlier conceptual models, for example, showed that glacial terminations are associated with the build-up of Northern Hemisphere 'excess <span class="hlt">ice</span>', but the physical mechanisms underpinning the 100,000-year cycle remain unclear. Here we show, using comprehensive climate and <span class="hlt">ice-sheet</span> models, that insolation and internal feedbacks between the climate, the <span class="hlt">ice</span> <span class="hlt">sheets</span> and the lithosphere-asthenosphere system explain the 100,000-year periodicity. The responses of equilibrium states of <span class="hlt">ice</span> <span class="hlt">sheets</span> 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> <span class="hlt">sheet</span> is such that after inception of the <span class="hlt">ice</span> <span class="hlt">sheet</span>, its mass balance remains mostly positive through several precession cycles, whose amplitudes decrease towards an eccentricity minimum. The larger the <span class="hlt">ice</span> <span class="hlt">sheet</span> grows and extends towards lower latitudes, the smaller is the insolation required to make the mass balance negative. Therefore, once a large <span class="hlt">ice</span> <span class="hlt">sheet</span> is established, a moderate increase in insolation is sufficient to trigger a negative mass balance, leading to an almost complete retreat of the <span class="hlt">ice</span> <span class="hlt">sheet</span> within several thousand years. This fast retreat is governed mainly by rapid ablation due to the lowered surface elevation resulting from delayed isostatic rebound, which is the lithosphere</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> <span class="hlt">Sheet</span></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> <span class="hlt">Sheet</span> during the last glacial/interglacial cycle is used to identify the main controls on <span class="hlt">ice</span> <span class="hlt">sheet</span> behavior. Using as input glaciological assumptions derived by W. F. Budd and I. N. Smith (1982, Annals of Glaciology3, 42-49), bedrock topography, isostatic compensation, and mass balance relationships, the model is driven by sea-level change over the last 40,000 yr in association with assumed changes in the rate of melting beneath <span class="hlt">ice</span> shelves. An <span class="hlt">ice</span> <span class="hlt">sheet</span> 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> <span class="hlt">sheet</span> behavior is most sensitive to sea-level change, basal marine melting, and accumulation and is less sensitive to isostasy, spatial variation in accumulation, calving rates, and <span class="hlt">ice</span> flow parameterization. Tests of the model against field evidence show good agreement in places, as well as discrepancies which require further work.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016TCry...10..639S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016TCry...10..639S"><span>Numerical simulations of the Cordilleran <span class="hlt">ice</span> <span class="hlt">sheet</span> through the last glacial cycle</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Seguinot, Julien; Rogozhina, Irina; Stroeven, Arjen P.; Margold, Martin; Kleman, Johan</p> <p>2016-03-01</p> <p>After more than a century of geological research, the Cordilleran <span class="hlt">ice</span> <span class="hlt">sheet</span> of North America remains among the least understood in terms of its former extent, volume, and dynamics. Because of the mountainous topography on which the <span class="hlt">ice</span> <span class="hlt">sheet</span> formed, geological studies have often had only local or regional relevance and shown such a complexity that <span class="hlt">ice-sheet</span>-wide spatial reconstructions of advance and retreat patterns are lacking. Here we use a numerical <span class="hlt">ice</span> <span class="hlt">sheet</span> model calibrated against field-based evidence to attempt a quantitative reconstruction of the Cordilleran <span class="hlt">ice</span> <span class="hlt">sheet</span> history through the last glacial cycle. A series of simulations is driven by time-dependent temperature offsets from six proxy records located around the globe. Although this approach reveals large variations in model response to evolving climate forcing, all simulations produce two major glaciations during marine oxygen isotope stages 4 (62.2-56.9 ka) and 2 (23.2-16.9 ka). The timing of glaciation is better reproduced using temperature reconstructions from Greenland and Antarctic <span class="hlt">ice</span> cores than from regional oceanic sediment cores. During most of the last glacial cycle, the modelled <span class="hlt">ice</span> cover is discontinuous and restricted to high mountain areas. However, widespread precipitation over the Skeena Mountains favours the persistence of a central <span class="hlt">ice</span> dome throughout the glacial cycle. It acts as a nucleation centre before the Last Glacial Maximum and hosts the last remains of Cordilleran <span class="hlt">ice</span> until the middle Holocene (6.7 ka).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19776741','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19776741"><span>Extensive dynamic thinning on the margins of the Greenland and Antarctic <span class="hlt">ice</span> <span class="hlt">sheets</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pritchard, Hamish D; Arthern, Robert J; Vaughan, David G; Edwards, Laura A</p> <p>2009-10-15</p> <p>Many glaciers along the margins of the Greenland and Antarctic <span class="hlt">ice</span> <span class="hlt">sheets</span> are accelerating and, for this reason, contribute increasingly to global sea-level rise. Globally, <span class="hlt">ice</span> losses contribute approximately 1.8 mm yr(-1) (ref. 8), but this could increase if the retreat of <span class="hlt">ice</span> shelves and tidewater glaciers further enhances the loss of grounded <span class="hlt">ice</span> or initiates the large-scale collapse of vulnerable parts of the <span class="hlt">ice</span> <span class="hlt">sheets</span>. <span class="hlt">Ice</span> loss as a result of accelerated flow, known as dynamic thinning, is so poorly understood that its potential contribution to sea level over the twenty-first century remains unpredictable. Thinning on the <span class="hlt">ice-sheet</span> scale has been monitored by using repeat satellite altimetry observations to track small changes in surface elevation, but previous sensors could not resolve most fast-flowing coastal glaciers. Here we report the use of high-resolution ICESat (<span class="hlt">Ice</span>, Cloud and land Elevation Satellite) laser altimetry to map change along the entire grounded margins of the Greenland and Antarctic <span class="hlt">ice</span> <span class="hlt">sheets</span>. To isolate the dynamic signal, we compare rates of elevation change from both fast-flowing and slow-flowing <span class="hlt">ice</span> with those expected from surface mass-balance fluctuations. We find that dynamic thinning of glaciers now reaches all latitudes in Greenland, has intensified on key Antarctic grounding lines, has endured for decades after <span class="hlt">ice</span>-shelf collapse, penetrates far into the interior of each <span class="hlt">ice</span> <span class="hlt">sheet</span> and is spreading as <span class="hlt">ice</span> shelves thin by ocean-driven melt. In Greenland, glaciers flowing faster than 100 m yr(-1) thinned at an average rate of 0.84 m yr(-1), and in the Amundsen Sea embayment of Antarctica, thinning exceeded 9.0 m yr(-1) for some glaciers. Our results show that the most profound changes in the <span class="hlt">ice</span> <span class="hlt">sheets</span> currently result from glacier dynamics at ocean margins.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20150021522&hterms=methodological&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dmethodological','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20150021522&hterms=methodological&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dmethodological"><span>On the Reconstruction of Palaeo-<span class="hlt">Ice</span> <span class="hlt">Sheets</span>: Recent Advances and Future Challenges</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stokes, Chris R.; Tarasov, Lev; Blomdin, Robin; Cronin, Thomas M.; Fisher, Timothy G.; Gyllencreutz, Richard; Hattestrand, Clas; Heyman, Jacob; Hindmarsh, Richard C. A.; Hughes, Anna L. C.; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20150021522'); toggleEditAbsImage('author_20150021522_show'); toggleEditAbsImage('author_20150021522_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20150021522_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20150021522_hide"></p> <p>2015-01-01</p> <p>Reconstructing the growth and decay of palaeo-<span class="hlt">ice</span> <span class="hlt">sheets</span> is critical to understanding mechanisms of global climate change and associated sea-level fluctuations in the past, present and future. The significance of palaeo-<span class="hlt">ice</span> <span class="hlt">sheets</span> is further underlined by the broad range of disciplines concerned with reconstructing their behaviour, many of which have undergone a rapid expansion since the 1980s. In particular, there has been a major increase in the size and qualitative diversity of empirical data used to reconstruct and date <span class="hlt">ice</span> <span class="hlt">sheets</span>, and major improvements in our ability to simulate their dynamics in numerical <span class="hlt">ice</span> <span class="hlt">sheet</span> models. These developments have made it increasingly necessary to forge interdisciplinary links between sub-disciplines and to link numerical modelling with observations and dating of proxy records. The aim of this paper is to evaluate recent developments in the methods used to reconstruct <span class="hlt">ice</span> <span class="hlt">sheets</span> and outline some key challenges that remain, with an emphasis on how future work might integrate terrestrial and marine evidence together with numerical modelling. Our focus is on pan-<span class="hlt">ice</span> <span class="hlt">sheet</span> reconstructions of the last deglaciation, but regional case studies are used to illustrate methodological achievements, challenges and opportunities. Whilst various disciplines have made important progress in our understanding of <span class="hlt">ice-sheet</span> dynamics, it is clear that data-model integration remains under-used, and that uncertainties remain poorly quantified in both empirically-based and numerical <span class="hlt">ice-sheet</span> reconstructions. The representation of past climate will continue to be the largest source of uncertainty for numerical modelling. As such, palaeo-observations are critical to constrain and validate modelling. State-of-the-art numerical models will continue to improve both in model resolution and in the breadth of inclusion of relevant processes, thereby enabling more accurate and more direct comparison with the increasing range of palaeo-observations. Thus</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70180974','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70180974"><span>On the reconstruction of palaeo-<span class="hlt">ice</span> <span class="hlt">sheets</span>: Recent advances and future challenges</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Stokes, Chris R.; Tarasov, Lev; Blomdin, Robin; Cronin, Thomas M.; Fisher, Timothy G.; Gyllencreutz, Richard; Hattestrand, Clas; Heyman, Jakob; Hindmarsh, Richard C. A.; Hughes, Anna L. C.; Jakobsson, Martin; Kirchner, Nina; Livingstone, Stephen J.; Margold, Martin; Murton, Julian B.; Noormets, Riko; Peltier, W. Richard; Peteet, Dorothy M.; Piper, David J. W.; Preusser, Frank; Renssen, Hans; Roberts, David H.; Roche, Didier M.; Saint-Ange, Francky; Stroeven, Arjen P.; Teller, James T.</p> <p>2015-01-01</p> <p>Reconstructing the growth and decay of palaeo-<span class="hlt">ice</span> <span class="hlt">sheets</span> is critical to understanding mechanisms of global climate change and associated sea-level fluctuations in the past, present and future. The significance of palaeo-<span class="hlt">ice</span> <span class="hlt">sheets</span> is further underlined by the broad range of disciplines concerned with reconstructing their behaviour, many of which have undergone a rapid expansion since the 1980s. In particular, there has been a major increase in the size and qualitative diversity of empirical data used to reconstruct and date <span class="hlt">ice</span> <span class="hlt">sheets</span>, and major improvements in our ability to simulate their dynamics in numerical <span class="hlt">ice</span> <span class="hlt">sheet</span> models. These developments have made it increasingly necessary to forge interdisciplinary links between sub-disciplines and to link numerical modelling with observations and dating of proxy records. The aim of this paper is to evaluate recent developments in the methods used to reconstruct <span class="hlt">ice</span> <span class="hlt">sheets</span> and outline some key challenges that remain, with an emphasis on how future work might integrate terrestrial and marine evidence together with numerical modelling. Our focus is on pan-<span class="hlt">ice</span> <span class="hlt">sheet</span> reconstructions of the last deglaciation, but regional case studies are used to illustrate methodological achievements, challenges and opportunities. Whilst various disciplines have made important progress in our understanding of <span class="hlt">ice-sheet</span> dynamics, it is clear that data-model integration remains under-used, and that uncertainties remain poorly quantified in both empirically-based and numerical <span class="hlt">ice-sheet</span> reconstructions. The representation of past climate will continue to be the largest source of uncertainty for numerical modelling. As such, palaeo-observations are critical to constrain and validate modelling. State-of-the-art numerical models will continue to improve both in model resolution and in the breadth of inclusion of relevant processes, thereby enabling more accurate and more direct comparison with the increasing range of palaeo-observations. Thus</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C21B0673W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C21B0673W"><span>Damage Mechanics in the Community <span class="hlt">Ice</span> <span class="hlt">Sheet</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>Whitcomb, R.; Cathles, L. M. M., IV; Bassis, J. N.; Lipscomb, W. H.; Price, S. F.</p> <p>2016-12-01</p> <p>Half of the mass that floating <span class="hlt">ice</span> shelves lose to the ocean comes from iceberg calving, which is a difficult process to simulate accurately. This is especially true in the large-scale <span class="hlt">ice</span> dynamics models that couple changes in the cryosphere to climate projections. Damage mechanics provide a powerful technique with the potential to overcome this obstacle by describing how fractures in <span class="hlt">ice</span> evolve over time. Here, we demonstrate the application of a damage model to <span class="hlt">ice</span> shelves that predicts realistic geometries. We incorporated this solver into the Community <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model, a three dimensional <span class="hlt">ice</span> <span class="hlt">sheet</span> model developed at Los Alamos National Laboratory. The damage mechanics formulation that we use comes from a first principles-based evolution law for the depth of basal and surface crevasses and depends on the large scale strain rate, stress state, and basal melt. We show that under idealized conditions it produces <span class="hlt">ice</span> tongue lengths that match well with observations for a selection of natural <span class="hlt">ice</span> tongues, including Erebus, Drygalski, and Pine Island in Antarctica, as well as Petermann in Greenland. We also apply the model to more generalized ideal <span class="hlt">ice</span> shelf geometries and show that it produces realistic calving front positions. Although our results are preliminary, the damage mechanics model that we developed provides a promising first principles method for predicting <span class="hlt">ice</span> shelf extent and how the calving margins of <span class="hlt">ice</span> shelves respond to climate change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5504289','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5504289"><span>MIS-11 duration key to disappearance of the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Robinson, Alexander; Alvarez-Solas, Jorge; Calov, Reinhard; Ganopolski, Andrey; Montoya, Marisa</p> <p>2017-01-01</p> <p>Palaeo data suggest that Greenland must have been largely <span class="hlt">ice</span> free during Marine Isotope Stage 11 (MIS-11). However, regional summer insolation anomalies were modest during this time compared to MIS-5e, when the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> likely lost less volume. Thus it remains unclear how such conditions led to an almost complete disappearance of the <span class="hlt">ice</span> <span class="hlt">sheet</span>. Here we use transient climate–<span class="hlt">ice</span> <span class="hlt">sheet</span> simulations to simultaneously constrain estimates of regional temperature anomalies and Greenland’s contribution to the MIS-11 sea-level highstand. We find that Greenland contributed 6.1 m (3.9–7.0 m, 95% credible interval) to sea level, ∼7 kyr after the peak in regional summer temperature anomalies of 2.8 °C (2.1–3.4 °C). The moderate warming produced a mean rate of mass loss in sea-level equivalent of only around 0.4 m per kyr, which means the long duration of MIS-11 interglacial conditions around Greenland was a necessary condition for the <span class="hlt">ice</span> <span class="hlt">sheet</span> to disappear almost completely. PMID:28681860</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017NatCo...816008R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017NatCo...816008R"><span>MIS-11 duration key to disappearance of the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Robinson, Alexander; Alvarez-Solas, Jorge; Calov, Reinhard; Ganopolski, Andrey; Montoya, Marisa</p> <p>2017-07-01</p> <p>Palaeo data suggest that Greenland must have been largely <span class="hlt">ice</span> free during Marine Isotope Stage 11 (MIS-11). However, regional summer insolation anomalies were modest during this time compared to MIS-5e, when the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> likely lost less volume. Thus it remains unclear how such conditions led to an almost complete disappearance of the <span class="hlt">ice</span> <span class="hlt">sheet</span>. Here we use transient climate-<span class="hlt">ice</span> <span class="hlt">sheet</span> simulations to simultaneously constrain estimates of regional temperature anomalies and Greenland's contribution to the MIS-11 sea-level highstand. We find that Greenland contributed 6.1 m (3.9-7.0 m, 95% credible interval) to sea level, ~7 kyr after the peak in regional summer temperature anomalies of 2.8 °C (2.1-3.4 °C). The moderate warming produced a mean rate of mass loss in sea-level equivalent of only around 0.4 m per kyr, which means the long duration of MIS-11 interglacial conditions around Greenland was a necessary condition for the <span class="hlt">ice</span> <span class="hlt">sheet</span> to disappear almost completely.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28681860','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28681860"><span>MIS-11 duration key to disappearance of the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Robinson, Alexander; Alvarez-Solas, Jorge; Calov, Reinhard; Ganopolski, Andrey; Montoya, Marisa</p> <p>2017-07-06</p> <p>Palaeo data suggest that Greenland must have been largely <span class="hlt">ice</span> free during Marine Isotope Stage 11 (MIS-11). However, regional summer insolation anomalies were modest during this time compared to MIS-5e, when the Greenland <span class="hlt">ice</span> <span class="hlt">sheet</span> likely lost less volume. Thus it remains unclear how such conditions led to an almost complete disappearance of the <span class="hlt">ice</span> <span class="hlt">sheet</span>. Here we use transient climate-<span class="hlt">ice</span> <span class="hlt">sheet</span> simulations to simultaneously constrain estimates of regional temperature anomalies and Greenland's contribution to the MIS-11 sea-level highstand. We find that Greenland contributed 6.1 m (3.9-7.0 m, 95% credible interval) to sea level, ∼7 kyr after the peak in regional summer temperature anomalies of 2.8 °C (2.1-3.4 °C). The moderate warming produced a mean rate of mass loss in sea-level equivalent of only around 0.4 m per kyr, which means the long duration of MIS-11 interglacial conditions around Greenland was a necessary condition for the <span class="hlt">ice</span> <span class="hlt">sheet</span> to disappear almost completely.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27547082','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27547082"><span>Modelling water flow under glaciers and <span class="hlt">ice</span> <span class="hlt">sheets</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Flowers, Gwenn E</p> <p>2015-04-08</p> <p>Recent observations of dynamic water systems beneath the Greenland and Antarctic <span class="hlt">ice</span> <span class="hlt">sheets</span> have sparked renewed interest in modelling subglacial drainage. The foundations of today's models were laid decades ago, inspired by measurements from mountain glaciers, discovery of the modern <span class="hlt">ice</span> streams and the study of landscapes evacuated by former <span class="hlt">ice</span> <span class="hlt">sheets</span>. Models have progressed from strict adherence to the principles of groundwater flow, to the incorporation of flow 'elements' specific to the subglacial environment, to sophisticated two-dimensional representations of interacting distributed and channelized drainage. Although presently in a state of rapid development, subglacial drainage models, when coupled to models of <span class="hlt">ice</span> flow, are now able to reproduce many of the canonical phenomena that characterize this coupled system. Model calibration remains generally out of reach, whereas widespread application of these models to large problems and real geometries awaits the next level of development.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4991255','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4991255"><span>Modelling water flow under glaciers and <span class="hlt">ice</span> <span class="hlt">sheets</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Flowers, Gwenn E.</p> <p>2015-01-01</p> <p>Recent observations of dynamic water systems beneath the Greenland and Antarctic <span class="hlt">ice</span> <span class="hlt">sheets</span> have sparked renewed interest in modelling subglacial drainage. The foundations of today's models were laid decades ago, inspired by measurements from mountain glaciers, discovery of the modern <span class="hlt">ice</span> streams and the study of landscapes evacuated by former <span class="hlt">ice</span> <span class="hlt">sheets</span>. Models have progressed from strict adherence to the principles of groundwater flow, to the incorporation of flow ‘elements’ specific to the subglacial environment, to sophisticated two-dimensional representations of interacting distributed and channelized drainage. Although presently in a state of rapid development, subglacial drainage models, when coupled to models of <span class="hlt">ice</span> flow, are now able to reproduce many of the canonical phenomena that characterize this coupled system. Model calibration remains generally out of reach, whereas widespread application of these models to large problems and real geometries awaits the next level of development. PMID:27547082</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011TCry....5..715W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011TCry....5..715W"><span>The Potsdam Parallel <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model (PISM-PIK) - Part 1: Model description</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Winkelmann, R.; Martin, M. A.; Haseloff, M.; Albrecht, T.; Bueler, E.; Khroulev, C.; Levermann, A.</p> <p>2011-09-01</p> <p>We present the Potsdam Parallel <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model (PISM-PIK), developed at the Potsdam Institute for Climate Impact Research to be used for simulations of large-scale <span class="hlt">ice</span> <span class="hlt">sheet</span>-shelf systems. It is derived from the Parallel <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model (Bueler and Brown, 2009). Velocities are calculated by superposition of two shallow stress balance approximations within the entire <span class="hlt">ice</span> covered region: the shallow <span class="hlt">ice</span> approximation (SIA) is dominant in grounded regions and accounts for shear deformation parallel to the geoid. The plug-flow type shallow shelf approximation (SSA) dominates the velocity field in <span class="hlt">ice</span> shelf regions and serves as a basal sliding velocity in grounded regions. <span class="hlt">Ice</span> streams can be identified diagnostically as regions with a significant contribution of membrane stresses to the local momentum balance. All lateral boundaries in PISM-PIK are free to evolve, including the grounding line and <span class="hlt">ice</span> fronts. <span class="hlt">Ice</span> shelf margins in particular are modeled using Neumann boundary conditions for the SSA equations, reflecting a hydrostatic stress imbalance along the vertical calving face. The <span class="hlt">ice</span> front position is modeled using a subgrid-scale representation of calving front motion (Albrecht et al., 2011) and a physically-motivated calving law based on horizontal spreading rates. The model is tested in experiments from the Marine <span class="hlt">Ice</span> <span class="hlt">Sheet</span> Model Intercomparison Project (MISMIP). A dynamic equilibrium simulation of Antarctica under present-day conditions is presented in Martin et al. (2011).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.6221B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.6221B"><span>The Last Interglacial History of the Antarctic <span class="hlt">Ice</span> <span class="hlt">sheet</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; Siddall, Mark; Milne, Glenn A.; Masson-Delmotte, Valerie; Wolff, Eric; Hindmarsh, Richard C. A.</p> <p>2014-05-01</p> <p>In this paper we present a summary of the work which was conducted as part of the 'PAST4FUTURE -WP4.1: Sea Level and <span class="hlt">Ice</span> <span class="hlt">sheets</span>' project. The overall aim of this study was to understand the response of the Antarctic <span class="hlt">Ice</span> <span class="hlt">sheet</span> (AIS) to climate forcing during the Last interglacial (LIG) and its contribution to the observed higher than present sea level during this period. The study involved the application and development of a novel technique which combined East Antarctic stable isotope <span class="hlt">ice</span> core data with the output from a Glacial Isostatic Adjustment (GIA) model [Bradley et al., 2012]. We investigated if the stable isotope <span class="hlt">ice</span> core data are sensitive to detecting isostatically driven changes in the surface elevation driven by changes in the <span class="hlt">ice</span>-loading history of the AIS and if so, could we address some key questions relating to the LIG history of the AIS. Although it is believed that the West Antarctic <span class="hlt">Ice</span> <span class="hlt">sheet</span> (WAIS) reduced in size during the LIG compared to the Holocene, major uncertainties and unknowns remain unresolved: Did the WAIS collapse? What would the contribution of such a collapse be the higher than present LIG eustatic sea level (ESL)? We will show that a simulated collapse of the WAIS does not generate a significant elevation driven signal at the EAIS LIG <span class="hlt">ice</span> core sites, and as such, these <span class="hlt">ice</span> core records cannot be used to assess WAIS stability over this period. However, we will present 'treasure maps' [Bradley et al., 2012] to identify regions of the AIS where results from geological studies and/or new paleoclimate data may be sensitive to detecting a WAIS collapse. These maps can act as a useful tool for the wider science community/field scientists as a guide to highlight sites suitable to constrain the evolution of the WAIS during the LIG. Studies have proposed that the surface temperature across the East Antarctic <span class="hlt">Ice</span> <span class="hlt">Sheet</span> (EAIS) was significantly warmer, 2-5°C during the LIG compared to present [Lang and Wolff, 2011]. These higher</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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