Sample records for ice mass content

  1. Retrieval of ice crystals' mass from ice water content and particle distribution measurements: a numerical optimization approach

    NASA Astrophysics Data System (ADS)

    Coutris, Pierre; Leroy, Delphine; Fontaine, Emmanuel; Schwarzenboeck, Alfons; Strapp, J. Walter

    2016-04-01

    A new method to retrieve cloud water content from in-situ measured 2D particle images from optical array probes (OAP) is presented. With the overall objective to build a statistical model of crystals' mass as a function of their size, environmental temperature and crystal microphysical history, this study presents the methodology to retrieve the mass of crystals sorted by size from 2D images using a numerical optimization approach. The methodology is validated using two datasets of in-situ measurements gathered during two airborne field campaigns held in Darwin, Australia (2014), and Cayenne, France (2015), in the frame of the High Altitude Ice Crystals (HAIC) / High Ice Water Content (HIWC) projects. During these campaigns, a Falcon F-20 research aircraft equipped with state-of-the art microphysical instrumentation sampled numerous mesoscale convective systems (MCS) in order to study dynamical and microphysical properties and processes of high ice water content areas. Experimentally, an isokinetic evaporator probe, referred to as IKP-2, provides a reference measurement of the total water content (TWC) which equals ice water content, (IWC) when (supercooled) liquid water is absent. Two optical array probes, namely 2D-S and PIP, produce 2D images of individual crystals ranging from 50 μm to 12840 μm from which particle size distributions (PSD) are derived. Mathematically, the problem is formulated as an inverse problem in which the crystals' mass is assumed constant over a size class and is computed for each size class from IWC and PSD data: PSD.m = IW C This problem is solved using numerical optimization technique in which an objective function is minimized. The objective function is defined as follows: 2 J(m)=∥P SD.m - IW C ∥ + λ.R (m) where the regularization parameter λ and the regularization function R(m) are tuned based on data characteristics. The method is implemented in two steps. First, the method is developed on synthetic crystal populations in

  2. A scheme for parameterizing ice cloud water content in general circulation models

    NASA Technical Reports Server (NTRS)

    Heymsfield, Andrew J.; Donner, Leo J.

    1989-01-01

    A method for specifying ice water content in GCMs is developed, based on theory and in-cloud measurements. A theoretical development of the conceptual precipitation model is given and the aircraft flights used to characterize the ice mass distribution in deep ice clouds is discussed. Ice water content values derived from the theoretical parameterization are compared with the measured values. The results demonstrate that a simple parameterization for atmospheric ice content can account for ice contents observed in several synoptic contexts.

  3. Antarctic Ice Mass Balance from GRACE

    NASA Astrophysics Data System (ADS)

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

    2014-12-01

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

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

    NASA Technical Reports Server (NTRS)

    Bindschadler, Robert

    1993-01-01

    The region in the mouth of Ice Stream B (the ice plain) and that in the vicinity of Crary Ice Rise are experiencing large and rapid changes. Based on velocity, ice thickness, and accumulation rate data, the patterns of net mass balance in these regions were calculated. Net mass balance, or the rate of ice thickness change, was calculated as the residual of all mass fluxes into and out of subregions (or boxes). Net mass balance provides a measure of the state of health of the ice sheet and clues to the current dynamics.

  5. Autonomous Ice Mass Balance Buoys for Seasonal Sea Ice

    NASA Astrophysics Data System (ADS)

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

    2017-12-01

    The ice mass-balance represents the integration of all surface and ocean heat fluxes and attributing the impact of these forcing fluxes on the ice cover can be accomplished by increasing temporal and spatial measurements. Mass balance information can be used to understand the ongoing changes in the Arctic sea ice cover and to improve predictions of future ice conditions. Thinner seasonal ice in the Arctic necessitates the deployment of Autonomous Ice Mass Balance buoys (IMB's) capable of long-term, in situ data collection in both ice and open ocean. Seasonal IMB's (SIMB's) are free floating IMB's that allow data collection in thick ice, thin ice, during times of transition, and even open water. The newest generation of SIMB aims to increase the number of reliable IMB's in the Arctic by leveraging inexpensive commercial-grade instrumentation when combined with specially developed monitoring hardware. Monitoring tasks are handled by a custom, expandable data logger that provides low-cost flexibility for integrating a large range of instrumentation. The SIMB features ultrasonic sensors for direct measurement of both snow depth and ice thickness and a digital temperature chain (DTC) for temperature measurements every 2cm through both snow and ice. Air temperature and pressure, along with GPS data complete the Arctic picture. Additionally, the new SIMB is more compact to maximize deployment opportunities from multiple types of platforms.

  6. Ice-sheet mass balance and climate change.

    PubMed

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

    2013-06-06

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

  7. Ice Particle Impact on Cloud Water Content Instrumentation

    NASA Technical Reports Server (NTRS)

    Emery, Edward F.; Miller, Dean R.; Plaskon, Stephen R.; Strapp, Walter; Lillie, Lyle

    2004-01-01

    Determining the total amount of water contained in an icing cloud necessitates the measurement of both the liquid droplets and ice particles. One commonly accepted method for measuring cloud water content utilizes a hot wire sensing element, which is maintained at a constant temperature. In this approach, the cloud water content is equated with the power required to keep the sense element at a constant temperature. This method inherently assumes that impinging cloud particles remain on the sensing element surface long enough to be evaporated. In the case of ice particles, this assumption requires that the particles do not bounce off the surface after impact. Recent tests aimed at characterizing ice particle impact on a thermally heated wing section, have raised questions about the validity of this assumption. Ice particles were observed to bounce off the heated wing section a very high percentage of the time. This result could have implications for Total Water Content sensors which are designed to capture ice particles, and thus do not account for bouncing or breakup of ice particles. Based on these results, a test was conducted to investigate ice particle impact on the sensing elements of the following hot-wire cloud water content probes: (1) Nevzorov Total Water Content (TWC)/Liquid Water Content (LWC) probe, (2) Science Engineering Associates TWC probe, and (3) Particle Measuring Systems King probe. Close-up video imaging was used to study ice particle impact on the sensing element of each probe. The measured water content from each probe was also determined for each cloud condition. This paper will present results from this investigation and attempt to evaluate the significance of ice particle impact on hot-wire cloud water content measurements.

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

    NASA Astrophysics Data System (ADS)

    Mitchell, D. L.

    2013-12-01

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

  9. 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.

  10. High Ice Water Content: DC-8 Aeronautics Campaign

    NASA Image and Video Library

    2015-09-10

    During the month of August, NASA’s DC-8 completed flights in Florida aimed at collecting data on high-altitude crystals for the High Ice Water Content (HIWC) mission. High ice water content can be found within large convective storms and can result in aircraft engines losing power or not functioning properly. Researchers will use the data to develop technology that can be used onboard commercial aircraft to avoid high ice water content conditions and provide a safer flight for passengers. This video gives an inside look at the HIWC mission, including research done in and around Hurricane Danny, as well as a look at the instruments being used onboard the research aircraft. Researchers and pilots onboard worked with satellite information from the ground to find regions of high ice water content within the convective systems.

  11. Greenland Ice Sheet Mass Balance

    NASA Technical Reports Server (NTRS)

    Reeh, N.

    1984-01-01

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

  12. Partitioning CloudSat Ice Water Content for Comparison with Upper-Tropospheric Ice in Global Atmospheric Models

    NASA Astrophysics Data System (ADS)

    Chen, W. A.; Woods, C. P.; Li, J. F.; Waliser, D. E.; Chern, J.; Tao, W.; Jiang, J. H.; Tompkins, A. M.

    2010-12-01

    CloudSat provides important estimates of vertically resolved ice water content (IWC) on a global scale based on radar reflectivity. These estimates of IWC have proven beneficial in evaluating the representations of ice clouds in global models. An issue when performing model-data comparisons of IWC particularly germane to this investigation, is the question of which component(s) of the frozen water mass are represented by retrieval estimates and how they relate to what is represented in models. The present study developed and applied a new technique to partition CloudSat total IWC into small and large ice hydrometeors, based on the CloudSat-retrieved ice particle size distribution (PSD) parameters. The new method allows one to make relevant model-data comparisons and provides new insights into the model’s representation of atmospheric IWC. The partitioned CloudSat IWC suggests that the small ice particles contribute to 20-30% of the total IWC in the upper troposphere when a threshold size of 100 μm is used. Sensitivity measures with respect to the threshold size, the PSD parameters, and the retrieval algorithms are presented. The new dataset is compared to model estimates, pointing to areas for model improvement. Cloud ice analyses from the European Centre for Medium-Range Weather Forecasts model agree well with the small IWC from CloudSat. The finite-volume multi-scale modeling framework model underestimates total IWC at 147 and 215 hPa, while overestimating the fractional contribution from the small ice species. These results are discussed in terms of their applications to, and implications for, the evaluation of global atmospheric models, providing constraints on the representations of cloud feedback and precipitation in global models, which in turn can help reduce uncertainties associated with climate change projections. Figure 1. A sample lognormal ice number distribution (red curve), and the corresponding mass distribution (black curve). The dotted line

  13. Determining ice water content from 2D crystal images in convective cloud systems

    NASA Astrophysics Data System (ADS)

    Leroy, Delphine; Coutris, Pierre; Fontaine, Emmanuel; Schwarzenboeck, Alfons; Strapp, J. Walter

    2016-04-01

    Cloud microphysical in-situ instrumentation measures bulk parameters like total water content (TWC) and/or derives particle size distributions (PSD) (utilizing optical spectrometers and optical array probes (OAP)). The goal of this work is to introduce a comprehensive methodology to compute TWC from OAP measurements, based on the dataset collected during recent HAIC (High Altitude Ice Crystals)/HIWC (High Ice Water Content) field campaigns. Indeed, the HAIC/HIWC field campaigns in Darwin (2014) and Cayenne (2015) provide a unique opportunity to explore the complex relationship between cloud particle mass and size in ice crystal environments. Numerous mesoscale convective systems (MCSs) were sampled with the French Falcon 20 research aircraft at different temperature levels from -10°C up to 50°C. The aircraft instrumentation included an IKP-2 (isokinetic probe) to get reliable measurements of TWC and the optical array probes 2D-S and PIP recording images over the entire ice crystal size range. Based on the known principle relating crystal mass and size with a power law (m=α•Dβ), Fontaine et al. (2014) performed extended 3D crystal simulations and thereby demonstrated that it is possible to estimate the value of the exponent β from OAP data, by analyzing the surface-size relationship for the 2D images as a function of time. Leroy et al. (2015) proposed an extended version of this method that produces estimates of β from the analysis of both the surface-size and perimeter-size relationships. Knowing the value of β, α then is deduced from the simultaneous IKP-2 TWC measurements for the entire HAIC/HIWC dataset. The statistical analysis of α and β values for the HAIC/HIWC dataset firstly shows that α is closely linked to β and that this link changes with temperature. From these trends, a generalized parameterization for α is proposed. Finally, the comparison with the initial IKP-2 measurements demonstrates that the method is able to predict TWC values

  14. Greenland ice sheet mass balance: a review.

    PubMed

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

    2015-04-01

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

  15. 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.

  16. Ice Mass Fluctuations and Earthquake Hazard

    NASA Technical Reports Server (NTRS)

    Sauber, J.

    2006-01-01

    In south central Alaska, tectonic strain rates are high in a region that includes large glaciers undergoing ice wastage over the last 100-150 years [Sauber et al., 2000; Sauber and Molnia, 2004]. In this study we focus on the region referred to as the Yakataga segment of the Pacific-North American plate boundary zone in Alaska. In this region, the Bering and Malaspina glacier ablation zones have average ice elevation decreases from 1-3 meters/year (see summary and references in Molnia, 2005). The elastic response of the solid Earth to this ice mass decrease alone would cause several mm/yr of horizontal motion and uplift rates of up to 10-12 mm/yr. In this same region observed horizontal rates of tectonic deformation range from 10 to 40 mm/yr to the north-northwest and the predicted tectonic uplift rates range from -2 mm/year near the Gulf of Alaska coast to 12mm/year further inland [Savage and Lisowski, 1988; Ma et al, 1990; Sauber et al., 1997, 2000, 2004; Elliot et al., 2005]. The large ice mass changes associated with glacial wastage and surges perturb the tectonic rate of deformation at a variety of temporal and spatial scales. The associated incremental stress change may enhance or inhibit earthquake occurrence. We report recent (seasonal to decadal) ice elevation changes derived from data from NASA's ICESat satellite laser altimeter combined with earlier DEM's as a reference surface to illustrate the characteristics of short-term ice elevation changes [Sauber et al., 2005, Muskett et al., 2005]. Since we are interested in evaluating the effect of ice changes on faulting potential, we calculated the predicted surface displacement changes and incremental stresses over a specified time interval and calculated the change in the fault stability margin using the approach given by Wu and Hasegawa [1996]. Additionally, we explored the possibility that these ice mass fluctuations altered the seismic rate of background seismicity. Although we primarily focus on

  17. 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.

  18. The Ice Sheet Mass Balance Inter-comparison Exercise

    NASA Astrophysics Data System (ADS)

    Shepherd, A.; Ivins, E. R.

    2015-12-01

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

  19. Permafrost - Relation between ice content and dielectric losses at 100 K

    NASA Technical Reports Server (NTRS)

    Alvarez, R.

    1973-01-01

    The dielectric response of permafrost at 100 K and vacuums of around 10 ntorr is analyzed, varying its percent ice content from 1 to 18.6. The distributions obtained correspond to dielectric relaxations of the Cole-Cole type, with maximum losses occurring in the 30- to 600-Hz frequency range. The logarithms of such maxima depend linearly on the permafrost ice content, two regions of linear variation being defined above and below 3.6% ice content. Such relations point out the feasibility of determining ice content in permafrost by electromagnetic means.

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

    NASA Astrophysics Data System (ADS)

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

    2016-12-01

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

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

    NASA Astrophysics Data System (ADS)

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

    2016-12-01

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

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

    NASA Astrophysics Data System (ADS)

    Huybrechts, P.

    2003-04-01

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

  3. Normalized vertical ice mass flux profiles from vertically pointing 8-mm-wavelength Doppler radar

    NASA Technical Reports Server (NTRS)

    Orr, Brad W.; Kropfli, Robert A.

    1993-01-01

    During the FIRE 2 (First International Satellite Cloud Climatology Project Regional Experiment) project, NOAA's Wave Propagation Laboratory (WPL) operated its 8-mm wavelength Doppler radar extensively in the vertically pointing mode. This allowed for the calculation of a number of important cirrus cloud parameters, including cloud boundary statistics, cloud particle characteristic sizes and concentrations, and ice mass content (imc). The flux of imc, or, alternatively, ice mass flux (imf), is also an important parameter of a cirrus cloud system. Ice mass flux is important in the vertical redistribution of water substance and thus, in part, determines the cloud evolution. It is important for the development of cloud parameterizations to be able to define the essential physical characteristics of large populations of clouds in the simplest possible way. One method would be to normalize profiles of observed cloud properties, such as those mentioned above, in ways similar to those used in the convective boundary layer. The height then scales from 0.0 at cloud base to 1.0 at cloud top, and the measured cloud parameter scales by its maximum value so that all normalized profiles have 1.0 as their maximum value. The goal is that there will be a 'universal' shape to profiles of the normalized data. This idea was applied to estimates of imf calculated from data obtained by the WPL cloud radar during FIRE II. Other quantities such as median particle diameter, concentration, and ice mass content can also be estimated with this radar, and we expect to also examine normalized profiles of these quantities in time for the 1993 FIRE II meeting.

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

    NASA Astrophysics Data System (ADS)

    Wohlleben, Trudy M. H.

    Canadian High Arctic terrestrial ice masses and the polar atmosphere evolve codependently, and interactions between the two systems can lead to feedbacks, positive and negative. The two primary positive cryosphere-atmosphere feedbacks are: (1) The snow/ice-albedo feedback (where area changes in snow and/or ice cause changes in surface albedo and surface air temperatures, leading to further area changes in snow/ice); and (2) The elevation - mass balance feedback (where thickness changes in terrestrial ice masses cause changes to atmospheric circulation and precipitation patterns, leading to further ice thickness changes). In this thesis, numerical experiments are performed to: (1) quantify the magnitudes of the two feedbacks for chosen Canadian High Arctic terrestrial ice masses; and (2) to examine the direct and indirect consequences of surface air temperature changes upon englacial temperatures with implications for ice flow, mass flux divergence, and topographic evolution. Model results show that: (a) for John Evans Glacier, Ellesmere Island, the magnitude of the terrestrial snow/ice-albedo feedback can locally exceed that of sea ice on less than decadal timescales, with implications for glacier response times to climate perturbations; (b) although historical air temperature changes might be the direct cause of measured englacial temperature anomalies in various glacier and ice cap accumulation zones, they can also be the indirect cause of their enhanced diffusive loss; (c) while the direct result of past air temperature changes has been to cool the interior of John Evans Glacier, and its bed, the indirect result has been to create and maintain warm (pressure melting point) basal temperatures in the ablation zone; and (d) for Devon Ice Cap, observed mass gains in the northwest sector of the ice cap would be smaller without orographic precipitation and the mass balance---elevation feedback, supporting the hypothesis that this feedback is playing a role in the

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

    NASA Astrophysics Data System (ADS)

    Fricker, H. A.

    2017-12-01

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

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

    NASA Astrophysics Data System (ADS)

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

    2014-12-01

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

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

    NASA Astrophysics Data System (ADS)

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

    2017-11-01

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

  9. Simultaneous measurement of unfrozen water content and ice content in frozen soil using gamma ray attenuation and TDR

    NASA Astrophysics Data System (ADS)

    Zhou, Xiaohai; Zhou, Jian; Kinzelbach, Wolfgang; Stauffer, Fritz

    2014-12-01

    The freezing temperature of water in soil is not constant but varies over a range determined by soil texture. Consequently, the amounts of unfrozen water and ice change with temperature in frozen soil, which in turn affects hydraulic, thermal, and mechanical properties of frozen soil. In this paper, an Am-241 gamma ray source and time-domain reflectometry (TDR) were combined to measure unfrozen water content and ice content in frozen soil simultaneously. The gamma ray attenuation was used to determine total water content. The TDR was used to determine the dielectric constant of the frozen soil. Based on a four-phase mixing model, the amount of unfrozen water content in the frozen soil could be determined. The ice content was inferred by the difference between total water content and unfrozen water content. The gamma ray attenuation and the TDR were both calibrated by a gravimetric method. Water contents measured by gamma ray attenuation and TDR in an unfrozen silt column under infiltration were compared and showed that the two methods have the same accuracy and response to changes of water content. Unidirectional column freezing experiments were performed to apply the combined method of gamma ray attenuation and TDR for measuring unfrozen water content and ice content. The measurement error of the gamma ray attenuation and TDR was around 0.02 and 0.01 m3/m3, respectively. The overestimation of unfrozen water in frozen soil by TDR alone was quantified and found to depend on the amount of ice content. The higher the ice content, the larger the overestimation. The study confirmed that the combined method could accurately determine unfrozen water content and ice content in frozen soil. The results of soil column freezing experiments indicate that total water content distribution is affected by available pore space and the freezing front advance rate. It was found that there is similarity between the soil water characteristic and the soil freezing characteristic of

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

    NASA Astrophysics Data System (ADS)

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

    2017-12-01

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

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

    NASA Astrophysics Data System (ADS)

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

    2015-05-01

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

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

    NASA Astrophysics Data System (ADS)

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

    2015-12-01

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

  13. HAIC/HIWC field project: characterizing the high ice water content environment

    NASA Astrophysics Data System (ADS)

    Leroy, Delphine; Coutris, Pierre; Fontaine, Emmanuel; Schwarzenboeck, Alfons; Strapp, J. Walter; Korolev, Alexei; McFarquhar, Greg; Gourbeyre, Christophe; Dupuy, Regis; Dezitter, Fabien; Calmels, Alice

    2016-04-01

    High ice water content (IWC) cloud regions in mesoscale convective systems (MCSs) are suspected to cause in-service engine power loss events and air-data probe malfunctions on commercial aircraft. In order to better document this particular environment, a multi-year international HAIC/HIWC (High Altitude Ice Crystals / High Ice Water Content) field project has been designed including two field campaigns. The first campaign was conducted in Darwin in 2014 while the second one took place in Cayenne in May 2015. The French Falcon 20 research aircraft has been deployed for the two campaigns, with an instrumental payload including an IKP-2 (isokinetic evaporator probe which provides a reference measurement of IWC), a CDP-2 (cloud droplet spectrometer probe measuring particles in the range 2-50 μm), and optical array probes 2D-S (2D-Stereo, 10-1280 μm) and PIP (precipitation imaging probe, 100-6400 μm). 23 flights were performed in Darwin, 18 in Cayenne, all sampling MCSs at different flight levels with temperatures from -10°C to -50°C. The study presented here focuses on ice crystal size properties related to IWC, thereby analyzing in detail the 2D image data from 2D-S and PIP optical array imaging probes. 2D images recorded with 2D-S and PIP probes were processed in order to produce particle size distributions (PSDs) and median mass diameters (MMDs). Darwin results shows that ice crystals properties are quite different in high IWC areas compared to the surrounding cloud regions. Most of the sampled MCS reveal that the higher the measured IWC, the smaller are the corresponding crystal MMD. This effect is interfering with a temperature trend, whereby colder temperatures are leading to smaller MMD. A preliminary analysis of the Cayenne data seems to be consistent with the above trends.

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

    PubMed

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

    2012-11-30

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

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

    PubMed

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

    2015-05-01

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

  16. A Reconciled Estimate of Ice-Sheet Mass Balance

    NASA Technical Reports Server (NTRS)

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

    2012-01-01

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

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

    NASA Astrophysics Data System (ADS)

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

    2013-09-01

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

  18. Sensible heat balance estimates of transient soil ice contents for freezing and thawing conditions

    USDA-ARS?s Scientific Manuscript database

    Soil ice content is an important component for winter soil hydrology. The sensible heat balance (SHB) method using measurements from heat pulse probes (HPP) is a possible way to determine transient soil ice content. In a previous study, in situ soil ice contents estimates with the SHB method were in...

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

    NASA Technical Reports Server (NTRS)

    vanderVeen, Cornelius

    2003-01-01

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

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

    NASA Technical Reports Server (NTRS)

    Li, Jun; Zwally, H. Jay

    2011-01-01

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

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

    NASA Astrophysics Data System (ADS)

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

    2012-12-01

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

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

    NASA Astrophysics Data System (ADS)

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

    2017-12-01

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

  3. Porosity and Salt Content Determine if Subduction Can Occur in Europa's Ice Shell

    NASA Astrophysics Data System (ADS)

    Johnson, Brandon C.; Sheppard, Rachel Y.; Pascuzzo, Alyssa C.; Fisher, Elizabeth A.; Wiggins, Sean E.

    2017-12-01

    Motivated by recent evidence for subduction in Europa's ice shell, we explore the geophysical feasibility of this process. Here we construct a simple model to track the evolution of porosity and temperature within a slab that is forced to subduct. We also vary the initial salt content in Europa's ice shell and determine the buoyancy of our simulated subducting slab. We find that porosity and salt content play a dominant role in determining whether the slab is nonbuoyant and subduction in Europa's ice shell is actually possible. Generally, we find that initially low porosities and high salt contents within the conductive lid are more conducive to subduction. If salt contents are laterally homogenous, and Europa has a reasonable surface porosity of ϕ0 = 0.1, the conductive portion of Europa's shell must have salt contents exceeding 22% for subduction to occur. However, if salt contents are laterally heterogeneous, with salt contents varying by a few percent, subduction may occur for a surface porosity of ϕ0 = 0.1 and overall salt contents of 5%. Thus, we argue that under plausible conditions, subduction in Europa's ice shell is possible. Moreover, assuming that subduction is actively occurring or has occurred in Europa's recent past provides important constraints on the structure and composition of the ice shell.

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

    NASA Technical Reports Server (NTRS)

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

    2003-01-01

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

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

    NASA Technical Reports Server (NTRS)

    Zwally, H. Jay

    2010-01-01

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

  6. Soil Water Content Sensors as a Method of Measuring Ice Depth

    NASA Astrophysics Data System (ADS)

    Whitaker, E.; Reed, D. E.; Desai, A. R.

    2015-12-01

    Lake ice depth provides important information about local and regional climate change, weather patterns, and recreational safety, as well as impacting in situ ecology and carbon cycling. However, it is challenging to measure ice depth continuously from a remote location, as existing methods are too large, expensive, and/or time-intensive. Therefore, we present a novel application that reduces the size and cost issues by using soil water content reflectometer sensors. Analysis of sensors deployed in an environmental chamber using a scale model of a lake demonstrated their value as accurate measures of the change in ice depth over any time period, through measurement of the liquid-to-solid phase change. A robust correlation exists between volumetric water content in time as a function of environmental temperature. This relationship allows us to convert volumetric water content into ice depth. An array of these sensors will be placed in Lake Mendota, Madison, Wisconsin in winter 2015-2016, to create a temporally high-resolution ice depth record, which will be used for ecological or climatological studies while also being transmitted to the public to increase recreational safety.

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

    NASA Technical Reports Server (NTRS)

    Rignot, Eric (Editor)

    1999-01-01

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

  8. Ice particle mass-dimensional parameter retrieval and uncertainty analysis using an Optimal Estimation framework applied to in situ data

    NASA Astrophysics Data System (ADS)

    Xu, Zhuocan; Mace, Jay; Avalone, Linnea; Wang, Zhien

    2015-04-01

    The extreme variability of ice particle habits in precipitating clouds affects our understanding of these cloud systems in every aspect (i.e. radiation transfer, dynamics, precipitation rate, etc) and largely contributes to the uncertainties in the model representation of related processes. Ice particle mass-dimensional power law relationships, M=a*(D ^ b), are commonly assumed in models and retrieval algorithms, while very little knowledge exists regarding the uncertainties of these M-D parameters in real-world situations. In this study, we apply Optimal Estimation (OE) methodology to infer ice particle mass-dimensional relationship from ice particle size distributions and bulk water contents independently measured on board the University of Wyoming King Air during the Colorado Airborne Multi-Phase Cloud Study (CAMPS). We also utilize W-band radar reflectivity obtained on the same platform (King Air) offering a further constraint to this ill-posed problem (Heymsfield et al. 2010). In addition to the values of retrieved M-D parameters, the associated uncertainties are conveniently acquired in the OE framework, within the limitations of assumed Gaussian statistics. We find, given the constraints provided by the bulk water measurement and in situ radar reflectivity, that the relative uncertainty of mass-dimensional power law prefactor (a) is approximately 80% and the relative uncertainty of exponent (b) is 10-15%. With this level of uncertainty, the forward model uncertainty in radar reflectivity would be on the order of 4 dB or a factor of approximately 2.5 in ice water content. The implications of this finding are that inferences of bulk water from either remote or in situ measurements of particle spectra cannot be more certain than this when the mass-dimensional relationships are not known a priori which is almost never the case.

  9. Specific findings on ice crystal microphysical properties from in-situ observation

    NASA Astrophysics Data System (ADS)

    Coutris, Pierre; Leroy, Delphine; Fontaine, Emmanuel; Schwarzenboeck, Alfons; Strapp, J. Walter

    2017-04-01

    This study focuses on microphysical properties of ice particles populating high ice water content areas in Mesoscale Convective Systems (MCS). These clouds have been extensively sampled during the High Altitude Ice Crystal - High Ice Water Content international projects (HAIC-HIWC, Dezitter et al. 2013, Strapp et al. 2015) with the objective of characterizing ice particle properties such as size distribution, radar reflectivity and ice water content. The in-situ data collected during these campaigns at different temperature levels and in different type of MCS (oceanic, continental) make the HAIC-HIWC data set a unique opportunity to study ice particle microphysical properties. Recently, a new approach to retrieve ice particle mass from in-situ measurements has been developed: a forward model that relates ice particles' mass to Particle Size Distribution (PSD) and Ice Water Content (IWC) is formulated as a linear system of equations and the retrieval process consists in solving the inverse problem with numerical optimization tools (Coutris et al. 2016). In this study, this new method is applied to HAIC-HIWC data set and main outcomes are discussed. First, the method is compared to a classical power-law based method using data from one single flight performed in Darwin area on February, 7th 2014. The observed differences in retrieved quantities such as ice particle mass, ice water content or median mass diameter, highlight the potential benefit of abandoning the power law simplistic assumption. The method is then applied to data measured at different cloud temperatures ranging from -40°C to -10°C during several flights of both Darwin 2014 and Cayenne 2015 campaigns. Specific findings about ice microphysical properties such as variations of effective density with particle size and the influence of cloud temperature on particle effective density are presented.

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

    NASA Astrophysics Data System (ADS)

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

    2017-12-01

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

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

    NASA Astrophysics Data System (ADS)

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

    2017-12-01

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

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

    USGS Publications Warehouse

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

    2008-01-01

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

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

    NASA Astrophysics Data System (ADS)

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

    2018-01-01

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

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

    NASA Astrophysics Data System (ADS)

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

    2017-04-01

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

  15. Examining impacts of mass-diameter (m-D) and area-diameter (A-D) relationships of ice particles on retrievals of effective radius and ice water content from radar and lidar measurements

    NASA Astrophysics Data System (ADS)

    Ham, Seung-Hee; Kato, Seiji; Rose, Fred G.

    2017-03-01

    Mass-diameter (m-D) and projected area-diameter (A-D) relations are often used to describe the shape of nonspherical ice particles. This study analytically investigates how retrieved effective radius (reff) and ice water content (IWC) from radar and lidar measurements depend on the assumption of m-D [m(D) = a Db] and A-D [A(D) = γ Dδ] relationships. We assume that unattenuated reflectivity factor (Z) and visible extinction coefficient (kext) by cloud particles are available from the radar and lidar measurements, respectively. A sensitivity test shows that reff increases with increasing a, decreasing b, decreasing γ, and increasing δ. It also shows that a 10% variation of a, b, γ, and δ induces more than a 100% change of reff. In addition, we consider both gamma and lognormal particle size distributions (PSDs) and examine the sensitivity of reff to the assumption of PSD. It is shown that reff increases by up to 10% with increasing dispersion (μ) of the gamma PSD by 2, when large ice particles are predominant. Moreover, reff decreases by up to 20% with increasing the width parameter (ω) of the lognormal PSD by 0.1. We also derive an analytic conversion equation between two effective radii when different particle shapes and PSD assumptions are used. When applying the conversion equation to nine types of m-D and A-D relationships, reff easily changes up to 30%. The proposed reff conversion method can be used to eliminate the inconsistency of assumptions that made in a cloud retrieval algorithm and a forward radiative transfer model.

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

    NASA Astrophysics Data System (ADS)

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

    2009-12-01

    Mountain glaciers and ice caps contribute roughly half of eustatic sea-level rise. Greenland has thousands of small mountain glaciers and several ice caps > 1000 sq. km that have not been included in previous mass balance calculations. To include small glaciers and ice caps in our study, we use Polar WRF, a next-generation regional climate data assimilation model is run at grid resolution less than 10 km. WRF provides surface mass balance data at sufficiently high resolution to resolve not only the narrow ice sheet ablation zone, but provides information useful in downscaling melt and accumulation rates on mountain glaciers and ice caps. In this study, we refine Polar WRF to simulate a realistic surface energy budget. Surface melting is calculated in-line from surface energy budget closure. Blowing snow sublimation is computed in-line. Melt water re-freeze is calculated using a revised scheme. Our results are compared with NASA's Gravity Recovery and Climate Experiment (GRACE) and associated error is calculated on a regional and local scale with validation from automated weather stations (AWS), snow pits and ice core data from various regions along the Greenland ice sheet.

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

    NASA Astrophysics Data System (ADS)

    Harig, C.

    2017-12-01

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

  18. Liquid water content and droplet size calibration of the NASA Lewis Icing Research Tunnel

    NASA Technical Reports Server (NTRS)

    Ide, Robert F.

    1989-01-01

    The icing research tunnel at the NASA Lewis Research Center underwent a major rehabilitation in 1986 to 1987, necessitating recalibration of the icing cloud. The methods used in the recalibration, including the procedure used to establish a uniform icing cloud and the use of a standard icing blade technique for measurement of liquid water content are described. PMS Forward Scattering Spectrometer and Optical Array probes were used for measurement of droplet size. Examples of droplet size distributions are shown for several median volumetric diameters. Finally, the liquid water content/droplet size operating envelopes of the icing tunnel are shown for a range of airspeeds and are compared to the FAA icing certification criteria.

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

    NASA Astrophysics Data System (ADS)

    Harig, Christopher; Simons, Frederik J.

    2015-04-01

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

  20. 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.

  1. 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.

  2. HAIC/HIWC field campaign - investigating ice microphysics in high ice water content regions of mesoscale convective systems

    NASA Astrophysics Data System (ADS)

    Leroy, Delphine; Fontaine, Emmanuel; Schwarzenboeck, Alfons; Strapp, J. Walter; Lilie, Lyle; Dezitter, Fabien; Grandin, Alice

    2015-04-01

    Despite existing research programs focusing on tropical convection, high ice water content (IWC) regions in Mesoscale Convective Systems (MCS) - potentially encountered by commercial aircraft and related to reported in-service events - remain poorly documented either because investigation of such high IWC regions was not of highest priority or because utilized instrumentation was not capable of providing accurate cloud microphysical measurements. To gather quantitative data in high IWC regions, a multi-year international HAIC/HIWC (High Altitude Ice Crystals / High Ice Water Content) field project has been designed including a first field campaign conducted out of Darwin (Australia) in 2014. The French Falcon 20 research aircraft had been equipped among others with a state-of-the-art in situ microphysics package including the IKP (isokinetic evaporator probe which provides a reference measurement of IWC and TWC), the CDP (cloud droplet spectrometer probe measuring particles in the range 2-50 µm), the 2D-S (2D-Stereo, 10-1280 µm) and PIP (precipitation imaging probe, 100-6400 µm) optical array probes. Microphysical data collection has been performed mainly at -40°C and -30°C levels, whereas little data could be sampled at -50°C and at -15C/-10°C. The study presented here focuses on ice crystal size properties, thereby analyzing in detail the 2D image data from 2D-S and PIP optical array imaging probes. 2D images recorded with 2D-S and PIP were processed in order to extract a large variety of geometrical parameters, such as maximum diameter (Dmax), 2D surface equivalent diameter (Deq), and the corresponding number particle size distribution (PSD). Using the PSD information from both probes, a composite size distribution was then built, with sizes ranging from few tens of µm to roughly 10 mm. Finally, mass-size relationships for ice crystals in tropical convection were established in terms of power laws in order to compute median mass diameters MMDmax and

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

    NASA Technical Reports Server (NTRS)

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

    2011-01-01

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

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

    NASA Technical Reports Server (NTRS)

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

    2011-01-01

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

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

    NASA Technical Reports Server (NTRS)

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

    2001-01-01

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

  6. High Ice Water Content at Low Radar Reflectivity near Deep Convection: Part II. Evaluation of Microphysical Pathways in Updraft Parcel Simulations

    NASA Technical Reports Server (NTRS)

    Ackerman, A. S.; Fridlind, A. M.; Grandin, A.; Dezitter, F.; Weber, M.; Strapp, J. W.; Korolev, A. V.

    2015-01-01

    The aeronautics industry has established that a threat to aircraft is posed by atmospheric conditions of substantial ice water content (IWC) where equivalent radar reflectivity (Ze) does not exceed 20-30 dBZ and supercooled water is not present; these conditions are encountered almost exclusively in the vicinity of deep convection. Part 1 (Fridlind et al., 2015) of this two-part study presents in situ measurements of such conditions sampled by Airbus in three tropical regions, commonly near 11 km and -43 C, and concludes that the measured ice particle size distributions are broadly consistent with past literature with profiling radar measurements of Z(sub e) and mean Doppler velocity obtained within monsoonal deep convection in one of the regions sampled. In all three regions, the Airbus measurements generally indicate variable IWC that often exceeds 2 gm (exp -3) with relatively uniform mass median area-equivalent diameter (MMD(sub eq) of 200-300 micrometers. Here we use a parcel model with size-resolved microphysics to investigate microphysical pathways that could lead to such conditions. Our simulations indicate that homogeneous freezing of water drops produces a much smaller ice MMD(sub eq) than observed, and occurs only in the absence of hydrometeor gravitational collection for the conditions considered. Development of a mass mode of ice aloft that overlaps with the measurements requires a substantial source of small ice particles at temperatures of about -10 C or warmer, which subsequently grow from water vapor. One conceivable source in our simulation framework is Hallett-Mossop ice production; another is abundant concentrations of heterogeneous ice freezing nuclei acting together with copious shattering of water drops upon freezing. Regardless of the production mechanism, the dominant mass modal diameter of vapor-grown ice is reduced as the ice-multiplication source strength increases and as competition for water vapor increases. Both mass and modal

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

    NASA Technical Reports Server (NTRS)

    SauberRosenberg, Jeanne M.; Molnia, Bruce F.

    2003-01-01

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

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

    NASA Astrophysics Data System (ADS)

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

    2016-06-01

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

  9. Prediction of dry ice mass for firefighting robot actuation

    NASA Astrophysics Data System (ADS)

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

    2017-11-01

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

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

    NASA Technical Reports Server (NTRS)

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

    2001-01-01

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

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

    NASA Astrophysics Data System (ADS)

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

    2012-04-01

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

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

    NASA Astrophysics Data System (ADS)

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

    2016-04-01

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

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

    NASA Astrophysics Data System (ADS)

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

    2013-03-01

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

  14. Strong linkage of polar cod (Boreogadus saida) to sea ice algae-produced carbon: Evidence from stomach content, fatty acid and stable isotope analyses

    NASA Astrophysics Data System (ADS)

    Kohlbach, Doreen; Schaafsma, Fokje L.; Graeve, Martin; Lebreton, Benoit; Lange, Benjamin Allen; David, Carmen; Vortkamp, Martina; Flores, Hauke

    2017-03-01

    The polar cod (Boreogadus saida) is considered an ecological key species, because it reaches high stock biomasses and constitutes an important carbon source for seabirds and marine mammals in high-Arctic ecosystems. Young polar cod (1-2 years) are often associated with the underside of sea ice. To evaluate the impact of changing Arctic sea ice habitats on polar cod, we examined the diet composition and quantified the contribution of ice algae-produced carbon (αIce) to the carbon budget of polar cod. Young polar cod were sampled in the ice-water interface layer in the central Arctic Ocean during late summer 2012. Diets and carbon sources of these fish were examined using 4 approaches: (1) stomach content analysis, (2) fatty acid (FA) analysis, (3) bulk nitrogen and carbon stable isotope analysis (BSIA) and (4) compound-specific stable isotope analysis (CSIA) of FAs. The ice-associated (sympagic) amphipod Apherusa glacialis dominated the stomach contents by mass, indicating a high importance of sympagic fauna in young polar cod diets. The biomass of food measured in stomachs implied constant feeding at daily rates of ∼1.2% body mass per fish, indicating the potential for positive growth. FA profiles of polar cod indicated that diatoms were the primary carbon source, indirectly obtained via amphipods and copepods. The αIce using bulk isotope data from muscle was estimated to be >90%. In comparison, αIce based on CSIA ranged from 34 to 65%, with the highest estimates from muscle and the lowest from liver tissue. Overall, our results indicate a strong dependency of polar cod on ice-algae produced carbon. This suggests that young polar cod may be particularly vulnerable to changes in the distribution and structure of sea ice habitats. Due to the ecological key role of polar cod, changes at the base of the sea ice-associated food web are likely to affect the higher trophic levels of high-Arctic ecosystems.

  15. 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.

  16. 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.

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

    NASA Astrophysics Data System (ADS)

    Visnjevic, Vjeran; Herman, Frédéric; Licul, Aleksandar

    2016-04-01

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

  18. Laboratory Investigation of Direct Measurement of Ice Water Content, Ice Surface Area, and Effective Radius of Ice Crystals Using a Laser-Diffraction Instrument

    NASA Technical Reports Server (NTRS)

    Gerber, H.; DeMott, P. J.; Rogers, D. C.

    1995-01-01

    The aircraft microphysics probe, PVM-100A, was tested in the Colorado State University dynamic cloud chamber to establish its ability to measure ice water content (IWC), PSA, and Re in ice clouds. Its response was compared to other means of measuring those ice-cloud parameters that included using FSSP-100 and 230-X 1-D optical probes for ice-crystal concentrations, a film-loop microscope for ice-crystal habits and dimensions, and an in-situ microscope for determining ice-crystal orientation. Intercomparisons were made in ice clouds containing ice crystals ranging in size from about 10 microns to 150 microns diameter, and ice crystals with plate, columnar, dendritic, and spherical shapes. It was not possible to determine conclusively that the PVM accurately measures IWC, PSA, and Re of ice crystals, because heat from the PVM evaporated in part the crystals in its vicinity in the chamber thus affecting its measurements. Similarities in the operating principle of the FSSP and PVM, and a comparison between Re measured by both instruments, suggest, however, that the PVM can make those measurements. The resolution limit of the PVM for IWC measurements was found to be on the order of 0.001 g/cubic m. Algorithms for correcting IWC measured by FSSP and PVM were developed.

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

    NASA Technical Reports Server (NTRS)

    James, Thomas S.; Ivins, Erik R.

    1995-01-01

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

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

    NASA Technical Reports Server (NTRS)

    James, Thomas S.; Ivins, Erik R.

    1995-01-01

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

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

    NASA Astrophysics Data System (ADS)

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

    2017-09-01

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

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

    NASA Astrophysics Data System (ADS)

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

    2017-12-01

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

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

    PubMed Central

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

    2012-01-01

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

  4. Effect of fat content on the physical properties and consumer acceptability of vanilla ice cream.

    PubMed

    Rolon, M Laura; Bakke, Alyssa J; Coupland, John N; Hayes, John E; Roberts, Robert F

    2017-07-01

    Ice cream is a complex food matrix that contains multiple physical phases. Removal of 1 ingredient may affect not only its physical properties but also multiple sensory characteristics that may or may not be important to consumers. Fat not only contributes to texture, mouth feel, and flavor, but also serves as a structural element. We evaluated the effect of replacing fat with maltodextrin (MD) on select physical properties of ice cream and on consumer acceptability. Vanilla ice creams were formulated to contain 6, 8, 10, 12, and 14% fat, and the difference was made up with 8, 6, 4, 2, and 0% maltodextrin, respectively, to balance the mix. Physical characterization included measurements of overrun, apparent viscosity, fat particle size, fat destabilization, hardness, and melting rate. A series of sensory tests were conducted to measure liking and the intensity of various attributes. Tests were also conducted after 19 weeks of storage at -18°C to assess changes in acceptance due to prolonged storage at unfavorable temperatures. Then, discrimination tests were performed to determine which differences in fat content were detectable by consumers. Mix viscosity decreased with increasing fat content and decreasing maltodextrin content. Fat particle size and fat destabilization significantly increased with increasing fat content. However, acceptability did not differ significantly across the samples for fresh or stored ice cream. Following storage, ice creams with 6, 12, and 14% fat did not differ in acceptability compared with fresh ice cream. However, the 8% fat, 6% MD and 10% fat, 4% MD ice creams showed a significant drop in acceptance after storage relative to fresh ice cream at the same fat content. Consumers were unable to detect a difference of 2 percentage points in fat level between 6 and 12% fat. They were able to detect a difference of 4 percentage points for ice creams with 6% versus 10%, but not for those with 8% versus 12% fat. Removing fat and replacing

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

    NASA Technical Reports Server (NTRS)

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

    2000-01-01

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

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

    NASA Astrophysics Data System (ADS)

    Sauber, Jeanne M.; Molnia, Bruce F.

    2004-07-01

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

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

    USGS Publications Warehouse

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

    2004-01-01

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

  8. Novel two-step laser ablation and ionization mass spectrometry (2S-LAIMS) of actor-spectator ice layers: Probing chemical composition of D{sub 2}O ice beneath a H{sub 2}O ice layer

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

    Yang, Rui, E-mail: ryang73@ustc.edu; Gudipati, Murthy S., E-mail: gudipati@jpl.nasa.gov

    2014-03-14

    In this work, we report for the first time successful analysis of organic aromatic analytes imbedded in D{sub 2}O ices by novel infrared (IR) laser ablation of a layered non-absorbing D{sub 2}O ice (spectator) containing the analytes and an ablation-active IR-absorbing H{sub 2}O ice layer (actor) without the analyte. With these studies we have opened up a new method for the in situ analysis of solids containing analytes when covered with an IR laser-absorbing layer that can be resonantly ablated. This soft ejection method takes advantage of the tenability of two-step infrared laser ablation and ultraviolet laser ionization mass spectrometry,more » previously demonstrated in this lab to study chemical reactions of polycyclic aromatic hydrocarbons (PAHs) in cryogenic ices. The IR laser pulse tuned to resonantly excite only the upper H{sub 2}O ice layer (actor) generates a shockwave upon impact. This shockwave penetrates the lower analyte-containing D{sub 2}O ice layer (spectator, a non-absorbing ice that cannot be ablated directly with the wavelength of the IR laser employed) and is reflected back, ejecting the contents of the D{sub 2}O layer into the vacuum where they are intersected by a UV laser for ionization and detection by a time-of-flight mass spectrometer. Thus, energy is transmitted from the laser-absorbing actor layer into the non-absorbing spectator layer resulting its ablation. We found that isotope cross-contamination between layers was negligible. We also did not see any evidence for thermal or collisional chemistry of PAH molecules with H{sub 2}O molecules in the shockwave. We call this “shockwave mediated surface resonance enhanced subsurface ablation” technique as “two-step laser ablation and ionization mass spectrometry of actor-spectator ice layers.” This method has its roots in the well-established MALDI (matrix assisted laser desorption and ionization) method. Our method offers more flexibility to optimize both the processes

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

    NASA Astrophysics Data System (ADS)

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

    2016-04-01

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

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

    NASA Technical Reports Server (NTRS)

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

    2013-01-01

    Atmospheric, oceanic, and subglacial forcing scenarios from the Sea-level Response to Ice Sheet Evolution (SeaRISE) project are applied to six three-dimensional thermomechanical ice-sheet models to assess Antarctic ice sheet sensitivity over a 500 year timescale and to inform future modeling and field studies. Results indicate (i) growth with warming, except within low-latitude basins (where inland thickening is outpaced by marginal thinning); (ii) mass loss with enhanced sliding (with basins dominated by high driving stresses affected more than basins with low-surface-slope streaming ice); and (iii) mass loss with enhanced ice shelf melting (with changes in West Antarctica dominating the signal due to its marine setting and extensive ice shelves; cf. minimal impact in the Terre Adelie, George V, Oates, and Victoria Land region of East Antarctica). Ice loss due to dynamic changes associated with enhanced sliding and/or sub-shelf melting exceeds the gain due to increased precipitation. Furthermore, differences in results between and within basins as well as the controlling impact of sub-shelf melting on ice dynamics highlight the need for improved understanding of basal conditions, grounding-zone processes, ocean-ice interactions, and the numerical representation of all three.

  11. Evolution of Summer Ocean Mixed Layer Heat Content and Ocean/Ice Fluxes in the Arctic Ocean During the Last Decade

    NASA Astrophysics Data System (ADS)

    Stanton, T. P.; Shaw, W. J.

    2014-12-01

    Since 2002, a series of 28 Autonomous Ocean Flux Buoys have been deployed in the Beaufort Sea and from the North Pole Environmental Observatory. These long-term ice-deployed instrument systems primarily measure vertical turbulent fluxes of heat, salt and momentum at a depth of 2 - 6 m below the ocean/ice interface, while concurrently measuring current profile every 2m down to approximately 40-50m depth, within the seasonal pycnocline. Additional sensors have been added to measure local ice melt rates acoustically, and finescale thermal structure from the eddy correlation flux sensor up into the ice to resolve summer near-surface heating. The AOFB buoys have typically been co-located with Ice Tethered Profilers, that measure the upper ocean T/S structure and ice mass balance instruments. Comparisons of near-surface heat fluxes, heat content and vertical structure over the last decade will be made for buoys in the Beaufort Sea and Transpolar Drift between the North Pole and Spitzbergen. The effects of enhanced basal melting from ice/albedo feedbacks can be clearly seen in the low ice concentration summer conditions found more recently in the Beaufort Sea, while there are less pronounced effects of enhanced summer surface heating in the higher ice concentrations still found in the transpolar drift.

  12. Ice core evidence for extensive melting of the greenland ice sheet in the last interglacial.

    PubMed

    Koerner, R M

    1989-05-26

    Evidence from ice at the bottom of ice cores from the Canadian Arctic Islands and Camp Century and Dye-3 in Greenland suggests that the Greenland ice sheet melted extensively or completely during the last interglacial period more than 100 ka (thousand years ago), in contrast to earlier interpretations. The presence of dirt particles in the basal ice has previously been thought to indicate that the base of the ice sheets had melted and that the evidence for the time of original growth of these ice masses had been destroyed. However, the particles most likely blew onto the ice when the dimensions of the ice caps and ice sheets were much smaller. Ice texture, gas content, and other evidence also suggest that the basal ice at each drill site is superimposed ice, a type of ice typical of the early growth stages of an ice cap or ice sheet. If the present-day ice masses began their growth during the last interglacial, the ice sheet from the earlier (Illinoian) glacial period must have competely or largely melted during the early part of the same interglacial period. If such melting did occur, the 6-meter higher-than-present sea level during the Sangamon cannot be attributed to disintegration of the West Antarctic ice sheet, as has been suggested.

  13. Breaking Off of Large Ice Masses From Hanging Glaciers

    NASA Astrophysics Data System (ADS)

    Pralong, A.; Funk, M.

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

  14. Field test and sensitivity analysis of a sensible heat balance method to determine ice contents

    USDA-ARS?s Scientific Manuscript database

    Soil ice content impacts winter vadose zone hydrology. It may be possible to estimate changes in soil ice content with a sensible heat balance (SHB) method, using measurements from heat pulse (HP) sensors. Feasibility of the SHB method is unknown because of difficulties in measuring soil thermal pro...

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

    NASA Astrophysics Data System (ADS)

    Millan, Romain; Mouginot, Jeremie; Rignot, Eric

    2017-02-01

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

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

    NASA Astrophysics Data System (ADS)

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

    2017-12-01

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

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

    NASA Technical Reports Server (NTRS)

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

    2001-01-01

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

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

    NASA Astrophysics Data System (ADS)

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

    2016-12-01

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

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

    NASA Astrophysics Data System (ADS)

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

    2007-10-01

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

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

    NASA Astrophysics Data System (ADS)

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

    2017-12-01

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

  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 snow in sea <span class="hlt">ice</span> <span class="hlt">mass</span> balance is largely two fold. Firstly, it can slow down growth and melt due to its high insulation and high reflectance, but secondly it can actually contribute to sea <span class="hlt">ice</span> growth if the snow cover is turned into <span class="hlt">ice</span>. The latter is largely a consequence of high <span class="hlt">mass</span> of snow on top of sea <span class="hlt">ice</span> that can push the surface of the sea <span class="hlt">ice</span> below sea level and seawater can flood the <span class="hlt">ice</span>. This mixture of seawater and snow can then freeze and add to the growth of sea <span class="hlt">ice</span>. This is very typical in the Antarctic but not believed to be so important in the Arctic. In this work we show, for the first time, that snow actually contributes significantly to the growth of Arctic sea <span class="hlt">ice</span>. This is likely a consequence of the thinning of the Arctic sea <span class="hlt">ice</span>. The conditions in the Arctic, with</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1352361-present-day-future-antarctic-ice-sheet-climate-surface-mass-balance-community-earth-system-model','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1352361-present-day-future-antarctic-ice-sheet-climate-surface-mass-balance-community-earth-system-model"><span>Present-day and future Antarctic <span class="hlt">ice</span> sheet climate and surface <span class="hlt">mass</span> balance in the Community Earth System Model</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Lenaerts, Jan T. M.; Vizcaino, Miren; Fyke, Jeremy Garmeson; ...</p> <p>2016-02-01</p> <p>Here, we present climate and surface <span class="hlt">mass</span> balance (SMB) of the Antarctic <span class="hlt">ice</span> sheet (AIS) as simulated by the global, coupled ocean–atmosphere–land Community Earth System Model (CESM) with a horizontal resolution of ~1° in the past, present and future (1850–2100). CESM correctly simulates present-day Antarctic sea <span class="hlt">ice</span> extent, large-scale atmospheric circulation and near-surface climate, but fails to simulate the recent expansion of Antarctic sea <span class="hlt">ice</span>. The present-day Antarctic <span class="hlt">ice</span> sheet SMB equals 2280 ± 131Gtyear –1, which concurs with existing independent estimates of AIS SMB. When forced by two CMIP5 climate change scenarios (high mitigation scenario RCP2.6 and high-emission scenariomore » RCP8.5), CESM projects an increase of Antarctic <span class="hlt">ice</span> sheet SMB of about 70 Gtyear –1 per degree warming. This increase is driven by enhanced snowfall, which is partially counteracted by more surface melt and runoff along the <span class="hlt">ice</span> sheet’s edges. This intensifying hydrological cycle is predominantly driven by atmospheric warming, which increases (1) the moisture-carrying capacity of the atmosphere, (2) oceanic source region evaporation, and (3) summer AIS cloud liquid water <span class="hlt">content</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.A23A0176K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A23A0176K"><span>Detecting High <span class="hlt">Ice</span> Water <span class="hlt">Content</span> Cloud Regions Using Airborne and Satellite Observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kheyrollah Pour, H.; Korolev, A.; Barker, H.; Wolde, M.; Heckman, I.; Duguay, C. R.</p> <p>2016-12-01</p> <p>Tropical mesoscale convective systems (MCS) have significant impacts on local and global hydrological cycles and radiation budgets. Moreover, high <span class="hlt">ice</span> water <span class="hlt">content</span> (HIWC) found inside MCS clouds at altitudes above 7 km have been identified as hazardous for aviation safety. The environment inside HIWC cloud regions may cause <span class="hlt">icing</span> of aircraft engines resulting in uncontrolled engine power loss or damage. This phenomenon is known as <span class="hlt">ice</span> crystal <span class="hlt">icing</span> (ICI). International aviation regulatory agencies are now attempting to define techniques that enable prediction and detection of potential ICI environments. Such techniques range from on-board HIWC detection to nowcasting of <span class="hlt">ice</span> crystal weather using satellite data and numerical weather prediction models. The most practical way to monitor continuously for areas of HIWC is by remote sensing with passive radiometers on geostationary satellites. Establishing correlations between HIWC cloud regions and radiances is, however, a challenging problem. This is because regions of HIWC can occur several kilometers below cloud top, while passive satellite radiometers response mainly to the upper kilometers of MCS clouds. The High Altitude <span class="hlt">Ice</span> Crystals - High <span class="hlt">Ice</span> Water <span class="hlt">Content</span> (HAIC-HIWC) field campaigns in Cayenne, French Guiana collected a rich dataset from aboard the Canadian NRC Convair-580 that was equipped with a suite of in-situ microphysical instruments and Dopplerized W- and X-band radars with vertically- and horizontally-directed antenna. This paper aims to describe an algorithm that has been developed to establish relationships between satellite radiances and locations of HIWC regions identified from in-situ measurements of microphysical properties, Doppler velocities, and vertical and horizontal radar reflectivity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C44B..01B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C44B..01B"><span>Improving Estimates of Greenland <span class="hlt">Ice</span> Sheet Surface <span class="hlt">Mass</span> Balance with Satellite Observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Briggs, K.</p> <p>2016-12-01</p> <p><span class="hlt">Mass</span> losses from the Greenland <span class="hlt">Ice</span> Sheet have been accelerating over recent years (e.g. McMillan et al., 2016; Velicogna et al., 2014). This acceleration has predominantly been linked to increasing rates of negative surface <span class="hlt">mass</span> balance, and in particular, increasing <span class="hlt">ice</span> surface melt rates (e.g. McMillan et al., 2016; Velicogna et al., 2014). At the <span class="hlt">ice</span> sheet scale, SMB is assessed using SMB model outputs, which in addition to enabling understanding of the origin of <span class="hlt">mass</span> balance signals, are required as ancillary data in <span class="hlt">mass</span> balance assessments from altimetry and the <span class="hlt">mass</span> budget method. Due to the importance of SMB for <span class="hlt">mass</span> balance over Greenland and the sensitivity of <span class="hlt">mass</span> balance assessments to SMB model outputs, high accuracy of these models is crucial. A critical limiting factor in SMB modeling is however, a lack of in-situ data that is required for model constraint and evaluation. Such data is limited in time and space due to inherent logistical and financial constraints. Remote sensing datasets, being spatially extensive and relatively densely sampled in both space and time, do not suffer such constraints. Here, we show satellite observations of Greenland SMB. McMillan, M., Leeson, A., Shepherd, A., Briggs, K., Armitage, T. W.K., Hogg, A., Kuipers Munneke, P., van den Broeke, M., Noël, B., van de Berg, W., Ligtenberg, S., Horwath, M., Groh, A. , Muir, A. and Gilbert, L. 2016. A high resolution record of Greenland <span class="hlt">Mass</span> Balance. Geophysical Research Letters. 43, doi:10.1002/2016GL069666 Velicogna, I., Sutterley, T. C. and van den Broeke, M. R. 2014. Regional acceleration in <span class="hlt">ice</span> <span class="hlt">mass</span> loss from Greenland and Antarctica using GRACE time-variable gravity data. Geophysical Research Letters. 41, 8130-8137, doi:10.1002/2014GL061052</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040081271','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040081271"><span>A New Way to Measure Cirrus <span class="hlt">Ice</span> Water <span class="hlt">Content</span> by Using <span class="hlt">Ice</span> Raman Scatter with Raman Lidar</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wang, Zhien; Whiteman, David N.; Demoz, Belay; Veselovskii, Igor</p> <p>2004-01-01</p> <p>High and cold cirrus clouds mainly contain irregular <span class="hlt">ice</span> crystals, such as, columns, hexagonal plates, bullet rosettes, and dendrites, and have different impacts on the climate system than low-level clouds, such as stratus, stratocumulus, and cumulus. The radiative effects of cirrus clouds on the current and future climate depend strongly on cirrus cloud microphysical properties including <span class="hlt">ice</span> water <span class="hlt">content</span> (IWC) and <span class="hlt">ice</span> crystal sizes, which are mostly an unknown aspect of cinus clouds. Because of the natural complexity of cirrus clouds and their high locations, it is a challenging task to get them accurately by both remote sensing and in situ sampling. This study presents a new method to remotely sense cirrus microphysical properties by using <span class="hlt">ice</span> Raman scatter with a Raman lidar. The intensity of Raman scattering is fundamentally proportional to the number of molecules involved. Therefore, <span class="hlt">ice</span> Raman scattering signal provides a more direct way to measure IWC than other remote sensing methods. Case studies show that this method has the potential to provide essential information of cirrus microphysical properties to study cloud physical processes in cirrus clouds.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016TCry...10.1259A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016TCry...10.1259A"><span>Greenland <span class="hlt">Ice</span> Sheet seasonal and spatial <span class="hlt">mass</span> variability from model simulations and GRACE (2003-2012)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alexander, Patrick M.; Tedesco, Marco; Schlegel, Nicole-Jeanne; Luthcke, Scott B.; Fettweis, Xavier; Larour, Eric</p> <p>2016-06-01</p> <p>Improving the ability of regional climate models (RCMs) and <span class="hlt">ice</span> sheet models (ISMs) to simulate spatiotemporal variations in the <span class="hlt">mass</span> of the Greenland <span class="hlt">Ice</span> Sheet (GrIS) is crucial for prediction of future sea level rise. While several studies have examined recent trends in GrIS <span class="hlt">mass</span> loss, studies focusing on <span class="hlt">mass</span> variations at sub-annual and sub-basin-wide scales are still lacking. At these scales, processes responsible for <span class="hlt">mass</span> change are less well understood and modeled, and could potentially play an important role in future GrIS <span class="hlt">mass</span> change. Here, we examine spatiotemporal variations in <span class="hlt">mass</span> over the GrIS derived from the Gravity Recovery and Climate Experiment (GRACE) satellites for the January 2003-December 2012 period using a "mascon" approach, with a nominal spatial resolution of 100 km, and a temporal resolution of 10 days. We compare GRACE-estimated <span class="hlt">mass</span> variations against those simulated by the Modèle Atmosphérique Régionale (MAR) RCM and the <span class="hlt">Ice</span> Sheet System Model (ISSM). In order to properly compare spatial and temporal variations in GrIS <span class="hlt">mass</span> from GRACE with model outputs, we find it necessary to spatially and temporally filter model results to reproduce leakage of <span class="hlt">mass</span> inherent in the GRACE solution. Both modeled and satellite-derived results point to a decline (of -178.9 ± 4.4 and -239.4 ± 7.7 Gt yr-1 respectively) in GrIS <span class="hlt">mass</span> over the period examined, but the models appear to underestimate the rate of <span class="hlt">mass</span> loss, especially in areas below 2000 m in elevation, where the majority of recent GrIS <span class="hlt">mass</span> loss is occurring. On an <span class="hlt">ice</span>-sheet-wide scale, the timing of the modeled seasonal cycle of cumulative <span class="hlt">mass</span> (driven by summer <span class="hlt">mass</span> loss) agrees with the GRACE-derived seasonal cycle, within limits of uncertainty from the GRACE solution. However, on sub-<span class="hlt">ice</span>-sheet-wide scales, some areas exhibit significant differences in the timing of peaks in the annual cycle of <span class="hlt">mass</span> change. At these scales, model biases, or processes not accounted for by models related</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005JGRA..110.8103X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005JGRA..110.8103X"><span>An <span class="hlt">ice</span>-cream cone model for coronal <span class="hlt">mass</span> ejections</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xue, X. H.; Wang, C. B.; Dou, X. K.</p> <p>2005-08-01</p> <p>In this study, we use an <span class="hlt">ice</span>-cream cone model to analyze the geometrical and kinematical properties of the coronal <span class="hlt">mass</span> ejections (CMEs). Assuming that in the early phase CMEs propagate with near-constant speed and angular width, some useful properties of CMEs, namely the radial speed (v), the angular width (α), and the location at the heliosphere, can be obtained considering the geometrical shapes of a CME as an <span class="hlt">ice</span>-cream cone. This model is improved by (1) using an <span class="hlt">ice</span>-cream cone to show the near real configuration of a CME, (2) determining the radial speed via fitting the projected speeds calculated from the height-time relation in different azimuthal angles, (3) not only applying to halo CMEs but also applying to nonhalo CMEs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16606711','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16606711"><span>Increasing the protein <span class="hlt">content</span> of <span class="hlt">ice</span> cream.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Patel, M R; Baer, R J; Acharya, M R</p> <p>2006-05-01</p> <p>Vanilla <span class="hlt">ice</span> cream was made with a mix composition of 10.5% milk fat, 10.5% milk SNF, 12% beet sugar, and 4% corn syrup solids. None of the batches made contained stabilizer or emulsifier. The control (treatment 1) contained 3.78% protein. Treatments 2 and 5 contained 30% more protein, treatments 3 and 6 contained 60% more protein, and treatments 4 and 7 contained 90% more protein compared with treatment 1 by addition of whey protein concentrate or milk protein concentrate powders, respectively. In all treatments, levels of milk fat, milk SNF, beet sugar, and corn syrup solids were kept constant at 37% total solids. Mix protein <span class="hlt">content</span> for treatment 1 was 3.78%, treatment 2 was 4.90%, treatment 5 was 4.91%, treatments 3 and 6 were 6.05%, and treatments 4 and 7 were 7.18%. This represented a 29.89, 60.05, 89.95, 29.63, 60.05, and 89.95% increase in protein for treatment 2 through treatment 7 compared with treatment 1, respectively. Milk protein level influenced <span class="hlt">ice</span> crystal size; with increased protein, the <span class="hlt">ice</span> crystal size was favorably reduced in treatments 2, 4, and 5 and was similar in treatments 3, 6, and 7 compared with treatment 1. At 1 wk postmanufacture, overall texture acceptance for all treatments was more desirable compared with treatment 1. When evaluating all parameters, treatment 2 with added whey protein concentrate and treatments 5 and 6 with added milk protein concentrate were similar or improved compared with treatment 1. It is possible to produce acceptable <span class="hlt">ice</span> cream with higher levels of protein.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29540750','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29540750"><span>Recent high-resolution Antarctic <span class="hlt">ice</span> velocity maps reveal increased <span class="hlt">mass</span> loss in Wilkes Land, East Antarctica.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Shen, Qiang; Wang, Hansheng; Shum, C K; Jiang, Liming; Hsu, Hou Tse; Dong, Jinglong</p> <p>2018-03-14</p> <p>We constructed Antarctic <span class="hlt">ice</span> velocity maps from Landsat 8 images for the years 2014 and 2015 at a high spatial resolution (100 m). These maps were assembled from 10,690 scenes of displacement vectors inferred from more than 10,000 optical images acquired from December 2013 through March 2016. We estimated the <span class="hlt">mass</span> discharge of the Antarctic <span class="hlt">ice</span> sheet in 2008, 2014, and 2015 using the Landsat <span class="hlt">ice</span> velocity maps, interferometric synthetic aperture radar (InSAR)-derived <span class="hlt">ice</span> velocity maps (~2008) available from prior studies, and <span class="hlt">ice</span> thickness data. An increased <span class="hlt">mass</span> discharge (53 ± 14 Gt yr -1 ) was found in the East Indian Ocean sector since 2008 due to unexpected widespread glacial acceleration in Wilkes Land, East Antarctica, while the other five oceanic sectors did not exhibit significant changes. However, present-day increased <span class="hlt">mass</span> loss was found by previous studies predominantly in west Antarctica and the Antarctic Peninsula. The newly discovered increased <span class="hlt">mass</span> loss in Wilkes Land suggests that the ocean heat flux may already be influencing <span class="hlt">ice</span> dynamics in the marine-based sector of the East Antarctic <span class="hlt">ice</span> sheet (EAIS). The marine-based sector could be adversely impacted by ongoing warming in the Southern Ocean, and this process may be conducive to destabilization.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1810633W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1810633W"><span><span class="hlt">Ice</span> <span class="hlt">Mass</span> Changes in the Russian High Arctic from Repeat High Resolution Topography.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Willis, Michael; Zheng, Whyjay; Pritchard, Matthew; Melkonian, Andrew; Morin, Paul; Porter, Claire; Howat, Ian; Noh, Myoung-Jong; Jeong, Seongsu</p> <p>2016-04-01</p> <p>We use a combination of ASTER and cartographically derived Digital Elevation Models (DEMs) supplemented with WorldView DEMs, the ArcticDEM and ICESat lidar returns to produce a time-series of <span class="hlt">ice</span> changes occurring in the Russian High Arctic between the mid-20th century and the present. Glaciers on the western, Barents Sea coast of Novaya Zemlya are in a state of general retreat and thinning, while those on the eastern, Kara Sea coast are retreating at a slower rate. Franz Josef Land has a complicated pattern of thinning and thickening, although almost all the thinning is associated with rapid outlet glaciers feeding <span class="hlt">ice</span> shelves. Severnaya Zemlya is also thinning in a complicated manner. A very rapid surging glacier is transferring <span class="hlt">mass</span> into the ocean from the western periphery of the Vavilov <span class="hlt">Ice</span> Cap on October Revolution Island, while glaciers feeding the former Matusevich <span class="hlt">Ice</span> Shelf continue to thin at rates that are faster than those observed during the operational period of ICESat, between 2003 and 2009. Passive microwave studies indicate the total number of melt days is increasing in the Russian Arctic, although much of the melt may refreeze within the firn. It is likely that <span class="hlt">ice</span> dynamic changes will drive <span class="hlt">mass</span> loss for the immediate future. The sub-marine basins beneath several of the <span class="hlt">ice</span> caps in the region suggest the possibility that <span class="hlt">mass</span> loss rates may accelerate in the future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160011350','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160011350"><span>Determining the Water <span class="hlt">Ice</span> <span class="hlt">Content</span> of Martian Regolith by Nonlinear Spectral Mixture Modeling</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gyalay, S.; Noe Dobrea, E. Z.</p> <p>2015-01-01</p> <p>In the search for evidence of life, Icebreaker will drill in to the Martian <span class="hlt">ice</span>-rich regolith to collect samples, which will then be analyzed by an array of instruments designed to identify biomarkers. In addition, drilling into the subsurface will provide the opportunity to assess the vertical distribution of <span class="hlt">ice</span> to a depth of 1 meter. The purpose of this particular project was to understand the uncertainties involved in the use of the imaging system to constrain the water <span class="hlt">ice</span> <span class="hlt">content</span> in regolith samples.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017TCry...11.2773W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017TCry...11.2773W"><span>Satellite-derived submarine melt rates and <span class="hlt">mass</span> balance (2011-2015) for Greenland's largest remaining <span class="hlt">ice</span> tongues</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wilson, Nat; Straneo, Fiammetta; Heimbach, Patrick</p> <p>2017-12-01</p> <p><span class="hlt">Ice</span>-shelf-like floating extensions at the termini of Greenland glaciers are undergoing rapid changes with potential implications for the stability of upstream glaciers and the <span class="hlt">ice</span> sheet as a whole. While submarine melting is recognized as a major contributor to <span class="hlt">mass</span> loss, the spatial distribution of submarine melting and its contribution to the total <span class="hlt">mass</span> balance of these floating extensions is incompletely known and understood. Here, we use high-resolution WorldView satellite imagery collected between 2011 and 2015 to infer the magnitude and spatial variability of melt rates under Greenland's largest remaining <span class="hlt">ice</span> tongues - Nioghalvfjerdsbræ (79 North Glacier, 79N), Ryder Glacier (RG), and Petermann Glacier (PG). Submarine melt rates under the <span class="hlt">ice</span> tongues vary considerably, exceeding 50 m a-1 near the grounding zone and decaying rapidly downstream. Channels, likely originating from upstream subglacial channels, give rise to large melt variations across the <span class="hlt">ice</span> tongues. We compare the total melt rates to the influx of <span class="hlt">ice</span> to the <span class="hlt">ice</span> tongue to assess their contribution to the current <span class="hlt">mass</span> balance. At Petermann Glacier and Ryder Glacier, we find that the combined submarine and aerial melt approximately balances the <span class="hlt">ice</span> flux from the grounded <span class="hlt">ice</span> sheet. At Nioghalvfjerdsbræ the total melt flux (14.2 ± 0.96 km3 a-1 w.e., water equivalent) exceeds the inflow of <span class="hlt">ice</span> (10.2 ± 0.59 km3 a-1 w.e.), indicating present thinning of the <span class="hlt">ice</span> tongue.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhDT........42L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhDT........42L"><span>Surface Energy and <span class="hlt">Mass</span> Balance Model for Greenland <span class="hlt">Ice</span> Sheet and Future Projections</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, Xiaojian</p> <p></p> <p>The Greenland <span class="hlt">Ice</span> Sheet contains nearly 3 million cubic kilometers of glacial <span class="hlt">ice</span>. If the entire <span class="hlt">ice</span> sheet completely melted, sea level would raise by nearly 7 meters. There is thus considerable interest in monitoring the <span class="hlt">mass</span> balance of the Greenland <span class="hlt">Ice</span> Sheet. Each year, the <span class="hlt">ice</span> sheet gains <span class="hlt">ice</span> from snowfall and loses <span class="hlt">ice</span> through iceberg calving and surface melting. In this thesis, we develop, validate and apply a physics based numerical model to estimate current and future surface <span class="hlt">mass</span> balance of the Greenland <span class="hlt">Ice</span> Sheet. The numerical model consists of a coupled surface energy balance and englacial model that is simple enough that it can be used for long time scale model runs, but unlike previous empirical parameterizations, has a physical basis. The surface energy balance model predicts <span class="hlt">ice</span> sheet surface temperature and melt production. The englacial model predicts the evolution of temperature and meltwater within the <span class="hlt">ice</span> sheet. These two models can be combined with estimates of precipitation (snowfall) to estimate the <span class="hlt">mass</span> balance over the Greenland <span class="hlt">Ice</span> Sheet. We first compare model performance with in-situ observations to demonstrate that the model works well. We next evaluate how predictions are degraded when we statistically downscale global climate data. We find that a simple, nearest neighbor interpolation scheme with a lapse rate correction is able to adequately reproduce melt patterns on the Greenland <span class="hlt">Ice</span> Sheet. These results are comparable to those obtained using empirical Positive Degree Day (PDD) methods. Having validated the model, we next drove the <span class="hlt">ice</span> sheet model using the suite of atmospheric model runs available through the CMIP5 atmospheric model inter-comparison, which in turn built upon the RCP 8.5 (business as usual) scenarios. From this exercise we predict how much surface melt production will increase in the coming century. This results in 4-10 cm sea level equivalent, depending on the CMIP5 models. Finally, we try to bound melt water</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1814608M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1814608M"><span>Present and Future Surface <span class="hlt">Mass</span> Budget of Small Arctic <span class="hlt">Ice</span> Caps in a High Resolution Regional Climate Model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mottram, Ruth; Langen, Peter; Koldtoft, Iben; Midefelt, Linnea; Hesselbjerg Christensen, Jens</p> <p>2016-04-01</p> <p>Globally, small <span class="hlt">ice</span> caps and glaciers make a substantial contribution to sea level rise; this is also true in the Arctic. Around Greenland small <span class="hlt">ice</span> caps are surprisingly important to the total <span class="hlt">mass</span> balance from the island as their marginal coastal position means they receive a large amount of precipitation and also experience high surface melt rates. Since small <span class="hlt">ice</span> caps and glaciers have had a disproportionate number of long-term monitoring and observational schemes in the Arctic, likely due to their relative accessibility, they can also be a valuable source of data. However, in climate models the surface <span class="hlt">mass</span> balance contributions are often not distinguished from the main <span class="hlt">ice</span> sheet and the presence of high relief topography is difficult to capture in coarse resolution climate models. At the same time, the diminutive size of marginal <span class="hlt">ice</span> <span class="hlt">masses</span> in comparison to the <span class="hlt">ice</span> sheet makes modelling their <span class="hlt">ice</span> dynamics difficult. Using observational data from the Devon <span class="hlt">Ice</span> Cap in Arctic Canada and the Renland <span class="hlt">Ice</span> Cap in Eastern Greenland, we assess the success of a very high resolution (~5km) regional climate model, HIRHAM5 in capturing the surface <span class="hlt">mass</span> balance (SMB) of these small <span class="hlt">ice</span> caps. The model is forced with ERA-Interim and we compare observed mean SMB and the interannual variability to assess model performance. The steep gradient in topography around Renland is challenging for climate models and additional statistical corrections are required to fit the calculated surface <span class="hlt">mass</span> balance to the high relief topography. Results from a modelling experiment at Renland <span class="hlt">Ice</span> Cap shows that this technique produces a better fit between modelled and observed surface topography. We apply this statistical relationship to modelled SMB on the Devon <span class="hlt">Ice</span> Cap and use the long time series of observations from this glacier to evaluate the model and the smoothed SMB. Measured SMB values from a number of other small <span class="hlt">ice</span> caps including Mittivakkat and A.P. Olsen <span class="hlt">ice</span> cap are also compared</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20150021521&hterms=sea&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dsea','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20150021521&hterms=sea&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dsea"><span>An Assessment of Southern Ocean Water <span class="hlt">Masses</span> and Sea <span class="hlt">Ice</span> During 1988-2007 in a Suite of Interannual CORE-II Simulations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Downes, Stephanie M.; Farneti, Riccardo; Uotila, Petteri; Griffies, Stephen M.; Marsland, Simon J.; Bailey, David; Behrens, Erik; Bentsen, Mats; Bi, Daohua; Biastoch, Arne; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20150021521'); toggleEditAbsImage('author_20150021521_show'); toggleEditAbsImage('author_20150021521_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20150021521_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20150021521_hide"></p> <p>2015-01-01</p> <p>We characterise the representation of the Southern Ocean water <span class="hlt">mass</span> structure and sea <span class="hlt">ice</span> within a suite of 15 global ocean-<span class="hlt">ice</span> models run with the Coordinated Ocean-<span class="hlt">ice</span> Reference Experiment Phase II (CORE-II) protocol. The main focus is the representation of the present (1988-2007) mode and intermediate waters, thus framing an analysis of winter and summer mixed layer depths; temperature, salinity, and potential vorticity structure; and temporal variability of sea <span class="hlt">ice</span> distributions. We also consider the interannual variability over the same 20 year period. Comparisons are made between models as well as to observation-based analyses where available. The CORE-II models exhibit several biases relative to Southern Ocean observations, including an underestimation of the model mean mixed layer depths of mode and intermediate water <span class="hlt">masses</span> in March (associated with greater ocean surface heat gain), and an overestimation in September (associated with greater high latitude ocean heat loss and a more northward winter sea-<span class="hlt">ice</span> extent). In addition, the models have cold and fresh/warm and salty water column biases centred near 50 deg S. Over the 1988-2007 period, the CORE-II models consistently simulate spatially variable trends in sea-<span class="hlt">ice</span> concentration, surface freshwater fluxes, mixed layer depths, and 200-700 m ocean heat <span class="hlt">content</span>. In particular, sea-<span class="hlt">ice</span> coverage around most of the Antarctic continental shelf is reduced, leading to a cooling and freshening of the near surface waters. The shoaling of the mixed layer is associated with increased surface buoyancy gain, except in the Pacific where sea <span class="hlt">ice</span> is also influential. The models are in disagreement, despite the common CORE-II atmospheric state, in their spatial pattern of the 20-year trends in the mixed layer depth and sea-<span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.C21B0585S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.C21B0585S"><span><span class="hlt">Mass</span> Balance of the Northern Antarctic Peninsula and its Ongoing Response to <span class="hlt">Ice</span> Shelf Loss</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Scambos, T. A.; Berthier, E.; Haran, T. M.; Shuman, C. A.; Cook, A. J.; Bohlander, J. A.</p> <p>2012-12-01</p> <p>An assessment of the most rapidly changing areas of the Antarctic Peninsula (north of 66°S) shows that <span class="hlt">ice</span> <span class="hlt">mass</span> loss for the region is dominated by areas affected by eastern-Peninsula <span class="hlt">ice</span> shelf losses in the past 20 years. Little if any of the <span class="hlt">mass</span> loss is compensated by increased snowfall in the northwestern or far northern areas. We combined satellite stereo-image DEM differencing and ICESat-derived along-track elevation changes to measure <span class="hlt">ice</span> <span class="hlt">mass</span> loss for the Antarctic Peninsula north of 66°S between 2001-2010, focusing on the ICESat-1 period of operation (2003-2009). This mapping includes all <span class="hlt">ice</span> drainages affected by recent <span class="hlt">ice</span> shelf loss in the northeastern Peninsula (Prince Gustav, Larsen Inlet, Larsen A, and Larsen B) as well as James Ross Island, Vega Island, Anvers Island, Brabant Island and the adjacent west-flowing glaciers. Polaris Glacier (feeding the Larsen Inlet, which collapsed in 1986) is an exception, and may have stabilized. Our method uses ASTER and SPOT-5 stereo-image DEMs to determine dh/dt for elevations below 800 m; at higher elevations ICESat along-track elevation differencing is used. To adjust along-track path offsets between its 2003-2009 campaigns, we use a recent DEM of the Peninsula to establish and correct for cross-track slope (Cook et al., 2012, doi:10.5194/essdd-5-365-2012; http://nsidc.org/data/nsidc-0516.html) . We reduce the effect of possible seasonal variations in elevation by using only integer-year repeats of the ICESat tracks for comparison. <span class="hlt">Mass</span> losses are dominated by the major glaciers that had flowed into the Prince Gustav (Boydell, Sjorgren, Röhss), Larsen A (Edgeworth, Bombardier, Dinsmoor, Drygalski), and Larsen B (Hektoria, Jorum, and Crane) embayments. The pattern of <span class="hlt">mass</span> loss emphasizes the significant and multi-decadal response to <span class="hlt">ice</span> shelf loss. Areas with shelf losses occurring 30 to 100s of years ago seem to be relatively stable or losing <span class="hlt">mass</span> only slowly (western glaciers, northernmost areas). The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120014297','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120014297"><span>An Iterated Global Mascon Solution with Focus on Land <span class="hlt">Ice</span> <span class="hlt">Mass</span> Evolution</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Luthcke, S. B.; Sabaka, T.; Rowlands, D. D.; Lemoine, F. G.; Loomis, B. D.; Boy, J. P.</p> <p>2012-01-01</p> <p>Land <span class="hlt">ice</span> <span class="hlt">mass</span> evolution is determined from a new GRACE global mascon solution. The solution is estimated directly from the reduction of the inter-satellite K-band range rate observations taking into account the full noise covariance, and formally iterating the solution. The new solution increases signal recovery while reducing the GRACE KBRR observation residuals. The mascons are estimated with 10-day and 1-arc-degree equal area sampling, applying anisotropic constraints for enhanced temporal and spatial resolution of the recovered land <span class="hlt">ice</span> signal. The details of the solution are presented including error and resolution analysis. An Ensemble Empirical Mode Decomposition (EEMD) adaptive filter is applied to the mascon solution time series to compute timing of balance seasons and annual <span class="hlt">mass</span> balances. The details and causes of the spatial and temporal variability of the land <span class="hlt">ice</span> regions studied are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170003991','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170003991"><span>An Assessment of the <span class="hlt">Icing</span> Blade and the SEA Multi-Element Sensor for Liquid Water <span class="hlt">Content</span> Calibration of the NASA GRC <span class="hlt">Icing</span> Research Tunnel</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Steen, Laura E.; Ide, Robert F.; Van Zante, Judith F.</p> <p>2016-01-01</p> <p>The <span class="hlt">Icing</span> Research Tunnel at NASA Glenn has recently switched from using the <span class="hlt">Icing</span> Blade to using the SEA Multi-Element Sensor (also known as the multi-wire) for its calibration of cloud liquid water <span class="hlt">content</span>. In order to peform this transition, tests were completed to compare the Multi-Element Sensor to the <span class="hlt">Icing</span> Blade, particularly with respect to liquid water <span class="hlt">content</span>, airspeed, and drop size. The two instruments were found to compare well for the majority of Appendix C conditions. However, it was discovered that the <span class="hlt">Icing</span> Blade under-measures when the conditions approach the Ludlam Limit. This paper also describes data processing procedures for the Multi-Element Sensor in the IRT, including collision efficiency corrections, mounting underneath a splitter plate, and correcting for a jump in the compensation wire power. Further data is presented to describe the repeatability of the IRT with the Multi-Element Sensor, health-monitoring checks for the instrument, and a sensing-element configuration comparison. Ultimately these tests showed that in the IRT, the multi-wire is a better instrument for measuring cloud liquid water <span class="hlt">content</span> than the blade.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120002071','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120002071"><span>Analysis of Antarctic <span class="hlt">Ice</span>-Sheet <span class="hlt">Mass</span> Balance from ICESat Measurements</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zwally, H. Jay; Li, Jun; Robbins, John; Saba, Jack L.; Yi, Donghui</p> <p>2011-01-01</p> <p>If protoplanets formed from 10 to 20 kilometer diameter planetesimals in a runaway accretion process prior to their oligarchic growth into the terrestrial planets, it is only logical to ask where these planetesimals may have formed in order to assess the initial composition of the Earth. We have used Weidenschilling's model for the formation of comets (1997) to calculate an efficiency factor for the formation of planetesimals from the solar nebula, then used this factor to calculate the feeding zones that contribute to material contained within 10, 15 and 20 kilometer diameter planetesimals at 1 A.V. as a function of nebular <span class="hlt">mass</span>. We find that for all reasonable nebular <span class="hlt">masses</span>, these planetesimals contain a minimum of 3% water as <span class="hlt">ice</span> by <span class="hlt">mass</span>. The fraction of <span class="hlt">ice</span> increases as the planetesimals increase in size and as the nebular <span class="hlt">mass</span> decreases, since both factors increase the feeding zones from which solids in the final planetesimals are drawn. Is there really a problem with the current accretion scenario that makes the Earth too dry, or is it possible that the nascent Earth lost significant quantities of water in the final stages of accretion?</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170000664','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170000664"><span>An Assessment of the <span class="hlt">Icing</span> Blade and the SEA Multi-Element Sensor for Liquid Water <span class="hlt">Content</span> Calibration of the NASA GRC <span class="hlt">Icing</span> Research Tunnel</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Steen, Laura E.; Ide, Robert F.; Van Zante, Judith Foss</p> <p>2017-01-01</p> <p>The <span class="hlt">Icing</span> Research Tunnel at NASA Glenn has recently switched to from using the <span class="hlt">Icing</span> Blade to using the SEA Multi-Element Sensor (also known as the multi-wire) for its calibration of cloud liquid water <span class="hlt">content</span>. In order to perform this transition, tests were completed to compare the Multi-Element Sensor to the <span class="hlt">Icing</span> Blade, particularly with respect to liquid water <span class="hlt">content</span>, airspeed, and drop size. The two instruments were found to compare well for the majority of Appendix C conditions. However, it was discovered that the <span class="hlt">Icing</span> Blade under-measures when the conditions approach the Ludlam Limit. This paper also describes data processing procedures for the Multi-Element Sensor in the IRT, including collection efficiency corrections, mounting underneath a splitter plate, and correcting for a jump in the compensation wire power. Further data is presented to describe the repeatability of the IRT with the Multi-Element sensor, health-monitoring checks for the instrument, and a sensing-element configuration comparison.</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_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li class="active"><span>6</span></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_6 --> <div id="page_7" 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_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li class="active"><span>7</span></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="121"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC43J..06R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC43J..06R"><span>The direct mechanical influence of sea <span class="hlt">ice</span> state on <span class="hlt">ice</span> sheet <span class="hlt">mass</span> loss via iceberg mélange</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Robel, A.</p> <p>2017-12-01</p> <p>The interaction between sea <span class="hlt">ice</span> and land <span class="hlt">ice</span> has typically been considered as a large-scale exchange of moisture, heat and salinity through the ocean and atmosphere. However, recent observations from marine-terminating glaciers in Greenland indicate that the long-term decline of local sea <span class="hlt">ice</span> cover has been accompanied by an increase in nearby iceberg calving and associated <span class="hlt">ice</span> sheet <span class="hlt">mass</span> loss. Near glacier calving fronts, sea <span class="hlt">ice</span> binds icebergs together into an aggregate granular material known as iceberg mélange. Studies have hypothesized that mélange may suppress calving by exerting a mechanical buttressing force directly on the glacier terminus. Here, we show explicitly how sea <span class="hlt">ice</span> thickness and concentration play a critical role in setting the material strength of mélange. To do so, we adapt a discrete element model to simulate mélange as a cohesive granular material. In these simulations, mélange laden with thick, dense, landfast sea <span class="hlt">ice</span> can produce enough resistance to shut down calving at the terminus. When sea <span class="hlt">ice</span> thins, mélange weakens, reducing the mechanical force of mélange on the glacier terminus, and increasing the likelihood of calving. We discuss whether longer periods of sea-<span class="hlt">ice</span>-free conditions in winter may lead to a transition from currently slow calving, predominantly occurring in the summer, to rapid calving, occurring throughout the year. We also discuss the potential role of freshwater discharge in promoting sea <span class="hlt">ice</span> formation in fjords, potentially strengthening mélange.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007E%26PSL.264..391S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007E%26PSL.264..391S"><span>Regional <span class="hlt">ice-mass</span> changes and glacial-isostatic adjustment in Antarctica from GRACE</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sasgen, Ingo; Martinec, Zdeněk; Fleming, Kevin</p> <p>2007-12-01</p> <p>We infer regional <span class="hlt">mass</span> changes in Antarctica using ca. 4 years of Gravity Recovery and Climate Experiment (GRACE) level 2 data. We decompose the time series of the Stokes coefficients into their linear as well as annual and semi-annual components by a least-squares adjustment and apply a statistical reliability test to the Stokes potential-coefficients' linear temporal trends. <span class="hlt">Mass</span> changes in three regions of Antarctica that display prominent geoid-height change are determined by adjusting predictions of glacier melting at the tip of the Antarctic Peninsula and in the Amundsen Sea Sector, and of the glacial-isostatic adjustment (GIA) over the Ronne <span class="hlt">Ice</span> Shelf. We use the GFZ RL04, CNES RL01C, JPL RL04 and CSR RL04 potential-coefficient releases, and show that, although all data sets consistently reflect the prominent <span class="hlt">mass</span> changes, differences in the <span class="hlt">mass</span>-change estimates are considerably larger than the uncertainties estimated by the propagation of the GRACE errors. We then use the bootstrapping method based on the four releases and six time intervals, each with 3.5 years of data, to quantify the variability of the mean <span class="hlt">mass</span>-change estimates. We find 95% of our estimates to lie within 0.08 and 0.09 mm/a equivalent sea-level (ESL) change for the Antarctic Peninsula and within 0.18 and 0.20 mm/a ESL for the Amundsen Sea Sector. Forward modelling of the GIA over the Ronne <span class="hlt">Ice</span> Shelf region suggests that the Antarctic continent was covered by 8.4 to 9.4 m ESL of additional <span class="hlt">ice</span> during the Last-Glacial Maximum (ca. 22 to 15 ka BP). With regards to the mantle-viscosity values and the glacial history used, this value is considered as a minimum estimate. The <span class="hlt">mass</span>-change estimates derived from all GRACE releases and time intervals lie within ca. 20% (Amundsen Sea Sector), 30% (Antarctic Peninsula) and 50% (Ronne <span class="hlt">Ice</span> Shelf region) of the bootstrap-estimated mean, demonstrating the reliability of results obtained using GRACE observations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28362423','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28362423"><span><span class="hlt">Ice</span> Generation and the Heat and <span class="hlt">Mass</span> Transfer Phenomena of Introducing Water to a Cold Bath of Brine.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yun, Xiao; Quarini, Giuseppe L</p> <p>2017-03-13</p> <p>We demonstrate a method for the study of the heat and <span class="hlt">mass</span> transfer and of the freezing phenomena in a subcooled brine environment. Our experiment showed that, under the proper conditions, <span class="hlt">ice</span> can be produced when water is introduced to a bath of cold brine. To make <span class="hlt">ice</span> form, in addition to having the brine and water mix, the rate of heat transfer must bypass that of <span class="hlt">mass</span> transfer. When water is introduced in the form of tiny droplets to the brine surface, the mode of heat and <span class="hlt">mass</span> transfer is by diffusion. The buoyancy stops water from mixing with the brine underneath, but as the <span class="hlt">ice</span> grows thicker, it slows down the rate of heat transfer, making <span class="hlt">ice</span> more difficult to grow as a result. When water is introduced inside the brine in the form of a flow, a number of factors are found to influence how much <span class="hlt">ice</span> can form. Brine temperature and concentration, which are the driving forces of heat and <span class="hlt">mass</span> transfer, respectively, can affect the water-to-<span class="hlt">ice</span> conversion ratio; lower bath temperatures and brine concentrations encourage more <span class="hlt">ice</span> to form. The flow rheology, which can directly affect both the heat and <span class="hlt">mass</span> transfer coefficients, is also a key factor. In addition, the flow rheology changes the area of contact of the flow with the bulk fluid.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GGG....18.2099C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GGG....18.2099C"><span>Short-term variations of Icelandic <span class="hlt">ice</span> cap <span class="hlt">mass</span> inferred from cGPS coordinate time series</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Compton, Kathleen; Bennett, Richard A.; Hreinsdóttir, Sigrún; van Dam, Tonie; Bordoni, Andrea; Barletta, Valentina; Spada, Giorgio</p> <p>2017-06-01</p> <p>As the global climate changes, understanding short-term variations in water storage is increasingly important. Continuously operating Global Positioning System (cGPS) stations in Iceland record annual periodic motion—the elastic response to winter accumulation and spring melt seasons—with peak-to-peak vertical amplitudes over 20 mm for those sites in the Central Highlands. Here for the first time for Iceland, we demonstrate the utility of these cGPS-measured displacements for estimating seasonal and shorter-term <span class="hlt">ice</span> cap <span class="hlt">mass</span> changes. We calculate unit responses to each of the five largest <span class="hlt">ice</span> caps in central Iceland at each of the 62 cGPS locations using an elastic half-space model and estimate <span class="hlt">ice</span> <span class="hlt">mass</span> variations from the cGPS time series using a simple least squares inversion scheme. We utilize all three components of motion, taking advantage of the seasonal motion recorded in the horizontal. We remove secular velocities and accelerations and explore the impact that seasonal motions due to atmospheric, hydrologic, and nontidal ocean loading have on our inversion results. Our results match available summer and winter <span class="hlt">mass</span> balance measurements well, and we reproduce the seasonal stake-based observations of loading and melting within the 1σ confidence bounds of the inversion. We identify nonperiodic <span class="hlt">ice</span> <span class="hlt">mass</span> changes associated with interannual variability in precipitation and other processes such as increased melting due to reduced <span class="hlt">ice</span> surface albedo or decreased melting due to <span class="hlt">ice</span> cap insulation in response to tephra deposition following volcanic eruptions, processes that are not resolved with once or twice-yearly stake measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5426515','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5426515"><span>Sea-level feedback lowers projections of future Antarctic <span class="hlt">Ice</span>-Sheet <span class="hlt">mass</span> loss</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Gomez, Natalya; Pollard, David; Holland, David</p> <p>2015-01-01</p> <p>The stability of marine sectors of the Antarctic <span class="hlt">Ice</span> Sheet (AIS) in a warming climate has been identified as the largest source of uncertainty in projections of future sea-level rise. Sea-level fall near the grounding line of a retreating marine <span class="hlt">ice</span> sheet has a stabilizing influence on the <span class="hlt">ice</span> sheets, and previous studies have established the importance of this feedback on <span class="hlt">ice</span> age AIS evolution. Here we use a coupled <span class="hlt">ice</span> sheet–sea-level model to investigate the impact of the feedback mechanism on future AIS retreat over centennial and millennial timescales for a range of emission scenarios. We show that the combination of bedrock uplift and sea-surface drop associated with <span class="hlt">ice</span>-sheet retreat significantly reduces AIS <span class="hlt">mass</span> loss relative to a simulation without these effects included. Sensitivity analyses show that the stabilization tends to be greatest for lower emission scenarios and Earth models characterized by a thin elastic lithosphere and low-viscosity upper mantle, as is the case for West Antarctica. PMID:26554381</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.H13N..09G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.H13N..09G"><span>Heating the <span class="hlt">Ice</span>-Covered Lakes of the McMurdo Dry Valleys, Antarctica - Decadal Trends in Heat <span class="hlt">Content</span>, <span class="hlt">Ice</span> Thickness, and Heat Exchange</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gooseff, M. N.; Priscu, J. C.; Doran, P. T.; Chiuchiolo, A.; Obryk, M.</p> <p>2014-12-01</p> <p>Lakes integrate landscape processes and climate conditions. Most of the permanently <span class="hlt">ice</span>-covered lakes in the McMurdo Dry Valleys, Antarctica are closed basin, receiving glacial melt water from streams for 10-12 weeks per year. Lake levels rise during the austral summer are balanced by sublimation of <span class="hlt">ice</span> covers (year-round) and evaporation of open water moats (summer only). Vertical profiles of water temperature have been measured in three lakes in Taylor Valley since 1988. Up to 2002, lake levels were dropping, <span class="hlt">ice</span> covers were thickening, and total heat <span class="hlt">contents</span> were decreasing. These lakes have been gaining heat since the mid-2000s, at rates as high as 19.5x1014 cal/decade). Since 2002, lake levels have risen substantially (as much as 2.5 m), and <span class="hlt">ice</span> covers have thinned (1.5 m on average). Analyses of lake <span class="hlt">ice</span> thickness, meteorological conditions, and stream water heat loads indicate that the main source of heat to these lakes is from latent heat released when <span class="hlt">ice</span>-covers form during the winter. An aditional source of heat to the lakes is water inflows from streams and direct glacieal melt. Mean lake temperatures in the past few years have stabilized or cooled, despite increases in lake level and total heat <span class="hlt">content</span>, suggesting increased direct inflow of meltwater from glaciers. These results indicate that McMurdo Dry Valley lakes are sensitive indicators of climate processes in this polar desert landscape and demonstrate the importance of long-term data sets when addressing the effects of climate on ecosystem processes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990071136&hterms=balance+sheet&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dbalance%2Bsheet','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990071136&hterms=balance+sheet&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dbalance%2Bsheet"><span>Large <span class="hlt">Ice</span> Discharge From the Greenland <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rignot, Eric</p> <p>1999-01-01</p> <p>The objectives of this work are to measure the <span class="hlt">ice</span> discharge of the Greenland <span class="hlt">Ice</span> Sheet close to the grounding line and/or calving front, and compare the results with <span class="hlt">mass</span> accumulation and ablation in the interior to estimate the <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150022412','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150022412"><span>Preliminary Flight Deck Observations During Flight in High <span class="hlt">Ice</span> Water <span class="hlt">Content</span> Conditions</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ratvasky, Thomas; Duchanoy, Dominque; Bourdinot, Jean-Francois; Harrah, Steven; Strapp, Walter; Schwarzenboeck, Alfons; Dezitter, Fabien; Grandin, Alice</p> <p>2015-01-01</p> <p>In 2006, Mason et al. identified common observations that occurred in engine power-loss events attributed to flight in high concentrations of <span class="hlt">ice</span> crystals. Observations included light to moderate turbulence, precipitation on the windscreen (often reported as rain), aircraft total temperature anomalies, lack of significant airframe <span class="hlt">icing</span>, and no flight radar echoes at the location and altitude of the engine event. Since 2006, Mason et al. and others have collected information from pilots who experienced engine power-loss events via interviews and questionnaires to substantiate earlier observations and support event analyses. In 2011, Mason and Grzych reported that vertical acceleration data showed increases in turbulence prior to engine events, although the turbulence was usually light to moderate and not unique to high <span class="hlt">ice</span> water <span class="hlt">content</span> (HIWC) clouds. Mason concluded that the observation of rain on the windscreen was due to melting of <span class="hlt">ice</span> high concentrations of <span class="hlt">ice</span> crystals on the windscreen, coalescing into drops. Mason also reported that these pilot observations of rain on the windscreen were varied. Many pilots indicated no rain was observed, while others observed moderate rain with unique impact sounds. Mason concluded that the variation in the reports may be due to variation in the <span class="hlt">ice</span> concentration, particle size, and temperature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20000070393&hterms=3G&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3D3G','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20000070393&hterms=3G&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3D3G"><span>Measuring Greenland <span class="hlt">Ice</span> <span class="hlt">Mass</span> Variation With Gravity Recovery and the Climate Experiment Gravity and GPS</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wu, Xiao-Ping</p> <p>1999-01-01</p> <p>The response of the Greenland <span class="hlt">ice</span> sheet to climate change could significantly alter sea level. The <span class="hlt">ice</span> sheet was much thicker at the last glacial maximum. To gain insight into the global change process and the future trend, it is important to evaluate the <span class="hlt">ice</span> <span class="hlt">mass</span> variation as a function of time and space. The Gravity Recovery and Climate Experiment (GRACE) mission to fly in 2001 for 5 years will measure gravity changes associated with the current <span class="hlt">ice</span> variation and the solid earth's response to past variations. Our objective is to assess the separability of different change sources, accuracy and resolution in the <span class="hlt">mass</span> variation determination by the new gravity data and possible Global Positioning System (GPS) bedrock uplift measurements. We use a reference parameter state that follows a dynamic <span class="hlt">ice</span> model for current <span class="hlt">mass</span> variation and a variant of the Tushingham and Peltier <span class="hlt">ICE</span>-3G deglaciation model for historical deglaciation. The current linear trend is also assumed to have started 5 kyr ago. The Earth model is fixed as preliminary reference Earth model (PREM) with four viscoelastic layers. A discrete Bayesian inverse algorithm is developed employing an isotropic Gaussian a priori covariance function over the <span class="hlt">ice</span> sheet and time. We use data noise predicted by the University of Texas and JPL for major GRACE error sources. A 2 mm/yr uplift uncertainty is assumed for GPS occupation time of 5 years. We then carry out covariance analysis and inverse simulation using GRACE geoid coefficients up to degree 180 in conjunction with a number of GPS uplift rates. Present-day <span class="hlt">ice</span> <span class="hlt">mass</span> variation and historical deglaciation are solved simultaneously over 146 grids of roughly 110 km x 110 km and with 6 time increments of 3 kyr each, along with a common starting epoch of the current trend. For present-day <span class="hlt">ice</span> thickness change, the covariance analysis using GRACE geoid data alone results in a root mean square (RMS) posterior root variance of 2.6 cm/yr, with fairly large a priori</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.7865I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.7865I"><span>On Land <span class="hlt">Ice</span> <span class="hlt">Mass</span> Change in Southernmost South America, Antarctic Peninsula and Coastal Antarctica consistent with GRACE, GPS and Reconstructed <span class="hlt">Ice</span> History for Past 1000 years.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ivins, Erik; Wiese, David; Watkins, Michael; Yuan, Dah-Ning; Landerer, Felix; Simms, Alex; Boening, Carmen</p> <p>2014-05-01</p> <p>The improved spatial coverage provided by high-quality Global Positioning System observing systems on exposed bedrock has allowed these space geodetic experiments to play an increasingly important role in constraining both glacial isostatic adjustment (GIA) processes and viscoelastic responses to present-day glacial <span class="hlt">mass</span> changes (PGMC). Improved constraints on models of <span class="hlt">ice</span> <span class="hlt">mass</span> change in the Southern Hemisphere at present-day, during the Little <span class="hlt">Ice</span> Age, and during the Late Holocene are invaluable for reconciling climate and sea-level variability on a global scale during the present solar radiation forcing and Milankovic orbital configuration. Studies by Jacobs et al. (1992), Whitehouse et al. (2012), King et al. (2012), Boening et al (2012), and others, support the <span class="hlt">contention</span> that GRACE observations of both GIA and PGMC in the Southern Hemisphere are dominated by the geography and climate of coastal environments. This makes the proper masking of those environments for GRACE-determinations of secular <span class="hlt">mass</span> balance especially sensitive, and downscaling, rescaling, and use of correlation mascon methods a non-trivial part of the analysis. Here we employ two analysis methods to determine the <span class="hlt">mass</span> balances of the Antarctic Peninsula and Patagonia and incorporate GPS observations of ongoing uplift for GIA correction into both. Using data that roughly span 2002-2013, we determine -25 ± 5 Gt/yr for the uncorrected Antarctic Peninsula (AP) and -12 Gt/yr for southern Patagonia and the Cordillera Darwin (PCD). With corrections for GIA these are increased to -34 ± 8 Gt/yr for AP and -22 ± 6 Gt/yr for PCD.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.G21B0875K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.G21B0875K"><span>Exploring the effect of East Antarctic <span class="hlt">ice</span> <span class="hlt">mass</span> loss on GIA-induced horizontal bedrock motions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Konfal, S. A.; Whitehouse, P. L.; Hermans, T.; van der Wal, W.; Wilson, T. J.; Bevis, M. G.; Kendrick, E. C.; Dalziel, I.; Smalley, R., Jr.</p> <p>2017-12-01</p> <p><span class="hlt">Ice</span> history inputs used in Antarctic models of GIA include major centers of <span class="hlt">ice</span> <span class="hlt">mass</span> loss in West Antarctica. In the Transantarctic Mountains (TAM) region spanning the boundary between East and West Antarctica, horizontal crustal motions derived from GPS observations from the Antarctic Network (ANET) component of the Polar Earth Observing Network (POLENET) are towards these West Antarctic <span class="hlt">ice</span> <span class="hlt">mass</span> centers, opposite to the pattern of radial crustal motion expected in an unloading scenario. We investigate alternative <span class="hlt">ice</span> history and earth structure inputs to GIA models in an attempt to reproduce observed crustal motions in the region. The W12 <span class="hlt">ice</span> history model is altered to create scenarios including <span class="hlt">ice</span> unloading in the Wilkes Subglacial Basin based on available glaciological records. These altered <span class="hlt">ice</span> history models, along with the unmodified W12 <span class="hlt">ice</span> history model, are coupled with 60 radially varying (1D) earth model combinations, including approximations of optimal earth profiles identified in published GIA models. The resulting model-predicted motions utilizing both the modified and unmodified <span class="hlt">ice</span> history models fit ANET GPS-derived crustal motions in the northern TAM region for a suite of earth model combinations. Further south, where the influence of simulated Wilkes unloading is weakest and West Antarctic unloading is strongest, observed and predicted motions do not agree. The influence of simulated Wilkes <span class="hlt">ice</span> unloading coupled with laterally heterogeneous earth models is also investigated. The resulting model-predicted motions do not differ significantly between the original W12 and W12 with simulated Wilkes unloading <span class="hlt">ice</span> histories.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014TCry....8..743G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014TCry....8..743G"><span>Empirical estimation of present-day Antarctic glacial isostatic adjustment and <span class="hlt">ice</span> <span class="hlt">mass</span> change</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gunter, B. C.; Didova, O.; Riva, R. E. M.; Ligtenberg, S. R. M.; Lenaerts, J. T. M.; King, M. A.; van den Broeke, M. R.; Urban, T.</p> <p>2014-04-01</p> <p>This study explores an approach that simultaneously estimates Antarctic <span class="hlt">mass</span> balance and glacial isostatic adjustment (GIA) through the combination of satellite gravity and altimetry data sets. The results improve upon previous efforts by incorporating a firn densification model to account for firn compaction and surface processes as well as reprocessed data sets over a slightly longer period of time. A range of different Gravity Recovery and Climate Experiment (GRACE) gravity models were evaluated and a new <span class="hlt">Ice</span>, Cloud, and Land Elevation Satellite (ICESat) surface height trend map computed using an overlapping footprint approach. When the GIA models created from the combination approach were compared to in situ GPS ground station displacements, the vertical rates estimated showed consistently better agreement than recent conventional GIA models. The new empirically derived GIA rates suggest the presence of strong uplift in the Amundsen Sea sector in West Antarctica (WA) and the Philippi/Denman sectors, as well as subsidence in large parts of East Antarctica (EA). The total GIA-related <span class="hlt">mass</span> change estimates for the entire Antarctic <span class="hlt">ice</span> sheet ranged from 53 to 103 Gt yr-1, depending on the GRACE solution used, with an estimated uncertainty of ±40 Gt yr-1. Over the time frame February 2003-October 2009, the corresponding <span class="hlt">ice</span> <span class="hlt">mass</span> change showed an average value of -100 ± 44 Gt yr-1 (EA: 5 ± 38, WA: -105 ± 22), consistent with other recent estimates in the literature, with regional <span class="hlt">mass</span> loss mostly concentrated in WA. The refined approach presented in this study shows the contribution that such data combinations can make towards improving estimates of present-day GIA and <span class="hlt">ice</span> <span class="hlt">mass</span> change, particularly with respect to determining more reliable uncertainties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..44.7328C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..44.7328C"><span><span class="hlt">Mass</span> balance reassessment of glaciers draining into the Abbot and Getz <span class="hlt">Ice</span> Shelves of West Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chuter, S. J.; Martín-Español, A.; Wouters, B.; Bamber, J. L.</p> <p>2017-07-01</p> <p>We present a reassessment of input-output method <span class="hlt">ice</span> <span class="hlt">mass</span> budget estimates for the Abbot and Getz regions of West Antarctica using CryoSat-2-derived <span class="hlt">ice</span> thickness estimates. The <span class="hlt">mass</span> budget is 8 ± 6 Gt yr-1 and 5 ± 17 Gt yr-1 for the Abbot and Getz sectors, respectively, for the period 2006-2008. Over the Abbot region, our results resolve a previous discrepancy with elevation rates from altimetry, due to a previous 30% overestimation of <span class="hlt">ice</span> thickness. For the Getz sector, our results are at the more positive bound of estimates from other techniques. Grounding line velocity increases up to 20% between 2007 and 2014 alongside mean elevation rates of -0.67 ± 0.13 m yr-1 between 2010 and 2013 indicate the onset of a dynamic thinning signal. Mean snowfall trends of -0.33 m yr-1 water equivalent since 2006 indicate recent <span class="hlt">mass</span> trends are driven by both <span class="hlt">ice</span> dynamics and surface processes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1918364H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1918364H"><span>Sea <span class="hlt">Ice</span> <span class="hlt">Mass</span> Balance Buoys (IMBs): First Results from a Data Processing Intercomparison Study</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hoppmann, Mario; Tiemann, Louisa; Itkin, Polona</p> <p>2017-04-01</p> <p>IMBs are autonomous instruments able to continuously monitor the growth and melt of sea <span class="hlt">ice</span> and its snow cover at a single point on an <span class="hlt">ice</span> floe. Complementing field expeditions, remote sensing observations and modelling studies, these in-situ data are crucial to assess the <span class="hlt">mass</span> balance and seasonal evolution of sea <span class="hlt">ice</span> and snow in the polar oceans. Established subtypes of IMBs combine coarse-resolution temperature profiles through air, snow, <span class="hlt">ice</span> and ocean with ultrasonic pingers to detect snow accumulation and <span class="hlt">ice</span> thermodynamic growth. Recent technological advancements enable the use of high-resolution temperature chains, which are also able to identify the surrounding medium through a „heating cycle". The temperature change during this heating cycle provides additional information on the internal properties and processes of the <span class="hlt">ice</span>. However, a unified data processing technique to reliably and accurately determine sea <span class="hlt">ice</span> thickness and snow depth from this kind of data is still missing, and an unambiguous interpretation remains a challenge. Following the need to improve techniques for remotely measuring sea <span class="hlt">ice</span> <span class="hlt">mass</span> balance, an international IMB working group has recently been established. The main goals are 1) to coordinate IMB deployments, 2) to enhance current IMB data processing and -interpretation techniques, and 3) to provide standardized IMB data products to a broader community. Here we present first results from two different data processing algorithms, applied to selected IMB datasets from the Arctic and Antarctic. Their performance with regard to sea <span class="hlt">ice</span> thickness and snow depth retrieval is evaluated, and an uncertainty is determined. Although several challenges and caveats in IMB data processing and -interpretation are found, such datasets bear great potential and yield plenty of useful information about sea <span class="hlt">ice</span> properties and processes. It is planned to include many more algorithms from contributors within the working group, and we explicitly invite</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26672555','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26672555"><span>Spatial and temporal distribution of <span class="hlt">mass</span> loss from the Greenland <span class="hlt">Ice</span> Sheet since AD 1900.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kjeldsen, Kristian K; Korsgaard, Niels J; Bjørk, Anders A; Khan, Shfaqat A; Box, Jason E; Funder, Svend; Larsen, Nicolaj K; Bamber, Jonathan L; Colgan, William; van den Broeke, Michiel; Siggaard-Andersen, Marie-Louise; Nuth, Christopher; Schomacker, Anders; Andresen, Camilla S; Willerslev, Eske; Kjær, Kurt H</p> <p>2015-12-17</p> <p>The response of the Greenland <span class="hlt">Ice</span> Sheet (GIS) to changes in temperature during the twentieth century remains contentious, largely owing to difficulties in estimating the spatial and temporal distribution of <span class="hlt">ice</span> <span class="hlt">mass</span> changes before 1992, when Greenland-wide observations first became available. The only previous estimates of change during the twentieth century are based on empirical modelling and energy balance modelling. Consequently, no observation-based estimates of the contribution from the GIS to the global-mean sea level budget before 1990 are included in the Fifth Assessment Report of the Intergovernmental Panel on Climate Change. Here we calculate spatial <span class="hlt">ice</span> <span class="hlt">mass</span> loss around the entire GIS from 1900 to the present using aerial imagery from the 1980s. This allows accurate high-resolution mapping of geomorphic features related to the maximum extent of the GIS during the Little <span class="hlt">Ice</span> Age at the end of the nineteenth century. We estimate the total <span class="hlt">ice</span> <span class="hlt">mass</span> loss and its spatial distribution for three periods: 1900-1983 (75.1 ± 29.4 gigatonnes per year), 1983-2003 (73.8 ± 40.5 gigatonnes per year), and 2003-2010 (186.4 ± 18.9 gigatonnes per year). Furthermore, using two surface <span class="hlt">mass</span> balance models we partition the <span class="hlt">mass</span> balance into a term for surface <span class="hlt">mass</span> balance (that is, total precipitation minus total sublimation minus runoff) and a dynamic term. We find that many areas currently undergoing change are identical to those that experienced considerable thinning throughout the twentieth century. We also reveal that the surface <span class="hlt">mass</span> balance term shows a considerable decrease since 2003, whereas the dynamic term is constant over the past 110 years. Overall, our observation-based findings show that during the twentieth century the GIS contributed at least 25.0 ± 9.4 millimetres of global-mean sea level rise. Our result will help to close the twentieth-century sea level budget, which remains crucial for evaluating the reliability of models used to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015Natur.528..396K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015Natur.528..396K"><span>Spatial and temporal distribution of <span class="hlt">mass</span> loss from the Greenland <span class="hlt">Ice</span> Sheet since AD 1900</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kjeldsen, Kristian K.; Korsgaard, Niels J.; Bjørk, Anders A.; Khan, Shfaqat A.; Box, Jason E.; Funder, Svend; Larsen, Nicolaj K.; Bamber, Jonathan L.; Colgan, William; van den Broeke, Michiel; Siggaard-Andersen, Marie-Louise; Nuth, Christopher; Schomacker, Anders; Andresen, Camilla S.; Willerslev, Eske; Kjær, Kurt H.</p> <p>2015-12-01</p> <p>The response of the Greenland <span class="hlt">Ice</span> Sheet (GIS) to changes in temperature during the twentieth century remains contentious, largely owing to difficulties in estimating the spatial and temporal distribution of <span class="hlt">ice</span> <span class="hlt">mass</span> changes before 1992, when Greenland-wide observations first became available. The only previous estimates of change during the twentieth century are based on empirical modelling and energy balance modelling. Consequently, no observation-based estimates of the contribution from the GIS to the global-mean sea level budget before 1990 are included in the Fifth Assessment Report of the Intergovernmental Panel on Climate Change. Here we calculate spatial <span class="hlt">ice</span> <span class="hlt">mass</span> loss around the entire GIS from 1900 to the present using aerial imagery from the 1980s. This allows accurate high-resolution mapping of geomorphic features related to the maximum extent of the GIS during the Little <span class="hlt">Ice</span> Age at the end of the nineteenth century. We estimate the total <span class="hlt">ice</span> <span class="hlt">mass</span> loss and its spatial distribution for three periods: 1900-1983 (75.1 ± 29.4 gigatonnes per year), 1983-2003 (73.8 ± 40.5 gigatonnes per year), and 2003-2010 (186.4 ± 18.9 gigatonnes per year). Furthermore, using two surface <span class="hlt">mass</span> balance models we partition the <span class="hlt">mass</span> balance into a term for surface <span class="hlt">mass</span> balance (that is, total precipitation minus total sublimation minus runoff) and a dynamic term. We find that many areas currently undergoing change are identical to those that experienced considerable thinning throughout the twentieth century. We also reveal that the surface <span class="hlt">mass</span> balance term shows a considerable decrease since 2003, whereas the dynamic term is constant over the past 110 years. Overall, our observation-based findings show that during the twentieth century the GIS contributed at least 25.0 ± 9.4 millimetres of global-mean sea level rise. Our result will help to close the twentieth-century sea level budget, which remains crucial for evaluating the reliability of models used to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.A23A0185Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A23A0185Y"><span>Combining In-situ Measurements, Passive Satellite Imagery, and Active Radar Retrievals for the Detection of High <span class="hlt">Ice</span> Water <span class="hlt">Content</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yost, C. R.; Minnis, P.; Bedka, K. M.; Nguyen, L.; Palikonda, R.; Spangenberg, D.; Strapp, J. W.; Delanoë, J.; Protat, A.</p> <p>2016-12-01</p> <p>At least one hundred jet engine power loss events since the 1990s have been attributed to the phenomenon known as <span class="hlt">ice</span> crystal <span class="hlt">icing</span> (ICI). Ingestion of high concentrations of <span class="hlt">ice</span> particles into aircraft engines is thought to cause these events, but it is clear that the use of current on-board weather radar systems alone is insufficient for detecting conditions that might cause ICI. Passive radiometers in geostationary orbit are valuable for monitoring systems that produce high <span class="hlt">ice</span> water <span class="hlt">content</span> (HIWC) and will play an important role in nowcasting, but are incapable of making vertically resolved measurements of <span class="hlt">ice</span> particle concentration, i.e., <span class="hlt">ice</span> water <span class="hlt">content</span> (IWC). Combined radar, lidar, and in-situ measurements are essential for developing a skilled satellite-based HIWC nowcasting technique. The High Altitude <span class="hlt">Ice</span> Crystals - High <span class="hlt">Ice</span> Water <span class="hlt">Content</span> (HAIC-HIWC) field campaigns in Darwin, Australia, and Cayenne, French Guiana, have produced a valuable dataset of in-situ total water <span class="hlt">content</span> (TWC) measurements with which to study conditions that produce HIWC. The NASA Langley Satellite ClOud and Radiative Property retrieval System (SatCORPS) was used to derive cloud physical and optical properties such cloud top height, temperature, optical depth, and <span class="hlt">ice</span> water path from multi-spectral satellite imagery acquired throughout the HAIC-HIWC campaigns. These cloud properties were collocated with the in-situ TWC measurements in order to characterize cloud properties in the vicinity of HIWC. Additionally, a database of satellite-derived overshooting cloud top (OT) detections was used to identify TWC measurements in close proximity to convective cores likely producing large concentrations of <span class="hlt">ice</span> crystals. Certain cloud properties show some sensitivity to increasing TWC and a multivariate probabilistic indicator of HIWC was developed from these datasets. This paper describes the algorithm development and demonstrates the HIWC indicator with imagery from the HAIC</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EPSC...11.1010K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EPSC...11.1010K"><span>Reproducing impact ionization <span class="hlt">mass</span> spectra of E and F ring <span class="hlt">ice</span> grains at different impact speeds</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Klenner, F.; Reviol, R.; Postberg, F.</p> <p>2017-09-01</p> <p>As impact speeds of E and F ring <span class="hlt">ice</span> grains impinging onto the target of impact ionization <span class="hlt">mass</span> spectrometers in space can vary greatly, the resulting cationic or anionic <span class="hlt">mass</span> spectra can have very different appearances. The <span class="hlt">mass</span> spectra can be accurately reproduced with an analog experimental setup IR-FL-MALDI-ToF-MS (Infrared Free Liquid Matrix Assisted Laser Desorption and Ionization Time of Flight <span class="hlt">Mass</span> Spectrometry). We compare <span class="hlt">mass</span> spectra of E and F ring <span class="hlt">ice</span> grains taken by the Cosmic Dust Analyzer (CDA) onboard Cassini recorded at different impact speeds with our analog spectra and prove the capability of the analog experiment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C41E0728S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C41E0728S"><span>On the Utilization of <span class="hlt">Ice</span> Flow Models and Uncertainty Quantification to Interpret the Impact of Surface Radiation Budget Errors on Estimates of Greenland <span class="hlt">Ice</span> Sheet Surface <span class="hlt">Mass</span> Balance and Regional Estimates of <span class="hlt">Mass</span> Balance</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schlegel, N.; Larour, E. Y.; Gardner, A. S.; Lang, C.; Miller, C. E.; van den Broeke, M. R.</p> <p>2016-12-01</p> <p>How Greenland <span class="hlt">ice</span> flow may respond to future increases in surface runoff and to increases in the frequency of extreme melt events is unclear, as it requires detailed comprehension of Greenland surface climate and the <span class="hlt">ice</span> sheet's sensitivity to associated uncertainties. With established uncertainty quantification tools run within the framework of <span class="hlt">Ice</span> Sheet System Model (ISSM), we conduct decadal-scale forward modeling experiments to 1) quantify the spatial resolution needed to effectively force distinct components of the surface radiation budget, and subsequently surface <span class="hlt">mass</span> balance (SMB), in various regions of the <span class="hlt">ice</span> sheet and 2) determine the dynamic response of Greenland <span class="hlt">ice</span> flow to variations in components of the net radiation budget. The Glacier Energy and <span class="hlt">Mass</span> Balance (GEMB) software is a column surface model (1-D) that has recently been embedded as a module within ISSM. Using the ISSM-GEMB framework, we perform sensitivity analyses to determine how perturbations in various components of the surface radiation budget affect model output; these model experiments allow us predict where and on what spatial scale the <span class="hlt">ice</span> sheet is likely to dynamically respond to changes in these parameters. Preliminary results suggest that SMB should be forced at at least a resolution of 23 km to properly capture dynamic <span class="hlt">ice</span> response. In addition, Monte-Carlo style sampling analyses reveals that the areas with the largest uncertainty in <span class="hlt">mass</span> flux are located near the equilibrium line altitude (ELA), upstream of major outlet glaciers in the North and West of the <span class="hlt">ice</span> sheet. Sensitivity analysis indicates that these areas are also the most vulnerable on the <span class="hlt">ice</span> sheet to persistent, far-field shifts in SMB, suggesting that continued warming, and upstream shift in the ELA, are likely to result in increased velocities, and consequentially SMB-induced thinning upstream of major outlet glaciers. Here, we extend our investigation to consider various components of the surface radiation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JPhCS.718e2017G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JPhCS.718e2017G"><span>Measurement of the Muon <span class="hlt">Content</span> of Air Showers with <span class="hlt">Ice</span>Top</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gonzalez, JG; <author pre="for ">IceCube Collaboration</p> <p>2016-05-01</p> <p><span class="hlt">Ice</span>Top, the surface component of the <span class="hlt">Ice</span>Cube detector, has measured the energy spectrum of cosmic ray primaries in the range between 1.6 PeV and 1.3 EeV. <span class="hlt">Ice</span>Top can also be used to measure the average density of GeV muons in the shower front at large radial distances (> 300 m) from the shower axis. Wei present the measurement of the muon lateral distribution function for primary cosmic rays with energies between 1.6 PeV and about 0.1 EeV, and compare it to proton and iron simulations. We also discuss how this information can be exploited in the reconstruction of single air shower events. By combining the information on the muon component with that of the electromagnetic component of the air shower, we expect to reduce systematic uncertainties in the inferred <span class="hlt">mass</span> composition of cosmic rays arising from theoretical uncertainties in hadronic interaction 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_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li class="active"><span>7</span></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_7 --> <div id="page_8" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="141"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.A42F..02Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A42F..02Z"><span>Bimodality and variability of particle size distributions in high <span class="hlt">Ice</span> Water <span class="hlt">Content</span> regions and their implications for microphysical models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhu, S.; McFarquhar, G. M.; Leroy, D.; Korolev, A.; Schwarzenboeck, A.; Wu, W.; Strapp, J. W.</p> <p>2016-12-01</p> <p>Aviation records since the 1990s indicate that aircraft engines are facing a threat of occasional power loss due to <span class="hlt">ice</span> ingestion over tropical oceanic convective clouds. The typical absence of radar echoes greater than 30 dBZ during such incidents suggests the existence of large amounts of small <span class="hlt">ice</span> particles. The industrial aviation safety concerns inspired the High Altitude <span class="hlt">Ice</span> Crystals / High <span class="hlt">Ice</span> Water <span class="hlt">Content</span> (HAIC/HIWC) campaign, whose Phase I was conducted between January and March 2014. A 2-D Stereo (2DS) probe, Precipitation Imaging Probe (PIP) and Isokinetic Evaporator Probe were installed on the French Falcon 20 making in-situ observations off the coast of Darwin, Australia. Composite particle size distributions (PSDs) using 2DS and PIP data were derived for each 5 second period in cloud. Using an automated technique to identify multiple modes in PSDs and an Incomplete Gamma Fit technique, the intercept (N0), slope (λ) and shape parameter (μ) of each mode of a gamma distribution were determined. The variation of PSDs and fit parameters for <span class="hlt">Ice</span> Water <span class="hlt">Contents</span> (IWCs) > 1.5 g m-3 with cloud and environmental parameters and their differences from PSDs measured outside of high IWC conditions are summarized here. Two types of HIWC conditions were observed, according to whether the median <span class="hlt">mass</span> diameters (MMD) were positively or negatively correlated with IWC. The principal findings about high IWC regions are as follows: 1) larger μ and N0 are found in high IWC regions while λ tends to remain unchanged; 2) PSDs are more likely to be bimodal at lower temperatures. 3) Positive MMD-IWC correlations are associated with larger μ and smaller N0; 4) Bimodal distributions are more frequent for positive MMD-IWC correlations; and 5) Positive MMD-IWC correlations are usually associated with longer-aged clouds, but there are exceptions, showing other factors affect the occurrence of frequent small particles in high IWC regions. Implications for modeling of high IWC</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150000279','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150000279"><span>A Range Correction for Icesat and Its Potential Impact on <span class="hlt">Ice</span>-sheet <span class="hlt">Mass</span> Balance Studies</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Borsa, A. A.; Moholdt, G.; Fricker, H. A.; Brunt, Kelly M.</p> <p>2014-01-01</p> <p>We report on a previously undocumented range error in NASA's <span class="hlt">Ice</span>, Cloud and land Elevation Satellite (ICESat) that degrades elevation precision and introduces a small but significant elevation trend over the ICESat mission period. This range error (the Gaussian-Centroid or 'G-C'offset) varies on a shot-to-shot basis and exhibits increasing scatter when laser transmit energies fall below 20 mJ. Although the G-C offset is uncorrelated over periods less than1 day, it evolves over the life of each of ICESat's three lasers in a series of ramps and jumps that give rise to spurious elevation trends of -0.92 to -1.90 cm yr(exp -1), depending on the time period considered. Using ICESat data over the Ross and Filchner-Ronne <span class="hlt">ice</span> shelves we show that (1) the G-C offset introduces significant biases in <span class="hlt">ice</span>-shelf <span class="hlt">mass</span> balance estimates, and (2) the <span class="hlt">mass</span> balance bias can vary between regions because of different temporal samplings of ICESat.We can reproduce the effect of the G-C offset over these two <span class="hlt">ice</span> shelves by fitting trends to sample-weighted mean G-C offsets for each campaign, suggesting that it may not be necessary to fully repeat earlier ICESat studies to determine the impact of the G-C offset on <span class="hlt">ice</span>-sheet <span class="hlt">mass</span> balance estimates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150019654','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150019654"><span>An Assessment of the SEA Multi-Element Sensor for Liquid Water <span class="hlt">Content</span> Calibration of the NASA GRC <span class="hlt">Icing</span> Research Tunnel</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Steen, Laura E.; Ide, Robert F.; Van Zante, Judith F.</p> <p>2015-01-01</p> <p>The NASA Glenn <span class="hlt">Icing</span> Research tunnel has been using an <span class="hlt">Icing</span> Blade technique to measure cloud liquid water <span class="hlt">content</span> (LWC) since 1980. The IRT conducted tests with SEA Multi-Element sensors from 2009 to 2011 to assess their performance in measuring LWC. These tests revealed that the Multi-Element sensors showed some significant advantages over the <span class="hlt">Icing</span> Blade, particularly at higher water <span class="hlt">contents</span>, higher impingement rates, and large drop sizes. Results of these and other tests are presented here.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013JGRF..118..667S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JGRF..118..667S"><span>Decadal-scale sensitivity of Northeast Greenland <span class="hlt">ice</span> flow to errors in surface <span class="hlt">mass</span> balance using ISSM</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schlegel, N.-J.; Larour, E.; Seroussi, H.; Morlighem, M.; Box, J. E.</p> <p>2013-06-01</p> <p>The behavior of the Greenland <span class="hlt">Ice</span> Sheet, which is considered a major contributor to sea level changes, is best understood on century and longer time scales. However, on decadal time scales, its response is less predictable due to the difficulty of modeling surface climate, as well as incomplete understanding of the dynamic processes responsible for <span class="hlt">ice</span> flow. Therefore, it is imperative to understand how modeling advancements, such as increased spatial resolution or more comprehensive <span class="hlt">ice</span> flow equations, might improve projections of <span class="hlt">ice</span> sheet response to climatic trends. Here we examine how a finely resolved climate forcing influences a high-resolution <span class="hlt">ice</span> stream model that considers longitudinal stresses. We simulate <span class="hlt">ice</span> flow using a two-dimensional Shelfy-Stream Approximation implemented within the <span class="hlt">Ice</span> Sheet System Model (ISSM) and use uncertainty quantification tools embedded within the model to calculate the sensitivity of <span class="hlt">ice</span> flow within the Northeast Greenland <span class="hlt">Ice</span> Stream to errors in surface <span class="hlt">mass</span> balance (SMB) forcing. Our results suggest that the model tends to smooth <span class="hlt">ice</span> velocities even when forced with extreme errors in SMB. Indeed, errors propagate linearly through the model, resulting in discharge uncertainty of 16% or 1.9 Gt/yr. We find that <span class="hlt">mass</span> flux is most sensitive to local errors but is also affected by errors hundreds of kilometers away; thus, an accurate SMB map of the entire basin is critical for realistic simulation. Furthermore, sensitivity analyses indicate that SMB forcing needs to be provided at a resolution of at least 40 km.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.P53H..07W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.P53H..07W"><span><span class="hlt">Mass</span> Fluxes of <span class="hlt">Ice</span> and Oxygen Across the Entire Lid of Lake Vostok from Observations of Englacial Radiowave Attenuation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Winebrenner, D. P.; Kintner, P. M. S.; MacGregor, J. A.</p> <p>2017-12-01</p> <p>Over deep Antarctic subglacial lakes, spatially varying <span class="hlt">ice</span> thickness and the pressure-dependent melting point of <span class="hlt">ice</span> result in areas of melting and accretion at the <span class="hlt">ice</span>-water interface, i.e., the lake lid. These <span class="hlt">ice</span> <span class="hlt">mass</span> fluxes drive lake circulation and, because basal Antarctic <span class="hlt">ice</span> contains air-clathrate, affect the input of oxygen to the lake, with implications for subglacial life. Inferences of melting and accretion from radar-layer tracking and geodesy are limited in spatial coverage and resolution. Here we develop a new method to estimate rates of accretion, melting, and the resulting oxygen input at a lake lid, using airborne radar data over Lake Vostok together with <span class="hlt">ice</span>-temperature and chemistry data from the Vostok <span class="hlt">ice</span> core. Because the lake lid is a coherent reflector of known reflectivity (at our radar frequency), we can infer depth-averaged radiowave attenuation in the <span class="hlt">ice</span>, with spatial resolution 1 km along flight lines. Spatial variation in attenuation depends mostly on variation in <span class="hlt">ice</span> temperature near the lid, which in turn varies strongly with <span class="hlt">ice</span> <span class="hlt">mass</span> flux at the lid. We model <span class="hlt">ice</span> temperature versus depth with <span class="hlt">ice</span> <span class="hlt">mass</span> flux as a parameter, thus linking that flux to (observed) depth-averaged attenuation. The resulting map of melt- and accretion-rates independently reproduces features known from earlier studies, but now covers the entire lid. We find that accretion is dominant when integrated over the lid, with an <span class="hlt">ice</span> imbalance of 0.05 to 0.07 km3 a-1, which is robust against uncertainties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C33D1227B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C33D1227B"><span>Modelling the contribution of supraglacial <span class="hlt">ice</span> cliffs to the <span class="hlt">mass</span>-balance of glaciers in the Langtang catchment, Nepalese Himalaya</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Buri, P.; Steiner, J. F.; Miles, E.; Ragettli, S.; Pellicciotti, F.</p> <p>2017-12-01</p> <p>Supraglacial cliffs are typical surface features of debris-covered glaciers worldwide, affecting surface evolution, and <span class="hlt">mass</span> balance by providing a direct <span class="hlt">ice</span>-atmosphere interface where melt rates can be very high. As a result, <span class="hlt">ice</span> cliffs act as windows of energy transfer from the atmosphere to the <span class="hlt">ice</span>, and enhance melt and <span class="hlt">mass</span> losses of otherwise insulated <span class="hlt">ice</span>. However, their contribution to glacier <span class="hlt">mass</span> balance has never been quantified at the glacier scale, and all inference has been obtained from upscaling results of point-scale models or observations at select individual cliffs. Here we use a 3D, physically-based backwasting model to estimate the volume losses associated with the melting and backwasting of supraglacial <span class="hlt">ice</span> cliffs for the entire debris-covered glacier area of the Langtang catchment. We estimate <span class="hlt">mass</span> losses for the 2014 melt season and compare them to recent values of glacier <span class="hlt">mass</span> balance determined from geodetic and numerical modelling approached. Cliff outlines and topography are derived from high-resolution stereo SPOT6-imagery from April 2014. Meteorological data to force the model are provided by automatic weather stations on- and off-glacier within the valley. The model simulates <span class="hlt">ice</span> cliff backwasting by considering the cliff-atmosphere energy-balance, reburial by debris and the effects of adjacent ponds. In the melt season of 2014, cliffs' distribution and patterns of <span class="hlt">mass</span> losses vary considerably from glacier to glacier, and we relate rates of volume loss to both glaciers' and cliffs' characteristics. Only cliffs with a northerly aspect account for substantial losses. Uncertainty in our estimates is due to the quality of the stereo DEM, uncertainties in the cliff delineation and the fact that we use a conservative approach to cliff delineation and discard very small cliffs and those for which uncertainty in topography is high. Despite these uncertainties, our work presents the first estimate of the importance of supraglacial <span class="hlt">ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19810068727','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19810068727"><span>The Calculated and Measured Performance Characteristics of a Heated-Wire Liquid-Water-<span class="hlt">Content</span> Meter for Measuring <span class="hlt">Icing</span> Severity</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Neel, Carr B.; Steinmetz, Charles P.</p> <p>1952-01-01</p> <p>Ground tests have been made of an instrument which, when assembled in a more compact form for flight installation, could be used to obtain statistical flight data on the liquid-water <span class="hlt">content</span> of <span class="hlt">icing</span> clouds and to provide an indication of <span class="hlt">icing</span> severity. The sensing element of the instrument consists of an electrically heated wire which is mounted in the air stream. The degree of cooling of the wire resulting from evaporation of the impinging water droplets is a measure. of the liquid-water <span class="hlt">content</span> of the cloud. Determination of the value of the liquid-water <span class="hlt">content</span> from the wire temperature at any instant requires a knowledge of the airspeed, altitude, and air temperature. An analysis was made of the temperature response of a heated wire exposed to an air stream containing water drops. Comparisons were made of the liquid-water <span class="hlt">content</span> as measured with several heated wires and absorbent cylinders in an artificially produced cloud. For one of the wires, comparative tests were made with a rotating-disk <span class="hlt">icing</span>-rate meter in an <span class="hlt">icing</span> wind tunnel. From the test results, it was shown that an instrument for measuring the concentration of liquid water in an air stream can be built using an electrically heated wire of known temperatureresistance characteristics, and that the performance of such a device can be predicted using appropriate theory. Although an instrument in a form suitable for gathering statistical data in flight was not built, the practicability of constructing such an instrument was illustrated. The ground-test results indicated that a flight heated-wire instrument would be simple and durable, would respond rapidly to variations in liquid-water <span class="hlt">content</span>, and could be used for the measurement of water <span class="hlt">content</span> in clouds which are above freezing temperature, as well as in <span class="hlt">icing</span> clouds.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.G44A..04H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.G44A..04H"><span>Earth Structure, <span class="hlt">Ice</span> <span class="hlt">Mass</span> Changes, and the Local Dynamic Geoid</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Harig, C.; Simons, F. J.</p> <p>2014-12-01</p> <p>Spherical Slepian localization functions are a useful method for studying regional <span class="hlt">mass</span> changes observed by satellite gravimetry. By projecting data onto a sparse basis set, the local field can be estimated more easily than with the full spherical harmonic basis. We have used this method previously to estimate the <span class="hlt">ice</span> <span class="hlt">mass</span> change in Greenland from GRACE data, and it can also be applied to other planetary problems such as global magnetic fields. Earth's static geoid, in contrast to the time-variable field, is in large part related to the internal density and rheological structure of the Earth. Past studies have used dynamic geoid kernels to relate this density structure and the internal deformation it induces to the surface geopotential at large scales. These now classical studies of the eighties and nineties were able to estimate the mantle's radial rheological profile, placing constraints on the ratio between upper and lower mantle viscosity. By combining these two methods, spherical Slepian localization and dynamic geoid kernels, we have created local dynamic geoid kernels which are sensitive only to density variations within an area of interest. With these kernels we can estimate the approximate local radial rheological structure that best explains the locally observed geoid on a regional basis. First-order differences of the regional mantle viscosity structure are accessible to this technique. In this contribution we present our latest, as yet unpublished results on the geographical and temporal pattern of <span class="hlt">ice</span> <span class="hlt">mass</span> changes in Antarctica over the past decade, and we introduce a new approach to extract regional information about the internal structure of the Earth from the static global gravity field. Both sets of results are linked in terms of the relevant physics, but also in being developed from the marriage of Slepian functions and geoid kernels. We make predictions on the utility of our approach to derive fully three-dimensional rheological Earth models, to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRC..123..864J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123..864J"><span>Ocean-Forced <span class="hlt">Ice</span>-Shelf Thinning in a Synchronously Coupled <span class="hlt">Ice</span>-Ocean Model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jordan, James R.; Holland, Paul R.; Goldberg, Dan; Snow, Kate; Arthern, Robert; Campin, Jean-Michel; Heimbach, Patrick; Jenkins, Adrian</p> <p>2018-02-01</p> <p>The first fully synchronous, coupled <span class="hlt">ice</span> shelf-ocean model with a fixed grounding line and imposed upstream <span class="hlt">ice</span> velocity has been developed using the MITgcm (Massachusetts Institute of Technology general circulation model). Unlike previous, asynchronous, approaches to coupled modeling our approach is fully conservative of heat, salt, and <span class="hlt">mass</span>. Synchronous coupling is achieved by continuously updating the <span class="hlt">ice</span>-shelf thickness on the ocean time step. By simulating an idealized, warm-water <span class="hlt">ice</span> shelf we show how raising the pycnocline leads to a reduction in both <span class="hlt">ice</span>-shelf <span class="hlt">mass</span> and back stress, and hence buttressing. Coupled runs show the formation of a western boundary channel in the <span class="hlt">ice</span>-shelf base due to increased melting on the western boundary due to Coriolis enhanced flow. Eastern boundary <span class="hlt">ice</span> thickening is also observed. This is not the case when using a simple depth-dependent parameterized melt, as the <span class="hlt">ice</span> shelf has relatively thinner sides and a thicker central "bulge" for a given <span class="hlt">ice</span>-shelf <span class="hlt">mass</span>. <span class="hlt">Ice</span>-shelf geometry arising from the parameterized melt rate tends to underestimate backstress (and therefore buttressing) for a given <span class="hlt">ice</span>-shelf <span class="hlt">mass</span> due to a thinner <span class="hlt">ice</span> shelf at the boundaries when compared to coupled model simulations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20010047828','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20010047828"><span><span class="hlt">Icing</span> Cloud Calibration of the NASA Glenn <span class="hlt">Icing</span> Research Tunnel</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ide, Robert F.; Oldenburg, John R.</p> <p>2001-01-01</p> <p>The <span class="hlt">icing</span> research tunnel at the NASA Glenn Research Center underwent a major rehabilitation in 1999, necessitating recalibration of the <span class="hlt">icing</span> clouds. This report describes the methods used in the recalibration, including the procedure used to establish a uniform <span class="hlt">icing</span> cloud and the use of a standard <span class="hlt">icing</span> blade technique for measurement of liquid water <span class="hlt">content</span>. The instruments and methods used to perform the droplet size calibration are also described. The liquid water <span class="hlt">content</span>/droplet size operating envelopes of the <span class="hlt">icing</span> tunnel are shown for a range of airspeeds and compared to the FAA <span class="hlt">icing</span> certification criteria. The capabilities of the IRT to produce large droplet <span class="hlt">icing</span> clouds is also detailed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1208660-changes-firn-structure-western-greenland-ice-sheet-caused-recent-warming','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1208660-changes-firn-structure-western-greenland-ice-sheet-caused-recent-warming"><span>Changes in the firn structure of the western Greenland <span class="hlt">Ice</span> Sheet caused by recent warming</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>de la Peña, S.; Howat, I. M.; Nienow, P. W.; ...</p> <p>2015-06-11</p> <p>Atmospheric warming over the Greenland <span class="hlt">Ice</span> Sheet during the last 2 decades has increased the amount of surface meltwater production, resulting in the migration of melt and percolation regimes to higher altitudes and an increase in the amount of <span class="hlt">ice</span> <span class="hlt">content</span> from refrozen meltwater found in the firn above the superimposed <span class="hlt">ice</span> zone. Here we present field and airborne radar observations of buried <span class="hlt">ice</span> layers within the near-surface (0–20 m) firn in western Greenland, obtained from campaigns between 1998 and 2014. We find a sharp increase in firn-<span class="hlt">ice</span> <span class="hlt">content</span> in the form of thick widespread layers in the percolation zone,more » which decreases the capacity of the firn to store meltwater. The estimated total annual <span class="hlt">ice</span> <span class="hlt">content</span> retained in the near-surface firn in areas with positive surface <span class="hlt">mass</span> balance west of the <span class="hlt">ice</span> divide in Greenland reached a maximum of 74 ± 25 Gt in 2012, when compared to the 1958–1999 average of 13 ± 2 Gt, while the percolation zone area more than doubled between 2003 and 2012. Increased melt and column densification resulted in surface lowering averaging -0.80 ± 0.39 m yr -1 between 1800 and 2800 m in the accumulation zone of western Greenland. Since 2007, modeled annual melt and refreezing rates in the percolation zone at elevations below 2100 m surpass the annual snowfall from the previous year, implying that <span class="hlt">mass</span> gain in the region is retained after melt in the form of refrozen meltwater. Furthermore, if current melt trends over high elevation regions continue, subsequent changes in firn structure will have implications for the hydrology of the <span class="hlt">ice</span> sheet and related abrupt seasonal densification could become increasingly significant for altimetry-derived <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balance estimates.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120002070','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120002070"><span>Assessment of Antarctic <span class="hlt">Ice</span>-Sheet <span class="hlt">Mass</span> Balance Estimates: 1992 - 2009</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zwally, H. Jay; Giovinetto, Mario B.</p> <p>2011-01-01</p> <p>Published <span class="hlt">mass</span> balance estimates for the Antarctic <span class="hlt">Ice</span> Sheet (AIS) lie between approximately +50 to -250 Gt/year for 1992 to 2009, which span a range equivalent to 15% of the annual <span class="hlt">mass</span> input and 0.8 mm/year Sea Level Equivalent (SLE). Two estimates from radar-altimeter measurements of elevation change by European Remote-sensing Satellites (ERS) (+28 and -31 Gt/year) lie in the upper part, whereas estimates from the Input-minus-Output Method (IOM) and the Gravity Recovery and Climate Experiment (GRACE) lie in the lower part (-40 to -246 Gt/year). We compare the various estimates, discuss the methodology used, and critically assess the results. Although recent reports of large and accelerating rates of <span class="hlt">mass</span> loss from GRACE=based studies cite agreement with IOM results, our evaluation does not support that conclusion. We find that the extrapolation used in the published IOM estimates for the 15 % of the periphery for which discharge velocities are not observed gives twice the rate of discharge per unit of associated <span class="hlt">ice</span>-sheet area than the 85% faster-moving parts. Our calculations show that the published extrapolation overestimates the <span class="hlt">ice</span> discharge by 282 Gt/yr compared to our assumption that the slower moving areas have 70% as much discharge per area as the faster moving parts. Also, published data on the time-series of discharge velocities and accumulation/precipitation do not support <span class="hlt">mass</span> output increases or input decreases with time, respectively. Our modified IOM estimate, using the 70% discharge assumption and substituting input from a field-data compilation for input from an atmospheric model over 6% of area, gives a loss of only 13 Gt/year (versus 136 Gt/year) for the period around 2000. Two ERS-based estimates, our modified IOM, and a GRACE-based estimate for observations within 1992 to 2005 lie in a narrowed range of +27 to - 40 Gt/year, which is about 3% of the annual <span class="hlt">mass</span> input and only 0.2 mm/year SLE. Our preferred estimate for 1992-2001 is - 47 Gt</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20060024016','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20060024016"><span><span class="hlt">Mass</span> Changes of the Greenland and Antarctic <span class="hlt">Ice</span> Sheets and Shelves and Contributions to Sea-level Rise: 1992-2002</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zwally, H. Jay; Giovinetto, Mario B.; Li, Jun; Cornejo, Helen G.; Beckley, Matthew A.; Brenner, Anita C.; Saba, Jack L.; Yi, Donghui</p> <p>2005-01-01</p> <p>Changes in <span class="hlt">ice</span> <span class="hlt">mass</span> are estimated from elevation changes derived from 10.5 years (Greenland) and 9 years (Antarctica) of satellite radar altimetry data from the European Remote-sensing Satellites ERS-1 and -2. For the first time, the dH/dt values are adjusted for changes in surface elevation resulting from temperature-driven variations in the rate of fun compaction. The Greenland <span class="hlt">ice</span> sheet is thinning at the margins (-42 plus or minus 2 Gta(sup -1) below the equilibrium line altitude (ELA)) and growing inland (+53 plus or minus 2 Gt a(sup -1)above the ELA) with a small overall <span class="hlt">mass</span> gain (+11 plus or minus 3 Gt a(sup -1); -0.03 mm a(sup -1) SLE (sea level equivalent)). The <span class="hlt">ice</span> sheet in West Antarctica (WA) is losing <span class="hlt">mass</span> (-47 (dot) 4 GT a(sup -1) and the <span class="hlt">ice</span> sheet in East Antarctica (EA) shows a small <span class="hlt">mass</span> gain (+16 plus or minus 11 Gt a(sup -1) for a combined net change of -31 plus or minus 12 Gt a(sup -1) (+0.08 mm a(sup -1) SLE)). The contribution of the three <span class="hlt">ice</span> sheets to sea level is +0.05 plus or minus 0.03 mm a(sup -1). The Antarctic <span class="hlt">ice</span> shelves show corresponding <span class="hlt">mass</span> changes of -95 (dot) 11 Gt a(sup -1) in WA and +142 plus or minus 10 Gt a(sup -1) in EA. Thinning at the margins of the Greenland <span class="hlt">ice</span> sheet and growth at higher elevations is an expected response to increasing temperatures and precipitation in a warming climate. The marked thinnings in the Pine Island and Thwaites Glacier basins of WA and the Totten Glacier basin in EA are probably <span class="hlt">ice</span>-dynamic responses to long-term climate change and perhaps past removal of their adjacent <span class="hlt">ice</span> shelves. The <span class="hlt">ice</span> growth in the southern Antarctic Peninsula and parts of EA may be due to increasing precipitation during the last century.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.G13B1099B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.G13B1099B"><span>Measuring Two Decades of <span class="hlt">Ice</span> <span class="hlt">Mass</span> Loss using GRACE and SLR</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bonin, J. A.; Chambers, D. P.</p> <p>2016-12-01</p> <p>We use Satellite Laser Ranging (SLR) to extend the time series of <span class="hlt">ice</span> <span class="hlt">mass</span> change back in time to 1994. The SLR series is of far lesser spatial resolution than GRACE, so we apply a constrained inversion technique to better localize the signal. We approximate the likely errors due to SLR's measurement errors combined with the inversion errors from using a low-resolution series, then estimate the interannual <span class="hlt">mass</span> change over Greenland and Antarctica.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.6251B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.6251B"><span>Quantifying <span class="hlt">ice</span> cliff contribution to debris-covered glacier <span class="hlt">mass</span> balance from multiple sensors</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brun, Fanny; Wagnon, Patrick; Berthier, Etienne; Kraaijenbrink, Philip; Immerzeel, Walter; Shea, Joseph; Vincent, Christian</p> <p>2017-04-01</p> <p><span class="hlt">Ice</span> cliffs on debris-covered glaciers have been recognized as a hot spot for glacier melt. <span class="hlt">Ice</span> cliffs are steep (even sometimes overhanging) and fast evolving surface features, which make them challenging to monitor. We surveyed the topography of Changri Nup Glacier (Nepalese Himalayas, Everest region) in November 2015 and 2016 using multiple sensors: terrestrial photogrammetry, Unmanned Aerial Vehicle (UAV) photogrammetry, Pléiades stereo images and ASTER stereo images. We derived 3D point clouds and digital elevation models (DEMs) following a Structure-from-Motion (SfM) workflow for the first two sets of data to monitor surface elevation changes and calculate the associated volume loss. We derived only DEMs for the two last data sets. The derived DEMs had resolutions ranging from < 5 cm to 30 m. The derived point clouds and DEMs are used to quantify the <span class="hlt">ice</span> melt of the cliffs at different scales. The very high resolution SfM point clouds, together with the surface velocity field, will be used to calculate the volume losses of 14 individual cliffs, depending on their size, aspect or the presence of supra glacial lake. Then we will extend this analysis to the whole glacier to quantify the contribution of <span class="hlt">ice</span> cliff melt to the overall glacier <span class="hlt">mass</span> balance, calculated with the UAV and Pléiades DEMs. This research will provide important tools to evaluate the role of <span class="hlt">ice</span> cliffs in regional <span class="hlt">mass</span> loss.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120010516','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120010516"><span>Greenland <span class="hlt">Ice</span> Sheet <span class="hlt">Mass</span> Balance: Distribution of Increased <span class="hlt">Mass</span> Loss with Climate Warming; 2003-07 Versus 1992-2002</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zwally, H. Jay; Li, Jun; Benner, Anita C.; Beckley, Matthew; Cornejo, Helen G.; DiMarzio, John; Giovinetto, Mario B.; Neumann, Thomas A.; Robbins, John; Saba, Jack L.; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20120010516'); toggleEditAbsImage('author_20120010516_show'); toggleEditAbsImage('author_20120010516_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20120010516_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20120010516_hide"></p> <p>2011-01-01</p> <p>We derive <span class="hlt">mass</span> changes of the Greenland <span class="hlt">ice</span> sheet (GIS) for 2003-07 from ICESat laser altimetry and compare them with results for 1992-2002 from ERS radar and airborne laser altimetry. The GIS continued to grow inland and thin at the margins during 2003 07, but surface melting and accelerated flow significantly increased the marginal thinning compared with the 1990s. The net balance changed from a small loss of 7 plus or minus 3 Gt a 1(sup -1) in the 1990s to 171 plus or minus 4 Gt a (sup -1) for 2003-07, contributing 0.5 mm a(sup -1) to recent global sea-level rise. We divide the derived <span class="hlt">mass</span> changes into two components: (1) from changes in melting and <span class="hlt">ice</span> dynamics and (2) from changes in precipitation and accumulation rate. We use our firn compaction model to calculate the elevation changes driven by changes in both temperature and accumulation rate and to calculate the appropriate density to convert the accumulation-driven changes to <span class="hlt">mass</span> changes. Increased losses from melting and <span class="hlt">ice</span> dynamics (17-206 Gt a(sup-1) are over seven times larger than increased gains from precipitation (10 35 Gt a(sup-1) during a warming period of approximately 2 K (10 a)(sup -1) over the GIS. Above 2000m elevation, the rate of gain decreased from 44 to 28 Gt a(sup-1), while below 2000m the rate of loss increased from 51 to 198 Gt a(sup-1). Enhanced thinning below the equilibrium line on outlet glaciers indicates that increased melting has a significant impact on outlet glaciers, as well as accelerating <span class="hlt">ice</span> flow. Increased thinning at higher elevations appears to be induced by dynamic coupling to thinning at the margins on decadal timescales.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110006429','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110006429"><span>Changes in the <span class="hlt">Mass</span> Balance of the Greenland <span class="hlt">Ice</span> Sheet in a Warming Climate During 2003-2009</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zwally, H. Jay; Luthcke, Scott</p> <p>2010-01-01</p> <p><span class="hlt">Mass</span> changes of the Greenland <span class="hlt">ice</span> sheet (GIS) derived from ICESat and GRACE data both show that the net <span class="hlt">mass</span> loss from GIS during 2003-2009 is about 175 Gt/year, which contributes 0.5mm/yr global sea-level rise. The rate of <span class="hlt">mass</span> loss has increased significantly since the 1990's when the GIS was close to <span class="hlt">mass</span> balance. Even though the GIS was close to <span class="hlt">mass</span> balance during the 1990's, it was already showing characteristics of responding to8 warmer climate, specifically thinning at the margins and thickening inland at higher elevations. During 2003-2009, increased <span class="hlt">ice</span> thinning due to increases in melting and acceleration of outlet glaciers began to strongly exceed the inland thickening from increases in accumulation. Over the entire GIS, the <span class="hlt">mass</span> loss between the two periods, from increased melting and <span class="hlt">ice</span> dynamics, increased by about 190 Gt/year while the <span class="hlt">mass</span> gain, from increased precipitation and accumulation, increased by only about 15Gt/year. These <span class="hlt">ice</span> changes occurred during a time when the temperature on GIS changed at rate of about 2K/decade. The distribution of elevation and <span class="hlt">mass</span> changes derived from ICESat have high spatial resolution showing details over outlet glaciers, by drainage systems, and by elevation. However, information on the seasonal cycle of changes from ICESat data is limited, because the ICESat lasers were only operated during two to three campaigns per year of about 35 days duration each. In contrast, the temporal resolution of GRACE data, provided by the continuous data collection, is much better showing details of the seasonal cycle and the inter-annual variability. The differing sensitivity of the ICESat altimetry and the GRACE gravity methods to motion of the underlying bedrock from glacial isostatic adjustment (GIA) is used to evaluate the GIA corrections provided by models. The two data types are also combined to make estimates of the partitioning of the <span class="hlt">mass</span> gains and losses among accumulation, melting, and <span class="hlt">ice</span> discharge from outlet</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA617621','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA617621"><span>Wave-<span class="hlt">Ice</span> and Air-<span class="hlt">Ice</span>-Ocean Interaction During the Chukchi Sea <span class="hlt">Ice</span> Edge Advance</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2014-09-30</p> <p>During cruise CU-B UAF UW Airborne expendable <span class="hlt">Ice</span> Buoy (AXIB) Ahead, at and inside <span class="hlt">ice</span> edge Surface meteorology T, SLP ~1 year CU-B UW...Balance (IMB) buoys Inside <span class="hlt">ice</span> edge w/ >50cm thickness <span class="hlt">Ice</span> <span class="hlt">mass</span> balance T in snow-<span class="hlt">ice</span>-ocean, T, SLP at surface ~1 year WHOI CRREL (SeaState DRI</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AMT....11.1615Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AMT....11.1615Y"><span>A prototype method for diagnosing high <span class="hlt">ice</span> water <span class="hlt">content</span> probability using satellite imager data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yost, Christopher R.; Bedka, Kristopher M.; Minnis, Patrick; Nguyen, Louis; Strapp, J. Walter; Palikonda, Rabindra; Khlopenkov, Konstantin; Spangenberg, Douglas; Smith, William L., Jr.; Protat, Alain; Delanoe, Julien</p> <p>2018-03-01</p> <p>Recent studies have found that ingestion of high <span class="hlt">mass</span> concentrations of <span class="hlt">ice</span> particles in regions of deep convective storms, with radar reflectivity considered safe for aircraft penetration, can adversely impact aircraft engine performance. Previous aviation industry studies have used the term high <span class="hlt">ice</span> water <span class="hlt">content</span> (HIWC) to define such conditions. Three airborne field campaigns were conducted in 2014 and 2015 to better understand how HIWC is distributed in deep convection, both as a function of altitude and proximity to convective updraft regions, and to facilitate development of new methods for detecting HIWC conditions, in addition to many other research and regulatory goals. This paper describes a prototype method for detecting HIWC conditions using geostationary (GEO) satellite imager data coupled with in situ total water <span class="hlt">content</span> (TWC) observations collected during the flight campaigns. Three satellite-derived parameters were determined to be most useful for determining HIWC probability: (1) the horizontal proximity of the aircraft to the nearest overshooting convective updraft or textured anvil cloud, (2) tropopause-relative infrared brightness temperature, and (3) daytime-only cloud optical depth. Statistical fits between collocated TWC and GEO satellite parameters were used to determine the membership functions for the fuzzy logic derivation of HIWC probability. The products were demonstrated using data from several campaign flights and validated using a subset of the satellite-aircraft collocation database. The daytime HIWC probability was found to agree quite well with TWC time trends and identified extreme TWC events with high probability. Discrimination of HIWC was more challenging at night with IR-only information. The products show the greatest capability for discriminating TWC ≥ 0.5 g m-3. Product validation remains challenging due to vertical TWC uncertainties and the typically coarse spatio-temporal resolution of the GEO data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.C23B0613H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.C23B0613H"><span>Polar <span class="hlt">Ice</span> Caps: a Canary for the Greenland <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Honsaker, W.; Lowell, T. V.; Sagredo, E.; Kelly, M. A.; Hall, B. L.</p> <p>2010-12-01</p> <p><span class="hlt">Ice</span> caps are glacier <span class="hlt">masses</span> that are highly sensitive to climate change. Because of their hypsometry they can have a binary state. When relatively slight changes in the equilibrium line altitude (ELA) either intersect or rise above the land the <span class="hlt">ice</span> can become established or disappear. Thus these upland <span class="hlt">ice</span> <span class="hlt">masses</span> have a fast response time. Here we consider a way to extract the ELA signal from independent <span class="hlt">ice</span> caps adjacent to the Greenland <span class="hlt">Ice</span> Sheet margin. It may be that these <span class="hlt">ice</span> caps are sensitive trackers of climate change that also impact the <span class="hlt">ice</span> sheet margin. One example is the Istorvet <span class="hlt">Ice</span> Cap located in Liverpool Land, East Greenland (70.881°N, 22.156°W). The <span class="hlt">ice</span> cap topography and the underlying bedrock surface dips to the north, with peak elevation of the current <span class="hlt">ice</span> ranging in elevation from 1050 to 745 m.a.s.l. On the eastern side of the <span class="hlt">ice</span> <span class="hlt">mass</span> the outlet glaciers extending down to sea level. The western margin has several small lobes in topographic depressions, with the margin reaching down to 300 m.a.s.l. Topographic highs separate the <span class="hlt">ice</span> cap into at least 5 main catchments, each having a pair of outlet lobes toward either side of the <span class="hlt">ice</span> cap. Because of the regional bedrock slope each catchment has its own elevation range. Therefore, as the ELA changes it is possible for some catchments of the <span class="hlt">ice</span> cap to experience positive <span class="hlt">mass</span> balance while others have a negative balance. Based on weather observations we estimate the present day ELA to be ~1000 m.a.s.l, meaning <span class="hlt">mass</span> balance is negative for the majority of the <span class="hlt">ice</span> cap. By tracking glacier presence/absence in these different catchments, we can reconstruct small changes in the ELA. Another example is the High <span class="hlt">Ice</span> Cap (informal name) in Milne Land (70.903°N, 25.626°W, 1080 m), East Greenland. Here at least 4 unconformities in <span class="hlt">ice</span> layers found near the southern margin of the <span class="hlt">ice</span> cap record changing intervals of accumulation and ablation. Therefore, this location may also be sensitive to slight</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_8 --> <div id="page_9" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="161"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.9829W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.9829W"><span><span class="hlt">Mass</span> loss of the Greenland peripheral glaciers and <span class="hlt">ice</span> caps from satellite altimetry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wouters, Bert; Noël, Brice; Moholdt, Geir; Ligtenberg, Stefan; van den Broeke, Michiel</p> <p>2017-04-01</p> <p>At its rapidly warming margins, the Greenland <span class="hlt">Ice</span> Sheet is surrounded by (semi-)detached glaciers and <span class="hlt">ice</span> caps (GIC). Although they cover only roughly 5% of the total glaciated area in the region, they are estimated to account for 15-20% of the total sea level rise contribution of Greenland. The spatial and temporal evolution of the <span class="hlt">mass</span> changes of the peripheral GICs, however, remains poorly constrained. In this presentation, we use satellite altimetry from ICESat and Cryosat-2 combined with a high-resolution regional climate model to derive a 14 year time series (2003-2016) of regional elevation and <span class="hlt">mass</span> changes. The total <span class="hlt">mass</span> loss has been relatively constant during this period, but regionally, the GICs show marked temporal variations. Whereas thinning was concentrated along the eastern margin during 2003-2009, western GICs became the prime sea level rise contributors in recent years. <span class="hlt">Mass</span> loss in the northern region has been steadily increasing throughout the record, due to a strong atmospheric warning and a deterioration of the capacity of the firn layer to buffer the resulting melt water.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMPP52A..04A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMPP52A..04A"><span>How and when to terminate the Pleistocene <span class="hlt">ice</span> ages?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Abe-Ouchi, A.; Saito, F.; Kawamura, K.; Takahashi, K.; Raymo, M. E.; Okuno, J.; Blatter, H.</p> <p>2015-12-01</p> <p>Climate change with wax and wane of large Northern Hemisphere <span class="hlt">ice</span> sheet occurred in the past 800 thousand years characterized by 100 thousand year cycle with a large amplitude of sawtooth pattern, following a transition from a period of 40 thousand years cycle with small amplitude of <span class="hlt">ice</span> sheet change at about 1 million years ago. Although the importance of insolation as the ultimate driver is now appreciated, the mechanism what determines timing and strength of terminations are far from clearly understood. Here we show, using comprehensive climate and <span class="hlt">ice</span>-sheet models, that insolation and internal feedbacks between the climate, the <span class="hlt">ice</span> sheets and the lithosphere-asthenosphere system explain the 100,000-year periodicity. The responses of equilibrium states of <span class="hlt">ice</span> sheets to summer insolation show hysteresis, with the shape and position of the hysteresis loop playing a key part in determining the periodicities of glacial cycles. The hysteresis loop of the North American <span class="hlt">ice</span> sheet is such that after inception of the <span class="hlt">ice</span> sheet, its <span class="hlt">mass</span> balance remains mostly positive through several precession cycles, whose amplitudes decrease towards an eccentricity minimum. The larger the <span class="hlt">ice</span> sheet grows and extends towards lower latitudes, the smaller is the insolation required to make the <span class="hlt">mass</span> balance negative. Therefore, once a large <span class="hlt">ice</span> sheet is established, a moderate increase in insolation is sufficient to trigger a negative <span class="hlt">mass</span> balance, leading to an almost complete retreat of the <span class="hlt">ice</span> sheet within several thousand years. We discuss further the mechanism which determine the timing of <span class="hlt">ice</span> age terminations by examining the role of astronomical forcing and change of atmospheric carbon dioxide <span class="hlt">contents</span> through sensitivity experiments and comparison of several <span class="hlt">ice</span> age cycles with different settings of astronomical forcings.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.G31E..01Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.G31E..01Z"><span>Transient <span class="hlt">ice</span> <span class="hlt">mass</span> variations over Greenland detected by the combination of GPS and GRACE data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, B.; Liu, L.; Khan, S. A.; van Dam, T. M.; Zhang, E.</p> <p>2017-12-01</p> <p>Over the past decade, the Greenland <span class="hlt">Ice</span> Sheet (GrIS) has been undergoing significant warming and <span class="hlt">ice</span> <span class="hlt">mass</span> loss. Such <span class="hlt">mass</span> loss was not always a steady process but had substantial temporal and spatial variabilities. Here we apply multi-channel singular spectral analysis to crustal deformation time series measured at about 50 Global Positioning System (GPS) stations mounted on bedrock around the Greenland coast and <span class="hlt">mass</span> changes inferred from Gravity Recovery and Climate Experiment (GRACE) to detect transient changes in <span class="hlt">ice</span> <span class="hlt">mass</span> balance over the GrIS. We detect two transient anomalies: one is a negative melting anomaly (Anomaly 1) that peaked around 2010; the other is a positive melting anomaly (Anomaly 2) that peaked between 2012 and 2013. The GRACE data show that both anomalies caused significant <span class="hlt">mass</span> changes south of 74°N but negligible changes north of 74°N. Both anomalies caused the maximum <span class="hlt">mass</span> change in southeast GrIS, followed by in west GrIS near Jakobshavn. Our results also show that the <span class="hlt">mass</span> change caused by Anomaly 1 first reached the maximum in late 2009 in the southeast GrIS and then migrated to west GrIS. However, in Anomaly 2, the southeast GrIS was the last place that reached the maximum <span class="hlt">mass</span> change in early 2013 and the west GrIS near Jakobshavn was the second latest place that reached the maximum <span class="hlt">mass</span> change. Most of the GPS data show similar spatiotemporal patterns as those obtained from the GRACE data. However, some GPS time series show discrepancies in either space or time, because of data gaps and different sensitivities of <span class="hlt">mass</span> loading change. Namely, loading deformation measured by GPS can be significantly affected by local dynamical <span class="hlt">mass</span> changes, which, yet, has little impact on GRACE observations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1710743B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1710743B"><span>Geomorphology and <span class="hlt">Ice</span> <span class="hlt">Content</span> of Glacier - Rock Glacier &ndash; Moraine Complexes in Ak-Shiirak Range (Inner Tien Shan, Kyrgyzstan)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bolch, Tobias; Kutuzov, Stanislav; Rohrbach, Nico; Fischer, Andrea; Osmonov, Azamat</p> <p>2015-04-01</p> <p>Meltwater originating from the Tien Shan is of high importance for the runoff to the arid and semi-arid region of Central Asia. Previous studies estimate a glaciers' contribution of about 40% for the Aksu-Tarim Catchment, a transboundary watershed between Kyrgyzstan and China. Large parts of the Ak-Shiirak Range drain into this watershed. Glaciers in Central and Inner Tien Shan are typically polythermal or even cold and surrounded by permafrost. Several glaciers terminate into large moraine complexes which show geomorphological indicators of <span class="hlt">ice</span> <span class="hlt">content</span> such as thermo-karst like depressions, and further downvalley signs of creep such as ridges and furrows and a fresh, steep rock front which are typical indicators for permafrost creep ("rock glacier"). Hence, glaciers and permafrost co-exist in this region and their interactions are important to consider, e.g. for the understanding of glacial and periglacial processes. It can also be assumed that the <span class="hlt">ice</span> stored in these relatively large dead-<span class="hlt">ice</span>/moraine-complexes is a significant amount of the total <span class="hlt">ice</span> storage. However, no detailed investigations exist so far. In an initial study, we investigated the structure and <span class="hlt">ice</span> <span class="hlt">content</span> of two typical glacier-moraine complexes in the Ak-Shiirak-Range using different ground penetrating radar (GPR) devices. In addition, the geomorphology was mapped using high resolution satellite imagery. The structure of the moraine-rock glacier complex is in general heterogeneous. Several dead <span class="hlt">ice</span> bodies with different thicknesses and moraine-derived rock glaciers with different stages of activities could be identified. Few parts of these "rock glaciers" contain also massive <span class="hlt">ice</span> but the largest parts are likely characterised by rock-<span class="hlt">ice</span> layers of different thickness and <span class="hlt">ice</span> <span class="hlt">contents</span>. In one glacier forefield, the thickness of the rock-<span class="hlt">ice</span> mixture is partly more than 300 m. This is only slightly lower than the maximum thickness of the glacier <span class="hlt">ice</span>. Our measurements revealed that up to 20% of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22525155-distinguishing-neutrino-mass-hierarchies-using-dark-matter-annihilation-signals-icecube','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22525155-distinguishing-neutrino-mass-hierarchies-using-dark-matter-annihilation-signals-icecube"><span>Distinguishing neutrino <span class="hlt">mass</span> hierarchies using dark matter annihilation signals at <span class="hlt">Ice</span>Cube</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Allahverdi, Rouzbeh; Knockel, Bradley; Dutta, Bhaskar</p> <p>2015-12-01</p> <p>We explore the possibility of distinguishing neutrino <span class="hlt">mass</span> hierarchies through the neutrino signal from dark matter annihilation at neutrino telescopes. We consider a simple extension of the standard model where the neutrino <span class="hlt">masses</span> and mixing angles are obtained via the type-II seesaw mechanism as an explicit example. We show that future extensions of <span class="hlt">Ice</span>Cube neutrino telescope may detect the neutrino signal from DM annihilation at the Galactic Center and inside the Sun, and differentiate between the normal and inverted <span class="hlt">mass</span> hierarchies, in this model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009GeoJI.176...95S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009GeoJI.176...95S"><span>Estimating the rates of <span class="hlt">mass</span> change, <span class="hlt">ice</span> volume change and snow volume change in Greenland from ICESat and GRACE data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Slobbe, D. C.; Ditmar, P.; Lindenbergh, R. C.</p> <p>2009-01-01</p> <p>The focus of this paper is on the quantification of ongoing <span class="hlt">mass</span> and volume changes over the Greenland <span class="hlt">ice</span> sheet. For that purpose, we used elevation changes derived from the <span class="hlt">Ice</span>, 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 <span class="hlt">mass</span> 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 <span class="hlt">mass</span> 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 <span class="hlt">mass</span> change rate for the whole of Greenland ranges between -128 and -218Gtonyr-1. Most GRACE solutions show much stronger <span class="hlt">mass</span> losses as obtained with ICESat, which might be related to a local undersampling of the <span class="hlt">mass</span> loss by ICESat and uncertainties in the used snow/<span class="hlt">ice</span> densities. To solve the problem of uncertainties in the snow and <span class="hlt">ice</span> 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 <span class="hlt">mass</span> change rate, estimates this rate in combination with an effective snow/<span class="hlt">ice</span> 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 <span class="hlt">ice</span> volume and variations of snow volume separately. Such an approach is expected to lead to new insights in ongoing <span class="hlt">mass</span> change processes over the Greenland <span class="hlt">ice</span> sheet. Our results show for different GRACE solutions a snow</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1367290','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1367290"><span>PU-<span class="hlt">ICE</span> Summary Information.</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>Moore, Michael</p> <p></p> <p>The Generator Knowledge Report for the Plutonium Isentropic Compression Experiment Containment Systems (GK Report) provides information for the Plutonium Isentropic Compression Experiment (Pu- <span class="hlt">ICE</span>) program to support waste management and characterization efforts. Attachment 3-18 presents generator knowledge (GK) information specific to the eighteenth Pu-<span class="hlt">ICE</span> conducted in August 2015, also known as ‘Shot 18 (Aug 2015) and Pu-<span class="hlt">ICE</span> Z-2841 (1).’ Shot 18 (Aug 2015) was generated on August 28, 2015 (1). Calculations based on the isotopic <span class="hlt">content</span> of Shot 18 (Aug 2015) and the measured <span class="hlt">mass</span> of the containment system demonstrate the post-shot containment system is low-level waste (LLW). Therefore, thismore » containment system will be managed at Sandia National Laboratory/New Mexico (SNL/NM) as LLW. Attachment 3-18 provides documentation of the TRU concentration and documents the concentration of any hazardous constituents.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28361871','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28361871"><span>A tipping point in refreezing accelerates <span class="hlt">mass</span> loss of Greenland's glaciers and <span class="hlt">ice</span> caps.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Noël, B; van de Berg, W J; Lhermitte, S; Wouters, B; Machguth, H; Howat, I; Citterio, M; Moholdt, G; Lenaerts, J T M; van den Broeke, M R</p> <p>2017-03-31</p> <p>Melting of the Greenland <span class="hlt">ice</span> sheet (GrIS) and its peripheral glaciers and <span class="hlt">ice</span> caps (GICs) contributes about 43% to contemporary sea level rise. While patterns of GrIS <span class="hlt">mass</span> loss are well studied, the spatial and temporal evolution of GICs <span class="hlt">mass</span> loss and the acting processes have remained unclear. Here we use a novel, 1 km surface <span class="hlt">mass</span> balance product, evaluated against in situ and remote sensing data, to identify 1997 (±5 years) as a tipping point for GICs <span class="hlt">mass</span> balance. That year marks the onset of a rapid deterioration in the capacity of the GICs firn to refreeze meltwater. Consequently, GICs runoff increases 65% faster than meltwater production, tripling the post-1997 <span class="hlt">mass</span> loss to 36±16 Gt -1 , or ∼14% of the Greenland total. In sharp contrast, the extensive inland firn of the GrIS retains most of its refreezing capacity for now, buffering 22% of the increased meltwater production. This underlines the very different response of the GICs and GrIS to atmospheric warming.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5380968','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5380968"><span>A tipping point in refreezing accelerates <span class="hlt">mass</span> loss of Greenland's glaciers and <span class="hlt">ice</span> caps</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Noël, B.; van de Berg, W. J; Lhermitte, S.; Wouters, B.; Machguth, H.; Howat, I.; Citterio, M.; Moholdt, G.; Lenaerts, J. T. M.; van den Broeke, M. R.</p> <p>2017-01-01</p> <p>Melting of the Greenland <span class="hlt">ice</span> sheet (GrIS) and its peripheral glaciers and <span class="hlt">ice</span> caps (GICs) contributes about 43% to contemporary sea level rise. While patterns of GrIS <span class="hlt">mass</span> loss are well studied, the spatial and temporal evolution of GICs <span class="hlt">mass</span> loss and the acting processes have remained unclear. Here we use a novel, 1 km surface <span class="hlt">mass</span> balance product, evaluated against in situ and remote sensing data, to identify 1997 (±5 years) as a tipping point for GICs <span class="hlt">mass</span> balance. That year marks the onset of a rapid deterioration in the capacity of the GICs firn to refreeze meltwater. Consequently, GICs runoff increases 65% faster than meltwater production, tripling the post-1997 <span class="hlt">mass</span> loss to 36±16 Gt−1, or ∼14% of the Greenland total. In sharp contrast, the extensive inland firn of the GrIS retains most of its refreezing capacity for now, buffering 22% of the increased meltwater production. This underlines the very different response of the GICs and GrIS to atmospheric warming. PMID:28361871</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017NatCo...814730N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017NatCo...814730N"><span>A tipping point in refreezing accelerates <span class="hlt">mass</span> loss of Greenland's glaciers and <span class="hlt">ice</span> caps</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Noël, B.; van de Berg, W. J.; Lhermitte, S.; Wouters, B.; Machguth, H.; Howat, I.; Citterio, M.; Moholdt, G.; Lenaerts, J. T. M.; van den Broeke, M. R.</p> <p>2017-03-01</p> <p>Melting of the Greenland <span class="hlt">ice</span> sheet (GrIS) and its peripheral glaciers and <span class="hlt">ice</span> caps (GICs) contributes about 43% to contemporary sea level rise. While patterns of GrIS <span class="hlt">mass</span> loss are well studied, the spatial and temporal evolution of GICs <span class="hlt">mass</span> loss and the acting processes have remained unclear. Here we use a novel, 1 km surface <span class="hlt">mass</span> balance product, evaluated against in situ and remote sensing data, to identify 1997 (+/-5 years) as a tipping point for GICs <span class="hlt">mass</span> balance. That year marks the onset of a rapid deterioration in the capacity of the GICs firn to refreeze meltwater. Consequently, GICs runoff increases 65% faster than meltwater production, tripling the post-1997 <span class="hlt">mass</span> loss to 36+/-16 Gt-1, or ~14% of the Greenland total. In sharp contrast, the extensive inland firn of the GrIS retains most of its refreezing capacity for now, buffering 22% of the increased meltwater production. This underlines the very different response of the GICs and GrIS to atmospheric warming.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.7457N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.7457N"><span>Quantifying the <span class="hlt">mass</span> loss of peripheral Greenland glaciers and <span class="hlt">ice</span> caps (1958-2014).</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Noël, Brice; van de Berg, Willem Jan; Machguth, Horst; van den Broeke, Michiel</p> <p>2016-04-01</p> <p>Since the 2000s, <span class="hlt">mass</span> loss from Greenland peripheral glaciers and <span class="hlt">ice</span> caps (GICs) has accelerated, becoming an important contributor to sea level rise. Under continued warming throughout the 21st century, GICs might yield up to 7.5 to 11 mm sea level rise, with increasing dominance of surface runoff at the expense of <span class="hlt">ice</span> discharge. However, despite multiple observation campaigns, little remains known about the contribution of GICs to total Greenland <span class="hlt">mass</span> loss. Furthermore, the relatively coarse resolutions in regional climate models, i.e. 5 km to 20 km, fail to represent the small scale patterns of surface <span class="hlt">mass</span> balance (SMB) components over these topographically complex regions including also narrow valley glaciers. Here, we present a novel approach to quantify the contribution of GICs to surface melt and runoff, based on an elevation dependent downscaling method. GICs daily SMB components at 1 km resolution are obtained by statistically downscaling the outputs of RACMO2.3 at 11 km resolution to a down-sampled version of the GIMP DEM for the period 1958-2014. This method has recently been successfully validated over the Greenland <span class="hlt">ice</span> sheet and is now applied to GICs. In this study, we first evaluate the 1 km daily downscaled GICs SMB against a newly available and comprehensive dataset of ablation stake measurements. Then, we investigate present-day trends of meltwater production and SMB for different regions and estimate GICs contribution to total Greenland <span class="hlt">mass</span> loss. These data are considered valuable for model evaluation and prediction of future sea level rise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C21A0690W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C21A0690W"><span>Impact of <span class="hlt">ice</span>-shelf sediment <span class="hlt">content</span> on the dynamics of plumes under melting <span class="hlt">ice</span> shelves</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wells, A.</p> <p>2015-12-01</p> <p>When a floating <span class="hlt">ice</span> shelf melts into an underlying warm salty ocean, the resulting fresh meltwater can rise in a buoyant <span class="hlt">Ice</span>-Shelf-Water plume under the <span class="hlt">ice</span>. In certain settings, <span class="hlt">ice</span> flowing across the grounding line carries a basal layer of debris rich <span class="hlt">ice</span>, entrained via basal freezing around till in the upstream <span class="hlt">ice</span> sheet. Melting of this debris-laden <span class="hlt">ice</span> from floating <span class="hlt">ice</span> shelves provides a flux of dense sediment to the ocean, in addition to the release of fresh buoyant meltwater. This presentation considers the impact of the resulting suspended sediment on the dynamics of <span class="hlt">ice</span> shelf water plumes, and identifies two key flow regimes depending on the sediment concentration frozen into the basal <span class="hlt">ice</span> layer. For large sediment concentration, melting of the debris-laden <span class="hlt">ice</span> shelf generates dense convectively unstable waters that drive convective overturning into the underlying ocean. For lower sediment concentration, the sediment initially remains suspended in a buoyant meltwater plume rising along the underside of the <span class="hlt">ice</span> shelf, before slowly depositing into the underlying ocean. A theoretical plume model is used to evaluate the significance of the negatively buoyant sediment on circulation strength and the feedbacks on melting rate, along with the expected depositional patterns under the <span class="hlt">ice</span> shelf.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26887494','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26887494"><span><span class="hlt">Ice</span> stream activity scaled to <span class="hlt">ice</span> sheet volume during Laurentide <span class="hlt">Ice</span> Sheet deglaciation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Stokes, C R; Margold, M; Clark, C D; Tarasov, L</p> <p>2016-02-18</p> <p>The contribution of the Greenland and West Antarctic <span class="hlt">ice</span> sheets to sea level has increased in recent decades, largely owing to the thinning and retreat of outlet glaciers and <span class="hlt">ice</span> streams. This dynamic loss is a serious concern, with some modelling studies suggesting that the collapse of a major <span class="hlt">ice</span> sheet could be imminent or potentially underway in West Antarctica, but others predicting a more limited response. A major problem is that observations used to initialize and calibrate models typically span only a few decades, and, at the <span class="hlt">ice</span>-sheet scale, it is unclear how the entire drainage network of <span class="hlt">ice</span> streams evolves over longer timescales. This represents one of the largest sources of uncertainty when predicting the contributions of <span class="hlt">ice</span> sheets to sea-level rise. A key question is whether <span class="hlt">ice</span> streams might increase and sustain rates of <span class="hlt">mass</span> loss over centuries or millennia, beyond those expected for a given ocean-climate forcing. Here we reconstruct the activity of 117 <span class="hlt">ice</span> streams that operated at various times during deglaciation of the Laurentide <span class="hlt">Ice</span> Sheet (from about 22,000 to 7,000 years ago) and show that as they activated and deactivated in different locations, their overall number decreased, they occupied a progressively smaller percentage of the <span class="hlt">ice</span> sheet perimeter and their total discharge decreased. The underlying geology and topography clearly influenced <span class="hlt">ice</span> stream activity, but--at the <span class="hlt">ice</span>-sheet scale--their drainage network adjusted and was linked to changes in <span class="hlt">ice</span> sheet volume. It is unclear whether these findings can be directly translated to modern <span class="hlt">ice</span> sheets. However, contrary to the view that sees <span class="hlt">ice</span> streams as unstable entities that can accelerate <span class="hlt">ice</span>-sheet deglaciation, we conclude that <span class="hlt">ice</span> streams exerted progressively less influence on <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balance during the retreat of the Laurentide <span class="hlt">Ice</span> Sheet.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Sci...358..781M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Sci...358..781M"><span>Cordilleran <span class="hlt">Ice</span> Sheet <span class="hlt">mass</span> loss preceded climate reversals near the Pleistocene Termination</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Menounos, B.; Goehring, B. M.; Osborn, G.; Margold, M.; Ward, B.; Bond, J.; Clarke, G. K. C.; Clague, J. J.; Lakeman, T.; Koch, J.; Caffee, M. W.; Gosse, J.; Stroeven, A. P.; Seguinot, J.; Heyman, J.</p> <p>2017-11-01</p> <p>The Cordilleran <span class="hlt">Ice</span> Sheet (CIS) once covered an area comparable to that of Greenland. Previous geologic evidence and numerical models indicate that the <span class="hlt">ice</span> sheet covered much of westernmost Canada as late as 12.5 thousand years ago (ka). New data indicate that substantial areas throughout westernmost Canada were <span class="hlt">ice</span> free prior to 12.5 ka and some as early as 14.0 ka, with implications for climate dynamics and the timing of meltwater discharge to the Pacific and Arctic oceans. Early Bølling-Allerød warmth halved the <span class="hlt">mass</span> of the CIS in as little as 500 years, causing 2.5 to 3.0 meters of sea-level rise. Dozens of cirque and valley glaciers, along with the southern margin of the CIS, advanced into recently deglaciated regions during the Bølling-Allerød and Younger Dryas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C33D1236L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C33D1236L"><span>Geodetic <span class="hlt">mass</span> balance measurements on debris and clean-<span class="hlt">ice</span> tropical glaciers in Ecuador</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>La Frenierre, J.; Decker, C. R.; Jordan, E.; Wigmore, O.; Hodge, B. E.; Niederriter, C.; Michels, A.</p> <p>2017-12-01</p> <p>Glaciers are recognized as highly sensitive indicators of climate change in high altitude, low latitude environments. In the tropical Andes, various analyses of glacier surface area change have helped illuminate the manifestation of climate change in this region, however, information about actual glacier <span class="hlt">mass</span> balance behavior is much more limited given the relatively small glaciers, difficult access, poor weather, and/or limited local resources common here. Several new technologies, including aerial and terrestrial LIDAR and structure-from-motion photogrammetry using small unmanned aerial vehicles (UAVs), make <span class="hlt">mass</span> balance measurements using geodetic approaches increasingly feasible in remote mountain locations, which can both further our understanding of changing climatic conditions, and improve our ability to evaluate the downstream hydrologic impacts of <span class="hlt">ice</span> loss. At Volcán Chimborazo, Ecuador, these new technologies, combined with a unique, 5-meter resolution digital elevation model derived from 1997 aerial imagery, make possible an analysis of the magnitude and spatial patterns of <span class="hlt">mass</span> balance behavior over the past two decades. Here, we evaluate <span class="hlt">ice</span> loss between 1997 and 2017 at the tongues of two adjacent glaciers, one debris-covered and detached from its accumulation area (Reschreiter Glacier), and one debris-free and intact (Hans Meyer Glacier). Additionally, we incorporate data from 2012 and 2013 terrestrial LIDAR surveys to evaluate the behavior of the Reschreiter at a finer temporal resolution. We find that on the Hans Meyer, the mean surface deflation rate since 1997 at the present-day tongue has been nearly 3 m yr-1, while on the lower-elevation Reschreiter, the mean deflation rate has been approximately 1 m yr-1. However, the processes by which debris-covered <span class="hlt">ice</span> becomes exposed results in highly heterogeneous patterns of <span class="hlt">ice</span> loss, with some areas experiencing surface deflation rates approaching 15 m yr-1 when energy absorption is unimpeded.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19900018976','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19900018976"><span>A scheme for parameterizing cirrus cloud <span class="hlt">ice</span> water <span class="hlt">content</span> in general circulation models</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Heymsfield, Andrew J.; Donner, Leo J.</p> <p>1990-01-01</p> <p>Clouds strongly influence th earth's energy budget. They control th amount of solar radiative energy absorbed by the climate system, partitioning the energy between the atmosphere and the earth's surface. They also control the loss of energy to space by their effect on thermal emission. Cirrus and altostratus are the most frequent cloud types, having an annual average global coverage of 35 and 40 percent, respectively. Cirrus is composed almost entirely of <span class="hlt">ice</span> crystals and the same is frequently true of the upper portions of altostratus since they are often formed by the thickening of cirrostratus and by the spreading of the middle or upper portions of thunderstorms. Thus, since <span class="hlt">ice</span> clouds cover such a large portion of the earth's surface, they almost certainly have an important effect on climate. With this recognition, researchers developing climate models are seeking largely unavailable methods for specifying the conditions for <span class="hlt">ice</span> cloud formation, and quantifying the spatial distribution of <span class="hlt">ice</span> water <span class="hlt">content</span>, IWC, a necessary step in deriving their radiative characteristics since radiative properties are apparently related to IWC. A method is developed for specifying IWC in climate models, based on theory and measurements in cirrus during FIRE and other experiments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009GeCoA..73.5959G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009GeCoA..73.5959G"><span>Ultra-low rare earth element <span class="hlt">content</span> in accreted <span class="hlt">ice</span> from sub-glacial Lake Vostok, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gabrielli, Paolo; Planchon, Frederic; Barbante, Carlo; Boutron, Claude F.; Petit, Jean Robert; Bulat, Sergey; Hong, Sungmin; Cozzi, Giulio; Cescon, Paolo</p> <p>2009-10-01</p> <p>This paper reports the first rare earth element (REE) concentrations in accreted <span class="hlt">ice</span> refrozen from sub-glacial Lake Vostok (East Antarctica). REE were determined in various sections of the Vostok <span class="hlt">ice</span> core in order to geochemically characterize its impurities. Samples were obtained from accreted <span class="hlt">ice</span> and, for comparison, from the upper glacier <span class="hlt">ice</span> of atmospheric origin (undisturbed, disturbed and glacial flour <span class="hlt">ice</span>). REE concentrations ranged between 0.8-56 pg g -1 for Ce and 0.0035-0.24 pg g -1 for Lu in glacier <span class="hlt">ice</span>, and between <0.1-24 pg g -1 for Ce and <0.0004-0.02 pg g -1 for Lu in accreted <span class="hlt">ice</span>. Interestingly, the REE concentrations in the upper accreted <span class="hlt">ice</span> (AC 1; characterized by visible aggregates containing a mixture of very fine terrigenous particles) and in the deeper accreted <span class="hlt">ice</span> (AC 2; characterized by transparent <span class="hlt">ice</span>) are lower than those in fresh water and seawater, respectively. We suggest that such ultra-low concentrations are unlikely to be representative of the real REE <span class="hlt">content</span> in Lake Vostok, but instead may reflect phase exclusion processes occurring at the <span class="hlt">ice</span>/water interface during refreezing. In particular, the uneven spatial distribution (on the order of a few cm) and the large range of REE concentrations observed in AC 1 are consistent with the occurrence/absence of the aggregates in adjacent <span class="hlt">ice</span>, and point to the presence of solid-phase concentration/exclusion processes occurring within separate pockets of frazil <span class="hlt">ice</span> during AC 1 formation. Interestingly, if the LREE enrichment found in AC 1 was not produced by chemical fractionation occurring in Lake Vostok water, this may reflect a contribution of bedrock material, possibly in combination with aeolian dust released into the lake by melting of the glacier <span class="hlt">ice</span>. Collectively, this valuable information provides new insight into the accreted <span class="hlt">ice</span> formation processes, the bedrock geology of East Antarctica as well as the water chemistry and circulation of Lake Vostok.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.U53C..12B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.U53C..12B"><span>Ultra-low rare earth element <span class="hlt">content</span> in accreted <span class="hlt">ice</span> from sub-glacial Lake Vostok, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barbante, C.; Gabrielli, P.; Turetta, C.; Planchon, F.; Boutron, C.; Petit, J. R.; Bulat, S.; Hong, S.; Cozzi, G.; Cescon, P.</p> <p>2009-12-01</p> <p>We report the first rare earth element (REE) concentrations in accreted <span class="hlt">ice</span> refrozen from sub-glacial Lake Vostok (East Antarctica). REE were determined in various sections of the Vostok <span class="hlt">ice</span> core in order to geochemically characterize its impurities. Samples were obtained from accreted <span class="hlt">ice</span> and, for comparison, from the upper glacier <span class="hlt">ice</span> of atmospheric origin (undisturbed, disturbed and glacial flour <span class="hlt">ice</span>). REE concentrations ranged between 0.8-56 pg g-1 for Ce and 0.0035- 0.24 pg g-1 for Lu in glacier <span class="hlt">ice</span>, and between <0.1-24 pg g-1 for Ce and <0.0004-0.02 pg g-1 for Lu in accreted <span class="hlt">ice</span>. Interestingly, the REE concentrations in the upper accreted <span class="hlt">ice</span> (AC1;characterized by visible aggregates containing a mixture of very fine terrigenous particles) and in the deeper accreted <span class="hlt">ice</span> (AC2; characterized by transparent <span class="hlt">ice</span>) are lower than those in fresh water and seawater, respectively. We suggest that such ultra-low concentrations are unlikely to be representative of the real REE <span class="hlt">content</span> in Lake Vostok, but instead may reflect phase exclusion processes occurring at the <span class="hlt">ice</span>/water interface during refreezing. In particular, the uneven spatial distribution (on the order of a few cm) and the large range of REE concentrations observed in AC1 are consistent with the occurrence/absence of the aggregates in adjacent <span class="hlt">ice</span>, and point to the presence of solid-phase concentration/exclusion processes occurring within separate pockets of frazil <span class="hlt">ice</span> during AC1 formation. Interestingly, if the LREE enrichment found in AC1 was not produced by chemical fractionation occurring in Lake Vostok water, this may reflect a contribution of bedrock material, possibly in combination with aeolian dust released into the lake by melting of the glacier <span class="hlt">ice</span>. Collectively, this valuable information provides new insight into the accreted <span class="hlt">ice</span> formation processes, the bedrock geology of East Antarctica as well as the water chemistry and circulation of Lake Vostok.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050160252','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050160252"><span>Preliminary Investigation of <span class="hlt">Ice</span> Shape Sensitivity to Parameter Variations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Miller, Dean R.; Potapczuk, Mark G.; Langhals, Tammy J.</p> <p>2005-01-01</p> <p>A parameter sensitivity study was conducted at the NASA Glenn Research Center's <span class="hlt">Icing</span> Research Tunnel (IRT) using a 36 in. chord (0.91 m) NACA-0012 airfoil. The objective of this preliminary work was to investigate the feasibility of using <span class="hlt">ice</span> shape feature changes to define requirements for the simulation and measurement of SLD <span class="hlt">icing</span> conditions. It was desired to identify the minimum change (threshold) in a parameter value, which yielded an observable change in the <span class="hlt">ice</span> shape. Liquid Water <span class="hlt">Content</span> (LWC), drop size distribution (MVD), and tunnel static temperature were varied about a nominal value, and the effects of these parameter changes on the resulting <span class="hlt">ice</span> shapes were documented. The resulting differences in <span class="hlt">ice</span> shapes were compared on the basis of qualitative and quantitative criteria (e.g., <span class="hlt">mass</span>, <span class="hlt">ice</span> horn thickness, <span class="hlt">ice</span> horn angle, <span class="hlt">icing</span> limits, and <span class="hlt">iced</span> area). This paper will provide a description of the experimental method, present selected experimental results, and conclude with an evaluation of these results, followed by a discussion of recommendations for future research.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28612479','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28612479"><span>Open-water and under-<span class="hlt">ice</span> seasonal variations in trace element <span class="hlt">content</span> and physicochemical associations in fluvial bed sediment.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Doig, Lorne E; Carr, Meghan K; Meissner, Anna G N; Jardine, Tim D; Jones, Paul D; Bharadwaj, Lalita; Lindenschmidt, Karl-Erich</p> <p>2017-11-01</p> <p>Across the circumpolar world, intensive anthropogenic activities in the southern reaches of many large, northward-flowing rivers can cause sediment contamination in the downstream depositional environment. The influence of <span class="hlt">ice</span> cover on concentrations of inorganic contaminants in bed sediment (i.e., sediment quality) is unknown in these rivers, where winter is the dominant season. A geomorphic response unit approach was used to select hydraulically diverse sampling sites across a northern test-case system, the Slave River and delta (Northwest Territories, Canada). Surface sediment samples (top 1 cm) were collected from 6 predefined geomorphic response units (12 sites) to assess the relationships between bed sediment physicochemistry (particle size distribution and total organic carbon <span class="hlt">content</span>) and trace element <span class="hlt">content</span> (mercury and 18 other trace elements) during open-water conditions. A subset of sites was resampled under-<span class="hlt">ice</span> to assess the influence of season on these relationships and on total trace element <span class="hlt">content</span>. Concentrations of the majority of trace elements were strongly correlated with percent fines and proxies for grain size (aluminum and iron), with similar trace element grain size/grain size proxy relationships between seasons. However, finer materials were deposited under <span class="hlt">ice</span> with associated increases in sediment total organic carbon <span class="hlt">content</span> and the concentrations of most trace elements investigated. The geomorphic response unit approach was effective at identifying diverse hydrological environments for sampling prior to field operations. Our data demonstrate the need for under-<span class="hlt">ice</span> sampling to confirm year-round consistency in trace element-geochemical relationships in fluvial systems and to define the upper extremes of these relationships. Whether contaminated or not, under-<span class="hlt">ice</span> bed sediment can represent a "worst-case" scenario in terms of trace element concentrations and exposure for sediment-associated organisms in northern fluvial systems</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_9 --> <div id="page_10" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="181"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1169518','SCIGOV-DOEDE'); return false;" href="https://www.osti.gov/servlets/purl/1169518"><span>Large Scale <span class="hlt">Ice</span> Water Path and 3-D <span class="hlt">Ice</span> Water <span class="hlt">Content</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/dataexplorer">DOE Data Explorer</a></p> <p>Liu, Guosheng</p> <p>2008-01-15</p> <p>Cloud <span class="hlt">ice</span> water concentration is one of the most important, yet poorly observed, cloud properties. Developing physical parameterizations used in general circulation models through single-column modeling is one of the key foci of the ARM program. In addition to the vertical profiles of temperature, water vapor and condensed water at the model grids, large-scale horizontal advective tendencies of these variables are also required as forcing terms in the single-column models. Observed horizontal advection of condensed water has not been available because the radar/lidar/radiometer observations at the ARM site are single-point measurement, therefore, do not provide horizontal distribution of condensed water. The intention of this product is to provide large-scale distribution of cloud <span class="hlt">ice</span> water by merging available surface and satellite measurements. The satellite cloud <span class="hlt">ice</span> water algorithm uses ARM ground-based measurements as baseline, produces datasets for 3-D cloud <span class="hlt">ice</span> water distributions in a 10 deg x 10 deg area near ARM site. The approach of the study is to expand a (surface) point measurement to an (satellite) areal measurement. That is, this study takes the advantage of the high quality cloud measurements at the point of ARM site. We use the cloud characteristics derived from the point measurement to guide/constrain satellite retrieval, then use the satellite algorithm to derive the cloud <span class="hlt">ice</span> water distributions within an area, i.e., 10 deg x 10 deg centered at ARM site.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12741536','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12741536"><span>Perception of melting and flavor release of <span class="hlt">ice</span> cream containing different types and <span class="hlt">contents</span> of fat.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hyvönen, L; Linna, M; Tuorila, H; Dijksterhuis, G</p> <p>2003-04-01</p> <p>Temporal effects of dairy and vegetable fats (0 to 18%) on perception of strawberry flavor release and melting of <span class="hlt">ice</span> cream were studied using the time intensity sensory method. Also, aroma and flavor attributes of the <span class="hlt">ice</span> cream samples were evaluated. Only slight effects of fat on the rate of flavor release and flavor intensity were perceived. A slightly faster flavor release from the vegetable fat compared with dairy fat was noticed. Polydextrose and maltodextrin as bodying agents in the fat-free <span class="hlt">ice</span> cream significantly increased flavor release and melting rate of the <span class="hlt">ice</span> cream. Increasing fat <span class="hlt">content</span> slightly retarded melting of <span class="hlt">ice</span> cream in the mouth. No significant effect of the fat quality on perceived melting was noticed. Significant differences in aroma and flavor attributes of the fat-free and other samples were perceived. Intensity and sharpness of the strawberry aroma and flavor were greater in fat-free samples and they were perceived as nontypical. Fattiness and creaminess were highly correlated. Maltodextrin and polydextrose increased perceived fattiness and creaminess of fat-free <span class="hlt">ice</span> cream.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170006540','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170006540"><span>Validation of a Compact Isokinetic Total Water <span class="hlt">Content</span> Probe for Wind Tunnel Characterization at NASA Glenn <span class="hlt">Icing</span> Research Tunnel and at NRC <span class="hlt">Ice</span> Crystal Tunnel</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Davison, Craig R.; Landreville, Charles; Ratvasky, Thomas P.</p> <p>2017-01-01</p> <p>A new compact isokinetic probe to measure total water <span class="hlt">content</span> in a wind tunnel environment has been developed. The probe has been previously tested under altitude conditions. This paper presents a comprehensive validation of the probe under a range of liquid water conditions at sea level in the NASA Glenn <span class="hlt">Icing</span> Research Tunnel and with <span class="hlt">ice</span> crystals at sea level at the NRC wind tunnel. The compact isokinetic probe is compared to tunnel calibrations and other probes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3950934','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3950934"><span>IR-MALDESI <span class="hlt">MASS</span> SPECTROMETRY IMAGING OF BIOLOGICAL TISSUE SECTIONS USING <span class="hlt">ICE</span> AS A MATRIX</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Robichaud, Guillaume; Barry, Jeremy A.; Muddiman, David C.</p> <p>2014-01-01</p> <p>Infrared Matrix-Assisted Laser Desorption Electrospray Ionization (IR-MALDESI) <span class="hlt">Mass</span> Spectrometry imaging of biological tissue sections using a layer of deposited <span class="hlt">ice</span> as an energy absorbing matrix was investigated. Dynamics of plume ablation were first explored using a nanosecond exposure shadowgraphy system designed to simultaneously collect pictures of the plume with a camera and collect the FT-ICR <span class="hlt">mass</span> spectrum corresponding to that same ablation event. Ablation of fresh tissue analyzed with and without using <span class="hlt">ice</span> as a matrix were both compared using this technique. Effect of spot-to-spot distance, number of laser shots per pixel and tissue condition (matrix) on ion abundance was also investigated for 50 µm thick tissue sections. Finally, the statistical method called design of experiments was used to compare source parameters and determine the optimal conditions for IR-MALDESI of tissue sections using deposited <span class="hlt">ice</span> as a matrix. With a better understanding of the fundamentals of ablation dynamics and a systematic approach to explore the experimental space, it was possible to improve ion abundance by nearly one order of magnitude. PMID:24385399</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C33B0793I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C33B0793I"><span>Spatiotemporal Patterns of <span class="hlt">Ice</span> <span class="hlt">Mass</span> Variations and the Local Climatic Factors in the Riparian Zone of Central Valley, California</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Inamdar, P.; Ambinakudige, S.</p> <p>2016-12-01</p> <p>Californian icefields are natural basins of fresh water. They provide irrigation water to the farms in the central valley. We analyzed the <span class="hlt">ice</span> <span class="hlt">mass</span> loss rates, air temperature and land surface temperature (LST) in Sacramento and San Joaquin basins in California. The digital elevation models from Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) were used to calculate <span class="hlt">ice</span> <span class="hlt">mass</span> loss rate between the years 2002 and 2015. Additionally, Landsat TIR data were used to extract the land surface temperature. Data from local weather stations were analyzed to understand the spatiotemporal trends in air temperature. The results showed an overall <span class="hlt">mass</span> recession of -0.8 ± 0.7 m w.e.a-1. We also noticed an about 60% loss in areal extent of the glaciers in the study basins between 2000 and 2015. Local climatic factors, along with the global climate patterns might have influenced the negative trends in the <span class="hlt">ice</span> <span class="hlt">mass</span> loss. Overall, there was an increase in the air temperature by 0.07± 0.02 °C in the central valley between 2000 and 2015. Furthermore, LST increased by 0.34 ± 0.4 °C and 0.55± 0.1 °C in the Sacramento and San Joaquin basins. Our preliminary results show the decrease in area and <span class="hlt">mass</span> of <span class="hlt">ice</span> <span class="hlt">mass</span> in the basins, and changing agricultural practices in the valley.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030067902','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030067902"><span>Spatial Analysis of Great Lakes Regional <span class="hlt">Icing</span> Cloud Liquid Water <span class="hlt">Content</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ryerson, Charles C.; Koenig, George G.; Melloh, Rae A.; Meese, Debra A.; Reehorst, Andrew L.; Miller, Dean R.</p> <p>2003-01-01</p> <p>Abstract Clustering of cloud microphysical conditions, such as liquid water <span class="hlt">content</span> (LWC) and drop size, can affect the rate and shape of <span class="hlt">ice</span> accretion and the airworthiness of aircraft. Clustering may also degrade the accuracy of cloud LWC measurements from radars and microwave radiometers being developed by the government for remotely mapping <span class="hlt">icing</span> conditions ahead of aircraft in flight. This paper evaluates spatial clustering of LWC in <span class="hlt">icing</span> clouds using measurements collected during NASA research flights in the Great Lakes region. We used graphical and analytical approaches to describe clustering. The analytical approach involves determining the average size of clusters and computing a clustering intensity parameter. We analyzed flight data composed of 1-s-frequency LWC measurements for 12 periods ranging from 17.4 minutes (73 km) to 45.3 minutes (190 km) in duration. Graphically some flight segments showed evidence of consistency with regard to clustering patterns. Cluster intensity varied from 0.06, indicating little clustering, to a high of 2.42. Cluster lengths ranged from 0.1 minutes (0.6 km) to 4.1 minutes (17.3 km). Additional analyses will allow us to determine if clustering climatologies can be developed to characterize cluster conditions by region, time period, or weather condition. Introduction</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..11.1656L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..11.1656L"><span>Air <span class="hlt">content</span> and O2/N2 tuned chronologies on local insolation signatures in the Vostok <span class="hlt">ice</span> core are similar</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lipenkov, V.; Raynaud, D.; Loutre, M.-F.; Duval, P.; Lemieux-Dudon, B.</p> <p>2009-04-01</p> <p>An accurate chronology of <span class="hlt">ice</span> cores is needed for interpreting the paleoclimatic record and understanding the relation between insolation and climate. A new domain of research in this area has been initially stimulated by the work of M. Bender (2002) linking the record of O2/N2 ratio in the air trapped in the Vostok <span class="hlt">ice</span> with the local insolation. More recently, it has been proposed that the long-term changes in air <span class="hlt">content</span>, V, recorded in <span class="hlt">ice</span> from the high Antarctic plateau is also dominantly imprinted by the local summer insolation (Raynaud et al., 2007). The present paper presents a new V record from Vostok, which is compared with the published Vostok O2/N2 record for the same period of time (150-400 ka BP) by using the same spectral analysis methods. The spectral differences between the two properties and the possible mechanisms linking them with insolation through the surface snow structure and the close-off processes are discussed. The main result of our study is that the two experimentally independent local insolation proxies lead to absolute (orbital) time scales, which agree together within a standard deviation of 0.6 ka. This result strongly adds credibility to the air <span class="hlt">content</span> of <span class="hlt">ice</span> and the O2 to N2 ratio of the air trapped in <span class="hlt">ice</span> as equally reliable and complementary tools for accurate dating of existing and future deep <span class="hlt">ice</span> cores. References: M. Bender, Orbital tuning chronology for the Vostok climate record supported by trapped gas composition, Earth and Planetary Science Letters 204(2002) 275-289. D. Raynaud, V. Lipenkov, B. Lemieux-Dudon, P. Duval, M.F. Loutre, N. Lhomme, The local insolation signature of air <span class="hlt">content</span> in Antarctic <span class="hlt">ice</span>: a new step toward an absolute dating of <span class="hlt">ice</span> records, Earth and Planetary Science Letters 261(2007) 337-349.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.C11D0699A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.C11D0699A"><span>Programme for Monitoring of the Greenland <span class="hlt">Ice</span> Sheet - <span class="hlt">Ice</span> Surface Velocities</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Andersen, S. B.; Ahlstrom, A. P.; Boncori, J. M.; Dall, J.</p> <p>2011-12-01</p> <p>In 2007, the Danish Ministry of Climate and Energy launched the Programme for Monitoring of the Greenland <span class="hlt">Ice</span> Sheet (PROMICE) as an ongoing effort to assess changes in the <span class="hlt">mass</span> budget of the Greenland <span class="hlt">Ice</span> Sheet. Iceberg calving from the outlet glaciers of the Greenland <span class="hlt">Ice</span> Sheet, often termed the <span class="hlt">ice</span>-dynamic <span class="hlt">mass</span> loss, is responsible for an important part of the <span class="hlt">mass</span> loss during the last decade. To quantify this part of the <span class="hlt">mass</span> loss, we combine airborne surveys yielding <span class="hlt">ice</span>-sheet thickness along the entire margin, with surface velocities derived from satellite synthetic-aperture radar (SAR). In order to derive <span class="hlt">ice</span> sheet surface velocities from SAR a processing chain has been developed for GEUS by DTU Space based on a commercial software package distributed by GAMMA Remote Sensing. The processor, named SUSIE (Scripts and Utilities for SAR <span class="hlt">Ice</span>-motion Estimation), can use both differential SAR interferometry and offset-tracking techniques to measure the horizontal velocity components, providing also an estimate of the corresponding measurement error. So far surface velocities have been derived for a number of sites including Nioghalvfjerdsfjord Glacier, the Kangerlussuaq region, the Nuuk region, Helheim Glacier and Daugaard-Jensen Glacier using data from ERS-1/ERS-2, ENVISAT ASAR and ALOS Palsar. Here we will present these first results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3917821','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3917821"><span><span class="hlt">Ice</span> hockey lung – a case of <span class="hlt">mass</span> nitrogen dioxide poisoning in the Czech Republic</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Brat, Kristian; Merta, Zdenek; Plutinsky, Marek; Skrickova, Jana; Ing, Miroslav Stanek</p> <p>2013-01-01</p> <p>Nitrogen dioxide (NO2) is a toxic gas, a product of combustion in malfunctioning <span class="hlt">ice</span>-resurfacing machines. NO2 poisoning is rare but potentially lethal. The authors report a case of <span class="hlt">mass</span> NO2 poisoning involving 15 amateur <span class="hlt">ice</span> hockey players in the Czech Republic. All players were treated in the Department of Respiratory Diseases at Brno University Hospital in November 2010 – three as inpatients because they developed pneumonitis. All patients were followed-up until November 2011. Complete recovery in all but one patient was achieved by December 2010. None of the 15 patients developed asthma-like disease or chronic cough. Corticosteroids appeared to be useful in treatment. Electric-powered <span class="hlt">ice</span>-resurfacing machines are preferable in indoor <span class="hlt">ice</span> skating arenas. PMID:24032121</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27904363','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27904363"><span>Effects of Green Banana Flour on the Physical, Chemical and Sensory Properties of <span class="hlt">Ice</span> Cream.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yangılar, Filiz</p> <p>2015-09-01</p> <p>In the present study, possible effects of the addition of banana flour at different <span class="hlt">mass</span> fractions (1 and 2%) are investigated on physical (overrun, viscosity), chemical (dry matter, fat and ash <span class="hlt">content</span>, acidity, pH, water and oil holding capacity and colour), mineral <span class="hlt">content</span> (Ca, K, Na, P, S, Mg, Fe, Mn, Zn and Ni) and sensory properties of <span class="hlt">ice</span> cream. Fibre--rich banana pieces were found to contain 66.8 g per 100 g of total dietary fibre, 58.6 g per 100 g of which were insoluble dietary fibre, while 8.2 g per 100 g were soluble dietary fibre. It can be concluded from these results that banana is a valuable dietary fibre source which can be used in food production. Flour obtained from green banana pulp and peel was found to have significant (p<0.05) effect on the chemical composition of <span class="hlt">ice</span> creams. Sulphur <span class="hlt">content</span> increased while calcium <span class="hlt">content</span> decreased in <span class="hlt">ice</span> cream depending on banana flour <span class="hlt">content</span>. Sensory results indicated that <span class="hlt">ice</span> cream sample containing 2% of green banana pulp flour received the highest score from panellists.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1912332S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1912332S"><span>Geodetic glacier <span class="hlt">mass</span> balancing on <span class="hlt">ice</span> caps - inseparably connected to firn modelling?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Saß, Björn L.; Sauter, Tobias; Seehaus, Thorsten; Braun, Matthias H.</p> <p>2017-04-01</p> <p>Observed melting of glaciers and <span class="hlt">ice</span> caps in the polar regions contribute to the ongoing global sea level rise (SLR). A rising sea level and its consequences are one of the major challenges for coastal societies in the next decades to centuries. Gaining knowledge about the main drivers of SLR and bringing it together is one recent key-challenge for environmental science. The high arctic Svalbard archipelago faced a strong climatic change in the last decades, associated with a change in the cryosphere. Vestfonna, a major Arctic <span class="hlt">ice</span> cap in the north east of Svalbard, harbors land and marine terminating glaciers, which expose a variability of behavior. We use high resolution remote sensing data from space-borne radar (TanDEM-X, TerraSAR-X, Sentinel-1a), acquired between 2009 and 2015, to estimate glacier velocity and high accurate surface elevation changes. For DEM registration we use space-borne laser altimetry (ICESat) and an existing in-situ data archive (IPY Kinnvika). In order to separate individual glacier basin changes for a detailed <span class="hlt">mass</span> balance study and for further SLR contribution estimates, we use glacier outlines from the Global Land <span class="hlt">Ice</span> Measurements from Space (GLIMS) project. Remaining challenges of space-borne observations are the reduction of measurement uncertainties, in the case of Synthetic Aperture Radar most notably signal penetration into the glacier surface. Furthermore, in order to convert volume to <span class="hlt">mass</span> change one has to use the density of the changed <span class="hlt">mass</span> (conversion factor) and one has to account for the <span class="hlt">mass</span> conservation processes in the firn package (firn compaction). Both, the conversion factor and the firn compaction are not (yet) measurable for extensive <span class="hlt">ice</span> bodies. They have to be modelled by coupling point measurements and regional gridded climate data. Results indicate a slight interior thickening contrasted with wide spread thinning in the ablation zone of the marine terminating outlets. While one glacier system draining to the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018TCry...12.1273R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018TCry...12.1273R"><span>Changing pattern of <span class="hlt">ice</span> flow and <span class="hlt">mass</span> balance for glaciers discharging into the Larsen A and B embayments, Antarctic Peninsula, 2011 to 2016</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rott, Helmut; Abdel Jaber, Wael; Wuite, Jan; Scheiblauer, Stefan; Floricioiu, Dana; Melchior van Wessem, Jan; Nagler, Thomas; Miranda, Nuno; van den Broeke, Michiel R.</p> <p>2018-04-01</p> <p>We analysed volume change and <span class="hlt">mass</span> balance of outlet glaciers on the northern Antarctic Peninsula over the periods 2011 to 2013 and 2013 to 2016, using high-resolution topographic data from the bistatic interferometric radar satellite mission TanDEM-X. Complementary to the geodetic method that applies DEM differencing, we computed the net <span class="hlt">mass</span> balance of the main outlet glaciers using the <span class="hlt">mass</span> budget method, accounting for the difference between the surface <span class="hlt">mass</span> balance (SMB) and the discharge of <span class="hlt">ice</span> into an ocean or <span class="hlt">ice</span> shelf. The SMB values are based on output of the regional climate model RACMO version 2.3p2. To study glacier flow and retrieve <span class="hlt">ice</span> discharge we generated time series of <span class="hlt">ice</span> velocity from data from different satellite radar sensors, with radar images of the satellites TerraSAR-X and TanDEM-X as the main source. The study area comprises tributaries to the Larsen A, Larsen Inlet and Prince Gustav Channel embayments (region A), the glaciers calving into the Larsen B embayment (region B) and the glaciers draining into the remnant part of the Larsen B <span class="hlt">ice</span> shelf in Scar Inlet (region C). The glaciers of region A, where the buttressing <span class="hlt">ice</span> shelf disintegrated in 1995, and of region B (<span class="hlt">ice</span> shelf break-up in 2002) show continuing losses in <span class="hlt">ice</span> <span class="hlt">mass</span>, with significant reduction of losses after 2013. The <span class="hlt">mass</span> balance numbers for the grounded glacier area of region A are -3.98 ± 0.33 Gt a-1 from 2011 to 2013 and -2.38 ± 0.18 Gt a-1 from 2013 to 2016. The corresponding numbers for region B are -5.75 ± 0.45 and -2.32 ± 0.25 Gt a-1. The <span class="hlt">mass</span> balance in region C during the two periods was slightly negative, at -0.54 ± 0.38 Gt a-1 and -0.58 ± 0.25 Gt a-1. The main share in the overall <span class="hlt">mass</span> losses of the region was contributed by two glaciers: Drygalski Glacier contributing 61 % to the <span class="hlt">mass</span> deficit of region A, and Hektoria and Green glaciers accounting for 67 % to the <span class="hlt">mass</span> deficit of region B. Hektoria and Green glaciers accelerated significantly in 2010</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19890004057','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19890004057"><span>Analytical <span class="hlt">ice</span> shape predictions for flight in natural <span class="hlt">icing</span> conditions</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Berkowitz, Brian M.; Riley, James T.</p> <p>1988-01-01</p> <p>LEWICE is an analytical <span class="hlt">ice</span> prediction code that has been evaluated against <span class="hlt">icing</span> tunnel data, but on a more limited basis against flight data. <span class="hlt">Ice</span> shapes predicted by LEWICE is compared with experimental <span class="hlt">ice</span> shapes accreted on the NASA Lewis <span class="hlt">Icing</span> Research Aircraft. The flight data selected for comparison includes liquid water <span class="hlt">content</span> recorded using a hot wire device and droplet distribution data from a laser spectrometer; the <span class="hlt">ice</span> shape is recorded using stereo photography. The main findings are as follows: (1) An equivalent sand grain roughness correlation different from that used for LEWICE tunnel comparisons must be employed to obtain satisfactory results for flight; (2) Using this correlation and making no other changes in the code, the comparisons to <span class="hlt">ice</span> shapes accreted in flight are in general as good as the comparisons to <span class="hlt">ice</span> shapes accreted in the tunnel (as in the case of tunnel <span class="hlt">ice</span> shapes, agreement is least reliable for large glaze <span class="hlt">ice</span> shapes at high angles of attack); (3) In some cases comparisons can be somewhat improved by utilizing the code so as to take account of the variation of parameters such as liquid water <span class="hlt">content</span>, which may vary significantly in flight.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.C53B0574L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.C53B0574L"><span><span class="hlt">Ice</span> Shelf-Ocean Interactions Near <span class="hlt">Ice</span> Rises and <span class="hlt">Ice</span> Rumples</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lange, M. A.; Rückamp, M.; Kleiner, T.</p> <p>2013-12-01</p> <p>The stability of <span class="hlt">ice</span> shelves depends on the existence of embayments and is largely influenced by <span class="hlt">ice</span> rises and <span class="hlt">ice</span> rumples, which act as 'pinning-points' for <span class="hlt">ice</span> shelf movement. Of additional critical importance are interactions between <span class="hlt">ice</span> shelves and the water <span class="hlt">masses</span> underlying them in <span class="hlt">ice</span> shelf cavities, particularly melting and refreezing processes. The present study aims to elucidate the role of <span class="hlt">ice</span> rises and <span class="hlt">ice</span> rumples in the context of climate change impacts on Antarctic <span class="hlt">ice</span> shelves. However, due to their smaller spatial extent, <span class="hlt">ice</span> rumples react more sensitively to climate change than <span class="hlt">ice</span> rises. Different forcings are at work and need to be considered separately as well as synergistically. In order to address these issues, we have decided to deal with the following three issues explicitly: oceanographic-, cryospheric and general topics. In so doing, we paid particular attention to possible interrelationships and feedbacks in a coupled <span class="hlt">ice</span>-shelf-ocean system. With regard to oceanographic issues, we have applied the ocean circulation model ROMBAX to ocean water <span class="hlt">masses</span> adjacent to and underneath a number of idealized <span class="hlt">ice</span> shelf configurations: wide and narrow as well as laterally restrained and unrestrained <span class="hlt">ice</span> shelves. Simulations were performed with and without small <span class="hlt">ice</span> rises located close to the calving front. For larger configurations, the impact of the <span class="hlt">ice</span> rises on melt rates at the <span class="hlt">ice</span> shelf base is negligible, while for smaller configurations net melting rates at the <span class="hlt">ice</span>-shelf base differ by a factor of up to eight depending on whether <span class="hlt">ice</span> rises are considered or not. We employed the thermo-coupled <span class="hlt">ice</span> flow model TIM-FD3 to simulate the effects of several <span class="hlt">ice</span> rises and one <span class="hlt">ice</span> rumple on the dynamics of <span class="hlt">ice</span> shelf flow. We considered the complete un-grounding of the <span class="hlt">ice</span> shelf in order to investigate the effect of pinning points of different characteristics (interior or near calving front, small and medium sized) on the resulting flow and stress fields</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016TCry...10.1965S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016TCry...10.1965S"><span>Application of GRACE to the assessment of model-based estimates of monthly Greenland <span class="hlt">Ice</span> Sheet <span class="hlt">mass</span> balance (2003-2012)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schlegel, Nicole-Jeanne; Wiese, David N.; Larour, Eric Y.; Watkins, Michael M.; Box, Jason E.; Fettweis, Xavier; van den Broeke, Michiel R.</p> <p>2016-09-01</p> <p>Quantifying the Greenland <span class="hlt">Ice</span> Sheet's future contribution to sea level rise is a challenging task that requires accurate estimates of <span class="hlt">ice</span> sheet sensitivity to climate change. Forward <span class="hlt">ice</span> sheet models are promising tools for estimating future <span class="hlt">ice</span> sheet behavior, yet confidence is low because evaluation of historical simulations is challenging due to the scarcity of continental-wide data for model evaluation. Recent advancements in processing of Gravity Recovery and Climate Experiment (GRACE) data using Bayesian-constrained <span class="hlt">mass</span> concentration ("mascon") functions have led to improvements in spatial resolution and noise reduction of monthly global gravity fields. Specifically, the Jet Propulsion Laboratory's JPL RL05M GRACE mascon solution (GRACE_JPL) offers an opportunity for the assessment of model-based estimates of <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balance (MB) at ˜ 300 km spatial scales. Here, we quantify the differences between Greenland monthly observed MB (GRACE_JPL) and that estimated by state-of-the-art, high-resolution models, with respect to GRACE_JPL and model uncertainties. To simulate the years 2003-2012, we force the <span class="hlt">Ice</span> Sheet System Model (ISSM) with anomalies from three different surface <span class="hlt">mass</span> balance (SMB) products derived from regional climate models. Resulting MB is compared against GRACE_JPL within individual mascons. Overall, we find agreement in the northeast and southwest where MB is assumed to be primarily controlled by SMB. In the interior, we find a discrepancy in trend, which we presume to be related to millennial-scale dynamic thickening not considered by our model. In the northwest, seasonal amplitudes agree, but modeled <span class="hlt">mass</span> trends are muted relative to GRACE_JPL. Here, discrepancies are likely controlled by temporal variability in <span class="hlt">ice</span> discharge and other related processes not represented by our model simulations, i.e., hydrological processes and <span class="hlt">ice</span>-ocean interaction. In the southeast, GRACE_JPL exhibits larger seasonal amplitude than predicted by</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUFM.U44A..01A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUFM.U44A..01A"><span>Recent Changes in Arctic Glaciers, <span class="hlt">Ice</span> Caps, and the Greenland <span class="hlt">Ice</span> Sheet: Cold Facts About Warm <span class="hlt">Ice</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Abdalati, W.</p> <p>2005-12-01</p> <p>One of the major manifestations of Arctic change can be observed in the state of balance of Arctic glaciers and <span class="hlt">ice</span> caps and the Greenland <span class="hlt">ice</span> sheet. These <span class="hlt">ice</span> <span class="hlt">masses</span> are estimated to contain nearly 3 million cubic kilometers of <span class="hlt">ice</span>, which is more than six times greater than all the water stored in the Earth's lakes, rivers, and snow combined and is the equivalent of over 7 meters of sea level. Most of these <span class="hlt">ice</span> <span class="hlt">masses</span> have been shrinking in recent in years, but their <span class="hlt">mass</span> balance is highly variable on a wide range of spatial and temporal scales. On the Greenland <span class="hlt">ice</span> sheet most of the coastal regions have thinned substantially as melt has increased and some of its outlet glaciers have accelerated. Near the equilibrium line in West Greenland, we have seen evidence of summer acceleration that is linked to surface meltwater production, suggesting a relatively rapid response mechanism of the <span class="hlt">ice</span> sheet change to a warming climate. At the same time, however, the vast interior regions of the Greenland <span class="hlt">ice</span> sheet have shown little change or slight growth, as accumulation in these areas may have increased. Throughout much of the rest of the Arctic, many glaciers and <span class="hlt">ice</span> caps have been shrinking in the past few decades, and in Canada and Alaska, the rate of <span class="hlt">ice</span> loss seems to have accelerated during the late 1990s. These recent observations offer only a snapshot in time of the long-term behavior, but they are providing crucial information about the current state of <span class="hlt">ice</span> <span class="hlt">mass</span> balance and the mechanisms that control it in one of the most climatically sensitive regions on Earth. As we continue to learn more through a combination of remote sensing observations, in situ measurements and improved modeling capabilities, it is important that we coordinate and integrate these approaches effectively in order to predict future changes and their impact on sea level, freshwater discharge, and ocean circulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12712582','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12712582"><span>[Dynamics of ecological-biochemical characteristics of the sea <span class="hlt">ice</span> in the coastal zone of the White sea].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mel'nikov, I A; Korneeva, G A; zhitina, L S; Shanin, S S</p> <p>2003-01-01</p> <p>The distribution of salinity, silicon and phosphorus <span class="hlt">contents</span>, and hydrolytic enzyme activities along a sea-coast transect was studied in melted <span class="hlt">ice</span> cores and water samples taken from under the <span class="hlt">ice</span> cover in the periods of active <span class="hlt">ice</span> formation and melting in the Kandalaksha Bay, White Sea. The species list of identified algae was compiled, which included 170 species and varieties (90% of them belonged to diatoms). Strong correlations were revealed between the salinity of water samples and the <span class="hlt">content</span> of silicon, protease activity, and the species composition of algae. Preliminary estimations of the rate of photosynthetic processes in individual cells of algae belonging to the <span class="hlt">mass</span> species of the <span class="hlt">ice</span> flora are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ACP....17.9599S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ACP....17.9599S"><span>A ubiquitous <span class="hlt">ice</span> size bias in simulations of tropical deep convection</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stanford, McKenna W.; Varble, Adam; Zipser, Ed; Strapp, J. Walter; Leroy, Delphine; Schwarzenboeck, Alfons; Potts, Rodney; Protat, Alain</p> <p>2017-08-01</p> <p>The High Altitude <span class="hlt">Ice</span> Crystals - High <span class="hlt">Ice</span> Water <span class="hlt">Content</span> (HAIC-HIWC) joint field campaign produced aircraft retrievals of total condensed water <span class="hlt">content</span> (TWC), hydrometeor particle size distributions (PSDs), and vertical velocity (w) in high <span class="hlt">ice</span> water <span class="hlt">content</span> regions of mature and decaying tropical mesoscale convective systems (MCSs). The resulting dataset is used here to explore causes of the commonly documented high bias in radar reflectivity within cloud-resolving simulations of deep convection. This bias has been linked to overly strong simulated convective updrafts lofting excessive condensate <span class="hlt">mass</span> but is also modulated by parameterizations of hydrometeor size distributions, single particle properties, species separation, and microphysical processes. Observations are compared with three Weather Research and Forecasting model simulations of an observed MCS using different microphysics parameterizations while controlling for w, TWC, and temperature. Two popular bulk microphysics schemes (Thompson and Morrison) and one bin microphysics scheme (fast spectral bin microphysics) are compared. For temperatures between -10 and -40 °C and TWC > 1 g m-3, all microphysics schemes produce median <span class="hlt">mass</span> diameters (MMDs) that are generally larger than observed, and the precipitating <span class="hlt">ice</span> species that controls this size bias varies by scheme, temperature, and w. Despite a much greater number of samples, all simulations fail to reproduce observed high-TWC conditions ( > 2 g m-3) between -20 and -40 °C in which only a small fraction of condensate <span class="hlt">mass</span> is found in relatively large particle sizes greater than 1 mm in diameter. Although more <span class="hlt">mass</span> is distributed to large particle sizes relative to those observed across all schemes when controlling for temperature, w, and TWC, differences with observations are significantly variable between the schemes tested. As a result, this bias is hypothesized to partly result from errors in parameterized hydrometeor PSD and single particle</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70026900','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70026900"><span>Reconciling different observations of the CO2 <span class="hlt">ice</span> <span class="hlt">mass</span> loading of the Martian north polar cap</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Haberle, R.M.; Mattingly, B.; Titus, T.N.</p> <p>2004-01-01</p> <p>The GRS measurements of the peak <span class="hlt">mass</span> loading of the north polar CO2 <span class="hlt">ice</span> cap on Mars are about 60% lower than those calculated from MGS TES radiation data and those inferred from the MOLA cap thicknesses. However, the GRS data provide the most accurate measurement of the <span class="hlt">mass</span> loading. We show that the TES and MOLA data can be reconciled with the GRS data if (1) subsurface heat conduction and atmospheric heat transport are included in the TES <span class="hlt">mass</span> budget calculations, and (2) the density of the polar deposits is ???600 kg m-3. The latter is much less than that expected for slab <span class="hlt">ice</span> (???1600 kg m-3) and suggests that processes unique to the north polar region are responsible for the low cap density. Copyright 2004 by the American Geophysical Union.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20170004574&hterms=antarctica+mean&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DWhat%2Bantarctica%2Bmean','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20170004574&hterms=antarctica+mean&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DWhat%2Bantarctica%2Bmean"><span><span class="hlt">Ice</span> <span class="hlt">Mass</span> Change in Greenland and Antarctica Between 1993 and 2013 from Satellite Gravity Measurements</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Talpe, Matthieu J.; Nerem, R. Steven; Forootan, Ehsan; Schmidt, Michael; Lemoine, Frank G.; Enderlin, Ellyn M.; Landerer, Felix W.</p> <p>2017-01-01</p> <p>We construct long-term time series of Greenland and Antarctic <span class="hlt">ice</span> sheet <span class="hlt">mass</span> change from satellite gravity measurements. A statistical reconstruction approach is developed based on a principal component analysis (PCA) to combine high-resolution spatial modes from the Gravity Recovery and Climate Experiment (GRACE) mission with the gravity information from conventional satellite tracking data. Uncertainties of this reconstruction are rigorously assessed; they include temporal limitations for short GRACE measurements, spatial limitations for the low-resolution conventional tracking data measurements, and limitations of the estimated statistical relationships between low- and high-degree potential coefficients reflected in the PCA modes. Trends of <span class="hlt">mass</span> variations in Greenland and Antarctica are assessed against a number of previous studies. The resulting time series for Greenland show a higher rate of <span class="hlt">mass</span> loss than other methods before 2000, while the Antarctic <span class="hlt">ice</span> sheet appears heavily influenced by interannual variations.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_10 --> <div id="page_11" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="201"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014ACP....14.1205J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014ACP....14.1205J"><span>On the relationship between Arctic <span class="hlt">ice</span> clouds and polluted air <span class="hlt">masses</span> over the North Slope of Alaska in April 2008</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jouan, C.; Pelon, J.; Girard, E.; Ancellet, G.; Blanchet, J. P.; Delanoë, J.</p> <p>2014-02-01</p> <p>Recently, two types of <span class="hlt">ice</span> clouds (TICs) properties have been characterized using the Indirect and Semi-Direct Aerosol Campaign (ISDAC) airborne measurements (Alaska, April 2008). TIC-2B were characterized by fewer (< 10 L-1) and larger (> 110 μm) <span class="hlt">ice</span> crystals, and a larger <span class="hlt">ice</span> supersaturation (> 15%) compared to TIC-1/2A. It has been hypothesized that emissions of SO2 may reduce the <span class="hlt">ice</span> nucleating properties of <span class="hlt">ice</span> nuclei (IN) through acidification, resulting in a smaller concentration of larger <span class="hlt">ice</span> crystals and leading to precipitation (e.g., cloud regime TIC-2B). Here, the origin of air <span class="hlt">masses</span> forming the ISDAC TIC-1/2A (1 April 2008) and TIC-2B (15 April 2008) is investigated using trajectory tools and satellite data. Results show that the synoptic conditions favor air <span class="hlt">masses</span> transport from three potential SO2 emission sources into Alaska: eastern China and Siberia where anthropogenic and biomass burning emissions, respectively, are produced, and the volcanic region of the Kamchatka/Aleutians. Weather conditions allow the accumulation of pollutants from eastern China and Siberia over Alaska, most probably with the contribution of acidic volcanic aerosol during the TIC-2B period. Observation Monitoring Instrument (OMI) satellite observations reveal that SO2 concentrations in air <span class="hlt">masses</span> forming the TIC-2B were larger than in air <span class="hlt">masses</span> forming the TIC-1/2A. Airborne measurements show high acidity near the TIC-2B flight where humidity was low. These results support the hypothesis that acidic coating on IN could be at the origin of the formation of TIC-2B.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.B21F..01H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.B21F..01H"><span>Pedogenesis on <span class="hlt">ice</span> (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hodson, A. J.</p> <p>2010-12-01</p> <p>It is well known from <span class="hlt">ice</span> cores that organic and mineral debris accumulates within glacier <span class="hlt">ice</span> following atmospheric deposition. However, the concentrations of such debris are usually greatest upon the <span class="hlt">ice</span> surface, especially at the margins of continental glaciers and <span class="hlt">ice</span> sheets, where it forms mm-scale aggregate particles called “cryoconite”. According to the literature, cryoconite covers about 2 % of the ablation areas of glaciers outside Greenland and Antarctica, equivalent to a <span class="hlt">mass</span> loading of ca. 25 g/m2. Of the great <span class="hlt">ice</span> sheets not included in this figure, Greenland is the easiest to estimate, and new observations from the NE and SW sectors indicate <span class="hlt">mass</span> loadings in the range 17 - 440 g/m2. Studies of cryoconite often report the presence of a significant biomass (usually 10^4 - 10^7 cells/g) that is capable of a wide range of biogeochemical functions. The first part of this presentation will therefore explore the <span class="hlt">contention</span> that the formation of cryoconite represents the first stages of pedogenesis, resulting in the production of soil-type aggregates that inoculate glacial forefields following glacier retreat. Emphasis will be given to the relevant processes that result in aggregate formation, including rapid cell-mineral attachment within melting snowpacks and the slower, biological processes of cementation within thermodynamically stable habitats such as cryoconite holes. The second part of the presentation will use examples from Svalbard, Greenland and Antarctica to consider the carbon balance of the cryoconite during the longest phase of its life cycle: upon the <span class="hlt">ice</span>. It will be demonstrated how the efficacy of photosynthesis is strongly influenced by thermodynamic conditions at or near this surface. Data from the Greenland and Antarctic <span class="hlt">ice</span> sheets will show how thermal equilibration decouples variations in photosynthesis from variations in incident radiation over timescales > 1 d, resulting in an equitable, low-carbon economy for aggregates within</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUFM.C41A..02R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUFM.C41A..02R"><span>Leakage of the Greenland <span class="hlt">Ice</span> Sheet through accelerated <span class="hlt">ice</span> flow</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rignot, E.</p> <p>2005-12-01</p> <p>A map of coastal velocities of the Greenland <span class="hlt">ice</span> sheet was produced from Radarsat-1 acquired during the background mission of 2000 and combined with radio echo sounding data to estimate the <span class="hlt">ice</span> discharge from the <span class="hlt">ice</span> sheet. On individual glaciers, <span class="hlt">ice</span> discharge was compared with snow input from the interior and melt above the flux gate to determine the glacier <span class="hlt">mass</span> balance. Time series of velocities on several glaciers at different latitudes reveal seasonal fluctuations of only 7-8 percent so that winter velocities are only 2 percent less than the yearly mean. The results show the northern Greenland glaciers to be close to balance yet losing <span class="hlt">mass</span>. No change in <span class="hlt">ice</span> flow is detected on Petermann, 79north and Zachariae Isstrom in 2000-2004. East Greenland glaciers are in balance and flowing steadily north of Kangerdlussuaq, but Kangerdlussuaq, Helheim and all the southeastern glaciers are thinning dramatically. All these glaciers accelerated, Kangerdlussuaq in 2000, Helheim prior to 2004, and southeast Greenland glaciers accelerated 10 to 50 percent in 2000-2004. Glacier acceleration is generally brutal, probably once the glacier reached a threshold, and sustained. In the northwest, most glaciers are largely out of balance. Jakobshavn accelerated significantly in 2002, and glaciers in its immediate vicinity accelerated more than 50 percent in 2000-2004. Less is known about southwest Greenland glaciers due to a lack of <span class="hlt">ice</span> thickness data but the glaciers have accelerated there as well and are likely to be strongly out of balance despite thickening of the interior. Overall, I estimate the <span class="hlt">mass</span> balance of the Greenland <span class="hlt">ice</span> sheet to be about -80 +/-10 cubic km of <span class="hlt">ice</span> per year in 2000 and -110 +/-15 cubic km of <span class="hlt">ice</span> per year in 2004, i.e. more negative than based on partial altimetry surveys of the outlet glaciers. As climate continues to warm, more glaciers will accelerate, and the <span class="hlt">mass</span> balance will become increasingly negative, regardless of the evolution of the <span class="hlt">ice</span> sheet</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.1579W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.1579W"><span>Early 21st-Century <span class="hlt">Mass</span> loss of the North-Atlantic Glaciers and <span class="hlt">Ice</span> Caps (Arne Richter Award for Outstanding Young Scientists Lecture)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wouters, Bert; Ligtenberg, Stefan; Moholdt, Geir; Gardner, Alex S.; Noel, Brice; Kuipers Munneke, Peter; van den Broeke, Michiel; Bamber, Jonathan L.</p> <p>2016-04-01</p> <p>Historically, <span class="hlt">ice</span> loss from mountain glaciers and <span class="hlt">ice</span> caps has been one of the largest contributors to sea level rise over the last century. Of particular interest are the glaciers and <span class="hlt">ice</span> caps in the North-Atlantic region of the Arctic. Despite the cold climate in this area, considerable melting and runoff occurs in summer. A small increase in temperature will have an immediate effect on these processes, so that a large change in the Arctic <span class="hlt">ice</span> volume can be expected in response to the anticipated climate change in the coming century. Unfortunately, direct observations of glaciers are sparse and are biased toward glaciers systems in accessible, mostly maritime, climate conditions. Remote sensing is therefore essential to monitor the state of the the North-Atlantic glaciers and <span class="hlt">ice</span> caps. In this presentation, we will discuss the progress that has been made in estimating the <span class="hlt">ice</span> <span class="hlt">mass</span> balance of these regions, with a particular focus on measurements made by ESA's Cryosat-2 radar altimeter mission (2010-present). Compared to earlier altimeter mission, Cryosat-2 provides unprecedented coverage of the cryosphere, with a resolution down to 1 km or better and sampling at monthly intervals. Combining the Cryosat-2 measurements with the laser altimetry data from ICESat (2003-2009) gives us a 12 yr time series of glacial <span class="hlt">mass</span> loss in the North Atlantic. We find excellent agreement between the altimetry measurements and independent observations by the GRACE mission, which directly 'weighs' the <span class="hlt">ice</span> caps, albeit at a much lower resolution. <span class="hlt">Mass</span> loss in the region has increased from 120 Gigatonnes per year in 2003-2009 to roughly 140 Gt/yr in 2010-2014, with an important contribution from Greenland's peripheral glaciers and <span class="hlt">ice</span> caps. Importantly, the <span class="hlt">mass</span> loss is not stationary, but shows large regional interannual variability, with <span class="hlt">mass</span> loss shifting between eastern and western regions from year to year. Comparison with regional climate models shows that these shifts can be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15131987','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15131987"><span>[Radiocarbon dating of pollen and spores in wedge <span class="hlt">ice</span> from Iamal and Kolyma].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Vasil'chuk, A K</p> <p>2004-01-01</p> <p>Radiocarbon dating of pollen concentrate from late Pleistocene syngenetic wedge <span class="hlt">ice</span> was carried out using acceleration <span class="hlt">mass</span> spectrometry (AMS) in Seyakha and Bizon sections. Comparison of the obtained dating with palynological analysis and AMS radiocarbon dating previously obtained for other organic fractions of the same samples allowed us to evaluate accuracy of dating of different fractions. Quantitative tests for data evaluation were considered in terms of possible autochthonous or allochthonous accumulation of the material on the basis of pre-Pleistocene pollen <span class="hlt">content</span> in these samples. Paleoecological information <span class="hlt">content</span> of pollen spectra from late Pleistocene syngenetic wedge <span class="hlt">ice</span> was evaluated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5068378','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5068378"><span>Effects of Green Banana Flour on the Physical, Chemical and Sensory Properties of <span class="hlt">Ice</span> Cream</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p></p> <p>2015-01-01</p> <p>Summary In the present study, possible effects of the addition of banana flour at different <span class="hlt">mass</span> fractions (1 and 2%) are investigated on physical (overrun, viscosity), chemical (dry matter, fat and ash <span class="hlt">content</span>, acidity, pH, water and oil holding capacity and colour), mineral <span class="hlt">content</span> (Ca, K, Na, P, S, Mg, Fe, Mn, Zn and Ni) and sensory properties of <span class="hlt">ice</span> cream. Fibre--rich banana pieces were found to contain 66.8 g per 100 g of total dietary fibre, 58.6 g per 100 g of which were insoluble dietary fibre, while 8.2 g per 100 g were soluble dietary fibre. It can be concluded from these results that banana is a valuable dietary fibre source which can be used in food production. Flour obtained from green banana pulp and peel was found to have significant (p<0.05) effect on the chemical composition of <span class="hlt">ice</span> creams. Sulphur <span class="hlt">content</span> increased while calcium <span class="hlt">content</span> decreased in <span class="hlt">ice</span> cream depending on banana flour <span class="hlt">content</span>. Sensory results indicated that <span class="hlt">ice</span> cream sample containing 2% of green banana pulp flour received the highest score from panellists. PMID:27904363</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1712799K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1712799K"><span>Characterization of signatures from organic compounds in CDA <span class="hlt">mass</span> spectra of <span class="hlt">ice</span> particles in Saturn's E-ring</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Khawaja, Nozair; Postberg, Frank; Reviol, Rene; Srama, Ralf</p> <p>2015-04-01</p> <p>The major source of <span class="hlt">ice</span> particles in Saturn's E-ring is Enceladus - a geological active moon of Saturn. Enceladus is emanating <span class="hlt">ice</span> particles from its fractured south polar terrain (SPT), the so-called "Tiger Stripes". The source of Enceladus activity and many of the <span class="hlt">ice</span> particles is a subsurface ocean. The Cosmic Dust Analyzer (CDA) onboard the Cassini spacecraft is sampling these icy particles and producing TOF <span class="hlt">mass</span> spectra of cations of impinging particles [1]. Three compositional types of <span class="hlt">ice</span> particles have been identified from CDA-<span class="hlt">mass</span> spectra: (i) pure water <span class="hlt">ice</span> (Type-1) (ii) organic rich (Type-2) (iii) salt rich (Type-3) [2][3]. These organic rich (Type-2) spectra are particularly abundant in the icy jets of Enceladus as we found out during the Cassini's Enceladus flybys (E17 and E18) in 2012 [4]. We present a compositional analysis of the CDA spectra of these organic rich icy grains sampled in the E ring. We have characterized hundreds of Type-2 spectra of impinging <span class="hlt">ice</span> particles. These were recorded at different impact velocities causing different molecular fragmentation patterns observed in the <span class="hlt">mass</span> spectra. We defined 3 typical impact speed intervals: (i) 4-7 km/s (ii) 8-11 km/s and (iii) 12-16km/s. Organic features best observed at slow (4-7 km/s) or at intermediate (8-11 km/s) impact velocity ranges. Several classes of organic rich spectra are identified. Classifying Type-2 spectra are according to their characteristic <span class="hlt">mass</span> lines of possible organic species. We try to infer the composition of each class of organic rich spectra is inferred by using an experimental setup (IR-FL-MALDI) to simulate the CDA spectra of different compositional types. In the laboratory we have used infrared laser to disperse a micro-beam of a water solution [5]. The laser energy is adjusted to simulate different impact velocities of <span class="hlt">ice</span> particles on the CDA. Four families of organic compounds including alcohols, fatty acids, amines and aromatic, with varying number of carbon</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.C54A..03L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.C54A..03L"><span>Inferring unknow boundary conditions of the Greenland <span class="hlt">Ice</span> Sheet by assimilating ICESat-1 and <span class="hlt">Ice</span>Bridge altimetry intothe <span class="hlt">Ice</span> Sheet System Model.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Larour, E. Y.; Khazendar, A.; Seroussi, H. L.; Schlegel, N.; Csatho, B. M.; Schenk, A. F.; Rignot, E. J.; Morlighem, M.</p> <p>2014-12-01</p> <p>Altimetry signals from missions such as ICESat-1, CryoSat, EnviSat, as well as altimeters onboard Operation <span class="hlt">Ice</span>Bridge provide vital insights into processes such as surface <span class="hlt">mass</span> balance, <span class="hlt">mass</span> transport and <span class="hlt">ice</span>-flow dynamics. Historically however, <span class="hlt">ice</span>-flow models have been focused on assimilating surface velocities from satellite-based radar observations, to infer properties such as basal friction or the position of the bedrock. Here, we leverage a new methodology based on automatic differentation of the <span class="hlt">Ice</span> Sheet System Model to assimilate surface altimetry data into a reconstruction of the past decade of <span class="hlt">ice</span> flow on the North Greenland area. We infer corrections to boundary conditions such as basal friction and surface <span class="hlt">mass</span> balance, as well as corrections to the <span class="hlt">ice</span> hardness, to best-match the observed altimetry record. We compare these corrections between glaciers such as Petermann Glacier, 79 North and Zacchariae Isstrom. The altimetry signals exhibit very different patterns between East and West, which translate into very different signatures for the inverted boundary conditions. This study gives us greater insights into what differentiates different basins, both in terms of <span class="hlt">mass</span> transport and <span class="hlt">ice</span>-flow dynamics, and what could bethe controlling mechanisms behind the very different evolutions of these basins.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140006602','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140006602"><span>Dynamic Inland Propagation of Thinning Due to <span class="hlt">Ice</span> Loss at the Margins of the Greenland <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wang, Wei Li; Li, Jun J.; Zwally, H. Jay</p> <p>2012-01-01</p> <p><span class="hlt">Mass</span>-balance analysis of the Greenland <span class="hlt">ice</span> sheet based on surface elevation changes observed by the European Remote-sensing Satellite (ERS) (1992-2002) and <span class="hlt">Ice</span>, Cloud and land Elevation Satellite (ICESat) (2003-07) indicates that the strongly increased <span class="hlt">mass</span> loss at lower elevations (<2000 m) of the <span class="hlt">ice</span> sheet, as observed during 2003-07, appears to induce interior <span class="hlt">ice</span> thinning at higher elevations. In this paper, we perform a perturbation experiment with a three-dimensional anisotropic <span class="hlt">ice</span>-flow model (AIF model) to investigate this upstream propagation. Observed thinning rates in the regions below 2000m elevation are used as perturbation inputs. The model runs with perturbation for 10 years show that the extensive <span class="hlt">mass</span> loss at the <span class="hlt">ice</span>-sheet margins does in fact cause interior thinning on short timescales (i.e. decadal). The modeled pattern of thinning over the <span class="hlt">ice</span> sheet agrees with the observations, which implies that the strong <span class="hlt">mass</span> loss since the early 2000s at low elevations has had a dynamic impact on the entire <span class="hlt">ice</span> sheet. The modeling results also suggest that even if the large <span class="hlt">mass</span> loss at the margins stopped, the interior <span class="hlt">ice</span> sheet would continue thinning for 300 years and would take thousands of years for full dynamic recovery.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013ACPD...13.4331J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013ACPD...13.4331J"><span>On the relationship between Arctic <span class="hlt">ice</span> clouds and polluted air <span class="hlt">masses</span> over the north slope of Alaska in April 2008</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jouan, C.; Pelon, J.; Girard, E.; Ancellet, G.; Blanchet, J. P.; Delanoë, J.</p> <p>2013-02-01</p> <p>Recently, two Types of <span class="hlt">Ice</span> Clouds (TICs) properties have been characterized using ISDAC airborne measurements (Alaska, April 2008). TIC-2B were characterized by fewer (<10 L-1) and larger (>110 μm) <span class="hlt">ice</span> crystals, a larger <span class="hlt">ice</span> supersaturation (>15%) and a fewer <span class="hlt">ice</span> nuclei (IN) concentration (<2 order of magnitude) when compared to TIC-1/2A. It has been hypothesized that emissions of SO2 may reduce the <span class="hlt">ice</span> nucleating properties of IN through acidification, resulting to a smaller concentration of larger <span class="hlt">ice</span> crystals and leading to precipitation (e.g. cloud regime TIC-2B) because of the reduced competition for the same available moisture. Here, the origin of air <span class="hlt">masses</span> forming the ISDAC TIC-1/2A (1 April 2008) and TIC-2B (15 April 2008) is investigated using trajectory tools and satellite data. Results show that the synoptic conditions favor air <span class="hlt">masses</span> transport from the three potentials SO2 emission areas to Alaska: eastern China and Siberia where anthropogenic and biomass burning emission respectively are produced and the volcanic region from the Kamchatka/Aleutians. Weather conditions allow the accumulation of pollutants from eastern China/Siberia over Alaska, most probably with the contribution of acid volcanic aerosol during the TIC-2B period. OMI observations reveal that SO2 concentrations in air <span class="hlt">masses</span> forming the TIC-2B were larger than in air <span class="hlt">masses</span> forming the TIC-1/2A. Airborne measurements show high acidity near the TIC-2B flight where humidity was low. These results strongly support the hypothesis that acidic coating on IN are at the origin of the formation of TIC-2B.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.C44A..02B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.C44A..02B"><span>connecting the dots between Greenland <span class="hlt">ice</span> sheet surface melting and <span class="hlt">ice</span> flow dynamics (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Box, J. E.; Colgan, W. T.; Fettweis, X.; Phillips, T. P.; Stober, M.</p> <p>2013-12-01</p> <p>This presentation is of a 'unified theory' in glaciology that first identifies surface albedo as a key factor explaining total <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balance and then surveys a mechanistic self-reinforcing interaction between melt water and <span class="hlt">ice</span> flow dynamics. The theory is applied in a near-real time total Greenland <span class="hlt">mass</span> balance retrieval based on surface albedo, a powerful integrator of the competing effects of accumulation and ablation. New snowfall reduces sunlight absorption and increases meltwater retention. Melting amplifies absorbed sunlight through thermal metamorphism and bare <span class="hlt">ice</span> expansion in space and time. By ';following the melt'; we reveal mechanisms linking existing science into a unified theory. Increasing meltwater softens the <span class="hlt">ice</span> sheet in three ways: 1.) sensible heating given the water temperature exceeds that of the <span class="hlt">ice</span> sheet interior; 2.) Some infiltrating water refreezes, transferring latent heat to the <span class="hlt">ice</span>; 3.) Friction from water turbulence heats the <span class="hlt">ice</span>. It has been shown that for a point on the <span class="hlt">ice</span> sheet, basal lubrication increases <span class="hlt">ice</span> flow speed to a time when an efficient sub-glacial drainage network develops that reduces this effect. Yet, with an increasing melt duration the point where the <span class="hlt">ice</span> sheet glides on a wet bed increases inland to a larger area. This effect draws down the <span class="hlt">ice</span> surface elevation, contributing to the ';elevation feedback'. In a perpetual warming scenario, the elevation feedback ultimately leads to <span class="hlt">ice</span> sheet loss reversible only through much slower <span class="hlt">ice</span> sheet growth in an <span class="hlt">ice</span> age environment. As the inland <span class="hlt">ice</span> sheet accelerates, the horizontal extension pulls cracks and crevasses open, trapping more sunlight, amplifying the effect of melt accelerated <span class="hlt">ice</span>. As the bare <span class="hlt">ice</span> area increases, the direct sun-exposed crevassed and infiltration area increases further allowing the <span class="hlt">ice</span> warming process to occur more broadly. Considering hydrofracture [a.k.a. hydrofracking]; surface meltwater fills cracks, attacking the <span class="hlt">ice</span> integrity</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C53C0799H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C53C0799H"><span>Validation of Modelled <span class="hlt">Ice</span> Dynamics of the Greenland <span class="hlt">Ice</span> Sheet using Historical Forcing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hoffman, M. J.; Price, S. F.; Howat, I. M.; Bonin, J. A.; Chambers, D. P.; Tezaur, I.; Kennedy, J. H.; Lenaerts, J.; Lipscomb, W. H.; Neumann, T.; Nowicki, S.; Perego, M.; Saba, J. L.; Salinger, A.; Guerber, J. R.</p> <p>2015-12-01</p> <p>Although <span class="hlt">ice</span> sheet models are used for sea level rise projections, the degree to which these models have been validated by observations is fairly limited, due in part to the limited duration of the satellite observation era and the long adjustment time scales of <span class="hlt">ice</span> sheets. Here we describe a validation framework for the Greenland <span class="hlt">Ice</span> Sheet applied to the Community <span class="hlt">Ice</span> Sheet Model by forcing the model annually with flux anomalies at the major outlet glaciers (Enderlin et al., 2014, observed from Landsat/ASTER/Operation <span class="hlt">Ice</span>Bridge) and surface <span class="hlt">mass</span> balance (van Angelen et al., 2013, calculated from RACMO2) for the period 1991-2012. The <span class="hlt">ice</span> sheet model output is compared to <span class="hlt">ice</span> surface elevation observations from ICESat and <span class="hlt">ice</span> sheet <span class="hlt">mass</span> change observations from GRACE. Early results show promise for assessing the performance of different model configurations. Additionally, we explore the effect of <span class="hlt">ice</span> sheet model resolution on validation skill.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..4411463S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..4411463S"><span>Algae Drive Enhanced Darkening of Bare <span class="hlt">Ice</span> on the Greenland <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stibal, Marek; Box, Jason E.; Cameron, Karen A.; Langen, Peter L.; Yallop, Marian L.; Mottram, Ruth H.; Khan, Alia L.; Molotch, Noah P.; Chrismas, Nathan A. M.; Calı Quaglia, Filippo; Remias, Daniel; Smeets, C. J. P. Paul; van den Broeke, Michiel R.; Ryan, Jonathan C.; Hubbard, Alun; Tranter, Martyn; van As, Dirk; Ahlstrøm, Andreas P.</p> <p>2017-11-01</p> <p>Surface ablation of the Greenland <span class="hlt">ice</span> sheet is amplified by surface darkening caused by light-absorbing impurities such as mineral dust, black carbon, and pigmented microbial cells. We present the first quantitative assessment of the microbial contribution to the <span class="hlt">ice</span> sheet surface darkening, based on field measurements of surface reflectance and concentrations of light-absorbing impurities, including pigmented algae, during the 2014 melt season in the southwestern part of the <span class="hlt">ice</span> sheet. The impact of algae on bare <span class="hlt">ice</span> darkening in the study area was greater than that of nonalgal impurities and yielded a net albedo reduction of 0.038 ± 0.0035 for each algal population doubling. We argue that algal growth is a crucial control of bare <span class="hlt">ice</span> darkening, and incorporating the algal darkening effect will improve <span class="hlt">mass</span> balance and sea level projections of the Greenland <span class="hlt">ice</span> sheet and <span class="hlt">ice</span> <span class="hlt">masses</span> elsewhere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.7879K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.7879K"><span>Tropospheric characteristics over sea <span class="hlt">ice</span> during N-<span class="hlt">ICE</span>2015</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kayser, Markus; Maturilli, Marion; Graham, Robert; Hudson, Stephen; Cohen, Lana; Rinke, Annette; Kim, Joo-Hong; Park, Sang-Jong; Moon, Woosok; Granskog, Mats</p> <p>2017-04-01</p> <p>Over recent years, the Arctic Ocean region has shifted towards a younger and thinner sea-<span class="hlt">ice</span> regime. The Norwegian young sea <span class="hlt">ICE</span> (N-<span class="hlt">ICE</span>2015) expedition was designed to investigate the atmosphere-snow-<span class="hlt">ice</span>-ocean interactions in this new <span class="hlt">ice</span> regime north of Svalbard. Here we analyze upper-air measurements made by radiosondes launched twice daily together with surface meteorology observations during N-<span class="hlt">ICE</span>2015 from January to June 2015. We study the multiple cyclonic events observed during N-<span class="hlt">ICE</span>2015 with respect to changes in the vertical thermodynamic structure, sudden increases in moisture <span class="hlt">content</span> and temperature, temperature inversions and boundary layer dynamics. The influence of synoptic cyclones is strongest under polar night conditions, when radiative cooling is most effective and the moisture <span class="hlt">content</span> is low. We find that transitions between the radiatively clear and opaque state are the largest drivers of changes to temperature inversion and stability characteristics in the boundary layer during winter. In spring radiative fluxes warm the surface leading to lifted temperature inversions and a statically unstable boundary layer. The unique N-<span class="hlt">ICE</span>2015 dataset is used for case studies investigating changes in the vertical structure of the atmosphere under varying synoptic conditions. The goal is to deepen our understanding of synoptic interactions within the Arctic climate system, to improve model performance, as well as to identify gaps in instrumentation, which precludes further investigations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1917148O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1917148O"><span>Water <span class="hlt">ice</span> cloud property retrievals at Mars with OMEGA:Spatial distribution and column <span class="hlt">mass</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Olsen, Kevin S.; Madeleine, Jean-Baptiste; Szantai, Andre; Audouard, Joachim; Geminale, Anna; Altieri, Francesca; Bellucci, Giancarlo; Montabone, Luca; Wolff, Michael J.; Forget, Francois</p> <p>2017-04-01</p> <p>Spectral images of Mars recorded by OMEGA (Observatoire pour la Minéralogie, l'Eau, les Glaces et l'Activité) on Mars Express can be used to deduce the mean effective radius (r_eff) and optical depth (τ_i) of water <span class="hlt">ice</span> particles in clouds. Using new data sets for a priori surface temperature, vertical profiles of atmospheric temperature, dust opacity, and multi-spectral surface albedo, we have analyzed over 40 OMEGA image cubes over the Tharsis, Arabia, and Syrtis Major quadrangles, and mapped the spatial distribution of r_eff, τ_i, and water <span class="hlt">ice</span> column <span class="hlt">mass</span>. We also explored the parameter space of r_eff and τ_i, which are inversely proportional, and the <span class="hlt">ice</span> cloud index (ICI), which is the ratio of the reflectance at 3.4 and 3.52 μm, and indicates the thickness of water <span class="hlt">ice</span> clouds. We found that the ICI, trivial to calculate for OMEGA image cubes, can be a proxy for column <span class="hlt">mass</span>, which is very expensive to compute, requiring accurate retrievals of surface albedo, r_eff, and τ_i. Observing the spatial distribution, we find that within each cloud system, r_eff varies about a mean of 2.1 μm, that τi is closely related to r_eff, and that the values allowed for τ_i, given r_eff, are related to the ICI. We also observe areas where our retrieval detects very thin clouds made of very large particles (mean of 12.5 μm), which are still under investigation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016TCry...10.2361N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016TCry...10.2361N"><span>A daily, 1 km resolution data set of downscaled Greenland <span class="hlt">ice</span> sheet surface <span class="hlt">mass</span> balance (1958-2015)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Noël, Brice; van de Berg, Willem Jan; Machguth, Horst; Lhermitte, Stef; Howat, Ian; Fettweis, Xavier; van den Broeke, Michiel R.</p> <p>2016-10-01</p> <p>This study presents a data set of daily, 1 km resolution Greenland <span class="hlt">ice</span> sheet (GrIS) surface <span class="hlt">mass</span> balance (SMB) covering the period 1958-2015. Applying corrections for elevation, bare <span class="hlt">ice</span> albedo and accumulation bias, the high-resolution product is statistically downscaled from the native daily output of the polar regional climate model RACMO2.3 at 11 km. The data set includes all individual SMB components projected to a down-sampled version of the Greenland <span class="hlt">Ice</span> Mapping Project (GIMP) digital elevation model and <span class="hlt">ice</span> mask. The 1 km mask better resolves narrow ablation zones, valley glaciers, fjords and disconnected <span class="hlt">ice</span> caps. Relative to the 11 km product, the more detailed representation of isolated glaciated areas leads to increased precipitation over the southeastern GrIS. In addition, the downscaled product shows a significant increase in runoff owing to better resolved low-lying marginal glaciated regions. The combined corrections for elevation and bare <span class="hlt">ice</span> albedo markedly improve model agreement with a newly compiled data set of ablation measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160000453','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160000453"><span>Incorporation of New Convective <span class="hlt">Ice</span> Microphysics into the NASA GISS GCM and Impacts on Cloud <span class="hlt">Ice</span> Water Path (IWP) Simulation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Elsaesser, Greg; Del Genio, Anthony</p> <p>2015-01-01</p> <p>The CMIP5 configurations of the GISS Model-E2 GCM simulated a mid- and high latitude <span class="hlt">ice</span> IWP that decreased by 50 relative to that simulated for CMIP3 (Jiang et al. 2012; JGR). Tropical IWP increased by 15 in CMIP5. While the tropical IWP was still within the published upper-bounds of IWP uncertainty derived using NASA A-Train satellite observations, it was found that the upper troposphere (200 mb) <span class="hlt">ice</span> water <span class="hlt">content</span> (IWC) exceeded the published upper-bound by a factor of 2. This was largely driven by IWC in deep-convecting regions of the tropics.Recent advances in the model-E2 convective parameterization have been found to have a substantial impact on tropical IWC. These advances include the development of both a cold pool parameterization (Del Genio et al. 2015) and new convective <span class="hlt">ice</span> parameterization. In this presentation, we focus on the new parameterization of convective cloud <span class="hlt">ice</span> that was developed using data from the NASA TC4 Mission. <span class="hlt">Ice</span> particle terminal velocity formulations now include information from a number of NASA field campaigns. The new parameterization predicts both an <span class="hlt">ice</span> water <span class="hlt">mass</span> weighted-average particle diameter and a particle cross sectional area weighted-average size diameter as a function of temperature and <span class="hlt">ice</span> water <span class="hlt">content</span>. By assuming a gamma-distribution functional form for the particle size distribution, these two diameter estimates are all that are needed to explicitly predict the distribution of <span class="hlt">ice</span> particles as a function of particle diameter.GCM simulations with the improved convective parameterization yield a 50 decrease in upper tropospheric IWC, bringing the tropical and global mean IWP climatologies into even closer agreement with the A-Train satellite observation best estimates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.A33P..05E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.A33P..05E"><span>Incorporation of New Convective <span class="hlt">Ice</span> Microphysics into the NASA GISS GCM and Impacts on Cloud <span class="hlt">Ice</span> Water Path (IWP) Simulation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Elsaesser, G.; Del Genio, A. D.</p> <p>2015-12-01</p> <p>The CMIP5 configurations of the GISS Model-E2 GCM simulated a mid- and high-latitude <span class="hlt">ice</span> IWP that decreased by ~50% relative to that simulated for CMIP3 (Jiang et al. 2012; JGR). Tropical IWP increased by ~15% in CMIP5. While the tropical IWP was still within the published upper-bounds of IWP uncertainty derived using NASA A-Train satellite observations, it was found that the upper troposphere (~200 mb) <span class="hlt">ice</span> water <span class="hlt">content</span> (IWC) exceeded the published upper-bound by a factor of ~2. This was largely driven by IWC in deep-convecting regions of the tropics. Recent advances in the model-E2 convective parameterization have been found to have a substantial impact on tropical IWC. These advances include the development of both a cold pool parameterization (Del Genio et al. 2015) and new convective <span class="hlt">ice</span> parameterization. In this presentation, we focus on the new parameterization of convective cloud <span class="hlt">ice</span> that was developed using data from the NASA TC4 Mission. <span class="hlt">Ice</span> particle terminal velocity formulations now include information from a number of NASA field campaigns. The new parameterization predicts both an <span class="hlt">ice</span> water <span class="hlt">mass</span> weighted-average particle diameter and a particle cross sectional area weighted-average size diameter as a function of temperature and <span class="hlt">ice</span> water <span class="hlt">content</span>. By assuming a gamma-distribution functional form for the particle size distribution, these two diameter estimates are all that are needed to explicitly predict the distribution of <span class="hlt">ice</span> particles as a function of particle diameter. GCM simulations with the improved convective parameterization yield a ~50% decrease in upper tropospheric IWC, bringing the tropical and global mean IWP climatologies into even closer agreement with the A-Train satellite observation best estimates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.C41C0419C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.C41C0419C"><span>High permafrost <span class="hlt">ice</span> <span class="hlt">contents</span> in Holocene slope deposits as observed from shallow geophysics and a coring program in Pangnirtung, Nunavut, Canada</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carbonneau, A.; Allard, M.; L'Hérault, E.; LeBlanc, A.</p> <p>2011-12-01</p> <p>A study of permafrost conditions was undertaken in the Hamlet of Pangnirtung, Nunavut, by the Geological Survey of Canada (GSC) and Université Laval's Centre d'études nordiques (CEN) to support decision makers in their community planning work. The methods used for this project were based on geophysical and geomorphological approaches, including permafrost cores drilled in surficial deposits and ground penetrating radar surveys using a GPR Pulse EKKO 100 extending to the complete community area and to its projected expansion sector. Laboratory analysis allowed a detailed characterization of permafrost in terms of water <span class="hlt">contents</span>, salinity and grain size. Cryostratigraphic analysis was done via CT-Scan imagery of frozen cores using medical imaging softwares such as Osiris. This non destructive method allows a 3D imaging of the entire core in order to locate the amount of the excess <span class="hlt">ice</span>, determine the volumetric <span class="hlt">ice</span> <span class="hlt">content</span> and also interpret the <span class="hlt">ice</span>-formation processes that took place during freezing of the permafrost. Our new map of the permafrost conditions in Pangnirtung illustrates that the dominant mapping unit consist of <span class="hlt">ice</span>-rich colluvial deposits. Aggradationnal <span class="hlt">ice</span> formed syngenitically with slope sedimentation. Buried soils were found imbedded in this colluvial layer and demonstrates that colluviation associated with overland-flow during snowmelt occurred almost continuously since 7080 cal. BP. In the eastern sector of town, the 1 to 4 meters thick colluviums cover till and a network of <span class="hlt">ice</span> wedges that were revealed as spaced hyperbolic reflectors on GPR profiles. The colluviums also cover <span class="hlt">ice</span>-rich marine silt and bedrock in the western sector of the hamlet; marine shells found in a permafrost core yielded a radiocarbon date of 9553 cal. BP which provides a revised age for the local deglaciation and also a revised marine submergence limit. Among the applied methods, shallow drilling in coarse grained permafrost, core recovery and CT-Scan allowed the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5489271','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5489271"><span>Decreasing cloud cover drives the recent <span class="hlt">mass</span> loss on the Greenland <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Hofer, Stefan; Tedstone, Andrew J.; Fettweis, Xavier; Bamber, Jonathan L.</p> <p>2017-01-01</p> <p>The Greenland <span class="hlt">Ice</span> Sheet (GrIS) has been losing <span class="hlt">mass</span> at an accelerating rate since the mid-1990s. This has been due to both increased <span class="hlt">ice</span> discharge into the ocean and melting at the surface, with the latter being the dominant contribution. This change in state has been attributed to rising temperatures and a decrease in surface albedo. We show, using satellite data and climate model output, that the abrupt reduction in surface <span class="hlt">mass</span> balance since about 1995 can be attributed largely to a coincident trend of decreasing summer cloud cover enhancing the melt-albedo feedback. Satellite observations show that, from 1995 to 2009, summer cloud cover decreased by 0.9 ± 0.3% per year. Model output indicates that the GrIS summer melt increases by 27 ± 13 gigatons (Gt) per percent reduction in summer cloud cover, principally because of the impact of increased shortwave radiation over the low albedo ablation zone. The observed reduction in cloud cover is strongly correlated with a state shift in the North Atlantic Oscillation promoting anticyclonic conditions in summer and suggests that the enhanced surface <span class="hlt">mass</span> loss from the GrIS is driven by synoptic-scale changes in Arctic-wide atmospheric circulation. PMID:28782014</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_11 --> <div id="page_12" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="221"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28782014','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28782014"><span>Decreasing cloud cover drives the recent <span class="hlt">mass</span> loss on the Greenland <span class="hlt">Ice</span> Sheet.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hofer, Stefan; Tedstone, Andrew J; Fettweis, Xavier; Bamber, Jonathan L</p> <p>2017-06-01</p> <p>The Greenland <span class="hlt">Ice</span> Sheet (GrIS) has been losing <span class="hlt">mass</span> at an accelerating rate since the mid-1990s. This has been due to both increased <span class="hlt">ice</span> discharge into the ocean and melting at the surface, with the latter being the dominant contribution. This change in state has been attributed to rising temperatures and a decrease in surface albedo. We show, using satellite data and climate model output, that the abrupt reduction in surface <span class="hlt">mass</span> balance since about 1995 can be attributed largely to a coincident trend of decreasing summer cloud cover enhancing the melt-albedo feedback. Satellite observations show that, from 1995 to 2009, summer cloud cover decreased by 0.9 ± 0.3% per year. Model output indicates that the GrIS summer melt increases by 27 ± 13 gigatons (Gt) per percent reduction in summer cloud cover, principally because of the impact of increased shortwave radiation over the low albedo ablation zone. The observed reduction in cloud cover is strongly correlated with a state shift in the North Atlantic Oscillation promoting anticyclonic conditions in summer and suggests that the enhanced surface <span class="hlt">mass</span> loss from the GrIS is driven by synoptic-scale changes in Arctic-wide atmospheric circulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040062258&hterms=major+depression&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dmajor%2Bdepression','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040062258&hterms=major+depression&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dmajor%2Bdepression"><span>Northern and Southern Permafrost Regions on Mars with High <span class="hlt">Content</span> of Water <span class="hlt">Ice</span>: Similarities and Differences</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mitrofanov, I. G.; Litvak, M. L.; Kozyrev, A. S.; Sanin, A. B.; Tretyakov, V. I.; Kuzmin, R. O.; Boynton, W. V.; Hamara, D. K.; Shinohara, C.; Saunders, R. S.</p> <p>2004-01-01</p> <p>The measurements by neutron detectors on Odyssey have revealed two large poleward regions with large depression of flux of epithermal and high energy neutrons. The flux of neutrons from Mars is known to be produced by the bombardment of the surface layer by galactic cosmic rays. The leakage flux of epithermal and fast neutrons has regional variation by a factor of 10 over the surface of Mars. These variations are mainly produced by variations of hydrogen <span class="hlt">content</span> in the shallow subsurface. On Mars hydrogen is associated with water. Therefore, the Northern and Southern depressions of neutron emission could be identified as permafrost regions with very high <span class="hlt">content</span> of water <span class="hlt">ice</span>. These regions are much larger than the residual polar caps, and could contain the major fraction of subsurface water <span class="hlt">ice</span>. Here we present the results of HEND neutron data deconvolution for these regions and describe the similarities and differences between them.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A13E2121S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A13E2121S"><span>Impacts of a Stochastic <span class="hlt">Ice</span> <span class="hlt">Mass</span>-Size Relationship on Squall Line Ensemble Simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stanford, M.; Varble, A.; Morrison, H.; Grabowski, W.; McFarquhar, G. M.; Wu, W.</p> <p>2017-12-01</p> <p>Cloud and precipitation structure, evolution, and cloud radiative forcing of simulated mesoscale convective systems (MCSs) are significantly impacted by <span class="hlt">ice</span> microphysics parameterizations. Most microphysics schemes assume power law relationships with constant parameters for <span class="hlt">ice</span> particle <span class="hlt">mass</span>, area, and terminal fallspeed relationships as a function of size, despite observations showing that these relationships vary in both time and space. To account for such natural variability, a stochastic representation of <span class="hlt">ice</span> microphysical parameters was developed using the Predicted Particle Properties (P3) microphysics scheme in the Weather Research and Forecasting model, guided by in situ aircraft measurements from a number of field campaigns. Here, the stochastic framework is applied to the "a" and "b" parameters of the unrimed <span class="hlt">ice</span> <span class="hlt">mass</span>-size (m-D) relationship (m=aDb) with co-varying "a" and "b" values constrained by observational distributions tested over a range of spatiotemporal autocorrelation scales. Diagnostically altering a-b pairs in three-dimensional (3D) simulations of the 20 May 2011 Midlatitude Continental Convective Clouds Experiment (MC3E) squall line suggests that these parameters impact many important characteristics of the simulated squall line, including reflectivity structure (particularly in the anvil region), surface rain rates, surface and top of atmosphere radiative fluxes, buoyancy and latent cooling distributions, and system propagation speed. The stochastic a-b P3 scheme is tested using two frameworks: (1) a large ensemble of two-dimensional idealized squall line simulations and (2) a smaller ensemble of 3D simulations of the 20 May 2011 squall line, for which simulations are evaluated using observed radar reflectivity and radial velocity at multiple wavelengths, surface meteorology, and surface and satellite measured longwave and shortwave radiative fluxes. Ensemble spreads are characterized and compared against initial condition ensemble spreads</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017TCry...11.1501B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017TCry...11.1501B"><span>Winter <span class="hlt">mass</span> balance of Drangajökull <span class="hlt">ice</span> cap (NW Iceland) derived from satellite sub-meter stereo images</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Belart, Joaquín M. C.; Berthier, Etienne; Magnússon, Eyjólfur; Anderson, Leif S.; Pálsson, Finnur; Thorsteinsson, Thorsteinn; Howat, Ian M.; Aðalgeirsdóttir, Guðfinna; Jóhannesson, Tómas; Jarosch, Alexander H.</p> <p>2017-06-01</p> <p>Sub-meter resolution, stereoscopic satellite images allow for the generation of accurate and high-resolution digital elevation models (DEMs) over glaciers and <span class="hlt">ice</span> caps. Here, repeated stereo images of Drangajökull <span class="hlt">ice</span> cap (NW Iceland) from Pléiades and WorldView2 (WV2) are combined with in situ estimates of snow density and densification of firn and fresh snow to provide the first estimates of the glacier-wide geodetic winter <span class="hlt">mass</span> balance obtained from satellite imagery. Statistics in snow- and <span class="hlt">ice</span>-free areas reveal similar vertical relative accuracy (< 0.5 m) with and without ground control points (GCPs), demonstrating the capability for measuring seasonal snow accumulation. The calculated winter (14 October 2014 to 22 May 2015) <span class="hlt">mass</span> balance of Drangajökull was 3.33 ± 0.23 m w.e. (meter water equivalent), with ∼ 60 % of the accumulation occurring by February, which is in good agreement with nearby ground observations. On average, the repeated DEMs yield 22 % less elevation change than the length of eight winter snow cores due to (1) the time difference between in situ and satellite observations, (2) firn densification and (3) elevation changes due to <span class="hlt">ice</span> dynamics. The contributions of these three factors were of similar magnitude. This study demonstrates that seasonal geodetic <span class="hlt">mass</span> balance can, in many areas, be estimated from sub-meter resolution satellite stereo images.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017TCry...11.2655S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017TCry...11.2655S"><span>GPS-derived estimates of surface <span class="hlt">mass</span> balance and ocean-induced basal melt for Pine Island Glacier <span class="hlt">ice</span> shelf, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shean, David E.; Christianson, Knut; Larson, Kristine M.; Ligtenberg, Stefan R. M.; Joughin, Ian R.; Smith, Ben E.; Stevens, C. Max; Bushuk, Mitchell; Holland, David M.</p> <p>2017-11-01</p> <p>In the last 2 decades, Pine Island Glacier (PIG) experienced marked speedup, thinning, and grounding-line retreat, likely due to marine <span class="hlt">ice</span>-sheet instability and <span class="hlt">ice</span>-shelf basal melt. To better understand these processes, we combined 2008-2010 and 2012-2014 GPS records with dynamic firn model output to constrain local surface and basal <span class="hlt">mass</span> balance for PIG. We used GPS interferometric reflectometry to precisely measure absolute surface elevation (zsurf) and Lagrangian surface elevation change (Dzsurf/ Dt). Observed surface elevation relative to a firn layer tracer for the initial surface (zsurf - zsurf0') is consistent with model estimates of surface <span class="hlt">mass</span> balance (SMB, primarily snow accumulation). A relatively abrupt ˜ 0.2-0.3 m surface elevation decrease, likely due to surface melt and increased compaction rates, is observed during a period of warm atmospheric temperatures from December 2012 to January 2013. Observed Dzsurf/ Dt trends (-1 to -4 m yr-1) for the PIG shelf sites are all highly linear. Corresponding basal melt rate estimates range from ˜ 10 to 40 m yr-1, in good agreement with those derived from <span class="hlt">ice</span>-bottom acoustic ranging, phase-sensitive <span class="hlt">ice</span>-penetrating radar, and high-resolution stereo digital elevation model (DEM) records. The GPS and DEM records document higher melt rates within and near features associated with longitudinal extension (i.e., transverse surface depressions, rifts). Basal melt rates for the 2012-2014 period show limited temporal variability despite large changes in ocean temperature recorded by moorings in Pine Island Bay. Our results demonstrate the value of long-term GPS records for <span class="hlt">ice</span>-shelf <span class="hlt">mass</span> balance studies, with implications for the sensitivity of <span class="hlt">ice</span>-ocean interaction at PIG.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.A11J0138N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A11J0138N"><span>Observed Aerosol Influence on <span class="hlt">Ice</span> Water <span class="hlt">Content</span> of Arctic Mixed-Phase Clouds</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Norgren, M.; de Boer, G.; Shupe, M.</p> <p>2016-12-01</p> <p>The response of <span class="hlt">ice</span> water <span class="hlt">content</span> (IWC) in Arctic mixed-phase stratocumulus to atmospheric aerosols is observed. IWC retrievals from ground based radars operated by the Atmospheric Radiation Measurement (ARM) program in Barrow, Alaska are used to construct composite profiles of cloud IWC from a 9-year radar record starting in January of 2000. The IWC profiles for high (polluted) and low (clean) aerosol loadings are compared. Generally, we find that clean clouds exhibit statistically significant higher levels of IWC than do polluted clouds by a factor of 2-4 at cloud base. For springtime clouds, with a maximum relative humidity with respect to <span class="hlt">ice</span> (RHI) above 110% in the cloud layer, the IWC at cloud base was a factor of 3.25 times higher in clean clouds than it was in polluted clouds. We infer that the aerosol loading of the cloud environment alters the liquid drop size distribution within the cloud, with larger drops being more frequent in clean clouds. Larger cloud drops promote riming within the cloud layer, which is one explanation for the higher IWC levels in clean clouds. The drop size distribution may also be a significant control of <span class="hlt">ice</span> nucleation events within mixed-phase clouds. Whether the high IWC levels in clean clouds are due to increased riming or nucleation events is unclear at this time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29104900','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29104900"><span>A simulation of <span class="hlt">ice</span> cloud particle size, humidity, and temperature measurements from the TWICE CubeSat.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jiang, Jonathan H; Yue, Qing; Su, Hui; Reising, Steven C; Kangaslahti, Pekka P; Deal, William R; Schlecht, Erich T; Wu, Longtao; Evans, K Franklin</p> <p>2017-08-01</p> <p>This paper describes a forward radiative transfer model and retrieval system (FMRS) for the Tropospheric Water and cloud <span class="hlt">ICE</span> (TWICE) CubeSat instrument. We use the FMRS to simulate radiances for the TWICE's 14 millimeter- and submillimeter-wavelength channels for a tropical atmospheric state produced by a Weather Research and Forecasting model simulation. We also perform simultaneous retrievals of cloud <span class="hlt">ice</span> particle size, <span class="hlt">ice</span> water <span class="hlt">content</span> (IWC), water vapor <span class="hlt">content</span> (H 2 O), and temperature from the simulated TWICE radiances using the FMRS. We show that the TWICE instrument is capable of retrieving <span class="hlt">ice</span> particle size in the range of ~50-1000 μm in <span class="hlt">mass</span> mean effective diameter with approximately 50% uncertainty. The uncertainties of other retrievals from TWICE are about 1 K for temperature, 50% for IWC, and 20% for H 2 O.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5656330','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5656330"><span>A simulation of <span class="hlt">ice</span> cloud particle size, humidity, and temperature measurements from the TWICE CubeSat</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Yue, Qing; Su, Hui; Reising, Steven C.; Kangaslahti, Pekka P.; Deal, William R.; Schlecht, Erich T.; Wu, Longtao; Evans, K. Franklin</p> <p>2017-01-01</p> <p>Abstract This paper describes a forward radiative transfer model and retrieval system (FMRS) for the Tropospheric Water and cloud <span class="hlt">ICE</span> (TWICE) CubeSat instrument. We use the FMRS to simulate radiances for the TWICE's 14 millimeter‐ and submillimeter‐wavelength channels for a tropical atmospheric state produced by a Weather Research and Forecasting model simulation. We also perform simultaneous retrievals of cloud <span class="hlt">ice</span> particle size, <span class="hlt">ice</span> water <span class="hlt">content</span> (IWC), water vapor <span class="hlt">content</span> (H2O), and temperature from the simulated TWICE radiances using the FMRS. We show that the TWICE instrument is capable of retrieving <span class="hlt">ice</span> particle size in the range of ~50–1000 μm in <span class="hlt">mass</span> mean effective diameter with approximately 50% uncertainty. The uncertainties of other retrievals from TWICE are about 1 K for temperature, 50% for IWC, and 20% for H2O. PMID:29104900</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A31D2210B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A31D2210B"><span>Information <span class="hlt">content</span> of thermal infrared a microwave bands for simultaneous retrieval of cirrus <span class="hlt">ice</span> water path and particle effective diameter</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bell, A.; Tang, G.; Yang, P.; Wu, D.</p> <p>2017-12-01</p> <p>Due to their high spatial and temporal coverage, cirrus clouds have a profound role in regulating the Earth's energy budget. Variability of their radiative, geometric, and microphysical properties can pose significant uncertainties in global climate model simulations if not adequately constrained. Thus, the development of retrieval methodologies able to accurately retrieve <span class="hlt">ice</span> cloud properties and present associated uncertainties is essential. The effectiveness of cirrus cloud retrievals relies on accurate a priori understanding of <span class="hlt">ice</span> radiative properties, as well as the current state of the atmosphere. Current studies have implemented information <span class="hlt">content</span> theory analyses prior to retrievals to quantify the amount of information that should be expected on parameters to be retrieved, as well as the relative contribution of information provided by certain measurement channels. Through this analysis, retrieval algorithms can be designed in a way to maximize the information in measurements, and therefore ensure enough information is present to retrieve <span class="hlt">ice</span> cloud properties. In this study, we present such an information <span class="hlt">content</span> analysis to quantify the amount of information to be expected in retrievals of cirrus <span class="hlt">ice</span> water path and particle effective diameter using sub-millimeter and thermal infrared radiometry. Preliminary results show these bands to be sensitive to changes in <span class="hlt">ice</span> water path and effective diameter, and thus lend confidence their ability to simultaneously retrieve these parameters. Further quantification of sensitivity and the information provided from these bands can then be used to design and optimal retrieval scheme. While this information <span class="hlt">content</span> analysis is employed on a theoretical retrieval combining simulated radiance measurements, the methodology could in general be applicable to any instrument or retrieval approach.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C54A..05H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C54A..05H"><span>Snow, Firn and <span class="hlt">Ice</span> Heterogeneity within Larsen C <span class="hlt">Ice</span> Shelf Revealed by Borehole Optical-televiewing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hubbard, B. P.; Ashmore, D.; Luckman, A. J.; Kulessa, B.; Bevan, S. L.; Booth, A.; Kuipers Munneke, P.; O'Leary, M.; Sevestre, H.</p> <p>2016-12-01</p> <p>The north-western sector of Larsen C <span class="hlt">Ice</span> Shelf (LCIS), Antarctica, hosts intermittent surface ponds resulting from intense melting, largely driven by warm föhn winds. The fate of such surface melt water is largely controlled by the shelf's firn structure, which also dictates shelf density (widely used to reconstruct <span class="hlt">ice</span> shelf thickness from altimetric data) and preconditioning to hydrofracture. Here, we report a suite of five 90 m long optical-televiewer (OPTV) borehole logs from the northern and central regions of LCIS recorded in spring 2014 and 2015. For each OPTV log we reconstruct vertical variations in material density via an empirical OPTV log-<span class="hlt">ice</span> core calibration, and apply a thresholding technique to estimate refrozen <span class="hlt">ice</span> <span class="hlt">content</span> within the firn column. These data are combined to define five material facies present within this sector of LCIS. The firn/<span class="hlt">ice</span> column is anomalously dense at all five sites, having an overall mean depth-averaged density of 873 +/-32 kg m-3. In terms of spatial variability, our findings generally support previous estimates of firn air <span class="hlt">content</span> fields and implied infiltration <span class="hlt">ice</span> <span class="hlt">content</span>. However, they also highlight finer-resolution complexity of <span class="hlt">ice</span> shelf structure. For example, the most dense <span class="hlt">ice</span>, with the lowest equivalent firn air <span class="hlt">content</span>, is not located within the most westerly inlets, where firn-driven melting and ponding are most active, but some tens of km down-flow of these areas. We interpret this effect in terms of the inheritance nearer the grounding line of relatively low-density glacial <span class="hlt">ice</span> (e.g., 52 m thick with a density of 852 +/-21 kg m-3 in northernmost Cabinet Inlet) advected from inland. This inherited <span class="hlt">ice</span> forms one of five facies identified across the study region. These are, extending broadly downwards into the shelf, and with different representation at each site: local accumulation (F1); local accumulation hosting substantial infiltration <span class="hlt">ice</span>, i.e. influenced by intense melt but insufficient to form</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040062239&hterms=major+depression&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dmajor%2Bdepression','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040062239&hterms=major+depression&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dmajor%2Bdepression"><span>Northern and Southern Permafrost Regions on Mars with High <span class="hlt">Content</span> of Water <span class="hlt">Ice</span>: Similarities and Differences</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mitrofanov, I. G.; Litvak, M. L.; Kozyrev, A. S.; Sanin, A. B.; Tretyakov, V. I.; Kuzmin, R. O.; Boynton, W. V.; Hamara, D. K.; Shinohara, C.; Saunders, R. S.</p> <p>2004-01-01</p> <p>The measurements by neutron detectors on Odyssey have revealed two large poleward regions with large depression of flux of epithermal and high energy neutrons [1-3]. The flux of neutrons from Mars is known to be produced by the bombardment of the surface layer by galactic cosmic rays. The leakage flux of epithermal and fast neutrons has regional variation by a factor of 10 over the surface of Mars (e.g. see [3- 5]). These variations are mainly produced by variations of hydrogen <span class="hlt">content</span> in the shallow subsurface. On Mars hydrogen is associated with water. Therefore, the Northern and Southern depressions of neutron emission could be identified as permafrost regions with very high <span class="hlt">content</span> of water <span class="hlt">ice</span> [1-5]. These regions are much larger than the residual polar caps, and could contain the major fraction of subsurface water <span class="hlt">ice</span>. Here we present the results of HEND neutron data deconvolution for these regions and describe the similarities and differences between them.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C41A0693Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C41A0693Z"><span>Time Series of Greenland <span class="hlt">Ice</span>-Sheet Elevations and <span class="hlt">Mass</span> Changes from ICESat 2003-2009</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zwally, H. J.; Li, J.; Medley, B.; Robbins, J. W.; Yi, D.</p> <p>2015-12-01</p> <p>We follow the repeat-track analysis (RTA) of ICESat surface-elevation data by a second stage that adjusts the measured elevations on repeat passes to the reference track taking into account the cross-track slope (αc), in order to construct elevation time series. αc are obtained from RTA simultaneous solutions for αc, dh/dt, and h0. The height measurements on repeat tracks are initially interpolated to uniform along-track reference points (every 172 m) and times (ti) giving the h(xi,ti) used in the RTA solutions. The xi are the cross-track spacings from the reference track and i is the laser campaign index. The adjusted elevation measurements at the along-track reference points are hr(ti) = h(xi,ti) - xi tan(αc) - h0. The hr(ti) time series are averaged over 50 km cells creating H(ti) series and further averaged (weighted by cell area) to H(t) time series over drainage systems (DS), elevation bands, regions, and the entire <span class="hlt">ice</span> sheet. Temperature-driven changes in the rate of firn compaction, CT(t), are calculated for 50 km cells with our firn-compaction model giving I(t) = H(t) - CT(t) - B(t) where B(t) is the vertical motion of the bedrock. During 2003 to 2009, the average dCT(t)/dt in the accumulation zone is -5 cm/yr, which amounts to a -75 km3/yr correction to <span class="hlt">ice</span> volume change estimates. The I(t) are especially useful for studying the seasonal cycle of <span class="hlt">mass</span> gains and losses and interannual variations. The H(t) for the ablation zone are fitted with a multi-variate function with a linear component describing the upward component of <span class="hlt">ice</span> flow plus winter accumulation (fall through spring) and a portion of a sine function describing the superimposed summer melting. During fall to spring the H(t) indicate that the upward motion of the <span class="hlt">ice</span> flow is at a rate of 1 m/yr, giving an annual <span class="hlt">mass</span> gain of 180 Gt/yr in the ablation zone. The summer loss from surface melting in the high-melt summer of 2005 is 350 Gt/yr, giving a net surface loss of 170 Gt/yr from the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRC..123.2422L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123.2422L"><span>Seasonal and Interannual Variations of Sea <span class="hlt">Ice</span> <span class="hlt">Mass</span> Balance From the Central Arctic to the Greenland Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lei, Ruibo; Cheng, Bin; Heil, Petra; Vihma, Timo; Wang, Jia; Ji, Qing; Zhang, Zhanhai</p> <p>2018-04-01</p> <p>The seasonal evolution of sea <span class="hlt">ice</span> <span class="hlt">mass</span> balance between the Central Arctic and Fram Strait, as well as the underlying driving forces, remain largely unknown because of a lack of observations. In this study, two and three buoys were deployed in the Central Arctic during the summers of 2010 and 2012, respectively. It was established that basal <span class="hlt">ice</span> growth commenced between mid-October and early December. Annual basal <span class="hlt">ice</span> growth, ranging from 0.21 to 1.14 m, was determined mainly by initial <span class="hlt">ice</span> thickness, air temperature, and oceanic heat flux during winter. An analytic thermodynamic model indicated that climate warming reduces the winter growth rate of thin <span class="hlt">ice</span> more than for thick <span class="hlt">ice</span> because of the weak thermal inertia of the former. Oceanic heat flux during the freezing season was 2-4 W m-2, which accounted for 18-31% of the basal <span class="hlt">ice</span> energy balance. We identified two mechanisms that modified the oceanic heat flux, i.e., solar energy absorbed by the upper ocean during summer, and interaction with warm waters south of Fram Strait; the latter resulted in basal <span class="hlt">ice</span> melt, even in winter. In summer 2010, <span class="hlt">ice</span> loss in the Central Arctic was considerable, which led to increased oceanic heat flux into winter and delayed <span class="hlt">ice</span> growth. The Transpolar Drift Stream was relatively weak in summer 2013. This reduced sea <span class="hlt">ice</span> advection out of the Arctic Ocean, and it restrained <span class="hlt">ice</span> melt because of the cool atmospheric conditions, weakened albedo feedback, and relatively small oceanic heat flux in the north.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMED34A..05S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMED34A..05S"><span>Incorporating Geodetic Data in Introductory Geoscience Classrooms through UNAVCO's GETSI "<span class="hlt">Ice</span> <span class="hlt">Mass</span> and Sea Level Changes" Module</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stearns, L. A.; Walker, B.; Pratt-Sitaula, B.</p> <p>2015-12-01</p> <p>GETSI (Geodesy Tools for Societal Issues) is an NSF-funded partnership program between UNAVCO, Indiana University, Mt. San Antonio College, and the Science Education Resource Center (SERC). We present results from classroom testing and assessment of the GETSI <span class="hlt">Ice</span> <span class="hlt">Mass</span> and Sea Level Changes module that utilizes geodetic data to teach about <span class="hlt">ice</span> sheet <span class="hlt">mass</span> loss in introductory undergraduate courses. The module explores the interactions between global sea level rise, Greenland <span class="hlt">ice</span> <span class="hlt">mass</span> loss, and the response of the solid Earth. It brings together topics typically addressed in introductory Earth science courses (isostatic rebound, geologic measurements, and climate change) in a way that highlights the interconnectivity of the Earth system and the interpretation of geodetic data. The module was tested 3 times at 3 different institution types (R1 institution, comprehensive university, and community college), and formative and summative assessment data were obtained. We will provide an overview of the instructional materials, describe our teaching methods, and discuss how formative and summative assessment data assisted in revisions of the teaching materials and changes in our pedagogy during subsequent implementation of the module. We will also provide strategies for faculty who wish to incorporate the module into their curricula. Instructional materials, faculty and student resources, and implementation tips are freely available on the GETSI website.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70015528','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70015528"><span><span class="hlt">Mass</span> balance and sliding velocity of the Puget lobe of the cordilleran <span class="hlt">ice</span> sheet during the last glaciation</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Booth, D.B.</p> <p>1986-01-01</p> <p>An estimate of the sliding velocity and basal meltwater discharge of the Puget lobe of the Cordilleran <span class="hlt">ice</span> sheet can be calculated from its reconstructed extent, altitude, and <span class="hlt">mass</span> balance. Lobe dimensions and surface altitudes are inferred from <span class="hlt">ice</span> limits and flow-direction indicators. Net annual <span class="hlt">mass</span> balance and total ablation are calculated from relations empirically derived from modern maritime glaciers. An equilibrium-line altitude between 1200 and 1250 m is calculated for the maximum glacial advance (ca. 15,000 yr B.P.) during the Vashon Stade of the Fraser Glaciation. This estimate is in accord with geologic data and is insensitive to plausible variability in the parameters used in the reconstruction. Resultant sliding velocities are as much as 650 m/a at the equilibrium line, decreasing both up- and downglacier. Such velocities for an <span class="hlt">ice</span> sheet of this size are consistent with nonsurging behavior. Average meltwater discharge increases monotonically downglacier to 3000 m3/sec at the terminus and is of a comparable magnitude to <span class="hlt">ice</span> discharge over much of the glacier's ablation area. Palcoclimatic inferences derived from this reconstruction are consistent with previous, independently derived studies of late Pleistocene temperature and precipitation in the Pacific Northwest. ?? 1986.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11049062','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11049062"><span>Rheological properties of <span class="hlt">ice</span> cream mixes and frozen <span class="hlt">ice</span> creams containing fat and fat replacers.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Adapa, S; Dingeldein, H; Schmidt, K A; Herald, T J</p> <p>2000-10-01</p> <p><span class="hlt">Ice</span> cream mixes and frozen <span class="hlt">ice</span> creams at milk fat levels of 12%, 8%, 6%, 6% plus a protein-based fat replacer, and 6% plus a carbohydrate-based fat replacer were evaluated for viscoelastic properties by dynamic testing with sinusoidal oscillatory tests at various frequencies. The storage modulus (G'), loss modulus (G"), and tan delta (G"/G') were calculated for all the treatments to determine changes in the viscous and elastic properties of the mixes and frozen <span class="hlt">ice</span> creams due to fat <span class="hlt">content</span>. In <span class="hlt">ice</span> cream mixes, G' and G" exhibited a strong frequency dependence. The G" was higher than G' throughout the frequency range (1 to 8 Hz) examined, without any crossover, except for the 12% mix. Elastic properties of the <span class="hlt">ice</span> cream mixes decreased as fat <span class="hlt">content</span> decreased. Tan delta values indicated that fat replacers did not enhance the elastic properties of the <span class="hlt">ice</span> cream mixes. In all frozen <span class="hlt">ice</span> creams, G' and G" again showed a frequency dependence throughout the range tested (0.5 to 10 Hz). The amount of fat in <span class="hlt">ice</span> creams and the degree of fat destabilization affected the elasticity in the frozen product. Even though the <span class="hlt">ice</span> creams did not have significant elastic properties, when compared as a group the samples with higher fat <span class="hlt">content</span> had higher elastic properties. The addition of protein-based and carbohydrate-based fat replacers did not enhance the elastic properties of the <span class="hlt">ice</span> creams but did increase the viscous properties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5097149','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5097149"><span>Production and evaluation of mineral and nutrient <span class="hlt">contents</span>, chemical composition, and sensory properties of <span class="hlt">ice</span> creams fortified with laboratory-prepared peach fibre</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Yangılar, Filiz</p> <p>2016-01-01</p> <p>Background In the coming years, a nutraceutical food may provide both physical and mental benefits that are commonly attributed to the active components of the food. Objective In this study, we determined the nutrient and mineral <span class="hlt">contents</span>, sensory properties, and physical and chemical characteristics of <span class="hlt">ice</span> creams manufactured using peach fibre at different concentrations (1 and 2%). Method A total of five experimental groups were formed: two types (from peach peel and pulp) of flour, two fibre concentrations (1 and 2%), and a control group without fibres. Results Flour obtained from peach pulp and peel was found to have a significant (p<0.05) effect on the chemical composition and elemental composition of <span class="hlt">ice</span> cream samples, especially the rates of Ca, K, Mg, and P, which increased in the samples depending on the <span class="hlt">content</span> of peach fibre. Sensory ratings and acceptability of <span class="hlt">ice</span> creams decreased significantly with increasing peach peel fibre, whereas <span class="hlt">ice</span> creams made with C (control) and B1 (<span class="hlt">ice</span> creams made from 1% peach pulp fibre) was the highest scored by the panellists. Conclusions Peach fibre concentrates might be used as a good source of nutraceutical ingredients. PMID:27814781</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRF..122.2324S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRF..122.2324S"><span>Assimilating the <span class="hlt">ICE</span>-6G_C Reconstruction of the Latest Quaternary <span class="hlt">Ice</span> Age Cycle Into Numerical Simulations of the Laurentide and Fennoscandian <span class="hlt">Ice</span> Sheets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stuhne, G. R.; Peltier, W. R.</p> <p>2017-12-01</p> <p>We analyze the effects of nudging 100 kyr numerical simulations of the Laurentide and Fennoscandian <span class="hlt">ice</span> sheets toward the glacial isostatic adjustment-based (GIA-based) <span class="hlt">ICE</span>-6G_C reconstruction of the most recent <span class="hlt">ice</span> age cycle. Starting with the <span class="hlt">ice</span> physics approximations of the PISM <span class="hlt">ice</span> sheet model and the SeaRISE simulation protocols, we incorporate nudging at characteristic time scales, τf, through anomalous <span class="hlt">mass</span> balance terms in the <span class="hlt">ice</span> <span class="hlt">mass</span> conservation equation. As should be expected, these <span class="hlt">mass</span> balances exhibit physically unrealistic details arising from pure GIA-based reconstruction geometry when nudging is very strong (τf=20 years for North America), while weakly nudged (τf=1,000 years) solutions deviate from <span class="hlt">ICE</span>-6G_C sufficiently to degrade its observational fit quality. For reasonable intermediate time scales (τf=100 years and 200 years), we perturbatively analyze nudged <span class="hlt">ice</span> dynamics as a superposition of "leading-order smoothing" that diffuses <span class="hlt">ICE</span>-6G_C in a physically and observationally consistent manner and "higher-order" deviations arising, for instance, from biases in the time dependence of surface climate boundary conditions. Based upon the relative deviations between respective nudged simulations in which these biases follow surface temperature from <span class="hlt">ice</span> cores and eustatic sea level from marine sediment cores, we compute "<span class="hlt">ice</span> core climate adjustments" that suggest how local paleoclimate observations may be applied to the systematic refinement of <span class="hlt">ICE</span>-6G_C. Our results are consistent with a growing body of evidence suggesting that the geographical origins of Meltwater Pulse 1B (MWP1b) may lie primarily in North America as opposed to Antarctica (as reconstructed in <span class="hlt">ICE</span>-6G_C).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19890018779','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19890018779"><span><span class="hlt">Ice</span> sheet radar altimetry</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zwally, J.</p> <p>1988-01-01</p> <p>The surface topography of the Greenland and Antarctic <span class="hlt">ice</span> sheets between 72 degrees north and south was mapped using radar altimetry data from the U.S. Navy GEOSAT. The glaciological objectives of this activity were to study the dynamics of the <span class="hlt">ice</span> flow, changes in the position of floating <span class="hlt">ice</span>-shelf fronts, and ultimately to measure temporal changes in <span class="hlt">ice</span> surface elevation indicative of <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C12B..07S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C12B..07S"><span>In-situ GPS records of surface <span class="hlt">mass</span> balance, firn compaction rates, and <span class="hlt">ice</span>-shelf basal melt rates for Pine Island Glacier, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shean, D. E.; Christianson, K.; Larson, K. M.; Ligtenberg, S.; Joughin, I. R.; Smith, B.; Stevens, C.</p> <p>2016-12-01</p> <p>In recent decades, Pine Island Glacier (PIG) has experienced marked retreat, speedup and thinning due to <span class="hlt">ice</span>-shelf basal melt, internal <span class="hlt">ice</span>-stream instability and feedbacks between these processes. In an effort to constrain recent <span class="hlt">ice</span>-stream dynamics and evaluate potential causes of retreat, we analyzed 2008-2010 and 2012-2014 GPS records for PIG. We computed time series of horizontal velocity, strain rate, multipath-based antenna height, surface elevation, and Lagrangian elevation change (Dh/Dt). These data provide validation for complementary high-resolution WorldView stereo digital elevation model (DEM) records, with sampled DEM vertical error of 0.7 m. The GPS antenna height time series document a relative surface elevation increase of 0.7-1.0 m/yr, which is consistent with estimated surface <span class="hlt">mass</span> balance (SMB) of 0.7-0.9 m.w.e./yr from RACMO2.3 and firn compaction rates from the IMAU-FDM dynamic firn model. An abrupt 0.2-0.3 m surface elevation decrease due to surface melt and/or greater near-surface firn compaction is observed during a period of warm atmospheric temperatures from December 2012 to January 2013. Observed surface Dh/Dt for all PIG shelf sites is highly linear with trends of -1 to -4 m/yr and <0.4 m residuals. Similar Dh/Dt estimates with reduced variability are obtained after removing expected downward GPS pole base velocity from observed GPS antenna Dh/Dt. Estimated Dh/Dt basal melt rates are 10 to 40 m/yr for the outer PIG shelf and 4 m/yr for the South shelf. These melt rates are similar to those derived from <span class="hlt">ice</span>-bottom acoustic ranging, phase-sensitive <span class="hlt">ice</span>-penetrating radar, and high-resolution stereo DEM records. The GPS/DEM records document higher melt rates within and near transverse surface depressions and rifts associated with longitudinal extension. Basal melt rates for the 2012-2014 period show limited temporal variability, despite significant change in ocean heat <span class="hlt">content</span>. This suggests that sub-shelf melt rates are less sensitive to</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_12 --> <div id="page_13" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="241"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14.3174F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.3174F"><span>Validation and Interpretation of a new sea <span class="hlt">ice</span> Glob<span class="hlt">Ice</span> dataset using buoys and the CICE sea <span class="hlt">ice</span> model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Flocco, D.; Laxon, S. W.; Feltham, D. L.; Haas, C.</p> <p>2012-04-01</p> <p>The Glob<span class="hlt">Ice</span> project has provided high resolution sea <span class="hlt">ice</span> product datasets over the Arctic derived from SAR data in the ESA archive. The products are validated sea <span class="hlt">ice</span> motion, deformation and fluxes through straits. Glob<span class="hlt">Ice</span> sea <span class="hlt">ice</span> velocities, deformation data and sea <span class="hlt">ice</span> concentration have been validated using buoy data provided by the International Arctic Buoy Program (IABP). Over 95% of the Glob<span class="hlt">Ice</span> and buoy data analysed fell within 5 km of each other. The Glob<span class="hlt">Ice</span> Eulerian image pair product showed a high correlation with buoy data. The sea <span class="hlt">ice</span> concentration product was compared to SSM/I data. An evaluation of the validity of the Glob<span class="hlt">ICE</span> data will be presented in this work. Glob<span class="hlt">ICE</span> sea <span class="hlt">ice</span> velocity and deformation were compared with runs of the CICE sea <span class="hlt">ice</span> model: in particular the <span class="hlt">mass</span> fluxes through the straits were used to investigate the correlation between the winter behaviour of sea <span class="hlt">ice</span> and the sea <span class="hlt">ice</span> state in the following summer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990026767&hterms=vertigo&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dvertigo','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990026767&hterms=vertigo&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dvertigo"><span><span class="hlt">Ice</span> as a Construction Material</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zuppero, Anthony; Lewis, J.</p> <p>1998-01-01</p> <p>This presentation shows how water and <span class="hlt">ice</span> can enable exceptionally simple ways to construct structures in deep space. Practicality is underscored by applying advanced tank methods being developed for Mars missions. Water or <span class="hlt">ice</span> is now known to be present or abundant on most objects in the solar system, starting with the planet Mercury. Thermal processes alone can be used to melt <span class="hlt">ice</span> . The cold of space can refreeze water back into <span class="hlt">ice</span>. The anomalous low vapor pressure of water, about 7 mm Hg, permits bladder containers. Tanks or bladders made with modern polymer fiber and film can exhibit very small (<0.1 %) equivalent tankage and ullage fractions and thus hold thousands of tons of water per ton bladder. Injecting water into a bladder whose shape when inflated is the desired final shape, such as a space vehicle, provides a convenient way to construct large structures. In space, structures of 1O,OOO-T <span class="hlt">mass</span> become feasible because the bladder <span class="hlt">mass</span> is low enough to be launched. The bladder can weigh 1OOO times less than its <span class="hlt">contents</span>, or 10 T. The bladder would be packed like a parachute. Shaped memory materials and/or gas inflation could reestablish the desired structure shape after unpacking. The water comes from space resources. An example examines construction of torus space vehicle with 100-m nominal dimension. People would live inside the torus. A torus, like a tire on an automobile, would spin and provide synthetic gravity at its inner surface. A torus of order 100 m across would provide a gravity with gradients low enough to mitigate against vertigo.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016TCry...10..811D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016TCry...10..811D"><span>Constraining variable density of <span class="hlt">ice</span> shelves using wide-angle radar measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Drews, Reinhard; Brown, Joel; Matsuoka, Kenichi; Witrant, Emmanuel; Philippe, Morgane; Hubbard, Bryn; Pattyn, Frank</p> <p>2016-04-01</p> <p>The thickness of <span class="hlt">ice</span> shelves, a basic parameter for <span class="hlt">mass</span> balance estimates, is typically inferred using hydrostatic equilibrium, for which knowledge of the depth-averaged density is essential. The densification from snow to <span class="hlt">ice</span> depends on a number of local factors (e.g., temperature and surface <span class="hlt">mass</span> balance) causing spatial and temporal variations in density-depth profiles. However, direct measurements of firn density are sparse, requiring substantial logistical effort. Here, we infer density from radio-wave propagation speed using ground-based wide-angle radar data sets (10 MHz) collected at five sites on Roi Baudouin <span class="hlt">Ice</span> Shelf (RBIS), Dronning Maud Land, Antarctica. We reconstruct depth to internal reflectors, local <span class="hlt">ice</span> thickness, and firn-air <span class="hlt">content</span> using a novel algorithm that includes traveltime inversion and ray tracing with a prescribed shape of the depth-density relationship. For the particular case of an <span class="hlt">ice</span>-shelf channel, where <span class="hlt">ice</span> thickness and surface slope change substantially over a few kilometers, the radar data suggest that firn inside the channel is about 5 % denser than outside the channel. Although this density difference is at the detection limit of the radar, it is consistent with a similar density anomaly reconstructed from optical televiewing, which reveals that the firn inside the channel is 4.7 % denser than that outside the channel. Hydrostatic <span class="hlt">ice</span> thickness calculations used for determining basal melt rates should account for the denser firn in <span class="hlt">ice</span>-shelf channels. The radar method presented here is robust and can easily be adapted to different radar frequencies and data-acquisition geometries.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.G31C0931W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.G31C0931W"><span>Temporal and spatial variabilities of Antarctic <span class="hlt">ice</span> <span class="hlt">mass</span> changes inferred by GRACE in a Bayesian framework</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, L.; Davis, J. L.; Tamisiea, M. E.</p> <p>2017-12-01</p> <p>The Antarctic <span class="hlt">ice</span> sheet (AIS) holds about 60% of all fresh water on the Earth, an amount equivalent to about 58 m of sea-level rise. Observation of AIS <span class="hlt">mass</span> change is thus essential in determining and predicting its contribution to sea level. While the <span class="hlt">ice</span> <span class="hlt">mass</span> loss estimates for West Antarctica (WA) and the Antarctic Peninsula (AP) are in good agreement, what the <span class="hlt">mass</span> balance over East Antarctica (EA) is, and whether or not it compensates for the <span class="hlt">mass</span> loss is under debate. Besides the different error sources and sensitivities of different measurement types, complex spatial and temporal variabilities would be another factor complicating the accurate estimation of the AIS <span class="hlt">mass</span> balance. Therefore, a model that allows for variabilities in both melting rate and seasonal signals would seem appropriate in the estimation of present-day AIS melting. We present a stochastic filter technique, which enables the Bayesian separation of the systematic stripe noise and <span class="hlt">mass</span> signal in decade-length GRACE monthly gravity series, and allows the estimation of time-variable seasonal and inter-annual components in the signals. One of the primary advantages of this Bayesian method is that it yields statistically rigorous uncertainty estimates reflecting the inherent spatial resolution of the data. By applying the stochastic filter to the decade-long GRACE observations, we present the temporal variabilities of the AIS <span class="hlt">mass</span> balance at basin scale, particularly over East Antarctica, and decipher the EA <span class="hlt">mass</span> variations in the past decade, and their role in affecting overall AIS <span class="hlt">mass</span> balance and sea level.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C23C0798L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C23C0798L"><span>How much can Greenland melt? An upper bound on <span class="hlt">mass</span> loss from the Greenland <span class="hlt">Ice</span> Sheet through surface melting</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, X.; Bassis, J. N.</p> <p>2015-12-01</p> <p>With observations showing accelerated <span class="hlt">mass</span> loss from the Greenland <span class="hlt">Ice</span> Sheet due to surface melt, the Greenland <span class="hlt">Ice</span> Sheet is becoming one of the most significant contributors to sea level rise. The contribution of the Greenland <span class="hlt">Ice</span> Sheet o sea level rise is likely to accelerate in the coming decade and centuries as atmospheric temperatures continue to rise, potentially triggering ever larger surface melt rates. However, at present considerable uncertainty remains in projecting the contribution to sea level of the Greenland <span class="hlt">Ice</span> Sheet both due to uncertainty in atmospheric forcing and the <span class="hlt">ice</span> sheet response to climate forcing. Here we seek an upper bound on the contribution of surface melt from the Greenland to sea level rise in the coming century using a surface energy balance model coupled to an englacial model. We use IPCC Representative Concentration Pathways (RCP8.5, RCP6, RCP4.5, RCP2.6) climate scenarios from an ensemble of global climate models in our simulations to project the maximum rate of <span class="hlt">ice</span> volume loss and related sea-level rise associated with surface melting. To estimate the upper bound, we assume the Greenland <span class="hlt">Ice</span> Sheet is perpetually covered in thick clouds, which maximize longwave radiation to the <span class="hlt">ice</span> sheet. We further assume that deposition of black carbon darkens the <span class="hlt">ice</span> substantially turning it nearly black, substantially reducing its albedo. Although assuming that all melt water not stored in the snow/firn is instantaneously transported off the <span class="hlt">ice</span> sheet increases <span class="hlt">mass</span> loss in the short term, refreezing of retained water warms the <span class="hlt">ice</span> and may lead to more melt in the long term. Hence we examine both assumptions and use the scenario that leads to the most surface melt by 2100. Preliminary models results suggest that under the most aggressive climate forcing, surface melt from the Greenland <span class="hlt">Ice</span> Sheet contributes ~1 m to sea level by the year 2100. This is a significant contribution and ignores dynamic effects. We also examined a lower bound</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGeod..92..299R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGeod..92..299R"><span>Statistically optimal estimation of Greenland <span class="hlt">Ice</span> Sheet <span class="hlt">mass</span> variations from GRACE monthly solutions using an improved mascon approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ran, J.; Ditmar, P.; Klees, R.; Farahani, H. H.</p> <p>2018-03-01</p> <p>We present an improved mascon approach to transform monthly spherical harmonic solutions based on GRACE satellite data into <span class="hlt">mass</span> anomaly estimates in Greenland. The GRACE-based spherical harmonic coefficients are used to synthesize gravity anomalies at satellite altitude, which are then inverted into <span class="hlt">mass</span> anomalies per mascon. The limited spectral <span class="hlt">content</span> of the gravity anomalies is properly accounted for by applying a low-pass filter as part of the inversion procedure to make the functional model spectrally consistent with the data. The full error covariance matrices of the monthly GRACE solutions are properly propagated using the law of covariance propagation. Using numerical experiments, we demonstrate the importance of a proper data weighting and of the spectral consistency between functional model and data. The developed methodology is applied to process real GRACE level-2 data (CSR RL05). The obtained <span class="hlt">mass</span> anomaly estimates are integrated over five drainage systems, as well as over entire Greenland. We find that the statistically optimal data weighting reduces random noise by 35-69%, depending on the drainage system. The obtained <span class="hlt">mass</span> anomaly time-series are de-trended to eliminate the contribution of <span class="hlt">ice</span> discharge and are compared with de-trended surface <span class="hlt">mass</span> balance (SMB) time-series computed with the Regional Atmospheric Climate Model (RACMO 2.3). We show that when using a statistically optimal data weighting in GRACE data processing, the discrepancies between GRACE-based estimates of SMB and modelled SMB are reduced by 24-47%.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150002346','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150002346"><span><span class="hlt">Ice</span> Roughness in Short Duration SLD <span class="hlt">Icing</span> Events</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>McClain, Stephen T.; Reed, Dana; Vargas, Mario; Kreeger, Richard E.; Tsao, Jen-Ching</p> <p>2014-01-01</p> <p><span class="hlt">Ice</span> accretion codes depend on models of roughness parameters to account for the enhanced heat transfer during the <span class="hlt">ice</span> accretion process. While mitigating supercooled large droplet (SLD or Appendix O) <span class="hlt">icing</span> is a significant concern for manufacturers seeking future vehicle certification due to the pending regulation, historical <span class="hlt">ice</span> roughness studies have been performed using Appendix C <span class="hlt">icing</span> clouds which exhibit mean volumetric diameters (MVD) much smaller than SLD clouds. Further, the historical studies of roughness focused on extracting parametric representations of <span class="hlt">ice</span> roughness using multiple images of roughness elements. In this study, the <span class="hlt">ice</span> roughness developed on a 21-in. NACA 0012 at 0deg angle of attack exposed to short duration SLD <span class="hlt">icing</span> events was measured in the <span class="hlt">Icing</span> Research Tunnel at the NASA Glenn Research Center. The MVD's used in the study ranged from 100 micrometer to 200 micrometers, in a 67 m/s flow, with liquid water <span class="hlt">contents</span> of either 0.6 gm/cubic meters or 0.75 gm/cubic meters. The <span class="hlt">ice</span> surfaces were measured using a Romer Absolute Arm laser scanning system. The roughness associated with each surface point cloud was measured using the two-dimensional self-organizing map approach developed by McClain and Kreeger (2013) resulting in statistical descriptions of the <span class="hlt">ice</span> roughness.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21142062','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21142062"><span>Quantification of dissolved organic carbon at very low levels in natural <span class="hlt">ice</span> samples by a UV-induced oxidation method.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Preunkert, S; Legrand, M; Stricker, P; Bulat, S; Alekhina, I; Petit, J R; Hoffmann, H; May, B; Jourdain, B</p> <p>2011-01-15</p> <p>The study of chemical impurities trapped in solid precipitation and accumulated in polar <span class="hlt">ice</span> sheets and high-elevation, midlatitude cold glaciers over the last several hundreds of years provides a unique way to reconstruct our changing atmosphere from the preindustrial era to the present day. Numerous <span class="hlt">ice</span> core studies of inorganic species have already evaluated the effects of growing anthropogenic emissions of SO(2) or NO(x) on the chemical composition of the atmosphere in various regions of the world. While it was recently shown that organic species dominate the atmospheric aerosol <span class="hlt">mass</span>, the contribution of anthropogenic emissions to their budget remains poorly understood. The study of organics in <span class="hlt">ice</span> is at the infancy stage, and it still is difficult to draw a consistent picture of the organic <span class="hlt">content</span> of polar <span class="hlt">ice</span> from sparse available data. A UV oxidation method and IR quantification of CO(2) was optimized to obtain measurements of dissolved organic carbon <span class="hlt">content</span> as low as a few ppbC. Stringent working conditions were defined to prevent contamination during the cleaning of <span class="hlt">ice</span>. Measurements in various <span class="hlt">ice</span> cores corresponding to preindustrial times revealed dissolved organic carbon <span class="hlt">content</span> of less than 10 ppbC in Antarctica and up to 75 ppbC in alpine <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1175859','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/1175859"><span>Methods and apparatus for rotor blade <span class="hlt">ice</span> detection</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>LeMieux, David Lawrence</p> <p>2006-08-08</p> <p>A method for detecting <span class="hlt">ice</span> on a wind turbine having a rotor and one or more rotor blades each having blade roots includes monitoring meteorological conditions relating to <span class="hlt">icing</span> conditions and monitoring one or more physical characteristics of the wind turbine in operation that vary in accordance with at least one of the <span class="hlt">mass</span> of the one or more rotor blades or a <span class="hlt">mass</span> imbalance between the rotor blades. The method also includes using the one or more monitored physical characteristics to determine whether a blade <span class="hlt">mass</span> anomaly exists, determining whether the monitored meteorological conditions are consistent with blade <span class="hlt">icing</span>; and signaling an <span class="hlt">icing</span>-related blade <span class="hlt">mass</span> anomaly when a blade <span class="hlt">mass</span> anomaly is determined to exist and the monitored meteorological conditions are determined to be consistent with <span class="hlt">icing</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16357267','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16357267"><span><span class="hlt">Ice</span> recrystallization inhibition in <span class="hlt">ice</span> cream as affected by <span class="hlt">ice</span> structuring proteins from winter wheat grass.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Regand, A; Goff, H D</p> <p>2006-01-01</p> <p><span class="hlt">Ice</span> recrystallization in quiescently frozen sucrose solutions that contained some of the ingredients commonly found in <span class="hlt">ice</span> cream and in <span class="hlt">ice</span> cream manufactured under commercial conditions, with or without <span class="hlt">ice</span> structuring proteins (ISP) from cold-acclimated winter wheat grass extract (AWWE), was assessed by bright field microscopy. In sucrose solutions, critical differences in moisture <span class="hlt">content</span>, viscosity, ionic strength, and other properties derived from the presence of other ingredients (skim milk powder, corn syrup solids, locust bean gum) caused a reduction in <span class="hlt">ice</span> crystal growth. Significant ISP activity in retarding <span class="hlt">ice</span> crystal growth was observed in all solutions (44% for the most complex mix) containing 0.13% total protein from AWWE. In heat-shocked <span class="hlt">ice</span> cream, <span class="hlt">ice</span> recrystallization rates were significantly reduced 40 and 46% with the addition of 0.0025 and 0.0037% total protein from AWWE. The ISP activity in <span class="hlt">ice</span> cream was not hindered by its inclusion in mix prior to pasteurization. A synergistic effect between ISP and stabilizer was observed, as ISP activity was reduced in the absence of stabilizer in <span class="hlt">ice</span> cream formulations. A remarkably smoother texture for <span class="hlt">ice</span> creams containing ISP after heat-shock storage was evident by sensory evaluation. The efficiency of ISP from AWWE in controlling <span class="hlt">ice</span> crystal growth in <span class="hlt">ice</span> cream has been demonstrated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20080023352&hterms=sauber&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsauber','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20080023352&hterms=sauber&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsauber"><span>Rapid <span class="hlt">Ice</span> <span class="hlt">Mass</span> Loss: Does It Have an Influence on Earthquake Occurrence in Southern Alaska?</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sauber, Jeanne M.</p> <p>2008-01-01</p> <p>The glaciers of southern Alaska are extensive, and many of them have undergone gigatons of <span class="hlt">ice</span> wastage on time scales on the order of the seismic cycle. Since the <span class="hlt">ice</span> loss occurs directly above a shallow main thrust zone associated with subduction of the Pacific-Yakutat plate beneath continental Alaska, the region between the Malaspina and Bering Glaciers is an excellent test site for evaluating the importance of recent <span class="hlt">ice</span> wastage on earthquake faulting potential. We demonstrate the influence of cumulative glacial <span class="hlt">mass</span> loss following the 1899 Yakataga earthquake (M=8.1) by using a two dimensional finite element model with a simple representation of <span class="hlt">ice</span> fluctuations to calculate the incremental stresses and change in the fault stability margin (FSM) along the main thrust zone (MTZ) and on the surface. Along the MTZ, our results indicate a decrease in FSM between 1899 and the 1979 St. Elias earthquake (M=7.4) of 0.2 - 1.2 MPa over an 80 km region between the coast and the 1979 aftershock zone; at the surface, the estimated FSM was larger but more localized to the lower reaches of glacial ablation zones. The <span class="hlt">ice</span>-induced stresses were large enough, in theory, to promote the occurrence of shallow thrust earthquakes. To empirically test the influence of short-term <span class="hlt">ice</span> fluctuations on fault stability, we compared the seismic rate from a reference background time period (1988-1992) against other time periods (1993-2006) with variable <span class="hlt">ice</span> or tectonic change characteristics. We found that the frequency of small tectonic events in the Icy Bay region increased in 2002-2006 relative to the background seismic rate. We hypothesize that this was due to a significant increase in the rate of <span class="hlt">ice</span> wastage in 2002-2006 instead of the M=7.9, 2002 Denali earthquake, located more than 100km away.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('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> sheet 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> sheet presently accounts for ~70% of global <span class="hlt">ice</span> sheet <span class="hlt">mass</span> loss. Because this <span class="hlt">mass</span> 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> sheet <span class="hlt">mass</span> balance is of paramount concern. Spaceborne <span class="hlt">mass</span> 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> sheet <span class="hlt">mass</span> balance. Seasonal loading and unloading of glacial <span class="hlt">mass</span> 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> sheet <span class="hlt">mass</span> balance, yielding new constraints on <span class="hlt">ice</span> sheet evolution and its contribution to global sea-level changes. An increased number of seismic stations in the vicinity of <span class="hlt">ice</span> sheets will enhance our ability to create detailed space-time records of <span class="hlt">ice</span> <span class="hlt">mass</span> variations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12368852','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12368852"><span>Switch of flow direction in an Antarctic <span class="hlt">ice</span> stream.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Conway, H; Catania, G; Raymond, C F; Gades, A M; Scambos, T A; Engelhardt, H</p> <p>2002-10-03</p> <p>Fast-flowing <span class="hlt">ice</span> streams transport <span class="hlt">ice</span> from the interior of West Antarctica to the ocean, and fluctuations in their activity control the <span class="hlt">mass</span> balance of the <span class="hlt">ice</span> sheet. The <span class="hlt">mass</span> balance of the Ross Sea sector of the West Antarctic <span class="hlt">ice</span> sheet is now positive--that is, it is growing--mainly because one of the <span class="hlt">ice</span> streams (<span class="hlt">ice</span> stream C) slowed down about 150 years ago. Here we present evidence from both surface measurements and remote sensing that demonstrates the highly dynamic nature of the Ross drainage system. We show that the flow in an area that once discharged into <span class="hlt">ice</span> stream C has changed direction, now draining into the Whillans <span class="hlt">ice</span> stream (formerly <span class="hlt">ice</span> stream B). This switch in flow direction is a result of continuing thinning of the Whillans <span class="hlt">ice</span> stream and recent thickening of <span class="hlt">ice</span> stream C. Further abrupt reorganization of the activity and configuration of the <span class="hlt">ice</span> streams over short timescales is to be expected in the future as the surface topography of the <span class="hlt">ice</span> sheet responds to the combined effects of internal dynamics and long-term climate change. We suggest that caution is needed when using observations of short-term <span class="hlt">mass</span> changes to draw conclusions about the large-scale <span class="hlt">mass</span> balance of the <span class="hlt">ice</span> sheet.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A22C..02M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A22C..02M"><span>Retrieving the properties of <span class="hlt">ice</span>-phase precipitation with multi-frequency radar measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mace, G. G.; Gergely, M.; Mascio, J.</p> <p>2017-12-01</p> <p>The objective of most retrieval algorithms applied to remote sensing measurements is the microphysical properties that a model might predict such as condensed water <span class="hlt">content</span>, particle number, or effective size. However, because <span class="hlt">ice</span> crystals grow and aggregate into complex non spherical shapes, the microphysical properties of interest are very much dependent on the physical characteristics of the precipitation such as how <span class="hlt">mass</span> and crystal area are distributed as a function of particle size. Such physical properties also have a strong influence on how microwave electromagnetic energy scatters from <span class="hlt">ice</span> crystals causing significant ambiguity in retrieval algorithms. In fact, passive and active microwave remote sensing measurements are typically nearly as sensitive to the <span class="hlt">ice</span> crystal physical properties as they are to the microphysical characteristics that are typically the aim of the retrieval algorithm. There has, however, been active development of multi frequency algorithms recently that attempt to ameliorate and even exploit this sensitivity. In this paper, we will review these approaches and present practical applications of retrieving <span class="hlt">ice</span> crystal properties such as <span class="hlt">mass</span>- and area dimensional relationships from single and dual frequency radar measurements of precipitating <span class="hlt">ice</span> using data collected aboard ship in the Southern Ocean and from remote sensors in the Rocky Mountains of the Western U.S.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C14B..04B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C14B..04B"><span>Understanding <span class="hlt">Ice</span> Shelf Basal Melting Using Convergent ICEPOD Data Sets: ROSETTA-<span class="hlt">Ice</span> Study of Ross <span class="hlt">Ice</span> Shelf</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bell, R. E.; Frearson, N.; Tinto, K. J.; Das, I.; Fricker, H. A.; Siddoway, C. S.; Padman, L.</p> <p>2017-12-01</p> <p>The future stability of the <span class="hlt">ice</span> shelves surrounding Antarctica will be susceptible to increases in both surface and basal melt as the atmosphere and ocean warm. The ROSETTA-<span class="hlt">Ice</span> program is targeted at using the ICEPOD airborne technology to produce new constraints on Ross <span class="hlt">Ice</span> Shelf, the underlying ocean, bathymetry, and geologic setting, using radar sounding, gravimetry and laser altimetry. This convergent approach to studying the <span class="hlt">ice</span>-shelf and basal processes enables us to develop an understanding of the fundamental controls on <span class="hlt">ice</span>-shelf evolution. This work leverages the stratigraphy of the <span class="hlt">ice</span> shelf, which is detected as individual reflectors by the shallow-<span class="hlt">ice</span> radar and is often associated with surface scour, form close to the grounding line or pinning points on the <span class="hlt">ice</span> shelf. Surface accumulation on the <span class="hlt">ice</span> shelf buries these reflectors as the <span class="hlt">ice</span> flows towards the calving front. This distinctive stratigraphy can be traced across the <span class="hlt">ice</span> shelf for the major East Antarctic outlet glaciers and West Antarctic <span class="hlt">ice</span> streams. Changes in the <span class="hlt">ice</span> thickness below these reflectors are a result of strain and basal melting and freezing. Correcting the estimated thickness changes for strain using RIGGS strain measurements, we can develop decadal-resolution flowline distributions of basal melt. Close to East Antarctica elevated melt-rates (>1 m/yr) are found 60-100 km from the calving front. On the West Antarctic side high melt rates primarily develop within 10 km of the calving front. The East Antarctic side of Ross <span class="hlt">Ice</span> Shelf is dominated by melt driven by saline water <span class="hlt">masses</span> that develop in Ross Sea polynyas, while the melting on the West Antarctic side next to Hayes Bank is associated with modified Continental Deep Water transported along the continental shelf. The two sides of Ross <span class="hlt">Ice</span> Shelf experience differing basal melt in part due to the duality in the underlying geologic structure: the East Antarctic side consists of relatively dense crust, with low amplitude</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRD..121.5809W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRD..121.5809W"><span>Retrieval of <span class="hlt">ice</span> cloud properties using an optimal estimation algorithm and MODIS infrared observations: 1. Forward model, error analysis, and information <span class="hlt">content</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Chenxi; Platnick, Steven; Zhang, Zhibo; Meyer, Kerry; Yang, Ping</p> <p>2016-05-01</p> <p>An optimal estimation (OE) retrieval method is developed to infer three <span class="hlt">ice</span> cloud properties simultaneously: optical thickness (τ), effective radius (reff), and cloud top height (h). This method is based on a fast radiative transfer (RT) model and infrared (IR) observations from the MODerate resolution Imaging Spectroradiometer (MODIS). This study conducts thorough error and information <span class="hlt">content</span> analyses to understand the error propagation and performance of retrievals from various MODIS band combinations under different cloud/atmosphere states. Specifically, the algorithm takes into account four error sources: measurement uncertainty, fast RT model uncertainty, uncertainties in ancillary data sets (e.g., atmospheric state), and assumed <span class="hlt">ice</span> crystal habit uncertainties. It is found that the ancillary and <span class="hlt">ice</span> crystal habit error sources dominate the MODIS IR retrieval uncertainty and cannot be ignored. The information <span class="hlt">content</span> analysis shows that for a given <span class="hlt">ice</span> cloud, the use of four MODIS IR observations is sufficient to retrieve the three cloud properties. However, the selection of MODIS IR bands that provide the most information and their order of importance varies with both the <span class="hlt">ice</span> cloud properties and the ambient atmospheric and the surface states. As a result, this study suggests the inclusion of all MODIS IR bands in practice since little a priori information is available.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1253683-testing-ice-microphysics-parameterizations-ncar-community-atmospheric-model-version-using-tropical-warm-pool-international-cloud-experiment-data','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1253683-testing-ice-microphysics-parameterizations-ncar-community-atmospheric-model-version-using-tropical-warm-pool-international-cloud-experiment-data"><span>Testing <span class="hlt">ice</span> microphysics parameterizations in the NCAR Community Atmospheric Model Version 3 using Tropical Warm Pool-International Cloud Experiment data</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Wang, Weiguo; Liu, Xiaohong; Xie, Shaocheng; ...</p> <p>2009-07-23</p> <p>Here, cloud properties have been simulated with a new double-moment microphysics scheme under the framework of the single-column version of NCAR Community Atmospheric Model version 3 (CAM3). For comparison, the same simulation was made with the standard single-moment microphysics scheme of CAM3. Results from both simulations compared favorably with observations during the Tropical Warm Pool–International Cloud Experiment by the U.S. Department of Energy Atmospheric Radiation Measurement Program in terms of the temporal variation and vertical distribution of cloud fraction and cloud condensate. Major differences between the two simulations are in the magnitude and distribution of <span class="hlt">ice</span> water <span class="hlt">content</span> within themore » mixed-phase cloud during the monsoon period, though the total frozen water (snow plus <span class="hlt">ice</span>) <span class="hlt">contents</span> are similar. The <span class="hlt">ice</span> <span class="hlt">mass</span> <span class="hlt">content</span> in the mixed-phase cloud from the new scheme is larger than that from the standard scheme, and <span class="hlt">ice</span> water <span class="hlt">content</span> extends 2 km further downward, which is in better agreement with observations. The dependence of the frozen water <span class="hlt">mass</span> fraction on temperature from the new scheme is also in better agreement with available observations. Outgoing longwave radiation (OLR) at the top of the atmosphere (TOA) from the simulation with the new scheme is, in general, larger than that with the standard scheme, while the surface downward longwave radiation is similar. Sensitivity tests suggest that different treatments of the <span class="hlt">ice</span> crystal effective radius contribute significantly to the difference in the calculations of TOA OLR, in addition to cloud water path. Numerical experiments show that cloud properties in the new scheme can respond reasonably to changes in the concentration of aerosols and emphasize the importance of correctly simulating aerosol effects in climate models for aerosol-cloud interactions. Further evaluation, especially for <span class="hlt">ice</span> cloud properties based on in-situ data, is needed.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EPJWC..9906002G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EPJWC..9906002G"><span>Measuring the muon <span class="hlt">content</span> of air showers with <span class="hlt">Ice</span>Top</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gonzalez, Javier G.</p> <p>2015-08-01</p> <p><span class="hlt">Ice</span>Top, the surface component of the <span class="hlt">Ice</span>Cube detector, has been used to measure the energy spectrum of cosmic ray primaries in the range between 1.58 PeV and 1.26 EeV. It can also be used to study the low energy muons in air showers by looking at large distances (> 300 m) from the shower axis. We will show the muon lateral distribution function at large lateral distances as measured with <span class="hlt">Ice</span>Top and discuss the implications of this measurement. We will also discuss the prospects for low energy muon studies with <span class="hlt">Ice</span>Top.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ApJ...837..168F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ApJ...837..168F"><span>Cometary Materials Originating from Interstellar <span class="hlt">Ices</span>: Clues from Laboratory Experiments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fresneau, A.; Abou Mrad, N.; d'Hendecourt, L. LS; Duvernay, F.; Flandinet, L.; Orthous-Daunay, F.-R.; Vuitton, V.; Thissen, R.; Chiavassa, T.; Danger, G.</p> <p>2017-03-01</p> <p>We use laboratory experiments to derive information on the chemistry occurring during the evolution of astrophysical <span class="hlt">ices</span> from dense molecular clouds to interplanetary objects. Through a new strategy that consists of coupling very high resolution <span class="hlt">mass</span> spectrometry and infrared spectroscopy (FT-IR), we investigate the molecular <span class="hlt">content</span> of the organic residues synthesized from different initial <span class="hlt">ice</span> compositions. We also obtain information on the evolution of the soluble part of the residues after their over-irradiation. The results give insight into the role of water <span class="hlt">ice</span> as a trapping and diluting agent during the chemical evolution. They also give information about the importance of the amount of ammonia in such <span class="hlt">ices</span>, particularly regarding its competition with the carbon chemistry. All of these results allow us to build a first mapping of the evolution of soluble organic matter based on its chemical and physical history. Furthermore, our results suggest that interstellar <span class="hlt">ices</span> should lead to organic materials enriched in heteroatoms that present similarities with cometary materials but strongly differ from meteoritic organic material, especially in their C/N ratios.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015NatGe...8..534U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015NatGe...8..534U"><span>Laurentide <span class="hlt">ice</span>-sheet instability during the last deglaciation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ullman, David J.; Carlson, Anders E.; Anslow, Faron S.; Legrande, Allegra N.; Licciardi, Joseph M.</p> <p>2015-07-01</p> <p>Changes in the amount of summer incoming solar radiation (insolation) reaching the Northern Hemisphere are the underlying pacemaker of glacial cycles. However, not all rises in boreal summer insolation over the past 800,000 years resulted in deglaciation to present-day <span class="hlt">ice</span> volumes, suggesting that there may be a climatic threshold for the disappearance of land-based <span class="hlt">ice</span>. Here we assess the surface <span class="hlt">mass</span> balance stability of the Laurentide <span class="hlt">ice</span> sheet--the largest glacial <span class="hlt">ice</span> <span class="hlt">mass</span> in the Northern Hemisphere--during the last deglaciation (24,000 to 9,000 years ago). We run a surface energy balance model with climate data from simulations with a fully coupled atmosphere-ocean general circulation model for key time slices during the last deglaciation. We find that the surface <span class="hlt">mass</span> balance of the Laurentide <span class="hlt">ice</span> sheet was positive throughout much of the deglaciation, and suggest that dynamic discharge was mainly responsible for <span class="hlt">mass</span> loss during this time. Total surface <span class="hlt">mass</span> balance became negative only in the early Holocene, indicating the transition to a new state where <span class="hlt">ice</span> loss occurred primarily by surface ablation. We conclude that the Laurentide <span class="hlt">ice</span> sheet remained a viable <span class="hlt">ice</span> sheet before the Holocene and began to fully deglaciate only once summer temperatures and radiative forcing over the <span class="hlt">ice</span> sheet increased by 6-7 °C and 16-20 W m-2, respectively, relative to full glacial conditions.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_13 --> <div id="page_14" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="261"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170007301','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170007301"><span>Evaluation of Alternative Altitude Scaling Methods for Thermal <span class="hlt">Ice</span> Protection System in NASA <span class="hlt">Icing</span> Research Tunnel</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lee, Sam; Addy, Harold; Broeren, Andy P.; Orchard, David M.</p> <p>2017-01-01</p> <p>A test was conducted at NASA <span class="hlt">Icing</span> Research Tunnel to evaluate altitude scaling methods for thermal <span class="hlt">ice</span> protection system. Two scaling methods based on Weber number were compared against a method based on the Reynolds number. The results generally agreed with the previous set of tests conducted in NRCC Altitude <span class="hlt">Icing</span> Wind Tunnel. The Weber number based scaling methods resulted in smaller runback <span class="hlt">ice</span> <span class="hlt">mass</span> than the Reynolds number based scaling method. The <span class="hlt">ice</span> accretions from the Weber number based scaling method also formed farther upstream. However there were large differences in the accreted <span class="hlt">ice</span> <span class="hlt">mass</span> between the two Weber number based scaling methods. The difference became greater when the speed was increased. This indicated that there may be some Reynolds number effects that isnt fully accounted for and warrants further study.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990071137&hterms=ice+mechanics&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dice%2Bmechanics','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990071137&hterms=ice+mechanics&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dice%2Bmechanics"><span><span class="hlt">Ice</span> Flow in the North East Greenland <span class="hlt">Ice</span> Stream</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Joughin, Ian; Kwok, Ron; Fahnestock, M.; MacAyeal, Doug</p> <p>1999-01-01</p> <p>Early observations with ERS-1 SAR image data revealed a large <span class="hlt">ice</span> stream in North East Greenland (Fahnestock 1993). The <span class="hlt">ice</span> stream has a number of the characteristics of the more closely studied <span class="hlt">ice</span> streams in Antarctica, including its large size and gross geometry. The onset of rapid flow close to the <span class="hlt">ice</span> divide and the evolution of its flow pattern, however, make this <span class="hlt">ice</span> stream unique. These features can be seen in the balance velocities for the <span class="hlt">ice</span> stream (Joughin 1997) and its outlets. The <span class="hlt">ice</span> stream is identifiable for more than 700 km, making it much longer than any other flow feature in Greenland. Our research goals are to gain a greater understanding of the <span class="hlt">ice</span> flow in the northeast Greenland <span class="hlt">ice</span> stream and its outlet glaciers in order to assess their impact on the past, present, and future <span class="hlt">mass</span> balance of the <span class="hlt">ice</span> sheet. We will accomplish these goals using a combination of remotely sensed data and <span class="hlt">ice</span> sheet models. We are using satellite radar interferometry data to produce a complete maps of velocity and topography over the entire <span class="hlt">ice</span> stream. We are in the process of developing methods to use these data in conjunction with existing <span class="hlt">ice</span> sheet models similar to those that have been used to improve understanding of the mechanics of flow in Antarctic <span class="hlt">ice</span> streams.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.C43E0587P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.C43E0587P"><span>A Changing Arctic Sea <span class="hlt">Ice</span> Cover and the Partitioning of Solar Radiation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Perovich, D. K.; Light, B.; Polashenski, C.; Nghiem, S. V.</p> <p>2010-12-01</p> <p>Certain recent changes in the Arctic sea <span class="hlt">ice</span> cover are well established. There has been a reduction in sea <span class="hlt">ice</span> extent, an overall thinning of the <span class="hlt">ice</span> cover, reduced prevalence of perennial <span class="hlt">ice</span> with accompanying increases in seasonal <span class="hlt">ice</span>, and a lengthening of the summer melt season. Here we explore the effects of these changes on the partitioning of solar energy between reflection to the atmosphere, absorption within the <span class="hlt">ice</span>, and transmission to the ocean. The physical changes in the <span class="hlt">ice</span> cover result in less light reflected and more light absorbed in the <span class="hlt">ice</span> and transmitted to the ocean. These changes directly affect the heat and <span class="hlt">mass</span> balance of the <span class="hlt">ice</span> as well as the amount of light available for photosynthesis within and beneath the <span class="hlt">ice</span> cover. The central driver is that seasonal <span class="hlt">ice</span> covers tend to have lower albedo than perennial <span class="hlt">ice</span> throughout the melt season, permitting more light to penetrate into the <span class="hlt">ice</span> and ocean. The enhanced light penetration increases the amount of internal melting of the <span class="hlt">ice</span> and the heat <span class="hlt">content</span> of the upper ocean. The physical changes in the <span class="hlt">ice</span> cover mentioned above have affected both the amount and the timing of the photosynthetically active radiation (PAR) transmitted into the <span class="hlt">ice</span> and ocean, increasing transmitted PAR, particularly in the spring. A comparison of the partitioning of solar irradiance and PAR for both historical and recent <span class="hlt">ice</span> conditions will be presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.C11A0533C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.C11A0533C"><span>From Outlet Glacier Changes to <span class="hlt">Ice</span> Sheet <span class="hlt">Mass</span> Balance - Evolution of Greenland <span class="hlt">Ice</span> Sheet from Laser Altimetry Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Csatho, B. M.; Schenk, A.; Nagarajan, S.; Babonis, G. S.</p> <p>2010-12-01</p> <p>Investigations of <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balance and the changing dynamics of outlet glaciers have been hampered by the lack of comprehensive data. In recent years, this situation has been remedied. Satellite laser altimetry data from the <span class="hlt">Ice</span> Cloud and land Elevation Satellite mission (ICESat), combined with airborne laser altimetry, provide accurate measurements of surface elevation changes, and surface velocities derived from various satellite platforms yield crucial information on changing glacier dynamics. Taken together, a rich and diverse data set is emerging that allows for characterizing the spatial and temporal evolution of <span class="hlt">ice</span> sheets and outlet glaciers. In particular, it enables quantitative studies of outlet glaciers undergoing rapid and complex changes. Although airborne and laser altimetry have been providing precise measurements of <span class="hlt">ice</span> sheet topography since the early 1990s, determining detailed and accurate spatial and temporal distribution of surface changes remains a challenging problem. We have developed a new, comprehensive method, called Surface Elevation Reconstruction And Change detection (SERAC), which estimates surface changes by a simultaneous reconstruction of surface topography from fused multisensor data. The mathematical model is based on the assumption that for a small surface area, only the absolute elevation changes over time but not the shape of the surface patch. Therefore, laser points of all time epochs contribute to the shape parameters; points of each time period determine the absolute elevation of the surface patch at that period. This method provides high-resolution surface topography, precise changes and a rigorous error estimate of the quantities. By using SERAC we combined ICESat and ATM laser altimetry data to determine the evolution of surface change rates of the whole Greenland <span class="hlt">Ice</span> Sheet between 2003 and 2009 on a high-resolution grid. Our reconstruction, consistent with GRACE results, shows <span class="hlt">ice</span> sheet thinning propagating</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.U32A..03R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.U32A..03R"><span>The Milankovitch Signature of the air <span class="hlt">Content</span> Along the EPICA DC <span class="hlt">Ice</span> Record: a Tool Towards an Absolute Dating and Implication for <span class="hlt">ice</span> Flow Modeling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Raynaud, D.; Duval, P.; Lemieux-Dudon, B.; Lipenkov, V.; Parrenin, F.</p> <p>2006-12-01</p> <p>Air <span class="hlt">content</span> of polar <span class="hlt">ice</span>, V, depends primarily on air pressure, temperature and pore volume at close-off prevailing at the site of <span class="hlt">ice</span> formation. Here we present the recently measured V record of the EPICA DC (EDC) Antarctic <span class="hlt">ice</span> core covering the last 650,000 years. The first 440,000 years remarkably displays the fundamental Milankovitch orbital frequencies. The 100 kyr period, corresponding to the eccentricity of the Earth's orbit and found in the V record, likely reflects essentially the pressure/elevation signature of V. But most of the variations observed in the V record cannot be explained neither by air pressure nor by temperature changes, and then should reflect properties influencing the porosity at close-off other than temperature. A wavelet analysis indicates a dominant period around 41 kyr, the period characteristic of the obliquity variations of the Earth's axis. We propose that the local insolation, via the solar radiation absorbed by the snow, leaves its imprint on the snow structure, then affects the snow-firn transition, and therefore is one of the controlling factors for the porosity at close-off. Such mechanism could account for the observed anti-correlation between local insolation and V. We estimate the variations of the absorbed solar flux in the near-surface snow layers on the basis of a simple albedo model (Lemieux-Dudon et al., this session). We compare the dating of the <span class="hlt">ice</span> obtained using the local insolation signal deduced from the V record with a chronology based on <span class="hlt">ice</span> flow modelling. We discuss the glaciological implications of the comparison between the two chronologies, as well as the potential of local insolation markers for approaching an absolute dating of <span class="hlt">ice</span> core. The latest results covering the period 440-650 kyr BP will also be presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.C41D..02R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.C41D..02R"><span><span class="hlt">Ice</span>-shelf melting around Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rignot, E.; Jacobs, S.</p> <p>2008-12-01</p> <p>The traditional view on the <span class="hlt">mass</span> balance of Antarctic <span class="hlt">ice</span> shelves is that they loose <span class="hlt">mass</span> principally from iceberg calving with bottom melting a much lower contributing factor. Because <span class="hlt">ice</span> shelves are now known to play a fundamental role in <span class="hlt">ice</span> sheet evolution, it is important to re-evaluate their wastage processes from a circumpolar perspective using a combination of remote sensing techniques. We present area average rates deduced from grounding line discharge, snow accumulation, firn depth correction and <span class="hlt">ice</span> shelf topography. We find that <span class="hlt">ice</span> shelf melting accounts for roughly half of <span class="hlt">ice</span>-shelf ablation, with a total melt water production of 1027 Gt/yr. The attrition fraction due to in-situ melting varies from 9 to 90 percent around Antarctica. High melt producers include the Ronne, Ross, Getz, Totten, Amery, George VI, Pine Island, Abbot, Dotson/Crosson, Shackleton, Thwaites and Moscow University <span class="hlt">Ice</span> Shelves. Low producers include the Larsen C, Princess Astrid and Ragnhild coast, Fimbul, Brunt and Filchner. Correlation between melt water production and grounding line discharge is low (R2 = 0.65). Correlation with thermal ocean forcing from the ocean are highest in the northern parts of West Antarctica where regressions yield R2 of 0.93-0.97. Melt rates in the Amundsen Sea exhibit a quadratic sensitivity to thermal ocean forcing. We conclude that <span class="hlt">ice</span> shelf melting plays a dominant role in <span class="hlt">ice</span> shelf <span class="hlt">mass</span> balance, with a potential to change rapidly in response to altered ocean heat transport onto the Antarctic continental shelf.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C11B0906W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C11B0906W"><span>Gaussian Process Model for Antarctic Surface <span class="hlt">Mass</span> Balance and <span class="hlt">Ice</span> Core Site Selection</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>White, P. A.; Reese, S.; Christensen, W. F.; Rupper, S.</p> <p>2017-12-01</p> <p>Surface <span class="hlt">mass</span> balance (SMB) is an important factor in the estimation of sea level change, and data are collected to estimate models for prediction of SMB on the Antarctic <span class="hlt">ice</span> sheet. Using Favier et al.'s (2013) quality-controlled aggregate data set of SMB field measurements, a fully Bayesian spatial model is posed to estimate Antarctic SMB and propose new field measurement locations. Utilizing Nearest-Neighbor Gaussian process (NNGP) models, SMB is estimated over the Antarctic <span class="hlt">ice</span> sheet. An Antarctic SMB map is rendered using this model and is compared with previous estimates. A prediction uncertainty map is created to identify regions of high SMB uncertainty. The model estimates net SMB to be 2173 Gton yr-1 with 95% credible interval (2021,2331) Gton yr-1. On average, these results suggest lower Antarctic SMB and higher uncertainty than previously purported [Vaughan et al. (1999); Van de Berg et al. (2006); Arthern, Winebrenner and Vaughan (2006); Bromwich et al. (2004); Lenaerts et al. (2012)], even though this model utilizes significantly more observations than previous models. Using the Gaussian process' uncertainty and model parameters, we propose 15 new measurement locations for field study utilizing a maximin space-filling, error-minimizing design; these potential measurements are identied to minimize future estimation uncertainty. Using currently accepted Antarctic <span class="hlt">mass</span> balance estimates and our SMB estimate, we estimate net <span class="hlt">mass</span> loss [Shepherd et al. (2012); Jacob et al. (2012)]. Furthermore, we discuss modeling details for both space-time data and combining field measurement data with output from mathematical models using the NNGP framework.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5916768','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5916768"><span>Retrieval of <span class="hlt">ice</span> cloud properties using an optimal estimation algorithm and MODIS infrared observations. Part I: Forward model, error analysis, and information <span class="hlt">content</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>Wang, Chenxi; Platnick, Steven; Zhang, Zhibo; Meyer, Kerry; Yang, Ping</p> <p>2018-01-01</p> <p>An optimal estimation (OE) retrieval method is developed to infer three <span class="hlt">ice</span> cloud properties simultaneously: optical thickness (τ), effective radius (reff), and cloud-top height (h). This method is based on a fast radiative transfer (RT) model and infrared (IR) observations from the MODerate resolution Imaging Spectroradiometer (MODIS). This study conducts thorough error and information <span class="hlt">content</span> analyses to understand the error propagation and performance of retrievals from various MODIS band combinations under different cloud/atmosphere states. Specifically, the algorithm takes into account four error sources: measurement uncertainty, fast RT model uncertainty, uncertainties in ancillary datasets (e.g., atmospheric state), and assumed <span class="hlt">ice</span> crystal habit uncertainties. It is found that the ancillary and <span class="hlt">ice</span> crystal habit error sources dominate the MODIS IR retrieval uncertainty and cannot be ignored. The information <span class="hlt">content</span> analysis shows that, for a given <span class="hlt">ice</span> cloud, the use of four MODIS IR observations is sufficient to retrieve the three cloud properties. However, the selection of MODIS IR bands that provide the most information and their order of importance varies with both the <span class="hlt">ice</span> cloud properties and the ambient atmospheric and the surface states. As a result, this study suggests the inclusion of all MODIS IR bands in practice since little a priori information is available. PMID:29707470</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170002706','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170002706"><span>Retrieval of <span class="hlt">Ice</span> Cloud Properties Using an Optimal Estimation Algorithm and MODIS Infrared Observations. Part I: Forward Model, Error Analysis, and Information <span class="hlt">Content</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wang, Chenxi; Platnick, Steven; Zhang, Zhibo; Meyer, Kerry; Yang, Ping</p> <p>2016-01-01</p> <p>An optimal estimation (OE) retrieval method is developed to infer three <span class="hlt">ice</span> cloud properties simultaneously: optical thickness (tau), effective radius (r(sub eff)), and cloud-top height (h). This method is based on a fast radiative transfer (RT) model and infrared (IR) observations from the MODerate resolution Imaging Spectroradiometer (MODIS). This study conducts thorough error and information <span class="hlt">content</span> analyses to understand the error propagation and performance of retrievals from various MODIS band combinations under different cloud/atmosphere states. Specifically, the algorithm takes into account four error sources: measurement uncertainty, fast RT model uncertainty, uncertainties in ancillary datasets (e.g., atmospheric state), and assumed <span class="hlt">ice</span> crystal habit uncertainties. It is found that the ancillary and <span class="hlt">ice</span> crystal habit error sources dominate the MODIS IR retrieval uncertainty and cannot be ignored. The information <span class="hlt">content</span> analysis shows that, for a given <span class="hlt">ice</span> cloud, the use of four MODIS IR observations is sufficient to retrieve the three cloud properties. However, the selection of MODIS IR bands that provide the most information and their order of importance varies with both the <span class="hlt">ice</span> cloud properties and the ambient atmospheric and the surface states. As a result, this study suggests the inclusion of all MODIS IR bands in practice since little a priori information is available.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170003730','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170003730"><span>Retrieval of <span class="hlt">Ice</span> Cloud Properties Using an Optimal Estimation Algorithm and MODIS Infrared Observations. Part I: Forward Model, Error Analysis, and Information <span class="hlt">Content</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wang, Chenxi; Platnick, Steven; Zhang, Zhibo; Meyer, Kerry; Yang, Ping</p> <p>2016-01-01</p> <p>An optimal estimation (OE) retrieval method is developed to infer three <span class="hlt">ice</span> cloud properties simultaneously: optical thickness (tau), effective radius (r(sub eff)), and cloud top height (h). This method is based on a fast radiative transfer (RT) model and infrared (IR) observations from the MODerate resolution Imaging Spectroradiometer (MODIS). This study conducts thorough error and information <span class="hlt">content</span> analyses to understand the error propagation and performance of retrievals from various MODIS band combinations under different cloud/atmosphere states. Specifically, the algorithm takes into account four error sources: measurement uncertainty, fast RT model uncertainty, uncertainties in ancillary data sets (e.g., atmospheric state), and assumed <span class="hlt">ice</span> crystal habit uncertainties. It is found that the ancillary and <span class="hlt">ice</span> crystal habit error sources dominate the MODIS IR retrieval uncertainty and cannot be ignored. The information <span class="hlt">content</span> analysis shows that for a given <span class="hlt">ice</span> cloud, the use of four MODIS IR observations is sufficient to retrieve the three cloud properties. However, the selection of MODIS IR bands that provide the most information and their order of importance varies with both the <span class="hlt">ice</span> cloud properties and the ambient atmospheric and the surface states. As a result, this study suggests the inclusion of all MODIS IR bands in practice since little a priori information is available.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29707470','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29707470"><span>Retrieval of <span class="hlt">ice</span> cloud properties using an optimal estimation algorithm and MODIS infrared observations. Part I: Forward model, error analysis, and information <span class="hlt">content</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Chenxi; Platnick, Steven; Zhang, Zhibo; Meyer, Kerry; Yang, Ping</p> <p>2016-05-27</p> <p>An optimal estimation (OE) retrieval method is developed to infer three <span class="hlt">ice</span> cloud properties simultaneously: optical thickness ( τ ), effective radius ( r eff ), and cloud-top height ( h ). This method is based on a fast radiative transfer (RT) model and infrared (IR) observations from the MODerate resolution Imaging Spectroradiometer (MODIS). This study conducts thorough error and information <span class="hlt">content</span> analyses to understand the error propagation and performance of retrievals from various MODIS band combinations under different cloud/atmosphere states. Specifically, the algorithm takes into account four error sources: measurement uncertainty, fast RT model uncertainty, uncertainties in ancillary datasets (e.g., atmospheric state), and assumed <span class="hlt">ice</span> crystal habit uncertainties. It is found that the ancillary and <span class="hlt">ice</span> crystal habit error sources dominate the MODIS IR retrieval uncertainty and cannot be ignored. The information <span class="hlt">content</span> analysis shows that, for a given <span class="hlt">ice</span> cloud, the use of four MODIS IR observations is sufficient to retrieve the three cloud properties. However, the selection of MODIS IR bands that provide the most information and their order of importance varies with both the <span class="hlt">ice</span> cloud properties and the ambient atmospheric and the surface states. As a result, this study suggests the inclusion of all MODIS IR bands in practice since little a priori information is available.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1990JGR....9515959H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1990JGR....9515959H"><span>One hundred years of Arctic <span class="hlt">ice</span> cover variations as simulated by a one-dimensional, <span class="hlt">ice</span>-ocean model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hakkinen, S.; Mellor, G. L.</p> <p>1990-09-01</p> <p>A one-dimensional <span class="hlt">ice</span>-ocean model consisting of a second moment, turbulent closure, mixed layer model and a three-layer snow-<span class="hlt">ice</span> model has been applied to the simulation of Arctic <span class="hlt">ice</span> <span class="hlt">mass</span> and mixed layer properties. The results for the climatological seasonal cycle are discussed first and include the salt and heat balance in the upper ocean. The coupled model is then applied to the period 1880-1985, using the surface air temperature fluctuations from Hansen et al. (1983) and from Wigley et al. (1981). The analysis of the simulated large variations of the Arctic <span class="hlt">ice</span> <span class="hlt">mass</span> during this period (with similar changes in the mixed layer salinity) shows that the variability in the summer melt determines to a high degree the variability in the average <span class="hlt">ice</span> thickness. The annual oceanic heat flux from the deep ocean and the maximum freezing rate and associated nearly constant minimum surface salinity flux did not vary significantly interannually. This also implies that the oceanic influence on the Arctic <span class="hlt">ice</span> <span class="hlt">mass</span> is minimal for the range of atmospheric variability tested.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19830046585&hterms=guinea+pig&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dguinea%2Bpig','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19830046585&hterms=guinea+pig&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dguinea%2Bpig"><span>Estimation of skeletal muscle <span class="hlt">mass</span> from body creatine <span class="hlt">content</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Pace, N.; Rahlmann, D. F.</p> <p>1982-01-01</p> <p>Procedures have been developed for studying the effect of changes in gravitational loading on skeletal muscle <span class="hlt">mass</span> through measurements of the body creatine <span class="hlt">content</span>. These procedures were developed for studies of gravitational scale effects in a four-species model, comprising the hamster, rat, guinea pig, and rabbit, which provides a sufficient range of body size for assessment of allometric parameters. Since intracellular muscle creatine concentration varies among species, and with age within a given species, the concentration values for metabolically mature individuals of these four species were established. The creatine <span class="hlt">content</span> of the carcass, skin, viscera, smooth muscle, and skeletal muscle was determined for each species. In addition, the skeletal muscle <span class="hlt">mass</span> of the major body components was determined, as well as the total and fat-free <span class="hlt">masses</span> of the body and carcass, and the percent skeletal muscle in each. It is concluded that these procedures are particularly useful for studying the effect of gravitational loading on the skeletal muscle <span class="hlt">content</span> of the animal carcass, which is the principal weight-bearing organ of the body.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20130009418','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130009418"><span>Airborne Tomographic Swath <span class="hlt">Ice</span> Sounding Processing System</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wu, Xiaoqing; Rodriquez, Ernesto; Freeman, Anthony; Jezek, Ken</p> <p>2013-01-01</p> <p>Glaciers and <span class="hlt">ice</span> sheets modulate global sea level by storing water deposited as snow on the surface, and discharging water back into the ocean through melting. Their physical state can be characterized in terms of their <span class="hlt">mass</span> balance and dynamics. To estimate the current <span class="hlt">ice</span> <span class="hlt">mass</span> balance, and to predict future changes in the motion of the Greenland and Antarctic <span class="hlt">ice</span> sheets, it is necessary to know the <span class="hlt">ice</span> sheet thickness and the physical conditions of the <span class="hlt">ice</span> sheet surface and bed. This information is required at fine resolution and over extensive portions of the <span class="hlt">ice</span> sheets. A tomographic algorithm has been developed to take raw data collected by a multiple-channel synthetic aperture sounding radar system over a polar <span class="hlt">ice</span> sheet and convert those data into two-dimensional (2D) <span class="hlt">ice</span> thickness measurements. Prior to this work, conventional processing techniques only provided one-dimensional <span class="hlt">ice</span> thickness measurements along profiles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19810068581','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19810068581"><span>Investigation of Aerodynamic and <span class="hlt">Icing</span> Characteristics of a Flush Alternate Inlet Induction System Air Scoop</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lewis, James P.</p> <p>1953-01-01</p> <p>An investigation has been made in the NACA Lewis <span class="hlt">icing</span> research tunnel to determine the aerodynamic and <span class="hlt">icing</span> characteristics of a full-scale induction-system air-scoop assembly incorporating a flush alternate inlet. The flush inlet was located immediately downstream of the offset ram inlet and included a 180 deg reversal and a 90 deg elbow in the ducting between inlet and carburetor top deck. The model also had a preheat-air inlet. The investigation was made over a range of <span class="hlt">mass</span>-air- flow ratios of 0 to 0.8, angles of attack of 0 and 4 deg airspeeds of 150 to 270 miles per hour, air temperatures of 0 and 25 F various liquid-water <span class="hlt">contents</span>, and droplet sizes. The ram inlet gave good pressure recovery in both clear air and <span class="hlt">icing</span> but rapid blockage of the top-deck screen occurred during <span class="hlt">icing</span>. The flush alternate inlet had poor pressure recovery in both clear air and <span class="hlt">icing</span>. The greatest decreases in the alternate-inlet pressure recovery were obtained at <span class="hlt">icing</span> conditions of low air temperature and high liquid-water <span class="hlt">content</span>. No serious screen <span class="hlt">icing</span> was observed with the alternate inlet. Pressure and temperature distributions on the carburetor top deck were determined using the preheat-air supply with the preheat- and alternate-inlet doors in various positions. No screen <span class="hlt">icing</span> occurred when the preheat-air system was operated in combination with alternate-inlet air flow.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.2064S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.2064S"><span>Using the glacial geomorphology of palaeo-<span class="hlt">ice</span> streams to understand mechanisms of <span class="hlt">ice</span> sheet collapse</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stokes, Chris R.; Margold, Martin; Clark, Chris; Tarasov, Lev</p> <p>2017-04-01</p> <p>Processes which bring about <span class="hlt">ice</span> sheet deglaciation are critical to our understanding of glacial-interglacial cycles and <span class="hlt">ice</span> sheet sensitivity to climate change. The precise mechanisms of deglaciation are also relevant to our understanding of modern-day <span class="hlt">ice</span> sheet stability and concerns over global sea level rise. <span class="hlt">Mass</span> loss from <span class="hlt">ice</span> sheets can be broadly partitioned between melting and a 'dynamic' component whereby rapidly-flowing <span class="hlt">ice</span> streams/outlet glaciers transfer <span class="hlt">ice</span> from the interior to the oceans. Surface and basal melting (e.g. of <span class="hlt">ice</span> shelves) are closely linked to atmospheric and oceanic conditions, but the mechanisms that drive dynamic changes in <span class="hlt">ice</span> stream discharge are more complex, which generates much larger uncertainties about their future contribution to <span class="hlt">ice</span> sheet <span class="hlt">mass</span> loss and sea level rise. A major problem is that observations of modern-day <span class="hlt">ice</span> streams typically span just a few decades and, at the <span class="hlt">ice</span>-sheet scale, it is unclear how the entire drainage network of <span class="hlt">ice</span> streams evolves during deglaciation. A key question is whether <span class="hlt">ice</span> streams might increase and sustain rates of <span class="hlt">mass</span> loss over centuries or millennia, beyond those expected for a given ocean-climate forcing. To address this issue, numerous workers have sought to understand <span class="hlt">ice</span> stream dynamics over longer time-scales using their glacial geomorphology in the palaeo-record. Indeed, our understanding of their geomorphology has grown rapidly in the last three decades, from almost complete ignorance to a detailed knowledge of their geomorphological products. Building on this body of work, this paper uses the glacial geomorphology of 117 <span class="hlt">ice</span> streams in the North American Laurentide <span class="hlt">Ice</span> Sheet to reconstruct their activity during its deglaciation ( 22,000 to 7,000 years ago). <span class="hlt">Ice</span> stream activity was characterised by high variability in both time and space, with <span class="hlt">ice</span> streams switching on and off in different locations. During deglaciation, we find that their overall number decreased, they occupied a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1258751-developing-bounding-ice-particle-mass-area-dimension-expressions-use-atmospheric-models-remote-sensing','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1258751-developing-bounding-ice-particle-mass-area-dimension-expressions-use-atmospheric-models-remote-sensing"><span>Developing and bounding <span class="hlt">ice</span> particle <span class="hlt">mass</span>- and area-dimension expressions for use in atmospheric models and remote sensing</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Erfani, Ehsan; Mitchell, David L.</p> <p>2016-04-07</p> <p>Here, <span class="hlt">ice</span> particle <span class="hlt">mass</span>- and projected area-dimension ( m- D and A- D) power laws are commonly used in the treatment of <span class="hlt">ice</span> cloud microphysical and optical properties and the remote sensing of <span class="hlt">ice</span> cloud properties. Although there has long been evidence that a single m- D or A- D power law is often not valid over all <span class="hlt">ice</span> particle sizes, few studies have addressed this fact. This study develops self-consistent m- D and A- D expressions that are not power laws but can easily be reduced to power laws for the <span class="hlt">ice</span> particle size (maximum dimension or D) rangemore » of interest, and they are valid over a much larger D range than power laws. This was done by combining ground measurements of individual <span class="hlt">ice</span> particle m and D formed at temperature T < –20 °C during a cloud seeding field campaign with 2-D stereo (2D-S) and cloud particle imager (CPI) probe measurements of D and A, and estimates of m, in synoptic and anvil <span class="hlt">ice</span> clouds at similar temperatures. The resulting m- D and A- D expressions are functions of temperature and cloud type (synoptic vs. anvil), and are in good agreement with m- D power laws developed from recent field studies considering the same temperature range (–60 °C < T < –20 °C).« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140001067','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140001067"><span>Correlation among Cirrus <span class="hlt">Ice</span> <span class="hlt">Content</span>, Water Vapor and Temperature in the TTL as Observed by CALIPSO and Aura-MLS</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Flury, T.; Wu, D. L.; Read, W. G.</p> <p>2012-01-01</p> <p>Water vapor in the tropical tropopause layer (TTL) has a local radiative cooling effect. As a source for <span class="hlt">ice</span> in cirrus clouds, however, it can also indirectly produce infrared heating. Using NASA A-Train satellite measurements of CALIPSO and Aura/MLS we calculated the correlation of water vapor, <span class="hlt">ice</span> water <span class="hlt">content</span> and temperature in the TTL. We find that temperature strongly controls water vapor (correlation r =0.94) and cirrus clouds at 100 hPa (r = -0.91). Moreover we observe that the cirrus seasonal cycle is highly (r =-0.9) anticorrelated with the water vapor variation in the TTL, showing higher cloud occurrence during December-January-February. We further investigate the anticorrelation on a regional scale and find that the strong anticorrelation occurs generally in the ITCZ (Intertropical Convergence Zone). The seasonal cycle of the cirrus <span class="hlt">ice</span> water <span class="hlt">content</span> is also highly anticorrelated to water vapor (r = -0.91) and our results support the hypothesis that the total water at 100 hPa is roughly constant. Temperature acts as a main regulator for balancing the partition between water vapor and cirrus clouds. Thus, to a large extent, the depleting water vapor in the TTL during DJF is a manifestation of cirrus formation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010TCD.....4.1525M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010TCD.....4.1525M"><span>First investigations of an <span class="hlt">ice</span> core from Eisriesenwelt cave (Austria)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>May, B.; Spötl, C.; Wagenbach, D.; Dublyansky, Y.; Liebl, J.</p> <p>2010-09-01</p> <p>Investigations into the genesis and dynamical properties of cave <span class="hlt">ice</span> are essential for assessing the climate significance of these underground glaciers. We drilled an <span class="hlt">ice</span> core through a 7.1 m thick <span class="hlt">ice</span> body filling a large cavern of the dynamic <span class="hlt">ice</span> cave Eisenriesenwelt (Austria). In addition to visual core inspections, quasi-continuous measurements at 2 cm resolution comprised particulate matter, stable water isotope (δ18O, δD) and electrolytic conductivity profiles supplemented by specifically selected samples analysed for tritium and radiocarbon. We found that recent ablation led to an almost complete loss of bomb derived tritium removing any <span class="hlt">ice</span> accumulated, since at least, the early fifties leaving the actual <span class="hlt">ice</span> surface even below the natural tritium level. The small particulate organic <span class="hlt">masses</span> made radiocarbon dating inconclusive, though a crude estimate gave a maximum <span class="hlt">ice</span> age in the order of several thousand years. The visual stratigraphy and all investigated parameters showed a clear dichotomy between the upper 4 m and the bottom 3 m of the core, which points to a substantial change in the <span class="hlt">ice</span> formation process. Main features of the core comprise the changing appearance and composition of distinct cyro-calcite layers, a extremely low total ion <span class="hlt">content</span> and a surprisingly high variability of the isotope signature. Co-isotope evaluation (δD versus δ18O) of the core in comparison with data from precipitation and karst spring water clearly indicate that <span class="hlt">ice</span> formation is governed by (slow) freezing of dripping water.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011TCry....5...81M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011TCry....5...81M"><span>First investigations of an <span class="hlt">ice</span> core from Eisriesenwelt cave (Austria)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>May, B.; Spötl, C.; Wagenbach, D.; Dublyansky, Y.; Liebl, J.</p> <p>2011-02-01</p> <p>Investigations into the genesis and dynamical properties of cave <span class="hlt">ice</span> are essential for assessing the climate significance of these underground glaciers. We drilled an <span class="hlt">ice</span> core through a 7.1 m-thick <span class="hlt">ice</span> body filling a large cavern of the dynamic <span class="hlt">ice</span> cave Eisenriesenwelt (Austria). In addition to visual core inspections, quasi-continuous measurements at 2 cm resolution comprised particulate matter, stable water isotope (δ18O, δD) and electrolytic conductivity profiles supplemented by specifically selected samples analyzed for tritium and radiocarbon. We found that recent ablation led to an almost complete loss of bomb-derived tritium removing any <span class="hlt">ice</span> accumulated since, at least, the early fifties leaving the actual <span class="hlt">ice</span> surface even below the natural tritium level. The small particulate organic <span class="hlt">masses</span> rendered radiocarbon dating inconclusive, though a crude estimate gave a basal <span class="hlt">ice</span> age in the order of several thousand years. The visual stratigraphy and all investigated parameters showed a clear dichotomy between the upper 2 m and the bottom 3 m of the core, which points to a substantial change in the <span class="hlt">ice</span> formation process. Main features of the core comprise the changing appearance and composition of distinct cryocalcite layers, extremely low total ion <span class="hlt">content</span> and a surprisingly high variability of the isotope signature. Co-isotope evaluation (δD versus δ18O) of the core in comparison with data from precipitation and karst spring water clearly indicate that <span class="hlt">ice</span> formation is governed by (slow) freezing of dripping water.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_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/2009EGUGA..11.2773E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..11.2773E"><span>Combined seismic and radar investigation to define <span class="hlt">ice</span> properties and structure of a cold alpine site</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Eisen, O.; Bohleber, P.; Drews, R.; Heilig, A.; Hofstede, C.</p> <p>2009-04-01</p> <p>The cold alpine saddle Colle Gnifetti, Monte Rosa, Swiss-Italian Alps resembles very much polar and subpolar <span class="hlt">ice</span> <span class="hlt">masses</span> in terms of glaciological conditions. It has been the site for several <span class="hlt">ice</span>-core drilling campaigns over more than 20 years to determine paleoclimatological and glaciological conditions. To investigate the feasibility of geophysical methods for improved characterization of <span class="hlt">ice</span> <span class="hlt">masses</span> surrounding borehole and <span class="hlt">ice</span>-core sites, a combined active reflection seismic and ground-penetrating radar pilot study has been carried out in summer 2008. Aims are the characterization of density, internal layering, seismic and radar wave speed and attenuation, identification of anisotropic features (like crystal orientation or bubble <span class="hlt">content</span> and shape). Here we present the overall setup and first results. Seismic and GPR profiles were centered on an existing borehole location covering the full <span class="hlt">ice</span> thickness of 62 m. Active seismics was carried out with 24-channel 3-m spacing recording, using a Seismic Impulse Source System (SISSY) along two profiles parallel and perpendicular to the <span class="hlt">ice</span>-flow direction. The same profiles were complemented with GPR measurements utilizing 250, 500 MHz frequencies. Additionally, circular profiles with 250, 500 and 800 MHz were carried out circumferencing the borehole to detect anisotropic features.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008E%26PSL.265..246N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008E%26PSL.265..246N"><span>Conditions for a steady <span class="hlt">ice</span> sheet <span class="hlt">ice</span> shelf junction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nowicki, S. M. J.; Wingham, D. J.</p> <p>2008-01-01</p> <p>This paper investigates the conditions under which a marine <span class="hlt">ice</span> sheet may adopt a steady profile. The <span class="hlt">ice</span> is treated as a linear viscous fluid caused to flow from a rigid base to and over water, treated as a denser but inviscid fluid. The solutions in the region around the point of flotation, or 'transition' zone, are calculated numerically. In-flow and out-flow conditions appropriate to <span class="hlt">ice</span> sheet and <span class="hlt">ice</span> shelf flow are applied at the ends of the transition zone and the rigid base is specified; the flow and steady free surfaces are determined as part of the solutions. The basal stress upstream, and the basal deflection downstream, of the flotation point are examined to determine which of these steady solutions satisfy 'contact' conditions that would prevent (i) the steady downstream basal deflection contacting the downstream base, and (ii) the upstream <span class="hlt">ice</span> commencing to float in the event it was melted at the base. In the case that the upstream bed is allowed to slide, we find only one <span class="hlt">mass</span> flux that satisfies the contact conditions. When no sliding is allowed at the bed, however, we find a range of <span class="hlt">mass</span> fluxes satisfy the contact conditions. The effect of 'backpressure' on the solutions is investigated, and is found to have no affect on the qualitative behaviour of the junctions. To the extent that the numerical, linearly viscous treatment may be applied to the case of <span class="hlt">ice</span> flowing out over the ocean, we conclude that when sliding is present, Weertman's 'instability' hypothesis holds.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.9455M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.9455M"><span>Submesoscale Sea <span class="hlt">Ice</span>-Ocean Interactions in Marginal <span class="hlt">Ice</span> Zones</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Manucharyan, Georgy E.; Thompson, Andrew F.</p> <p>2017-12-01</p> <p>Signatures of ocean eddies, fronts, and filaments are commonly observed within marginal <span class="hlt">ice</span> zones (MIZs) from satellite images of sea <span class="hlt">ice</span> concentration, and in situ observations via <span class="hlt">ice</span>-tethered profilers or underice gliders. However, localized and intermittent sea <span class="hlt">ice</span> heating and advection by ocean eddies are currently not accounted for in climate models and may contribute to their biases and errors in sea <span class="hlt">ice</span> forecasts. Here, we explore mechanical sea <span class="hlt">ice</span> interactions with underlying submesoscale ocean turbulence. We demonstrate that the release of potential energy stored in meltwater fronts can lead to energetic submesoscale motions along MIZs with spatial scales O(10 km) and Rossby numbers O(1). In low-wind conditions, cyclonic eddies and filaments efficiently trap the sea <span class="hlt">ice</span> and advect it over warmer surface ocean waters where it can effectively melt. The horizontal eddy diffusivity of sea <span class="hlt">ice</span> <span class="hlt">mass</span> and heat across the MIZ can reach O(200 m2 s-1). Submesoscale ocean variability also induces large vertical velocities (order 10 m d-1) that can bring relatively warm subsurface waters into the mixed layer. The ocean-sea <span class="hlt">ice</span> heat fluxes are localized over cyclonic eddies and filaments reaching about 100 W m-2. We speculate that these submesoscale-driven intermittent fluxes of heat and sea <span class="hlt">ice</span> can contribute to the seasonal evolution of MIZs. With the continuing global warming and sea <span class="hlt">ice</span> thickness reduction in the Arctic Ocean, submesoscale sea <span class="hlt">ice</span>-ocean processes are expected to become increasingly prominent.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C41E0718L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C41E0718L"><span>Firn Thickness Changes (1982-2015) Driven by SMB from MERRA-2, RACMO2.3, ERA-Int and AVHRR Surface Temperature and the Impacts to Greenland <span class="hlt">Ice</span> Sheet <span class="hlt">Mass</span> Balance</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, J.; Medley, B.; Neumann, T.; Smith, B. E.; Luthcke, S. B.; Zwally, H. J.</p> <p>2016-12-01</p> <p>Surface <span class="hlt">mass</span> balance (SMB) data are essential in the derivation of <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balance. This is because <span class="hlt">ice</span> sheet <span class="hlt">mass</span> change consists of short-term and long-term variations. The short-term variations are directly given by the SMB data. For altimetry based <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balance studies, these short-term <span class="hlt">mass</span> changes are converted to firn thickness changes by using a firn densification-elevation model, and then the variations are subtracted from the altimetry measurements to give the long-term <span class="hlt">ice</span> thickness changes that are associated with the density of <span class="hlt">ice</span>. So far various SMB data sets such as ERA-Interim, RACMO and MERRA are available and some have been widely used in large number of <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balance studies. However theses data sets exhibit the clear discrepancies in both random and systematic manner. In this study, we use our time dependent firn densification- elevation model, driven by the SMB data from MERRA-2, RACMO2.3 and ERA-Int for the period of 1982-2015 and the temperature variations from AVHRR for the same period to examine the corresponding firn thickness variations and the impacts to the <span class="hlt">mass</span> changes over the Greenland <span class="hlt">ice</span> sheet. The model was initialized with the1980's climate. Our results show that the relative smaller (centimeter level) differences in the firn thickness driven by the different data set occur at the early stage (1980's) of the model run. As the time progressing, the discrepancies between the SMB data sets accumulate, and the corresponding firn thickness differences quickly become larger with the value > 2m at the end of the period. Although the overall rates for the whole period driven by each of the three data sets are small ranging -0.2 - 0.2 cm a-1 (-3.0-2.7 Gt a-1), the decadal rates can vary greatly with magnitude > 3 cm a-1 and the impact to the Greenland <span class="hlt">mass</span> change exceeds 30 Gt a-1.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19950012869','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19950012869"><span>Methods for Scaling <span class="hlt">Icing</span> Test Conditions</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Anderson, David N.</p> <p>1995-01-01</p> <p>This report presents the results of tests at NASA Lewis to evaluate several methods to establish suitable alternative test conditions when the test facility limits the model size or operating conditions. The first method was proposed by Olsen. It can be applied when full-size models are tested and all the desired test conditions except liquid-water <span class="hlt">content</span> can be obtained in the facility. The other two methods discussed are: a modification of the French scaling law and the AEDC scaling method. <span class="hlt">Icing</span> tests were made with cylinders at both reference and scaled conditions representing mixed and glaze <span class="hlt">ice</span> in the NASA Lewis <span class="hlt">Icing</span> Research Tunnel. Reference and scale <span class="hlt">ice</span> shapes were compared to evaluate each method. The Olsen method was tested with liquid-water <span class="hlt">content</span> varying from 1.3 to .8 g/m(exp3). Over this range, <span class="hlt">ice</span> shapes produced using the Olsen method were unchanged. The modified French and AEDC methods produced scaled <span class="hlt">ice</span> shapes which approximated the reference shapes when model size was reduced to half the reference size for the glaze-<span class="hlt">ice</span> cases tested.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.7451H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.7451H"><span>Organic components in hair-<span class="hlt">ice</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hofmann, Diana; Steffen, Bernhard; Disko, Ulrich; Wagner, Gerhard; Mätzler, Christian</p> <p>2013-04-01</p> <p>Hair-<span class="hlt">ice</span> is a rather unknown phenomenon. In contrast to generally known frost needles, originating from atmospheric water and expanding e.g. from plant surfaces in all directions, hair <span class="hlt">ice</span> grows from the basis of wet, rotten hardwood. The hair-like, flexible, linear structures may reach up to 10 cm in length without any ramifications. Hair-<span class="hlt">ice</span> appears to be related to the biological activity of a fungus mycelium within the wood. Hair-<span class="hlt">ice</span> can attract winter-active Collemboles (snow flea, Isotoma nivalis). At the onset of hair-<span class="hlt">ice</span> melt a very thin fibre becomes apparent, which carries brownish pearl-like water drops. Therefore, it is supposed that organic substances are inherent, which could possibly act as freezing catalyst as well as recrystallization inhibitor. The aim of this work was the chemical characterization of organic substances contained in hair-<span class="hlt">ice</span>. First analyses of melted hair-<span class="hlt">ice</span> show a total organic carbon (TOC) value of 235 mg/l in contrast to 11 mg/l total nitrogen. Most of inherent nitrogen (70 %) exists thereby as ammonium. Screened by different (<span class="hlt">mass</span> spectrometric) methods, no evidence could be found for the initially expected organic substances like proteins, lipids, small volatile substances or carboxylic acids. By coupling of Ultra Performance Liquid Chromatography with a triple quadrupol <span class="hlt">mass</span> spectrometer (UPLC-MS) a non-resolved chromatogram from a melted hair-<span class="hlt">ice</span> sample was received. Averaged spectra from different regions are similar among themselves with a broad peak spreading over the <span class="hlt">mass</span> range 100-650 Da with favored intense, odd-numbered peaks. Such spectra are similar to dissolved organic matter (DOM), known e.g. from terrestrial and marine waters, soil extracts or aerosols. In the next step, samples were desalted and concentrated by solid phase extraction (SPE) and subsequently analyzed by flow injection analysis (FIA) in a Fourier Transform Ion Cyclotron Resonance <span class="hlt">Mass</span> Spectrometer (FTICR-MS), equipped with an ESI source and a 7 T</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C23C..03S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C23C..03S"><span>Surface water hydrology and the Greenland <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Smith, L. C.; Yang, K.; Pitcher, L. H.; Overstreet, B. T.; Chu, V. W.; Rennermalm, A. K.; Cooper, M. G.; Gleason, C. J.; Ryan, J.; Hubbard, A.; Tedesco, M.; Behar, A.</p> <p>2016-12-01</p> <p><span class="hlt">Mass</span> loss from the Greenland <span class="hlt">Ice</span> Sheet now exceeds 260 Gt/year, raising global sea level by >0.7 mm annually. Approximately two-thirds of this total <span class="hlt">mass</span> loss is now driven by negative <span class="hlt">ice</span> sheet surface <span class="hlt">mass</span> balance (SMB), attributed mainly to production and runoff of meltwater from the <span class="hlt">ice</span> sheet surface. This new dominance of runoff as a driver of GrIS total <span class="hlt">mass</span> loss will likely persist owing to anticipated further increases in surface melting, reduced meltwater storage in firn, and the waning importance of dynamical <span class="hlt">mass</span> losses (<span class="hlt">ice</span> calving) as the <span class="hlt">ice</span> sheets retreat from their marine-terminating margins. It also creates the need and opportunity for integrative research pairing traditional surface water hydrology approaches with glaciology. As one example, we present a way to measure supraglacial "runoff" (i.e. specific discharge) at the supraglacial catchment scale ( 101-102 km2), using in situ measurements of supraglacial river discharge and high-resolution satellite/drone mapping of upstream catchment area. This approach, which is standard in terrestrial hydrology but novel for <span class="hlt">ice</span> sheet science, enables independent verification and improvement of modeled SMB runoff estimates used to project sea level rise. Furthermore, because current SMB models do not consider the role of fluvial watershed processes operating on the <span class="hlt">ice</span> surface, inclusion of even a simple surface routing model materially improves simulations of runoff delivered to moulins, the critical pathways for meltwater entry into the <span class="hlt">ice</span> sheet. Incorporating principles of surface water hydrology and fluvial geomorphology and into glaciological models will thus aid estimates of Greenland meltwater runoff to the global ocean as well as connections to subglacial hydrology and <span class="hlt">ice</span> sheet dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ApJ...839...82N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ApJ...839...82N"><span>Development of a Full <span class="hlt">Ice</span>-cream Cone Model for Halo Coronal <span class="hlt">Mass</span> Ejections</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Na, Hyeonock; Moon, Y.-J.; Lee, Harim</p> <p>2017-04-01</p> <p>It is essential to determine three-dimensional parameters (e.g., radial speed, angular width, and source location) of coronal <span class="hlt">mass</span> ejections (CMEs) for the space weather forecast. In this study, we investigate which cone type represents a halo CME morphology using 29 CMEs (12 Solar and Heliospheric Observatory (SOHO)/Large Angle and Spectrometric Coronagraph (LASCO) halo CMEs and 17 Solar Terrestrial Relations Observatory (STEREO)/Sun-Earth Connection Coronal and Heliospheric Investigation COR2 halo CMEs) from 2010 December to 2011 June. These CMEs are identified as halo CMEs by one spacecraft (SOHO or one of STEREO A and B) and limb ones by the other spacecraft (One of STEREO A and B or SOHO). From cone shape parameters of these CMEs, such as their front curvature, we find that the CME observational structures are much closer to a full <span class="hlt">ice</span>-cream cone type than a shallow <span class="hlt">ice</span>-cream cone type. Thus, we develop a full <span class="hlt">ice</span>-cream cone model based on a new methodology that the full <span class="hlt">ice</span>-cream cone consists of many flat cones with different heights and angular widths to estimate the three-dimensional parameters of the halo CMEs. This model is constructed by carrying out the following steps: (1) construct a cone for a given height and angular width, (2) project the cone onto the sky plane, (3) select points comprising the outer boundary, and (4) minimize the difference between the estimated projection speeds with the observed ones. By applying this model to 12 SOHO/LASCO halo CMEs, we find that 3D parameters from our method are similar to those from other stereoscopic methods (I.e., a triangulation method and a Graduated Cylindrical Shell model).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C21E1165W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C21E1165W"><span>A Detailed Geophysical Investigation of the Grounding of Henry <span class="hlt">Ice</span> Rise, with Implications for Holocene <span class="hlt">Ice</span>-Sheet Extent.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wearing, M.; Kingslake, J.</p> <p>2017-12-01</p> <p>It is generally assumed that since the Last Glacial Maximum the West Antarctic <span class="hlt">Ice</span> Sheet (WAIS) has experienced monotonic retreat of the grounding line (GL). However, recent studies have cast doubt on this assumption, suggesting that the retreat of the WAIS grounding line may have been followed by a significant advance during the Holocene in the Weddell and Ross Sea sectors. Constraining this evolution is important as reconstructions of past <span class="hlt">ice</span>-sheet extent are used to spin-up predictive <span class="hlt">ice</span>-sheet models and correct <span class="hlt">mass</span>-balance observations for glacial isostatic adjustment. Here we examine in detail the formation of the Henry <span class="hlt">Ice</span> Rise (HIR), which <span class="hlt">ice</span>-sheet model simulations suggest played a key role in Holocene <span class="hlt">ice-mass</span> changes in the Weddell Sea sector. Observations from a high-resolution ground-based, <span class="hlt">ice</span>-penetrating radar survey are best explained if the <span class="hlt">ice</span> rise formed when the Ronne <span class="hlt">Ice</span> Shelf grounded on a submarine high, underwent a period of <span class="hlt">ice</span>-rumple flow, before the GL migrated outwards to form the present-day <span class="hlt">ice</span> rise. We constrain the relative chronology of this evolution by comparing the alignment and intersection of isochronal internal layers, relic crevasses, surface features and investigating the dynamic processes leading to their complex structure. We also draw analogies between HIR and the neighbouring Doake <span class="hlt">Ice</span> Rumples. The date of formation is estimated using vertical velocities derived with a phase-sensitive radio-echo sounder (pRES). <span class="hlt">Ice</span>-sheet models suggest that the formation of the HIR and other <span class="hlt">ice</span> rises may have halted and reversed large-scale GL retreat. Hence the small-scale dynamics of these crucial regions could have wide-reaching consequences for future <span class="hlt">ice</span>-sheet <span class="hlt">mass</span> changes and constraining their formation and evolution further would be beneficial. One stringent test of our geophysics-based conclusions would be to drill to the bed of HIR to sample the <span class="hlt">ice</span> for isotopic analysis and the bed for radiocarbon analysis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19860049995&hterms=uranium&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Duranium','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19860049995&hterms=uranium&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Duranium"><span>Uranium series dating of Allan Hills <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>Fireman, E. L.</p> <p>1986-01-01</p> <p>Uranium-238 decay series nuclides dissolved in Antarctic <span class="hlt">ice</span> samples were measured in areas of both high and low concentrations of volcanic glass shards. <span class="hlt">Ice</span> from the Allan Hills site (high shard <span class="hlt">content</span>) had high Ra-226, Th-230 and U-234 activities but similarly low U-238 activities in comparison with Antarctic <span class="hlt">ice</span> samples without shards. The Ra-226, Th-230 and U-234 excesses were found to be proportional to the shard <span class="hlt">content</span>, while the U-238 decay series results were consistent with the assumption that alpha decay products recoiled into the <span class="hlt">ice</span> from the shards. Through this method of uranium series dating, it was learned that the Allen Hills Cul de Sac <span class="hlt">ice</span> is approximately 325,000 years old.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=61546&keyword=high+AND+mountain+AND+ecosystems&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=61546&keyword=high+AND+mountain+AND+ecosystems&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>ION COMPOSITION ELUCIDATION (<span class="hlt">ICE</span>)</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p><br><br>Ion Composition Elucidation (<span class="hlt">ICE</span>) utilizes selected ion recording with a double focusing <span class="hlt">mass</span> spectrometer to simultaneously determine exact <span class="hlt">masses</span> and relative isotopic abundances from <span class="hlt">mass</span> peak profiles. These can be determined more accurately and at higher sensitivity ...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C31D..06T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C31D..06T"><span>Submesoscale sea <span class="hlt">ice</span>-ocean interactions in marginal <span class="hlt">ice</span> zones</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thompson, A. F.; Manucharyan, G.</p> <p>2017-12-01</p> <p>Signatures of ocean eddies, fronts and filaments are commonly observed within the marginal <span class="hlt">ice</span> zones (MIZ) from satellite images of sea <span class="hlt">ice</span> concentration, in situ observations via <span class="hlt">ice</span>-tethered profilers or under-<span class="hlt">ice</span> gliders. Localized and intermittent sea <span class="hlt">ice</span> heating and advection by ocean eddies are currently not accounted for in climate models and may contribute to their biases and errors in sea <span class="hlt">ice</span> forecasts. Here, we explore mechanical sea <span class="hlt">ice</span> interactions with underlying submesoscale ocean turbulence via a suite of numerical simulations. We demonstrate that the release of potential energy stored in meltwater fronts can lead to energetic submesoscale motions along MIZs with sizes O(10 km) and Rossby numbers O(1). In low-wind conditions, cyclonic eddies and filaments efficiently trap the sea <span class="hlt">ice</span> and advect it over warmer surface ocean waters where it can effectively melt. The horizontal eddy diffusivity of sea <span class="hlt">ice</span> <span class="hlt">mass</span> and heat across the MIZ can reach O(200 m2 s-1). Submesoscale ocean variability also induces large vertical velocities (order of 10 m day-1) that can bring relatively warm subsurface waters into the mixed layer. The ocean-sea <span class="hlt">ice</span> heat fluxes are localized over cyclonic eddies and filaments reaching about 100 W m-2. We speculate that these submesoscale-driven intermittent fluxes of heat and sea <span class="hlt">ice</span> can potentially contribute to the seasonal evolution of MIZs. With continuing global warming and sea <span class="hlt">ice</span> thickness reduction in the Arctic Ocean, as well as the large expanse of thin sea <span class="hlt">ice</span> in the Southern Ocean, submesoscale sea <span class="hlt">ice</span>-ocean processes are expected to play a significant role in the climate system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMSH51B2010N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMSH51B2010N"><span>Comparison of Asymmetric and <span class="hlt">Ice</span>-cream Cone Models for Halo Coronal <span class="hlt">Mass</span> Ejections</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Na, H.; Moon, Y.</p> <p>2011-12-01</p> <p>Halo coronal <span class="hlt">mass</span> ejections (HCMEs) are major cause of the geomagnetic storms. To minimize the projection effect by coronagraph observation, several cone models have been suggested: an <span class="hlt">ice</span>-cream cone model, an asymmetric cone model etc. These models allow us to determine the three dimensional parameters of HCMEs such as radial speed, angular width, and the angle between sky plane and central axis of the cone. In this study, we compare these parameters obtained from different models using 48 well-observed HCMEs from 2001 to 2002. And we obtain the root mean square error (RMS error) between measured projection speeds and calculated projection speeds for both cone models. As a result, we find that the radial speeds obtained from the models are well correlated with each other (R = 0.86), and the correlation coefficient of angular width is 0.6. The correlation coefficient of the angle between sky plane and central axis of the cone is 0.31, which is much smaller than expected. The reason may be due to the fact that the source locations of the asymmetric cone model are distributed near the center, while those of the <span class="hlt">ice</span>-cream cone model are located in a wide range. The average RMS error of the asymmetric cone model (85.6km/s) is slightly smaller than that of the <span class="hlt">ice</span>-cream cone model (87.8km/s).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C13C0833S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C13C0833S"><span>Using ATM laser altimetry to constrain surface <span class="hlt">mass</span> balance estimates and supraglacial hydrology of the Greenland <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Studinger, M.; Medley, B.; Manizade, S.; Linkswiler, M. A.</p> <p>2016-12-01</p> <p>Repeat airborne laser altimetry measurements can provide large-scale field observations to better quantify spatial and temporal variability of surface processes contributing to seasonal elevation change and therefore surface <span class="hlt">mass</span> balance. As part of NASA's Operation <span class="hlt">Ice</span>Bridge the Airborne Topographic Mapper (ATM) laser altimeter measured the surface elevation of the Greenland <span class="hlt">Ice</span> Sheet during spring (March - May) and fall (September - October) of 2015. Comparison of the two surveys reveals a general trend of thinning for outlet glaciers and for the <span class="hlt">ice</span> sheet in a manner related to elevation and latitude. In contrast, some thickening is observed on the west (but not on the east) side of the <span class="hlt">ice</span> divide above 2200 m elevation in the southern half, below latitude 69°N.The observed magnitude and spatial patterns of the summer melt signal can be utilized as input into <span class="hlt">ice</span> sheet models and for validating reanalysis of regional climate models such as RACMO and MAR. We use seasonal anomalies in MERRA-2 climate fields (temperature, precipitation) to understand the observed spatial signal in seasonal change. Aside from surface elevation change, runoff from meltwater pooling in supraglacial lakes and meltwater channels accounts for at least half of the total <span class="hlt">mass</span> loss. The ability of the ATM laser altimeters to image glacial hydrological features in 3-D and determine the depth of supraglacial lakes could be used for process studies and for quantifying melt processes over large scales. The 1-meter footprint diameter of ATM laser on the surface, together with a high shot density, allows for the production of large-scale, high-resolution, geodetic quality DEMs (50 x 50 cm) suitable for fine-scale glacial hydrology research and as input to hydrological models quantifying runoff.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1255085-reactivation-kamb-ice-stream-tributaries-triggers-century-scale-reorganization-siple-coast-ice-flow-west-antarctica','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1255085-reactivation-kamb-ice-stream-tributaries-triggers-century-scale-reorganization-siple-coast-ice-flow-west-antarctica"><span>Reactivation of Kamb <span class="hlt">Ice</span> Stream tributaries triggers century-scale reorganization of Siple Coast <span class="hlt">ice</span> flow in West Antarctica</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Bougamont, M.; Christoffersen, P.; Price, S. F.; ...</p> <p>2015-10-21</p> <p>Ongoing, centennial-scale flow variability within the Ross <span class="hlt">ice</span> streams of West Antarctica suggests that the present-day positive <span class="hlt">mass</span> balance in this region may reverse in the future. Here we use a three-dimensional <span class="hlt">ice</span> sheet model to simulate <span class="hlt">ice</span> flow in this region over 250 years. The flow responds to changing basal properties, as a subglacial till layer interacts with water transported in an active subglacial hydrological system. We show that a persistent weak bed beneath the tributaries of the dormant Kamb <span class="hlt">Ice</span> Stream is a source of internal <span class="hlt">ice</span> flow instability, which reorganizes all <span class="hlt">ice</span> streams in this region, leadingmore » to a reduced (positive) <span class="hlt">mass</span> balance within decades and a net loss of <span class="hlt">ice</span> within two centuries. This hitherto unaccounted for flow variability could raise sea level by 5 mm this century. Furthermore, better constraints on future sea level change from this region will require improved estimates of geothermal heat flux and subglacial water transport.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29016475','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29016475"><span>Relationship between Physiological Off-<span class="hlt">Ice</span> Testing, On-<span class="hlt">Ice</span> Skating, and Game Performance in Division I Women's <span class="hlt">Ice</span> Hockey Players.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Boland, Michelle; Miele, Emily M; Delude, Katie</p> <p>2017-10-07</p> <p>The purpose was to identify off-<span class="hlt">ice</span> testing variables that correlate to skating and game performance in Division I collegiate women <span class="hlt">ice</span> hockey players. Twenty female, forward and defensive players (19.95 ± 1.35 yr) were assessed for weight, height, percent fat <span class="hlt">mass</span> (%FAT), bone mineral density, predicted one repetition maximum (RM) absolute and relative (REL%) bench press (BP) and hex bar deadlift (HDL), lower body explosive power, anaerobic power, countermovement vertical jump (CMJ), maximum inspiratory pressure (MIP), and on-<span class="hlt">ice</span> repeated skate sprint (RSS) performance. The on-<span class="hlt">ice</span> RSS test included 6 timed 85.6 m sprints with participants wearing full hockey equipment; fastest time (FT), average time (AT) and fatigue index (FI) for the first length skate (FLS; 10 m) and total length skate (TLS; 85.6 m) were used for analysis. Game performance was evaluated with game statistics: goals, assists, points, plus-minus, and shots on goal (SOG). Correlation coefficients were used to determine relationships. Percent fat <span class="hlt">mass</span> was positively correlated (p < 0.05) with FLS-FI and TLS-AT; TLS-FT was negatively correlated with REL%HDL; BP-RM was negatively correlated with FLS-FT and FLS-AT; MIP positively correlated with assists, points, and SOG; FLS-AT negatively correlated with assists. Game performance in women <span class="hlt">ice</span> hockey players may be enhanced by greater MIP, repeat acceleration ability, and mode-specific training. Faster skating times were associated with lower %FAT. Skating performance in women <span class="hlt">ice</span> hockey players may be enhanced by improving body composition, anaerobic power, and both lower and upper body strength in off-<span class="hlt">ice</span> training.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24037377','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24037377"><span>Calving fluxes and basal melt rates of Antarctic <span class="hlt">ice</span> shelves.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Depoorter, M A; Bamber, J L; Griggs, J A; Lenaerts, J T M; Ligtenberg, S R M; van den Broeke, M R; Moholdt, G</p> <p>2013-10-03</p> <p>Iceberg calving has been assumed to be the dominant cause of <span class="hlt">mass</span> loss for the Antarctic <span class="hlt">ice</span> sheet, with previous estimates of the calving flux exceeding 2,000 gigatonnes per year. More recently, the importance of melting by the ocean has been demonstrated close to the grounding line and near the calving front. So far, however, no study has reliably quantified the calving flux and the basal <span class="hlt">mass</span> balance (the balance between accretion and ablation at the <span class="hlt">ice</span>-shelf base) for the whole of Antarctica. The distribution of fresh water in the Southern Ocean and its partitioning between the liquid and solid phases is therefore poorly constrained. Here we estimate the <span class="hlt">mass</span> balance components for all <span class="hlt">ice</span> shelves in Antarctica, using satellite measurements of calving flux and grounding-line flux, modelled <span class="hlt">ice</span>-shelf snow accumulation rates and a regional scaling that accounts for unsurveyed areas. We obtain a total calving flux of 1,321 ± 144 gigatonnes per year and a total basal <span class="hlt">mass</span> balance of -1,454 ± 174 gigatonnes per year. This means that about half of the <span class="hlt">ice</span>-sheet surface <span class="hlt">mass</span> gain is lost through oceanic erosion before reaching the <span class="hlt">ice</span> front, and the calving flux is about 34 per cent less than previous estimates derived from iceberg tracking. In addition, the fraction of <span class="hlt">mass</span> loss due to basal processes varies from about 10 to 90 per cent between <span class="hlt">ice</span> shelves. We find a significant positive correlation between basal <span class="hlt">mass</span> loss and surface elevation change for <span class="hlt">ice</span> shelves experiencing surface lowering and enhanced discharge. We suggest that basal <span class="hlt">mass</span> loss is a valuable metric for predicting future <span class="hlt">ice</span>-shelf vulnerability to oceanic forcing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1915674M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1915674M"><span>The future of the Devon <span class="hlt">Ice</span> cap: results from climate and <span class="hlt">ice</span> dynamics modelling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mottram, Ruth; Rodehacke, Christian; Boberg, Fredrik</p> <p>2017-04-01</p> <p>The Devon <span class="hlt">Ice</span> Cap is an example of a relatively well monitored small <span class="hlt">ice</span> cap in the Canadian Arctic. Close to Greenland, it shows a similar surface <span class="hlt">mass</span> balance signal to glaciers in western Greenland. Here we use high resolution (5km) simulations from HIRHAM5 to drive the PISM glacier model in order to model the present day and future prospects of this small Arctic <span class="hlt">ice</span> cap. Observational data from the Devon <span class="hlt">Ice</span> Cap in Arctic Canada is used to evaluate the surface <span class="hlt">mass</span> balance (SMB) data output from the HIRHAM5 model for simulations forced with the ERA-Interim climate reanalysis data and the historical emissions scenario run by the EC-Earth global climate model. The RCP8.5 scenario simulated by EC-Earth is also downscaled by HIRHAM5 and this output is used to force the PISM model to simulate the likely future evolution of the Devon <span class="hlt">Ice</span> Cap under a warming climate. We find that the Devon <span class="hlt">Ice</span> Cap is likely to continue its present day retreat, though in the future increased precipitation partly offsets the enhanced melt rates caused by climate change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70168468','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70168468"><span>Do digestive <span class="hlt">contents</span> confound body <span class="hlt">mass</span> as a measure of relative condition in nestling songbirds?</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Streby, Henry M.; Peterson, Sean M.; Lehman, Justin A.; Kramer, Gunnar R.; Vernasco, Ben J.; Andersen, David E.</p> <p>2014-01-01</p> <p>Relative nestling condition, typically measured as nestling <span class="hlt">mass</span> or as an index including nestling <span class="hlt">mass</span>, is commonly purported to correlate with fledgling songbird survival. However, most studies directly investigating fledgling survival have found no such relationship. We weighed feces and stomach <span class="hlt">contents</span> of nestling golden-winged warblers (Vermivora chrysoptera) to investigate the potential contribution of variation in digestive <span class="hlt">contents</span> to differences in nestling <span class="hlt">mass</span>. We estimated that the <span class="hlt">mass</span> of a seventh-day (near fledging) nestling golden-winged warbler varies by 0.65 g (approx. 9% of mean nestling <span class="hlt">mass</span>) depending on the <span class="hlt">contents</span> of the nestling's digestive system at the time of weighing, and that digestive <span class="hlt">contents</span> are dissimilar among nestlings at any moment the brood is removed from the nest for weighing. Our conservative estimate of within-individual variation in digestive <span class="hlt">contents</span> equals 72% and 24% of the mean within-brood and population-wide range in nestling <span class="hlt">mass</span>, respectively. Based on our results, a substantive but typically unknown amount of the variation in body <span class="hlt">mass</span> among nestlings is confounded by differences in digestive <span class="hlt">contents</span>. We conclude that short-term variation in digestive <span class="hlt">contents</span> likely precludes the use of body <span class="hlt">mass</span>, and therefore any <span class="hlt">mass</span>-dependent index, as a measure of relative nestling condition or as a predictor of survival in golden-winged warblers and likely in many other songbirds of similar size.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16782607','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16782607"><span><span class="hlt">Ice</span>-sheet contributions to future sea-level change.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gregory, J M; Huybrechts, P</p> <p>2006-07-15</p> <p>Accurate simulation of <span class="hlt">ice</span>-sheet surface <span class="hlt">mass</span> balance requires higher spatial resolution than is afforded by typical atmosphere-ocean general circulation models (AOGCMs), owing, in particular, to the need to resolve the narrow and steep margins where the majority of precipitation and ablation occurs. We have developed a method for calculating <span class="hlt">mass</span>-balance changes by combining <span class="hlt">ice</span>-sheet average time-series from AOGCM projections for future centuries, both with information from high-resolution climate models run for short periods and with a 20km <span class="hlt">ice</span>-sheet <span class="hlt">mass</span>-balance model. Antarctica contributes negatively to sea level on account of increased accumulation, while Greenland contributes positively because ablation increases more rapidly. The uncertainty in the results is about 20% for Antarctica and 35% for Greenland. Changes in <span class="hlt">ice</span>-sheet topography and dynamics are not included, but we discuss their possible effects. For an annual- and area-average warming exceeding 4.5+/-0.9K in Greenland and 3.1+/-0.8K in the global average, the net surface <span class="hlt">mass</span> balance of the Greenland <span class="hlt">ice</span> sheet becomes negative, in which case it is likely that the <span class="hlt">ice</span> sheet would eventually be eliminated, raising global-average sea level by 7m.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_15 --> <div id="page_16" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="301"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018RvGeo..56..142P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018RvGeo..56..142P"><span>Ocean Tide Influences on the Antarctic and Greenland <span class="hlt">Ice</span> Sheets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Padman, Laurie; Siegfried, Matthew R.; Fricker, Helen A.</p> <p>2018-03-01</p> <p>Ocean tides are the main source of high-frequency variability in the vertical and horizontal motion of <span class="hlt">ice</span> sheets near their marine margins. Floating <span class="hlt">ice</span> shelves, which occupy about three quarters of the perimeter of Antarctica and the termini of four outlet glaciers in northern Greenland, rise and fall in synchrony with the ocean tide. Lateral motion of floating and grounded portions of <span class="hlt">ice</span> sheets near their marine margins can also include a tidal component. These tide-induced signals provide insight into the processes by which the oceans can affect <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balance and dynamics. In this review, we summarize in situ and satellite-based measurements of the tidal response of <span class="hlt">ice</span> shelves and grounded <span class="hlt">ice</span>, and spatial variability of ocean tide heights and currents around the <span class="hlt">ice</span> sheets. We review sensitivity of tide heights and currents as ocean geometry responds to variations in sea level, <span class="hlt">ice</span> shelf thickness, and <span class="hlt">ice</span> sheet <span class="hlt">mass</span> and extent. We then describe coupled <span class="hlt">ice</span>-ocean models and analytical glacier models that quantify the effect of ocean tides on lower-frequency <span class="hlt">ice</span> sheet <span class="hlt">mass</span> loss and motion. We suggest new observations and model developments to improve the representation of tides in coupled models that are used to predict future <span class="hlt">ice</span> sheet <span class="hlt">mass</span> loss and the associated contribution to sea level change. The most critical need is for new data to improve maps of bathymetry, <span class="hlt">ice</span> shelf draft, spatial variability of the drag coefficient at the <span class="hlt">ice</span>-ocean interface, and higher-resolution models with improved representation of tidal energy sinks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C41E0713C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C41E0713C"><span>Evaluation of a 12-km Satellite-Era Reanalysis of Surface <span class="hlt">Mass</span> Balance for the Greenland <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cullather, R. I.; Nowicki, S.; Zhao, B.; Max, S.</p> <p>2016-12-01</p> <p>The recent contribution to sea level change from the Greenland <span class="hlt">Ice</span> Sheet is thought to be strongly driven by surface processes including melt and runoff. Global reanalyses are potential means of reconstructing the historical time series of <span class="hlt">ice</span> sheet surface <span class="hlt">mass</span> balance (SMB), but lack spatial resolution needed to resolve ablation areas along the periphery of the <span class="hlt">ice</span> sheet. In this work, the Modern-Era Retrospective analysis for Research and Applications, version 2 (MERRA-2) is used to examine the spatial and temporal variability of surface melt over the Greenland <span class="hlt">Ice</span> Sheet. MERRA-2 is produced for the period 1980 to the present at a grid spacing of ½° latitude by ⅝° longitude, and includes snow hydrology processes including compaction, meltwater percolation and refreezing, runoff, and a prognostic surface albedo. The configuration of the MERRA-2 system allows for the background model - the Goddard Earth Observing System model, version 5 (GEOS-5) - to be carried in phase space through analyzed states via the computation of analysis increments, a capability referred to as "replay". Here, a MERRA-2 replay integration is conducted in which atmospheric forcing fields are interpolated and adjusted to sub- atmospheric grid-scale resolution. These adjustments include lapse-rate effects on temperature, humidity, precipitation, and other atmospheric variables that are known to have a strong elevation dependency over <span class="hlt">ice</span> sheets. The surface coupling is performed such that <span class="hlt">mass</span> and energy are conserved. The atmospheric forcing influences the surface representation, which operates on land surface tiles with an approximate 12-km spacing. This produces a high-resolution, downscaled SMB which is interactively coupled to the reanalysis model. We compare the downscaled SMB product with other reanalyses, regional climate model values, and a second MERRA-2 replay in which the background model has been replaced with a 12-km, non-hydrostatic version of GEOS-5. The assessment</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRD..122.4944C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRD..122.4944C"><span>Information <span class="hlt">content</span> of visible and midinfrared radiances for retrieving tropical <span class="hlt">ice</span> cloud properties</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chang, Kai-Wei; L'Ecuyer, Tristan S.; Kahn, Brian H.; Natraj, Vijay</p> <p>2017-05-01</p> <p>Hyperspectral instruments such as Atmospheric Infrared Sounder (AIRS) have spectrally dense observations effective for <span class="hlt">ice</span> cloud retrievals. However, due to the large number of channels, only a small subset is typically used. It is crucial that this subset of channels be chosen to contain the maximum possible information about the retrieved variables. This study describes an information <span class="hlt">content</span> analysis designed to select optimal channels for <span class="hlt">ice</span> cloud retrievals. To account for variations in <span class="hlt">ice</span> cloud properties, we perform channel selection over an ensemble of cloud regimes, extracted with a clustering algorithm, from a multiyear database at a tropical Atmospheric Radiation Measurement site. Multiple satellite viewing angles over land and ocean surfaces are considered to simulate the variations in observation scenarios. The results suggest that AIRS channels near wavelengths of 14, 10.4, 4.2, and 3.8 μm contain the most information. With an eye toward developing a joint AIRS-MODIS (Moderate Resolution Imaging Spectroradiometer) retrieval, the analysis is also applied to combined measurements from both instruments. While application of this method to MODIS yields results consistent with previous channel sensitivity studies, the analysis shows that this combination may yield substantial improvement in cloud retrievals. MODIS provides most information on optical thickness and particle size, aided by a better constraint on cloud vertical placement from AIRS. An alternate scenario where cloud top boundaries are supplied by the active sensors in the A-train is also explored. The more robust cloud placement afforded by active sensors shifts the optimal channels toward the window region and shortwave infrared, further constraining optical thickness and particle size.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.C41C0417K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.C41C0417K"><span>Pleistocene <span class="hlt">ice</span>-rich yedoma in Interior Alaska</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kanevskiy, M. Z.; Shur, Y.; Jorgenson, T. T.; Sturm, M.; Bjella, K.; Bray, M.; Harden, J. W.; Dillon, M.; Fortier, D.; O'Donnell, J.</p> <p>2011-12-01</p> <p>Yedoma, or the <span class="hlt">ice</span>-rich syngenetic permafrost with large <span class="hlt">ice</span> wedges, widely occurs in parts of Alaska that were unglaciated during the last glaciation including Interior Alaska, Foothills of Brooks Range and Seward Peninsula. A thick layer of syngenetic permafrost was formed by simultaneous accumulation of silt and upward permafrost aggradation. Until recently, yedoma has been studied mainly in Russia. In Interior Alaska, we have studied yedoma at several field sites (Erickson Creek area, Boot Lake area, and several sites around Fairbanks, including well-known CRREL Permafrost tunnel). All these locations are characterized by thick sequences of <span class="hlt">ice</span>-rich silt with large <span class="hlt">ice</span> wedges up to 30 m deep. Our study in the CRREL Permafrost tunnel and surrounding area revealed a yedoma section up to 18 m thick, whose formation began about 40,000 yr BP. The volume of wedge-<span class="hlt">ice</span> (about 10-15%) is not very big in comparison with other yedoma sites (typically more than 30%), but soils between <span class="hlt">ice</span> wedges are extremely <span class="hlt">ice</span>-rich - an average value of gravimetric moisture <span class="hlt">content</span> of undisturbed yedoma silt with micro-cryostructures is about 130%. Numerous bodies of thermokarst-cave <span class="hlt">ice</span> were detected in the tunnel. Geotechnical investigations along the Dalton Highway near Livengood (Erickson Creek area) provided opportunities for studies of yedoma cores from deep boreholes. The radiocarbon age of sediments varies from 20,000 to 45,000 yr BP. Most of soils in the area are extremely <span class="hlt">ice</span>-rich. Thickness of <span class="hlt">ice</span>-rich silt varies from 10 m to more than 26 m, and volume of wedge-<span class="hlt">ice</span> reaches 35-45%. Soil between <span class="hlt">ice</span> wedges has mainly micro-cryostructures and average gravimetric moisture <span class="hlt">content</span> from 80% to 100%. Our studies have shown that the top part of yedoma in many locations was affected by deep thawing during the Holocene, which resulted in formation of the layer of thawed and refrozen soils up to 6 m thick on top of yedoma deposits. Thawing of the upper permafrost could be related to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20000074257&hterms=Antarctic+icebergs&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DAntarctic%2Bicebergs','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20000074257&hterms=Antarctic+icebergs&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DAntarctic%2Bicebergs"><span>Glacier and <span class="hlt">Ice</span> Shelves Studies Using Satellite SAR Interferometry</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rignot, Eric</p> <p>1999-01-01</p> <p>Satellite radar interferometry is a powerful technique to measure the surface velocity and topography of glacier <span class="hlt">ice</span>. On <span class="hlt">ice</span> shelves, a quadruple difference technique separates tidal motion from the steady creep flow deformation of <span class="hlt">ice</span>. The results provide a wealth of information about glacier grounding lines , <span class="hlt">mass</span> fluxes, stability, elastic properties of <span class="hlt">ice</span>, and tidal regime. The grounding line, which is where the glacier detaches from its bed and becomes afloat, is detected with a precision of a few tens of meters. Combining this information with satellite radar altimetry makes it possible to measure glacier discharge into the ocean and state of <span class="hlt">mass</span> balance with greater precision than ever before, and in turn provide a significant revision of past estimates of <span class="hlt">mass</span> balance of the Greenland and Antarctic <span class="hlt">Ice</span> Sheets. Analysis of creep rates on floating <span class="hlt">ice</span> permits an estimation of basal melting at the <span class="hlt">ice</span> shelf underside. The results reveal that the action of ocean water in sub-<span class="hlt">ice</span>-shelf cavities has been largely underestimated by oceanographic models and is the dominant mode of <span class="hlt">mass</span> release to the ocean from an <span class="hlt">ice</span> shelf. Precise mapping of grounding line positions also permits the detection of grounding line migration, which is a fine indicator of glacier change, independent of our knowledge of snow accumulation and <span class="hlt">ice</span> melting. This technique has been successfully used to detect the rapid retreat of Pine Island Glacier, the largest <span class="hlt">ice</span> stream in West Antarctica. Finally, tidal motion of <span class="hlt">ice</span> shelves measured interferometrically provides a modern, synoptic view of the physical processes which govern the formation of tabular icebergs in the Antarctic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.C51A0254Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.C51A0254Y"><span>Modelling the Climate - Greenland <span class="hlt">Ice</span> Sheet Interaction in the Coupled <span class="hlt">Ice</span>-sheet/Climate Model EC-EARTH - PISM</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, S.; Madsen, M. S.; Rodehacke, C. B.; Svendsen, S. H.; Adalgeirsdottir, G.</p> <p>2014-12-01</p> <p>Recent observations show that the Greenland <span class="hlt">ice</span> sheet (GrIS) has been losing <span class="hlt">mass</span> with an increasing speed during the past decades. Predicting the GrIS changes and their climate consequences relies on the understanding of the interaction of the GrIS with the climate system on both global and local scales, and requires climate model systems with an explicit and physically consistent <span class="hlt">ice</span> sheet module. A fully coupled global climate model with a dynamical <span class="hlt">ice</span> sheet model for the GrIS has recently been developed. The model system, EC-EARTH - PISM, consists of the EC-EARTH, an atmosphere, ocean and sea <span class="hlt">ice</span> model system, and the Parallel <span class="hlt">Ice</span> Sheet Model (PISM). The coupling of PISM includes a modified surface physical parameterization in EC-EARTH adapted to the land <span class="hlt">ice</span> surface over glaciated regions in Greenland. The PISM <span class="hlt">ice</span> sheet model is forced with the surface <span class="hlt">mass</span> balance (SMB) directly computed inside the EC-EARTH atmospheric module and accounting for the precipitation, the surface evaporation, and the melting of snow and <span class="hlt">ice</span> over land <span class="hlt">ice</span>. PISM returns the simulated basal melt, <span class="hlt">ice</span> discharge and <span class="hlt">ice</span> cover (extent and thickness) as boundary conditions to EC-EARTH. This coupled system is <span class="hlt">mass</span> and energy conserving without being constrained by any anomaly correction or flux adjustment, and hence is suitable for investigation of <span class="hlt">ice</span> sheet - climate feedbacks. Three multi-century experiments for warm climate scenarios under (1) the RCP85 climate forcing, (2) an abrupt 4xCO2 and (3) an idealized 1% per year CO2 increase are performed using the coupled model system. The experiments are compared with their counterparts of the standard CMIP5 simulations (without the interactive <span class="hlt">ice</span> sheet) to evaluate the performance of the coupled system and to quantify the GrIS feedbacks. In particular, the evolution of the Greenland <span class="hlt">ice</span> sheet under the warm climate and its impacts on the climate system are investigated. Freshwater fluxes from the Greenland <span class="hlt">ice</span> sheet melt to the Arctic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4881027','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4881027"><span>The decisive role of free water in determining homogenous <span class="hlt">ice</span> nucleation behavior of aqueous solutions</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Wang, Qiang; Zhao, Lishan; Li, Chenxi; Cao, Zexian</p> <p>2016-01-01</p> <p>It is a challenging issue to quantitatively characterize how the solute and pressure affect the homogeneous <span class="hlt">ice</span> nucleation in a supercooled solution. By measuring the glass transition behavior of solutions, a universal feature of water-<span class="hlt">content</span> dependence of glass transition temperature is recognized, which can be used to quantify hydration water in solutions. The amount of free water can then be determined for water-rich solutions, whose <span class="hlt">mass</span> fraction, Xf, is found to serve as a universal relevant parameter for characterizing the homogeneous <span class="hlt">ice</span> nucleation temperature, the meting temperature of primary <span class="hlt">ice</span>, and even the water activity of solutions of electrolytes and smaller organic molecules. Moreover, the effects of hydrated solute and pressure on <span class="hlt">ice</span> nucleation is comparable, and the pressure, when properly scaled, can be incorporated into the universal parameter Xf. These results help establish the decisive role of free water in determining <span class="hlt">ice</span> nucleation and other relevant properties of aqueous solutions. PMID:27225427</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12..761D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12..761D"><span>Compression experiments on artificial, alpine and marine <span class="hlt">ice</span>: implications for <span class="hlt">ice</span>-shelf/continental interactions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dierckx, Marie; Goossens, Thomas; Samyn, Denis; Tison, Jean-Louis</p> <p>2010-05-01</p> <p>Antarctic <span class="hlt">ice</span> shelves are important components of continental <span class="hlt">ice</span> dynamics, in that they control grounded <span class="hlt">ice</span> flow towards the ocean. As such, Antarctic <span class="hlt">ice</span> shelves are a key parameter to the stability of the Antarctic <span class="hlt">ice</span> sheet in the context of global change. Marine <span class="hlt">ice</span>, formed by sea water accretion beneath some <span class="hlt">ice</span> shelves, displays distinct physical (grain textures, bubble <span class="hlt">content</span>, ...) and chemical (salinity, isotopic composition, ...) characteristics as compared to glacier <span class="hlt">ice</span> and sea <span class="hlt">ice</span>. The aim is to refine Glen's flow relation (generally used for <span class="hlt">ice</span> behaviour in deformation) under various parameters (temperature, salinity, debris, grain size ...) to improve deformation laws used in dynamic <span class="hlt">ice</span> shelf models, which would then give more accurate and / or realistic predictions on <span class="hlt">ice</span> shelf stability. To better understand the mechanical properties of natural <span class="hlt">ice</span>, deformation experiments were performed on <span class="hlt">ice</span> samples in laboratory, using a pneumatic compression device. To do so, we developed a custom built compression rig operated by pneumatic drives. It has been designed for performing uniaxial compression tests at constant load and under unconfined conditions. The operating pressure ranges from about 0.5 to 10 Bars. This allows modifying the experimental conditions to match the conditions found at the grounding zone (in the 1 Bar range). To maintain the <span class="hlt">ice</span> at low temperature, the samples are immersed in a Silicone oil bath connected to an external refrigeration system. During the experiments, the vertical displacement of the piston and the applied force is measured by sensors which are connected to a digital acquisition system. We started our experiments with artificial <span class="hlt">ice</span> and went on with continental <span class="hlt">ice</span> samples from glaciers in the Alps. The first results allowed us to acquire realistic mechanical data for natural <span class="hlt">ice</span>. <span class="hlt">Ice</span> viscosity was calculated for different types of artificial <span class="hlt">ice</span>, using Glen's flow law, and showed the importance of impurities</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018TCry...12..811N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018TCry...12..811N"><span>Modelling the climate and surface <span class="hlt">mass</span> balance of polar <span class="hlt">ice</span> sheets using RACMO2 - Part 1: Greenland (1958-2016)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Noël, Brice; van de Berg, Willem Jan; Melchior van Wessem, J.; van Meijgaard, Erik; van As, Dirk; Lenaerts, Jan T. M.; Lhermitte, Stef; Kuipers Munneke, Peter; Smeets, C. J. P. Paul; van Ulft, Lambertus H.; van de Wal, Roderik S. W.; van den Broeke, Michiel R.</p> <p>2018-03-01</p> <p>We evaluate modelled Greenland <span class="hlt">ice</span> sheet (GrIS) near-surface climate, surface energy balance (SEB) and surface <span class="hlt">mass</span> balance (SMB) from the updated regional climate model RACMO2 (1958-2016). The new model version, referred to as RACMO2.3p2, incorporates updated glacier outlines, topography and <span class="hlt">ice</span> albedo fields. Parameters in the cloud scheme governing the conversion of cloud condensate into precipitation have been tuned to correct inland snowfall underestimation: snow properties are modified to reduce drifting snow and melt production in the <span class="hlt">ice</span> sheet percolation zone. The <span class="hlt">ice</span> albedo prescribed in the updated model is lower at the <span class="hlt">ice</span> sheet margins, increasing <span class="hlt">ice</span> melt locally. RACMO2.3p2 shows good agreement compared to in situ meteorological data and point SEB/SMB measurements, and better resolves the spatial patterns and temporal variability of SMB compared with the previous model version, notably in the north-east, south-east and along the K-transect in south-western Greenland. This new model version provides updated, high-resolution gridded fields of the GrIS present-day climate and SMB, and will be used for projections of the GrIS climate and SMB in response to a future climate scenario in a forthcoming study.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22663702-development-full-ice-cream-cone-model-halo-coronal-mass-ejections','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22663702-development-full-ice-cream-cone-model-halo-coronal-mass-ejections"><span>Development of a Full <span class="hlt">Ice</span>-cream Cone Model for Halo Coronal <span class="hlt">Mass</span> Ejections</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Na, Hyeonock; Moon, Y.-J.; Lee, Harim, E-mail: nho0512@khu.ac.kr, E-mail: moonyj@khu.ac.kr</p> <p></p> <p>It is essential to determine three-dimensional parameters (e.g., radial speed, angular width, and source location) of coronal <span class="hlt">mass</span> ejections (CMEs) for the space weather forecast. In this study, we investigate which cone type represents a halo CME morphology using 29 CMEs (12 Solar and Heliospheric Observatory (SOHO) /Large Angle and Spectrometric Coronagraph (LASCO) halo CMEs and 17 Solar Terrestrial Relations Observatory ( STEREO )/Sun–Earth Connection Coronal and Heliospheric Investigation COR2 halo CMEs) from 2010 December to 2011 June. These CMEs are identified as halo CMEs by one spacecraft ( SOHO or one of STEREO A and B ) and limbmore » ones by the other spacecraft (One of STEREO A and B or SOHO ). From cone shape parameters of these CMEs, such as their front curvature, we find that the CME observational structures are much closer to a full <span class="hlt">ice</span>-cream cone type than a shallow <span class="hlt">ice</span>-cream cone type. Thus, we develop a full <span class="hlt">ice</span>-cream cone model based on a new methodology that the full <span class="hlt">ice</span>-cream cone consists of many flat cones with different heights and angular widths to estimate the three-dimensional parameters of the halo CMEs. This model is constructed by carrying out the following steps: (1) construct a cone for a given height and angular width, (2) project the cone onto the sky plane, (3) select points comprising the outer boundary, and (4) minimize the difference between the estimated projection speeds with the observed ones. By applying this model to 12 SOHO /LASCO halo CMEs, we find that 3D parameters from our method are similar to those from other stereoscopic methods (i.e., a triangulation method and a Graduated Cylindrical Shell model).« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910001140','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910001140"><span>Cirrus cloud model parameterizations: Incorporating realistic <span class="hlt">ice</span> particle generation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sassen, Kenneth; Dodd, G. C.; Starr, David OC.</p> <p>1990-01-01</p> <p>Recent cirrus cloud modeling studies have involved the application of a time-dependent, two dimensional Eulerian model, with generalized cloud microphysical parameterizations drawn from experimental findings. For computing the <span class="hlt">ice</span> versus vapor phase changes, the <span class="hlt">ice</span> <span class="hlt">mass</span> <span class="hlt">content</span> is linked to the maintenance of a relative humidity with respect to <span class="hlt">ice</span> (RHI) of 105 percent; <span class="hlt">ice</span> growth occurs both with regard to the introduction of new particles and the growth of existing particles. In a simplified cloud model designed to investigate the basic role of various physical processes in the growth and maintenance of cirrus clouds, these parametric relations are justifiable. In comparison, the one dimensional cloud microphysical model recently applied to evaluating the nucleation and growth of <span class="hlt">ice</span> crystals in cirrus clouds explicitly treated populations of haze and cloud droplets, and <span class="hlt">ice</span> crystals. Although these two modeling approaches are clearly incompatible, the goal of the present numerical study is to develop a parametric treatment of new <span class="hlt">ice</span> particle generation, on the basis of detailed microphysical model findings, for incorporation into improved cirrus growth models. For example, the relation between temperature and the relative humidity required to generate <span class="hlt">ice</span> crystals from ammonium sulfate haze droplets, whose probability of freezing through the homogeneous nucleation mode are a combined function of time and droplet molality, volume, and temperature. As an example of this approach, the results of cloud microphysical simulations are presented showing the rather narrow domain in the temperature/humidity field where new <span class="hlt">ice</span> crystals can be generated. The microphysical simulations point out the need for detailed CCN studies at cirrus altitudes and haze droplet measurements within cirrus clouds, but also suggest that a relatively simple treatment of <span class="hlt">ice</span> particle generation, which includes cloud chemistry, can be incorporated into cirrus cloud growth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/10903197','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/10903197"><span><span class="hlt">Mass</span> Balance of the Greenland <span class="hlt">Ice</span> Sheet at High Elevations.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Thomas; Akins; Csatho; Fahnestock; Gogineni; Kim; Sonntag</p> <p>2000-07-21</p> <p>Comparison of <span class="hlt">ice</span> discharge from higher elevation areas of the entire Greenland <span class="hlt">Ice</span> Sheet with total snow accumulation gives estimates of <span class="hlt">ice</span> thickening rates over the past few decades. On average, the region has been in balance, but with thickening of 21 centimeters per year in the southwest and thinning of 30 centimeters per year in the southeast. The north of the <span class="hlt">ice</span> sheet shows less variability, with average thickening of 2 centimeters per year in the northeast and thinning of about 5 centimeters per year in the northwest. These results agree well with those from repeated altimeter surveys, except in the extreme south, where we find substantially higher rates of both thickening and thinning.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19879587','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19879587"><span>Ultra-trace determination of Persistent Organic Pollutants in Arctic <span class="hlt">ice</span> using stir bar sorptive extraction and gas chromatography coupled to <span class="hlt">mass</span> spectrometry.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lacorte, S; Quintana, J; Tauler, R; Ventura, F; Tovar-Sánchez, A; Duarte, C M</p> <p>2009-12-04</p> <p>This study presents the optimization and application of an analytical method based on the use of stir bar sorptive extraction (SBSE) gas chromatography coupled to <span class="hlt">mass</span> spectrometry (GC-MS) for the ultra-trace analysis of POPs (Persistent Organic Pollutants) in Arctic <span class="hlt">ice</span>. In a first step, the <span class="hlt">mass</span>-spectrometry conditions were optimized to quantify 48 compounds (polycyclic aromatic hydrocarbons, brominated diphenyl ethers, chlorinated biphenyls, and organochlorinated pesticides) at the low pg/L level. In a second step, the performance of this analytical method was evaluated to determine POPs in Arctic cores collected during an oceanographic campaign. Using a calibration range from 1 to 1800 pg/L and by adjusting acquisition parameters, limits of detection at the 0.1-99 and 102-891 pg/L for organohalogenated compounds and polycyclic aromatic hydrocarbons, respectively, were obtained by extracting 200 mL of unfiltered <span class="hlt">ice</span> water. alpha-hexachlorocyclohexane, DDTs, chlorinated biphenyl congeners 28, 101 and 118 and brominated diphenyl ethers congeners 47 and 99 were detected in <span class="hlt">ice</span> cores at levels between 0.5 to 258 pg/L. We emphasise the advantages and disadvantages of in situ SBSE in comparison with traditional extraction techniques used to analyze POPs in <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28753208','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28753208"><span><span class="hlt">Ice</span> nucleation active bacteria in precipitation are genetically diverse and nucleate <span class="hlt">ice</span> by employing different mechanisms.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Failor, K C; Schmale, D G; Vinatzer, B A; Monteil, C L</p> <p>2017-12-01</p> <p>A growing body of circumstantial evidence suggests that <span class="hlt">ice</span> nucleation active (<span class="hlt">Ice</span> + ) bacteria contribute to the initiation of precipitation by heterologous freezing of super-cooled water in clouds. However, little is known about the concentration of <span class="hlt">Ice</span> + bacteria in precipitation, their genetic and phenotypic diversity, and their relationship to air <span class="hlt">mass</span> trajectories and precipitation chemistry. In this study, 23 precipitation events were collected over 15 months in Virginia, USA. Air <span class="hlt">mass</span> trajectories and water chemistry were determined and 33 134 isolates were screened for <span class="hlt">ice</span> nucleation activity (INA) at -8 °C. Of 1144 isolates that tested positive during initial screening, 593 had confirmed INA at -8 °C in repeated tests. Concentrations of <span class="hlt">Ice</span> + strains in precipitation were found to range from 0 to 13 219 colony forming units per liter, with a mean of 384±147. Most <span class="hlt">Ice</span> + bacteria were identified as members of known and unknown <span class="hlt">Ice</span> + species in the Pseudomonadaceae, Enterobacteriaceae and Xanthomonadaceae families, which nucleate <span class="hlt">ice</span> employing the well-characterized membrane-bound INA protein. Two <span class="hlt">Ice</span> + strains, however, were identified as Lysinibacillus, a Gram-positive genus not previously known to include <span class="hlt">Ice</span> + bacteria. INA of the Lysinibacillus strains is due to a nanometer-sized molecule that is heat resistant, lysozyme and proteinase resistant, and secreted. <span class="hlt">Ice</span> + bacteria and the INA mechanisms they employ are thus more diverse than expected. We discuss to what extent the concentration of culturable <span class="hlt">Ice</span> + bacteria in precipitation and the identification of a new heat-resistant biological INA mechanism support a role for <span class="hlt">Ice</span> + bacteria in the initiation of precipitation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1913308B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1913308B"><span>Longwave radiative effects of Saharan dust during the <span class="hlt">ICE-D</span> campaign</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brooke, Jennifer; Havemann, Stephan; Ryder, Claire; O'Sullivan, Debbie</p> <p>2017-04-01</p> <p>The Havemann-Taylor Fast Radiative Transfer Code (HT-FRTC) is a fast radiative transfer model based on Principal Components. Scattering has been incorporated into HT-FRTC which allows simulations of aerosol as well as clear-sky atmospheres. This work evaluates the scattering scheme in HT-FRTC and investigates dust-affected brightness temperatures using in-situ observations from <span class="hlt">Ice</span> in Clouds Experiment - Dust (<span class="hlt">ICE-D</span>) campaign. The <span class="hlt">ICE-D</span> campaign occurred during August 2015 and was based from Cape Verde. The <span class="hlt">ICE-D</span> campaign is a multidisciplinary project which achieved measurements of in-situ mineral dust properties of the dust advected from the Sahara, and on the aerosol-cloud interactions using the FAAM BAe-146 research aircraft. <span class="hlt">ICE-D</span> encountered a range of low (0.3), intermediate (0.8) and high (1.3) aerosol optical depths, AODs, and therefore provides a range of atmospheric dust loadings in the assessment of dust scattering in HT-FRTC. Spectral radiances in the thermal infrared window region (800 - 1200 cm-1) are sensitive to the presence of mineral dust; mineral dust acts to reduce the upwelling infrared radiation caused by the absorption and re-emission of radiation by the dust layer. ARIES (Airborne Research Interferometer Evaluation System) is a nadir-facing interferometer, measuring infrared radiances between 550 and 3000 cm-1. The ARIES spectral radiances are converted to brightness temperatures by inversion of the Planck function. The mineral dust size distribution is important for radiative transfer applications as it provides a measure of aerosol scattering. The longwave spectral mineral dust optical properties including the <span class="hlt">mass</span> extinction coefficients, single scattering albedos and the asymmetry parameter have been derived from the mean <span class="hlt">ICE-D</span> size distribution. HT-FRTC scattering simulations are initialised with vertical <span class="hlt">mass</span> fractions which can be derived from extinction profiles from the lidar along with the specific extinction coefficient, kext (m2</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1916805B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1916805B"><span><span class="hlt">Ice</span> nucleation of natural desert dust including organics sourced from nine deserts worldwide</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Boose, Yvonne; Welti, André; Atkinson, James; Danielczok, Anja; Bingemer, Heinz; Plötze, Michael; Lohmann, Ulrike; Kanji, Zamin A.</p> <p>2017-04-01</p> <p>The extraordinary high <span class="hlt">ice</span> nucleation (IN) potential of microcline, a K-feldspar mineral, at temperatures (T) above 248 and up to 271 K has been show recently. However, it is unclear if microcline is also found at the surface of airborne mineral dust particles or if chemical and mechanical aging processes lead to its destruction or shielding and thus reduced IN ability in the atmosphere. It is suggested that instead organic material mixed with inorganic minerals is responsible for cloud glaciation at T ≥ 253 K. We collected airborne Saharan dust at 4 locations at different distances from the desert and 11 samples from the surface of 9 of the major deserts worldwide. We studied immersion IN on these samples between 235 - 263 K using the IMCA-ZINC (immersion mode cooling chamber - Zurich <span class="hlt">ice</span> nucleation chamber) setup and the FRIDGE (Franfurt <span class="hlt">Ice</span> Nuclei Deposition Freezing Experiment) instrument run in droplet freezing mode. By correlating the results with the bulk mineralogy of the dust samples, determined by X-ray diffraction analysis, we show that at 253 K, K-feldspar indeed predicts best the IN behavior of the samples. At lower T (238 - 245 K) however, quartz and the total feldspar <span class="hlt">contents</span> correlate best. Furthermore, microcline is only found in one of the airborne Saharan dust samples (3.9 wt%) while in the others the amount is below the detection limit or completely absent. Relative humidity (RH) scans at constant T = 238, 240 and 242 K were additionally performed with the portable <span class="hlt">ice</span> nucleation counter, PINC. Above and below water saturation a similar prominent role of quartz is found as in the immersion mode. To investigate the role of organic material on the IN ability, we heated some of the samples at 573 K for 10 h and repeated the RH-scans. Furthermore, we performed thermogravimetric analysis of the dusts. The two tested airborne Saharan samples loose between 2.8 and 7.5 % of their <span class="hlt">mass</span> at T ≤ 573 K, partly due to water release, partly due to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018EPJWC.16804010P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018EPJWC.16804010P"><span>Searches for magnetic monopoles with <span class="hlt">Ice</span>Cube</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pollmann, Anna</p> <p>2018-01-01</p> <p>Particles that carry a magnetic monopole charge are proposed by various theories which go beyond the Standard Model of particle physics. The expected <span class="hlt">mass</span> of magnetic monopoles varies depending on the theory describing its origin, generally the monopole <span class="hlt">mass</span> far exceeds those which can be created at accelerators. Magnetic monopoles gain kinetic energy in large scale galactic magnetic fields and, depending on their <span class="hlt">mass</span>, can obtain relativistic velocities. <span class="hlt">Ice</span>Cube is a high energy neutrino detector using the clear <span class="hlt">ice</span> at the South Pole as a detection medium. As monopoles pass through this <span class="hlt">ice</span> they produce optical light by a variety of mechanisms. With increasing velocity, they produce light by catalysis of baryon decay, luminescence in the <span class="hlt">ice</span> associated with electronic excitations, indirect and direct Cherenkov light from the monopole track, and Cherenkov light from cascades induced by pair creation and photonuclear reactions. By searching for this light, current best limits for the monopole flux over a broad range of velocities was achieved using the <span class="hlt">Ice</span>Cube detector. A review of these magnetic monopole searches is presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22259152','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22259152"><span>Arctic <span class="hlt">ice</span> cover, <span class="hlt">ice</span> thickness and tipping points.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wadhams, Peter</p> <p>2012-02-01</p> <p>We summarize the latest results on the rapid changes that are occurring to Arctic sea <span class="hlt">ice</span> thickness and extent, the reasons for them, and the methods being used to monitor the changing <span class="hlt">ice</span> thickness. Arctic sea <span class="hlt">ice</span> extent had been shrinking at a relatively modest rate of 3-4% per decade (annually averaged) but after 1996 this speeded up to 10% per decade and in summer 2007 there was a massive collapse of <span class="hlt">ice</span> extent to a new record minimum of only 4.1 million km(2). Thickness has been falling at a more rapid rate (43% in the 25 years from the early 1970s to late 1990s) with a specially rapid loss of <span class="hlt">mass</span> from pressure ridges. The summer 2007 event may have arisen from an interaction between the long-term retreat and more rapid thinning rates. We review thickness monitoring techniques that show the greatest promise on different spatial and temporal scales, and for different purposes. We show results from some recent work from submarines, and speculate that the trends towards retreat and thinning will inevitably lead to an eventual loss of all <span class="hlt">ice</span> in summer, which can be described as a 'tipping point' in that the former situation, of an Arctic covered with mainly multi-year <span class="hlt">ice</span>, cannot be retrieved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=Remote+AND+sensing&id=EJ1016786','ERIC'); return false;" href="https://eric.ed.gov/?q=Remote+AND+sensing&id=EJ1016786"><span>Reading the <span class="hlt">Ice</span>: Using Remote Sensing to Analyze Radar Data</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Gillette, Brandon; Leinmiller-Renick, Kelsey; Foga, Steve</p> <p>2013-01-01</p> <p>Understanding the behavior of <span class="hlt">ice</span> sheets (thick, continent-size <span class="hlt">ice</span> <span class="hlt">masses</span>) and glaciers (smaller, flowing <span class="hlt">masses</span> of <span class="hlt">ice</span>) is increasingly important as our climate changes, particularly in the Polar Regions. This article describes two lessons, based on the 5E (engage, explore, explain, elaborate, and evaluate) model, that help students practice…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20010066068','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20010066068"><span>Determining Greenland <span class="hlt">Ice</span> Sheet Accumulation Rates from Radar Remote Sensing</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jezek, Kenneth C.</p> <p>2001-01-01</p> <p>An important component of NASA's Program for Arctic Regional Climate Assessment (PARCA) is a <span class="hlt">mass</span> balance investigation of the Greenland <span class="hlt">Ice</span> Sheet. The <span class="hlt">mass</span> balance is calculated by taking the difference between the snow accumulation and the <span class="hlt">ice</span> discharge of the <span class="hlt">ice</span> sheet. Uncertainties in this calculation include the snow accumulation rate, which has traditionally been determined by interpolating data from <span class="hlt">ice</span> core samples taken throughout the <span class="hlt">ice</span> sheet. The sparse data associated with <span class="hlt">ice</span> cores, coupled with the high spatial and temporal resolution provided by remote sensing, have motivated scientists to investigate relationships between accumulation rate and microwave observations.</p> </li> </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/2060/20170002537','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170002537"><span>Numerical Analysis of Mixed-Phase <span class="hlt">Icing</span> Cloud Simulations in the NASA Propulsion Systems Laboratory</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bartkus, Tadas; Tsao, Jen-Ching; Struk, Peter; Van Zante, Judith</p> <p>2017-01-01</p> <p>This presentation describes the development of a numerical model that couples the thermal interaction between <span class="hlt">ice</span> particles, water droplets, and the flowing gas of an <span class="hlt">icing</span> wind tunnel for simulation of NASA Glenn Research Centers Propulsion Systems Laboratory (PSL). The ultimate goal of the model is to better understand the complex interactions between the test parameters and have greater confidence in the conditions at the test section of the PSL tunnel. The model attempts to explain the observed changes in test conditions by coupling the conservation of <span class="hlt">mass</span> and energy equations for both the cloud particles and flowing gas <span class="hlt">mass</span>. Model predictions were compared to measurements taken during May 2015 testing at PSL, where test conditions varied gas temperature, pressure, velocity and humidity levels, as well as the cloud total water <span class="hlt">content</span>, particle initial temperature, and particle size distribution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170009576','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170009576"><span>Numerical Analysis of Mixed-Phase <span class="hlt">Icing</span> Cloud Simulations in the NASA Propulsion Systems Laboratory</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bartkus, Tadas P.; Tsao, Jen-Ching; Struk, Peter M.; Van Zante, Judith F.</p> <p>2017-01-01</p> <p>This paper describes the development of a numerical model that couples the thermal interaction between <span class="hlt">ice</span> particles, water droplets, and the flowing gas of an <span class="hlt">icing</span> wind tunnel for simulation of NASA Glenn Research Centers Propulsion Systems Laboratory (PSL). The ultimate goal of the model is to better understand the complex interactions between the test parameters and have greater confidence in the conditions at the test section of the PSL tunnel. The model attempts to explain the observed changes in test conditions by coupling the conservation of <span class="hlt">mass</span> and energy equations for both the cloud particles and flowing gas <span class="hlt">mass</span>. Model predictions were compared to measurements taken during May 2015 testing at PSL, where test conditions varied gas temperature, pressure, velocity and humidity levels, as well as the cloud total water <span class="hlt">content</span>, particle initial temperature, and particle size distribution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70012549','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70012549"><span><span class="hlt">Ice</span> sheet topography by satellite altimetry</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Brooks, R.L.; Campbell, W.J.; Ramseier, R.O.; Stanley, H.R.; Zwally, H.J.</p> <p>1978-01-01</p> <p>The surface elevation of the southern Greenland <span class="hlt">ice</span> sheet and surface features of the <span class="hlt">ice</span> flow are obtained from the radar altimeter on the GEOS 3 satellite. The achieved accuracy in surface elevation is ???2 m. As changes in surface elevation are indicative of changes in <span class="hlt">ice</span> volume, the <span class="hlt">mass</span> balance of the present <span class="hlt">ice</span> sheets could be determined by repetitive mapping of the surface elevation and the surface could be monitored to detect surging or significant changes in <span class="hlt">ice</span> flow. ?? 1978 Nature Publishing Group.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA572179','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA572179"><span><span class="hlt">Mass</span> Balance of Multiyear Sea <span class="hlt">Ice</span> in the Southern Beaufort Sea</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2012-09-30</p> <p>datasets. Table 1 lists the primary data sources to be used. To determine sources and sinks of MY <span class="hlt">ice</span>, we use a simple model of MY <span class="hlt">ice</span> circulation, which is...shown in Figure 1. In this model , we consider the Beaufort Sea to consist of four zones defined by mean drift of sea <span class="hlt">ice</span> in summer and winter, such...Healy/Louis S. St. Laurant cruises 1 Seasonal <span class="hlt">Ice</span> Zone Observing Network 2 Polar Airborne Measurements and Arctic Regional Climate Model</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18..575B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18..575B"><span>Investigating <span class="hlt">ice</span> cliff evolution and contribution to glacier <span class="hlt">mass</span>-balance using a physically-based dynamic model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Buri, Pascal; Miles, Evan; Ragettli, Silvan; Brun, Fanny; Steiner, Jakob; Pellicciotti, Francesca</p> <p>2016-04-01</p> <p>Supraglacial cliffs are a surface feature typical of debris-covered glaciers, affecting surface evolution, glacier downwasting and <span class="hlt">mass</span> balance by providing a direct <span class="hlt">ice</span>-atmosphere interface. As a result, melt rates can be very high and <span class="hlt">ice</span> cliffs may account for a significant portion of the total glacier <span class="hlt">mass</span> loss. However, their contribution to glacier <span class="hlt">mass</span> balance has rarely been quantified through physically-based models. Most cliff energy balance models are point scale models which calculate energy fluxes at individual cliff locations. Results from the only grid based model to date accurately reflect energy fluxes and cliff melt, but modelled backwasting patterns are in some cases unrealistic, as the distribution of melt rates would lead to progressive shallowing and disappearance of cliffs. Based on a unique multitemporal dataset of cliff topography and backwasting obtained from high-resolution terrestrial and aerial Structure-from-Motion analysis on Lirung Glacier in Nepal, it is apparent that cliffs exhibit a range of behaviours but most do not rapidly disappear. The patterns of evolution cannot be explained satisfactorily by atmospheric melt alone, and are moderated by the presence of supraglacial ponds at the base of cliffs and by cliff reburial with debris. Here, we document the distinct patterns of evolution including disappearance, growth and stability. We then use these observations to improve the grid-based energy balance model, implementing periodic updates of the cliff geometry resulting from modelled melt perpendicular to the <span class="hlt">ice</span> surface. Based on a slope threshold, pixels can be reburied by debris or become debris-free. The effect of ponds are taken into account through enhanced melt rates in horizontal direction on pixels selected based on an algorithm considering distance to the water surface, slope and lake level. We use the dynamic model to first study the evolution of selected cliffs for which accurate, high resolution DEMs are available</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018QSRv..189....1M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018QSRv..189....1M"><span>Reconciling records of <span class="hlt">ice</span> streaming and <span class="hlt">ice</span> margin retreat to produce a palaeogeographic reconstruction of the deglaciation of the Laurentide <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Margold, Martin; Stokes, Chris R.; Clark, Chris D.</p> <p>2018-06-01</p> <p>This paper reconstructs the deglaciation of the Laurentide <span class="hlt">Ice</span> Sheet (LIS; including the Innuitian <span class="hlt">Ice</span> Sheet) from the Last Glacial Maximum (LGM), with a particular focus on the spatial and temporal 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> sheet lost its marine margin. <span class="hlt">Ice</span> streams with a terrestrial <span class="hlt">ice</span> margin in the west and south were more transient and <span class="hlt">ice</span> flow directions changed with the build-up, peak-phase and collapse of the Cordilleran-Laurentide <span class="hlt">ice</span> saddle. The south-eastern marine margin in Atlantic Canada started to retreat relatively early and some of the <span class="hlt">ice</span> streams in this region switched off at or shortly after the LGM. In contrast, the <span class="hlt">ice</span> streams draining towards the north-western and north-eastern marine margins in the Beaufort Sea and in Baffin Bay appear to have remained stable throughout most of the Late Glacial, and some of them continued to function until after the Younger Dryas (YD). The YD influenced the dynamics of the deglaciation, but there remains uncertainty about the response of the <span class="hlt">ice</span> sheet in several sectors. We tentatively ascribe the switching-on of some major <span class="hlt">ice</span> streams during this period (e.g. M'Clintock Channel <span class="hlt">Ice</span> Stream at the north-west margin), but for other large <span class="hlt">ice</span> streams whose timing partially overlaps with the YD, the drivers are less clear and <span class="hlt">ice</span>-dynamical processes, rather than effects of climate and surface <span class="hlt">mass</span> balance are viewed as more likely drivers. Retreat</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012ApJ...756L..24G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012ApJ...756L..24G"><span>In-situ Probing of Radiation-induced Processing of Organics in Astrophysical <span class="hlt">Ice</span> Analogs—Novel Laser Desorption Laser Ionization Time-of-flight <span class="hlt">Mass</span> Spectroscopic Studies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gudipati, Murthy S.; Yang, Rui</p> <p>2012-09-01</p> <p>Understanding the evolution of organic molecules in <span class="hlt">ice</span> grains in the interstellar medium (ISM) under cosmic rays, stellar radiation, and local electrons and ions is critical to our understanding of the connection between ISM and solar systems. Our study is aimed at reaching this goal of looking directly into radiation-induced processing in these <span class="hlt">ice</span> grains. We developed a two-color laser-desorption laser-ionization time-of-flight <span class="hlt">mass</span> spectroscopic method (2C-MALDI-TOF), similar to matrix-assisted laser desorption and ionization time-of-flight (MALDI-TOF) <span class="hlt">mass</span> spectroscopy. Results presented here with polycyclic aromatic hydrocarbon (PAH) probe molecules embedded in water-<span class="hlt">ice</span> at 5 K show for the first time that hydrogenation and oxygenation are the primary chemical reactions that occur in astrophysical <span class="hlt">ice</span> analogs when subjected to Lyα radiation. We found that hydrogenation can occur over several unsaturated bonds and the product distribution corresponds to their stabilities. Multiple hydrogenation efficiency is found to be higher at higher temperatures (100 K) compared to 5 K—close to the interstellar <span class="hlt">ice</span> temperatures. Hydroxylation is shown to have similar efficiencies at 5 K or 100 K, indicating that addition of O atoms or OH radicals to pre-ionized PAHs is a barrierless process. These studies—the first glimpses into interstellar <span class="hlt">ice</span> chemistry through analog studies—show that once accreted onto <span class="hlt">ice</span> grains PAHs lose their PAH spectroscopic signatures through radiation chemistry, which could be one of the reason for the lack of PAH detection in interstellar <span class="hlt">ice</span> grains, particularly the outer regions of cold, dense clouds or the upper molecular layers of protoplanetary disks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25920464','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25920464"><span>Functionality of kumquat (Fortunella margarita) in the production of fruity <span class="hlt">ice</span> cream.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Çakmakçı, Songül; Topdaş, Elif Feyza; Çakır, Yusuf; Kalın, Pınar</p> <p>2016-03-30</p> <p>The aim of this study was to investigate the effect of kumquat (Fortunella margarita) on the quality characteristics of <span class="hlt">ice</span> cream. Kumquat paste (KP) was added to an <span class="hlt">ice</span> cream mix at four concentrations, 0 (control), 5, 10 and 15% (w/w), for <span class="hlt">ice</span> cream production. The increment of KP level caused an increase in acidity, vitamin C <span class="hlt">content</span>, b* value and overrun value compared with the control <span class="hlt">ice</span> cream. The apparent viscosity of samples decreased with the addition of KP at concentrations of 5 and 10% compared with the control. Results indicated that lyophilized water extract of KP (LKE) contained remarkable phenolic compounds. It was observed that LKE exhibited moderate in vitro antioxidant capacity. KP enhanced the color, flavor, vitamin C <span class="hlt">content</span> and Mg and K <span class="hlt">contents</span> of the <span class="hlt">ice</span> cream. The addition of KP positively affected the sensory properties. KP may be used as a suitable source of natural color and flavor agent in <span class="hlt">ice</span> cream production. KP enhanced the vitamin C <span class="hlt">content</span> and Mg and K <span class="hlt">contents</span> of <span class="hlt">ice</span> cream and improved its sensory properties. © 2015 Society of Chemical Industry.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.P34A..05S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.P34A..05S"><span>Breaking <span class="hlt">Ice</span>: Fracture Processes in Floating <span class="hlt">Ice</span> on Earth and Elsewhere</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Scambos, T. A.</p> <p>2016-12-01</p> <p>Rapid, intense fracturing events in the <span class="hlt">ice</span> shelves of the Antarctic Peninsula reveal a set of processes that were not fully appreciated prior to the series of <span class="hlt">ice</span> shelf break-ups observed in the late 1990s and early 2000s. A series of studies have uncovered a fascinating array of relationships between climate, ocean, and <span class="hlt">ice</span>: intense widespread hydrofracture; repetitive hydrofracture induced by <span class="hlt">ice</span> plate bending; the ability for sub-surface flooded firn to support hydrofracture; potential triggering by long-period wave action; accelerated fracturing by trapped tsunamic waves; iceberg disintegration, and a remarkable <span class="hlt">ice</span> rebound process from lake drainage that resembles runaway nuclear fission. The events and subsequent studies have shown that rapid regional warming in <span class="hlt">ice</span> shelf areas leads to catastrophic changes in a previously stable <span class="hlt">ice</span> <span class="hlt">mass</span>. More typical fracturing of thick <span class="hlt">ice</span> plates is a natural consequence of <span class="hlt">ice</span> flow in a complex geographic setting, i.e., it is induced by shear and divergence of spreading plate flow around obstacles. While these are not a result of climate or ocean change, weather and ocean processes may impact the exact timing of final separation of an iceberg from a shelf. Taking these terrestrial perspectives to other <span class="hlt">ice</span>-covered ocean worlds, cautiously, provides an observational framework for interpreting features on Europa and Enceladus.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.7677A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.7677A"><span>Melting beneath Greenland outlet glaciers and <span class="hlt">ice</span> streams</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alexander, David; Perrette, Mahé; Beckmann, Johanna</p> <p>2015-04-01</p> <p>Basal melting of fast-flowing Greenland outlet glaciers and <span class="hlt">ice</span> streams due to frictional heating at the <span class="hlt">ice</span>-bed interface contributes significantly to total glacier <span class="hlt">mass</span> balance and subglacial meltwater flux, yet modelling this basal melt process in Greenland has received minimal research attention. A one-dimensional dynamic <span class="hlt">ice</span>-flow model is calibrated to the present day longitudinal profiles of 10 major Greenland outlet glaciers and <span class="hlt">ice</span> streams (including the Jakobshavn Isbrae, Petermann Glacier and Helheim Glacier) and is validated against published <span class="hlt">ice</span> flow and surface elevation measurements. Along each longitudinal profile, basal melt is calculated as a function of <span class="hlt">ice</span> flow velocity and basal shear stress. The basal shear stress is dependent on the effective pressure (difference between <span class="hlt">ice</span> overburden pressure and water pressure), basal roughness and a sliding parametrization. Model output indicates that where outlet glaciers and <span class="hlt">ice</span> streams terminate into the ocean with either a small floating <span class="hlt">ice</span> tongue or no floating tongue whatsoever, the proportion of basal melt to total melt (surface, basal and submarine melt) is 5-10% (e.g. Jakobshavn Isbrae; Daugaard-Jensen Glacier). This proportion is, however, negligible where larger <span class="hlt">ice</span> tongues lose <span class="hlt">mass</span> mostly by submarine melt (~1%; e.g. Nioghalvfjerdsfjorden Glacier). Modelled basal melt is highest immediately upvalley of the grounding line, with contributions typically up to 20-40% of the total melt for slippery beds and up to 30-70% for resistant beds. Additionally, modelled grounding line and calving front migration inland for all outlet glaciers and <span class="hlt">ice</span> streams of hundreds of metres to several kilometres occurs. Including basal melt due to frictional heating in outlet glacier and <span class="hlt">ice</span> stream models is important for more accurately modelling <span class="hlt">mass</span> balance and subglacial meltwater flux, and therefore, more accurately modelling outlet glacier and <span class="hlt">ice</span> stream dynamics and responses to future climate change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.C54A..02A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.C54A..02A"><span>Ground <span class="hlt">ice</span> conditions in Salluit, Northern Quebec</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Allard, M.; Fortier, R.; Calmels, F.; Gagnon, O.; L'Hérault, E.</p> <p>2011-12-01</p> <p>Salluit in Northern Québec (ca. 1300 inhabitants) faces difficult ground <span class="hlt">ice</span> conditions for its development. The village is located in a U-shaped valley, along a fjord that was deglaciated around 8000 cal BP. The post-glacial marine limit is at the current elevation of 150 m ASL. Among the mapped surficial geology units, three contain particularly <span class="hlt">ice</span>-rich permafrost: marine clays, till and silty colluviums. A diamond drill was used to extract 10 permafrost cores down to 23 m deep. In addition, 18 shallow cores (to 5 m deep) were extracted with a portable drill. All the frozen cores were shipped to Québec city where ground <span class="hlt">ice</span> <span class="hlt">contents</span> were measured and cryostructures were imaged by CT-Scanning. Water <span class="hlt">contents</span>, grain-size and pore water salinity were measured. Refraction seismic profiles were run to measure the depth to bedrock. GPR and electrical resistivity surveys helped to map <span class="hlt">ice</span>-rich areas. Three cone penetration tests (CPT) were run in the frozen clays to depths ranging from 8 to 21 m. Maximum clay thickness is ca. 50 m deep near the shoreline. The cone penetration tests and all the cores in clays revealed large amounts of both segregated and aggradational <span class="hlt">ice</span> (volumetric <span class="hlt">contents</span> up to 93% over thicknesses of one meter) to depths varying between 2.5 and 4 m, below which the <span class="hlt">ice</span> <span class="hlt">content</span> decreases and the salinity increases (values measured up to 42 gr/L between 4.5 and 6 m deep). Chunks of organic matter buried below the actual active layer base indicate past cryoturbations under a somewhat warmer climate, most probably associated with intense frost boil action, as widely observed today. The stony till has developed large quantities of segregation <span class="hlt">ice</span> which can be seen in larger concentrations and as thicker lenses under boulders and in matrix rich (≥ 50% sand and silt) parts of the glacial sediment. As digging for a sewage pond was undertaken in winter 2008 by blasting, the clast-influenced cryostructure of the till could be observed in cuts and in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/7061','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/7061"><span>Columbia Glacier stake location, <span class="hlt">mass</span> balance, glacier surface altitude, and <span class="hlt">ice</span> radar data, 1978 measurement year</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Mayo, L.R.; Trabant, D.C.; March, Rod; Haeberli, Wilfried</p> <p>1979-01-01</p> <p>A 1 year data-collection program on Columbia Glacier, Alaska has produced a data set consisting of near-surface <span class="hlt">ice</span> kinematics, <span class="hlt">mass</span> balance, and altitude change at 57 points and 34 <span class="hlt">ice</span> radar soundings. These data presented in two tables, are part of the basic data required for glacier dynamic analysis, computer models, and predictions of the number and size of icebergs which Columbia Glacier will calve into shipping lanes of eastern Prince William Sound. A metric, sea-level coordinate system was developed for use in surveying throughout the basin. Its use is explained and monument coordinates listed. A series of seven integrated programs for calculators were used in both the field and office to reduce the surveying data. These programs are thoroughly documented and explained in the report. (Kosco-USGS)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.5867S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.5867S"><span>Changes in <span class="hlt">ice</span> dynamics along the northern Antarctic Peninsula</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Seehaus, Thorsten; Marinsek, Sebastian; Cook, Alison; Van Wessem, Jan-Melchior; Braun, Matthias</p> <p>2017-04-01</p> <p>The climatic conditions along the Antarctic Peninsula have undergone considerable changes during the last 50 years. A period of pronounced air temperature rise, increasing ocean temperatures as well as changes in the precipitation pattern have been reported by various authors. Consequently, the glacial systems showed changes including widespread retreat, surface lowering as well as variations in flow speeds. During the last decades numerous <span class="hlt">ice</span> shelves along the Antarctic Peninsula retreated, started to break-up or disintegrated completely. The loss of the buttressing effect caused tributary glaciers to accelerate with increasing <span class="hlt">ice</span> discharge along the Antarctic Peninsula. Quantification of the <span class="hlt">mass</span> changes is still subject to considerable errors although numbers derived from the different methods are converging. The aim is to study the reaction of glaciers at the northern Antarctic Peninsula to the changing climatic conditions and the readjustments of tributary glaciers to <span class="hlt">ice</span> shelf disintegration, as well as to better quantify the <span class="hlt">ice</span> <span class="hlt">mass</span> loss and its temporal changes. We analysed time series of various satellite sensors (ERS-1/2 SAR, ENVISAT ASAR, RADARSAT-1, ALOS PALSAR, TerraSAR-X/TanDEM-X, ASTER, Landsat) to detect changes in <span class="hlt">ice</span> dynamics of 74 glacier basins along the northern Antarctic Peninsula (<65°). Intensity feature tracking techniques were applied on data stacks from different SAR satellites over the last 20 years to infer temporal trends in glacier surface velocities. In combination with <span class="hlt">ice</span> thickness reconstructions and modeled climatic <span class="hlt">mass</span> balance fields regional imbalances were calculated. Variations in <span class="hlt">ice</span> front position were mapped based on optical and SAR satellite data sets. Along the west coast of the northern Antarctic Peninsula an increase in flow speeds by 40% between 1992 and 2014 was observed, whereas glaciers on the east side (north of former Prince-Gustav <span class="hlt">Ice</span> Shelf) showed a strong deceleration. Nearly all former <span class="hlt">ice</span> shelf</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19830062257&hterms=marginal&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dmarginal','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19830062257&hterms=marginal&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dmarginal"><span>Sensitivity studies with a coupled <span class="hlt">ice</span>-ocean model of the marginal <span class="hlt">ice</span> zone</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Roed, L. P.</p> <p>1983-01-01</p> <p>An analytical coupled <span class="hlt">ice</span>-ocean model is considered which is forced by a specified wind stress acting on the open ocean as well as the <span class="hlt">ice</span>. The analysis supports the conjecture that the upwelling dynamics at <span class="hlt">ice</span> edges can be understood by means of a simple analytical model. In similarity with coastal problems it is shown that the <span class="hlt">ice</span> edge upwelling is determined by the net <span class="hlt">mass</span> flux at the boundaries of the considered region. The model is used to study the sensitivity of the upwelling dynamics in the marginal <span class="hlt">ice</span> zone to variation in the controlling parameters. These parameters consist of combinations of the drag coefficients used in the parameterization of the stresses on the three interfaces atmosphere-<span class="hlt">ice</span>, atmosphere-ocean, and <span class="hlt">ice</span>-ocean. The response is shown to be sensitive to variations in these parameters in that one set of parameters may give upwelling while a slightly different set of parameters may give downwelling.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19884496','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19884496"><span>The future of <span class="hlt">ice</span> sheets and sea <span class="hlt">ice</span>: between reversible retreat and unstoppable loss.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Notz, Dirk</p> <p>2009-12-08</p> <p>We discuss the existence of cryospheric "tipping points" in the Earth's climate system. Such critical thresholds have been suggested to exist for the disappearance of Arctic sea <span class="hlt">ice</span> and the retreat of <span class="hlt">ice</span> sheets: Once these <span class="hlt">ice</span> <span class="hlt">masses</span> have shrunk below an anticipated critical extent, the <span class="hlt">ice</span>-albedo feedback might lead to the irreversible and unstoppable loss of the remaining <span class="hlt">ice</span>. We here give an overview of our current understanding of such threshold behavior. By using conceptual arguments, we review the recent findings that such a tipping point probably does not exist for the loss of Arctic summer sea <span class="hlt">ice</span>. Hence, in a cooler climate, sea <span class="hlt">ice</span> could recover rapidly from the loss it has experienced in recent years. In addition, we discuss why this recent rapid retreat of Arctic summer sea <span class="hlt">ice</span> might largely be a consequence of a slow shift in <span class="hlt">ice</span>-thickness distribution, which will lead to strongly increased year-to-year variability of the Arctic summer sea-<span class="hlt">ice</span> extent. This variability will render seasonal forecasts of the Arctic summer sea-<span class="hlt">ice</span> extent increasingly difficult. We also discuss why, in contrast to Arctic summer sea <span class="hlt">ice</span>, a tipping point is more likely to exist for the loss of the Greenland <span class="hlt">ice</span> sheet and the West Antarctic <span class="hlt">ice</span> sheet.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.C11A0094S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.C11A0094S"><span>Estimation of Greenland's <span class="hlt">Ice</span> Sheet <span class="hlt">Mass</span> Balance Using ICESat and GRACE Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Slobbe, D.; Ditmar, P.; Lindenbergh, R.</p> <p>2007-12-01</p> <p>Data of the GRACE gravity mission and the ICESat laser altimetry mission are used to create two independent estimates of Greenland's <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balance over the full measurement period. For ICESat data, a processing strategy is developed using the elevation differences of geometrically overlapping footprints of both crossing and repeated tracks. The dataset is cleaned using quality flags defined by the GLAS science team. The cleaned dataset reveals some strong, spatially correlated signals that are shown to be related to physical phenomena. Different processing strategies are used to convert the observed temporal height differences to <span class="hlt">mass</span> changes for 6 different drainage systems, further divided into a region above and below 2000 meter elevation. The results are compared with other altimetry based <span class="hlt">mass</span> balance estimates. In general, the obtained results confirm trends discovered by others, but we also show that the choice of processing strategy strongly influences our results, especially for the areas below 2000 meter. Furthermore, GRACE based monthly variations of the Earth's gravity field as processed by CNES, CSR, GFZ and DEOS are used to estimate the <span class="hlt">mass</span> balance change for North and South Greenland. It is shown that our results are comparable with recently published GRACE estimates (mascon solutions). On the other hand, the estimates based on GRACE data are only partly confirmed by the ICESat estimates. Possible explanations for the obvious differences will be discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45.4086A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45.4086A"><span>Variable Basal Melt Rates of Antarctic Peninsula <span class="hlt">Ice</span> Shelves, 1994-2016</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Adusumilli, Susheel; Fricker, Helen Amanda; Siegfried, Matthew R.; Padman, Laurie; Paolo, Fernando S.; Ligtenberg, Stefan R. M.</p> <p>2018-05-01</p> <p>We have constructed 23-year (1994-2016) time series of Antarctic Peninsula (AP) <span class="hlt">ice</span>-shelf height change using data from four satellite radar altimeters (ERS-1, ERS-2, Envisat, and CryoSat-2). Combining these time series with output from atmospheric and firn models, we partitioned the total height-change signal into contributions from varying surface <span class="hlt">mass</span> balance, firn state, <span class="hlt">ice</span> dynamics, and basal <span class="hlt">mass</span> balance. On the Bellingshausen coast of the AP, <span class="hlt">ice</span> shelves lost 84 ± 34 Gt a-1 to basal melting, compared to contributions of 50 ± 7 Gt a-1 from surface <span class="hlt">mass</span> balance and <span class="hlt">ice</span> dynamics. Net basal melting on the Weddell coast was 51 ± 71 Gt a-1. Recent changes in <span class="hlt">ice</span>-shelf height include increases over major AP <span class="hlt">ice</span> shelves driven by changes in firn state. Basal melt rates near Bawden <span class="hlt">Ice</span> Rise, a major pinning point of Larsen C <span class="hlt">Ice</span> Shelf, showed large increases, potentially leading to substantial loss of buttressing if sustained.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19..187K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19..187K"><span>Last Glacial-Interglacial Transition <span class="hlt">ice</span> dynamics in the Wicklow Mountains, Ireland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Knight, Lauren; Boston, Clare; Lovell, Harold; Pepin, Nick</p> <p>2017-04-01</p> <p>Understanding of the extent and dynamics of former <span class="hlt">ice</span> <span class="hlt">masses</span> in the Wicklow Mountains, Ireland, during the Last Glacial-Interglacial Transition (LGIT; 15-10 ka BP) is currently unresolved. Whilst it is acknowledged that the region hosted a local <span class="hlt">ice</span> cap within the larger British-Irish <span class="hlt">Ice</span> Sheet at the Last Glacial Maximum (LGM; 27 ka BP), there has been little consideration of <span class="hlt">ice</span> cap disintegration to a topographically constrained <span class="hlt">ice</span> <span class="hlt">mass</span> during the LGIT. This research has produced the first regional glacial geomorphological map, through remote sensing (aerial photograph and digital terrain model interrogation) and field mapping. This has allowed both the style and extent of mountain glaciation and <span class="hlt">ice</span> recession dynamics during the LGIT to be established. This geomorphological mapping has highlighted that evidence for local glaciation in the Wicklow Mountains is more extensive than previously recognised, and that small icefields and associated outlet valley glaciers existed during the LGIT following disintegration of the Wicklow <span class="hlt">Ice</span> Cap. A relative chronology based on morphostratigraphic principles is developed, which indicates complex patterns of <span class="hlt">ice</span> <span class="hlt">mass</span> oscillation characterised by periods of both sustained retreat and minor readvance. Variations in the pattern of recession across the Wicklow Mountains are evident and appear to be influenced, in part, by topographic controls (e.g. slope, aspect, glacier hypsometry). In summary, this research establishes a relative chronology of glacial events in the region during the LGIT and presents constraints on <span class="hlt">ice</span> <span class="hlt">mass</span> extent, dynamics and retreat patterns, offering an insight into small <span class="hlt">ice</span> <span class="hlt">mass</span> behaviour in a warming climate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.P31A2080G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.P31A2080G"><span>Do Europa's Mountains Have Roots? Erosion of Topography at the <span class="hlt">Ice</span>-Water Interface via the "<span class="hlt">Ice</span> Pump"</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goodman, J. C.</p> <p>2016-12-01</p> <p>Are topographic features on the surface of Europa and other icy worlds isostatically compensated by variations in shell thickness (Airy isostasy)? This is only possible if variations in shell thickness can remain stable over geologic time. Here we show that melting and freezing driven by the pressure dependence of the melting point of water - the "<span class="hlt">ice</span> pump" - can rapidly erase topography at the <span class="hlt">ice</span>/water interface. We consider <span class="hlt">ice</span> pumps driven by both tidal action and buoyancy-driven flow. We first show that as tidal action drives the ocean up and down along a sloping interface, <span class="hlt">ice</span> will be melted from areas where it's thickest and deposited where the <span class="hlt">ice</span> is thinnest. We show that this process causes the <span class="hlt">ice</span> interface topography to relax according to a simple "diffusion" linear partial differential equation. We estimate that a 10-km-wide topographic feature would be erased by the tidal <span class="hlt">ice</span> pump in 3000 years if Europa's tidal current amplitude is 1 cm/s; however, this timescale is inversely proportional to the cube of the tidal velocity! Next, we consider an <span class="hlt">ice</span> pump powered by ascent of meltwater along a sloping <span class="hlt">ice</span>-water interface. We consider layer-averaged budgets for heat, <span class="hlt">mass</span>, and momentum, along with turbulent mixing of the meltwater layer with underlying seawater via a Richardson number dependent entrainment process, and use these to estimate the thickness and <span class="hlt">mass</span> flux of the meltwater layer. From this we estimate the rate of melting and freezing at the interface. These two <span class="hlt">ice</span> pump processes combine with the glacial flow of warm basal <span class="hlt">ice</span> to rapidly flatten out any variations in the height of the <span class="hlt">ice</span>-water interface: Europa's <span class="hlt">ice</span>/water interface may be perfectly flat! If so, topography at Europa's surface can only be supported by variations in density of the shell or the strength of the brittle surface <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3997805','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3997805"><span>Marine <span class="hlt">ice</span> regulates the future stability of a large Antarctic <span class="hlt">ice</span> shelf</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Kulessa, Bernd; Jansen, Daniela; Luckman, Adrian J.; King, Edward C.; Sammonds, Peter R.</p> <p>2014-01-01</p> <p>The collapses of the Larsen A and B <span class="hlt">ice</span> shelves on the Antarctic Peninsula in 1995 and 2002 confirm the impact of southward-propagating climate warming in this region. Recent <span class="hlt">mass</span> and dynamic changes of Larsen B’s southern neighbour Larsen C, the fourth largest <span class="hlt">ice</span> shelf in Antarctica, may herald a similar instability. Here, using a validated <span class="hlt">ice</span>-shelf model run in diagnostic mode, constrained by satellite and in situ geophysical data, we identify the nature of this potential instability. We demonstrate that the present-day spatial distribution and orientation of the principal stresses within Larsen C <span class="hlt">ice</span> shelf are akin to those within pre-collapse Larsen B. When Larsen B’s stabilizing frontal portion was lost in 1995, the unstable remaining shelf accelerated, crumbled and ultimately collapsed. We hypothesize that Larsen C <span class="hlt">ice</span> shelf may suffer a similar fate if it were not stabilized by warm and mechanically soft marine <span class="hlt">ice</span>, entrained within narrow suture zones. PMID:24751641</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_17 --> <div id="page_18" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="341"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AAS...23135437M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AAS...23135437M"><span>Probing the Origin and Evolution of Interstellar and Protoplanetary Biogenic <span class="hlt">Ices</span> with SPHEREx</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Melnick, Gary; SPHEREx Science Team</p> <p>2018-01-01</p> <p>Many of the most important building blocks of life are locked in interstellar and protoplanetary <span class="hlt">ices</span>. Examples include H2O, CO, CO2, and CH3OH, among others. There is growing evidence that within the cores of dense molecular clouds and the mid-plane of protoplanetary disks the abundance of these species in <span class="hlt">ices</span> far exceeds that in the gas phase. As a result, collisions between <span class="hlt">ice</span>-bearing bodies and newly forming planets are thought to be a major means of delivering these key species to young planets. There currently exist fewer than 250 <span class="hlt">ice</span> absorption spectra toward Galactic molecular clouds, which is insufficient to reliably trace the <span class="hlt">ice</span> <span class="hlt">content</span> of clouds through the various evolutionary stages of collapse to form stars and planets. Likewise, the current number of spectra is inadequate to assess the effects of environment, such as cloud density and temperature, presence or absence of embedded sources, external FUV and X-ray radiation, gas-phase composition, or cosmic-ray ionization rate, on the <span class="hlt">ice</span> composition of clouds at similar stages of evolution. Ultimately, our goal is to understand how these findings connect to our own Solar System.SPHEREx will be a game changer for the study of interstellar, circumstellar, and protoplanetary disk <span class="hlt">ices</span>. SPHEREx will obtain spectra over the entire sky in the optical and near-IR, including the 2.5 to 5.0 micron region, which contains the above biogenic <span class="hlt">ice</span> features. SPHEREx will detect millions of potential background continuum point sources already catalogued by NASA’s Wide-field Infrared Survey Explorer (WISE) at 3.4 and 4.6 microns for which there is evidence for intervening gas and dust based on the 2<span class="hlt">MASS</span>+WISE colors with sufficient sensitivity to yield <span class="hlt">ice</span> absorption spectra with SNR ≥ 100 per spectral resolution element. The resulting > 100-fold increase in the number of high-quality <span class="hlt">ice</span> absorption spectra toward a wide variety of regions distributed throughout the Galaxy will reveal correlations between <span class="hlt">ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22836643','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22836643"><span>Relation of fat-<span class="hlt">mass</span> and obesity-associated gene polymorphism to fat <span class="hlt">mass</span> <span class="hlt">content</span> and body <span class="hlt">mass</span> index in obese children.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pyrzak, Beata; Wisniewska, Alicja; Majcher, Anna; Tysarowski, Andrzej; Demkow, Urszula</p> <p>2013-01-01</p> <p>Fat <span class="hlt">mass</span> <span class="hlt">content</span>, fat distribution, and fat-<span class="hlt">mass</span> and obesity associated (FTO) gene have been reported among a broad spectrum of genetic variation connected with body weight. The aim of our study was to investigate whether the T/A rs9939609 polymorphism of the FTO gene may influence obesity and metabolic indices in children. A 160 children were examined (136 obese and 24 non-obese). The anthropometric measurements and calculations included: height, weight, waist and hip circumference, sum of the thickness of 3 and 10 skin folds, % of fat <span class="hlt">content</span>, % FAT- BIA , % LBM-BIA. BMI, SDS of BMI, WHR, and WHtR. Fasting plasma total cholesterol (TC), HDL and LDL-cholesterol, triglycerides (TG), oral glucose tolerance test (OGTT), and HOMA-IR were analyzed and the blood pressure were measured. The rs9939609 polymorphism of FTO gene was genotyped by allele-specific real-time polymerase chain- reaction (RT-PCR). We found that the mean concentrations of TC, TG, LDLC, and HOMA-IR were significantly higher, and HDL was lower in the obese than in non-obese children. The presence of TT, but not AA alleles, related to the percentage of fat <span class="hlt">content</span>, BMI, and z-score of BMI. None of the other anthropometric indices did differ between the children with gene polymorphism and wild homozygous. In conclusion, rs9939609 polymorphism in the fat-<span class="hlt">mass</span> and obesity-associated gene is associated with BMI and the percent of fat <span class="hlt">content</span> in children.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.A33C0234Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.A33C0234Y"><span>Minimalist model of <span class="hlt">ice</span> microphysics in mixed-phase stratiform clouds</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, F.; Ovchinnikov, M.; Shaw, R. A.</p> <p>2013-12-01</p> <p>The question of whether persistent <span class="hlt">ice</span> crystal precipitation from supercooled layer clouds can be explained by time-dependent, stochastic <span class="hlt">ice</span> nucleation is explored using an approximate, analytical model and a large-eddy simulation (LES) cloud model. The updraft velocity in the cloud defines an accumulation zone, where small <span class="hlt">ice</span> particles cannot fall out until they are large enough, which will increase the residence time of <span class="hlt">ice</span> particles in the cloud. <span class="hlt">Ice</span> particles reach a quasi-steady state between growth by vapor deposition and fall speed at cloud base. The analytical model predicts that <span class="hlt">ice</span> water <span class="hlt">content</span> (wi) has a 2.5 power-law relationship with <span class="hlt">ice</span> number concentration (ni). wi and ni from a LES cloud model with stochastic <span class="hlt">ice</span> nucleation confirm the 2.5 power-law relationship, and initial indications of the scaling law are observed in data from the Indirect and Semi-Direct Aerosol Campaign. The prefactor of the power law is proportional to the <span class="hlt">ice</span> nucleation rate and therefore provides a quantitative link to observations of <span class="hlt">ice</span> microphysical properties. <span class="hlt">Ice</span> water <span class="hlt">content</span> (wi) and <span class="hlt">ice</span> number concentration (ni) relationship from LES. a and c: Accumulation zone region; b and d: Selective accumulation zone region. Black lines in c and d are best fitted 2.5 slope lines. Colors in Figures a and b represent updraft velocity, while colors in c and d represent altitude. The cloud base and top are at about 600 m and 800 m, respectively. <span class="hlt">Ice</span> water <span class="hlt">content</span> (wi) and <span class="hlt">ice</span> number concentration (ni) relationship for two <span class="hlt">ice</span> nucleation rates. Blue points are from LES with low <span class="hlt">ice</span> nucleation rate and red points with high <span class="hlt">ice</span> nucleation rate. Solid and dashed lines are best fitted 2.5 slope lines.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2791593','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2791593"><span>The future of <span class="hlt">ice</span> sheets and sea <span class="hlt">ice</span>: Between reversible retreat and unstoppable loss</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Notz, Dirk</p> <p>2009-01-01</p> <p>We discuss the existence of cryospheric “tipping points” in the Earth's climate system. Such critical thresholds have been suggested to exist for the disappearance of Arctic sea <span class="hlt">ice</span> and the retreat of <span class="hlt">ice</span> sheets: Once these <span class="hlt">ice</span> <span class="hlt">masses</span> have shrunk below an anticipated critical extent, the ice–albedo feedback might lead to the irreversible and unstoppable loss of the remaining <span class="hlt">ice</span>. We here give an overview of our current understanding of such threshold behavior. By using conceptual arguments, we review the recent findings that such a tipping point probably does not exist for the loss of Arctic summer sea <span class="hlt">ice</span>. Hence, in a cooler climate, sea <span class="hlt">ice</span> could recover rapidly from the loss it has experienced in recent years. In addition, we discuss why this recent rapid retreat of Arctic summer sea <span class="hlt">ice</span> might largely be a consequence of a slow shift in <span class="hlt">ice</span>-thickness distribution, which will lead to strongly increased year-to-year variability of the Arctic summer sea-<span class="hlt">ice</span> extent. This variability will render seasonal forecasts of the Arctic summer sea-<span class="hlt">ice</span> extent increasingly difficult. We also discuss why, in contrast to Arctic summer sea <span class="hlt">ice</span>, a tipping point is more likely to exist for the loss of the Greenland <span class="hlt">ice</span> sheet and the West Antarctic <span class="hlt">ice</span> sheet. PMID:19884496</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.C23E0542F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.C23E0542F"><span>Validation and Interpretation of a New Sea <span class="hlt">Ice</span> Globice Dataset Using Buoys and the Cice Sea <span class="hlt">Ice</span> Model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Flocco, D.; Laxon, S. W.; Feltham, D. L.; Haas, C.</p> <p>2011-12-01</p> <p>The Glob<span class="hlt">Ice</span> project has provided high resolution sea <span class="hlt">ice</span> product datasets over the Arctic derived from SAR data in the ESA archive. The products are validated sea <span class="hlt">ice</span> motion, deformation and fluxes through straits. Glob<span class="hlt">Ice</span> sea <span class="hlt">ice</span> velocities, deformation data and sea <span class="hlt">ice</span> concentration have been validated using buoy data provided by the International Arctic Buoy Program (IABP). Over 95% of the Glob<span class="hlt">Ice</span> and buoy data analysed fell within 5 km of each other. The Glob<span class="hlt">Ice</span> Eulerian image pair product showed a high correlation with buoy data. The sea <span class="hlt">ice</span> concentration product was compared to SSM/I data. An evaluation of the validity of the Glob<span class="hlt">ICE</span> data will be presented in this work. Glob<span class="hlt">ICE</span> sea <span class="hlt">ice</span> velocity and deformation were compared with runs of the CICE sea <span class="hlt">ice</span> model: in particular the <span class="hlt">mass</span> fluxes through the straits were used to investigate the correlation between the winter behaviour of sea <span class="hlt">ice</span> and the sea <span class="hlt">ice</span> state in the following summer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C33C0838L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C33C0838L"><span>Deglaciation-induced uplift of the Petermann glacier <span class="hlt">ice</span> margin observed with InSAR</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lu, Q.; Amelung, F.; Wdowinski, S.</p> <p>2016-12-01</p> <p>The Greenland <span class="hlt">ice</span> sheet is rapidly shrinking with the fastest retreat and thinning occurring at the <span class="hlt">ice</span> sheet margin and near the outlet glaciers. The changes of the <span class="hlt">ice</span> <span class="hlt">mass</span> cause an elastic response of the bedrock. <span class="hlt">Ice</span> <span class="hlt">mass</span> loss during the summer months is associated with uplift, whereas <span class="hlt">ice</span> <span class="hlt">mass</span> increase during the winter months is associated with subsidence.The German TerraSAR-X and TanDEM-X satellites have systematically observed selected sites along the Greenland Petermann <span class="hlt">ice</span> sheet margin since summer 2012. Here we present ground deformation observations obtained using an InSAR time-series approach based on small baseline interferograms. We observed rapid deglaciation-induced uplift on naked bedrock near the Petermann glacier <span class="hlt">ice</span> margin Deformation observed by InSAR is consistent with GPS vertical observations. The time series displacement data reveal not only net uplift but also the seasonal variations. There is no strong relative between displacement changes and SMB <span class="hlt">ice</span> <span class="hlt">mass</span> change. The seasonal variations in local area may caused by both nearby SMB changes and <span class="hlt">ice</span> dynamic changes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20030111522&hterms=Molas&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DMolas','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20030111522&hterms=Molas&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DMolas"><span>The Enhancement of Water <span class="hlt">Ice</span> <span class="hlt">Content</span> in the Local Area Northeast of Arcadia Planitia: Evidence from Neutron Data from HEND (Mars Odyssey) and Elevation from MOLA (MGS)</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sanin, A. B.; Mitrofanov, I. G.; Kozyrev, A. S.; Litvak, M. L.; Tretyakov, V.; Smith, D. E.; Zuber, M. T.; Boynton, W.; Saunders, R. S.</p> <p>2003-01-01</p> <p>The first year of neutron mapping measurements from the Mars Odyssey spacecraft revealed enormous hydrogen-rich regions in the southern and northern hemispheres of the Martian crust that imply significant amounts of near surface water <span class="hlt">ice</span>. The hydrogen-rich areas of the southern and northern regions appear generally comparable in spatial extent and water <span class="hlt">ice</span> <span class="hlt">content</span>. This observation is interesting in light of topography measured by the Mars Orbiter Laser Altimeter (MOLA) on the Mars Global Surveyor (MGS) spacecraft, which shows a significant difference in elevation between northern lowlands and southern highlands that could imply a difference in seasonal CO2 condensation. In this study we correlate the high energy neutron flux observed by HEND (Mars Odyssey) and surface elevation measured by MOLA in order to interpret the seasonal change in epithermal neutron flux in terms near-surface water <span class="hlt">ice</span> <span class="hlt">content</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A33M..02W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A33M..02W"><span>Upper-Tropospheric Cloud <span class="hlt">Ice</span> from <span class="hlt">Ice</span>Cube</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wu, D. L.</p> <p>2017-12-01</p> <p>Cloud <span class="hlt">ice</span> plays important roles in Earth's energy budget and cloud-precipitation processes. Knowledge of global cloud <span class="hlt">ice</span> and its properties is critical for understanding and quantifying its roles in Earth's atmospheric system. It remains a great challenge to measure these variables accurately from space. Submillimeter (submm) wave remote sensing has capability of penetrating clouds and measuring <span class="hlt">ice</span> <span class="hlt">mass</span> and microphysical properties. In particular, the 883-GHz frequency is a highest spectral window in microwave frequencies that can be used to fill a sensitivity gap between thermal infrared (IR) and mm-wave sensors in current spaceborne cloud <span class="hlt">ice</span> observations. <span class="hlt">Ice</span>Cube is a cubesat spaceflight demonstration of 883-GHz radiometer technology. Its primary objective is to raise the technology readiness level (TRL) of 883-GHz cloud radiometer for future Earth science missions. By flying a commercial receiver on a 3U cubesat, <span class="hlt">Ice</span>Cube is able to achieve fast-track maturation of space technology, by completing its development, integration and testing in 2.5 years. <span class="hlt">Ice</span>Cube was successfully delivered to ISS in April 2017 and jettisoned from the International Space Station (ISS) in May 2017. The <span class="hlt">Ice</span>Cube cloud-<span class="hlt">ice</span> radiometer (ICIR) has been acquiring data since the jettison on a daytime-only operation. <span class="hlt">Ice</span>Cube adopted a simple design without payload mechanism. It makes maximum utilization of solar power by spinning the spacecraft continuously about the Sun vector at a rate of 1.2° per second. As a result, the ICIR is operated under the limited resources (8.6 W without heater) and largely-varying (18°C-28°C) thermal environments. The spinning cubesat also allows ICIR to have periodical views between the Earth (atmosphere and clouds) and cold space (calibration), from which the first 883-GHz cloud map is obtained. The 883-GHz cloud radiance, sensitive to <span class="hlt">ice</span> particle scattering, is proportional to cloud <span class="hlt">ice</span> amount above 10 km. The ICIR cloud map acquired during June 20-July 2</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19970040868&hterms=feather&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dfeather','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19970040868&hterms=feather&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dfeather"><span>Implementation of Combined Feather and Surface-Normal <span class="hlt">Ice</span> Growth Models in LEWICE/X</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Velazquez, M. T.; Hansman, R. J., Jr.</p> <p>1995-01-01</p> <p>Experimental observations have shown that discrete rime <span class="hlt">ice</span> growths called feathers, which grow in approximately the direction of water droplet impingement, play an important role in the growth of <span class="hlt">ice</span> on accreting surfaces for some thermodynamic conditions. An improved physical model of <span class="hlt">ice</span> accretion has been implemented in the LEWICE 2D panel-based <span class="hlt">ice</span> accretion code maintained by the NASA Lewis Research Center. The LEWICE/X model of <span class="hlt">ice</span> accretion explicitly simulates regions of feather growth within the framework of the LEWICE model. Water droplets impinging on an accreting surface are withheld from the normal LEWICE <span class="hlt">mass</span>/energy balance and handled in a separate routine; <span class="hlt">ice</span> growth resulting from these droplets is performed with enhanced convective heat transfer approximately along droplet impingement directions. An independent underlying <span class="hlt">ice</span> shape is grown along surface normals using the unmodified LEWICE method. The resulting dual-surface <span class="hlt">ice</span> shape models roughness-induced feather growth observed in <span class="hlt">icing</span> wind tunnel tests. Experiments indicate that the exact direction of feather growth is dependent on external conditions. Data is presented to support a linear variation of growth direction with temperature and cloud water <span class="hlt">content</span>. Test runs of LEWICE/X indicate that the sizes of surface regions containing feathers are influenced by initial roughness element height. This suggests that a previous argument that feather region size is determined by boundary layer transition may be incorrect. Simulation results for two typical test cases give improved shape agreement over unmodified LEWICE.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1208720-molecular-simulations-heterogeneous-ice-nucleation-controlling-ice-nucleation-through-surface-hydrophilicity','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1208720-molecular-simulations-heterogeneous-ice-nucleation-controlling-ice-nucleation-through-surface-hydrophilicity"><span>Molecular simulations of heterogeneous <span class="hlt">ice</span> nucleation. I. Controlling <span class="hlt">ice</span> nucleation through surface hydrophilicity</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>Cox, Stephen J.; Kathmann, Shawn M.; Slater, B.</p> <p>2015-05-14</p> <p><span class="hlt">Ice</span> formation is one of the most common and important processes on earth and almost always occurs at the surface of a material. A basic understanding of how the physicochemical properties of a material’s surface affect its ability to form <span class="hlt">ice</span> has remained elusive. Here, we use molecular dynamics simulations to directly probe heterogeneous <span class="hlt">ice</span> nucleation at a hexagonal surface of a nanoparticle of varying hydrophilicity. Surprisingly, we find that structurally identical surfaces can both inhibit and promote <span class="hlt">ice</span> formation and analogous to a chemical catalyst, it is found that an optimal interaction between the surface and the water existsmore » for promoting <span class="hlt">ice</span> nucleation.We use our microscopic understanding of the mechanism to design a modified surface in silico with enhanced <span class="hlt">ice</span> nucleating ability. C 2015 Author(s). All article <span class="hlt">content</span>, except where otherwise noted, is licensed under a Creative Commons Attribution 3.0 Unported License.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28973875','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28973875"><span>Katabatic winds diminish precipitation contribution to the Antarctic <span class="hlt">ice</span> <span class="hlt">mass</span> balance.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Grazioli, Jacopo; Madeleine, Jean-Baptiste; Gallée, Hubert; Forbes, Richard M; Genthon, Christophe; Krinner, Gerhard; Berne, Alexis</p> <p>2017-10-10</p> <p>Snowfall in Antarctica is a key term of the <span class="hlt">ice</span> sheet <span class="hlt">mass</span> budget that influences the sea level at global scale. Over the continental margins, persistent katabatic winds blow all year long and supply the lower troposphere with unsaturated air. We show that this dry air leads to significant low-level sublimation of snowfall. We found using unprecedented data collected over 1 year on the coast of Adélie Land and simulations from different atmospheric models that low-level sublimation accounts for a 17% reduction of total snowfall over the continent and up to 35% on the margins of East Antarctica, significantly affecting satellite-based estimations close to the ground. Our findings suggest that, as climate warming progresses, this process will be enhanced and will limit expected precipitation increases at the ground level.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20070035753','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20070035753"><span>Validation and Determination of <span class="hlt">Ice</span> Water <span class="hlt">Content</span> - Radar Reflectivity Relationships during CRYSTAL-FACE: Flight Requirements for Future Comparisons</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sayres, D. S.; Smith, J. B.; Pittman, J. V.; Weinstock, E. M.; Anderson, J. G.; Heymsfield, G.; Fridland, A. M.; Ackerman, A. S.</p> <p>2007-01-01</p> <p>In order for clouds to be more accurately represented in global circulation models (GCM), there is need for improved understanding of the properties of <span class="hlt">ice</span> such as the total water in <span class="hlt">ice</span> clouds, called <span class="hlt">ice</span> water <span class="hlt">content</span> (IWC), <span class="hlt">ice</span> particle sizes and their shapes. Improved representation of clouds in models will enable GCMs to better predict for example, how changes in emissions of pollutants affect cloud formation and evolution, upper tropospheric water vapor, and the radiative budget of the atmosphere that is crucial for climate change studies. An extensive cloud measurement campaign called CRYSTAL-FACE was conducted during Summer 2002 using instrumented aircraft and a variety of instruments to measure properties of <span class="hlt">ice</span> clouds. This paper deals with the measurement of IWC using the Harvard water vapor and total water instruments on the NASA WB-57 high-altitude aircraft. The IWC is measured directly by these instruments at the altitude of the WB-57, and it is compared with remote measurements from the Goddard Cloud Radar System (CRS) on the NASA ER-2. CRS measures vertical profiles of radar reflectivity from which IWC can be estimated at the WB-57 altitude. The IWC measurements obtained from the Harvard instruments and CRS were found to be within 20-30% of each other. Part of this difference was attributed to errors associated with comparing two measurements that are not collocated in time an space since both aircraft were not in identical locations. This study provides some credibility to the Harvard and CRS-derived IWC measurements that are in general difficult to validate except through consistency checks using different measurement approaches.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013Sci...341..266R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013Sci...341..266R"><span><span class="hlt">Ice</span>-Shelf Melting Around Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rignot, E.; Jacobs, S.; Mouginot, J.; Scheuchl, B.</p> <p>2013-07-01</p> <p>We compare the volume flux divergence of Antarctic <span class="hlt">ice</span> shelves in 2007 and 2008 with 1979 to 2010 surface accumulation and 2003 to 2008 thinning to determine their rates of melting and <span class="hlt">mass</span> balance. Basal melt of 1325 ± 235 gigatons per year (Gt/year) exceeds a calving flux of 1089 ± 139 Gt/year, making <span class="hlt">ice</span>-shelf melting the largest ablation process in Antarctica. The giant cold-cavity Ross, Filchner, and Ronne <span class="hlt">ice</span> shelves covering two-thirds of the total <span class="hlt">ice</span>-shelf area account for only 15% of net melting. Half of the meltwater comes from 10 small, warm-cavity Southeast Pacific <span class="hlt">ice</span> shelves occupying 8% of the area. A similar high melt/area ratio is found for six East Antarctic <span class="hlt">ice</span> shelves, implying undocumented strong ocean thermal forcing on their deep grounding lines.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.C13D..06G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.C13D..06G"><span>The response of grounded <span class="hlt">ice</span> to ocean temperature forcing in a coupled <span class="hlt">ice</span> sheet-<span class="hlt">ice</span> shelf-ocean cavity model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goldberg, D. N.; Little, C. M.; Sergienko, O. V.; Gnanadesikan, A.</p> <p>2010-12-01</p> <p><span class="hlt">Ice</span> shelves provide a pathway for the heat <span class="hlt">content</span> of the ocean to influence continental <span class="hlt">ice</span> sheets. Changes in the rate or location of basal melting can alter their geometry and effect changes in stress conditions at the grounding line, leading to a grounded <span class="hlt">ice</span> response. Recent observations of <span class="hlt">ice</span> streams and <span class="hlt">ice</span> shelves in the Amundsen Sea sector of West Antarctica have been consistent with this story. On the other hand, <span class="hlt">ice</span> dynamics in the grounding 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> sheet-<span class="hlt">ice</span> shelf, can be quite strong. We examine the response of the <span class="hlt">ice</span> sheet-<span class="hlt">ice</span> shelf-ocean cavity system to changes in ocean temperature using a recently developed coupled model. The coupled model consists a 3-D ocean model (GFDL's Generalized Ocean Layered Dynamics model, or GOLD) to a two-dimensional <span class="hlt">ice</span> sheet-<span class="hlt">ice</span> shelf model (Goldberg et al, 2009), and allows for changing cavity geometry and a migrating grounding line. Steady states of the coupled system are found even under considerable forcing. The <span class="hlt">ice</span> shelf morphology and basal melt rate patterns of the steady states exhibit detailed structure, and furthermore seem to be unique and robust. The relationship between temperature forcing and area-averaged melt rate is influenced by the response of <span class="hlt">ice</span> shelf morphology to thermal forcing, and is found to be sublinear in the range of forcing considered. However, results suggest that area-averaged melt rate is not the best predictor of overall system response, as grounding line stability depends on local aspects of the basal melt field. Goldberg, D N, D M Holland and C G Schoof, 2009. Grounding line movement and <span class="hlt">ice</span> shelf buttressing in marine <span class="hlt">ice</span> sheets, Journal of Geophysical Research-Earth Surfaces, 114, F04026.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016OcSci..12..507M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016OcSci..12..507M"><span>Turbulent heat transfer as a control of platelet <span class="hlt">ice</span> growth in supercooled under-<span class="hlt">ice</span> ocean boundary layers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McPhee, Miles G.; Stevens, Craig L.; Smith, Inga J.; Robinson, Natalie J.</p> <p>2016-04-01</p> <p>Late winter measurements of turbulent quantities in tidally modulated flow under land-fast sea <span class="hlt">ice</span> near the Erebus Glacier Tongue, McMurdo Sound, Antarctica, identified processes that influence growth at the interface of an <span class="hlt">ice</span> surface in contact with supercooled seawater. The data show that turbulent heat exchange at the ocean-<span class="hlt">ice</span> boundary is characterized by the product of friction velocity and (negative) water temperature departure from freezing, analogous to similar results for moderate melting rates in seawater above freezing. Platelet <span class="hlt">ice</span> growth appears to increase the hydraulic roughness (drag) of fast <span class="hlt">ice</span> compared with undeformed fast <span class="hlt">ice</span> without platelets. Platelet growth in supercooled water under thick <span class="hlt">ice</span> appears to be rate-limited by turbulent heat transfer and that this is a significant factor to be considered in <span class="hlt">mass</span> transfer at the underside of <span class="hlt">ice</span> shelves and sea <span class="hlt">ice</span> in the vicinity of <span class="hlt">ice</span> shelves.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-GSFC_20171208_Archive_e002001.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-GSFC_20171208_Archive_e002001.html"><span>Sea <span class="hlt">Ice</span> in McClure Strait</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2017-12-08</p> <p>NASA image acquired August 17, 2010 In mid-August 2010, the Northwest Passage was almost—but not quite—free of <span class="hlt">ice</span>. The <span class="hlt">ice</span> <span class="hlt">content</span> in the northern route through the passage (through the Western Parry Channel) was very light, but <span class="hlt">ice</span> remained in McClure (or M’Clure) Strait. The Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Terra satellite captured this natural-color image on August 17, 2010. Although most of McClure Strait looks perfectly <span class="hlt">ice</span>-free, immediately west of Prince Patrick Island, a band of sea <span class="hlt">ice</span> stretches southward across the strait (left edge of the image). The National Snow and <span class="hlt">Ice</span> Data Center Sea <span class="hlt">Ice</span> News and Analysis blog reported that even more <span class="hlt">ice</span> remained in the southern route (through Amundsen’s Passage) of the Northwest Passage in mid-August 2010. Nevertheless, the <span class="hlt">ice</span> <span class="hlt">content</span> in the northern route was not only well below the 1968–2000 average, but also nearly a month ahead of the clearing observed in 2007, when Arctic sea <span class="hlt">ice</span> set a record low. As of mid-August 2010, however, overall sea <span class="hlt">ice</span> extent was higher than it had been at the same time of year in 2007. Credit: NASA/GSFC/Jeff Schmaltz/MODIS Land Rapid Response Team Caption by Michon Scott. To learn more go to: earthobservatory.nasa.gov/NaturalHazards/view.php?id=45333 Instrument: Terra - MODIS NASA Goddard Space Flight Center is home to the nation's largest organization of combined scientists, engineers and technologists that build spacecraft, instruments and new technology to study the Earth, the sun, our solar system, and the universe. Follow us on Twitter Join us on Facebook Click here to see more images from NASA Goddard’s Earth Observatory</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22538614','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22538614"><span>Antarctic <span class="hlt">ice</span>-sheet loss driven by basal melting of <span class="hlt">ice</span> shelves.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pritchard, H D; Ligtenberg, S R M; Fricker, H A; Vaughan, D G; van den Broeke, M R; Padman, L</p> <p>2012-04-25</p> <p>Accurate prediction of global sea-level rise requires that we understand the cause of recent, widespread and intensifying glacier acceleration along Antarctic <span class="hlt">ice</span>-sheet coastal margins. Atmospheric and oceanic forcing have the potential to reduce the thickness and extent of floating <span class="hlt">ice</span> shelves, potentially limiting their ability to buttress the flow of grounded tributary glaciers. Indeed, recent <span class="hlt">ice</span>-shelf collapse led to retreat and acceleration of several glaciers on the Antarctic Peninsula. But the extent and magnitude of <span class="hlt">ice</span>-shelf thickness change, the underlying causes of such change, and its link to glacier flow rate are so poorly understood that its future impact on the <span class="hlt">ice</span> sheets cannot yet be predicted. Here we use satellite laser altimetry and modelling of the surface firn layer to reveal the circum-Antarctic pattern of <span class="hlt">ice</span>-shelf thinning through increased basal melt. We deduce that this increased melt is the primary control of Antarctic <span class="hlt">ice</span>-sheet loss, through a reduction in buttressing of the adjacent <span class="hlt">ice</span> sheet leading to accelerated glacier flow. The highest thinning rates occur where warm water at depth can access thick <span class="hlt">ice</span> shelves via submarine troughs crossing the continental shelf. Wind forcing could explain the dominant patterns of both basal melting and the surface melting and collapse of Antarctic <span class="hlt">ice</span> shelves, through ocean upwelling in the Amundsen and Bellingshausen seas, and atmospheric warming on the Antarctic Peninsula. This implies that climate forcing through changing winds influences Antarctic <span class="hlt">ice</span>-sheet <span class="hlt">mass</span> balance, and hence global sea level, on annual to decadal timescales.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C53C0787S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C53C0787S"><span>Development of a multi-sensor elevation time series pole-ward of 86°S in support of altimetry validation and <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balance studies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Studinger, M.; Brunt, K. M.; Casey, K.; Medley, B.; Neumann, T.; Manizade, S.; Linkswiler, M. A.</p> <p>2015-12-01</p> <p>In order to produce a cross-calibrated long-term record of <span class="hlt">ice</span>-surface elevation change for input into <span class="hlt">ice</span> sheet models and <span class="hlt">mass</span> balance studies it is necessary to "link the measurements made by airborne laser altimeters, satellite measurements of ICESat, ICESat-2, and CryoSat-2" [<span class="hlt">Ice</span>Bridge Level 1 Science Requirements, 2012] and determine the biases and the spatial variations between radar altimeters and laser altimeters using different wavelengths. The convergence zones of all ICESat tracks (86°S) and all ICESat-2 and CryoSat-2 tracks (88°S) are in regions of relatively low accumulation, making them ideal for satellite altimetry calibration. In preparation for ICESat-2 validation, the <span class="hlt">Ice</span>Bridge and ICESat-2 science teams have designed <span class="hlt">Ice</span>Bridge data acquisitions around 86°S and 88°S. Several aspects need to be considered when comparing and combining elevation measurements from different radar and laser altimeters, including: a) foot print size and spatial sampling pattern; b) accuracy and precision of each data sets; c) varying signal penetration into the snow; and d) changes in geodetic reference frames over time, such as the International Terrestrial Reference Frame (ITRF). The presentation will focus on the analysis of several <span class="hlt">Ice</span>Bridge flights around 86 and 88°S with the LVIS and ATM airborne laser altimeters and will evaluate the accuracy and precision of these data sets. To properly interpret the observed elevation change (dh/dt) as <span class="hlt">mass</span> change, however, the various processes that control surface elevation fluctuations must be quantified and therefore future work will quantify the spatial variability in snow accumulation rates pole-ward of 86°S and in particular around 88°S. Our goal is to develop a cross-validated multi-sensor time series of surface elevation change pole-ward of 86°S that, in combination with measured accumulation rates, will support ICESat-2 calibration and validation and <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balance studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JPhCS.718e2033R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JPhCS.718e2033R"><span>Cosmic ray spectrum and composition from three years of <span class="hlt">Ice</span>Top and <span class="hlt">Ice</span>Cube</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rawlins, K.; <author pre="for ">IceCube Collaboration</p> <p>2016-05-01</p> <p><span class="hlt">Ice</span>Top is the surface component of the <span class="hlt">Ice</span>Cube Observatory, composed of frozen water tanks at the top of <span class="hlt">Ice</span>Cube’s strings. Data from this detector can be analyzed in different ways with the goal of measuring cosmic ray spectrum and composition. The shower size S125 from <span class="hlt">Ice</span>Top alone can be used as a proxy for primary energy, and unfolded into an all-particle spectrum. In addition, S125 from the surface can be combined with high-energy muon energy loss information from the deep <span class="hlt">Ice</span>Cube detector for those air showers which pass through both. Using these coincident events in a complementary analysis, both the spectrum and <span class="hlt">mass</span> composition of primary cosmic rays can be extracted in parallel using a neural network. Both of these analyses have been performed on three years of <span class="hlt">Ice</span>Top and <span class="hlt">Ice</span>Cube data. Both all-particle spectra as well as individual spectra for elemental groups are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040035786&hterms=ships+location&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dships%2Blocation','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040035786&hterms=ships+location&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dships%2Blocation"><span>Studies of the Antarctic Sea <span class="hlt">Ice</span> Edges and <span class="hlt">Ice</span> Extents from Satellite and Ship Observations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Worby, Anthony P.; Comiso, Josefino C.</p> <p>2003-01-01</p> <p>Passive-microwave derived <span class="hlt">ice</span> edge locations in Antarctica are assessed against other satellite data as well as in situ observations of <span class="hlt">ice</span> edge location made between 1989 and 2000. The passive microwave data generally agree with satellite and ship data but the <span class="hlt">ice</span> concentration at the observed <span class="hlt">ice</span> edge varies greatly with averages of 14% for the TEAM algorithm and 19% for the Bootstrap algorithm. The comparisons of passive microwave with the field data show that in the <span class="hlt">ice</span> growth season (March - October) the agreement is extremely good, with r(sup 2) values of 0.9967 and 0.9797 for the Bootstrap and TEAM algorithms respectively. In the melt season however (November - February) the passive microwave <span class="hlt">ice</span> edge is typically 1-2 degrees south of the observations due to the low concentration and saturated nature of the <span class="hlt">ice</span>. Sensitivity studies show that these results can have significant impact on trend and <span class="hlt">mass</span> balance studies of the sea <span class="hlt">ice</span> cover in the Southern Ocean.</p> </li> </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/2015AGUFM.P53E2187S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.P53E2187S"><span>Geomorphological Evidence for Pervasive Ground <span class="hlt">Ice</span> on Ceres from Dawn Observations of Craters and Flows.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schmidt, B. E.; Chilton, H.; Hughson, K.; Scully, J. E. C.; Russell, C. T.; Sizemore, H. G.; Nathues, A.; Platz, T.; Bland, M. T.; Schenk, P.; Hiesinger, H.; Jaumann, R.; Byrne, S.; Schorghofer, N.; Ammannito, E.; Marchi, S.; O'Brien, D. P.; Sykes, M. V.; Le Corre, L.; Capria, M. T.; Reddy, V.; Raymond, C. A.; Mest, S. C.; Feldman, W. C.</p> <p>2015-12-01</p> <p>Five decades of observations of Ceres' albedo, surface composition, shape and density suggest that Ceres is comprised of both silicates and tens of percent of <span class="hlt">ice</span>. Historical suggestions of surficial hydrated silicates and evidence for water emission, coupled with its bulk density of ~2100 kg/m3 and Dawn observations of young craters containing high albedo spots support this conclusion. We report geomorphological evidence from survey data demonstrating that evaporative and fluid-flow processes within silicate-<span class="hlt">ice</span> mixtures are prevalent on Ceres, and indicate that its surface materials contain significant water <span class="hlt">ice</span>. Here we highlight three classes of features that possess strong evidence for ground <span class="hlt">ice</span>. First, ubiquitous scalloped and "breached" craters are characterized by <span class="hlt">mass</span> wasting and by the recession of crater walls in asymmetric patterns; these appear analogous to scalloped terrain on Mars and protalus lobes formed by <span class="hlt">mass</span> wasting in terrestrial glaciated regions. The degradation of crater walls appears to be responsible for the nearly complete removal of some craters, particularly at low latitudes. Second, several high latitude, high elevation craters feature lobed flows that emanate from cirque-shaped head walls and bear strikingly similar morphology to terrestrial rock glaciers. These similarities include lobate toes and indications of furrows and ridges consistent with <span class="hlt">ice</span>-cored or <span class="hlt">ice</span>-cemented material. Other lobed flows persist at the base of crater walls and <span class="hlt">mass</span> wasting features. Many flow features evidently terminate at ramparts. Third, there are frequent irregular domes, peaks and mounds within crater floors that depart from traditional crater central peaks or peak complexes. In some cases the irregular domes show evidence for high albedo or activity, and thus given other evidence for <span class="hlt">ice</span>, these could be due to local melt and extrusion via hydrologic gradients, forming domes similar to pingos. The global distribution of these classes of features</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120014316','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120014316"><span>Particle Trajectory and <span class="hlt">Icing</span> Analysis of the E(sup 3) Turbofan Engine Using LEWICE3D Version 3</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bidwell, Colin S.</p> <p>2011-01-01</p> <p>Particle trajectory and <span class="hlt">ice</span> shape calculations were made for the Energy Efficient Engine (E(sup 3)) using the LEWICE3D Version 3 software. The particle trajectory and <span class="hlt">icing</span> computations were performed using the new "block-to-block" collection efficiency method which has been incorporated into the LEWICE3D Version 3 software. The E(sup 3) was developed by NASA and GE in the early 1980 s as a technology demonstrator and is representative of a modern high bypass turbofan engine. The E(sup 3) flow field was calculated using the NASA Glenn ADPAC turbomachinery flow solver. Computations were performed for the low pressure compressor of the E(sup 3) for a Mach 0.8 cruise condition at 11,887 m assuming a standard warm day for three drop sizes and two drop distributions typically used in aircraft design and certification. Particle trajectory computations were made for water drop sizes of 5, 20, and 100 microns. Particle trajectory and <span class="hlt">ice</span> shape predictions were made for a 20 micron Langmuir-D distribution and for a 92 mm Super-cooled Large Droplet (SLD) distribution with and without splashing effects for a Liquid Water <span class="hlt">Content</span> (LWC) of 0.3 g/cu m and an <span class="hlt">icing</span> time of 30 min. The E3 fan and spinner combination proved to be an effective <span class="hlt">ice</span> removal mechanism as they removed greater than 36 percent of the <span class="hlt">mass</span> entering the inlet for the <span class="hlt">icing</span> cases. The maximum free stream catch fraction for the fan and spinner combination was 0.60 while that on the elements downstream of the fan was 0.03. The non-splashing trajectory and collection efficiency results showed that as drop size increased impingement rates increased on the spinner and fan leaving less <span class="hlt">mass</span> to impinge on downstream components. The SLD splashing case yielded more <span class="hlt">mass</span> downstream of the fan than the SLD non-splashing case due to <span class="hlt">mass</span> being splashed from the upstream inlet lip, spinner and fan components. The <span class="hlt">ice</span> shapes generated downstream of the fan were either small or nonexistent due to the small available <span class="hlt">mass</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4371949','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4371949"><span>Ocean-driven thinning enhances iceberg calving and retreat of Antarctic <span class="hlt">ice</span> shelves</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Liu, Yan; Moore, John C.; Cheng, Xiao; Gladstone, Rupert M.; Bassis, Jeremy N.; Liu, Hongxing; Wen, Jiahong; Hui, Fengming</p> <p>2015-01-01</p> <p>Iceberg calving from all Antarctic <span class="hlt">ice</span> shelves has never been directly measured, despite playing a crucial role in <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balance. Rapid changes to iceberg calving naturally arise from the sporadic detachment of large tabular bergs but can also be triggered by climate forcing. Here we provide a direct empirical estimate of <span class="hlt">mass</span> loss due to iceberg calving and melting from Antarctic <span class="hlt">ice</span> shelves. We find that between 2005 and 2011, the total <span class="hlt">mass</span> loss due to iceberg calving of 755 ± 24 gigatonnes per year (Gt/y) is only half the total loss due to basal melt of 1516 ± 106 Gt/y. However, we observe widespread retreat of <span class="hlt">ice</span> shelves that are currently thinning. Net <span class="hlt">mass</span> loss due to iceberg calving for these <span class="hlt">ice</span> shelves (302 ± 27 Gt/y) is comparable in magnitude to net <span class="hlt">mass</span> loss due to basal melt (312 ± 14 Gt/y). Moreover, we find that iceberg calving from these decaying <span class="hlt">ice</span> shelves is dominated by frequent calving events, which are distinct from the less frequent detachment of isolated tabular icebergs associated with <span class="hlt">ice</span> shelves in neutral or positive <span class="hlt">mass</span> balance regimes. Our results suggest that thinning associated with ocean-driven increased basal melt can trigger increased iceberg calving, implying that iceberg calving may play an overlooked role in the demise of shrinking <span class="hlt">ice</span> shelves, and is more sensitive to ocean forcing than expected from steady state calving estimates. PMID:25733856</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1914046W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1914046W"><span>Bayesian inference of <span class="hlt">ice</span> thickness from remote-sensing data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Werder, Mauro A.; Huss, Matthias</p> <p>2017-04-01</p> <p>Knowledge about <span class="hlt">ice</span> thickness and volume is indispensable for studying <span class="hlt">ice</span> dynamics, future sea-level rise due to glacier melt or their contribution to regional hydrology. Accurate measurements of glacier thickness require on-site work, usually employing radar techniques. However, these field measurements are time consuming, expensive and sometime downright impossible. Conversely, measurements of the <span class="hlt">ice</span> surface, namely elevation and flow velocity, are becoming available world-wide through remote sensing. The model of Farinotti et al. (2009) calculates <span class="hlt">ice</span> thicknesses based on a <span class="hlt">mass</span> conservation approach paired with shallow <span class="hlt">ice</span> physics using estimates of the surface <span class="hlt">mass</span> balance. The presented work applies a Bayesian inference approach to estimate the parameters of a modified version of this forward model by fitting it to both measurements of surface flow speed and of <span class="hlt">ice</span> thickness. The inverse model outputs <span class="hlt">ice</span> thickness as well the distribution of the error. We fit the model to ten test glaciers and <span class="hlt">ice</span> caps and quantify the improvements of thickness estimates through the usage of surface <span class="hlt">ice</span> flow measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20000025583','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20000025583"><span>LWC and Temperature Effects on <span class="hlt">Ice</span> Accretion Formation on Swept Wings at Glaze <span class="hlt">Ice</span> Conditions</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Vargas, Mario; Reshotko, Eli</p> <p>2000-01-01</p> <p>An experiment was conducted to study the effect of liquid water <span class="hlt">content</span> and temperature on the critical distance in <span class="hlt">ice</span> accretion formation on swept wings at glaze <span class="hlt">ice</span> conditions. The critical distance is defined as the distance from the attachment line to tile beginning of the zone where roughness elements develop into glaze <span class="hlt">ice</span> feathers. A baseline case of 150 mph, 25 F, 0.75 g/cu m. Cloud Liquid Water <span class="hlt">Content</span> (LWC) and 20 micrometers in Water Droplet Median Volume Diameter (MVD) was chosen. <span class="hlt">Icing</span> runs were performed on a NACA 0012 swept wing tip at 150 mph and MVD of 20 micrometers for liquid water <span class="hlt">contents</span> of 0.5 g/cu m, 0.75 g/cu m, and 1.0 g/cu m, and for total temperatures of 20 F, 25 F and 30 F. At each tunnel condition, the sweep angle was changed from 0 deg to 45 deg in 5 deg increments. Casting data, <span class="hlt">ice</span> shape tracings, and close-up photographic data were obtained. The results showed that decreasing the LWC to 0.5 g/cu m decreases the value of the critical distance at a given sweep angle compared to the baseline case, and starts the formation of complete scallops at 30 sweep angle. Increasing the LWC to 1.0 g/cu m increases the value of the critical distance compared to the baseline case, the critical distance remains always above 0 millimeters and complete scallops are not formed. Decreasing the total temperature to 20 F decreases the critical distance with respect to the baseline case and formation of complete scallops begins at 25 deg sweep angle. When the total temperature is increased to 30 F, bumps covered with roughness elements appear on the <span class="hlt">ice</span> accretion at 25 deg and 30 deg sweep angles, large <span class="hlt">ice</span> structures appear at 35 deg and 40 deg sweep angles, and complete scallops are formed at 45 deg sweep angle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080022412','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080022412"><span><span class="hlt">Ice</span>Val DatAssistant: An Interactive, Automated <span class="hlt">Icing</span> Data Management System</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Levinson, Laurie H.; Wright, William B.</p> <p>2008-01-01</p> <p>As with any scientific endeavor, the foundation of <span class="hlt">icing</span> research at the NASA Glenn Research Center (GRC) is the data acquired during experimental testing. In the case of the GRC <span class="hlt">Icing</span> Branch, an important part of this data consists of <span class="hlt">ice</span> tracings taken following tests carried out in the GRC <span class="hlt">Icing</span> Research Tunnel (IRT), as well as the associated operational and environmental conditions documented during these tests. Over the years, the large number of experimental runs completed has served to emphasize the need for a consistent strategy for managing this data. To address the situation, the <span class="hlt">Icing</span> Branch has recently elected to implement the <span class="hlt">Ice</span>Val DatAssistant automated data management system. With the release of this system, all publicly available IRT-generated experimental <span class="hlt">ice</span> shapes with complete and verifiable conditions have now been compiled into one electronically-searchable database. Simulation software results for the equivalent conditions, generated using the latest version of the LEWICE <span class="hlt">ice</span> shape prediction code, are likewise included and are linked to the corresponding experimental runs. In addition to this comprehensive database, the <span class="hlt">Ice</span>Val system also includes a graphically-oriented database access utility, which provides reliable and easy access to all data contained in the database. In this paper, the issues surrounding historical <span class="hlt">icing</span> data management practices are discussed, as well as the anticipated benefits to be achieved as a result of migrating to the new system. A detailed description of the software system features and database <span class="hlt">content</span> is also provided; and, finally, known issues and plans for future work are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20070031804','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20070031804"><span><span class="hlt">Ice</span>Val DatAssistant: An Interactive, Automated <span class="hlt">Icing</span> Data Management System</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Levinson, Laurie H.; Wright, William B.</p> <p>2008-01-01</p> <p>As with any scientific endeavor, the foundation of <span class="hlt">icing</span> research at the NASA Glenn Research Center (GRC) is the data acquired during experimental testing. In the case of the GRC <span class="hlt">Icing</span> Branch, an important part of this data consists of <span class="hlt">ice</span> tracings taken following tests carried out in the GRC <span class="hlt">Icing</span> Research Tunnel (IRT), as well as the associated operational and environmental conditions during those tests. Over the years, the large number of experimental runs completed has served to emphasize the need for a consistent strategy to manage the resulting data. To address this situation, the <span class="hlt">Icing</span> Branch has recently elected to implement the <span class="hlt">Ice</span>Val DatAssistant automated data management system. With the release of this system, all publicly available IRT-generated experimental <span class="hlt">ice</span> shapes with complete and verifiable conditions have now been compiled into one electronically-searchable database; and simulation software results for the equivalent conditions, generated using the latest version of the LEWICE <span class="hlt">ice</span> shape prediction code, are likewise included and linked to the corresponding experimental runs. In addition to this comprehensive database, the <span class="hlt">Ice</span>Val system also includes a graphically-oriented database access utility, which provides reliable and easy access to all data contained in the database. In this paper, the issues surrounding historical <span class="hlt">icing</span> data management practices are discussed, as well as the anticipated benefits to be achieved as a result of migrating to the new system. A detailed description of the software system features and database <span class="hlt">content</span> is also provided; and, finally, known issues and plans for future work are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19980151107','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19980151107"><span>West-Antarctic <span class="hlt">Ice</span> Streams: Analog to <span class="hlt">Ice</span> Flow in Channels on Mars</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lucchitta, B. K.</p> <p>1997-01-01</p> <p>Sounding of the sea floor in front of the Ross <span class="hlt">Ice</span> Shelf in Antarctica recently revealed large persistent patterns of longitudinal megaflutes and drumlinoid forms, which are interpreted to have formed at the base of <span class="hlt">ice</span> streams during the list glacial advance. The flutes bear remarkable resemblance to longitudinal grooves and highly elongated streamlined islands found on the floors of some large martian channels, called outflow channels. ln addition, other similarities exist between Antarctic <span class="hlt">ice</span> streams and outflow channels. <span class="hlt">Ice</span> streams are 30 to 80 km wide and hundreds of kilometers long, as are the martian channels. <span class="hlt">Ice</span> stream beds are below sea level. Floors of many martian outflow channels lie below martian datum, which may have been close to or below past martian sea levels. The Antarctic <span class="hlt">ice</span> stream bed gradient is flat and locally may go uphill, and surface slopes are exceptionally low. So are gradients of martian channels. The depth to the bed in <span class="hlt">ice</span> streams is 1 to 1.5 km. At bankful stage, the depth of the fluid in outflow channels would have been 1 to 2 km. These similarities suggest that the martian outflow channels, whose origin is commonly attributed to gigantic catastrophic floods, were locally filled by <span class="hlt">ice</span> that left a conspicuous morphologic imprint. Unlike the West-Antarctic-<span class="hlt">ice</span> streams, which discharge <span class="hlt">ice</span> from an <span class="hlt">ice</span> sheet, <span class="hlt">ice</span> in the martian channels came from water erupting from the ground. In the cold martian environment, this water, if of moderate volume, would eventually freeze. Thus it may have formed <span class="hlt">icings</span> on springs, <span class="hlt">ice</span> dams and jams on constrictions in the channel path, or frozen pools. Given sufficient thickness and downhill surface gradient, these <span class="hlt">ice</span> <span class="hlt">masses</span> would have moved; and given the right conditions, they could have moved like Antarctic <span class="hlt">ice</span> streams.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17733504','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17733504"><span>Devon island <span class="hlt">ice</span> cap: core stratigraphy and paleoclimate.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Koerner, R M</p> <p>1977-04-01</p> <p>Valuable paleoclimatic information can be gained by studying the distribution of melt layers in deep <span class="hlt">ice</span> cores. A profile representing the percentage of <span class="hlt">ice</span> in melt layers in a core drilled from the Devon Island <span class="hlt">ice</span> cap plotted against both time and depth shows that the <span class="hlt">ice</span> cap has experienced a period of very warm summers since 1925, following a period of colder summers between about 1600 and 1925. The earlier period was coldest between 1680 and 1730. There is a high correlation between the melt-layer <span class="hlt">ice</span> percentage and the <span class="hlt">mass</span> balance of the <span class="hlt">ice</span> cap. The relation between them suggests that the <span class="hlt">ice</span> cap <span class="hlt">mass</span> balance was zero (accumulation equaled ablation) during the colder period but is negative in the present warmer one. There is no firm evidence of a present cooling trend in the summer conditions on the <span class="hlt">ice</span> cap. A comparison with the melt-layer <span class="hlt">ice</span> percentage in cores from the other major Canadian Arctic <span class="hlt">ice</span> caps shows that the variation of summer conditions found for the Devon Island <span class="hlt">ice</span> cap is representative for all the large <span class="hlt">ice</span> caps for about 90 percent of the time. There is also a good correlation between melt-layer percentage and summer sea-<span class="hlt">ice</span> conditions in the archipelago. This suggests that the search for the northwest passage was influenced by changing climate, with the 19th-century peak of the often tragic exploration coinciding with a period of very cold summers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007JGRC..11211013D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007JGRC..11211013D"><span>Influence of sea <span class="hlt">ice</span> cover and icebergs on circulation and water <span class="hlt">mass</span> formation in a numerical circulation model of the Ross Sea, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dinniman, Michael S.; Klinck, John M.; Smith, Walker O.</p> <p>2007-11-01</p> <p>Satellite imagery shows that there was substantial variability in the sea <span class="hlt">ice</span> extent in the Ross Sea during 2001-2003. Much of this variability is thought to be due to several large icebergs that moved through the area during that period. The effects of these changes in sea <span class="hlt">ice</span> on circulation and water <span class="hlt">mass</span> distributions are investigated with a numerical general circulation model. It would be difficult to simulate the highly variable sea <span class="hlt">ice</span> from 2001 to 2003 with a dynamic sea <span class="hlt">ice</span> model since much of the variability was due to the floating icebergs. Here, sea <span class="hlt">ice</span> concentration is specified from satellite observations. To examine the effects of changes in sea <span class="hlt">ice</span> due to iceberg C-19, simulations were performed using either climatological <span class="hlt">ice</span> concentrations or the observed <span class="hlt">ice</span> for that period. The heat balance around the Ross Sea Polynya (RSP) shows that the dominant term in the surface heat budget is the net exchange with the atmosphere, but advection of oceanic warm water is also important. The area average annual basal melt rate beneath the Ross <span class="hlt">Ice</span> Shelf is reduced by 12% in the observed sea <span class="hlt">ice</span> simulation. The observed sea <span class="hlt">ice</span> simulation also creates more High-Salinity Shelf Water. Another simulation was performed with observed sea <span class="hlt">ice</span> and a fixed iceberg representing B-15A. There is reduced advection of warm surface water during summer from the RSP into McMurdo Sound due to B-15A, but a much stronger reduction is due to the late opening of the RSP in early 2003 because of C-19.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA601787','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA601787"><span><span class="hlt">Mass</span> Balance of Multiyear Sea <span class="hlt">Ice</span> in the Southern Beaufort Sea</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2013-09-30</p> <p>model of MY <span class="hlt">ice</span> circulation, which is shown in Figure 1. In this model , we consider the Beaufort Sea to consist of four zones defined by mean drift...Arctic Regional Climate Model Simulation Project 3 International Arctic Buoy Program 4 Sea <span class="hlt">ice</span> Experiment - Dynamic Nature of the Arctic 5Cold...2 Table 2: Datasets compiled to date Geophysical data type Source Time period acquired Buoy tracks IABP 12 hrly position data 1978-2012 <span class="hlt">Ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1013710','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1013710"><span><span class="hlt">Mass</span> Balance of Multiyear Sea <span class="hlt">Ice</span> in the Southern Beaufort Sea</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2015-09-30</p> <p>1) Determination of the net growth and melt of multiyear (MY) sea <span class="hlt">ice</span> during its transit through the southern Beaufort Sea 2) Identification of...which we refer to as the FGIV dataset. Analysis of melt processes from <span class="hlt">ice</span> core and IMB data (Eicken) Through stratigraphic analysis of sea <span class="hlt">ice</span>...samples that are brought back to shore were melted and used to determine profiles of salinity and stable isotope ratios. These data allow us to identify</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GMD....11.1257N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GMD....11.1257N"><span>Intercomparison of Antarctic <span class="hlt">ice</span>-shelf, ocean, and sea-<span class="hlt">ice</span> interactions simulated by MetROMS-iceshelf and FESOM 1.4</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Naughten, Kaitlin A.; Meissner, Katrin J.; Galton-Fenzi, Benjamin K.; England, Matthew H.; Timmermann, Ralph; Hellmer, Hartmut H.; Hattermann, Tore; Debernard, Jens B.</p> <p>2018-04-01</p> <p>An increasing number of Southern Ocean models now include Antarctic <span class="hlt">ice</span>-shelf cavities, and simulate thermodynamics at the <span class="hlt">ice</span>-shelf/ocean interface. This adds another level of complexity to Southern Ocean simulations, as <span class="hlt">ice</span> shelves interact directly with the ocean and indirectly with sea <span class="hlt">ice</span>. Here, we present the first model intercomparison and evaluation of present-day ocean/sea-<span class="hlt">ice/ice</span>-shelf interactions, as simulated by two models: a circumpolar Antarctic configuration of MetROMS (ROMS: Regional Ocean Modelling System coupled to CICE: Community <span class="hlt">Ice</span> CodE) and the global model FESOM (Finite Element Sea-<span class="hlt">ice</span> Ocean Model), where the latter is run at two different levels of horizontal resolution. From a circumpolar Antarctic perspective, we compare and evaluate simulated <span class="hlt">ice</span>-shelf basal melting and sub-<span class="hlt">ice</span>-shelf circulation, as well as sea-<span class="hlt">ice</span> properties and Southern Ocean water <span class="hlt">mass</span> characteristics as they influence the sub-<span class="hlt">ice</span>-shelf processes. Despite their differing numerical methods, the two models produce broadly similar results and share similar biases in many cases. Both models reproduce many key features of observations but struggle to reproduce others, such as the high melt rates observed in the small warm-cavity <span class="hlt">ice</span> shelves of the Amundsen and Bellingshausen seas. Several differences in model design show a particular influence on the simulations. For example, FESOM's greater topographic smoothing can alter the geometry of some <span class="hlt">ice</span>-shelf cavities enough to affect their melt rates; this improves at higher resolution, since less smoothing is required. In the interior Southern Ocean, the vertical coordinate system affects the degree of water <span class="hlt">mass</span> erosion due to spurious diapycnal mixing, with MetROMS' terrain-following coordinate leading to more erosion than FESOM's z coordinate. Finally, increased horizontal resolution in FESOM leads to higher basal melt rates for small <span class="hlt">ice</span> shelves, through a combination of stronger circulation and small-scale intrusions of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28694490','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28694490"><span>Sea <span class="hlt">ice</span> breakup and marine melt of a retreating tidewater outlet glacier in northeast Greenland (81°N).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bendtsen, Jørgen; Mortensen, John; Lennert, Kunuk; K Ehn, Jens; Boone, Wieter; Galindo, Virginie; Hu, Yu-Bin; Dmitrenko, Igor A; Kirillov, Sergei A; Kjeldsen, Kristian K; Kristoffersen, Yngve; G Barber, David; Rysgaard, Søren</p> <p>2017-07-10</p> <p>Rising temperatures in the Arctic cause accelerated <span class="hlt">mass</span> loss from the Greenland <span class="hlt">Ice</span> Sheet and reduced sea <span class="hlt">ice</span> cover. Tidewater outlet glaciers represent direct connections between glaciers and the ocean where melt rates at the <span class="hlt">ice</span>-ocean interface are influenced by ocean temperature and circulation. However, few measurements exist near outlet glaciers from the northern coast towards the Arctic Ocean that has remained nearly permanently <span class="hlt">ice</span> covered. Here we present hydrographic measurements along the terminus of a major retreating tidewater outlet glacier from Flade Isblink <span class="hlt">Ice</span> Cap. We show that the region is characterized by a relatively large change of the seasonal freshwater <span class="hlt">content</span>, corresponding to ~2 m of freshwater, and that solar heating during the short open water period results in surface layer temperatures above 1 °C. Observations of temperature and salinity supported that the outlet glacier is a floating <span class="hlt">ice</span> shelf with near-glacial subsurface temperatures at the freezing point. Melting from the surface layer significantly influenced the <span class="hlt">ice</span> foot morphology of the glacier terminus. Hence, melting of the tidewater outlet glacier was found to be critically dependent on the retreat of sea <span class="hlt">ice</span> adjacent to the terminus and the duration of open water.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/14749827','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/14749827"><span>Enhanced <span class="hlt">ice</span> sheet growth in Eurasia owing to adjacent <span class="hlt">ice</span>-dammed lakes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Krinner, G; Mangerud, J; Jakobsson, M; Crucifix, M; Ritz, C; Svendsen, J I</p> <p>2004-01-29</p> <p>Large proglacial lakes cool regional summer climate because of their large heat capacity, and have been shown to modify precipitation through mesoscale atmospheric feedbacks, as in the case of Lake Agassiz. Several large <span class="hlt">ice</span>-dammed lakes, with a combined area twice that of the Caspian Sea, were formed in northern Eurasia about 90,000 years ago, during the last glacial period when an <span class="hlt">ice</span> sheet centred over the Barents and Kara seas blocked the large northbound Russian rivers. Here we present high-resolution simulations with an atmospheric general circulation model that explicitly simulates the surface <span class="hlt">mass</span> balance of the <span class="hlt">ice</span> sheet. We show that the main influence of the Eurasian proglacial lakes was a significant reduction of <span class="hlt">ice</span> sheet melting at the southern margin of the Barents-Kara <span class="hlt">ice</span> sheet through strong regional summer cooling over large parts of Russia. In our simulations, the summer melt reduction clearly outweighs lake-induced decreases in moisture and hence snowfall, such as has been reported earlier for Lake Agassiz. We conclude that the summer cooling mechanism from proglacial lakes accelerated <span class="hlt">ice</span> sheet growth and delayed <span class="hlt">ice</span> sheet decay in Eurasia and probably also in North America.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19878734','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19878734"><span>Intracellular <span class="hlt">ice</span> formation in insects: unresolved after 50 years?</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sinclair, Brent J; Renault, David</p> <p>2010-01-01</p> <p>Many insects survive internal <span class="hlt">ice</span> formation. The general model of freeze tolerance is of extracellular <span class="hlt">ice</span> formation (EIF) whereby <span class="hlt">ice</span> formation in the haemocoel leads to osmotic dehydration of the cells, whose <span class="hlt">contents</span> remain unfrozen. However, survivable intracellular <span class="hlt">ice</span> formation (IIF) has been reported in fat body and certain other cells of some insects. Although the cellular location of <span class="hlt">ice</span> has been determined only in vitro, several lines of evidence suggest that IIF occurs in vivo. Both cell-to-cell propagation of intracellular <span class="hlt">ice</span> and inoculation from the haemocoel may be important, although the route of <span class="hlt">ice</span> into the cell is unclear. It is unclear why some cells survive IIF and others do not, but it is suggested that the shape, size, and low water <span class="hlt">content</span> of fat body cells may predispose them towards surviving <span class="hlt">ice</span> formation. We speculate that IIF may reduce water loss in some freeze tolerant species, but there are too few data to build a strong conceptual model of the advantages of IIF. We suggest that new developments in microscopy and other forms of imaging may allow investigation of the cellular location of <span class="hlt">ice</span> in freeze tolerant insects in vivo.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20492279','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20492279"><span>Effect of solid fat <span class="hlt">content</span> on structure in <span class="hlt">ice</span> creams containing palm kernel oil and high-oleic sunflower oil.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sung, Kristine K; Goff, H Douglas</p> <p>2010-04-01</p> <p>The development of a structural fat network in <span class="hlt">ice</span> cream as influenced by the solid:liquid fat ratio at the time of freezing/whipping was investigated. The solid fat <span class="hlt">content</span> was varied with blends of a hard fraction of palm kernel oil (PKO) and high-oleic sunflower oil ranging from 40% to 100% PKO. Fat globule size and adsorbed protein levels in mix and overrun, fat destabilization, meltdown resistance, and air bubble size in <span class="hlt">ice</span> cream were measured. It was found that blends comprising 60% to 80% solid fat produced the highest rates of fat destabilization that could be described as partial coalescence (as opposed to coalescence), lowest rates of meltdown, and smallest air bubble sizes. Lower levels of solid fat produced fat destabilization that was better characterized as coalescence, leading to loss of structural integrity, whereas higher levels of solid fat led to lower levels of fat network formation and thus also to reduced structural integrity. Blends of highly saturated palm kernel oil and monounsaturated high-oleic sunflower oil were used to modify the solid:liquid ratio of fat blends used for <span class="hlt">ice</span> cream manufacture. Blends that contained 60% to 80% solid fat at freezing/whipping temperatures produced optimal structures leading to low rates of meltdown. This provides a useful reference for manufacturers to help in the selection of appropriate fat blends for nondairy-fat <span class="hlt">ice</span> cream.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70074767','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70074767"><span>Climatic impact of glacial cycle polar motion: Coupled oscillations of <span class="hlt">ice</span> sheet <span class="hlt">mass</span> and rotation pole position</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Bills, Bruce G.; James, Thomas S.; Mengel, John G.</p> <p>1999-01-01</p> <p>Precessional motion of Earth's rotation axis relative to its orbit is a well-known source of long-period climatic variation. It is less well appreciated that growth and decay of polar <span class="hlt">ice</span> sheets perturb the symmetry of the global <span class="hlt">mass</span> distribution enough that the geographic location of the rotation axis will change by at least 15 km and possibly as much as 100 km during a single glacial cycle. This motion of the pole will change the seasonal and latitudinal pattern of temperatures. We present calculations, based on a diurnal average energy balance, which compare the summer and winter temperature anomalies due to a 1° decrease in obliquity with those due to a 1° motion of the rotation pole toward Hudson Bay. Both effects result in peak temperature perturbations of about 1° Celsius. The obliquity change primarily influences the amplitude of the seasonal cycle, while the polar motion primarily changes the annual mean temperatures. The polar motion induced temperature anomaly is such that it will act as a powerful negative feedback on <span class="hlt">ice</span> sheet growth. We also explore the evolution of the coupled system composed of <span class="hlt">ice</span> sheet <span class="hlt">mass</span> and pole position. Oscillatory solutions result from the conflicting constraints of rotational and thermal stability. A positive <span class="hlt">mass</span> anomaly on an otherwise featureless Earth is in rotational equilibrium only at the poles or the equator. The two polar equilibria are rotationally unstable, and the equatorial equilibrium, though rotationally stable, is thermally unstable. We find that with a plausible choice for the strength of coupling between the thermal and rotational systems, relatively modest external forcing can produce significant response at periods of 104–106 years, but it strongly attenuates polar motion at longer periods. We suggest that these coupled oscillations may contribute to the observed dominance of 100 kyr glacial cycles since the mid-Pleistocene and will tend to stabilize geographic patterns that are suitable to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940008608','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940008608"><span><span class="hlt">ICE</span>/ISEE plasma wave data analysis</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Greenstadt, E. W.</p> <p>1992-01-01</p> <p>The interval reported on, from Jan. 1990 to Dec. 1991, has been one of continued processing and archiving of <span class="hlt">ICE</span> plasma wave (pw) data and transition from analysis of ISEE 3 and <span class="hlt">ICE</span> cometary data to <span class="hlt">ICE</span> data taken along its cruise trajectory, where coronal <span class="hlt">mass</span> ejections are the focus of attention. We have continued to examine with great interest the last year of ISEE 3's precomet phase, when it spent considerable time far downwind from Earth, recording conditions upstream, downstream, and across the very weak, distant flank bow shock. Among other motivations was the apparent similarity of some shock and post shock structures to the signatures of the bow wave surrounding comet Giacobini-Zinner, whose <span class="hlt">ICE</span>-phase data was revisited. While pursuing detailed, second-order scientific inquiries still pending from the late ISEE 3 recordings, we have also sought to position ourselves for study of CME's by instituting a data processing format new to the ISEE 3/<span class="hlt">ICE</span> pw detector. Processed detector output has always been summarized and archived in 24-hour segments, with all pw channels individually plotted and stacked one above the next down in frequency, with each channel calibrated separately to keep all data patterns equally visible in the plots, regardless of gross differences in energy <span class="hlt">content</span> at the various frequencies. Since CME's, with their preceding and following solar wind plasmas, can take more than one day to pass by the spacecraft, a more condensed synoptic view of the pw data is required to identify, let alone assess, CME characteristics than has been afforded by the traditional routines. This requirement is addressed in a major new processing initiative in the past two years. Besides our own ongoing and fresh investigations, we have cooperated, within our resources, with studies conducted extramurally by distant colleagues irrespective of the phase of the ISEE 3/<span class="hlt">ICE</span> mission under scrutiny. The remainder of this report summarizes our processing activities, our</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.G13B1098S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.G13B1098S"><span>An integrated approach for estimating global glacio isostatic adjustment, land <span class="hlt">ice</span>, hydrology and ocean <span class="hlt">mass</span> trends within a complete coupled Earth system framework</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schumacher, M.; Bamber, J. L.; Martin, A.</p> <p>2016-12-01</p> <p>Future sea level rise (SLR) is one of the most serious consequences of climate change. Therefore, understanding the drivers of past sea level change is crucial for improving predictions. SLR integrates many Earth system components including oceans, land <span class="hlt">ice</span>, terrestrial water storage, as well as solid Earth effects. Traditionally, each component have been tackled separately, which has often lead to inconsistencies between discipline-specific estimates of each part of the sea level budget. To address these issues, the European Research Council has funded a five year project aimed at producing a physically-based, data-driven solution for the complete coupled land-ocean-solid Earth system that is consistent with the full suite of observations, prior knowledge and fundamental geophysical constraints. The project is called "Global<span class="hlt">Mass</span>" and based at University of Bristol. Observed <span class="hlt">mass</span> movement from the GRACE mission plus vertical land motion from a global network of permanent GPS stations will be utilized in a data-driven approach to estimate glacial isostatic adjustment (GIA) without introducing any assumptions about the Earth structure or <span class="hlt">ice</span> loading history. A Bayesian Hierarchical Model (BHM) will be used as the framework to combine the satellite and in-situ observations alongside prior information that incorporates the physics of the coupled system such as conservation of <span class="hlt">mass</span> and characteristic length scales of different processes in both space and time. The BHM is used to implement a simultaneous solution at a global scale. It will produce a consistent partitioning of the integrated SLR signal into its steric (thermal) and barystatic (<span class="hlt">mass</span>) component for the satellite era. The latter component is induced by hydrological <span class="hlt">mass</span> trends and melting of land <span class="hlt">ice</span>. The BHM was developed and tested on Antarctica, where it has been used to separate surface, <span class="hlt">ice</span> dynamic and GIA signals simultaneously. We illustrate the approach and concepts with examples from this test case</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_19 --> <div id="page_20" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="381"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5642703','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5642703"><span>Katabatic winds diminish precipitation contribution to the Antarctic <span class="hlt">ice</span> <span class="hlt">mass</span> balance</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Grazioli, Jacopo; Madeleine, Jean-Baptiste; Gallée, Hubert; Forbes, Richard M.; Genthon, Christophe; Krinner, Gerhard; Berne, Alexis</p> <p>2017-01-01</p> <p>Snowfall in Antarctica is a key term of the <span class="hlt">ice</span> sheet <span class="hlt">mass</span> budget that influences the sea level at global scale. Over the continental margins, persistent katabatic winds blow all year long and supply the lower troposphere with unsaturated air. We show that this dry air leads to significant low-level sublimation of snowfall. We found using unprecedented data collected over 1 year on the coast of Adélie Land and simulations from different atmospheric models that low-level sublimation accounts for a 17% reduction of total snowfall over the continent and up to 35% on the margins of East Antarctica, significantly affecting satellite-based estimations close to the ground. Our findings suggest that, as climate warming progresses, this process will be enhanced and will limit expected precipitation increases at the ground level. PMID:28973875</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009QSRv...28.3101G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009QSRv...28.3101G"><span>Reconstructing the last Irish <span class="hlt">Ice</span> Sheet 2: a geomorphologically-driven model of <span class="hlt">ice</span> sheet growth, retreat and dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Greenwood, Sarah L.; Clark, Chris D.</p> <p>2009-12-01</p> <p>The <span class="hlt">ice</span> sheet that once covered Ireland has a long history of investigation. Much prior work focussed on localised evidence-based reconstructions and <span class="hlt">ice</span>-marginal dynamics and chronologies, with less attention paid to an <span class="hlt">ice</span> sheet wide view of the first order properties of the <span class="hlt">ice</span> sheet: centres of <span class="hlt">mass</span>, <span class="hlt">ice</span> divide structure, <span class="hlt">ice</span> flow geometry and behaviour and changes thereof. In this paper we focus on the latter aspect and use our new, countrywide glacial geomorphological mapping of the Irish landscape (>39 000 landforms), and our analysis of the palaeo-glaciological significance of observed landform assemblages (article Part 1), to build an <span class="hlt">ice</span> sheet reconstruction yielding these fundamental <span class="hlt">ice</span> sheet properties. We present a seven stage model of <span class="hlt">ice</span> sheet evolution, from initiation to demise, in the form of palaeo-geographic maps. An early incursion of <span class="hlt">ice</span> from Scotland likely coalesced with local <span class="hlt">ice</span> caps and spread in a south-westerly direction 200 km across Ireland. A semi-independent Irish <span class="hlt">Ice</span> Sheet was then established during <span class="hlt">ice</span> sheet growth, with a branching <span class="hlt">ice</span> divide structure whose main axis migrated up to 140 km from the west coast towards the east. <span class="hlt">Ice</span> stream systems converging on Donegal Bay in the west and funnelling through the North Channel and Irish Sea Basin in the east emerge as major flow components of the maximum stages of glaciation. <span class="hlt">Ice</span> cover is reconstructed as extending to the continental shelf break. The Irish <span class="hlt">Ice</span> Sheet became autonomous (i.e. separate from the British <span class="hlt">Ice</span> Sheet) during deglaciation and fragmented into multiple <span class="hlt">ice</span> <span class="hlt">masses</span>, each decaying towards the west. Final sites of demise were likely over the mountains of Donegal, Leitrim and Connemara. Patterns of growth and decay of the <span class="hlt">ice</span> sheet are shown to be radically different: asynchronous and asymmetric in both spatial and temporal domains. We implicate collapse of the <span class="hlt">ice</span> stream system in the North Channel - Irish Sea Basin in driving such asymmetry, since rapid</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70027302','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70027302"><span>DEM, tide and velocity over sulzberger <span class="hlt">ice</span> shelf, West Antarctica</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Baek, S.; Shum, C.K.; Lee, H.; Yi, Y.; Kwoun, Oh-Ig; Lu, Z.; Braun, Andreas</p> <p>2005-01-01</p> <p>Arctic and Antarctic <span class="hlt">ice</span> sheets preserve more than 77% of the global fresh water and could raise global sea level by several meters if completely melted. Ocean tides near and under <span class="hlt">ice</span> shelves shifts the grounding line position significantly and are one of current limitations to study glacier dynamics and <span class="hlt">mass</span> balance. The Sulzberger <span class="hlt">ice</span> shelf is an area of <span class="hlt">ice</span> <span class="hlt">mass</span> flux change in West Antarctica and has not yet been well studied. In this study, we use repeat-pass synthetic aperture radar (SAR) interferometry data from the ERS-1 and ERS-2 tandem missions for generation of a high-resolution (60-m) Digital Elevation Model (DEM) including tidal deformation detection and <span class="hlt">ice</span> stream velocity of the Sulzberger <span class="hlt">Ice</span> Shelf. Other satellite data such as laser altimeter measurements with fine foot-prints (70-m) from NASA's ICESat are used for validation and analyses. The resulting DEM has an accuracy of-0.57??5.88 m and is demonstrated to be useful for grounding line detection and <span class="hlt">ice</span> <span class="hlt">mass</span> balance studies. The deformation observed by InSAR is found to be primarily due to ocean tides and atmospheric pressure. The 2-D <span class="hlt">ice</span> stream velocities computed agree qualitatively with previous methods on part of the <span class="hlt">Ice</span> Shelf from passive microwave remote-sensing data (i.e., LANDSAT). ?? 2005 IEEE.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28518108','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28518108"><span>Identification of Plant <span class="hlt">Ice</span>-binding Proteins Through Assessment of <span class="hlt">Ice</span>-recrystallization Inhibition and Isolation Using <span class="hlt">Ice</span>-affinity Purification.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bredow, Melissa; Tomalty, Heather E; Walker, Virginia K</p> <p>2017-05-05</p> <p><span class="hlt">Ice</span>-binding proteins (IBPs) belong to a family of stress-induced proteins that are synthesized by certain organisms exposed to subzero temperatures. In plants, freeze damage occurs when extracellular <span class="hlt">ice</span> crystals grow, resulting in the rupture of plasma membranes and possible cell death. Adsorption of IBPs to <span class="hlt">ice</span> crystals restricts further growth by a process known as <span class="hlt">ice</span>-recrystallization inhibition (IRI), thereby reducing cellular damage. IBPs also demonstrate the ability to depress the freezing point of a solution below the equilibrium melting point, a property known as thermal hysteresis (TH) activity. These protective properties have raised interest in the identification of novel IBPs due to their potential use in industrial, medical and agricultural applications. This paper describes the identification of plant IBPs through 1) the induction and extraction of IBPs in plant tissue, 2) the screening of extracts for IRI activity, and 3) the isolation and purification of IBPs. Following the induction of IBPs by low temperature exposure, extracts are tested for IRI activity using a 'splat assay', which allows the observation of <span class="hlt">ice</span> crystal growth using a standard light microscope. This assay requires a low protein concentration and generates results that are quickly obtained and easily interpreted, providing an initial screen for <span class="hlt">ice</span> binding activity. IBPs can then be isolated from contaminating proteins by utilizing the property of IBPs to adsorb to <span class="hlt">ice</span>, through a technique called '<span class="hlt">ice</span>-affinity purification'. Using cell lysates collected from plant extracts, an <span class="hlt">ice</span> hemisphere can be slowly grown on a brass probe. This incorporates IBPs into the crystalline structure of the polycrystalline <span class="hlt">ice</span>. Requiring no a priori biochemical or structural knowledge of the IBP, this method allows for recovery of active protein. <span class="hlt">Ice</span>-purified protein fractions can be used for downstream applications including the identification of peptide sequences by <span class="hlt">mass</span> spectrometry and the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRC..123..324B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123..324B"><span>Multiphase Reactive Transport and Platelet <span class="hlt">Ice</span> Accretion in the Sea <span class="hlt">Ice</span> of McMurdo Sound, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Buffo, J. J.; Schmidt, B. E.; Huber, C.</p> <p>2018-01-01</p> <p>Sea <span class="hlt">ice</span> seasonally to interannually forms a thermal, chemical, and physical boundary between the atmosphere and hydrosphere over tens of millions of square kilometers of ocean. Its presence affects both local and global climate and ocean dynamics, <span class="hlt">ice</span> shelf processes, and biological communities. Accurate incorporation of sea <span class="hlt">ice</span> growth and decay, and its associated thermal and physiochemical processes, is underrepresented in large-scale models due to the complex physics that dictate oceanic <span class="hlt">ice</span> formation and evolution. Two phenomena complicate sea <span class="hlt">ice</span> simulation, particularly in the Antarctic: the multiphase physics of reactive transport brought about by the inhomogeneous solidification of seawater, and the buoyancy driven accretion of platelet <span class="hlt">ice</span> formed by supercooled <span class="hlt">ice</span> shelf water onto the basal surface of the overlying <span class="hlt">ice</span>. Here a one-dimensional finite difference model capable of simulating both processes is developed and tested against <span class="hlt">ice</span> core data. Temperature, salinity, liquid fraction, fluid velocity, total salt <span class="hlt">content</span>, and <span class="hlt">ice</span> structure are computed during model runs. The model results agree well with empirical observations and simulations highlight the effect platelet <span class="hlt">ice</span> accretion has on overall <span class="hlt">ice</span> thickness and characteristics. Results from sensitivity studies emphasize the need to further constrain sea <span class="hlt">ice</span> microstructure and the associated physics, particularly permeability-porosity relationships, if a complete model of sea <span class="hlt">ice</span> evolution is to be obtained. Additionally, implications for terrestrial <span class="hlt">ice</span> shelves and icy moons in the solar system are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70028080','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70028080"><span>Satellite-derived, melt-season surface temperature of the Greenland <span class="hlt">Ice</span> Sheet (2000-2005) and its relationship to <span class="hlt">mass</span> balance</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hall, D.K.; Williams, R.S.; Casey, K.A.; DiGirolamo, N.E.; Wan, Z.</p> <p>2006-01-01</p> <p>Mean, clear-sky surface temperature of the Greenland <span class="hlt">Ice</span> Sheet was measured for each melt season from 2000 to 2005 using Moderate-Resolution Imaging Spectroradiometer (MODIS)–derived land-surface temperature (LST) data-product maps. During the period of most-active melt, the mean, clear-sky surface temperature of the <span class="hlt">ice</span> sheet was highest in 2002 (−8.29 ± 5.29°C) and 2005 (−8.29 ± 5.43°C), compared to a 6-year mean of −9.04 ± 5.59°C, in agreement with recent work by other investigators showing unusually extensive melt in 2002 and 2005. Surface-temperature variability shows a correspondence with the dry-snow facies of the <span class="hlt">ice</span> sheet; a reduction in area of the dry-snow facies would indicate a more-negative <span class="hlt">mass</span> balance. Surface-temperature variability generally increased during the study period and is most pronounced in the 2005 melt season; this is consistent with surface instability caused by air-temperature fluctuations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19890018778','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19890018778"><span>Analysis of sea <span class="hlt">ice</span> dynamics</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zwally, J.</p> <p>1988-01-01</p> <p>The ongoing work has established the basis for using multiyear sea <span class="hlt">ice</span> concentrations from SMMR passive microwave for studies of largescale advection and convergence/divergence of the Arctic sea <span class="hlt">ice</span> pack. Comparisons were made with numerical model simulations and buoy data showing qualitative agreement on daily to interannual time scales. Analysis of the 7-year SMMR data set shows significant interannual variations in the total area of multiyear <span class="hlt">ice</span>. The scientific objective is to investigate the dynamics, <span class="hlt">mass</span> balance, and interannual variability of the Arctic sea <span class="hlt">ice</span> pack. The research emphasizes the direct application of sea <span class="hlt">ice</span> parameters derived from passive microwave data (SMMR and SSMI) and collaborative studies using a sea <span class="hlt">ice</span> dynamics model. The possible causes of observed interannual variations in the multiyear <span class="hlt">ice</span> area are being examined. The relative effects of variations in the large scale advection and convergence/divergence within the <span class="hlt">ice</span> pack on a regional and seasonal basis are investigated. The effects of anomolous atmospheric forcings are being examined, including the long-lived effects of synoptic events and monthly variations in the mean geostrophic winds. Estimates to be made will include the amount of new <span class="hlt">ice</span> production within the <span class="hlt">ice</span> pack during winter and the amount of <span class="hlt">ice</span> exported from the pack.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011MsT.........18M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011MsT.........18M"><span>Quantification of Changes for the Milne <span class="hlt">Ice</span> Shelf, Nunavut, Canada, 1950 -- 2009</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mortimer, Colleen Adel</p> <p></p> <p>This study presents a comprehensive overview of the current state of the Milne <span class="hlt">Ice</span> Shelf and how it has changed over the last 59 years. The 205 +/-1 km2 <span class="hlt">ice</span> shelf experienced a 28% (82 +/-0.8 km 2) reduction in area between 1950 -- 2009, and a 20% (2.5 +/-0.9km 3 water equivalent (w.e.)) reduction in volume between 1981 -- 2008/2009, suggesting a long-term state of negative <span class="hlt">mass</span> balance. Comparison of mean annual specific <span class="hlt">mass</span> balances (up to -0.34 m w.e. yr-1) with surface <span class="hlt">mass</span> balance measurements for the nearby Ward Hunt <span class="hlt">Ice</span> Shelf suggest that basal melt is a key contributor to total <span class="hlt">ice</span> shelf thinning. The development and expansion of new and existing surface cracks, as well as <span class="hlt">ice</span>-marginal and epishelf lake development, indicate significant <span class="hlt">ice</span> shelf weakening. Over the next few decades it is likely that the Milne <span class="hlt">Ice</span> Shelf will continue to deteriorate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC43H1150W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC43H1150W"><span>Geoengineering Marine <span class="hlt">Ice</span> Sheets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wolovick, M.</p> <p>2017-12-01</p> <p><span class="hlt">Mass</span> loss from Greenland and Antarctica is highly sensitive to the presence of warm ocean water that drives melting at the grounding line. Rapid melting near the grounding line causes <span class="hlt">ice</span> shelf thinning, loss of buttressing, flow acceleration, grounding line retreat, and ultimately <span class="hlt">mass</span> loss and sea-level rise. If the grounding line enters a section of overdeepened bed the <span class="hlt">ice</span> sheet may even enter a runaway collapse via the marine <span class="hlt">ice</span> sheet instability. The warm water that triggers this process resides offshore at depth and accesses the grounding line through deep troughs in the continental shelf. In Greenland, warm water transport is further constricted through narrow fjords. Here, I propose blocking warm water transport through these choke points with an artificial sill. Using a simple width- and depth-averaged model of <span class="hlt">ice</span> stream flow coupled to a buoyant-plume model of ocean melting, I find that grounding line retreat and sea level rise can be delayed or reversed for hundreds of years if warm water is prevented from accessing the grounding line at depth. Blocking of warm water from the sub-<span class="hlt">ice</span> cavity causes <span class="hlt">ice</span> shelf thickening, increased buttressing, and grounding line readvance. The increase in buttressing is greatly magnified if the thickened <span class="hlt">ice</span> shelf regrounds on a bathymetric high or on the artificial sill itself. In some experiments for Thwaites Glacier the grounding line is able to recover from a severely retreated state over 100 km behind its present-day position. Such a dramatic recovery demonstrates that it is possible, at least in principle, to stop and reverse an ongoing marine <span class="hlt">ice</span> sheet collapse. If the <span class="hlt">ice</span> shelf regrounds on the artificial sill itself, erosion of the sill beneath the grounded <span class="hlt">ice</span> could reduce the effectiveness of the intervention. However, experiments including sill erosion suggest that even a very weak sill (1 kPa) could delay a collapse for centuries. The scale of the artificial sills in Greenlandic fjords is comparable to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..44.5969Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..44.5969Z"><span>The influence of meridional <span class="hlt">ice</span> transport on Europa's ocean stratification and heat <span class="hlt">content</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhu, Peiyun; Manucharyan, Georgy E.; Thompson, Andrew F.; Goodman, Jason C.; Vance, Steven D.</p> <p>2017-06-01</p> <p>Jupiter's moon Europa likely hosts a saltwater ocean beneath its icy surface. Geothermal heating and rotating convection in the ocean may drive a global overturning circulation that redistributes heat vertically and meridionally, preferentially warming the <span class="hlt">ice</span> shell at the equator. Here we assess the previously unconstrained influence of ocean-<span class="hlt">ice</span> coupling on Europa's ocean stratification and heat transport. We demonstrate that a relatively fresh layer can form at the <span class="hlt">ice</span>-ocean interface due to a meridional <span class="hlt">ice</span> transport forced by the differential <span class="hlt">ice</span> shell heating between the equator and the poles. We provide analytical and numerical solutions for the layer's characteristics, highlighting their sensitivity to critical ocean parameters. For a weakly turbulent and highly saline ocean, a strong buoyancy gradient at the base of the freshwater layer can suppress vertical tracer exchange with the deeper ocean. As a result, the freshwater layer permits relatively warm deep ocean temperatures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.U13B..31Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.U13B..31Z"><span>The influence of meridional <span class="hlt">ice</span> transport on Europa's ocean stratification and heat <span class="hlt">content</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhu, P.; Manucharyan, G.; Thompson, A. F.; Goodman, J. C.; Vance, S.</p> <p>2017-12-01</p> <p>Jupiter's moon Europa likely hosts a saltwater ocean beneath its icy surface. Geothermal heating and rotating convection in the ocean may drive a global overturning circulation that redistributes heat vertically and meridionally, preferentially warming the <span class="hlt">ice</span> shell at the equator. Here we assess thepreviously unconstrained influence of ocean-<span class="hlt">ice</span> coupling on Europa's ocean stratification and heat transport. We demonstrate that a relatively fresh layer can form at the <span class="hlt">ice</span>-ocean interface due to a meridional <span class="hlt">ice</span> transport forced by the differential <span class="hlt">ice</span> shell heating between the equator and the poles. We provide analytical and numerical solutions for the layer's characteristics, highlighting their sensitivity to critical ocean parameters. For a weakly turbulent and highly saline ocean, a strong buoyancy gradient at the base of the freshwater layer can suppress vertical tracer exchange with the deeper ocean. As a result, the freshwater layer permits relatively warm deep ocean temperatures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AcMSn..31....1Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AcMSn..31....1Z"><span>Modeling ocean wave propagation under sea <span class="hlt">ice</span> covers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhao, Xin; Shen, Hayley H.; Cheng, Sukun</p> <p>2015-02-01</p> <p>Operational ocean wave models need to work globally, yet current ocean wave models can only treat <span class="hlt">ice</span>-covered regions crudely. The purpose of this paper is to provide a brief overview of <span class="hlt">ice</span> effects on wave propagation and different research methodology used in studying these effects. Based on its proximity to land or sea, sea <span class="hlt">ice</span> can be classified as: landfast <span class="hlt">ice</span> zone, shear zone, and the marginal <span class="hlt">ice</span> zone. All <span class="hlt">ice</span> covers attenuate wave energy. Only long swells can penetrate deep into an <span class="hlt">ice</span> cover. Being closest to open water, wave propagation in the marginal <span class="hlt">ice</span> zone is the most complex to model. The physical appearance of sea <span class="hlt">ice</span> in the marginal <span class="hlt">ice</span> zone varies. Grease <span class="hlt">ice</span>, pancake <span class="hlt">ice</span>, brash <span class="hlt">ice</span>, floe aggregates, and continuous <span class="hlt">ice</span> sheet may be found in this zone at different times and locations. These types of <span class="hlt">ice</span> are formed under different thermal-mechanical forcing. There are three classic models that describe wave propagation through an idealized <span class="hlt">ice</span> cover: <span class="hlt">mass</span> loading, thin elastic plate, and viscous layer models. From physical arguments we may conjecture that <span class="hlt">mass</span> loading model is suitable for disjoint aggregates of <span class="hlt">ice</span> floes much smaller than the wavelength, thin elastic plate model is suitable for a continuous <span class="hlt">ice</span> sheet, and the viscous layer model is suitable for grease <span class="hlt">ice</span>. For different sea <span class="hlt">ice</span> types we may need different wave <span class="hlt">ice</span> interaction models. A recently proposed viscoelastic model is able to synthesize all three classic models into one. Under suitable limiting conditions it converges to the three previous models. The complete theoretical framework for evaluating wave propagation through various <span class="hlt">ice</span> covers need to be implemented in the operational ocean wave models. In this review, we introduce the sea <span class="hlt">ice</span> types, previous wave <span class="hlt">ice</span> interaction models, wave attenuation mechanisms, the methods to calculate wave reflection and transmission between different <span class="hlt">ice</span> covers, and the effect of <span class="hlt">ice</span> floe breaking on shaping the sea <span class="hlt">ice</span> morphology</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..11.5463B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..11.5463B"><span>Preliminary biogeochemical assessment of EPICA LGM and Holocene <span class="hlt">ice</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>Bulat, S.; Alekhina, I.; Marie, D.; Wagenbach, D.; Raynaud, D.; Petit, J. R.</p> <p>2009-04-01</p> <p>We are investigating the biological <span class="hlt">content</span> (biomass and microbial diversity of Aeolian origin) of EPICA <span class="hlt">ice</span> core within the frame of EPICA Microbiology consortium*. Two <span class="hlt">ice</span> core sections were selected from EPICA Dome C and Droning Maud Land, both from LGM and Holocene. Preliminary measurements of DOC (dissolved organic <span class="hlt">content</span>) and microbial cell concentrations have been performed. Both analyses showed the very low biomass and ultra low DOC <span class="hlt">content</span>. Trace DNA analyses are in a progress. The <span class="hlt">ice</span> sections were decontaminated in LGGE cold and clean room facilities benefiting the protocol developed for Vostok <span class="hlt">ice</span> core studies. The melt water was then shared between two party laboratories for a complementary approach in studying microbial <span class="hlt">content</span>. Prior to biology the melt water was tested for chemical contaminant ions and organic acids, DOC and dust <span class="hlt">contents</span>. The biological methods included all the spectra of appropriate molecular techniques (gDNA extraction, PCR, clone libraries and sequencing). As preliminary results, both LGM (well identified by dust fallout) and Holocene <span class="hlt">ice</span> samples (EDC99 and EDML) proved to be extremely clear (i.e. pristine) in terms of biomass (less then 4 cells per ml) and DOC <span class="hlt">contents</span> (less then 5 ppbC). There was no obvious difference between LGM and Holocene in cell counts, while LGM showed a bit high organic carbon <span class="hlt">content</span>. The latter in terms of biology means ultra-oligotrophic conditions (i.e., no possibility for heterotrophic life style). In fact no metabolizing microbial cells or propagating populations are expected at these depths at temperature -38oC and lower (limiting life temperature threshold is -20°C). Nevertheless some life seeds brought in Antarctica with precipitation could be well preserved because the age is rather young (21 kyr and less). Trying to identify these aliens and document their distribution during last climate cycle the meltwater was concentrated about 1000 times down. The genomic DNA was extracted and very</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19800053750&hterms=methane+composition&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dmethane%2Bcomposition','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19800053750&hterms=methane+composition&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dmethane%2Bcomposition"><span><span class="hlt">Mass</span>-radius relationships and constraints on the composition of Pluto</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lupo, M. J.; Lewis, J. S.</p> <p>1980-01-01</p> <p>With the new upper limit of Pluto's <span class="hlt">mass</span>, an upper limit for Pluto's density of 1.74 g/cu cm has been found. Assuming Pluto to be 100% methane, available methane density data can be used to set a lower limit of 0.53 g/cu cm on Pluto's density, thus placing an absolute upper limit of 1909 km on the radius and a lower limit of 0.32 on the albedo. The results of 280 computer models covering a wide range of composition ratios of rock, water <span class="hlt">ice</span>, and methane <span class="hlt">ice</span> are reported. Limits are placed on Pluto's silicate <span class="hlt">content</span>, and a simple spacecraft method for determining Pluto's water <span class="hlt">content</span> from its density and moment of inertia is given. The low thermal conductivity and strength of solid methane suggest rapid solid-state convection in Pluto's methane layer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19810068588','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19810068588"><span>Correlations Among <span class="hlt">Ice</span> Measurements, Impingement Rates <span class="hlt">Icing</span> Conditions, and Drag Coefficients for Unswept NACA 65A004 Airfoil</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gray, Vernon H.</p> <p>1958-01-01</p> <p>An empirical relation has been obtained by which the change in drag coefficient caused by <span class="hlt">ice</span> formations on an unswept NACA 65AO04 airfoil section can be determined from the following <span class="hlt">icing</span> and operating conditions: <span class="hlt">icing</span> time, airspeed, air total temperature, liquid-water <span class="hlt">content</span>, cloud droplet impingement efficiencies, airfoil chord length, and angles of attack. The correlation was obtained by use of measured <span class="hlt">ice</span> heights and <span class="hlt">ice</span> angles. These measurements were obtained from a variety of <span class="hlt">ice</span> formations, which were carefully photographed, cross-sectioned, and weighed. <span class="hlt">Ice</span> weights increased at a constant rate with <span class="hlt">icing</span> time in a rime <span class="hlt">icing</span> condition and at progressively increasing rates in glaze <span class="hlt">icing</span> conditions. Initial rates of <span class="hlt">ice</span> collection agreed reasonably well with values predicted from droplet impingement data. Experimental droplet impingement rates obtained on this airfoil section agreed with previous theoretical calculations for angles of attack of 40 or less. Disagreement at higher angles of attack was attributed to flow separation from the upper surface of the experimental airfoil model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.4621R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.4621R"><span>State of Arctic Sea <span class="hlt">Ice</span> North of Svalbard during N-<span class="hlt">ICE</span>2015</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rösel, Anja; King, Jennifer; Gerland, Sebastian</p> <p>2016-04-01</p> <p>The N-<span class="hlt">ICE</span>2015 cruise, led by the Norwegian Polar Institute, was a drift experiment with the research vessel R/V Lance from January to June 2015, where the ship started the drift North of Svalbard at 83°14.45' N, 21°31.41' E. The drift was repeated as soon as the vessel drifted free. Altogether, 4 <span class="hlt">ice</span> stations where installed and the complex ocean-sea <span class="hlt">ice</span>-atmosphere system was studied with an interdisciplinary Approach. During the N-<span class="hlt">ICE</span>2015 cruise, extensive <span class="hlt">ice</span> thickness and snow depth measurements were performed during both, winter and summer conditions. Total <span class="hlt">ice</span> and snow thickness was measured with ground-based and airborne electromagnetic instruments; snow depth was measured with a GPS snow depth probe. Additionally, <span class="hlt">ice</span> <span class="hlt">mass</span> balance and snow buoys were deployed. Snow and <span class="hlt">ice</span> thickness measurements were performed on repeated transects to quantify the <span class="hlt">ice</span> growth or loss as well as the snow accumulation and melt rate. Additionally, we collected independent values on surveys to determine the general <span class="hlt">ice</span> thickness distribution. Average snow depths of 32 cm on first year <span class="hlt">ice</span>, and 52 cm on multi-year <span class="hlt">ice</span> were measured in January, the mean snow depth on all <span class="hlt">ice</span> types even increased until end of March to 49 cm. The average total <span class="hlt">ice</span> and snow thickness in winter conditions was 1.92 m. During winter we found a small growth rate on multi-year <span class="hlt">ice</span> of about 15 cm in 2 months, due to above-average snow depths and some extraordinary storm events that came along with mild temperatures. In contrast thereto, we also were able to study new <span class="hlt">ice</span> formation and thin <span class="hlt">ice</span> on newly formed leads. In summer conditions an enormous melt rate, mainly driven by a warm Atlantic water inflow in the marginal <span class="hlt">ice</span> zone, was observed during two <span class="hlt">ice</span> stations with melt rates of up to 20 cm per 24 hours. To reinforce the local measurements around the ship and to confirm their significance on a larger scale, we compare them to airborne thickness measurements and classified SAR-satellite scenes. The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C51E..07C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C51E..07C"><span>Investigation of Controls on <span class="hlt">Ice</span> Dynamics in Northeast Greenland from <span class="hlt">Ice</span>-Thickness Change Record Using <span class="hlt">Ice</span> Sheet System Model (ISSM)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Csatho, B. M.; Larour, E. Y.; Schenk, A. F.; Schlegel, N.; Duncan, K.</p> <p>2015-12-01</p> <p>We present a new, complete <span class="hlt">ice</span> thickness change reconstruction of the NE sector of the Greenland <span class="hlt">Ice</span> Sheet for 1978-2014, partitioned into changes due to surface processes and <span class="hlt">ice</span> dynamics. Elevation changes are computed from all available stereoscopic DEMs, and laser altimetry data (ICESat, ATM, LVIS). Surface <span class="hlt">Mass</span> Balance and firn-compaction estimates are from RACMO2.3. Originating nearly at the divide of the Greenland <span class="hlt">Ice</span> Sheet (GrIS), the dynamically active North East <span class="hlt">Ice</span> Stream (NEGIS) is capable of rapidly transmitting <span class="hlt">ice</span>-marginal forcing far inland. Thus, NEGIS provides a possible mechanism for a rapid drawdown of <span class="hlt">ice</span> from the <span class="hlt">ice</span> sheet interior as marginal warming, thinning and retreat continues. Our altimetry record shows accelerating dynamic thinning of Zachariæ Isstrom, initially limited to the deepest part of the fjord near the calving front (1978-2000) and then extending at least 75 km inland. At the same time, changes over the Nioghalvfjerdsfjorden (N79) Glacier are negligible. We also detect localized large dynamic changes at higher elevations on the <span class="hlt">ice</span> sheet. These thickness changes, often occurring at the onset of fast flow, could indicate rapid variations of basal lubrication due to rerouting of subglacial drainage. We investigate the possible causes of the observed spatiotemporal pattern of <span class="hlt">ice</span> sheet elevation changes using the <span class="hlt">Ice</span> Sheet System Model (ISSM). This work build on our previous studies examining the sensitivity of <span class="hlt">ice</span> flow within the Northeast Greenland <span class="hlt">Ice</span> Stream (NEGIS) to key fields, including <span class="hlt">ice</span> viscosity, basal drag. We assimilate the new altimetry record into ISSM to improve the reconstruction of basal friction and <span class="hlt">ice</span> viscosity. Finally, airborne geophysical (gravity, magnetic) and <span class="hlt">ice</span>-penetrating radar data is examined to identify the potential geologic controls on the <span class="hlt">ice</span> thickness change pattern. Our study provides the first comprehensive reconstruction of <span class="hlt">ice</span> thickness changes for the entire NEGIS drainage basin during</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AMT....11.3221B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AMT....11.3221B"><span>Design, construction and commissioning of the Braunschweig <span class="hlt">Icing</span> Wind Tunnel</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bansmer, Stephan E.; Baumert, Arne; Sattler, Stephan; Knop, Inken; Leroy, Delphine; Schwarzenboeck, Alfons; Jurkat-Witschas, Tina; Voigt, Christiane; Pervier, Hugo; Esposito, Biagio</p> <p>2018-06-01</p> <p>Beyond its physical importance in both fundamental and climate research, atmospheric <span class="hlt">icing</span> is considered as a severe operational condition in many engineering applications like aviation, electrical power transmission and wind-energy production. To reproduce such <span class="hlt">icing</span> conditions in a laboratory environment, <span class="hlt">icing</span> wind tunnels are frequently used. In this paper, a comprehensive overview on the design, construction and commissioning of the Braunschweig <span class="hlt">Icing</span> Wind Tunnel is given. The tunnel features a test section of 0.5 m × 0.5 m with peak velocities of up to 40 m s-1. The static air temperature ranges from -25 to +30 °C. Supercooled droplet <span class="hlt">icing</span> with liquid water <span class="hlt">contents</span> up to 3 g m-3 can be reproduced. The unique aspect of this facility is the combination of an <span class="hlt">icing</span> tunnel with a cloud chamber system for making <span class="hlt">ice</span> particles. These <span class="hlt">ice</span> particles are more realistic in shape and density than those usually used for mixed phase and <span class="hlt">ice</span> crystal <span class="hlt">icing</span> experiments. <span class="hlt">Ice</span> water <span class="hlt">contents</span> up to 20 g m-3 can be generated. We further show how current state-of-the-art measurement techniques for particle sizing are performed on <span class="hlt">ice</span> particles. The data are compared to those of in-flight measurements in mesoscale convective cloud systems in tropical regions. Finally, some applications of the <span class="hlt">icing</span> wind tunnel are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20170002775&hterms=inversion&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dinversion','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20170002775&hterms=inversion&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dinversion"><span>Spatial and Temporal Antarctic <span class="hlt">Ice</span> Sheet <span class="hlt">Mass</span> Trends, Glacio-Isostatic Adjustment, and Surface Processes from a Joint Inversion of Satellite Altimeter, Gravity, and GPS Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Martin-Espanol, Alba; Zammit-Mangion, Andrew; Clarke, Peter J.; Flament, Thomas; Helm, Veit; King, Matt A.; Luthcke, Scott B.; Petrie, Elizabeth; Remy, Frederique; Schon, Nana; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20170002775'); toggleEditAbsImage('author_20170002775_show'); toggleEditAbsImage('author_20170002775_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20170002775_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20170002775_hide"></p> <p>2016-01-01</p> <p>We present spatiotemporal <span class="hlt">mass</span> balance trends for the Antarctic <span class="hlt">Ice</span> Sheet from a statistical inversion of satellite altimetry, gravimetry, and elastic-corrected GPS data for the period 2003-2013. Our method simultaneously determines annual trends in <span class="hlt">ice</span> dynamics, surface <span class="hlt">mass</span> balance anomalies, and a time-invariant solution for glacio-isostatic adjustment while remaining largely independent of forward models. We establish that over the period 2003-2013, Antarctica has been losing <span class="hlt">mass</span> at a rateof -84 +/- 22 Gt per yr, with a sustained negative mean trend of dynamic imbalance of -111 +/- 13 Gt per yr. West Antarctica is the largest contributor with -112 +/- 10 Gt per yr, mainly triggered by high thinning rates of glaciers draining into the Amundsen Sea Embayment. The Antarctic Peninsula has experienced a dramatic increase in <span class="hlt">mass</span> loss in the last decade, with a mean rate of -28 +/- 7 Gt per yr and significantly higher values for the most recent years following the destabilization of the Southern Antarctic Peninsula around 2010. The total <span class="hlt">mass</span> loss is partly compensated by a significant <span class="hlt">mass</span> gain of 56 +/- 18 Gt per yr in East Antarctica due to a positive trend of surface <span class="hlt">mass</span> balance anomalies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C51A0967B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C51A0967B"><span>Mapping Ross <span class="hlt">Ice</span> Shelf with ROSETTA-<span class="hlt">Ice</span> airborne 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>Becker, M. K.; Fricker, H. A.; Padman, L.; Bell, R. E.; Siegfried, M. R.; Dieck, C. C. M.</p> <p>2017-12-01</p> <p>The Ross Ocean and <span class="hlt">ice</span> Shelf Environment and Tectonic setting Through Aerogeophysical surveys and modeling (ROSETTA-<span class="hlt">Ice</span>) project combines airborne glaciological, geological, and oceanographic observations to enhance our understanding of the history and dynamics of the large ( 500,000 square km) Ross <span class="hlt">Ice</span> Shelf (RIS). Here, we focus on the Light Detection And Ranging (LiDAR) data collected in 2015 and 2016. This data set represents a significant advance in resolution: Whereas the last attempt to systematically map RIS (the surface-based RIGGS program in the 1970s) was at 55 km grid spacing, the ROSETTA-<span class="hlt">Ice</span> grid has 10-20 km line spacing and much higher along-track resolution. We discuss two different strategies for processing the raw LiDAR data: one that requires proprietary software (Riegl's RiPROCESS package), and one that employs open-source programs and libraries. With the processed elevation data, we are able to resolve fine-scale <span class="hlt">ice</span>-shelf features such as the "rampart-moat" <span class="hlt">ice</span>-front morphology, which has previously been observed on and modeled for icebergs. This feature is also visible in the ROSETTA-<span class="hlt">Ice</span> shallow-<span class="hlt">ice</span> radar data; comparing the laser data with radargrams provides insight into the processes leading to their formation. Near-surface firn state and total firn air <span class="hlt">content</span> can also be investigated through combined analysis of laser altimetry and radar data. By performing similar analyses with data from the radar altimeter aboard CryoSat-2, we demonstrate the utility of the ROSETTA-<span class="hlt">Ice</span> LiDAR data set in satellite validation efforts. The incorporation of the LiDAR data from the third and final field season (December 2017) will allow us to construct a DEM and an <span class="hlt">ice</span> thickness map of RIS for the austral summers of 2015-2017. These products will be used to validate and extend observations of height changes from satellite radar and laser altimetry, as well as to update regional models of ocean circulation 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_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_20 --> <div id="page_21" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="401"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C44A..03Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C44A..03Y"><span>Greenland <span class="hlt">ice</span> sheet beyond 2100: Simulating its evolution and influence using the coupled climate-<span class="hlt">ice</span> sheet model EC-Earth - PISM</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, S.; Christensen, J. H.; Madsen, M. S.; Ringgaard, I. M.; Petersen, R. A.; Langen, P. P.</p> <p>2017-12-01</p> <p>Greenland <span class="hlt">ice</span> sheet (GrIS) is observed undergoing a rapid change in the recent decades, with an increasing area of surface melting and ablation and a speeding <span class="hlt">mass</span> loss. Predicting the GrIS changes and their climate consequences relies on the understanding of the interaction of the GrIS with the climate system on both global and local scales, and requires climate model systems incorporating with an explicit and physically consistent <span class="hlt">ice</span> sheet module. In this work we study the GrIS evolution and its interaction with the climate system using a fully coupled global climate model with a dynamical <span class="hlt">ice</span> sheet model for the GrIS. The coupled model system, EC-EARTH - PISM, consisting of the atmosphere-ocean-sea <span class="hlt">ice</span> model system EC-EARTH, and the Parallel <span class="hlt">Ice</span> Sheet Model (PISM), has been employed for a 1400-year simulation forced by CMIP5 historical forcing from 1850 to 2005 and continued along an extended RCP8.5 scenario with the forcing peaking at 2200 and stabilized hereafter. The simulation reveals that, following the anthropogenic forcing increase, the global mean surface temperature rapidly rises about 10 °C in the 21st and 22nd century. After the forcing stops increasing after 2200, the temperature change slows down and eventually stabilizes at about 12.5 °C above the preindustrial level. In response to the climate warming, the GrIS starts losing <span class="hlt">mass</span> slowly in the 21st century, but the <span class="hlt">ice</span> retreat accelerates substantially after 2100 and <span class="hlt">ice</span> <span class="hlt">mass</span> loss continues hereafter at a constant rate of approximately 0.5 m sea level rise equivalence per 100 years, even as the warming rate gradually levels off. Ultimately the volume and extent of GrIS reduce to less than half of its preindustrial value. To understand the interaction of GrIS with the climate system, the characteristics of atmospheric and oceanic circulation in the warm climate are analyzed. The circulation patterns associated with the negative surface <span class="hlt">mass</span> balance that leads to GrIS retreat are investigated</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24910517','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24910517"><span>A century of variation in the dependence of Greenland iceberg calving on <span class="hlt">ice</span> sheet surface <span class="hlt">mass</span> balance and regional 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>Bigg, G R; Wei, H L; Wilton, D J; Zhao, Y; Billings, S A; Hanna, E; Kadirkamanathan, V</p> <p>2014-06-08</p> <p>Iceberg calving is a major component of the total <span class="hlt">mass</span> balance of the Greenland <span class="hlt">ice</span> sheet (GrIS). A century-long record of Greenland icebergs comes from the International <span class="hlt">Ice</span> Patrol's record of icebergs (I48N) passing latitude 48° N, off Newfoundland. I48N exhibits strong interannual variability, with a significant increase in amplitude over recent decades. In this study, we show, through a combination of nonlinear system identification and coupled ocean-iceberg modelling, that I48N's variability is predominantly caused by fluctuation in GrIS calving discharge rather than open ocean iceberg melting. We also demonstrate that the episodic variation in iceberg discharge is strongly linked to a nonlinear combination of recent changes in the surface <span class="hlt">mass</span> balance (SMB) of the GrIS and regional atmospheric and oceanic climate variability, on the scale of the previous 1-3 years, with the dominant causal mechanism shifting between glaciological (SMB) and climatic (ocean temperature) over time. We suggest that this is a change in whether glacial run-off or under-<span class="hlt">ice</span> melting is dominant, respectively. We also suggest that GrIS calving discharge is episodic on at least a regional scale and has recently been increasing significantly, largely as a result of west Greenland sources.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.5738V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.5738V"><span>The Tweeting <span class="hlt">Ice</span> Shelf: geophysics and outreach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Van Liefferinge, Brice; Berger, Sophie; Drews, Reinhard; Pattyn, Frank</p> <p>2015-04-01</p> <p>Over the last decade the Antarctic and Greenland <span class="hlt">ice</span> sheets have contributed about one third of the annual sea level rise (Hanna et al., 2013). However, it remains difficult to reconcile global <span class="hlt">mass</span> balance estimates obtained from different satellite-based methods. A typical approach is to balance the <span class="hlt">mass</span> input from atmospheric modelling with the outgoing <span class="hlt">mass</span> flux at the <span class="hlt">ice</span>-sheet boundary (Shepherd et al., 2012). The flux calculations at the boundary rely on satellite-derived surface velocities, which are currently only available as snapshots in time, and which need ground truth for validation. Here, we report on continuous, year-round measurements that aim at improving the input-output method in several aspects and carefully map the flow speed allowing for detecting seasonal variability. For this purpose, we set up in December 2014 three stand-alone single-frequency GPSes on the Roi Baudouin <span class="hlt">ice</span> shelf (East Antarctica). The GPSes are installed across a surface depression (typical for large <span class="hlt">ice</span>-shelf channels), where subglacial melting is expected. This setup allows us to investigate how these channels behave, i.e., if they become wider, whether or not they enhance the <span class="hlt">ice</span> flow, and, in combination with an installed phase-sensitive radar, what amount of melting occurs below the channels in contact with the ocean. The GPS data are transmitted on a daily basis. <span class="hlt">Ice</span>-shelf velocity is derived from the raw hourly location following the methods described in den Ouden et al. (2010), Dunse et al. (2012), and Ahlstrøm et al. (2013). However, a reference station has not been used for the correction. Basic processing involves outliers removal, smoothing, time-series analysis and comparison with tidal models. The project comes alongside an outreach event: on a weekly basis, the <span class="hlt">ice</span> shelf 'tweets' its position, motion and relays other information with respect to the project. The GPS systems can be followed on Twitter via @Tweetin<span class="hlt">Ice</span>Shelf as well as the Tweeting <span class="hlt">Ice</span> Shelf</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012JGRC..117.9031G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012JGRC..117.9031G"><span>Modeling the basal melting and marine <span class="hlt">ice</span> accretion of the Amery <span class="hlt">Ice</span> Shelf</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Galton-Fenzi, B. K.; Hunter, J. R.; Coleman, R.; Marsland, S. J.; Warner, R. C.</p> <p>2012-09-01</p> <p>The basal <span class="hlt">mass</span> balance of the Amery <span class="hlt">Ice</span> Shelf (AIS) in East Antarctica is investigated using a numerical ocean model. The main improvements of this model over previous studies are the inclusion of frazil formation and dynamics, tides and the use of the latest estimate of the sub-<span class="hlt">ice</span>-shelf cavity geometry. The model produces a net basal melt rate of 45.6 Gt year-1 (0.74 m <span class="hlt">ice</span> year-1) which is in good agreement with reviewed observations. The melting at the base of the <span class="hlt">ice</span> shelf is primarily due to interaction with High Salinity Shelf Water created from the surface sea-<span class="hlt">ice</span> formation in winter. The temperature difference between the coldest waters created in the open ocean and the in situ freezing point of ocean water in contact with the deepest part of the AIS drives a melt rate that can exceed 30 m of <span class="hlt">ice</span> year-1. The inclusion of frazil dynamics is shown to be important for both melting and marine <span class="hlt">ice</span> accretion (refreezing). Frazil initially forms in the supercooled water layer adjacent to the base of the <span class="hlt">ice</span> shelf. The net accretion of marine <span class="hlt">ice</span> is 5.3 Gt year-1, comprised of 3.7 Gt year-1 of frazil accretion and 1.6 Gt year-1 of direct basal refreezing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMPA13A1975T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMPA13A1975T"><span>Guide to Sea <span class="hlt">Ice</span> Information and Sea <span class="hlt">Ice</span> Data Online - the Sea <span class="hlt">Ice</span> Knowledge and Data Platform www.meereisportal.de and www.seaiceportal.de</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Treffeisen, R. E.; Nicolaus, M.; Bartsch, A.; Fritzsch, B.; Grosfeld, K.; Haas, C.; Hendricks, S.; Heygster, G.; Hiller, W.; Krumpen, T.; Melsheimer, C.; Ricker, R.; Weigelt, M.</p> <p>2016-12-01</p> <p>The combination of multi-disciplinary sea <span class="hlt">ice</span> science and the rising demand of society for up-to-date information and user customized products places emphasis on creating new ways of communication between science and society. The new knowledge platform is a contribution to the cross-linking of scientifically qualified information on climate change, and focuses on the theme: `sea <span class="hlt">ice</span>' in both Polar Regions. With this platform, the science opens to these changing societal demands. It is the first comprehensive German speaking knowledge platform on sea <span class="hlt">ice</span>; the platform went online in 2013. The web site delivers popularized information for the general public as well as scientific data meant primarily for the more expert readers and scientists. It also provides various tools allowing for visitor interaction. The demand for the web site indicates a high level of interest from both the general public and experts. It communicates science-based information to improve awareness and understanding of sea <span class="hlt">ice</span> related research. The principle concept of the new knowledge platform is based on three pillars: (1) sea <span class="hlt">ice</span> knowledge and background information, (2) data portal with visualizations, and (3) expert knowledge, latest research results and press releases. Since then, the <span class="hlt">content</span> and selection of data sets increased and the data portal received increasing attention, also from the international science community. Meanwhile, we are providing near-real time and archived data of many key parameters of sea <span class="hlt">ice</span> and its snow cover. The data sets result from measurements acquired by various platforms as well as numerical simulations. Satellite observations (e.g., AMSR2, CryoSat-2 and SMOS) of sea <span class="hlt">ice</span> concentration, freeboard, thickness and drift are available as gridded data sets. Sea <span class="hlt">ice</span> and snow temperatures and thickness as well as atmospheric parameters are available from autonomous <span class="hlt">ice</span>-tethered platforms (buoys). Additional ship observations, <span class="hlt">ice</span> station measurements, and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26139868','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26139868"><span>Development of technology for manufacture of ragi <span class="hlt">ice</span> cream.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Patel, I J; Dharaiya, C N; Pinto, S V</p> <p>2015-07-01</p> <p>Ragi (Finger millet) improves the nutritional value of <span class="hlt">ice</span> cream by enhancing the iron and fibre <span class="hlt">content</span>. Caramel flavoured medium fat <span class="hlt">ice</span> cream (6 % fat) was prepared by addition of gelatinized malted ragi flour roasted in butter (MRB) @ 8 %, 9 % and 10 % by weight of mix and compared with control (C) i.e. vanilla <span class="hlt">ice</span> cream containing 10 % fat. The overall acceptability score of product prepared using 9 % MRB was statistically (P > 0.05) at par with the C, hence, it was selected. In the next part of the study, ragi <span class="hlt">ice</span> cream was prepared using 4 different flavours viz. vanilla, mango, chocolate and caramel. Chocolate flavoured ragi <span class="hlt">ice</span> cream was adjudged as best, followed by mango, caramel and vanilla <span class="hlt">ice</span> cream. The iron and fibre <span class="hlt">content</span> of chocolate flavoured ragi <span class="hlt">ice</span> cream was found to be 12.8 ppm and 1.36 % respectively. vs. 1.5 ppm and 0.18 % respectively in control (C). Heat shock treatment as well as storage up to 30 days had no adverse effect on the sensory quality of the chocolate flavored ragi <span class="hlt">ice</span> cream. Incorporation of finger millet in <span class="hlt">ice</span> cream resulted in reduction in the amount of stabilizer used and effectively functioned as fat replacer in <span class="hlt">ice</span> cream.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C13F1017M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C13F1017M"><span>Atmospheric river impacts on Greenland <span class="hlt">Ice</span> Sheet surface melt and <span class="hlt">mass</span> balance</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mattingly, K.; Mote, T. L.</p> <p>2017-12-01</p> <p><span class="hlt">Mass</span> loss from the Greenland <span class="hlt">Ice</span> Sheet (GrIS) has accelerated during the early part of the 21st Century. Several episodes of widespread GrIS melt in recent years have coincided with intense poleward moisture transport by atmospheric rivers (ARs), suggesting that variability in the frequency and intensity of these events may be an important driver of the surface <span class="hlt">mass</span> balance (SMB) of the GrIS. ARs may contribute to GrIS surface melt through the greenhouse effect of water vapor, the radiative effects of clouds, condensational latent heating within poleward-advected air <span class="hlt">masses</span>, and the energy provided by liquid precipitation. However, ARs may also provide significant positive contributions to GrIS SMB through enhanced snow accumulation. Prior research on the role of ARs in Arctic climate has consisted of case studies of ARs associated with major GrIS melt events or examined the effects of poleward moisture flux on Arctic sea <span class="hlt">ice</span>. In this study, a long-term (1979-2016) record of intense moisture transport events affecting Greenland is compiled using a conventional AR identification algorithm as well as a self-organizing map (SOM) classification applied to integrated water vapor transport (IVT) data from several atmospheric reanalysis datasets. An analysis of AR effects on GrIS melt and SMB is then performed with GrIS surface melt data from passive microwave satellite observations and the Modèle Atmosphérique Régional (MAR) regional climate model. Results show that meltwater production is above normal during and after AR impact days throughout the GrIS during all seasons, with surface melt enhanced most by strong (> 85th percentile IVT) and extreme (> 95th percentile IVT) ARs. This relationship holds at the seasonal scale, as the total amount of water vapor transported to the GrIS by ARs is significantly greater during above-normal melt seasons. ARs exert a more complex influence on SMB. Normal (< 85th percentile IVT) ARs generally do not have a substantial impact on</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23274717','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23274717"><span><span class="hlt">Mass</span> carbon monoxide poisoning at an <span class="hlt">ice</span>-hockey game: initial approach and long-term follow-up.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mortelmans, Luc J M; Populaire, Jacques; Desruelles, Didier; Sabbe, Marc B</p> <p>2013-12-01</p> <p>A <span class="hlt">mass</span> carbon monoxide (CO) intoxication during an <span class="hlt">ice</span>-hockey game is described. Two hundred and thirty-five patients were seen in different hospitals, 88 of them the same night at the nearby emergency department. To evaluate long-term implications and to identify relevant indicators, a follow-up study was organized 1 year after the incident. Apart from the file data from the emergency departments, a 1-year follow-up mailing was sent to all patients. One hundred and ninety-one patients returned their questionnaire (86%). The mean age of the patients was 28 years, with 61% men. The mean carboxyhaemoglobin (COHb) was 9.9%. COHb levels were significantly higher for individuals on the <span class="hlt">ice</span> (referee, players and maintenance personnel). There was a significant relationship with the initial presence of dizziness, fatigue and the COHb level. Headache, abdominal pain, nausea and vomiting were not significantly related to the COHb levels. The relationship between symptoms and CO level, however, should be interpreted with caution as there was a wide range between exposure and blood tests. 5.2% of patients had residual complaints, all including headache, with a significant higher incidence with high COHb levels. Only two patients had an abnormal neurological control (one slightly disturbed electroencephalography and one persistent encephalopathic complaint). Work incapacity was also significantly related to COHb levels. CO <span class="hlt">mass</span> poisonings remain a risk in indoor sporting events. Although it causes an acute <span class="hlt">mass</span> casualty incident, it is limited in time and delayed problems are scarce. Symptomatology is a poor tool for triage. The best prevention is the use of nonmineral energy sources such as for example electricity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19830034350&hterms=drainage+blocked&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Ddrainage%2Bblocked','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19830034350&hterms=drainage+blocked&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Ddrainage%2Bblocked"><span><span class="hlt">Ice</span> sculpture in the Martian outflow channels</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lucchitta, B. K.</p> <p>1982-01-01</p> <p>Viking Orbiter and terrestrial satellite images are examined at similar resolution to compare features of the Martian outflow channels with features produced by the movement of <span class="hlt">ice</span> on earth, and many resemblances are found. These include the anastomoses, sinuosities, and U-shaped cross profiles of valleys; hanging valleys; linear scour marks on valley walls; grooves and ridges on valley floors; and the streamlining of bedrock highs. Attention is given to the question whether <span class="hlt">ice</span> could have moved in the Martian environment. It is envisaged that springs or small catastrophic outbursts discharged fluids from structural outlets or chaotic terrains. These fluids built <span class="hlt">icings</span> that may have grown into substantial <span class="hlt">masses</span> and eventually flowed like glaciers down preexisting valleys. An alternative is that the fluids formed rivers or floods that in turn formed <span class="hlt">ice</span> jams and consolidated into icy <span class="hlt">masses</span> in places where obstacles blocked their flow.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20080018456&hterms=Secret&qs=N%3D0%26Ntk%3DTitle%26Ntx%3Dmode%2Bmatchall%26Ntt%3DThe%2BSecret','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20080018456&hterms=Secret&qs=N%3D0%26Ntk%3DTitle%26Ntx%3Dmode%2Bmatchall%26Ntt%3DThe%2BSecret"><span>The Secret of the Svalbard Sea <span class="hlt">Ice</span> Barrier</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nghiem, Son V.; Van Woert, Michael L.; Neumann, Gregory</p> <p>2004-01-01</p> <p>An elongated sea <span class="hlt">ice</span> feature called the Svalbard sea <span class="hlt">ice</span> barrier rapidly formed over an area in the Barents Sea to the east of Svalbard posing navigation hazards. The secret of its formation lies in the bottom bathymetry that governs the distribution of cold Arctic waters <span class="hlt">masses</span>, which impacts sea <span class="hlt">ice</span> growth on the water surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/990526-global-simulations-ice-nucleation-ice-supersaturation-improved-cloud-scheme-community-atmosphere-model','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/990526-global-simulations-ice-nucleation-ice-supersaturation-improved-cloud-scheme-community-atmosphere-model"><span>Global Simulations of <span class="hlt">Ice</span> nucleation and <span class="hlt">Ice</span> Supersaturation with an Improved Cloud Scheme in the Community Atmosphere Model</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Gettelman, A.; Liu, Xiaohong; Ghan, Steven J.</p> <p>2010-09-28</p> <p>A process-based treatment of <span class="hlt">ice</span> supersaturation and <span class="hlt">ice</span>-nucleation is implemented in the National Center for Atmospheric Research (NCAR) Community Atmosphere Model (CAM). The new scheme is designed to allow (1) supersaturation with respect to <span class="hlt">ice</span>, (2) <span class="hlt">ice</span> nucleation by aerosol particles and (3) <span class="hlt">ice</span> cloud cover consistent with <span class="hlt">ice</span> microphysics. The scheme is implemented with a 4-class 2 moment microphysics code and is used to evaluate <span class="hlt">ice</span> cloud nucleation mechanisms and supersaturation in CAM. The new model is able to reproduce field observations of <span class="hlt">ice</span> <span class="hlt">mass</span> and mixed phase cloud occurrence better than previous versions of the model. Simulations indicatemore » heterogeneous freezing and contact nucleation on dust are both potentially important over remote areas of the Arctic. Cloud forcing and hence climate is sensitive to different formulations of the <span class="hlt">ice</span> microphysics. Arctic radiative fluxes are sensitive to the parameterization of <span class="hlt">ice</span> clouds. These results indicate that <span class="hlt">ice</span> clouds are potentially an important part of understanding cloud forcing and potential cloud feedbacks, particularly in the Arctic.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22386469','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22386469"><span>Total solids <span class="hlt">content</span> drives high solid anaerobic digestion via <span class="hlt">mass</span> transfer limitation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Abbassi-Guendouz, Amel; Brockmann, Doris; Trably, Eric; Dumas, Claire; Delgenès, Jean-Philippe; Steyer, Jean-Philippe; Escudié, Renaud</p> <p>2012-05-01</p> <p>The role of the total solids (TS) <span class="hlt">content</span> on anaerobic digestion was investigated in batch reactors. A range of TS <span class="hlt">contents</span> from 10% to 35% was evaluated, four replicates were performed. The total methane production slightly decreased with TS concentrations increasing from 10% to 25% TS. Two behaviors were observed at 30% TS: two replicates had similar performances to that at 25% TS; for the two other replicates, the methane production was inhibited as observed at 35% TS. This difference suggested that 30% TS <span class="hlt">content</span> corresponded to a threshold of the solids <span class="hlt">content</span>, above which methanogenesis was strongly inhibited. The Anaerobic Digestion Model No. 1 (ADM1) was used to describe the experimental data. The effects of hydrolysis step and liquid/gas <span class="hlt">mass</span> transfer were particularly investigated. The simulations showed that <span class="hlt">mass</span> transfer limitation could explain the low methane production at high TS, and that hydrolysis rate constants slightly decreased with increasing TS. Copyright © 2012 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.4115C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.4115C"><span>Antarctic <span class="hlt">ice</span> shelf thickness from CryoSat-2 radar altimetry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chuter, Stephen; Bamber, Jonathan</p> <p>2016-04-01</p> <p>The Antarctic <span class="hlt">ice</span> shelves provide buttressing to the inland grounded <span class="hlt">ice</span> sheet, and therefore play a controlling role in regulating <span class="hlt">ice</span> dynamics and <span class="hlt">mass</span> imbalance. Accurate knowledge of <span class="hlt">ice</span> shelf thickness is essential for input-output method <span class="hlt">mass</span> balance calculations, sub-<span class="hlt">ice</span> shelf ocean models and buttressing parameterisations in <span class="hlt">ice</span> sheet models. <span class="hlt">Ice</span> shelf thickness has previously been inferred from satellite altimetry elevation measurements using the assumption of hydrostatic equilibrium, as direct measurements of <span class="hlt">ice</span> thickness do not provide the spatial coverage necessary for these applications. The sensor limitations of previous radar altimeters have led to poor data coverage and a lack of accuracy, particularly the grounding zone where a break in slope exists. We present a new <span class="hlt">ice</span> shelf thickness dataset using four years (2011-2014) of CryoSat-2 elevation measurements, with its SARIn dual antennae mode of operation alleviating the issues affecting previous sensors. These improvements and the dense across track spacing of the satellite has resulted in ˜92% coverage of the <span class="hlt">ice</span> shelves, with substantial improvements, for example, of over 50% across the Venable and Totten <span class="hlt">Ice</span> Shelves in comparison to the previous dataset. Significant improvements in coverage and accuracy are also seen south of 81.5° for the Ross and Filchner-Ronne <span class="hlt">Ice</span> Shelves. Validation of the surface elevation measurements, used to derive <span class="hlt">ice</span> thickness, against NASA ICESat laser altimetry data shows a mean bias of less than 1 m (equivalent to less than 9 m in <span class="hlt">ice</span> thickness) and a fourfold decrease in standard deviation in comparison to the previous continental dataset. Importantly, the most substantial improvements are found in the grounding zone. Validation of the derived thickness data has been carried out using multiple Radio Echo Sounding (RES) campaigns across the continent. Over the Amery <span class="hlt">ice</span> shelf, where extensive RES measurements exist, the mean difference between the datasets is 3</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19990021112','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19990021112"><span>Analytical Tools for Cloudscope <span class="hlt">Ice</span> Measurement</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Arnott, W. Patrick</p> <p>1998-01-01</p> <p> synthesizes each slice and separates the new from the sublimating particles. The new particle information is used to generate quantitative particle concentration, area, and <span class="hlt">mass</span> size spectra along with total concentration, solar extinction coefficient, and <span class="hlt">ice</span> water <span class="hlt">content</span>. This program directly creates output in html format for viewing with a web browser.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015E%26PSL.430..427R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015E%26PSL.430..427R"><span>Modelling the feedbacks between <span class="hlt">mass</span> balance, <span class="hlt">ice</span> flow and debris transport to predict the response to climate change of debris-covered glaciers in the Himalaya</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rowan, Ann V.; Egholm, David L.; Quincey, Duncan J.; Glasser, Neil F.</p> <p>2015-11-01</p> <p>Many Himalayan glaciers are characterised in their lower reaches by a rock debris layer. This debris insulates the glacier surface from atmospheric warming and complicates the response to climate change compared to glaciers with clean-<span class="hlt">ice</span> surfaces. Debris-covered glaciers can persist well below the altitude that would be sustainable for clean-<span class="hlt">ice</span> glaciers, resulting in much longer timescales of <span class="hlt">mass</span> loss and meltwater production. The properties and evolution of supraglacial debris present a considerable challenge to understanding future glacier change. Existing approaches to predicting variations in glacier volume and meltwater production rely on numerical models that represent the processes governing glaciers with clean-<span class="hlt">ice</span> surfaces, and yield conflicting results. We developed a numerical model that couples the flow of <span class="hlt">ice</span> and debris and includes important feedbacks between debris accumulation and glacier <span class="hlt">mass</span> balance. To investigate the impact of debris transport on the response of a glacier to recent and future climate change, we applied this model to a large debris-covered Himalayan glacier-Khumbu Glacier in Nepal. Our results demonstrate that supraglacial debris prolongs the response of the glacier to warming and causes lowering of the glacier surface in situ, concealing the magnitude of <span class="hlt">mass</span> loss when compared with estimates based on glacierised area. Since the Little <span class="hlt">Ice</span> Age, Khumbu Glacier has lost 34% of its volume while its area has reduced by only 6%. We predict a decrease in glacier volume of 8-10% by AD2100, accompanied by dynamic and physical detachment of the debris-covered tongue from the active glacier within the next 150 yr. This detachment will accelerate rates of glacier decay, and similar changes are likely for other debris-covered glaciers in the Himalaya.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150019752','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150019752"><span>Preliminary Findings of Inflight <span class="hlt">Icing</span> Field Test to Support <span class="hlt">Icing</span> Remote Sensing Technology Assessment</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>King, Michael; Reehorst, Andrew; Serke, Dave</p> <p>2015-01-01</p> <p>NASA and the National Center for Atmospheric Research have developed an <span class="hlt">icing</span> remote sensing technology that has demonstrated skill at detecting and classifying <span class="hlt">icing</span> hazards in a vertical column above an instrumented ground station. This technology has recently been extended to provide volumetric coverage surrounding an airport. Building on the existing vertical pointing system, the new method for providing volumetric coverage will utilize a vertical pointing cloud radar, a multifrequency microwave radiometer with azimuth and elevation pointing, and a NEXRAD radar. The new terminal area <span class="hlt">icing</span> remote sensing system processes the data streams from these instruments to derive temperature, liquid water <span class="hlt">content</span>, and cloud droplet size for each examined point in space. These data are then combined to ultimately provide <span class="hlt">icing</span> hazard classification along defined approach paths into an airport.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014P%26SS...96...62V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014P%26SS...96...62V"><span>Ganymede's internal structure including thermodynamics of magnesium sulfate oceans in contact with <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>Vance, Steve; Bouffard, Mathieu; Choukroun, Mathieu; Sotin, Christophe</p> <p>2014-06-01</p> <p>The large icy moons of Jupiter contain vast quantities of liquid water, a key ingredient for life. Ganymede and Callisto are weaker candidates for habitability than Europa, in part because of the model-based assumption that high-pressure <span class="hlt">ice</span> layers cover their seafloors and prevent significant water-rock interaction. Water-rock interactions may occur, however, if heating at the rock-<span class="hlt">ice</span> interface melts the high pressure <span class="hlt">ice</span>. Highly saline fluids would be gravitationally stable, and might accumulate under the <span class="hlt">ice</span> due to upward migration, refreezing, and fractionation of salt from less concentrated liquids. To assess the influence of salinity on Ganymede's internal structure, we use available phase-equilibrium data to calculate activity coefficients and predict the freezing of water <span class="hlt">ice</span> in the presence of aqueous magnesium sulfate. We couple this new equation of state with thermal profiles in Ganymede's interior-employing recently published thermodynamic data for the aqueous phase-to estimate the thicknesses of layers of <span class="hlt">ice</span> I, III, V, and VI. We compute core and silicate mantle radii consistent with available constraints on Ganymede's <span class="hlt">mass</span> and gravitational moment of inertia. Mantle radii range from 800 to 900 km for the values of salt and heat flux considered here (4-44 mW m-2 and 0 to 10 wt% MgSO4). Ocean concentrations with salinity higher than 10 wt% have little high pressure <span class="hlt">ice</span>. Even in a Ganymede ocean that is mostly liquid, achieving such high ocean salinity is permissible for the range of likely S/Si ratios. However, elevated salinity requires a smaller silicate mantle radius to satisfy <span class="hlt">mass</span> and moment-of-inertia constraints, so <span class="hlt">ice</span> VI is always present in Ganymede's ocean. For lower values of heat flux, oceans with salinity as low as 3 wt% can co-exist with <span class="hlt">ice</span> III. Available experimental data indicate that <span class="hlt">ice</span> phases III and VI become buoyant for salinity higher than 5 wt% and 10 wt%, respectively. Similar behavior probably occurs for <span class="hlt">ice</span> V at salinities</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24322733','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24322733"><span>Infrared and reflectron time-of-flight <span class="hlt">mass</span> spectroscopic analysis of methane (CH4)-carbon monoxide (CO) <span class="hlt">ices</span> exposed to ionization radiation--toward the formation of carbonyl-bearing molecules in extraterrestrial <span class="hlt">ices</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kaiser, Ralf I; Maity, Surajit; Jones, Brant M</p> <p>2014-02-28</p> <p><span class="hlt">Ice</span> mixtures of methane and carbon monoxide were exposed to ionizing radiation in the form of energetic electrons at 5.5 K to investigate the formation of carbonyl bearing molecules in extraterrestrial <span class="hlt">ices</span>. The radiation induced chemical processing of the mixed <span class="hlt">ices</span> along with their isotopically labeled counterparts was probed online and in situ via infrared spectroscopy (solid state) aided with reflectron time-of-flight <span class="hlt">mass</span> spectrometry (ReTOFMS) coupled to single photon photoionization (PI) at 10.49 eV (gas phase). Deconvolution of the carbonyl absorption feature centered at 1727 cm(-1) in the processed <span class="hlt">ices</span> and subsequent kinetic fitting to the temporal growth of the newly formed species suggests the formation of acetaldehyde (CH3CHO) together with four key classes of carbonyl-bearing molecules: (i) alkyl aldehydes, (ii) alkyl ketones, (iii) α,β-unsaturated ketones/aldehydes and (iv) α,β,γ,δ-unsaturated ketones/α,β-dicarbonyl compounds in keto-enol form. The mechanistical studies indicate that acetaldehyde acts as the key building block of higher aldehydes (i) and ketones (ii) with unsaturated ketones/aldehydes (iii) and/or α,β-dicarbonyl compounds (iv) formed from the latter. Upon sublimation of the newly synthesized molecules, ReTOFMS together with isotopic shifts of the <span class="hlt">mass</span>-to-charge ratios was exploited to identify eleven product classes containing molecules with up to six carbon atoms, which can be formally derived from C1-C5 hydrocarbons incorporating up to three carbon monoxide building blocks. The classes are (i) saturated aldehydes/ketones, (ii) unsaturated aldehydes/ketones, (iii) doubly unsaturated aldehydes/ketones, (iv) saturated dicarbonyls (aldehydes/ketones), (v) unsaturated dicarbonyls (aldehydes/ketones), (vi) saturated tricarbonyls (aldehydes/ketones), molecules containing (vii) one carbonyl - one alcohol (viii), two carbonyls - one alcohol, (ix) one carbonyl - two alcohol groups along with (x) alcohols and (xi) diols. Reaction</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1912373U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1912373U"><span>Comparison of ocean <span class="hlt">mass</span> <span class="hlt">content</span> change from direct and inversion based approaches</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Uebbing, Bernd; Kusche, Jürgen; Rietbroek, Roelof</p> <p>2017-04-01</p> <p>The GRACE satellite mission provides an indispensable tool for measuring oceanic <span class="hlt">mass</span> variations. Such time series are essential to separate global mean sea level rise in thermosteric and <span class="hlt">mass</span> driven contributions, and thus to constrain ocean heat <span class="hlt">content</span> and (deep) ocean warming when viewed together with altimetry and Argo data. However, published estimates over the GRACE era differ, not only depending on the time window considered. Here, we will look into sources of such differences with direct and inverse approaches. Deriving ocean <span class="hlt">mass</span> time series requires several processing steps; choosing a GRACE (and altimetry and Argo) product, data coverage, masks and filters to be applied in either spatial or spectral domain, corrections related to spatial leakage, GIA and geocenter motion need to be accounted for. In this study, we quantify the effects of individual processing choices and assumptions of the direct and inversion based approaches to derive ocean <span class="hlt">mass</span> <span class="hlt">content</span> change. Furthermore, we compile the different estimates from existing literature and sources, to highlight the differences.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012SPIE.8315E..0AN','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012SPIE.8315E..0AN"><span>A <span class="hlt">content</span>-based retrieval of mammographic <span class="hlt">masses</span> using the curvelet descriptor</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Narváez, Fabian; Díaz, Gloria; Gómez, Francisco; Romero, Eduardo</p> <p>2012-03-01</p> <p>Computer-aided diagnosis (CAD) that uses <span class="hlt">content</span> based image retrieval (CBIR) strategies has became an important research area. This paper presents a retrieval strategy that automatically recovers mammography <span class="hlt">masses</span> from a virtual repository of mammographies. Unlike other approaches, we do not attempt to segment <span class="hlt">masses</span> but instead we characterize the regions previously selected by an expert. These regions are firstly curvelet transformed and further characterized by approximating the marginal curvelet subband distribution with a generalized gaussian density (GGD). The <span class="hlt">content</span> based retrieval strategy searches similar regions in a database using the Kullback-Leibler divergence as the similarity measure between distributions. The effectiveness of the proposed descriptor was assessed by comparing the automatically assigned label with a ground truth available in the DDSM database.1 A total of 380 <span class="hlt">masses</span> with different shapes, sizes and margins were used for evaluation, resulting in a mean average precision rate of 89.3% and recall rate of 75.2% for the retrieval task.</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/2017EGUGA..19.1573J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.1573J"><span>Coupled <span class="hlt">ice</span> sheet-ocean modelling to investigate ocean driven melting of marine <span class="hlt">ice</span> sheets in Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jong, Lenneke; Gladstone, Rupert; Galton-Fenzi, Ben</p> <p>2017-04-01</p> <p>Ocean induced melting below the <span class="hlt">ice</span> shelves of marine <span class="hlt">ice</span> sheets is a major source of uncertainty for predictions of <span class="hlt">ice</span> <span class="hlt">mass</span> loss and Antarctica's resultant contribution to future sea level rise. The floating <span class="hlt">ice</span> shelves provide a buttressing force against the flow of <span class="hlt">ice</span> across the grounding line into the ocean. Thinning of these <span class="hlt">ice</span> shelves due to an increase in melting reduces this force and can lead to an increase in the discharge of grounded <span class="hlt">ice</span>. Fully coupled modelling of <span class="hlt">ice</span> sheet-ocean interactions is key to improving understanding the influence of the Southern ocean on the evolution of the Antarctic <span class="hlt">ice</span> sheet, and to predicting its future behaviour under changing climate conditions. Coupling of ocean and <span class="hlt">ice</span> sheet models is needed to provide more realistic melt rates at the base of <span class="hlt">ice</span> shelves and hence make better predictions of the behaviour of the grounding line and the shape of the <span class="hlt">ice</span>-shelf cavity as the <span class="hlt">ice</span> sheet evolves. The Framework for <span class="hlt">Ice</span> Sheet - Ocean Coupling (FISOC) has been developed to provide a flexible platform for performing coupled <span class="hlt">ice</span> sheet - ocean modelling experiments. We present preliminary results using FISOC to couple the Regional Ocean Modelling System (ROMS) with Elmer/<span class="hlt">Ice</span> in idealised experiments Marine <span class="hlt">Ice</span> 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 <span class="hlt">ice</span> and grounding line retreat.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19870027099&hterms=microwaves+water+structure&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dmicrowaves%2Bwater%2Bstructure','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19870027099&hterms=microwaves+water+structure&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dmicrowaves%2Bwater%2Bstructure"><span>Satellite microwave and in situ observations of the Weddell Sea <span class="hlt">ice</span> cover and its marginal <span class="hlt">ice</span> zone</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Comiso, J. C.; Sullivan, C. W.</p> <p>1986-01-01</p> <p>The radiative and physical characteristics of the Weddell Sea <span class="hlt">ice</span> cover and its marginal <span class="hlt">ice</span> zone are analyzed using multichannel satellite passive microwave data and ship and helicopter observations obtained during the 1983 Antarctic Marine Ecosystem Research. Winter and spring brightness temperatures are examined; spatial variability in the brightness temperatures of consolidated <span class="hlt">ice</span> in winter and spring cyclic increases and decrease in brightness temperatures of consolidated <span class="hlt">ice</span> with an amplitude of 50 K at 37 GHz and 20 K at 18 GHz are observed. The roles of variations in air temperature and surface characteristics in the variability of spring brightness temperatures are investigated. <span class="hlt">Ice</span> concentrations are derived using the frequency and polarization techniques, and the data are compared with the helicopter and ship observations. Temporal changes in the <span class="hlt">ice</span> margin structure and the <span class="hlt">mass</span> balance of fresh water and of biological features of the marginal <span class="hlt">ice</span> zone are studied.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C54A..02H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C54A..02H"><span><span class="hlt">Ice</span> shelf thickness change from 2010 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>Hogg, A.; Shepherd, A.; Gilbert, L.; Muir, A. S.</p> <p>2017-12-01</p> <p>Floating <span class="hlt">ice</span> shelves fringe 74 % of Antarctica's coastline, providing a direct link between the <span class="hlt">ice</span> sheet and the surrounding oceans. Over the last 25 years, <span class="hlt">ice</span> shelves have retreated, thinned, and collapsed catastrophically. While change in the <span class="hlt">mass</span> of floating <span class="hlt">ice</span> shelves has only a modest steric impact on the rate of sea-level rise, their loss can affect the <span class="hlt">mass</span> balance of the grounded <span class="hlt">ice</span>-sheet by influencing the rate of <span class="hlt">ice</span> flow inland, due to the buttressing effect. Here we use CryoSat-2 altimetry data to map the detailed pattern of <span class="hlt">ice</span> shelf thickness change in Antarctica. We exploit the dense spatial sampling and repeat coverage provided by the CryoSat-2 synthetic aperture radar interferometric mode (SARIn) to investigate data acquired between 2010 to the present day. We find that <span class="hlt">ice</span> shelf thinning rates can exhibit large fluctuations over short time periods, and that the improved spatial resolution of CryoSat-2 enables us to resolve the spatial pattern of thinning with ever greater detail in Antarctica. In the Amundsen Sea, <span class="hlt">ice</span> shelves at the terminus of the Pine Island and Thwaites glaciers have thinned at rates in excess of 5 meters per year for more than two decades. We observe the highest rates of basal melting near to the <span class="hlt">ice</span> sheet grounding line, reinforcing the importance of high resolution datasets. On the Antarctic Peninsula, in contrast to the 3.8 m per decade of thinning observed since 1992, we measure an increase in the surface elevation of the Larsen-C <span class="hlt">Ice</span>-Shelf during the CryoSat-2 period.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70038745','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70038745"><span>History of the Greenland <span class="hlt">Ice</span> Sheet: paleoclimatic insights</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Alley, Richard B.; Andrews, John T.; Brigham-Grette, J.; Clarke, G.K.C.; Cuffey, Kurt M.; Fitzpatrick, J.J.; Funder, S.; Marshall, S.J.; Miller, G.H.; Mitrovica, J.X.; Muhs, D.R.; Otto-Bliesner, B. L.; Polyak, L.; White, J.W.C.</p> <p>2010-01-01</p> <p>Paleoclimatic records show that the Greenland<span class="hlt">Ice</span> Sheet consistently has lost <span class="hlt">mass</span> in response to warming, and grown in response to cooling. Such changes have occurred even at times of slow or zero sea-level change, so changing sea level cannot have been the cause of at least some of the <span class="hlt">ice</span>-sheet changes. In contrast, there are no documented major <span class="hlt">ice</span>-sheet changes that occurred independent of temperature changes. Moreover, snowfall has increased when the climate warmed, but the <span class="hlt">ice</span> sheet lost <span class="hlt">mass</span> nonetheless; increased accumulation in the <span class="hlt">ice</span> sheet's center has not been sufficient to counteract increased melting and flow near the edges. Most documented forcings and <span class="hlt">ice</span>-sheet responses spanned periods of several thousand years, but limited data also show rapid response to rapid forcings. In particular, regions near the <span class="hlt">ice</span> margin have responded within decades. However, major changes of central regions of the <span class="hlt">ice</span> sheet are thought to require centuries to millennia. The paleoclimatic record does not yet strongly constrain how rapidly a major shrinkage or nearly complete loss of the <span class="hlt">ice</span> sheet could occur. The evidence suggests nearly total <span class="hlt">ice</span>-sheet loss may result from warming of more than a few degrees above mean 20th century values, but this threshold is poorly defined (perhaps as little as 2 °C or more than 7 °C). Paleoclimatic records are sufficiently sketchy that the <span class="hlt">ice</span> sheet may have grown temporarily in response to warming, or changes may have been induced by factors other than temperature, without having been recorded.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.amap.no/documents/doc/snow-water-ice-and-permafrost-in-the-arctic-swipa-climate-change-and-the-cryosphere/743','USGSPUBS'); return false;" href="http://www.amap.no/documents/doc/snow-water-ice-and-permafrost-in-the-arctic-swipa-climate-change-and-the-cryosphere/743"><span>Mountain Glaciers and <span class="hlt">Ice</span> Caps</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Ananichheva, Maria; Arendt, Anthony; Hagen, Jon-Ove; Hock, Regine; Josberger, Edward G.; Moore, R. Dan; Pfeffer, William Tad; Wolken, Gabriel J.</p> <p>2011-01-01</p> <p>Projections of future rates of <span class="hlt">mass</span> loss from mountain glaciers and <span class="hlt">ice</span> caps in the Arctic focus primarily on projections of changes in the surface <span class="hlt">mass</span> balance. Current models are not yet capable of making realistic forecasts of changes in losses by calving. Surface <span class="hlt">mass</span> balance models are forced with downscaled output from climate models driven by forcing scenarios that make assumptions about the future rate of growth of atmospheric greenhouse gas concentrations. Thus, <span class="hlt">mass</span> loss projections vary considerably, depending on the forcing scenario used and the climate model from which climate projections are derived. A new study in which a surface <span class="hlt">mass</span> balance model is driven by output from ten general circulation models (GCMs) forced by the IPCC (Intergovernmental Panel on Climate Change) A1B emissions scenario yields estimates of total <span class="hlt">mass</span> loss of between 51 and 136 mm sea-level equivalent (SLE) (or 13% to 36% of current glacier volume) by 2100. This implies that there will still be substantial glacier <span class="hlt">mass</span> in the Arctic in 2100 and that Arctic mountain glaciers and <span class="hlt">ice</span> caps will continue to influence global sea-level change well into the 22nd century.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1918710V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1918710V"><span>A Transient Initialization Routine of the Community <span class="hlt">Ice</span> Sheet Model for the Greenland <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>van der Laan, Larissa; van den Broeke, Michiel; Noël, Brice; van de Wal, Roderik</p> <p>2017-04-01</p> <p>The Community <span class="hlt">Ice</span> Sheet Model (CISM) is to be applied in future simulations of the Greenland <span class="hlt">Ice</span> Sheet under a range of climate change scenarios, determining the sensitivity of the <span class="hlt">ice</span> sheet to individual climatic forcings. In order to achieve reliable results regarding <span class="hlt">ice</span> sheet stability and assess the probability of future occurrence of tipping points, a realistic initial <span class="hlt">ice</span> 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 <span class="hlt">mass</span> 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 <span class="hlt">ice</span> sheet with a transient memory of the last glacial-interglacial cycle, which will serve as the future runs' initial condition.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030004821','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030004821"><span>ICESat: <span class="hlt">Ice</span>, Cloud and Land Elevation Satellite</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zwally, Jay; Shuman, Christopher</p> <p>2002-01-01</p> <p><span class="hlt">Ice</span> exists in the natural environment in many forms. The Earth dynamic <span class="hlt">ice</span> features shows that at high elevations and/or high latitudes,snow that falls to the ground can gradually build up tu form thick consolidated <span class="hlt">ice</span> <span class="hlt">masses</span> 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 <span class="hlt">ice</span> sheet, separates the <span class="hlt">ice</span> areas that melt on the surface and become show free in summer (net ablation zone) from the <span class="hlt">ice</span> 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 <span class="hlt">ice</span> is called firm.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA159060','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA159060"><span>Marginal <span class="hlt">Ice</span> Zone Bibliography.</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1985-06-01</p> <p>A Voyage of Discovery. George Deacon 70th An-niversary Volume, (M. Angel, ed.), Pergamon Press, Oxford, p.15-41. Coachman, L.K., C.A. Barnes, 1961...some polar contrasts. In: S "" RUsium on Antarctic <span class="hlt">Ice</span> and Water <span class="hlt">Masses</span>, ( George Deacon, ed.), Sci- 72 Lebedev, A.A., 1968: Zone of possible <span class="hlt">icing</span> of...Atlantic and Western Europe. British Meteorological Office. Geophysical Memoirs, 4(41). Brost , R.A., J.C. Wyngaard, 1978: A model study of the stably</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> sheet 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 <span class="hlt">mass</span> balance of <span class="hlt">ice</span> sheets 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> sheets 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> Sheet 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> sheet runoff is primarily associated with albedo effects due to deposition of ash sourced from high-latitude volcanic eruptions. Climate and snowpack <span class="hlt">mass</span>-balance simulations show evidence for enhanced <span class="hlt">ice</span> sheet runoff under volcanically forced conditions despite atmospheric cooling. The sensitivity of past <span class="hlt">ice</span> sheets to volcanic ashfall highlights the need for an accurate coupling between atmosphere and <span class="hlt">ice</span> sheet components in climate models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6085044-arctic-ice-shelves-ice-islands-origin-growth-disintegration-physical-characteristics-structural-stratigraphic-variability-dynamics','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6085044-arctic-ice-shelves-ice-islands-origin-growth-disintegration-physical-characteristics-structural-stratigraphic-variability-dynamics"><span>Arctic <span class="hlt">ice</span> shelves and <span class="hlt">ice</span> islands: Origin, growth and disintegration, physical characteristics, structural-stratigraphic variability, and 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>Jeffries, M.O.</p> <p>1992-08-01</p> <p><span class="hlt">Ice</span> shelves are thick, floating <span class="hlt">ice</span> <span class="hlt">masses</span> most often associated with Antarctica where they are seaward extensions of the grounded Antarctic <span class="hlt">ice</span> sheet and sources of many icebergs. However, there are also <span class="hlt">ice</span> shelves in the Arctic, primarily located along the north coast of Ellesmere Island in the Canadian High Arctic. The only <span class="hlt">ice</span> shelves in North America and the most extensive in the north polar region, the Ellesmere <span class="hlt">ice</span> shelves originate from glaciers and from sea <span class="hlt">ice</span> and are the source of <span class="hlt">ice</span> islands, the tabular icebergs of the Arctic Ocean. The present state of knowledge and understanding ofmore » these <span class="hlt">ice</span> features is summarized in this paper. It includes historical background to the discovery and early study of <span class="hlt">ice</span> shelves and <span class="hlt">ice</span> islands, including the use of <span class="hlt">ice</span> islands as floating laboratories for polar geophysical research. Growth mechanisms and age, the former extent and the twentieth century disintegration of the Ellesmere <span class="hlt">ice</span> shelves, and the processes and mechanisms of <span class="hlt">ice</span> island calving are summarized. Surface features, thickness, thermal regime, and the size, shape, and numbers of <span class="hlt">ice</span> islands are discussed. The structural-stratigraphic variability of <span class="hlt">ice</span> islands and <span class="hlt">ice</span> shelves and the complex nature of their growth and development are described. Large-scale and small-scale dynamics of <span class="hlt">ice</span> islands are described, and the results of modeling their drift and recurrence intervals are presented. The conclusion identifies some unanswered questions and future research opportunities and needs. 97 refs., 18 figs.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.C41A0044S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.C41A0044S"><span>Studies of contemporary glacier basal <span class="hlt">ice</span> cryostructures to identify buried basal <span class="hlt">ice</span> in the permafrost: an example from the Matanuska Glacier, Alaska.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stephani, E.; Fortier, D.; Kanevskiy, M.; Dillon, M.; Shur, Y.</p> <p>2007-12-01</p> <p>In the permafrost, massive <span class="hlt">ice</span> bodies occur as buried glacier <span class="hlt">ice</span>, aufeis <span class="hlt">ice</span>, recrystalized snow, massive segregated <span class="hlt">ice</span>, injection <span class="hlt">ice</span>, <span class="hlt">ice</span> wedges or <span class="hlt">ice</span> formed in underground cavities ("pool <span class="hlt">ice</span>", "thermokarst-cave <span class="hlt">ice</span>"). The origin of massive <span class="hlt">ice</span> bodies in the permafrost bears considerable implications for the reconstructions of paleoenvironments and paleoclimates. Our work aims to help the permafrost scientists working on massive icy sediments to distinguish buried basal glacier <span class="hlt">ice</span> from other types of buried <span class="hlt">ice</span>. To do so, the properties and structure of contemporary basal <span class="hlt">ice</span> must be well known. Field investigations at the Matanuska Glacier (Chugach range, South-central Alaska), consisted in descriptions and sampling of natural basal <span class="hlt">ice</span> exposures. We have used the basal <span class="hlt">ice</span> facies classification of Lawson (1979) which is simple, easy to use in the field and provides a good framework for the description of basal <span class="hlt">ice</span> exposures. Cores were extracted and brought back to the laboratory for water and grain-size analyses. The sediments forming the cryostructure were mostly polymodal, poorly sorted gravelly silt to gravelly fine sand, with mud <span class="hlt">contents</span> generally over 50%. These data will be used to calibrate three-dimensional (3D) models produced from micro-tomographic scans of basal <span class="hlt">ice</span> which will produce quantitative estimates of volumetric <span class="hlt">ice</span> and sediments <span class="hlt">contents</span> of basal <span class="hlt">ice</span> cryostructures. Ultimately, visual qualitative and quantitative characterization of the basal <span class="hlt">ice</span> components of 3D models together with field observations and laboratory analysis will allow for a new micro-facies and cryostructures classification of the basal <span class="hlt">ice</span>. Our work will also have applications in glaciology, glacial geology, geomorphology, Quaternary and paleo-climatological studies based on inferences made from the structure of basal glacier <span class="hlt">ice</span>. This paper presents the internal composition of the basal <span class="hlt">ice</span> facies in terms of cryostructures assemblages (Fortier et al.: 2007) and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.7840N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.7840N"><span>Online sea <span class="hlt">ice</span> data platform: www.seaiceportal.de</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nicolaus, Marcel; Asseng, Jölund; Bartsch, Annekathrin; Bräuer, Benny; Fritzsch, Bernadette; Grosfeld, Klaus; Hendricks, Stefan; Hiller, Wolfgang; Heygster, Georg; Krumpen, Thomas; Melsheimer, Christian; Ricker, Robert; Treffeisen, Renate; Weigelt, Marietta; Nicolaus, Anja; Lemke, Peter</p> <p>2016-04-01</p> <p>There is an increasing public interest in sea <span class="hlt">ice</span> information from both Polar Regions, which requires up-to-date background information and data sets at different levels for various target groups. In order to serve this interest and need, seaiceportal.de (originally: meereisportal.de) was developed as a comprehensive German knowledge platform on sea <span class="hlt">ice</span> and its snow cover in the Arctic and Antarctic. It was launched in April 2013. Since then, the <span class="hlt">content</span> and selection of data sets increased and the data portal received increasing attention, also from the international science community. Meanwhile, we are providing near-real time and archive data of many key parameters of sea <span class="hlt">ice</span> and its snow cover. The data sets result from measurements acquired by various platforms as well as numerical simulations. Satellite observations of sea <span class="hlt">ice</span> concentration, freeboard, thickness and drift are available as gridded data sets. Sea <span class="hlt">ice</span> and snow temperatures and thickness as well as atmospheric parameters are available from autonomous platforms (buoys). Additional ship observations, <span class="hlt">ice</span> station measurements, and mooring time series are compiled as data collections over the last decade. In parallel, we are continuously extending our meta-data and uncertainty information for all data sets. In addition to the data portal, seaiceportal.de provides general comprehensive background information on sea <span class="hlt">ice</span> and snow as well as expert statements on recent observations and developments. This <span class="hlt">content</span> is mostly in German in order to complement the various existing international sites for the German speaking public. We will present the portal, its <span class="hlt">content</span> and function, but we are also asking for direct user feedback.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017jwst.prop.1309M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017jwst.prop.1309M"><span><span class="hlt">Ice</span>Age: Chemical Evolution of <span class="hlt">Ices</span> during Star Formation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McClure, Melissa; Bailey, J.; Beck, T.; Boogert, A.; Brown, W.; Caselli, P.; Chiar, J.; Egami, E.; Fraser, H.; Garrod, R.; Gordon, K.; Ioppolo, S.; Jimenez-Serra, I.; Jorgensen, J.; Kristensen, L.; Linnartz, H.; McCoustra, M.; Murillo, N.; Noble, J.; Oberg, K.; Palumbo, M.; Pendleton, Y.; Pontoppidan, K.; Van Dishoeck, E.; Viti, S.</p> <p>2017-11-01</p> <p>Icy grain mantles are the main reservoir for volatile elements in star-forming regions across the Universe, as well as the formation site of pre-biotic complex organic molecules (COMs) seen in our Solar System. We propose to trace the evolution of pristine and complex <span class="hlt">ice</span> chemistry in a representative low-<span class="hlt">mass</span> star-forming region through observations of a: pre-stellar core, Class 0 protostar, Class I protostar, and protoplanetary disk. Comparing high spectral resolution (R 1500-3000) and sensitivity (S/N 100-300) observations from 3 to 15 um to template spectra, we will map the spatial distribution of <span class="hlt">ices</span> down to 20-50 AU in these targets to identify when, and at what visual extinction, the formation of each <span class="hlt">ice</span> species begins. Such high-resolution spectra will allow us to search for new COMs, as well as distinguish between different <span class="hlt">ice</span> morphologies,thermal histories, and mixing environments. The analysis of these data will result in science products beneficial to Cycle 2 proposers. A newly updated public laboratory <span class="hlt">ice</span> database will provide feature identifications for all of the expected <span class="hlt">ices</span>, while a chemical model fit to the observed <span class="hlt">ice</span> abundances will be released publically as a grid, with varied metallicity and UV fields to simulate other environments. We will create improved algorithms to extract NIRCAM WFSS spectra in crowded fields with extended sources as well as optimize the defringing of MIRI LRS spectra in order to recover broad spectral features. We anticipate that these resources will be particularly useful for astrochemistry and spectroscopy of fainter, extended targets like star forming regions of the SMC/LMC or more distant galaxies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170008004','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170008004"><span>Bimodal SLD <span class="hlt">Ice</span> Accretion on a NACA 0012 Airfoil Model</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Potapczuk, Mark; Tsao, Jen-Ching; King-Steen, Laura</p> <p>2016-01-01</p> <p>This presentation describes the results of <span class="hlt">ice</span> accretion measurements on a NACA 0012 airfoil model, from the NASA <span class="hlt">Icing</span> Research Tunnel, using an <span class="hlt">icing</span> cloud composed of a bimodal distribution of Supercooled Large Droplets. The data consists of photographs, laser scans of the <span class="hlt">ice</span> surface, and measurements of the <span class="hlt">mass</span> of <span class="hlt">ice</span> for each <span class="hlt">icing</span> condition. The results of <span class="hlt">ice</span> shapes accumulated as a result of exposure to an <span class="hlt">icing</span> cloud with a bimodal droplet distribution were compared to the <span class="hlt">ice</span> shapes resulting from an equivalent cloud composed of a droplet distribution with a standard bell curve shape.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45.3173N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45.3173N"><span>New <span class="hlt">Mass</span>-Conserving Bedrock Topography for Pine Island Glacier Impacts Simulated Decadal Rates of <span class="hlt">Mass</span> Loss</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nias, I. J.; Cornford, S. L.; Payne, A. J.</p> <p>2018-04-01</p> <p>High-resolution <span class="hlt">ice</span> flow modeling requires bedrock elevation and <span class="hlt">ice</span> thickness data, consistent with one another and with modeled physics. Previous studies have shown that gridded <span class="hlt">ice</span> thickness products that rely on standard interpolation techniques (such as Bedmap2) can be inconsistent with the conservation of <span class="hlt">mass</span>, given observed velocity, surface elevation change, and surface <span class="hlt">mass</span> balance, for example, near the grounding line of Pine Island Glacier, West Antarctica. Using the BISICLES <span class="hlt">ice</span> flow model, we compare results of simulations using both Bedmap2 bedrock and thickness data, and a new interpolation method that respects <span class="hlt">mass</span> conservation. We find that simulations using the new geometry result in higher sea level contribution than Bedmap2 and reveal decadal-scale trends in the <span class="hlt">ice</span> stream dynamics. We test the impact of several sliding laws and find that it is at least as important to accurately represent the bedrock and initial <span class="hlt">ice</span> thickness as the choice of sliding law.</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> Sheets</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> sheets 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> <span class="hlt">masses</span> 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('https://ntrs.nasa.gov/search.jsp?R=20080045463&hterms=Ackerman&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAuthor-Name%26N%3D0%26No%3D40%26Ntt%3DAckerman','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20080045463&hterms=Ackerman&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAuthor-Name%26N%3D0%26No%3D40%26Ntt%3DAckerman"><span>Observing <span class="hlt">Ice</span> in Clouds from Space</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ackerman, S.; Star, D. O'C.; Skofronick-Jackson, G.; Evans, F.; Wang, J. R.; Norris, P.; daSilva, A.; Soden, B.</p> <p>2006-01-01</p> <p>There are many satellite observations of cloud top properties and the liquid and rain <span class="hlt">content</span> of clouds, however, we do not yet quantitatively understand the processes that control the water budget of the upper troposphere where <span class="hlt">ice</span> is the predominant phase, and how these processes are linked to precipitation processes and the radiative energy budget. The <span class="hlt">ice</span> in clouds in the upper troposphere either melts into rain or is detrained, and persists, as cirrus clouds affecting the hydrological and energy cycle, respectively. Fully modeling the Earth's climate and improving weather and climate forecasts requires accurate satellite measurements of various cloud properties at the temporal and spatial scales of cloud processes. These properties include cloud horizontal and vertical structure, cloud water <span class="hlt">content</span> and some measure of particle sizes and shapes. The uncertainty in knowledge of these <span class="hlt">ice</span> characteristics is reflected in the large discrepancies in model simulations of the upper tropospheric water budget. Model simulations are sensitive to the partition of <span class="hlt">ice</span> between precipitation and outflow processes, i.e., to the parameterization of <span class="hlt">ice</span> clouds and <span class="hlt">ice</span> processes. One barrier to achieving accurate global <span class="hlt">ice</span> cloud properties is the lack of adequate observations at millimeter and submillimeter wavelengths (183-874 GHz). Recent advances in instrumentation have allowed for the development and implementation of an airborne submillimeter-wave radiometer. The brightness temperatures at these frequencies are especially sensitive to cirrus <span class="hlt">ice</span> particle sizes (because they are comparable to the wavelength). This allows for more accurate <span class="hlt">ice</span> water path estimates when multiple channels are used to probe into the cloud layers. Further, submillimeter wavelengths offer simplicity in the retrieval algorithms because they do not probe into the liquid and near surface portions of clouds, thus requiring only one term of the radiative transfer equation (<span class="hlt">ice</span> scattering) to relate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27918670','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27918670"><span>Improvement of <span class="hlt">Ice</span> Hockey Players' On-<span class="hlt">Ice</span> Sprint With Combined Plyometric and Strength Training.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dæhlin, Torstein E; Haugen, Ole C; Haugerud, Simen; Hollan, Ivana; Raastad, Truls; Rønnestad, Bent R</p> <p>2017-08-01</p> <p>Combined plyometric and strength training has previously been suggested as a strategy to improve skating performance in <span class="hlt">ice</span> hockey players. However, the effects of combined plyometric and strength training have not previously been compared with the effects of strength training only. To compare the effects of combined plyometric and strength training on <span class="hlt">ice</span> hockey players' skating sprint performance with those of strength training only. Eighteen participants were randomly assigned to 2 groups that completed 5 strength-training sessions/wk for 8 wk. One group included plyometric exercises at the start of 3 sessions/wk (PLY+ST), and the other group included core exercises in the same sessions (ST). Tests of 10- and 35-m skating sprints, horizontal jumping, 1-repetition-maximum (1 RM) squat, skating multistage aerobic test (SMAT), maximal oxygen consumption, repeated cycle sprints, and body composition were performed before and after the intervention. The participants increased their 1RM squat, lean <span class="hlt">mass</span>, and body <span class="hlt">mass</span> (P < .05), with no difference between the groups. Furthermore, they improved their 3×broad jump, repeated cycle sprint, and SMAT performance (P < .05), with no difference between the groups. PLY+ST gained a larger improvement in 10-m on-<span class="hlt">ice</span> sprint performance than ST (P < .025). Combining plyometric and strength training for 8 wk was superior to strength training alone at improving 10-m on-<span class="hlt">ice</span> sprint performance in high-level <span class="hlt">ice</span> hockey players.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19294740','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19294740"><span>Prediction of <span class="hlt">ice</span> <span class="hlt">content</span> in biological model solutions when frozen under high pressure.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Guignon, B; Aparicio, C; Otero, L; Sanz, P D</p> <p>2009-01-01</p> <p>High pressure is, at least, as effective as cryoprotective agents (CPAs) and are used for decreasing both homogenous nucleation and freezing temperatures. This fact gives rise to a great variety of possible cryopreservation processes under high pressure. They have not been optimized yet, since they are relatively recent and are mainly based on the pressure-temperature phase diagram of pure water. Very few phase diagrams of biological material are available under pressure. This is owing to the lack of suitable equipment and to the difficulties encountered in carrying out the measurements. Different aqueous solutions of salt and CPAs as biological models are studied in the range of 0 degrees C down to -35 degrees C, 0.1 up to 250 MPa, and 0-20% w/w total solute concentration. The phase transition curves of glycerol and of sodium chloride with either glycerol or sucrose in aqueous solutions are determined in a high hydrostatic pressure vessel. The experimental phase diagrams of binary solutions were well described by a third-degree polynomial equation. It was also shown that Robinson and Stokes' equation at high pressure succeeds in predicting the phase diagrams of both binary and ternary solutions. The solute cryoconcentration and the <span class="hlt">ice</span> <span class="hlt">content</span> were calculated as a function of temperature and pressure conditions during the freezing of a binary solution. This information should provide a basis upon which high-pressure cryopreservation processes may be performed and the damages derived from <span class="hlt">ice</span> formation evaluated. (c) 2009 American Institute of Chemical Engineers Biotechnol.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19840011675','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19840011675"><span>Hydromechanics and heat and <span class="hlt">mass</span> exchange in weightlessness (Russian book): Table of <span class="hlt">contents</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Avduyevskiy, V. S.; Poleshayev, V. I.</p> <p>1983-01-01</p> <p>The table of <span class="hlt">contents</span> is given for a book on hydromechanics and heat and <span class="hlt">mass</span> exchange in weightlessness. The book covers such subjects as hydromechanics, convection and heat and <span class="hlt">mass</span> exchange, and technological experiments and complicated systems.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_22 --> <div id="page_23" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="441"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20020061866','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20020061866"><span><span class="hlt">Icing</span> Sensor Probe</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Emery, Edward; Kok, Gregory L.</p> <p>2002-01-01</p> <p>Aircraft <span class="hlt">icing</span> is a serious safety problem for the general aviation and some commuter transport airplanes. There has been tremendous growth in the commuter aviation industry in the last few years, Since these type of aircraft generally operate at lower altitudes they consequently spend a far greater proportion of their time operating in <span class="hlt">icing</span> conditions. For the past thirty years airborne and ground based facilities have relied primarily on two types of cloud physics instrumentation to measure the characteristics of <span class="hlt">icing</span> clouds: hot wire liquid water <span class="hlt">content</span> probes and laser based particle sizing probes for the measurement of water droplet size. The instrumentation is severely limited by the technology that was developed during the 1970's and is quite large in size. The goal of this research is to develop one instrument with a wide bandwidth, better response time, higher resolution, user selectability, and small and lightweight. NASA Glenn Research Center, Droplet Measurement Technology, and Meteorology Society of Canada have developed a collaborative effort to develop such an instrument. This paper describes the development and test results of the prototype <span class="hlt">Icing</span> Sensor Probe.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040034042','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040034042"><span>Effective <span class="hlt">Ice</span> Particle Densities for Cold Anvil Cirrus</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Heymsfield, Andrew J.; Schmitt, Carl G.; Bansemer, Aaron; Baumgardner, Darrel; Weinstock, Elliot M.; Smith, Jessica</p> <p>2002-01-01</p> <p>This study derives effective <span class="hlt">ice</span> particle densities from data collected from the NASA WB-57F aircraft near the tops of anvils during the Cirrus Regional Study of Tropical Anvils and Cirrus Layers (CRYSTAL) Florida Area Cirrus Experiment (FACE) in southern Florida in July 2002. The effective density, defined as the <span class="hlt">ice</span> particle <span class="hlt">mass</span> divided by the volume of an equivalent diameter liquid sphere, is obtained for particle populations and single sizes containing mixed particle habits using measurements of condensed water <span class="hlt">content</span> and particle size distributions. The mean effective densities for populations decrease with increasing slopes of the gamma size distributions fitted to the size distributions. The population-mean densities range from near 0.91 g/cu m to 0.15 g/cu m. Effective densities for single sizes obey a power-law with an exponent of about -0.55, somewhat less steep than found from earlier studies. Our interpretations apply to samples where particle sizes are generally below 200-300 microns in maximum dimension because of probe limitations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016TCry...10.2501P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016TCry...10.2501P"><span><span class="hlt">Ice</span> core evidence for a 20th century increase in surface <span class="hlt">mass</span> balance in coastal Dronning Maud Land, East Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Philippe, Morgane; Tison, Jean-Louis; Fjøsne, Karen; Hubbard, Bryn; Kjær, Helle A.; Lenaerts, Jan T. M.; Drews, Reinhard; Sheldon, Simon G.; De Bondt, Kevin; Claeys, Philippe; Pattyn, Frank</p> <p>2016-10-01</p> <p><span class="hlt">Ice</span> cores provide temporal records of surface <span class="hlt">mass</span> balance (SMB). Coastal areas of Antarctica have relatively high and variable SMB, but are under-represented in records spanning more than 100 years. Here we present SMB reconstruction from a 120 m-long <span class="hlt">ice</span> core drilled in 2012 on the Derwael <span class="hlt">Ice</span> Rise, coastal Dronning Maud Land, East Antarctica. Water stable isotope (δ18O and δD) stratigraphy is supplemented by discontinuous major ion profiles and continuous electrical conductivity measurements. The base of the <span class="hlt">ice</span> core is dated to AD 1759 ± 16, providing a climate proxy for the past ˜ 250 years. The core's annual layer thickness history is combined with its gravimetric density profile to reconstruct the site's SMB history, corrected for the influence of <span class="hlt">ice</span> deformation. The mean SMB for the core's entire history is 0.47 ± 0.02 m water equivalent (w.e.) a-1. The time series of reconstructed annual SMB shows high variability, but a general increase beginning in the 20th century. This increase is particularly marked during the last 50 years (1962-2011), which yields mean SMB of 0.61 ± 0.01 m w.e. a-1. This trend is compared with other reported SMB data in Antarctica, generally showing a high spatial variability. Output of the fully coupled Community Earth System Model (CESM) suggests that, although atmospheric circulation is the main factor influencing SMB, variability in sea surface temperatures and sea <span class="hlt">ice</span> cover in the precipitation source region also explain part of the variability in SMB. Local snow redistribution can also influence interannual variability but is unlikely to influence long-term trends significantly. This is the first record from a coastal <span class="hlt">ice</span> core in East Antarctica to show an increase in SMB beginning in the early 20th century and particularly marked during the last 50 years.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110014136','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110014136"><span>Instrument for Aircraft-<span class="hlt">Icing</span> and Cloud-Physics Measurements</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lilie, Lyle; Bouley, Dan; Sivo, Chris</p> <p>2006-01-01</p> <p>The figure shows a compact, rugged, simple sensor head that is part of an instrumentation system for making measurements to characterize the severity of aircraft-<span class="hlt">icing</span> conditions and/or to perform research on cloud physics. The quantities that are calculated from measurement data acquired by this system and that are used to quantify the severity of <span class="hlt">icing</span> conditions include sizes of cloud water drops, cloud liquid water <span class="hlt">content</span> (LWC), cloud <span class="hlt">ice</span> water <span class="hlt">content</span> (IWC), and cloud total water <span class="hlt">content</span> (TWC). The sensor head is mounted on the outside of an aircraft, positioned and oriented to intercept the ambient airflow. The sensor head consists of an open housing that is heated in a controlled manner to keep it free of <span class="hlt">ice</span> and that contains four hot-wire elements. The hot-wire sensing elements have different shapes and sizes and, therefore, exhibit different measurement efficiencies with respect to droplet size and water phase (liquid, frozen, or mixed). Three of the hot-wire sensing elements are oriented across the airflow so as to intercept incoming cloud water. For each of these elements, the LWC or TWC affects the power required to maintain a constant temperature in the presence of cloud water.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=content+AND+analysis&pg=6&id=EJ994864','ERIC'); return false;" href="https://eric.ed.gov/?q=content+AND+analysis&pg=6&id=EJ994864"><span>Climate Change Discourse in <span class="hlt">Mass</span> Media: Application of Computer-Assisted <span class="hlt">Content</span> Analysis</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>Kirilenko, Andrei P.; Stepchenkova, Svetlana O.</p> <p>2012-01-01</p> <p><span class="hlt">Content</span> analysis of <span class="hlt">mass</span> media publications has become a major scientific method used to analyze public discourse on climate change. We propose a computer-assisted <span class="hlt">content</span> analysis method to extract prevalent themes and analyze discourse changes over an extended period in an objective and quantifiable manner. The method includes the following: (1)…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910004108','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910004108"><span>A review of <span class="hlt">ice</span> accretion data from a model rotor <span class="hlt">icing</span> test and comparison with theory</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Britton, Randall K.; Bond, Thomas H.</p> <p>1991-01-01</p> <p>An experiment was conducted by the Helicopter <span class="hlt">Icing</span> Consortium (HIC) in the NASA Lewis <span class="hlt">Icing</span> Research Tunnel (IRT) in which a 1/6 scale fuselage model of a UH-60A Black Hawk helicopter with a generic rotor was subjected to a wide range of <span class="hlt">icing</span> conditions. The HIC consists of members from NASA, Bell Helicopter, Boeing Helicopter, McDonnell Douglas Helicopters, Sikorsky Aircraft, and Texas A&M University. Data was taken in the form of rotor torque, internal force balance measurements, blade strain gage loading, and two dimensional <span class="hlt">ice</span> shape tracings. A review of the <span class="hlt">ice</span> shape data is performed with special attention given to repeatability and correctness of trends in terms of radial variation, rotational speed, <span class="hlt">icing</span> time, temperature, liquid water <span class="hlt">content</span>, and volumetric median droplet size. Moreover, an indepth comparison between the experimental data and the analysis of NASA's <span class="hlt">ice</span> accretion code LEWICE is given. Finally, conclusions are drawn as to the quality of the <span class="hlt">ice</span> accretion data and the predictability of the data base as a whole. Recommendations are also given for improving data taking technique as well as potential future work.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27679819','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27679819"><span>Geodetic measurements reveal similarities between post-Last Glacial Maximum and present-day <span class="hlt">mass</span> loss from the Greenland <span class="hlt">ice</span> sheet.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Khan, Shfaqat A; Sasgen, Ingo; Bevis, Michael; van Dam, Tonie; Bamber, Jonathan L; Wahr, John; Willis, Michael; Kjær, Kurt H; Wouters, Bert; Helm, Veit; Csatho, Beata; Fleming, Kevin; Bjørk, Anders A; Aschwanden, Andy; Knudsen, Per; Munneke, Peter Kuipers</p> <p>2016-09-01</p> <p>Accurate quantification of the millennial-scale <span class="hlt">mass</span> balance of the Greenland <span class="hlt">ice</span> sheet (GrIS) and its contribution to global sea-level rise remain challenging because of sparse in situ observations in key regions. Glacial isostatic adjustment (GIA) is the ongoing response of the solid Earth to <span class="hlt">ice</span> and ocean load changes occurring since the Last Glacial Maximum (LGM; ~21 thousand years ago) and may be used to constrain the GrIS deglaciation history. We use data from the Greenland Global Positioning System network to directly measure GIA and estimate basin-wide <span class="hlt">mass</span> changes since the LGM. Unpredicted, large GIA uplift rates of +12 mm/year are found in southeast Greenland. These rates are due to low upper mantle viscosity in the region, from when Greenland passed over the Iceland hot spot about 40 million years ago. This region of concentrated soft rheology has a profound influence on reconstructing the deglaciation history of Greenland. We reevaluate the evolution of the GrIS since LGM and obtain a loss of 1.5-m sea-level equivalent from the northwest and southeast. These same sectors are dominating modern <span class="hlt">mass</span> loss. We suggest that the present destabilization of these marine-based sectors may increase sea level for centuries to come. Our new deglaciation history and GIA uplift estimates suggest that studies that use the Gravity Recovery and Climate Experiment satellite mission to infer present-day changes in the GrIS may have erroneously corrected for GIA and underestimated the <span class="hlt">mass</span> loss by about 20 gigatons/year.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5031466','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5031466"><span>Geodetic measurements reveal similarities between post–Last Glacial Maximum and present-day <span class="hlt">mass</span> loss from the Greenland <span class="hlt">ice</span> sheet</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Khan, Shfaqat A.; Sasgen, Ingo; Bevis, Michael; van Dam, Tonie; Bamber, Jonathan L.; Wahr, John; Willis, Michael; Kjær, Kurt H.; Wouters, Bert; Helm, Veit; Csatho, Beata; Fleming, Kevin; Bjørk, Anders A.; Aschwanden, Andy; Knudsen, Per; Munneke, Peter Kuipers</p> <p>2016-01-01</p> <p>Accurate quantification of the millennial-scale <span class="hlt">mass</span> balance of the Greenland <span class="hlt">ice</span> sheet (GrIS) and its contribution to global sea-level rise remain challenging because of sparse in situ observations in key regions. Glacial isostatic adjustment (GIA) is the ongoing response of the solid Earth to <span class="hlt">ice</span> and ocean load changes occurring since the Last Glacial Maximum (LGM; ~21 thousand years ago) and may be used to constrain the GrIS deglaciation history. We use data from the Greenland Global Positioning System network to directly measure GIA and estimate basin-wide <span class="hlt">mass</span> changes since the LGM. Unpredicted, large GIA uplift rates of +12 mm/year are found in southeast Greenland. These rates are due to low upper mantle viscosity in the region, from when Greenland passed over the Iceland hot spot about 40 million years ago. This region of concentrated soft rheology has a profound influence on reconstructing the deglaciation history of Greenland. We reevaluate the evolution of the GrIS since LGM and obtain a loss of 1.5-m sea-level equivalent from the northwest and southeast. These same sectors are dominating modern <span class="hlt">mass</span> loss. We suggest that the present destabilization of these marine-based sectors may increase sea level for centuries to come. Our new deglaciation history and GIA uplift estimates suggest that studies that use the Gravity Recovery and Climate Experiment satellite mission to infer present-day changes in the GrIS may have erroneously corrected for GIA and underestimated the <span class="hlt">mass</span> loss by about 20 gigatons/year. PMID:27679819</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70037558','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70037558"><span>On the nature of the dirty <span class="hlt">ice</span> at the bottom of the GISP2 <span class="hlt">ice</span> core</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Bender, Michael L.; Burgess, Edward; Alley, Richard B.; Barnett, Bruce; Clow, Gary D.</p> <p>2010-01-01</p> <p>We present data on the triple Ar isotope composition in trapped gas from clean, stratigraphically disturbed <span class="hlt">ice</span> between 2800 and 3040m depth in the GISP2 <span class="hlt">ice</span> core, and from basal dirty <span class="hlt">ice</span> from 3040 to 3053m depth. We also present data for the abundance and isotopic composition of O2 and N2, and abundance of Ar, in the basal dirty <span class="hlt">ice</span>. The Ar/N2 ratio of dirty basal <span class="hlt">ice</span>, the heavy isotope enrichment (reflecting gravitational fractionation), and the total gas <span class="hlt">content</span> all indicate that the gases in basal dirty <span class="hlt">ice</span> originate from the assimilation of clean <span class="hlt">ice</span> of the overlying glacier, which comprises most of the <span class="hlt">ice</span> in the dirty bottom layer. O2 is partly to completely depleted in basal <span class="hlt">ice</span>, reflecting active metabolism. The gravitationally corrected ratio of 40Ar/38Ar, which decreases with age in the global atmosphere, is compatible with an age of 100-250ka for clean disturbed <span class="hlt">ice</span>. In basal <span class="hlt">ice</span>, 40Ar is present in excess due to injection of radiogenic 40Ar produced in the underlying continental crust. The weak depth gradient of 40Ar in the dirty basal <span class="hlt">ice</span>, and the distribution of dirt, indicate mixing within the basal <span class="hlt">ice</span>, while various published lines of evidence indicate mixing within the overlying clean, disturbed <span class="hlt">ice</span>. Excess CH4, which reaches thousands of ppm in basal dirty <span class="hlt">ice</span> at GRIP, is virtually absent in overlying clean disturbed <span class="hlt">ice</span>, demonstrating that mixing of dirty basal <span class="hlt">ice</span> into the overlying clean <span class="hlt">ice</span>, if it occurs at all, is very slow. Order-of-magnitude estimates indicate that the mixing rate of clean <span class="hlt">ice</span> into dirty <span class="hlt">ice</span> is sufficient to maintain a steady thickness of dirty <span class="hlt">ice</span> against thinning from the mean <span class="hlt">ice</span> flow. The dirty <span class="hlt">ice</span> appears to consist of two or more basal components in addition to clean glacial <span class="hlt">ice</span>. A small amount of soil or permafrost, plus preglacial snow, lake or ground <span class="hlt">ice</span> could explain the observations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27134805','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27134805"><span>Spatial and temporal Antarctic <span class="hlt">Ice</span> Sheet <span class="hlt">mass</span> trends, glacio-isostatic adjustment, and surface processes from a joint inversion of satellite altimeter, gravity, and GPS data.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Martín-Español, Alba; Zammit-Mangion, Andrew; Clarke, Peter J; Flament, Thomas; Helm, Veit; King, Matt A; Luthcke, Scott B; Petrie, Elizabeth; Rémy, Frederique; Schön, Nana; Wouters, Bert; Bamber, Jonathan L</p> <p>2016-02-01</p> <p>We present spatiotemporal <span class="hlt">mass</span> balance trends for the Antarctic <span class="hlt">Ice</span> Sheet from a statistical inversion of satellite altimetry, gravimetry, and elastic-corrected GPS data for the period 2003-2013. Our method simultaneously determines annual trends in <span class="hlt">ice</span> dynamics, surface <span class="hlt">mass</span> balance anomalies, and a time-invariant solution for glacio-isostatic adjustment while remaining largely independent of forward models. We establish that over the period 2003-2013, Antarctica has been losing <span class="hlt">mass</span> at a rate of -84 ± 22 Gt yr -1 , with a sustained negative mean trend of dynamic imbalance of -111 ± 13 Gt yr -1 . West Antarctica is the largest contributor with -112 ± 10 Gt yr -1 , mainly triggered by high thinning rates of glaciers draining into the Amundsen Sea Embayment. The Antarctic Peninsula has experienced a dramatic increase in <span class="hlt">mass</span> loss in the last decade, with a mean rate of -28 ± 7 Gt yr -1 and significantly higher values for the most recent years following the destabilization of the Southern Antarctic Peninsula around 2010. The total <span class="hlt">mass</span> loss is partly compensated by a significant <span class="hlt">mass</span> gain of 56 ± 18 Gt yr -1 in East Antarctica due to a positive trend of surface <span class="hlt">mass</span> balance anomalies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C21A0719B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C21A0719B"><span>Freshwater fluxes into the subpolar North Atlantic from secular trends in Arctic land <span class="hlt">ice</span> <span class="hlt">mass</span> balance</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bamber, J. L.; Enderlin, E. M.; Howat, I. M.; Wouters, B.; van den Broeke, M.</p> <p>2015-12-01</p> <p>Freshwater fluxes (FWF) from river runoff and precipitation minus evaporation for the pan Arctic seas are relatively well documented and prescribed in ocean GCMs. Fluxes from Greenland and Arctic glaciers and <span class="hlt">ice</span> caps on the other hand are generally ignored, despite their potential impacts on ocean circulation and marine biology and growing evidence for changes to the hydrography of parts of the subpolar North Atlantic. In a previous study we determined the FWF from Greenland for the period 1958-2010 using a combination of observations and regional climate modeling. Here, we update the analysis with data from new satellite observations to extend the record both in space and time. The new FWF estimates cover the period 1958-2014 and include the Canadian, Russian and Norwegian Arctic (Svalbard) in addition to the contributions from Greenland. We combine satellite altimetry (including CryoSat 2) with grounding line flux data, regional climate modeling of surface <span class="hlt">mass</span> balance and gravimetry to produce consistent estimates of solid <span class="hlt">ice</span> and liquid FWF into the Arctic and North Atlantic Oceans. The total cumulative FWF anomaly from land <span class="hlt">ice</span> <span class="hlt">mass</span> loss started to increase significantly in the mid 1990s and now exceeds 5000 km^3, a value that is about half of the Great Salinity Anomaly of the 1970s. The majority of the anomaly is entering two key areas of deep water overturning in the Labrador and Irminger Seas, at a rate that has been increasing steadily over the last ~20 years. Since the mid 2000s, however, the Canadian Arctic archipelago has been making a significant contribution to the FW anomaly entering Baffin Bay. Tracer experiments with eddy-permitting ocean GCMs suggest that the FW input from southern Greenland and the Canadian Arctic should accumulate in Baffin Bay with the potential to affect geostrophic circulation, stratification in the region and possibly the strength of the Atlantic Meridional Overturning Circulation. We also examine the trajectory of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26912699','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26912699"><span>Holocene deceleration of the Greenland <span class="hlt">Ice</span> Sheet.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>MacGregor, Joseph A; Colgan, William T; Fahnestock, Mark A; Morlighem, Mathieu; Catania, Ginny A; Paden, John D; Gogineni, S Prasad</p> <p>2016-02-05</p> <p>Recent peripheral thinning of the Greenland <span class="hlt">Ice</span> Sheet is partly offset by interior thickening and is overprinted on its poorly constrained Holocene evolution. On the basis of the <span class="hlt">ice</span> sheet's radiostratigraphy, <span class="hlt">ice</span> 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 <span class="hlt">ice</span> sheet's dynamic response to the decreasing proportion of softer <span class="hlt">ice</span> from the last glacial period and the deglacial collapse of the <span class="hlt">ice</span> bridge across Nares Strait also contributed to this pattern. Thus, recent interior thickening of the Greenland <span class="hlt">Ice</span> Sheet is partly an ongoing dynamic response to the last deglaciation that is large enough to affect interpretation of its <span class="hlt">mass</span> balance from altimetry. Copyright © 2016, American Association for the Advancement of Science.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70073409','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70073409"><span>HiRISE observations of new impact craters exposing Martian ground <span class="hlt">ice</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Dundas, Colin M.; Byrne, Shane; McEwen, Alfred S.; Mellon, Michael T.; Kennedy, Megan R.; Daubar, Ingrid J.; Saper, Lee</p> <p>2014-01-01</p> <p>Twenty small new impact craters or clusters have been observed to excavate bright material inferred to be <span class="hlt">ice</span> at mid and high latitudes on Mars. In the northern hemisphere, the craters are widely distributed geographically and occur at latitudes as low as 39°N. Stability modeling suggests that this <span class="hlt">ice</span> distribution requires a long-term average atmospheric water vapor <span class="hlt">content</span> around 25 precipitable microns, more than double the present value, which is consistent with the expected effect of recent orbital variations. Alternatively, near-surface humidity could be higher than expected for current column abundances if water vapor is not well-mixed with atmospheric CO2, or the vapor pressure at the <span class="hlt">ice</span> table could be lower due to salts. <span class="hlt">Ice</span> in and around the craters remains visibly bright for months to years, indicating that it is clean <span class="hlt">ice</span> rather than <span class="hlt">ice</span>-cemented regolith. Although some clean <span class="hlt">ice</span> may be produced by the impact process, it is likely that the original ground <span class="hlt">ice</span> was excess <span class="hlt">ice</span> (exceeding dry soil pore space) in many cases. Observations of the craters suggest small-scale heterogeneities in this excess <span class="hlt">ice</span>. The origin of such <span class="hlt">ice</span> is uncertain. <span class="hlt">Ice</span> lens formation by migration of thin films of liquid is most consistent with local heterogeneity in <span class="hlt">ice</span> <span class="hlt">content</span> and common surface boulders, but in some cases nearby thermokarst landforms suggest large amounts of excess <span class="hlt">ice</span> that may be best explained by a degraded <span class="hlt">ice</span> sheet.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C41E0727D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C41E0727D"><span>Continuous measurements of surface <span class="hlt">mass</span> balance, firn compaction, and meltwater retention in Greenland for altimetry validation.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>de la Peña, S.; Howat, I.; Behar, A.; Price, S. F.; Thanga, J.; Crowell, J. M.; Huseas, S.; Tedesco, M.</p> <p>2016-12-01</p> <p>Observations made in recent years by repeated altimetry from CryoSat-2 and NASA's Operation <span class="hlt">Ice</span>Bridge reveal large fluctuations in the firn volume of the Greenland <span class="hlt">Ice</span> Sheet. Although an order of magnitude smaller than <span class="hlt">ice</span> thinning rates observed in some areas at the margins of the <span class="hlt">ice</span> sheet, short-term departures in surface elevation trends occur over most of the accumulation zone of Greenland. Changes in the thickness of the firn column are influenced by variability in surface <span class="hlt">mass</span> balance, firn compaction, and abrupt seasonal densification near the surface caused by refreezing at depth of variable amounts of surface meltwater in the summer. These processes and dynamic thinning cannot be differentiated from each other by altimetry alone. Until recently, nearly all information on density and surface <span class="hlt">mass</span> balance changes over the firn layer came from <span class="hlt">ice</span> core and snow pit stratigraphy that provided annual rates with relatively large uncertainties. Here we present direct, continuous measurements of firn density and surface <span class="hlt">mass</span> balance along with annual estimates of firn <span class="hlt">ice</span> <span class="hlt">content</span> used to assess observed elevation change in the percolation zone of western Greenland in relation to firn processes. Since 2012, autonomous in-situ firn compaction sensors have monitored several sites in the catchment area of Jakobshavn Isbrae, and since 2015 surface <span class="hlt">mass</span> balance and surface displacement has been measured continuously using a combination of sensors. In addition to identify the different components in the altimetry signal, The temporal resolution of the data acquired provide a means to monitor short-term changes in the near-surface firn, and identifying individual events causing surface elevation displacement.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C41E..05D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C41E..05D"><span>Multi-Decadal Averages of Basal Melt for Ross <span class="hlt">Ice</span> Shelf, Antarctica Using Airborne Observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Das, I.; Bell, R. E.; Tinto, K. J.; Frearson, N.; Kingslake, J.; Padman, L.; Siddoway, C. S.; Fricker, H. A.</p> <p>2017-12-01</p> <p>Changes in <span class="hlt">ice</span> shelf <span class="hlt">mass</span> balance are key to the long term stability of the Antarctic <span class="hlt">Ice</span> Sheet. Although the most extensive <span class="hlt">ice</span> shelf <span class="hlt">mass</span> loss currently is occurring in the Amundsen Sea sector of West Antarctica, many other <span class="hlt">ice</span> shelves experience changes in thickness on time scales from annual to <span class="hlt">ice</span> age cycles. Here, we focus on the Ross <span class="hlt">Ice</span> Shelf. An 18-year record (1994-2012) of satellite radar altimetry shows substantial variability in Ross <span class="hlt">Ice</span> Shelf height on interannual time scales, complicating detection of potential long-term climate-change signals in the <span class="hlt">mass</span> budget of this <span class="hlt">ice</span> shelf. Variability of radar signal penetration into the <span class="hlt">ice</span>-shelf surface snow and firn layers further complicates assessment of <span class="hlt">mass</span> changes. We investigate Ross <span class="hlt">Ice</span> Shelf <span class="hlt">mass</span> balance using aerogeophysical data from the ROSETTA-<span class="hlt">Ice</span> surveys using <span class="hlt">Ice</span>Pod. We use two <span class="hlt">ice</span>-penetrating radars; a 2 GHz unit that images fine-structure in the upper 400 m of the <span class="hlt">ice</span> surface and a 360 MHz radar to identify the <span class="hlt">ice</span> shelf base. We have identified internal layers that are continuous along flow from the grounding line to the <span class="hlt">ice</span> shelf front. Based on layer continuity, we conclude that these layers must be the horizons between the continental <span class="hlt">ice</span> of the outlet glaciers and snow accumulation once the <span class="hlt">ice</span> is afloat. We use the Lagrangian change in thickness of these layers, after correcting for strain rates derived using modern day InSAR velocities, to estimate multidecadal averaged basal melt rates. This method provides a novel way to quantify basal melt, avoiding the confounding impacts of spatial and short-timescale variability in surface accumulation and firn densification processes. Our estimates show elevated basal melt rates (> -1m/yr) around Byrd and Mullock glaciers within 100 km from the <span class="hlt">ice</span> shelf front. We also compare modern InSAR velocity derived strain rates with estimates from the comprehensive ground-based RIGGS observations during 1973-1978 to estimate the potential magnitude of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012JGRF..117.2037G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012JGRF..117.2037G"><span>Investigation of land <span class="hlt">ice</span>-ocean interaction with a fully coupled <span class="hlt">ice</span>-ocean model: 1. Model description and behavior</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goldberg, D. N.; Little, C. M.; Sergienko, O. V.; Gnanadesikan, A.; Hallberg, R.; Oppenheimer, M.</p> <p>2012-06-01</p> <p>Antarctic <span class="hlt">ice</span> shelves interact closely with the ocean cavities beneath them, with <span class="hlt">ice</span> shelf geometry influencing ocean cavity circulation, and heat from the ocean driving changes in the <span class="hlt">ice</span> shelves, as well as the grounded <span class="hlt">ice</span> streams that feed them. We present a new coupled model of an <span class="hlt">ice</span> stream-<span class="hlt">ice</span> shelf-ocean system that is used to study this interaction. The model is capable of representing a moving grounding line and dynamically responding ocean circulation within the <span class="hlt">ice</span> shelf cavity. Idealized experiments designed to investigate the response of the coupled system to instantaneous increases in ocean temperature show <span class="hlt">ice</span>-ocean system responses on multiple timescales. Melt rates and <span class="hlt">ice</span> shelf basal slopes near the grounding line adjust in 1-2 years, and downstream advection of the resulting <span class="hlt">ice</span> shelf thinning takes place on decadal timescales. Retreat of the grounding line and adjustment of grounded <span class="hlt">ice</span> takes place on a much longer timescale, and the system takes several centuries to reach a new steady state. During this slow retreat, and in the absence of either an upward-or downward-sloping bed or long-term trends in ocean heat <span class="hlt">content</span>, the <span class="hlt">ice</span> shelf and melt rates maintain a characteristic pattern relative to the grounding line.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.4898V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.4898V"><span>Reconstruction of past equilibrium line altitude using <span class="hlt">ice</span> extent data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Visnjevic, Vjeran; Herman, Frederic; Podladchikov, Yuri</p> <p>2017-04-01</p> <p>With the end of the Last Glacial Maximum (LGM), about 20 000 years ago, ended the most recent long-lasting cold phase in Earth's history. This last glacial advance left a strong observable imprint on the landscape, such as abandoned moraines, trimlines and other glacial geomorphic features. These features provide a valuable record of past continental climate. In particular, terminal moraines reflect the extent of glaciers and <span class="hlt">ice</span>-caps, which itself reflects past temperature and precipitation conditions. Here we present an inverse approach, based on a Tikhonov regularization, we have recently developed to reconstruct the LGM <span class="hlt">mass</span> balance from observed <span class="hlt">ice</span> extent data. The <span class="hlt">ice</span> flow model is developed using the shallow <span class="hlt">ice</span> approximation and solved explicitly using Graphical Processing Units (GPU). The <span class="hlt">mass</span> balance field, b, is the constrained variable defined by the <span class="hlt">ice</span> surface S, balance rate β and the spatially variable equilibrium line altitude field (ELA): b = min (β ṡ(S(x,y)- ELA (x,y)),c). (1) where c is a maximum accumulation rate. We show that such a <span class="hlt">mass</span> balance, and thus the spatially variable ELA field, can be inferred from the observed past <span class="hlt">ice</span> extent and <span class="hlt">ice</span> thickness at high resolution and very efficiently. The GPU implementation allows us solve one 1024x1024 grid points forward model run under 0.5s, which significantly reduces the time needed for our inverse method to converge. We start with synthetic test to demonstrate the method. We then apply the method to LGM <span class="hlt">ice</span> extents of South Island of New Zealand, the Patagonian Andes, where we can see a clear influence of Westerlies on the ELA, and the European Alps. These examples show that the method is capable of constraining spatial variations in <span class="hlt">mass</span> balance at the scale of a mountain range, and provide us with information on past continental climate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70011332','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70011332"><span>Snow and <span class="hlt">ice</span> in a changing hydrological world.</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Meier, M.F.</p> <p>1983-01-01</p> <p>Snow cover on land (especially in the Northern Hemisphere) and sea <span class="hlt">ice</span> (especially in the Southern Hemisphere) vary seasonally, and this seasonal change has an important affect on the world climate because snow and sea <span class="hlt">ice</span> reflect solar radiation efficiently and affect other heat flow processes between atmosphere and land or ocean. Glaciers, including <span class="hlt">ice</span> sheets, store most of the fresh water on Earth, but change dimensions relatively slowly. There is no clear evidence that the glacier <span class="hlt">ice</span> volume currently is declining, but more needs to be known about mountain glacier and <span class="hlt">ice</span> sheet <span class="hlt">mass</span> balances. -from Author</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1911309W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1911309W"><span>Submarine melt rates under Greenland's <span class="hlt">ice</span> tongues</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wilson, Nat; Straneo, Fiametta; Heimbach, Patrick; Cenedese, Claudia</p> <p>2017-04-01</p> <p>The few remaining <span class="hlt">ice</span> tongues (<span class="hlt">ice</span>-shelf like extensions) of Greenland's glaciers are undergoing rapid changes with potential implications for the stability of the <span class="hlt">ice</span> sheet. Submarine melting is recognized as a major contributor to <span class="hlt">mass</span> loss, yet the magnitude and spatial distribution of melt are poorly known or understood. Here, we use high resolution satellite imagery to infer the magnitude and spatial variability of melt rates under Greenland's largest remaining <span class="hlt">ice</span> tongues: Ryder Glacier, Petermann Glacier and Nioghalvfjerdsbræ (79 North Glacier). We find that submarine plus aerial melt approximately balance the <span class="hlt">ice</span> flux from the grounded <span class="hlt">ice</span> sheet for the first two while at Nioghalvfjerdsbræ the total melt flux exceeds the inflow of <span class="hlt">ice</span> indicating thinning of the <span class="hlt">ice</span> tongue. We also show that melt rates under the <span class="hlt">ice</span> tongues vary considerably, exceeding 60 m yr-1 near the grounding zone and decaying rapidly downstream. Channels, likely originating from upstream subglacial channels, give rise to large melt variations across the <span class="hlt">ice</span> tongues. Using derived melt rates, we test simplified melt parameterizations appropriate for <span class="hlt">ice</span> sheet models and find the best agreement with those that incorporate <span class="hlt">ice</span> tongue geometry in the form of depth and slope.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.P53H..03K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.P53H..03K"><span>Water <span class="hlt">ice</span> is water <span class="hlt">ice</span>: some applications and limitations of Earth analogues to Mars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Koutnik, M.; Pathare, A.; Waddington, E. D.; Winebrenner, D. P.</p> <p>2017-12-01</p> <p> particular, we discuss why internal layers alone are not a diagnostic test for <span class="hlt">ice</span> flow. We also present progress in applying models of debris-covered glacier flow to LDAs where dynamic debris cover, <span class="hlt">ice</span> flow, and accumulation/ablation act to shape the <span class="hlt">ice-mass</span> surface.</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://hdl.handle.net/2060/20040034050','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040034050"><span>African Dust Aerosols as Atmospheric <span class="hlt">Ice</span> Nuclei</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>DeMott, Paul J.; Brooks, Sarah D.; Prenni, Anthony J.; Kreidenweis, Sonia M.; Sassen, Kenneth; Poellot, Michael; Rogers, David C.; Baumgardner, Darrel</p> <p>2003-01-01</p> <p>Measurements of the <span class="hlt">ice</span> nucleating ability of aerosol particles in air <span class="hlt">masses</span> over Florida having sources from North Africa support the potential importance of dust aerosols for indirectly affecting cloud properties and climate. The concentrations of <span class="hlt">ice</span> nuclei within dust layers at particle sizes below 1 pn exceeded 1/cu cm; the highest ever reported with our device at temperatures warmer than homogeneous freezing conditions. These measurements add to previous direct and indirect evidence of the <span class="hlt">ice</span> nucleation efficiency of desert dust aerosols, but also confirm their contribution to <span class="hlt">ice</span> nuclei populations at great distances from source regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140006604','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140006604"><span>Extent of Low-accumulation 'Wind Glaze' Areas on the East Antarctic Plateau: Implications for Continental <span class="hlt">Ice</span> <span class="hlt">Mass</span> Balance</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Scambos, Theodore A.; Frezzotti, Massimo; Haran, T.; Bohlander, J.; Lenaerts, J. T. M.; Van Den Broeke, M. R.; Jezek, K.; Long, D.; Urbini, S.; Farness, K.; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20140006604'); toggleEditAbsImage('author_20140006604_show'); toggleEditAbsImage('author_20140006604_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20140006604_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20140006604_hide"></p> <p>2012-01-01</p> <p>Persistent katabatic winds form widely distributed localized areas of near-zero net surface accumulation on the East Antarctic <span class="hlt">ice</span> sheet (EAIS) plateau. These areas have been called 'glaze' surfaces due to their polished appearance. They are typically 2-200 square kilometers in area and are found on leeward slopes of <span class="hlt">ice</span>-sheet undulations and megadunes. Adjacent, leeward high-accumulation regions (isolated dunes) are generally smaller and do not compensate for the local low in surface <span class="hlt">mass</span> balance (SMB). We use a combination of satellite remote sensing and field-gathered datasets to map the extent of wind glaze in the EAIS above 1500m elevation. Mapping criteria are derived from distinctive surface and subsurface characteristics of glaze areas resulting from many years of intense annual temperature cycling without significant burial. Our results show that 11.2 plus or minus 1.7%, or 950 plus or minus 143 x 10(exp 3) square kilometers, of the EAIS above 1500m is wind glaze. Studies of SMB interpolate values across glaze regions, leading to overestimates of net <span class="hlt">mass</span> input. Using our derived wind-glaze extent, we estimate this excess in three recent models of Antarctic SMB at 46-82 Gt. The lowest-input model appears to best match the mean in regions of extensive wind glaze.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=ice&pg=2&id=EJ1001296','ERIC'); return false;" href="https://eric.ed.gov/?q=ice&pg=2&id=EJ1001296"><span>Simple Cloud Chambers Using Gel <span class="hlt">Ice</span> Packs</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>Kamata, Masahiro; Kubota, Miki</p> <p>2012-01-01</p> <p>Although cloud chambers are highly regarded as teaching aids for radiation education, school teachers have difficulty in using cloud chambers because they have to prepare dry <span class="hlt">ice</span> or liquid nitrogen before the experiment. We developed a very simple and inexpensive cloud chamber that uses the <span class="hlt">contents</span> of gel <span class="hlt">ice</span> packs which can substitute for dry…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.G31B0907M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.G31B0907M"><span>Regionally Optimized GRACE Processing and Inter-comparison on the Antarctic <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mohajerani, Y.; Velicogna, I.; Sutterley, T. C.; Rignot, E. J.</p> <p>2017-12-01</p> <p>The Antarctic <span class="hlt">ice</span> sheet is losing <span class="hlt">mass</span> at an accelerating rate, with a sea level contribution that changed from 0.08mm/yr from 1992 to 2001 to 0.4mm/yr from 2002 to 2011. While most of this contribution comes from West Antarctica, Totten Glacier has the largest discharge of <span class="hlt">ice</span> in East Antarctica, with a sea level rise potential of 3.9 m. Furthermore, the drainage basin of Totten Glacier, along the neighboring Moscow University Glacier are below sea level, extending hundreds of kilometers inland. Therefore, obtaining regional estimates of both western and eastern Antarctic basins are of critical importance. The GRACE (Gravity Recovery and Climate Experiment) satellite has been providing <span class="hlt">mass</span> balance time-series from geoid changes since 2002. Several mascon and harmonic GRACE solutions are available from different processing centers. Here, we evaluate the various solutions across the <span class="hlt">ice</span> sheet and a new set of regionally optimized mascons to study the <span class="hlt">mass</span> balance of Totten and Moscow University glaciers. We obtain a trend of -16.5±4.1Gt/yr with an acceleration of -2.0±1.8Gt/yr2 for the two glaciers for the period April 2002 to December 2016 using the Ivins et al (2013) GIA model (errors include leakage, GIA, and regression errors). We compare the results with the <span class="hlt">Mass</span> Budget Method that combines <span class="hlt">ice</span> discharge (D) and surface <span class="hlt">mass</span> balance (SMB) from two models: 1) RACMO2.3, and 2) MAR3.6.4. MBM/RACMO2.3 shows the best agreement with the GRACE estimates. Within the common period from April 2002 to December 2015, the MBM/RACMO2.3 and MAR3.6.4 results are -15.6±1.8Gt/yr and -6.7±1.5Gt/yr respectively, while the GRACE time-series has a trend of -14.8±2.7 Gt/yr. We extend the study to the Getz <span class="hlt">Ice</span> Shelf, the third largest <span class="hlt">ice</span> shelf in West Antarctica after Ronne and Ross West <span class="hlt">ice</span> shelves. We compare our gravity-derived <span class="hlt">mass</span> estimates, the <span class="hlt">mass</span> budget estimates, and the volume changes from altimetry data to compare the estimates and obtain a multi-sensor assessment</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900041437&hterms=hydrofluoric+acid+weak+acid&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DWhy%2Bhydrofluoric%2Bacid%2Bweak%2Bacid','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900041437&hterms=hydrofluoric+acid+weak+acid&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DWhy%2Bhydrofluoric%2Bacid%2Bweak%2Bacid"><span>Incorporation of stratospheric acids into water <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>Elliott, Scott; Turco, Richard P.; Toon, Owen B.; Hamill, Patrick</p> <p>1990-01-01</p> <p>Hydrochloric and hydrofluoric acids are absorbed within the water <span class="hlt">ice</span> lattice at mole fractions maximizing below 0.00001 and 0.0001 in a variety of solid impurity studies. The absorption mechanism may be substitutional or interstitial, leading in either case to a weak permeation of stratospheric <span class="hlt">ices</span> by the acids at equilibrium. Impurities could also inhabit grain boundaries, and the acid <span class="hlt">content</span> of atmospheric <span class="hlt">ice</span> crystals will then depend on details of their surface and internal microstructures. Limited evidence indicates similar properties for the absorption of HNO3. Water <span class="hlt">ice</span> lattices saturated with acid cannot be a significant local reservoir for HCl in the polar stratosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004PhDT.......117B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004PhDT.......117B"><span><span class="hlt">Mass</span> spectrometric imaging and laser desorption ionization (LDI) with <span class="hlt">ice</span> as a matrix using femtosecond laser pulses</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Berry, Jamal Ihsan</p> <p></p> <p>The desorption of biomolecules from frozen aqueous solutions on metal substrates with femtosecond laser pulses is presented for the first time. Unlike previous studies using nanosecond pulses, this approach produces high quality <span class="hlt">mass</span> spectra of biomolecules repeatedly and reproducibly. This novel technique allows analysis of biomolecules directly from their native frozen environments. The motivation for this technique stems from molecular dynamics computer simulations comparing nanosecond and picosecond heating of water overlayers frozen on Au substrates which demonstrate large water cluster formation and ejection upon substrate heating within ultrashort timescales. As the frozen aqueous matrix and analyte molecules are transparent at the wavelengths used, the laser energy is primarily absorbed by the substrate, causing rapid heating and explosive boiling of the <span class="hlt">ice</span> overlayer, followed by the ejection of <span class="hlt">ice</span> clusters and the entrained analyte molecule. Spectral characteristics at a relatively high fluence of 10 J/cm 2 reveal the presence of large molecular weight metal clusters when a gold substrate is employed, with smaller cluster species observed from frozen aqueous solutions on Ag, Cu, and Pb substrates. The presence of the metal clusters is indicative of an evaporative cooling mechanism which stabiles cluster ion formation and the ejection of biomolecules from frozen aqueous solutions. Solvation is necessary as the presence of metal clusters and biomolecular ion signals are not observed from bare metal substrates in absence of the frozen overlayer. The potential for <span class="hlt">mass</span> spectrometric imaging with femtosecond LDI of frozen samples is also presented. The initial results for the characterization of peptides and peptoids linked to combinatorial beads frozen in <span class="hlt">ice</span> and the assay of frozen brain tissue from the serotonin transporter gene knockout mouse via LDI imaging are discussed. Images of very good quality and resolution are obtained with 400 nm, 200 fs pulses</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150021071','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150021071"><span><span class="hlt">Ice</span>Cube: CubeSat 883-GHz Radiometry for Future <span class="hlt">Ice</span> Cloud Remote Sensing</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wu, Dongliang; Esper, Jaime; Ehsan, Negar; Johnson, Thomas; Mast, William; Piepmeier, Jeffery R.; Racette, Paul E.</p> <p>2015-01-01</p> <p><span class="hlt">Ice</span> clouds play a key role in the Earth's radiation budget, mostly through their strong regulation of infrared radiation exchange. Accurate observations of global cloud <span class="hlt">ice</span> and its distribution have been a challenge from space, and require good instrument sensitivities to both cloud <span class="hlt">mass</span> and microphysical properties. Despite great advances from recent spaceborne radar and passive sensors, uncertainty of current <span class="hlt">ice</span> water path (IWP) measurements is still not better than a factor of 2. Submillimeter (submm) wave remote sensing offers great potential for improving cloud <span class="hlt">ice</span> measurements, with simultaneous retrievals of cloud <span class="hlt">ice</span> and its microphysical properties. The <span class="hlt">Ice</span>Cube project is to enable this cloud <span class="hlt">ice</span> remote sensing capability in future missions, by raising 874-GHz receiver technology TRL from 5 to 7 in a spaceflight demonstration on 3-U CubeSat in a low Earth orbit (LEO) environment. The NASAs Goddard Space Flight Center (GSFC) is partnering with Virginia Diodes Inc (VDI) on the 874-GHz receiver through its Vector Network Analyzer (VNA) extender module product line, to develop an instrument with precision of 0.2 K over 1-second integration and accuracy of 2.0 K or better. <span class="hlt">Ice</span>Cube is scheduled to launch to and subsequent release from the International Space Station (ISS) in mid-2016 for nominal operation of 28 plus days. We will present the updated design of the payload and spacecraft systems, as well as the operation concept. We will also show the simulated 874-GHz radiances from the ISS orbits and cloud scattering signals as expected for the <span class="hlt">Ice</span>Cube cloud radiometer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14.5339F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.5339F"><span>Assessing the accuracy of Greenland <span class="hlt">ice</span> sheet <span class="hlt">ice</span> ablation measurements by pressure transducer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fausto, R. S.; van As, D.; Ahlstrøm, A. P.</p> <p>2012-04-01</p> <p>In the glaciological community there is a need for reliable <span class="hlt">mass</span> balance measurements of glaciers and <span class="hlt">ice</span> sheets, ranging from daily to yearly time scales. Here we present a method to measure <span class="hlt">ice</span> ablation using a pressure transducer. The pressure transducer is drilled into the <span class="hlt">ice</span>, en-closed in a hose filled with a liquid that is non-freezable at common Greenlandic temperatures. The pressure signal registered by the transducer is that of the vertical column of liquid over the sensor, which can be translated in depth knowing the density of the liquid. As the free-standing AWS moves down with the ablating surface and the hose melts out of the <span class="hlt">ice</span>, an increasingly large part of the hose will lay flat on the <span class="hlt">ice</span> surface, and the hydrostatic pressure from the vertical column of liquid in the hose will get smaller. This reduction in pressure provides us with the ablation rate. By measuring at (sub-) daily timescales this assembly is well-suited to monitor <span class="hlt">ice</span> ablation in remote regions, with clear advantages over other well-established methods of measuring <span class="hlt">ice</span> ablation in the field. The pressure transducer system has the potential to monitor <span class="hlt">ice</span> ablation for several years without re-drilling and the system is suitable for high ablation areas. A routine to transform raw measurements into ablation values will also be presented, including a physically based method to remove air pressure variability from the signal. The pressure transducer time-series is compared to that recorded by a sonic ranger for the climatically hostile setting on the Greenland <span class="hlt">ice</span> sheet.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20010002431&hterms=BALANCE+SHEET&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DBALANCE%2BSHEET','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20010002431&hterms=BALANCE+SHEET&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DBALANCE%2BSHEET"><span>Troughs on Martian <span class="hlt">Ice</span> Sheets: Analysis of Their Closure and <span class="hlt">Mass</span> Balance</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fountain, A.; Kargel, J.; Lewis, K.; MacAyeal, D.; Pfeffer, T.; Zwally, J.</p> <p>2000-01-01</p> <p>At the Copenhagen workshop on Martian polar processes, Ralf Greve commented that the flow regime surrounding scarps and troughs of the Martian polar <span class="hlt">ice</span> sheets cannot be modeled using traditional "plan view" <span class="hlt">ice</span>-sheet models. Such models are inadequate because they typically use reduced equations that embody certain simplifications applicable only to terrestrial <span class="hlt">ice</span> sheets where the upper <span class="hlt">ice</span> sheet surface is smooth. In response to this suggestion, we have constructed a 2-dimensional, time dependent "side view" (two spatial dimensions: one horizontal, one vertical) model of scarp closure that is designed to overcome the difficulties described by Greve. The purpose of the model is to evaluate the scales of stress variation and styles of flow closure so as to estimate errors that may be encountered by "plan view" models. We show that there may be avenues whereby the complications associated with scarp closure can be overcome in "plan view" models through appropriate parameterizations of 3-dimensional effects. Following this, we apply the flow model to simulate the evolution of a typical scarp on the North Polar Cap of Mars. Our simulations investigate: (a) the role of "radiation trapping" (see our companion abstract) in creating and maintaining "spiral-like" scarps on the <span class="hlt">ice</span> sheet, (b) the consequences of different flowlaws and <span class="hlt">ice</span> compositions on scarp evolution and, in particular, scarp age, and (c) the role of dust and debris in scarp evolution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMGC31H1195T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMGC31H1195T"><span>A regional-scale estimation of <span class="hlt">ice</span> wedge <span class="hlt">ice</span> volumes in the Canadian High Arctic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Templeton, M.; Pollard, W. H.; Grand'Maison, C. B.</p> <p>2016-12-01</p> <p><span class="hlt">Ice</span> wedges are both prominent and environmentally vulnerable features in continuous permafrost environments. As the world's Arctic regions begin to warm, concern over the potential effects of <span class="hlt">ice</span> wedge melt out has become an immediate issue, receiving much attention in the permafrost literature. In this study we estimate the volume of <span class="hlt">ice</span> wedge <span class="hlt">ice</span> for large areas in the Canadian High Arctic through the use of high resolution satellite imagery and the improved capabilities of Geographic Information Systems (GIS). The methodology used for this study is similar to that of one performed in Siberia and Alaska by Ulrich et al, in 2014. Utilizing Ulrich's technique, this study detected <span class="hlt">ice</span> wedge polygons from satellite imagery using ArcGIS. The average width and depth of these <span class="hlt">ice</span> wedges were obtained from a combination of field data and long-term field studies for the same location. The assumptions used in the analysis of <span class="hlt">ice</span> wedge volume have been tested, including trough width being representative of <span class="hlt">ice</span> wedge width, and <span class="hlt">ice</span> wedge <span class="hlt">ice</span> <span class="hlt">content</span> (Pollard and French 1980). This study used specific field sites located near Eureka on Ellesmere Island (N80°01', W85°43') and at Expedition Fiord on Axel Heiberg Island (N79°23', W90°59'). The preliminary results indicate that the methodology used by Ulrich et al, 2014 is transferrable to the Canadian High Arctic, and that <span class="hlt">ice</span> wedge volumes range between 3-10% of the upper part of permafrost. These findings are similar to previous studies and their importance is made all the more evident by the dynamic nature of <span class="hlt">ice</span> wedges where it could be argued that they are a key driver of thermokarst terrain. The ubiquitous nature of <span class="hlt">ice</span> wedges across arctic terrain highlights the importance and the need to improve our understanding of <span class="hlt">ice</span> wedge dynamics, as subsidence from <span class="hlt">ice</span> wedge melt-out could lead to large scale landscape change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1911372D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1911372D"><span>Towards multi-decadal to multi-millennial <span class="hlt">ice</span> core records from coastal west Greenland <span class="hlt">ice</span> caps</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Das, Sarah B.; Osman, Matthew B.; Trusel, Luke D.; McConnell, Joseph R.; Smith, Ben E.; Evans, Matthew J.; Frey, Karen E.; Arienzo, Monica; Chellman, Nathan</p> <p>2017-04-01</p> <p>The Arctic region, and Greenland in particular, is undergoing dramatic change as characterized by atmospheric warming, decreasing sea <span class="hlt">ice</span>, shifting ocean circulation patterns, and rapid <span class="hlt">ice</span> sheet <span class="hlt">mass</span> loss, but longer records are needed to put these changes into context. <span class="hlt">Ice</span> core records from the Greenland <span class="hlt">ice</span> sheet have yielded invaluable insight into past climate change both regionally and globally, and provided important constraints on past surface <span class="hlt">mass</span> balance more directly, but these <span class="hlt">ice</span> cores are most often from the interior <span class="hlt">ice</span> sheet accumulation zone, at high altitude and hundreds of kilometers from the coast. Coastal <span class="hlt">ice</span> caps, situated around the margins of Greenland, have the potential to provide novel high-resolution records of local and regional maritime climate and sea surface conditions, as well as contemporaneous glaciological changes (such as accumulation and surface melt history). But obtaining these records is extremely challenging. Most of these <span class="hlt">ice</span> caps are unexplored, and thus their thickness, age, stratigraphy, and utility as sites of new and unique paleoclimate records is largely unknown. Access is severely limited due to their high altitude, steep relief, small surface area, and inclement weather. Furthermore, their relatively low elevation and marine moderated climate can contribute to significant surface melting and degradation of the <span class="hlt">ice</span> stratigraphy. We recently targeted areas near the Disko Bay region of central west Greenland where maritime <span class="hlt">ice</span> caps are prevalent but unsampled, as potential sites for new multi-decadal to multi-millennial <span class="hlt">ice</span> core records. In 2014 & 2015 we identified two promising <span class="hlt">ice</span> caps, one on Disko Island (1250 m. asl) and one on Nuussuaq Peninsula (1980 m. asl) based on airborne and ground-based geophysical observations and physical and glaciochemical stratigraphy from shallow firn cores. In spring 2015 we collected <span class="hlt">ice</span> cores at both sites using the Badger-Eclipse electromechanical drill, transported by a medley</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1913217L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1913217L"><span>ROBUST hot wire probe efficiency for total water <span class="hlt">content</span> measurements in glaciated conditions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Leroy, Delphine; Lilie, Lyle; Weber, Marc; Schwarzenboeck, Alfons; Strapp, J. Walter</p> <p>2017-04-01</p> <p> airborne instrument package but no clear trend has been highlighted for the moment. References : Davison, C., J. MacLeod, J. Strapp, and D. Buttsworth, 2008: Isokinetic Total Water <span class="hlt">Content</span> Probe in a Naturally Aspirating Configuration: Initial Aerodynamic Design and Testing. 46th AIAA Aerospace Sciences Meeting and Exhibit, American Institute of Aeronautics and Astronautics http://arc.aiaa.org/doi/abs/10.2514/6.2008-435 (Accessed February 9, 2015). Davison, C. R., J. W. Strapp, L. E. Lilie, T. P. Ratvasky, and C. Dumont, 2016: Isokinetic TWC Evaporator Probe: Calculations and Systemic Error Analysis. American Institute of Aeronautics and Astronautics http://arc.aiaa.org/doi/10.2514/6.2016-4060 (Accessed July 29, 2016). Dezitter, F., A. Grandin, J.-L. Brenguier, F. Hervy, H. Schlager, P. Villedieu, and G. Zalamansky, 2013: HAIC - High Altitude <span class="hlt">Ice</span> Crystals. 5th AIAA Atmospheric and Space Environments Conference, American Institute of Aeronautics and Astronautics http://arc.aiaa.org/doi/abs/10.2514/6.2013-2674 (Accessed February 9, 2015). Grandin, A., J.-M. Merle, M. Weber, J. Strapp, A. Protat, and P. King, 2014: AIRBUS Flight Tests in High Total Water <span class="hlt">Content</span> Regions. American Institute of Aeronautics and Astronautics http://arc.aiaa.org/doi/abs/10.2514/6.2014-2753 (Accessed March 8, 2016). Leroy, D., and Coauthors, 2016: HAIC/HIWC field campaigns - Specific findings on <span class="hlt">ice</span> crystals characteristics in high <span class="hlt">ice</span> water <span class="hlt">content</span> cloud regions. American Institute of Aeronautics and Astronautics http://arc.aiaa.org/doi/10.2514/6.2016-4056 (Accessed January 10, 2017). Leroy, D., and Coauthors, 2017: <span class="hlt">Ice</span> Crystal Sizes in High <span class="hlt">Ice</span> Water <span class="hlt">Content</span> Clouds. Part II: Statistics of <span class="hlt">Mass</span> Diameter Percentiles in Tropical Convection Observed during the HAIC/HIWC Project. J. Atmospheric Ocean. Technol., 34, 117-136, doi:10.1175/JTECH-D-15-0246.1. Strapp, J. W., J. MacLeod, and L. Lilie, 2008: Calibration of <span class="hlt">ice</span> water <span class="hlt">content</span> in a wind tunnel/engine test cell facility. 15th Intl. Conf. on Cloud</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.A13D0966Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.A13D0966Y"><span>Seasonal origins of air <span class="hlt">masses</span> transported to Mount Wrangell, Alaska, and comparison with the past atmospheric dust and tritium variations in its <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>Yasunari, T. J.; Shiraiwa, T.; Kanamori, S.; Fujii, Y.; Igarashi, M.; Yamazaki, K.; Benson, C. S.; Hondoh, T.</p> <p>2006-12-01</p> <p>The North Pacific region is subject to various climatic phenomena such as the Pacific Decadal Oscillation (PDO), the El Niño-Southern Oscillation (ENSO), and the Arctic Oscillation (AO), significantly affecting the ocean and the atmosphere. Additionally, material circulation is also very active in this region such as spring dust storms in the desert and arid regions of East Asia and forest fires in Siberia and Alaska. Understanding the complex connections among the climatic phenomena and the material circulation would help in attempts to predict future climate changes. For this subject, we drilled a 50-m <span class="hlt">ice</span> core at the summit of Mount Wrangell, which is located near the coast of Alaska (62°162'170"162°171'N, 144°162'170"162;°171'W, and 4100-m). We analyzed dust particle number density, tritium concentration, and 171 171 171 171 170 162 171 D in the core. The <span class="hlt">ice</span> core spanned the years from 1992 to 2002 and we finally divided the years into five parts (early-spring; late-spring; summer; fall; winter). Dust and tritium amounts varied annually and intra-annually. For further understanding of the factors on those variations, we should know the origins of the seasonal dust and tritium. Hence, we examined their origins by the calculation of everyday 10-days backward trajectory analysis from January 1992 to August 2002 with 3-D wind data of the European Center for Medium-Range Weather Forecast (ECMWF). In early spring, the air <span class="hlt">mass</span> from East Asia increased and it also explained dust increases in springtime, although the air contribution in winter increased too. In late spring, the air <span class="hlt">mass</span> from the stratosphere increased, and it also corresponded to the stratospheric tritium increase in the <span class="hlt">ice</span> core. The air <span class="hlt">masses</span> from Siberia and the North Pacific in the mid-latitude always significantly contributed to Mount Wrangell, although those maximum contributions were fall and summer, respectively. The air <span class="hlt">mass</span> originating in the interior of Alaska and North America did</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JMS...166....4S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JMS...166....4S"><span>Modelling sea <span class="hlt">ice</span> formation in the Terra Nova Bay polynya</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sansiviero, M.; Morales Maqueda, M. Á.; Fusco, G.; Aulicino, G.; Flocco, D.; Budillon, G.</p> <p>2017-02-01</p> <p>Antarctic sea <span class="hlt">ice</span> is constantly exported from the shore by strong near surface winds that open leads and large polynyas in the pack <span class="hlt">ice</span>. The latter, known as wind-driven polynyas, are responsible for significant water <span class="hlt">mass</span> modification due to the high salt flux into the ocean associated with enhanced <span class="hlt">ice</span> growth. In this article, we focus on the wind-driven Terra Nova Bay (TNB) polynya, in the western Ross Sea. Brine rejected during sea <span class="hlt">ice</span> formation processes that occur in the TNB polynya densifies the water column leading to the formation of the most characteristic water <span class="hlt">mass</span> of the Ross Sea, the High Salinity Shelf Water (HSSW). This water <span class="hlt">mass</span>, in turn, takes part in the formation of Antarctic Bottom Water (AABW), the densest water <span class="hlt">mass</span> of the world ocean, which plays a major role in the global meridional overturning circulation, thus affecting the global climate system. A simple coupled sea <span class="hlt">ice</span>-ocean model has been developed to simulate the seasonal cycle of sea <span class="hlt">ice</span> formation and export within a polynya. The sea <span class="hlt">ice</span> model accounts for both thermal and mechanical <span class="hlt">ice</span> processes. The oceanic circulation is described by a one-and-a-half layer, reduced gravity model. The domain resolution is 1 km × 1 km, which is sufficient to represent the salient features of the coastline geometry, notably the Drygalski <span class="hlt">Ice</span> Tongue. The model is forced by a combination of Era Interim reanalysis and in-situ data from automatic weather stations, and also by a climatological oceanic dataset developed from in situ hydrographic observations. The sensitivity of the polynya to the atmospheric forcing is well reproduced by the model when atmospheric in situ measurements are combined with reanalysis data. Merging the two datasets allows us to capture in detail the strength and the spatial distribution of the katabatic winds that often drive the opening of the polynya. The model resolves fairly accurately the sea <span class="hlt">ice</span> drift and sea <span class="hlt">ice</span> production rates in the TNB polynya, leading to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120002589','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120002589"><span>Analysis of a Hovering Rotor in <span class="hlt">Icing</span> Conditions</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Narducci, Robert; Kreeger, Richard E.</p> <p>2012-01-01</p> <p>A high fidelity analysis method is proposed to evaluate the <span class="hlt">ice</span> accumulation and the ensuing rotor performance degradation for a helicopter flying through an <span class="hlt">icing</span> cloud. The process uses computational fluid dynamics (CFD) coupled to a rotorcraft comprehensive code to establish the aerodynamic environment of a trimmed rotor prior to <span class="hlt">icing</span>. Based on local aerodynamic conditions along the rotor span and accounting for the azimuthal variation, an <span class="hlt">ice</span> accumulation analysis using NASA's Lewice3D code is made to establish the <span class="hlt">ice</span> geometry. Degraded rotor performance is quantified by repeating the high fidelity rotor analysis with updates which account for <span class="hlt">ice</span> shape and <span class="hlt">mass</span>. The process is applied on a full-scale UH-1H helicopter in hover using data recorded during the Helicopter <span class="hlt">Icing</span> Flight Test Program.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1913441D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1913441D"><span><span class="hlt">ICE</span> CONTROL - Towards optimizing wind energy production during <span class="hlt">icing</span> events</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dorninger, Manfred; Strauss, Lukas; Serafin, Stefano; Beck, Alexander; Wittmann, Christoph; Weidle, Florian; Meier, Florian; Bourgeois, Saskia; Cattin, René; Burchhart, Thomas; Fink, Martin</p> <p>2017-04-01</p> <p>Forecasts of wind power production loss caused by <span class="hlt">icing</span> weather conditions are produced by a chain of physical models. The model chain consists of a numerical weather prediction model, an <span class="hlt">icing</span> model and a production loss model. Each element of the model chain is affected by significant uncertainty, which can be quantified using targeted observations and a probabilistic forecasting approach. In this contribution, we present preliminary results from the recently launched project <span class="hlt">ICE</span> CONTROL, an Austrian research initiative on measurements, probabilistic forecasting, and verification of <span class="hlt">icing</span> on wind turbine blades. <span class="hlt">ICE</span> CONTROL includes an experimental field phase, consisting of measurement campaigns in a wind park in Rhineland-Palatinate, Germany, in the winters 2016/17 and 2017/18. Instruments deployed during the campaigns consist of a conventional <span class="hlt">icing</span> detector on the turbine hub and newly devised <span class="hlt">ice</span> sensors (eologix Sensor System) on the turbine blades, as well as meteorological sensors for wind, temperature, humidity, visibility, and precipitation type and spectra. Liquid water <span class="hlt">content</span> and spectral characteristics of super-cooled water droplets are measured using a Fog Monitor FM-120. Three cameras document the <span class="hlt">icing</span> conditions on the instruments and on the blades. Different modelling approaches are used to quantify the components of the model-chain uncertainties. The uncertainty related to the initial conditions of the weather prediction is evaluated using the existing global ensemble prediction system (EPS) of the European Centre for Medium-Range Weather Forecasts (ECMWF). Furthermore, observation system experiments are conducted with the AROME model and its 3D-Var data assimilation to investigate the impact of additional observations (such as Mode-S aircraft data, SCADA data and MSG cloud mask initialization) on the numerical <span class="hlt">icing</span> forecast. The uncertainty related to model formulation is estimated from multi-physics ensembles based on the Weather Research</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150000744','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150000744"><span>A Thermal Analysis of a Hot-Wire Probe for <span class="hlt">Icing</span> Applications</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Struk, Peter M.; Rigby, David L.; Venkataraman, Krishna</p> <p>2014-01-01</p> <p>This paper presents a steady-state thermal model of a hot-wire instrument applicable to atmospheric measurement of water <span class="hlt">content</span> in clouds. In this application, the power required to maintain the wire at a given temperature is used to deduce the water <span class="hlt">content</span> of the cloud. The model considers electrical resistive heating, axial conduction, convection to the flow, radiation to the surroundings, as well as energy loss due to the heating, melting, and evaporation of impinging liquid and or <span class="hlt">ice</span>. All of these parameters can be varied axially along the wire. The model further introduces a parameter called the evaporation potential which locally gauges the maximum fraction of incoming water that evaporates. The primary outputs of the model are the steady-state power required to maintain a spatially-average constant temperature as well as the variation of that temperature and other parameters along the wire. The model is used to understand the sensitivity of the hot-wire performance to various flow and boundary conditions including a detailed comparison of dry air and wet (i.e. cloud-on) conditions. The steady-state power values are compared to experimental results from a Science Engineering Associates (SEA) Multi-Element probe, a commonly used water-<span class="hlt">content</span> measurement instrument. The model results show good agreement with experiment for both dry and cloud-on conditions with liquid water <span class="hlt">content</span>. For <span class="hlt">ice</span>, the experimental measurements under read the actual water <span class="hlt">content</span> due to incomplete evaporation and splashing. Model results, which account for incomplete evaporation, are still higher than experimental results where the discrepancy is attributed to splashing <span class="hlt">mass</span>-loss which is not accounted in the model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120009089','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120009089"><span>Overview and Assessment of Antarctic <span class="hlt">Ice</span>-Sheet <span class="hlt">Mass</span> Balance Estimates: 1992-2009</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zwally, H. Jay; Giovinetto, Mario B.</p> <p>2011-01-01</p> <p><span class="hlt">Mass</span> balance estimates for the Antarctic <span class="hlt">Ice</span> Sheet (AIS) in the 2007 report by the Intergovernmental Panel on Climate Change and in more recent reports lie between approximately ?50 to -250 Gt/year for 1992 to 2009. The 300 Gt/year range is approximately 15% of the annual <span class="hlt">mass</span> input and 0.8 mm/year Sea Level Equivalent (SLE). Two estimates from radar altimeter measurements of elevation change by European Remote-sensing Satellites (ERS) (?28 and -31 Gt/year) lie in the upper part, whereas estimates from the Input-minus-Output Method (IOM) and the Gravity Recovery and Climate Experiment (GRACE) lie in the lower part (-40 to -246 Gt/year). We compare the various estimates, discuss the methodology used, and critically assess the results. We also modify the IOM estimate using (1) an alternate extrapolation to estimate the discharge from the non-observed 15% of the periphery, and (2) substitution of input from a field data compilation for input from an atmospheric model in 6% of area. The modified IOM estimate reduces the loss from 136 Gt/year to 13 Gt/year. Two ERS-based estimates, the modified IOM, and a GRACE-based estimate for observations within 1992 2005 lie in a narrowed range of ?27 to -40 Gt/year, which is about 3% of the annual <span class="hlt">mass</span> input and only 0.2 mm/year SLE. Our preferred estimate for 1992 2001 is -47 Gt/year for West Antarctica, ?16 Gt/year for East Antarctica, and -31 Gt/year overall (?0.1 mm/year SLE), not including part of the Antarctic Peninsula (1.07% of the AIS area). Although recent reports of large and increasing rates of <span class="hlt">mass</span> loss with time from GRACE-based studies cite agreement with IOM results, our evaluation does not support that conclusion</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C41B0664M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C41B0664M"><span>Oceanographic Influences on <span class="hlt">Ice</span> Shelves and Drainage in the Amundsen Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Minzoni, R. T.; Anderson, J. B.; Majewski, W.; Yokoyama, Y.; Fernandez, R.; Jakobsson, M.</p> <p>2016-12-01</p> <p>Marine sediment cores collected during the IB OdenSouthern Ocean 2009-2010 cruise are used to reconstruct the Holocene history of the Cosgrove <span class="hlt">Ice</span> Shelf, which today occupies Ferrero Bay, a large embayment of eastern Pine Island Bay. Detailed sedimentology, geochemistry, and micropaleontology of cores, in conjunction with subbottom profiles, reveal an unexpected history of recession. Presence of planktic foraminifera at the base of Kasten Core-15 suggests an episode of enhanced circulation beneath a large <span class="hlt">ice</span> shelf that covered the Amundsen Sea during the Early Holocene, and relatively warm water incursion has been interpreted as a potential culprit for major recession and <span class="hlt">ice</span> <span class="hlt">mass</span> loss by 10.7 cal kyr BP from radiocarbon dating. Fine sediment deposition and low productivity throughout the Mid Holocene indicate long-lived stability of the Cosgrove <span class="hlt">Ice</span> Shelf in Ferrero Bay, despite regional warming evident from <span class="hlt">ice</span> core data and <span class="hlt">ice</span> shelf loss in the Antarctic Peninsula. High productivity and diatom abundance signify opening of Ferrero Bay and recession of the Cosgrove <span class="hlt">Ice</span> Shelf to its present day configuration by 2.0 cal kyr BP. This coincides with deglaciation of an island near Canisteo Peninsula according to published cosmogenic exposure ages. Presence of benthic foraminifera imply that warm deep water influx beneath the extended Cosgrove <span class="hlt">Ice</span> Shelf was a mechanism for under-melting the <span class="hlt">ice</span> shelf and destabilizing the grounding line. Major <span class="hlt">ice</span> shelf recession may also entail continental <span class="hlt">ice</span> <span class="hlt">mass</span> loss from the eastern sector of the Amundsen Sea during the Late Holocene. Oceanographic forcing remains a key concern for the current stability of the Antarctic <span class="hlt">Ice</span> Sheet, especially along the tidewater margins of West Antarctica. Ongoing work on diatom and foraminiferal assemblages of the Late Holocene in Ferrero Bay and other fjord settings will improve our understanding of recent oceanographic changes and their potential influence on <span class="hlt">ice</span> shelves and outlet glaciers</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20070032808','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20070032808"><span>A Database of Supercooled Large Droplet <span class="hlt">Ice</span> Accretions</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>VanZante, Judith Foss</p> <p>2007-01-01</p> <p>A unique, publicly available database regarding supercooled large droplet <span class="hlt">ice</span> accretions has been developed in NASA Glenn's <span class="hlt">Icing</span> Research Tunnel. Identical cloud and flight conditions were generated for five different airfoil models. The models chosen represent a variety of aircraft types from the horizontal stabilizer of a large trans-port aircraft to the wings of regional, business, and general aviation aircraft. In addition to the standard documentation methods of 2D <span class="hlt">ice</span> shape tracing and imagery, <span class="hlt">ice</span> <span class="hlt">mass</span> measurements were also taken. This database will also be used to validate and verify the extension of the <span class="hlt">ice</span> accretion code, LEWICE, into the SLD realm.</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.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3742901','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3742901"><span>Usefulness of the <span class="hlt">Ice</span>-Cream Cone Pattern in Computed Tomography for Prediction of Angiomyolipoma in Patients With a Small Renal <span class="hlt">Mass</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>Kim, Kwang Ho; Yun, Bu Hyeon; Hwang, In Sang; Hwang, Eu Chang; Kang, Taek Won; Kwon, Dong Deuk; Park, Kwangsung; Kim, Jin Woong</p> <p>2013-01-01</p> <p>Purpose A morphologic contour method for assessing an exophytic renal <span class="hlt">mass</span> as benign versus malignant on the basis of the shape of the interface with the renal parenchyma was recently developed. We investigated the usefulness of this morphologic contour method for predicting angiomyolipoma (AML) in patients who underwent partial nephrectomy for small renal <span class="hlt">masses</span> (SRMs). Materials and Methods From January 2004 to March 2013, among 197 patients who underwent partial nephrectomy for suspicious renal cell carcinoma (RCC), the medical records of 153 patients with tumors (AML or RCC) ≤3 cm in diameter were retrospectively reviewed. Patient characteristics including age, gender, type of surgery, size and location of tumor, pathologic results, and specific findings of the imaging study ("<span class="hlt">ice</span>-cream cone" shape) were compared between the AML and RCC groups. Results AML was diagnosed in 18 patients and RCC was diagnosed in 135 patients. Gender (p=0.001), tumor size (p=0.032), and presence of the <span class="hlt">ice</span>-cream cone shape (p=0.001) showed statistically significant differences between the AML group and the RCC group. In the multivariate logistic regression analysis, female gender (odds ratio [OR], 5.20; 95% confidence interval [CI], 1.45 to 18.57; p=0.011), tumor size (OR, 0.34; 95% CI, 0.12 to 0.92; p=0.034), and presence of the <span class="hlt">ice</span>-cream cone shape (OR, 18.12; 95% CI, 4.97 to 66.06; p=0.001) were predictors of AML. Conclusions This study confirmed a high incidence of AML in females. Also, the <span class="hlt">ice</span>-cream cone shape and small tumor size were significant predictors of AML in SRMs. These finding could be beneficial for counseling patients with SRMs. PMID:23956824</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.C23C0646G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.C23C0646G"><span>Numerical model of <span class="hlt">ice</span> melange expansion during abrupt <span class="hlt">ice</span>-shelf collapse</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Guttenberg, N.; Abbot, D. S.; Amundson, J. M.; Burton, J. C.; Cathles, L. M.; Macayeal, D. R.; Zhang, W.</p> <p>2010-12-01</p> <p>Satellite imagery of the February 2008 Wilkins <span class="hlt">Ice</span>-Shelf Collapse event reveals that a large percentage of the involved <span class="hlt">ice</span> shelf was converted to capsized icebergs and broken fragments of icebergs over a relatively short period of time, possibly less than 24 hours. The extreme violence and short time scale of the event, and the considerable reduction of gravitational potential energy between upright and capsized icebergs, suggests that iceberg capsize might be an important driving mechanism controlling both the rate and spatial extent of <span class="hlt">ice</span> shelf collapse. To investigate this suggestion, we have constructed an idealized, 2-dimensional model of a disintegrating <span class="hlt">ice</span> shelf composed of a large number (N~100 to >1000) of initially well-packed icebergs of rectangular cross section. The model geometry consists of a longitudinal cross section of the idealized <span class="hlt">ice</span> shelf from grounding line (or the upstream extent of <span class="hlt">ice</span>-shelf fragmentation) to seaward <span class="hlt">ice</span> front, and includes the region beyond the initial <span class="hlt">ice</span> front to cover the open, <span class="hlt">ice</span>-free water into which the collapsing <span class="hlt">ice</span> shelf expands. The seawater in which the icebergs float is treated as a hydrostatic fluid in the computation of iceberg orientation (e.g., the evaluation of buoyancy forces and torques), thereby eliminating the complexities of free-surface waves, but net horizontal drift of the icebergs is resisted by a linear drag law designed to energy dissipation by viscous forces and surface-gravity-wave radiation. Icebergs interact via both elastic and inelastic contacts (typically a corner of one iceberg will scrape along the face of its neighbor). <span class="hlt">Ice</span>-shelf collapse in the model is embodied by the <span class="hlt">mass</span> capsize of a large proportion of the initially packed icebergs and the consequent advancement of the <span class="hlt">ice</span> front (leading edge). Model simulations are conducted to examine (a) the threshold of stability (e.g., what density of initially capsizable icebergs is needed to allow a small perturbation to the system</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120009093','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120009093"><span>The Antarctic <span class="hlt">Ice</span> Sheet, Sea <span class="hlt">Ice</span>, and the Ozone Hole: Satellite Observations of how they are Changing</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parkinson, Claire L.</p> <p>2012-01-01</p> <p>Antarctica is the Earth's coldest and highest continent and has major impacts on the climate and life of the south polar vicinity. It is covered almost entirely by the Earth's largest <span class="hlt">ice</span> sheet by far, with a volume of <span class="hlt">ice</span> so great that if all the Antarctic <span class="hlt">ice</span> were to go into the ocean (as <span class="hlt">ice</span> or liquid water), this would produce a global sea level rise of about 60 meters (197 feet). The continent is surrounded by sea <span class="hlt">ice</span> that in the wintertime is even more expansive than the continent itself and in the summertime reduces to only about a sixth of its wintertime extent. Like the continent, the expansive sea <span class="hlt">ice</span> cover has major impacts, reflecting the sun's radiation back to space, blocking exchanges between the ocean and the atmosphere, and providing a platform for some animal species while impeding other species. Far above the continent, the Antarctic ozone hole is a major atmospheric phenomenon recognized as human-caused and potentially quite serious to many different life forms. Satellites are providing us with remarkable information about the <span class="hlt">ice</span> sheet, the sea <span class="hlt">ice</span>, and the ozone hole. Satellite visible and radar imagery are providing views of the large scale structure of the <span class="hlt">ice</span> sheet never seen before; satellite laser altimetry has produced detailed maps of the topography of the <span class="hlt">ice</span> sheet; and an innovative gravity-measuring two-part satellite has allowed mapping of regions of <span class="hlt">mass</span> loss and <span class="hlt">mass</span> gain on the <span class="hlt">ice</span> sheet. The surrounding sea <span class="hlt">ice</span> cover has a satellite record that goes back to the 1970s, allowing trend studies that show a decreasing sea <span class="hlt">ice</span> presence in the region of the Bellingshausen and Amundsen seas, to the west of the prominent Antarctic Peninsula, but increasing sea <span class="hlt">ice</span> presence around much of the rest of the continent. Overall, sea <span class="hlt">ice</span> extent around Antarctica has increased at an average rate of about 17,000 square kilometers per year since the late 1970s, as determined from satellite microwave data that can be collected under both light and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C21H..01L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C21H..01L"><span><span class="hlt">Ice</span> sheet climate modeling: past achievements, ongoing challenges, and future endeavors</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lenaerts, J.</p> <p>2017-12-01</p> <p>Fluctuations in surface <span class="hlt">mass</span> balance (SMB) mask out a substantial portion of contemporary Greenland and Antarctic <span class="hlt">ice</span> sheet <span class="hlt">mass</span> loss. That implies that we need accurate, consistent, and long-term SMB time series to isolate the <span class="hlt">mass</span> loss signal. This in turn requires understanding of the processes driving SMB, and how they interplay. The primary controls on present-day <span class="hlt">ice</span> sheet SMB are snowfall, which is regulated by large-scale atmospheric variability, and surface meltwater production at the <span class="hlt">ice</span> 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 <span class="hlt">ice</span> sheets. Climate models provide an integrated framework to simulate all these individual <span class="hlt">ice</span> 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 <span class="hlt">ice</span> sheet climate system, but also enabled to obtain increasingly accurate estimates of <span class="hlt">ice</span> sheet SMB. However, regional models are not suitable to capture the mutual interactions between <span class="hlt">ice</span> 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 <span class="hlt">ice</span> sheet climate in the Community Earth System Model (CESM). In particular, we focus on an improved representation of polar firn, <span class="hlt">ice</span> 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 <span class="hlt">ice</span> sheet SMB, its drivers, and past and present changes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EPJWC.14501003D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EPJWC.14501003D"><span>Investigating cosmic rays and air shower physics with <span class="hlt">IceCube/Ice</span>Top</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dembinski, Hans</p> <p>2017-06-01</p> <p><span class="hlt">Ice</span>Cube is a cubic-kilometer detector in the deep <span class="hlt">ice</span> at South Pole. Its square-kilometer surface array, <span class="hlt">Ice</span>Top, is located at 2800 m altitude. <span class="hlt">Ice</span>Top is large and dense enough to cover the cosmic-ray energy spectrum from PeV to EeV energies with a remarkably small systematic uncertainty, thanks to being close to the shower maximum. The experiment offers new insights into hadronic physics of air showers by observing three components: the electromagnetic signal at the surface, GeV muons in the periphery of the showers, and TeV muons in the deep <span class="hlt">ice</span>. The cosmic-ray flux is measured with the surface signal. The <span class="hlt">mass</span> composition is extracted from the energy loss of TeV muons observed in the deep <span class="hlt">ice</span> in coincidence with signals at the surface. The muon lateral distribution is obtained from GeV muons identified in surface signals in the periphery of the shower. The energy spectrum of the most energetic TeV muons is also under study, as well as special events with laterally separated TeV muon tracks which originate from high-pT TeV muons. A combination of all these measurements opens the possibility to perform powerful new tests of hadronic interaction models used to simulate air showers. The latest results will be reviewed from this perspective.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C23C0797N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C23C0797N"><span>A downscaled 1 km dataset of daily Greenland <span class="hlt">ice</span> sheet surface <span class="hlt">mass</span> balance components (1958-2014)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Noel, B.; Van De Berg, W. J.; Fettweis, X.; Machguth, H.; Howat, I. M.; van den Broeke, M. R.</p> <p>2015-12-01</p> <p>The current spatial resolution in regional climate models (RCMs), typically around 5 to 20 km, remains too coarse to accurately reproduce the spatial variability in surface <span class="hlt">mass</span> balance (SMB) components over the narrow ablation zones, marginal outlet glaciers and neighbouring <span class="hlt">ice</span> caps of the Greenland <span class="hlt">ice</span> sheet (GrIS). In these topographically rough terrains, the SMB components are highly dependent on local variations in topography. However, the relatively low-resolution elevation and <span class="hlt">ice</span> mask prescribed in RCMs contribute to significantly underestimate melt and runoff in these regions due to unresolved valley glaciers and fjords. Therefore, near-km resolution topography is essential to better capture SMB variability in these spatially restricted regions. We present a 1 km resolution dataset of daily GrIS SMB covering the period 1958-2014, which is statistically downscaled from data of the polar regional climate model RACMO2.3 at 11 km, using an elevation dependence. The dataset includes all individual SMB components projected on the elevation and <span class="hlt">ice</span> mask from the GIMP DEM, down-sampled to 1 km. Daily runoff and sublimation are interpolated to the 1 km topography using a local regression to elevation valid for each day specifically; daily precipitation is bi-linearly downscaled without elevation corrections. The daily SMB dataset is then reconstructed by summing downscaled precipitation, sublimation and runoff. High-resolution elevation and <span class="hlt">ice</span> mask allow for properly resolving the narrow ablation zones and valley glaciers at the GrIS margins, leading to significant increase in runoff estimate. In these regions, and especially over narrow glaciers tongues, the downscaled products improve on the original RACMO2.3 outputs by better representing local SMB patterns through a gradual ablation increase towards the GrIS margins. We discuss the impact of downscaling on the SMB components in a case study for a spatially restricted region, where large elevation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMED11E..02D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMED11E..02D"><span>School of <span class="hlt">Ice</span>: US <span class="hlt">Ice</span> Drilling Program Made Accessible to Faculty at Minority-Serving Institutions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Davis, H. B.; Hoffman, L. T.</p> <p>2017-12-01</p> <p>The School of <span class="hlt">Ice</span> program is designed for college faculty who teach at minority-serving institutions or historically black colleges and universities to help build their background knowledge about <span class="hlt">ice</span> core science and climate change and gain activities and labs for transferring information to their students. In this session, you will learn about the information and activities shared with faculty and the effect of the Institute on faculty. This session will provide an overview of activities that faculty can use to engage students in <span class="hlt">ice</span> drilling processes and results. Faculty who have attended this institute in the last four years have reported increases in their understanding of the <span class="hlt">content</span> and how to teach it.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JGRF..119.1995M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JGRF..119.1995M"><span>Field-calibrated model of melt, refreezing, and runoff for polar <span class="hlt">ice</span> caps: Application to Devon <span class="hlt">Ice</span> Cap</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Morris, Richard M.; Mair, Douglas W. F.; Nienow, Peter W.; Bell, Christina; Burgess, David O.; Wright, Andrew P.</p> <p>2014-09-01</p> <p>Understanding the controls on the amount of surface meltwater that refreezes, rather than becoming runoff, over polar <span class="hlt">ice</span> <span class="hlt">masses</span> is necessary for modeling their surface <span class="hlt">mass</span> balance and ultimately for predicting their future contributions to global sea level change. We present a modified version of a physically based model that includes an energy balance routine and explicit calculation of near-surface meltwater refreezing capacity, to simulate the evolution of near-surface density and temperature profiles across Devon <span class="hlt">Ice</span> Cap in Arctic Canada. Uniquely, our model is initiated and calibrated using high spatial resolution measurements of snow and firn densities across almost the entire elevation range of the <span class="hlt">ice</span> cap for the summer of 2004 and subsequently validated with the same type of measurements obtained during the very different meteorological conditions of summer 2006. The model captures the spatial variability across the transect in bulk snowpack properties although it slightly underestimates the flow of meltwater into the firn of previous years. The percentage of meltwater that becomes runoff is similar in both years; however, the spatial pattern of this melt-runoff relationship is different in the 2 years. The model is found to be insensitive to variation in the depth of impermeable layers within the firn but is very sensitive to variation in air temperature, since the refreezing capacity of firn decreases with increasing temperature. We highlight that the sensitivity of the <span class="hlt">ice</span> cap's surface <span class="hlt">mass</span> balance to air temperature is itself dependent on air temperature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AHEEM..64..115S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AHEEM..64..115S"><span>SPH Modelling of Sea-<span class="hlt">ice</span> Pack Dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Staroszczyk, Ryszard</p> <p>2017-12-01</p> <p>The paper is concerned with the problem of sea-<span class="hlt">ice</span> pack motion and deformation under the action of wind and water currents. Differential equations describing the dynamics of <span class="hlt">ice</span>, with its very distinct mateFfigrial responses in converging and diverging flows, express the <span class="hlt">mass</span> and linear momentum balances on the horizontal plane (the free surface of the ocean). These equations are solved by the fully Lagrangian method of smoothed particle hydrodynamics (SPH). Assuming that the <span class="hlt">ice</span> behaviour can be approximated by a non-linearly viscous rheology, the proposed SPH model has been used to simulate the evolution of a sea-<span class="hlt">ice</span> pack driven by wind drag stresses. The results of numerical simulations illustrate the evolution of an <span class="hlt">ice</span> pack, including variations in <span class="hlt">ice</span> thickness and <span class="hlt">ice</span> area fraction in space and time. The effects of different initial <span class="hlt">ice</span> pack configurations and of different conditions assumed at the coast-<span class="hlt">ice</span> interface are examined. In particular, the SPH model is applied to a pack flow driven by a vortex wind to demonstrate how well the Lagrangian formulation can capture large deformations and displacements of sea <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018TCry...12.1511H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018TCry...12.1511H"><span>Simulating <span class="hlt">ice</span> thickness and velocity evolution of Upernavik Isstrøm 1849-2012 by forcing prescribed terminus positions in ISSM</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Haubner, Konstanze; Box, Jason E.; Schlegel, Nicole J.; Larour, Eric Y.; Morlighem, Mathieu; Solgaard, Anne M.; Kjeldsen, Kristian K.; Larsen, Signe H.; Rignot, Eric; Dupont, Todd K.; Kjær, Kurt H.</p> <p>2018-04-01</p> <p>Tidewater glacier velocity and <span class="hlt">mass</span> balance are known to be highly responsive to terminus position change. Yet it remains challenging for <span class="hlt">ice</span> flow models to reproduce observed <span class="hlt">ice</span> margin changes. Here, using the <span class="hlt">Ice</span> Sheet System Model (ISSM; Larour et al. 2012), we simulate the <span class="hlt">ice</span> velocity and thickness changes of Upernavik Isstrøm (north-western Greenland) by prescribing a collection of 27 observed terminus positions spanning 164 years (1849-2012). The simulation shows increased <span class="hlt">ice</span> velocity during the 1930s, the late 1970s and between 1995 and 2012 when terminus retreat was observed along with negative surface <span class="hlt">mass</span> balance anomalies. Three distinct <span class="hlt">mass</span> balance states are evident in the reconstruction: (1849-1932) with near zero <span class="hlt">mass</span> balance, (1932-1992) with <span class="hlt">ice</span> <span class="hlt">mass</span> loss dominated by <span class="hlt">ice</span> dynamical flow, and (1998-2012), when increased retreat and negative surface <span class="hlt">mass</span> balance anomalies led to <span class="hlt">mass</span> loss that was twice that of any earlier period. Over the multi-decadal simulation, <span class="hlt">mass</span> loss was dominated by thinning and acceleration responsible for 70 % of the total <span class="hlt">mass</span> loss induced by prescribed change in terminus position. The remaining 30 % of the total <span class="hlt">ice</span> <span class="hlt">mass</span> loss resulted directly from prescribed terminus retreat and decreasing surface <span class="hlt">mass</span> balance. Although the method can not explain the cause of glacier retreat, it enables the reconstruction of <span class="hlt">ice</span> flow and geometry during 1849-2012. Given annual or seasonal observed terminus front positions, this method could be a useful tool for evaluating simulations investigating the effect of calving laws.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C41A0692S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C41A0692S"><span>A Newly Updated Database of Elevation-changes of the Greenand <span class="hlt">Ice</span> Sheet to Study Surface Processes and <span class="hlt">Ice</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>Schenk, A. F.; Csatho, B. M.; van den Broeke, M.; Kuipers Munneke, P.</p> <p>2015-12-01</p> <p>This paper reports about important upgrades of the Greenland <span class="hlt">Ice</span> Sheet (GrIS) surface elevation and elevation-change database obtained with our Surface Elevation And Change detection (SERAC) software suite. We have developed SERAC to derive information from laser altimetry data, particularly time series of elevation changes and their partitioning into changes caused by <span class="hlt">ice</span> dynamics. This allows direct investigation of <span class="hlt">ice</span> dynamic processes that is much needed for improving the predictive power of <span class="hlt">ice</span> sheet models. SERAC is different from most other change detection methods. It is based on detecting changes of surface patches, about 1 km by 1 km in size, rather than deriving elevation changes from individual laser points. The current database consists of ~100,000 time series with satellite laser altimetry data from ICESat, airborne laser observations obtained by NASA's Airborne Topographic Mapper (ATM) and the Land, Vegetation and <span class="hlt">Ice</span> Sensor (LVIS). The upgrade is significant, because not only new observations from 2013 and 2014 have been added but also a number of improvements lead to a more comprehensive and consistent record of elevation-changes. First, we used the model that gives in addition to <span class="hlt">ice</span> sheet also information about <span class="hlt">ice</span> caps and glaciers (Rastner et al., 2012) for deciding if a laser point is on the <span class="hlt">ice</span> sheet or <span class="hlt">ice</span> cap. Then we added small gaps that exist in the ICESat GLA12 data set because the <span class="hlt">ice</span> sheet mask is not wide enough. The new database is now more complete and will facilitate more accurate comparisons of <span class="hlt">mass</span> balance studies obtained from the Gravity Recovery and Climate Experiment system (GRACE). For determining the part of a time series caused by <span class="hlt">ice</span> dynamics we used the new firn compaction model and Surface <span class="hlt">Mass</span> Balance (SMB) estimates from RACMO2.3. The new database spans the time period from 1993 to 2014. Adding new observations amounts to a spatial densification of the old record and at the same time extends the time domain by two</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-GSFC_20171208_Archive_e001453.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-GSFC_20171208_Archive_e001453.html"><span>Antarctic <span class="hlt">Ice</span> Shelf Loss Comes From Underneath</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2017-12-08</p> <p>Calving front of an <span class="hlt">ice</span> shelf in West Antarctica. The traditional view on <span class="hlt">ice</span> shelves, the floating extensions of seaward glaciers, has been that they mostly lose <span class="hlt">ice</span> by shedding icebergs. A new study by NASA and university researchers has found that warm ocean waters melting the <span class="hlt">ice</span> sheets from underneath account for 55 percent of all <span class="hlt">ice</span> shelf <span class="hlt">mass</span> loss in Antarctica. This image was taken during the 2012 Antarctic campaign of NASA's Operation <span class="hlt">Ice</span>Bridge, a mission that provided data for the new <span class="hlt">ice</span> shelf study. Read more: www.nasa.gov/topics/earth/features/earth20130613.html Credit: NASA/GSFC/Jefferson Beck NASA image use policy. NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. Follow us on Twitter Like us on Facebook Find us on Instagram</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19850017733&hterms=glacier+melt&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dglacier%2Bmelt','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19850017733&hterms=glacier+melt&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dglacier%2Bmelt"><span>Potential Climatic Effects on the Greenland <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bindschadler, R. A.</p> <p>1984-01-01</p> <p>The Greenland <span class="hlt">Ice</span> Sheet covers an area of 1,720,000 sq. km and contains approximately 2,600,000 cu km of <span class="hlt">ice</span>. Most of the <span class="hlt">ice</span> sheet receives an excess of snow accumulation over the amount of <span class="hlt">ice</span> lost to wind, meltwater run-off or other ablative processes. The majority of <span class="hlt">mass</span> loss occurs at the margin of the <span class="hlt">ice</span> sheet as either surface melt, which flows into the sea or calving of icebergs from the tongues of outlet glaciers. Many estimates of these processes were published. An average of five published estimates is summarized. If these estimates are correct, then the Greenland <span class="hlt">Ice</span> Sheet is in approximate equilibrium and contributes 490 cu km/a of fresh water to the North Atlantic and Arctic Oceans. Climate effects, <span class="hlt">ice</span> sheet flow, and application of remote sensing to tracking of the <span class="hlt">ice</span> sheet are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28025536','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28025536"><span>Simultaneous Moisture <span class="hlt">Content</span> and <span class="hlt">Mass</span> Flow Measurements in Wood Chip Flows Using Coupled Dielectric and Impact Sensors.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pan, Pengmin; McDonald, Timothy; Fulton, John; Via, Brian; Hung, John</p> <p>2016-12-23</p> <p>An 8-electrode capacitance tomography (ECT) sensor was built and used to measure moisture <span class="hlt">content</span> (MC) and <span class="hlt">mass</span> flow of pine chip flows. The device was capable of directly measuring total water quantity in a sample but was sensitive to both dry matter and moisture, and therefore required a second measurement of <span class="hlt">mass</span> flow to calculate MC. Two means of calculating the <span class="hlt">mass</span> flow were used: the first being an impact sensor to measure total <span class="hlt">mass</span> flow, and the second a volumetric approach based on measuring total area occupied by wood in images generated using the capacitance sensor's tomographic mode. Tests were made on 109 groups of wood chips ranging in moisture <span class="hlt">content</span> from 14% to 120% (dry basis) and wet weight of 280 to 1100 g. Sixty groups were randomly selected as a calibration set, and the remaining were used for validation of the sensor's performance. For the combined capacitance/force transducer system, root mean square errors of prediction (RMSEP) for wet <span class="hlt">mass</span> flow and moisture <span class="hlt">content</span> were 13.42% and 16.61%, respectively. RMSEP using the combined volumetric <span class="hlt">mass</span> flow/capacitance sensor for dry <span class="hlt">mass</span> flow and moisture <span class="hlt">content</span> were 22.89% and 24.16%, respectively. Either of the approaches was concluded to be feasible for prediction of moisture <span class="hlt">content</span> in pine chip flows, but combining the impact and capacitance sensors was easier to implement. In situations where flows could not be impeded, however, the tomographic approach would likely be more useful.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.C21D0668Q','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.C21D0668Q"><span>Evaluation of <span class="hlt">Ice</span> sheet evolution and coastline changes from 1960s in Amery <span class="hlt">Ice</span> Shelf using multi-source remote sensing images</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Qiao, G.; Ye, W.; Scaioni, M.; Liu, S.; Feng, T.; Liu, Y.; Tong, X.; Li, R.</p> <p>2013-12-01</p> <p>Global change is one of the major challenges that all the nations are commonly facing, and the Antarctica <span class="hlt">ice</span> sheet changes have been playing a critical role in the global change research field during the past years. Long time-series of <span class="hlt">ice</span> sheet observations in Antarctica would contribute to the quantitative evaluation and precise prediction of the effects on global change induced by the <span class="hlt">ice</span> sheet, of which the remote sensing technology would make critical contributions. As the biggest <span class="hlt">ice</span> shelf and one of the dominant drainage systems in East Antarctic, the Amery <span class="hlt">Ice</span> Shelf has been making significant contributions to the <span class="hlt">mass</span> balance of the Antarctic. Study of Amery <span class="hlt">Ice</span> shelf changes would advance the understanding of Antarctic <span class="hlt">ice</span> shelf evolution as well as the overall <span class="hlt">mass</span> balance. At the same time, as one of the important indicators of Antarctica <span class="hlt">ice</span> sheet characteristics, coastlines that can be detected from remote sensing imagery can help reveal the nature of the changes of <span class="hlt">ice</span> sheet evolution. Most of the scientific research on Antarctica with satellite remote sensing dated from 1970s after LANDSAT satellite was brought into operation. It was the declassification of the cold war satellite reconnaissance photographs in 1995, known as Declassified Intelligence Satellite Photograph (DISP) that provided a direct overall view of the Antarctica <span class="hlt">ice</span>-sheet's configuration in 1960s, greatly extending the time span of Antarctica surface observations. This paper will present the evaluation of <span class="hlt">ice</span>-sheet evolution and coastline changes in Amery <span class="hlt">Ice</span> Shelf from 1960s, by using multi-source remote sensing images including the DISP images and the modern optical satellite images. The DISP images scanned from negatives were first interior-oriented with the associated parameters, and then bundle block adjustment technology was employed based on the tie points and control points, to derive the mosaic image of the research region. Experimental results of coastlines generated</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26761671','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26761671"><span>Studies on Physical and Sensory Properties of Premium Vanilla <span class="hlt">Ice</span> Cream Distributed in Korean Market.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Choi, Mi-Jung; Shin, Kwang-Soon</p> <p>2014-01-01</p> <p>The object of this study was to investigate the difference in physical and sensory properties of various premium <span class="hlt">ice</span> creams. The physical properties of the various <span class="hlt">ice</span> creams were compared by manufacturing brand. The water <span class="hlt">contents</span> of the samples differed, with BR having the highest value at 60.5%, followed by NT and CS at 57.8% and 56.9%, respectively. The higher the water <span class="hlt">content</span>, the lower Brix and milk fat <span class="hlt">contents</span> in all samples. The density of the samples showed almost similar values in all samples (p>0.05). The viscosity of each <span class="hlt">ice</span> cream had no effect on the water <span class="hlt">content</span> in any of the brands. Before melting of the <span class="hlt">ice</span> cream, the total color difference was dependent on the lightness, especially in the vanilla <span class="hlt">ice</span> cream, owing to the reflection of light on the surface of the <span class="hlt">ice</span> crystals. The CS product melted the fastest. In the sensory test, CS obtained a significantly higher sweetness intensity score but a lower score for color intensity, probably due to the smaller difference in total color, by which consumers might consider the color of CS as less intense. From this study, the cold chain system for <span class="hlt">ice</span> cream distribution might be important to decide the physical properties although the concentration of milk fat is key factor in premium <span class="hlt">ice</span> cream.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4662189','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4662189"><span>Studies on Physical and Sensory Properties of Premium Vanilla <span class="hlt">Ice</span> Cream Distributed in Korean Market</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Choi, Mi-Jung</p> <p>2014-01-01</p> <p>The object of this study was to investigate the difference in physical and sensory properties of various premium <span class="hlt">ice</span> creams. The physical properties of the various <span class="hlt">ice</span> creams were compared by manufacturing brand. The water <span class="hlt">contents</span> of the samples differed, with BR having the highest value at 60.5%, followed by NT and CS at 57.8% and 56.9%, respectively. The higher the water <span class="hlt">content</span>, the lower Brix and milk fat <span class="hlt">contents</span> in all samples. The density of the samples showed almost similar values in all samples (p>0.05). The viscosity of each <span class="hlt">ice</span> cream had no effect on the water <span class="hlt">content</span> in any of the brands. Before melting of the <span class="hlt">ice</span> cream, the total color difference was dependent on the lightness, especially in the vanilla <span class="hlt">ice</span> cream, owing to the reflection of light on the surface of the <span class="hlt">ice</span> crystals. The CS product melted the fastest. In the sensory test, CS obtained a significantly higher sweetness intensity score but a lower score for color intensity, probably due to the smaller difference in total color, by which consumers might consider the color of CS as less intense. From this study, the cold chain system for <span class="hlt">ice</span> cream distribution might be important to decide the physical properties although the concentration of milk fat is key factor in premium <span class="hlt">ice</span> cream. PMID:26761671</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.P43C2117H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.P43C2117H"><span><span class="hlt">Ice</span> under cover: Using bulk spatial and physical properties of probable ground <span class="hlt">ice</span> driven <span class="hlt">mass</span> wasting features on Ceres to better understand its surface</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hughson, K.; Russell, C.; Schmidt, B. E.; Chilton, H.; Scully, J. E. C.; Castillo, J. C.; Combe, J. P.; Ammannito, E.; Sizemore, H.; Platz, T.; Byrne, S.; Nathues, A.; Raymond, C. A.</p> <p>2016-12-01</p> <p>NASA's Dawn spacecraft arrived at Ceres on March 6, 2015, and has been studying the dwarf planet through a series of successively lower orbits, obtaining morphological and topographical image, mineralogical, elemental composition, and gravity data (Russell et al., 2016). Images taken by Dawn's Framing Camera show a multitude of flow features that were broadly interpreted as ground <span class="hlt">ice</span> related structures either similar to <span class="hlt">ice</span> cored/<span class="hlt">ice</span> cemented flows (as seen on Earth and Mars), long run-out landslides, or fluidized ejecta (as seen on Mars) by Schmidt et al. (2016a and 2016b) and Buczkowski et al. (2016). The aforementioned <span class="hlt">ice</span> cored/<span class="hlt">ice</span> cemented-like flows are present only at high latitudes. Results from Dawn's Gamma Ray and Neutron Detector (GRaND) indicate a shallow <span class="hlt">ice</span> table on Ceres above 45-50°N/S, which supports the interpretation that these flows are <span class="hlt">ice</span>-rich (Prettyman et al., 2016). A near coincident spectral detection of H2O <span class="hlt">ice</span> with one of these <span class="hlt">ice</span> cored/<span class="hlt">ice</span> cemented-like flows in Oxo crater by Dawn's Visual and Infrared spectrometer (VIR) further bolsters this claim (Combe et al., 2016). We use aggregate spatial and physical properties of these <span class="hlt">ice</span> attributed cerean flows, such as flow orientation, inclination, preference for north or south facing slopes, drop height to run-out length ratio, geographical location, and areal number density to better understand the rheology and distribution of ground <span class="hlt">ice</span> in Ceres' uppermost layer. By combining these data with local spectroscopic, global elemental abundance, experimentally derived physical properties of cerean analogue material, and other morphological information (such as the morphologies of flow hosting craters) we intend to further test the ground <span class="hlt">ice</span> hypothesis for the formation of these flows and constrain the global distribution of near surface ground <span class="hlt">ice</span> on Ceres to a higher fidelity than what would be possible using GRaND and VIR observations alone. References: Buczkowski et al., (2016) Science</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.C21C0458P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.C21C0458P"><span>Outlet Glacier-<span class="hlt">Ice</span> Shelf-Ocean Interactions: Is the Tail Wagging the Dog?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Parizek, B. R.; Walker, R. T.; Rinehart, S. K.</p> <p>2009-12-01</p> <p>While the massive interior regions of the Antarctic and Greenland <span class="hlt">Ice</span> Sheets are presently ``resting quietly", the lower elevations of many outlet glaciers are experiencing dramatic adjustments due to changes in <span class="hlt">ice</span> dynamics and/or surface <span class="hlt">mass</span> balance. Oceanic and/or atmospheric forcing in these marginal regions often leads to <span class="hlt">mass</span> deficits for entire outlet basins. Therefore, coupling the wagging tail of <span class="hlt">ice</span>-ocean interactions with the vast <span class="hlt">ice</span>-sheet reservoirs is imperative for accurate assessments of future sea-level rise. To study <span class="hlt">ice</span>-ocean dynamic processes, we couple an ocean-plume model that simulates <span class="hlt">ice</span>-shelf basal melting rates based on temperature and salinity profiles combined with plume dynamics associated with the geometry of the <span class="hlt">ice</span>-shelf cavity (following Jenkins, 1991 and Holland and Jenkins, 1999) with a two-dimensional, isothermal model of outlet glacier-<span class="hlt">ice</span> shelf flow (as used in Alley et al., 2007; Walker et al., 2008; Parizek et al., in review). Depending on the assigned temperature and salinity profiles, the ocean model can simulate both water-<span class="hlt">mass</span> end-members: either cold High Salinity Shelf Water (HSSW) or relatively warm Circumpolar Deep Water (CDW), as well as between-member conditions. Notably, the coupled system exhibits sensitivity to the initial conditions. In particular, melting concentrated near the grounding line has the greatest effect in forcing grounding-line retreat. Retreat is further enhanced by a positive feedback between the ocean and <span class="hlt">ice</span>, as the focused melt near the grounding line leads to an increase in the local slope of the basal <span class="hlt">ice</span>, thereby enhancing buoyancy-driven plume flow and subsequent melt rates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Icar..303..280S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Icar..303..280S"><span>Chlorine-containing salts as water <span class="hlt">ice</span> nucleating particles 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>Santiago-Materese, D. L.; Iraci, L. T.; Clapham, M. E.; Chuang, P. Y.</p> <p>2018-03-01</p> <p>Water <span class="hlt">ice</span> cloud formation on Mars largely is expected to occur on the most efficient <span class="hlt">ice</span> nucleating particle available. Salts have been observed on the Martian surface and have been known to facilitate water cloud formation on Earth. We examined heterogeneous <span class="hlt">ice</span> nucleation onto sodium chloride and sodium perchlorate substrates under Martian atmospheric conditions, in the range of 150 to 180 K and 10-7 to 10-5 Torr water partial pressure. Sub-155 K data for the critical saturation ratio (Scrit) suggests an exponential model best describes the temperature-dependence of nucleation onset of water <span class="hlt">ice</span> for all substrates tested. While sodium chloride does not facilitate water <span class="hlt">ice</span> nucleation more easily than bare silicon, sodium perchlorate does support depositional nucleation at lower saturation levels than other substrates shown and is comparable to smectite-rich clay in its ability to support cloud initiation. Perchlorates could nucleate water <span class="hlt">ice</span> at partial pressures up to 40% lower than other substrates examined to date under Martian atmospheric conditions. These findings suggest air <span class="hlt">masses</span> on Mars containing uplifted salts such as perchlorates could form water <span class="hlt">ice</span> clouds at lower saturation ratios than in air <span class="hlt">masses</span> absent similar particles.</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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